A. Omont

Publication List Details

Period

1960 - 2009

Number

316

Co-Authors

Molecular Gas in Submillimetre-Faint, Star-Forming Ultraluminous Galaxies at z>1 (2009)

Casey, C. M., Chapman, S. C., Neri, R., Bertoldi, F., Smail, I., Greve, T. R., ...

We present interferometric CO observations of twelve z~2 submillimeter-faint, star-forming radio galaxies (SFRGs) which are thought to be ultraluminous infrared galaxies (ULIRGs) dominated by hotter...

Multi-wavelength properties of Spitzer-selected starbursts at z~2 (2009)

Fiolet, N., Omont, A., Polletta, M., Owen, F., Berta, S., Shupe, D., ...

A complete sample of 33 sources believed to be starbursts ("5.8micron-peakers") was selected in the (0.5 sq. deg.) J1046+56 field with selection criteria F_(24micron)>400muJy, the presence of a...

A Search for Neutral Carbon towards two z=4.05 Submillimetre Galaxies, GN20 and GN20.2 (2009)

Casey, C. M., Chapman, S. C., Daddi, E., Dannerbauer, H., Pope, A., Scott, D., ...

Using the IRAM Plateau-de-Bure Interferometer (PdBI) we have searched for the upper fine structure line of neutral carbon (CI(2->1), nu_rest = 809 GHz) and 12CO(J=7->6) (nu_rest=806GHz) towards the...

Infrared Spectrograph Spectroscopy and Multi-Wavelength Study of Luminous Star-Forming Galaxies at z ≃ 1.9 (2009)

Faber, S. M., Daddi, E., Laird, E. S., Lai, K., Omont, A., ...

We analyze a sample of galaxies chosen to have F_(24μm) > 0.5 mJy and satisfy a certain IRAC color criterion. Infrared Spectrograph (IRS) spectra yield redshifts, spectral types, and polycyclic...

IRS Spectroscopy and Multi-wavelength Study of Luminous Star-forming Galaxies at z~1.9 (2009)

Faber, S. M., Daddi, E., Laird, E. S., Lai, K., Omont, A., ...

We analyze a sample of galaxies chosen to have F24>0.5 mJy and satisfy a certain IRAC color criterion. IRS spectra yield redshifts, spectral types, and PAH luminosities, to which we add...

CO line emission in the halo of a radio galaxy at z=2.6 (2009)

Nesvadba, N. P. H., Neri, R., De Breuck, C., Lehnert, M. D., Downes, D., Walter, F., ...

We report the detection of luminous CO(3-2) line emission in the halo of the z=2.6 radio galaxy (HzRG) TXS0828+193, which has no detected counterpart at optical to mid-infrared wavelengths implying a...

Imaging the cool gas, dust, star formation, and AGN in the first galaxies (2009)

Carilli, C. L., Myers, S., Appleton, P., Bertoldi, F., Blain, A., Dale, D., ...

When, and how, did the first galaxies and supermassive black holes (SMBH) form, and how did they reionization the Universe? First galaxy formation and cosmic reionization are among the last frontiers...

Six more quasars at redshift 6 discovered by the Canada-France High-z Quasar Survey (2009)

Willott, C. J., Delorme, P., Reyle, C., Albert, L., Bergeron, J., Crampton, D., ...

We present imaging and spectroscopic observations for six quasars at z>5.9 discovered by the Canada-France High-z Quasar Survey (CFHQS). The CFHQS contains sub-surveys with a range of flux and area...

Interferometric CO observations of submillimeter-faint, radio-selected starburst galaxies at z ~ 2 (2008)

Chapman, S. C., Neri, R., Bertoldi, F., Smail, Ian, Greve, T. R., Trethewey, D., ...

High-redshift, dust-obscured galaxies, selected to be luminous in the radio but relatively faint at 850 µm, appear to represent a different population from the ultraluminous submillimeter-bright...

A Millimetre Survey of Starburst Dominated Ultraluminous Infrared Galaxies at z~2 (2008)

Younger, J. D., Omont, A., Fiolet, N., Fazio, G. G., Lai, K., ...

We present millimetre observations of a sample of 12 high redshift ultraluminous infrared galaxies (ULIRGs) in the Extended Growth Strip (EGS). These objects were initially selected on the basis of...

Obscured and powerful AGN and starburst activities at z~3.5 (2008)

Polletta, M., Omont, A., Berta, S., Bergeron, J., Stalin, C. S., Petitjean, P., ...

We report the discovery of two sources at z=3.867 and z=3.427 that exhibit powerful starburst and AGN activities. They benefit from data from radio to X rays from the CFHTLS-D1/SWIRE/XMDS surveys....

MAMBO 1.2mm observations of luminous starbursts at z~2 in the SWIRE fields (2008)

Lonsdale, C. J., Polletta, M., Omont, A., Shupe, D., Berta, S., Zylka, R., ...

We report on--off pointed MAMBO observations at 1.2 mm of 61 Spitzer-selected star-forming galaxies from the SWIRE survey. The sources are selected on the basis of bright 24um fluxes (f_24um>0.4mJy)...

Stellar populations in a standard ISOGAL field in the Galactic disk (2008)

Ganesh, S., Omont, A., Joshi, U. C., Baliyan, K. S., Schultheis, M., Schuller, F., ...

We aim to identify the stellar populations (mostly red giants and young stars) detected in the ISOGAL survey at 7 and 15micron towards a field (LN45) in the direction l=-45, b=0.0. The sources...

Submillimeter observations of the J2142-4423 Lyα protocluster at z = 2.38 (2008)

Beelen, A., Omont, A., Bavouzet, N., Kovács, A., Lagache, G., De Breuck, C., ...

Aims. We present observations aimed at exploring both the nature of Lyα emitting nebulae ("Lyα blobs") at z=2.38 and the way they trace large scale structure (LSS), by exploring their proximity to...

Thermal Emission from Warm Dust in the Most Distant Quasars (2008)

Wang, R., Carilli, C. L., Wagg, J., Bertoldi, F., Walter, F., Menten, K. M., ...

We report new continuum observations of fourteen z~6 quasars at 250 GHz and fourteen quasars at 1.4 GHz. We summarize all recent millimeter and radio observations of the sample of the thirty-three...

Submillimeter galaxies at z ~ 2: evidence for major mergers and constraints on lifetimes, IMP and CO-H_2 conversion factor (2008)

Tacconi, L. J., Genzel, R., Smail, I., Neri, R., Chapman, S. C., Ivison, R. J., ...

We report subarcsecond resolution IRAM PdBI millimeter CO interferometry of four z ~ 2 submillimeter galaxies (SMGs), and sensitive CO(3-2) flux limits toward three z ~ 2 UV/optically selected...

Submillimeter observations of the J2142-4423 Lya protocluster at z = 2.38 (2008)

Beelen, A., Omont, A., Bavouzet, N., Kovacs, A., Lagache, G., De Breuck, C., ...

We present observations aimed at exploring both the nature of Lya emitting nebulae (Lya blobs) at z=2.38 and the way they trace large scale structure (LSS), by exploring their proximity to maximum...

Submillimeter Galaxies at z~2: Evidence for Major Mergers & Constraints on Lifetimes, IMF and CO-H2 Conversion Factor (2008)

Tacconi, L. J., Genzel, R., Smail, I., Neri, R., Chapman, S. C., Ivison, R. J., ...

We report sub-arcsecond resolution IRAM PdBI millimeter CO interferometry of four z~2 submillimeter galaxies (SMGs), and sensitive CO (3-2) flux limits toward three z~2 UV-/optically selected star...

Testing the Evolutionary Link Between Submillimetre Galaxies and Quasars: CO Observations of QSOs at z~2. (2008)

Coppin, K., Swinbank, M., Neri, R., Cox, P., Alexander, D., Smail, I., ...

‘The definitive version is available at www3.interscience.wiley.com '. Copyright Blackwell Publishing / RAS. DOI: 10.1111/j.1365-2966.2008.13553.x

Submillimeter galaxies at z ~ 2: evidence for major mergers and constraints on lifetimes, IMF, and CO-H2 conversion factor (2008)

Tacconi, L. J., Genzel, R., Smail, I., Neri, R., Chapman, S. C., Ivison, R. J., ...

We report subarcsecond resolution IRAM PdBI millimeter CO interferometry of four z~2 submillimeter galaxies (SMGs), and sensitive CO(3-2) flux limits toward three z~2 UV/optically selected...

Obscured and powerful AGN and starburst activities at z ~ 3.5 (2008)

Polletta, M., Omont, A., Berta, S., Bergeron, J., Stalin, C. S., Petitjean, P., ...

Aims. Short phases of coeval powerful starburst and AGN activity during the lifetimes of the most massive galaxies are predicted by various models of galaxy formation and evolution. In spite of their...

Interferometric CO observations of submillimeter-faint, radio-selected starburst galaxies at z ~ 2 (2008)

Chapman, S. C., Neri, R., Bertoldi, F., Smail, Ian, Greve, T. R., Trethewey, D., ...

High-redshift, dust-obscured galaxies, selected to be luminous in the radio but relatively faint at 850 mum, appear to represent a different population from the ultraluminous submillimeter-bright...

Studying the first galaxies with ALMA (2008)

Carilli, C. L., Walter, F., Wang, R., Wootten, A., Menten, K., Bertoldi, F., ...

We discuss observations of the first galaxies, within cosmic reionization, at centimeter and millimeter wavelengths. We present a summary of current observations of the host galaxies of the most...

The Dust Sequence along the AGB (2008)

Vanhollebeke, E., Cami, J., Groenewegen, M.A.T., Habing, H.J., Markwick-Kemper, F., ...

With Spitzer--IRS we observed a homogeneous sample of AGB stars in the Galactic Bulge. The Spitzer--IRS wavelength range 5.2 - 38 mum contains the major spectral features of aluminium oxides and...

6 (2007)

A. Omont, S. Ganesh, C. Alard, B. Caillaud, E. Copet, G. Gilmore, ...

A&A manuscript no. (will be inserted by hand later) Your thesaurus codes are:

The second detection of CO at redshift larger than 4 (2007)

Guilloteau Omont Mcmahon, S. Guilloteau, A. Omont, R. G. Mcmahon, P. Cox, P. Petitjean

. We report the detection of the 3mm J=5-4 CO line ( rest =576267.70 MHz) in the radio quiet quasar BRI 1335-0415 at redshift 4.41 with the IRAM interferometer. After BR 1202-0725 at z=4.69, this is...

Mass-losing AGB stars in galactic bulge ISOGAL fields (2007)

S. Ganesh, A. Omont, M. Schultheis, D. Ojha, C. Alard, ...

. First results on AGB stars with the ISOGAL mid-infrared survey are presented. We show that M6 and later spectral type giants are detected at 7 and 15 m up to the distance of the galactic centre....

Detection of Young Stellar Objects with ISO (2007)

Testi Felli, L. Testi, M. Felli, A. Omont, G. Comoretto, G. Gilmore

. Preliminary 15¯m results obtained with ISOCAM are compared with deep K-band and H 2 O maser observations of a 0:244 deg 2 field in the galactic plane at l = +45 ffi . A new maser source is found...

First ISOCAM images of the Milky Way (2007)

Erault Omont, A. Omont, G. Simon, D. Ojha, J. Blommaert, M. Felli, ...

. ISOGAL is a 15 ¯m ISOCAM survey of ¸ 12 deg 2 in the Galactic Plane interior to j`j = 45 ffi . In combination with IJK data from the near-infrared southern sky survey DENIS, the ISO images allow...

6 (2007)

I. S. Glass, S. Ganesh, C. Alard, G. Gilmore, T. Lloyd Evans, A. Omont, ...

The ISOGAL mid-infrared survey of areas close to the Galactic Plane aims to determine their stellar content and its possible bearing on the history of the Galaxy. The NGC 6522 and Sgr I Baade's...

Detection of 1.6 × 10^(10) M_⊙ of Molecular Gas in the Host Galaxy of the z = 5.77 SDSS Quasar J0927+2001 (2007)

Carilli, C. L., Neri, R., Wang, R., Cox, P., Bertoldi, F., Walter, F., ...

We have detected emission by the CO(5-4) and (6-5) rotational transitions at z = 5.7722 ± 0.0006 from the host galaxy of the SDSS quasar J0927+2001 using the Plateau de Bure Interferometer. The peak...

High mass-loss AGB stars detected by MSX in the "intermediate" and "outer" Galactic bulge (2007)

Ojha, D. K., Tej, A., Schultheis, M., Omont, A., Schuller, F.

We present a study of MSX point sources in the Galactic bulge (|l| < 3 deg, 1 deg < |b| < 5 deg), observed at A, C, D and E-band (8 to 21 micron), with a total area ~ 48 deg^2. We discuss the nature...

Molecular gas in QSO host galaxies at z>5 (2007)

Maiolino, R., Neri, R., Beelen, A., Bertoldi, F., Carilli, C. L., Caselli, P., ...

We present observations with the IRAM Plateau de Bure Interferometer of three QSOs at z>5 aimed at detecting molecular gas in their host galaxies as traced by CO transitions. CO (5-4) is detected in...

Detection of $1.6\times 10^{10}$ M$_\odot$ of molecular gas in the host galaxy of the $z=5.77$ SDSS quasar J0927+2001 (2007)

Carilli, C., Neri, R., Wang, R., Cox, P., Bertoldi, F., Walter, F., ...

We have detected emission by the CO 5-4 and 6-5 rotational transitions at $z = 5.7722\pm 0.0006$ from the host galaxy of the SDSS quasar J0927+2001 using the Plateau de Bure interferometer. The peak...

Studying the first galaxies with ALMA (2007)

Carilli, C. L., Walter, F., Wang, R., Wootten, A., Menten, K., Bertoldi, F., ...

We discuss observations of the first galaxies, within cosmic reionization, at centimeter and millimeter wavelengths. We present a summary of current observations of the host galaxies of the most...

Molecular gas in QSO host galaxies at z > 5 (2007)

Maiolino, R., Neri, R., Beelen, A., Bertoldi, F., Carilli, C. L., Caselli, P., ...

We present observations with the IRAM Plateau de Bure Interferometer of three QSOs at z>5 aimed at detecting molecular gas in their host galaxies as traced by CO transitions. CO (5-4) is detected in...

Detection of 1.6 × 1010 Msolar of molecular gas in the host galaxy of the z = 5.77 SDSS quasar J0927+2001 (2007)

Carilli, C. L., Neri, R., Wang, R., Cox, P., Bertoldi, F., Walter, F., ...

We have detected emission by the CO(5-4) and (6-5) rotational transitions at z=5.7722+/-0.0006 from the host galaxy of the SDSS quasar J0927+2001 using the Plateau de Bure Interferometer. The peak...

Radio and millimeter observations of z~2 luminous QSOs (2006)

Petric, A., Carilli, C. L., Bertoldi, F., Beelen, A., Cox, P., Omont, A.

We present Very Large Array observations at 1.4 and 5 GHz of a sample of 16 quasi-stellar objects (QSOs) at z = 1.78 to 2.71. Half of the chosen quasars are bright at mm wavelengths (250 or 350 GHz)...

Recent star formation in the inner Galactic Bulge seen by ISOGAL. I - Classification of bright mid-IR sources in a test field (2006)

Schuller, F., Omont, A., Glass, I. S., Schultheis, M., Egan, M. P., Price, S. D., ...

Context: The stellar populations in the central region of the Galaxy are poorly known because of the high visual extinction and very great source density in this direction. Aims: To use recent...

350 Micron Dust Emission from High Redshift Quasars (2006)

Beelen, A., Cox, P., Benford, D. J., Dowell, C. D., Kovacs, A., Bertoldi, F., ...

We report detections of six high-redshift (1.8 < z < 6.4), optically luminous, radio-quiet quasars at 350 micron, using the SHARC II bolometer camera at the Caltech Submillimeter Observatory. Our...

An interferometric CO survey of luminous submm galaxies (2005)

Greve, T. R., Bertoldi, F., Smail, Ian, Neri, R., Chapman, S. C., Blain, A. W., ...

In this paper we present results from an IRAM Plateau de Bure millimetre-wave Interferometer (PdBI) survey for CO emission towards radio-detected submillimetre galaxies (SMGs) with known optical and...

High-resolution Millimeter Imaging of Submillimeter Galaxies (2005)

Tacconi, L. J., Neri, R., Chapman, S. C., Genzel, R., Smail, I., Ivison, R. J., ...

We present sub-arcsecond resolution IRAM PdBI interferometry of eight submillimeter galaxies at redshifts from 2 to 3.4, where we detect continuum at 1mm and/or CO lines at 3 and 1 mm. The CO 3-2/4-3...

Extinctions at 7um and 15um from the ISOGAL survey (2005)

Jiang, B. W., Gao, J., Omont, A., Schuller, F., Simon, G.

The extinction laws at 7um and 15um are derived for more than 120 sightlines in the inner Galactic plane based on the ISOGAL survey data and the near-infrared data from DENIS and 2MASS. The tracers...

First detection of [CII]158um at high redshift: vigorous star formation in the early universe (2005)

Maiolino, R., Cox, P., Caselli, P., Beelen, A., Bertoldi, F., Carilli, C. L., ...

We report the detection of the 2P_3/2 -> 2P_1/2 fine-structure line of C+ at 157.74 micron in SDSSJ114816.64+525150.3 (hereafter J1148+5251), the most distant known quasar, at z=6.42, using the IRAM...

The DENIS Point Source Catalogue towards the Magellanic Clouds (2005)

Cioni, M-R., Loup, C., Habing, H. J., Fouque', P., Bertin, E., Deul, E., ...

We have compiled the near infrared Point Source Catalogue (PSC) towards the Magellanic Clouds (MCs) extracted from the data obtained with the Deep Near Infrared Survey of the Southern Sky - DENIS...

Infrared stellar populations in the central parts of the Milky Way galaxy (2005)

Van Loon, Jacco Th., Gilmore, G. F., Omont, A., Glass, I. S., Messineo, M., ...

Near- and mid-IR survey data from DENIS and ISOGAL are used to investigate the structure and formation history of the inner 10 degree (1.4 kpc) of the Milky Way galaxy. Synthetic bolometric...

Low resolution spectroscopy of ISOGAL sources: Search for early-type stars with infrared excess (2005)

Schultheis, M., Parthasarathy, M., Omont, A., Cohen, M., Ganesh, S., Sevre, F., ...

An analysis of low resolution spectra and infared data of 29 ISOGAL-DENIS sources with mid-IR excess is presented. Eight ISOGAL sources from our sample with 7-15 micron excess are found to be B and...

CO and Dust in PSS2322+1944 at a redshift of 4.12 (2005)

Cox, P., Omont, A., Djorgovski, S. G., Bertoldi, F., Pety, J., Carilli, C. L., ...

Using the IRAM interferometer we have detected J=4-3 and 5-4 CO line emission toward the radio quiet quasar PSS2322+1944. At a redshift of z_CO=4.1199 this is the fourth and strongest detection of CO...

Imaging low order CO emission from the z=4.12 QSO PSS 2322+1944 (2005)

Carilli, C., Cox, P., Bertoldi, F., Menten, K. M., Omont, A.

We present observations of CO 1-0 and CO 2-1 emission from the z = 4.12 QSO PSS 2322+1944 using the Very Large Array. The CO emission is extended on a spatial scale of 2\'\'. This extension could...

Young massive stars in the ISOGAL survey II. The catalogue of bright YSO candidates (2005)

Felli, M., Testi, L., Schuller, F., Omont, A.

The 7 and 15 um observations of selected fields in the Galactic Plane obtained with ISOCAM during the ISOGAL program offer an unique possibility to search for previously unknown YSOs, undetected by...

86 GHz SiO maser survey of late-type stars in the Inner Galaxy. I. Observational data (2005)

Messineo, M., Habing, H. J., Sjouwerman, L. O., Omont, A., Menten, K. M.

We present 86 GHz (v = 1, J = 2 -1) SiO maser line observations with the IRAM 30-m telescope of a sample of 441 late-type stars in the Inner Galaxy (-4 degr < l < +30 degr). These stars were selected...

A 1.2mm MAMBO/IRAM-30m Survey of Dust Emission from the Highest Redshift PSS Quasars (2005)

Omont, A., Cox, P., Bertoldi, F., McMahon, R. G., Carilli, C., Isaak, K. G.

We report 250 GHz (1.2mm) observations of redshift > 3.8 quasars from the Palomar Sky Survey (PSS) sample, using the Max-Planck Millimetre Bolometer (MAMBO) array at the IRAM 30-metre telescope....

Mass-Losing Semiregular Variable Stars in Baade's Windows (2005)

Alard, C., Blommaert, J., Cesarsky, C., Epchtein, N., Felli, M., Fouque, P., ...

By cross-correlating the results of two recent large-scale surveys, the general properties of a well defined sample of semi-regular variable stars have been determined. ISOGAL mid-infrared photometry...

A deep submillimetre survey of the Galactic Centre (2005)

Pierce-Price, D., Richer, J. S., Greaves, J. S., Holland, W. S., Jenness, T., Lasenby, A. N., ...

We present first results from a submillimetre continuum survey of the Galactic Centre `Central Molecular Zone\' (CMZ), made with SCUBA on the James Clerk Maxwell Telescope. SCUBA\'s scan-map mode has...

CO lines in high redshift galaxies: perspective for future mm instruments (2005)

Combes, F., Maoli, R., Omont, A.

Nearly 10 high redshift (z>2) starburst galaxies have recently been detected in the CO lines, revealing the early presence in the universe of objects with large amounts of already-enriched molecular...

ISOGAL Survey of Baade\'s Windows in the Mid-infrared (2005)

Glass, I. S, Ganesh, S., Alard, C., Gilmore, G., Evans, T. Lloyd, ...

The ISOGAL mid-infrared survey of areas close to the Galactic Plane aims to determine their stellar content and its possible bearing on the history of the Galaxy. The NGC6522 and Sgr I Baade\'s...

ISOGAL-DENIS detection of red giants with weak mass loss in the Galactic Bulge (2005)

Omont, A., Ganesh, S., Alard, C., Caillaud, B., Copet, E., ...

The ISOGAL project is a survey of the stellar populations, structure, and recent star formation history of the inner disk and bulge of the Galaxy. ISOGAL combines 15 and 7micron ISOCAM observations...

CO(4-3) and dust emission in two powerful high-z radio galaxies, and CO lines at high redshifts (2005)

Papadopoulos, Padeli P., Rottgering, H. J. A., Van Der Werf, P. P., Guilloteau, S., Omont, A., ...

We report the detection of sub-mm emission from dust at 850 microns and of the 12CO J=4-3 line in the two distant powerful radio galaxies 4C 60.07 (z=3.79) and 6C 1909+722 (z=3.53). In the case of 4C...

Interstellar extinction towards the inner Galactic Bulge (2005)

Schultheis, M., Ganesh, S., Simon, G., Omont, A., Alard, C., Borsenberger, J., ...

DENIS observations in the J (1.2 micron) and K_S (2.15 micron) bands together with isochrones calculated for the RGB and AGB phase are used to draw an extinction map of the inner Galactic Bulge. The...

2.4 - 197 micron spectroscopy of OH/IR stars: The IR characteristics of circumstellar dust in O-rich environments (2005)

Sylvester, R. J., Kemper, F., Barlow, M. J., De Jong, T., ...

Infrared spectra of a number of evolved O-rich stars have been obtained with the Short- and Long- Wavelength spectrometers on board the Infrared Space Observatory. The very broad wavelength coverage...

Deep Galaxy survey at 6.75 micron with the ISO satellite (2005)

Flores, H., Hammer, F., Désert, F. X., Césarsky, C., Thuan, T., Crampton, D., ...

Deep 6.75um mid-IR ISOCAM observations were obtained of the Canada-France Redshift Survey (CFRS) 1415+52 field with the Infrared Space Observatory. The identification of the sources with optical...

A 1.2mm MAMBO/IRAM-30m Study of Dust Emission from optically luminous z~2 Quasars (2005)

Omont, A., Beelen, A., Bertoldi, F., Cox, P., Carilli, C., Priddey, R. S., ...

We report 250GHz (1.2mm) observations of redshift 1.8 < z < 2.8 optically luminous (M_B < -27.0), radio quiet quasars using the Max-Planck Millimeter Bolometer (MAMBO) array at the IRAM 30-metre...

Radio Observations of Infrared Luminous High Redshift QSOs (2005)

Carilli, C. L., Bertoldi, F., Omont, A., Cox, P., McMahon, R. G., Isaak, K. G.

We present Very Large Array (VLA) observations at 1.4 GHz and 5 GHz of a sample of 12 Quasi-stellar Objects (QSOs) at z = 3.99 to 4.46. The sources were selected as the brightest sources at 250 GHz...

The ISOGAL field FC--01863+00035: Mid-IR interstellar extinction and stellar populations (2005)

Jiang, B. W., Omont, A., Ganesh, S., Simon, G., Schuller, F.

A 0.35\\degr $\\times$ 0.29\\degr field centered at $l$=--18.63\\degr, $b$=0.35\\degr was observed during the ISOGAL survey by ISOCAM imaging at 7$\\mu$m and 15{\\rm $\\mu$m}. 648 objects were...

Stellar sources in the ISOGAL intermediate bulge fields (2005)

Ojha, D. K., Omont, A., Schuller, F., Simon, G., Ganesh, S., Schultheis, M.

We present a study of ISOGAL sources in the \"intermediate\" galactic bulge ($|$$l$$|$ $

Near-IR spectra of ISOGAL sources in the Inner Galactic Bulge (2005)

Schultheis, M., Lançon, A., Omont, A., Schuller, F., Ojha, D. K.

In this work we present near-IR spectra (HK-band) of a sample of 107 sources with mid-IR excesses at 7 and 15 $\\rm \\mu$m detected during the ISOGAL survey. Making use of the DENIS interstellar...

Sensitive observations at 1.4 and 250 GHz of z > 5 QSOs (2005)

Petric, A. O., Carilli, C. L., Bertoldi, F., Fan, Xiaohui, Cox, P., Strauss, Michael A., ...

We present 1.4 and 5 GHz observations taken with the Very Large Array (VLA), and observations at 250 GHz obtained with the Max-Planck millimeter bolometer (MAMBO) at the IRAM 30~m telescope, of ten...

A Molecular Einstein Ring: Imaging a Starburst Disk Surrounding a Quasi-Stellar Object (2005)

Carilli, C. L., Lewis, G. F., Djorgovski, S. G., Mahabal, A., Cox, P., Bertoldi, F., ...

Images of the CO 2-1 line emission, and the radio continuum emission, from the redshift 4.12 gravitationally lensed quasi-stellar object (QSO) PSS J2322+1944 reveal an Einstein ring with a diameter...

Long Period Variables detected by ISO in the SMC (2005)

Cioni, M. -R. L., Groenewegen, M. A. T., Habing, H. J., Hron, J., Kerschbaum, F., ...

This article presents the study of the light-curves extracted from the MACHO database of a sample of stars observed by the ISO in the SMC. These stars belong to the ISO-Mini-Survey catalogue of the...

Explanatory Supplement of the ISOGAL-DENIS Point Source Catalogue (2005)

Schuller, F., Ganesh, S., Messineo, M., Moneti, A., Alard, C., ...

We present version 1.0 of the ISOGAL-DENIS Point Source Catalogue (PSC), containing more than 100,000 point sources detected at 7 and/or 15 micron in the ISOGAL survey of the inner Galaxy with the...

ISOGAL: A deep survey of the obscured inner Milky Way with ISO at 7 and 15 micron and with DENIS in the near-infrared (2005)

Omont, A., Gilmore, G., Alard, C., Aracil, B., August, T., Baliyan, K., ...

The ISOGAL project is an infrared survey of specific regions sampling the Galactic Plane selected to provide information on Galactic structure,stellar populations,stellar mass-loss and the recent...

Dust emission from the most distant quasars (2005)

Bertoldi, F., Carilli, C. L., Cox, P., Fan, X., Strauss, M. A., Beelen, A., ...

We report observations of three SDSS z>6 QSOs at 250 GHz (1.2mm) using the 117-channel Max-Planck Millimeter Bolometer (MAMBO-2) array at the IRAM 30-meter telescope. J1148+5251 (z=6.41) and...

Interferometric Observations of Powerful CO Emission from the three Submillimeter Galaxies at z=2.30, 2.51 and 3.35 (2005)

Neri, R., Genzel, R., Ivison, R. J., Bertoldi, F., Blain, A. W., Chapman, S. C., ...

We report IRAM Plateau de Bure, millimeter interferometry of three z=~2.4 to 3.4, SCUBA deep field galaxies. Our CO line observations confirm the rest-frame UV/optical redshifts, thus more than...

High-excitation CO in a quasar host galaxy at z=6.42 (2005)

Bertoldi, F., Cox, P., Neri, R., Carilli, C. L., Walter, F., Omont, A., ...

We report the detection of high excitation CO emission from the most distant quasar currently known, SDSS J114816.64+525150.3 (hereafter J1148+5251), at a redshift z=6.419. The CO (J=6-5) and (J=7-6)...

86 GHz SiO maser survey of late-type stars in the Inner Galaxy II. Infrared photometry of the SiO Target Stars (2005)

Messineo, M., Habing, H. J., Menten, K. M., Omont, A., Sjouwerman, L. O.

We present a compilation and study of DENIS, 2MASS, ISOGAL, MSX and IRAS 1--25 micron photometry for a sample of 441 late-type stars in the inner Galaxy, which we previously searched for 86 GHz SiO...

Starburst activity in the host galaxy of the z=2.58 quasar J1409+5628 (2005)

Beelen, A., Cox, P., Pety, J., Carilli, C. L., Bertoldi, F., Momjian, E., ...

We report the detection of CO emission from the optically luminous, radio-quiet quasar J140955.5+562827, at a redshift z_CO =2.583. We also present VLA continuum mapping results and VLBA high spatial...

Radio continuum imaging of FIR luminous QSOs at z>6 (2005)

Carilli, C. L., Walter, F., Bertoldi, F., Menten, K. M., Fan, X., Lewis, G. F., ...

We present sensitive imaging at 1.4 GHz of the two highest redshift far-infrared (FIR) luminous QSOs SDSS J114816.65+525150.2 (z=6.42) and SDSS J104845.05+463718.3 (z=6.2). Radio continuum emission...

A Search for Dense Molecular Gas in High Redshift Infrared-Luminous Galaxies (2005)

Carilli, C. L., Solomon, P., Bout, P. Vanden, Walter, F., Beelen, Alexandre, Cox, Pierre, ...

We present a search for HCN emission from four high redshift far infrared (IR) luminous galaxies. Current data and models suggest that these high $z$ IR luminous galaxies represent a major starburst...

Atomic carbon in PSS 2322+1944, a quasar at redshift 4.12 (2005)

Pety, J., Beelen, A., Cox, P., Downes, D., Omont, A., Bertoldi, F., ...

We report the detection of the 3P1 to 3P0 fine-structure line of neutral carbon in the z=4.12 quasar PSS 2322+1944, obtained at the IRAM Plateau de Bure interferometer. The CI 3P1-3P0 line is...

Multiwavelength study of the inner regions of the Milky Way Galaxy (2005)

Ganesh, S, Joshi, U. C, Baliyan, K. S, Omont, A, Simon, G

The inner regions of the Milky Way have received a lot of attention in recent years. Multiwavelength observations have been made at varying spatial, temporal and spectral resolutions. We have studied...

86 GHz SiO maser survey of late-type stars in the Inner Galaxy III. Interstellar extinction and colours of the SiO targets (2005)

Messineo, M., Habing, H. J., Menten, K. M., Omont, A., Sjouwerman, L. O., Bertoldi, F.

We have determined extinction corrections for a sample of 441 late-type stars in the inner Galaxy, which we previously searched for SiO maser emission, using the 2MASS near-infrared photometry of the...

An interferometric CO survey of luminous submm galaxies (2005)

Greve, T. R., Bertoldi, F., Smail, Ian, Neri, R., Chapman, S. C., Blain, A. W., ...

In this paper we present results from an IRAM Plateau de Bure millimetre-wave Interferometer (PdBI) survey for CO emission towards radio-detected submillimetre galaxies (SMGs) with known optical and...

An interferometric CO survey of luminous submm galaxies (2005)

Greve, T. R., Bertoldi, F., Smail, Ian, Neri, R., Chapman, S. C., Blain, A. W., ...

In this paper we present results from an IRAM Plateau de Bure millimetre-wave Interferometer (PdBI) survey for CO emission towards radio-detected submillimetre galaxies (SMGs) with known optical and...

An interferometric CO survey of luminous submm galaxies (2005)

Greve, T. R., Bertoldi, F., Smail, Ian, Neri, R., Chapman, S. C., Blain, A. W., ...

In this paper we present results from an IRAM Plateau de Bure millimetre-wave Interferometer (PdBI) survey for CO emission towards radio-detected submillimetre galaxies (SMGs) with known optical and...

First detection of [CII]158 µm at high redshift: Vigorous star formation in the early Universe (2005)

Maiolino, R., Cox, P., Caselli, P., Beelen, A., Bertoldi, F., Carilli, C. L., ...

We report the detection of the 2P3/2 --> 2P1/2 fine-structure line of C+ at 157.74 mu m in SDSS J114816.64+525150.3 (hereafter J1148+5251), the most distant known quasar, at z=6.42, using the IRAM...

A search for dense molecular gas in high-redshift infrared-luminous galaxies (2005)

Carilli, C. L., Solomon, P., Vanden Bout, P., Walter, F., Beelen, Alexandre, Cox, Pierre, ...

We present a search for HCN emission from four high-redshift far-IR-luminous galaxies. Current data and models suggest that these high-z IR-luminous galaxies represent a major starburst phase in the...

Atomic carbon in PSS 2322+1944, a quasar at redshift 4.12 (2004)

Pety, J., Beelen, A., Cox, P., Downes, D., Omont, A., Bertoldi, F., ...

We report the detection of the 3P1 to 3P0 fine-structure line of neutral carbon in the z=4.12 quasar PSS 2322+1944, obtained at the IRAM Plateau de Bure interferometer. The CI 3P1-3P0 line is...

A Search for Dense Molecular Gas in High Redshift Infrared-Luminous Galaxies (2004)

Carilli, C. L., Solomon, P., Bout, P. Vanden, Walter, F., Beelen, Alexandre, Cox, Pierre, ...

We present a search for HCN emission from four high redshift far infrared (IR) luminous galaxies. Current data and models suggest that these high $z$ IR luminous galaxies represent a major starburst...

Radio continuum imaging of FIR luminous QSOs at z>6 (2004)

Carilli, C. L., Walter, F., Bertoldi, F., Menten, K. M., Fan, X., Lewis, G. F., ...

We present sensitive imaging at 1.4 GHz of the two highest redshift far-infrared (FIR) luminous QSOs SDSS J114816.65+525150.2 (z=6.42) and SDSS J104845.05+463718.3 (z=6.2). Radio continuum emission...

Starburst activity in the host galaxy of the z=2.58 quasar J1409+5628 (2004)

Beelen, A., Cox, P., Pety, J., Carilli, C. L., Bertoldi, F., Momjian, E., ...

We report the detection of CO emission from the optically luminous, radio-quiet quasar J140955.5+562827, at a redshift z_CO =2.583. We also present VLA continuum mapping results and VLBA high spatial...

Submillimeter Galaxies as Tracers of Mass Assembly at Large M (2004)

Genzel, R., Baker, A. J., Ivison, R. J., Bertoldi, F., Blain, A. W., Chapman, S. C., ...

Luminous submillimeter galaxies (SMGs) have been known for some time to produce a substantial fraction of the far-IR/submillimeter background. New observations show that these systems are not only...

Molecular gas in high redshift QSOs (2004)

Carilli, C. L., Bertoldi, F., Walter, F., Menten, K. M., Beelen, A., Cox, P., ...

We review cm and mm observations of thermal molecular line emission from high redshift QSOs. These observations reveal the massive gas reservoirs (10^{10} to 10^{11} M_sun) required to fuel star...

86 GHz SiO maser survey of late-type stars in the Inner Galaxy II. Infrared photometry of the SiO Target Stars (2004)

Messineo, M., Habing, H. J., Menten, K. M., Omont, A., Sjouwerman, L. O.

We present a compilation and study of DENIS, 2MASS, ISOGAL, MSX and IRAS 1--25 micron photometry for a sample of 441 late-type stars in the inner Galaxy, which we previously searched for 86 GHz SiO...

86 GHz SiO maser survey of late-type stars in the Inner Galaxy II. Infrared photometry of the SiO Target Stars (2004)

Messineo, M., Habing, H. J., Menten, K. M., Omont, A., Sjouwerman, L. O.

We present a compilation and study of DENIS, 2MASS, ISOGAL, MSX and IRAS 1--25 micron photometry for a sample of 441 late-type stars in the inner Galaxy, which we previously searched for 86 GHz SiO...

Starburst activity in the host galaxy of the z=2.58 quasar J1409+5628 (2004)

Beelen, A., Cox, P., Pety, J., Carilli, C. L., Bertoldi, F., Momjian, E., ...

We report the detection of CO emission from the optically luminous, radio-quiet quasar J140955.5+562827, at a redshift z_CO =2.583. We also present VLA continuum mapping results and VLBA high spatial...

Radio continuum imaging of FIR luminous QSOs at z>6 (2004)

Carilli, C. L., Walter, F., Bertoldi, F., Menten, K. M., Fan, X., Lewis, G. F., ...

We present sensitive imaging at 1.4 GHz of the two highest redshift far-infrared (FIR) luminous QSOs SDSS J114816.65+525150.2 (z=6.42) and SDSS J104845.05+463718.3 (z=6.2). Radio continuum emission...

A Search for Dense Molecular Gas in High Redshift Infrared-Luminous Galaxies (2004)

Carilli, C. L., Solomon, P., Bout, P. Vanden, Walter, F., Beelen, Alexandre, Cox, Pierre, ...

We present a search for HCN emission from four high redshift far infrared (IR) luminous galaxies. Current data and models suggest that these high $z$ IR luminous galaxies represent a major starburst...

Atomic carbon in PSS 2322+1944, a quasar at redshift 4.12 (2004)

Pety, J., Beelen, A., Cox, P., Downes, D., Omont, A., Bertoldi, F., ...

We report the detection of the 3P1 to 3P0 fine-structure line of neutral carbon in the z=4.12 quasar PSS 2322+1944, obtained at the IRAM Plateau de Bure interferometer. The CI 3P1-3P0 line is...

86 GHz SiO maser survey of late-type stars in the Inner Galaxy II. Infrared photometry of the SiO Target Stars (2004)

Messineo, M., Habing, H. J., Menten, K. M., Omont, A., Sjouwerman, L. O.

We present a compilation and study of DENIS, 2MASS, ISOGAL, MSX and IRAS 1--25 micron photometry for a sample of 441 late-type stars in the inner Galaxy, which we previously searched for 86 GHz SiO...

Starburst activity in the host galaxy of the z=2.58 quasar J1409+5628 (2004)

Beelen, A., Cox, P., Pety, J., Carilli, C. L., Bertoldi, F., Momjian, E., ...

We report the detection of CO emission from the optically luminous, radio-quiet quasar J140955.5+562827, at a redshift z_CO =2.583. We also present VLA continuum mapping results and VLBA high spatial...

Radio continuum imaging of FIR luminous QSOs at z>6 (2004)

Carilli, C. L., Walter, F., Bertoldi, F., Menten, K. M., Fan, X., Lewis, G. F., ...

We present sensitive imaging at 1.4 GHz of the two highest redshift far-infrared (FIR) luminous QSOs SDSS J114816.65+525150.2 (z=6.42) and SDSS J104845.05+463718.3 (z=6.2). Radio continuum emission...

A Search for Dense Molecular Gas in High Redshift Infrared-Luminous Galaxies (2004)

Carilli, C. L., Solomon, P., Bout, P. Vanden, Walter, F., Beelen, Alexandre, Cox, Pierre, ...

We present a search for HCN emission from four high redshift far infrared (IR) luminous galaxies. Current data and models suggest that these high $z$ IR luminous galaxies represent a major starburst...

Atomic carbon in PSS 2322+1944, a quasar at redshift 4.12 (2004)

Pety, J., Beelen, A., Cox, P., Downes, D., Omont, A., Bertoldi, F., ...

We report the detection of the 3P1 to 3P0 fine-structure line of neutral carbon in the z=4.12 quasar PSS 2322+1944, obtained at the IRAM Plateau de Bure interferometer. The CI 3P1-3P0 line is...

The European Large-Area ISO Survey (ELAIS): the final band-merged catalogue (2004)

Rowan-Robinson, M., Lari, C., Perez-Fournon, I., Gonzalez-Solares, E. A., La Franca, F., Vaccari, M., ...

We present the final band-merged European Large-Area ISO Survey (ELAIS) Catalogue at 6.7, 15, 90 and 175 ‚‚mu;m, and the associated data at U, g', r', i', Z, J, H, K and 20 cm. The origin of the...

ELAIS: final band-merged catalogue (2004)

Rowan-Robinson, M., Lari, C., Perez-Fournon, I., Gonzalez-Solares, E. A., Franca, F. L., Vaccari, M., ...

The catalog represents the final band-merged European Large-Area ISO Survey (ELAIS) Catalogue at 6.7, 15, 90 and 175{mu}m, and the associated data at U, g', r', i', Z, J, H, K and 20cm. Details about...

High-excitation CO in a quasar host galaxy at z=6.42 (2003)

Bertoldi, F., Cox, P., Neri, R., Carilli, C. L., Walter, F., Omont, A., ...

We report the detection of high excitation CO emission from the most distant quasar currently known, SDSS J114816.64+525150.3 (hereafter J1148+5251), at a redshift z=6.419. The CO (J=6-5) and (J=7-6)...

Interferometric Observations of Powerful CO Emission from the three Submillimeter Galaxies at z=2.30, 2.51 and 3.35 (2003)

Neri, R., Genzel, R., Ivison, R. J., Bertoldi, F., Blain, A. W., Chapman, S. C., ...

We report IRAM Plateau de Bure, millimeter interferometry of three z=~2.4 to 3.4, SCUBA deep field galaxies. Our CO line observations confirm the rest-frame UV/optical redshifts, thus more than...

Dust emission from the most distant quasars (2003)

Bertoldi, F., Carilli, C. L., Cox, P., Fan, X., Strauss, M. A., Beelen, A., ...

We report observations of three SDSS z>6 QSOs at 250 GHz (1.2mm) using the 117-channel Max-Planck Millimeter Bolometer (MAMBO-2) array at the IRAM 30-meter telescope. J1148+5251 (z=6.41) and...

ISOGAL: A deep survey of the obscured inner Milky Way with ISO at 7 and 15 micron and with DENIS in the near-infrared (2003)

Omont, A., Gilmore, G., Alard, C., Aracil, B., August, T., Baliyan, K., ...

The ISOGAL project is an infrared survey of specific regions sampling the Galactic Plane selected to provide information on Galactic structure,stellar populations,stellar mass-loss and the recent...

Explanatory Supplement of the ISOGAL-DENIS Point Source Catalogue (2003)

Schuller, F., Ganesh, S., Messineo, M., Moneti, A., Alard, C., ...

We present version 1.0 of the ISOGAL-DENIS Point Source Catalogue (PSC), containing more than 100,000 point sources detected at 7 and/or 15 micron in the ISOGAL survey of the inner Galaxy with the...

Long Period Variables detected by ISO in the SMC (2003)

Cioni, M. -R. L., Groenewegen, M. A. T., Habing, H. J., Hron, J., Kerschbaum, F., ...

This article presents the study of the light-curves extracted from the MACHO database of a sample of stars observed by the ISO in the SMC. These stars belong to the ISO-Mini-Survey catalogue of the...

A Molecular Einstein Ring: Imaging a Starburst Disk Surrounding a Quasi-Stellar Object (2003)

Carilli, C. L., Lewis, G. F., Djorgovski, S. G., Mahabal, A., Cox, P., Bertoldi, F., ...

Images of the CO 2-1 line emission, and the radio continuum emission, from the redshift 4.12 gravitationally lensed quasi-stellar object (QSO) PSS J2322+1944 reveal an Einstein ring with a diameter...

Sensitive observations at 1.4 and 250 GHz of z > 5 QSOs (2003)

Petric, A. O., Carilli, C. L., Bertoldi, F., Fan, Xiaohui, Cox, P., Strauss, Michael A., ...

We present 1.4 and 5 GHz observations taken with the Very Large Array (VLA), and observations at 250 GHz obtained with the Max-Planck millimeter bolometer (MAMBO) at the IRAM 30~m telescope, of ten...

Near-IR spectra of ISOGAL sources in the Inner Galactic Bulge (2003)

Schultheis, M., Lançon, A., Omont, A., Schuller, F., Ojha, D. K.

In this work we present near-IR spectra (HK-band) of a sample of 107 sources with mid-IR excesses at 7 and 15 $\rm \mu$m detected during the ISOGAL survey. Making use of the DENIS interstellar...

Stellar sources in the ISOGAL intermediate bulge fields (2003)

Ojha, D. K., Omont, A., Schuller, F., Simon, G., Ganesh, S., Schultheis, M.

We present a study of ISOGAL sources in the "intermediate" galactic bulge ($|$$l$$|$ $

The ISOGAL field FC--01863+00035: Mid-IR interstellar extinction and stellar populations (2003)

Jiang, B. W., Omont, A., Ganesh, S., Simon, G., Schuller, F.

A 0.35\degr $\times$ 0.29\degr field centered at $l$=--18.63\degr, $b$=0.35\degr was observed during the ISOGAL survey by ISOCAM imaging at 7$\mu$m and 15{\rm $\mu$m}. 648 objects were detected and...

The ISOGAL field FC--01863+00035: Mid-IR interstellar extinction and stellar populations (2003)

Jiang, B. W., Omont, A., Ganesh, S., Simon, G., Schuller, F.

A 0.35\\degr $\\times$ 0.29\\degr field centered at $l$=--18.63\\degr, $b$=0.35\\degr was observed during the ISOGAL survey by ISOCAM imaging at 7$\\mu$m and 15{\\rm $\\mu$m}. 648 objects were...

Stellar sources in the ISOGAL intermediate bulge fields (2003)

Ojha, D. K., Omont, A., Schuller, F., Simon, G., Ganesh, S., Schultheis, M.

We present a study of ISOGAL sources in the \"intermediate\" galactic bulge ($|$$l$$|$ $

Near-IR spectra of ISOGAL sources in the Inner Galactic Bulge (2003)

Schultheis, M., Lançon, A., Omont, A., Schuller, F., Ojha, D. K.

In this work we present near-IR spectra (HK-band) of a sample of 107 sources with mid-IR excesses at 7 and 15 $\\rm \\mu$m detected during the ISOGAL survey. Making use of the DENIS interstellar...

Sensitive observations at 1.4 and 250 GHz of z > 5 QSOs (2003)

Petric, A. O., Carilli, C. L., Bertoldi, F., Fan, Xiaohui, Cox, P., Strauss, Michael A., ...

We present 1.4 and 5 GHz observations taken with the Very Large Array (VLA), and observations at 250 GHz obtained with the Max-Planck millimeter bolometer (MAMBO) at the IRAM 30~m telescope, of ten...

A Molecular Einstein Ring: Imaging a Starburst Disk Surrounding a Quasi-Stellar Object (2003)

Carilli, C. L., Lewis, G. F., Djorgovski, S. G., Mahabal, A., Cox, P., Bertoldi, F., ...

Images of the CO 2-1 line emission, and the radio continuum emission, from the redshift 4.12 gravitationally lensed quasi-stellar object (QSO) PSS J2322+1944 reveal an Einstein ring with a diameter...

Long Period Variables detected by ISO in the SMC (2003)

Cioni, M. -R. L., Groenewegen, M. A. T., Habing, H. J., Hron, J., Kerschbaum, F., ...

This article presents the study of the light-curves extracted from the MACHO database of a sample of stars observed by the ISO in the SMC. These stars belong to the ISO-Mini-Survey catalogue of the...

Explanatory Supplement of the ISOGAL-DENIS Point Source Catalogue (2003)

Schuller, F., Ganesh, S., Messineo, M., Moneti, A., Alard, C., ...

We present version 1.0 of the ISOGAL-DENIS Point Source Catalogue (PSC), containing more than 100,000 point sources detected at 7 and/or 15 micron in the ISOGAL survey of the inner Galaxy with the...

ISOGAL: A deep survey of the obscured inner Milky Way with ISO at 7 and 15 micron and with DENIS in the near-infrared (2003)

Omont, A., Gilmore, G., Alard, C., Aracil, B., August, T., Baliyan, K., ...

The ISOGAL project is an infrared survey of specific regions sampling the Galactic Plane selected to provide information on Galactic structure,stellar populations,stellar mass-loss and the recent...

Dust emission from the most distant quasars (2003)

Bertoldi, F., Carilli, C. L., Cox, P., Fan, X., Strauss, M. A., Beelen, A., ...

We report observations of three SDSS z>6 QSOs at 250 GHz (1.2mm) using the 117-channel Max-Planck Millimeter Bolometer (MAMBO-2) array at the IRAM 30-meter telescope. J1148+5251 (z=6.41) and...

Interferometric Observations of Powerful CO Emission from the three Submillimeter Galaxies at z=2.30, 2.51 and 3.35 (2003)

Neri, R., Genzel, R., Ivison, R. J., Bertoldi, F., Blain, A. W., Chapman, S. C., ...

We report IRAM Plateau de Bure, millimeter interferometry of three z=~2.4 to 3.4, SCUBA deep field galaxies. Our CO line observations confirm the rest-frame UV/optical redshifts, thus more than...

High-excitation CO in a quasar host galaxy at z=6.42 (2003)

Bertoldi, F., Cox, P., Neri, R., Carilli, C. L., Walter, F., Omont, A., ...

We report the detection of high excitation CO emission from the most distant quasar currently known, SDSS J114816.64+525150.3 (hereafter J1148+5251), at a redshift z=6.419. The CO (J=6-5) and (J=7-6)...

The ISOGAL field FC--01863+00035: Mid-IR interstellar extinction and stellar populations (2003)

Jiang, B. W., Omont, A., Ganesh, S., Simon, G., Schuller, F.

A 0.35\\degr $\\times$ 0.29\\degr field centered at $l$=--18.63\\degr, $b$=0.35\\degr was observed during the ISOGAL survey by ISOCAM imaging at 7$\\mu$m and 15{\\rm $\\mu$m}. 648 objects were...

Stellar sources in the ISOGAL intermediate bulge fields (2003)

Ojha, D. K., Omont, A., Schuller, F., Simon, G., Ganesh, S., Schultheis, M.

We present a study of ISOGAL sources in the \"intermediate\" galactic bulge ($|$$l$$|$ $

Near-IR spectra of ISOGAL sources in the Inner Galactic Bulge (2003)

Schultheis, M., Lançon, A., Omont, A., Schuller, F., Ojha, D. K.

In this work we present near-IR spectra (HK-band) of a sample of 107 sources with mid-IR excesses at 7 and 15 $\\rm \\mu$m detected during the ISOGAL survey. Making use of the DENIS interstellar...

Sensitive observations at 1.4 and 250 GHz of z > 5 QSOs (2003)

Petric, A. O., Carilli, C. L., Bertoldi, F., Fan, Xiaohui, Cox, P., Strauss, Michael A., ...

We present 1.4 and 5 GHz observations taken with the Very Large Array (VLA), and observations at 250 GHz obtained with the Max-Planck millimeter bolometer (MAMBO) at the IRAM 30~m telescope, of ten...

A Molecular Einstein Ring: Imaging a Starburst Disk Surrounding a Quasi-Stellar Object (2003)

Carilli, C. L., Lewis, G. F., Djorgovski, S. G., Mahabal, A., Cox, P., Bertoldi, F., ...

Images of the CO 2-1 line emission, and the radio continuum emission, from the redshift 4.12 gravitationally lensed quasi-stellar object (QSO) PSS J2322+1944 reveal an Einstein ring with a diameter...

Long Period Variables detected by ISO in the SMC (2003)

Cioni, M. -R. L., Groenewegen, M. A. T., Habing, H. J., Hron, J., Kerschbaum, F., ...

This article presents the study of the light-curves extracted from the MACHO database of a sample of stars observed by the ISO in the SMC. These stars belong to the ISO-Mini-Survey catalogue of the...

Explanatory Supplement of the ISOGAL-DENIS Point Source Catalogue (2003)

Schuller, F., Ganesh, S., Messineo, M., Moneti, A., Alard, C., ...

We present version 1.0 of the ISOGAL-DENIS Point Source Catalogue (PSC), containing more than 100,000 point sources detected at 7 and/or 15 micron in the ISOGAL survey of the inner Galaxy with the...

ISOGAL: A deep survey of the obscured inner Milky Way with ISO at 7 and 15 micron and with DENIS in the near-infrared (2003)

Omont, A., Gilmore, G., Alard, C., Aracil, B., August, T., Baliyan, K., ...

The ISOGAL project is an infrared survey of specific regions sampling the Galactic Plane selected to provide information on Galactic structure,stellar populations,stellar mass-loss and the recent...

Dust emission from the most distant quasars (2003)

Bertoldi, F., Carilli, C. L., Cox, P., Fan, X., Strauss, M. A., Beelen, A., ...

We report observations of three SDSS z>6 QSOs at 250 GHz (1.2mm) using the 117-channel Max-Planck Millimeter Bolometer (MAMBO-2) array at the IRAM 30-meter telescope. J1148+5251 (z=6.41) and...

Interferometric Observations of Powerful CO Emission from the three Submillimeter Galaxies at z=2.30, 2.51 and 3.35 (2003)

Neri, R., Genzel, R., Ivison, R. J., Bertoldi, F., Blain, A. W., Chapman, S. C., ...

We report IRAM Plateau de Bure, millimeter interferometry of three z=~2.4 to 3.4, SCUBA deep field galaxies. Our CO line observations confirm the rest-frame UV/optical redshifts, thus more than...

High-excitation CO in a quasar host galaxy at z=6.42 (2003)

Bertoldi, F., Cox, P., Neri, R., Carilli, C. L., Walter, F., Omont, A., ...

We report the detection of high excitation CO emission from the most distant quasar currently known, SDSS J114816.64+525150.3 (hereafter J1148+5251), at a redshift z=6.419. The CO (J=6-5) and (J=7-6)...

A 1.2 mm MAMBO/IRAM-30 m study of dust emission from optically luminous z approximate to 2 quasars (2003)

Omont, A., Beelen, A., Bertoldi, F., Cox, P., Carilli, C. L., Priddey, R. S., ...

We report 250 GHz (1.2 mm) observations of redshift 1.8 < z < 2.8 optically luminous (M-B < -27.0), radio quiet quasars using the Max-Planck Millimeter Bolometer (MAMBO) array at the IRAM 30-metre...

A molecular Einstein ring : imaging a starburst disk surrounding a quasi-stellar object (2003)

Carilli, C. L., Lewis, G. F., Djorgovski, S. G., Mahabal, A., Cox, P., Bertoldi, F., ...

Images of the molecular CO 2-1 line emission and the radio continuum emission from the redshift 4.12 gravitationally lensed quasi-stellar object (QSO) PSS J2322 + 1944 reveal an Einstein ring with a...

Dust emission from the most distant quasars (2003)

Bertoldi, F., Carilli, C. L., Cox, P., Fan, X., Strauss, M. A., Beelen, A., ...

We report observations of three SDSS z > 6 QSOs at 250 GHz (1.2 mm) using the 117-channel Max-Planck Millimeter Bolometer (MAMBO-2) array at the IRAM 30-meter telescope. J1148 + 5251 (z = 6.42) and...

High-excitation CO in a quasar host galaxy at z=6.42 (2003)

Bertoldi, F., Cox, P., Neri, R., Carilli, C. L., Walter, F., Omont, A., ...

We report the detection of high excitation CO emission from the most distant quasar currently known, SDSS J114816.64+525150.3 (hereafter J1148+5251), at a redshift z = 6.419. The CO (J = 6 --> 5) and...

Interferometric observations of powerful CO emission from three submillimeter galaxies at z=2.39, 2.51, and 3.35 (2003)

Neri, R., Genzel, R., Ivison, R. J., Bertoldi, F., Blain, A. W., Chapman, S. C., ...

We report IRAM millimeter interferometry of three zsimilar to2.4-3.4 Submillimeter Common-User Bolometric Array deep field galaxies. Our CO line observations confirm the rest-frame UV/optical...

Molecular gas in the host galaxy of a quasar at redshift z=6.42 (2003)

Walter, F., Bertoldi, F., Carilli, C., Cox, P., Lo, K. Y., Neri, R., ...

Observations of molecular hydrogen in quasar host galaxies at high redshifts provide fundamental constraints on galaxy evolution, because it is out of this molecular gas that stars form. Molecular...

Sensitive observations at 1.4 and 250 GHz of z > 5 QSOs (2003)

Petric, A. O., Carilli, C. L., Bertoldi, F., Fan, X. H., Cox, P., Strauss, M. A., ...

We present 1.4 and 5 GHz observations taken with the Very Large Array, and observations at 250 GHz obtained with the Max Planck Millimeter Bolometer Array at the IRAM 30 m telescope, of 10 optically...

Long period variables detected by ISO in the Small Magellanic Cloud. (2003)

Cioni, M-R.L., Groenewegen, M.A.T., Habing, H.J., Hron, J., Kerschbaum, F., ...

Original article can be found at: http://www.aanda.org/ Copyright The European Southern Observatory DOI: 10.1051/0004-6361:20030707

A 1.2mm MAMBO/IRAM-30m Study of Dust Emission from optically luminous z~2 Quasars (2002)

Omont, A., Beelen, A., Bertoldi, F., Cox, P., Carilli, C., Priddey, R. S., ...

We report 250GHz (1.2mm) observations of redshift 1.8 < z < 2.8 optically luminous (M_B < -27.0), radio quiet quasars using the Max-Planck Millimeter Bolometer (MAMBO) array at the IRAM 30-metre...

Mm/submm observations of symbiotic binary stars (2002)

Mikolajewska, J., Ivison, R. J., Omont, A.

We present and discuss mm/submm observations of quiescent S-type symbiotic systems, and compare them with popular models proposed to account for their radio emission. We find that the M giant...

Infrared stellar populations in the central parts of the Milky Way galaxy (2002)

Van Loon, Jacco Th., Gilmore, G. F., Omont, A., Glass, I. S., Messineo, M., ...

Near- and mid-IR survey data from DENIS and ISOGAL are used to investigate the structure and formation history of the inner 10 degree (1.4 kpc) of the Milky Way galaxy. Synthetic bolometric...

86 GHz SiO maser survey of late-type stars in the Inner Galaxy. I. Observational data (2002)

Messineo, M., Habing, H. J., Sjouwerman, L. O., Omont, A., Menten, K. M.

We present 86 GHz (v = 1, J = 2 -1) SiO maser line observations with the IRAM 30-m telescope of a sample of 441 late-type stars in the Inner Galaxy (-4 degr < l < +30 degr). These stars were selected...

Young massive stars in the ISOGAL survey II. The catalogue of bright YSO candidates (2002)

Felli, M., Testi, L., Schuller, F., Omont, A.

The 7 and 15 um observations of selected fields in the Galactic Plane obtained with ISOCAM during the ISOGAL program offer an unique possibility to search for previously unknown YSOs, undetected by...

Imaging low order CO emission from the z=4.12 QSO PSS 2322+1944 (2002)

Carilli, C., Cox, P., Bertoldi, F., Menten, K. M., Omont, A.

We present observations of CO 1-0 and CO 2-1 emission from the z = 4.12 QSO PSS 2322+1944 using the Very Large Array. The CO emission is extended on a spatial scale of 2''. This extension could...

CO and Dust in PSS2322+1944 at a redshift of 4.12 (2002)

Cox, P., Omont, A., Djorgovski, S. G., Bertoldi, F., Pety, J., Carilli, C. L., ...

Using the IRAM interferometer we have detected J=4-3 and 5-4 CO line emission toward the radio quiet quasar PSS2322+1944. At a redshift of z_CO=4.1199 this is the fourth and strongest detection of CO...

Low resolution spectroscopy of ISOGAL sources: Search for early-type stars with infrared excess (2002)

Schultheis, M., Parthasarathy, M., Omont, A., Cohen, M., Ganesh, S., Sevre, F., ...

An analysis of low resolution spectra and infared data of 29 ISOGAL-DENIS sources with mid-IR excess is presented. Eight ISOGAL sources from our sample with 7-15 micron excess are found to be B and...

Infrared stellar populations in the central parts of the Milky Way galaxy (2002)

Van Loon, Jacco Th., Gilmore, G. F., Omont, A., Glass, I. S., Messineo, M., ...

Near- and mid-IR survey data from DENIS and ISOGAL are used to investigate the structure and formation history of the inner 10 degree (1.4 kpc) of the Milky Way galaxy. Synthetic bolometric...

Low resolution spectroscopy of ISOGAL sources: Search for early-type stars with infrared excess (2002)

Schultheis, M., Parthasarathy, M., Omont, A., Cohen, M., Ganesh, S., Sevre, F., ...

An analysis of low resolution spectra and infared data of 29 ISOGAL-DENIS sources with mid-IR excess is presented. Eight ISOGAL sources from our sample with 7-15 micron excess are found to be B and...

CO and Dust in PSS2322+1944 at a redshift of 4.12 (2002)

Cox, P., Omont, A., Djorgovski, S. G., Bertoldi, F., Pety, J., Carilli, C. L., ...

Using the IRAM interferometer we have detected J=4-3 and 5-4 CO line emission toward the radio quiet quasar PSS2322+1944. At a redshift of z_CO=4.1199 this is the fourth and strongest detection of CO...

Imaging low order CO emission from the z=4.12 QSO PSS 2322+1944 (2002)

Carilli, C., Cox, P., Bertoldi, F., Menten, K. M., Omont, A.

We present observations of CO 1-0 and CO 2-1 emission from the z = 4.12 QSO PSS 2322+1944 using the Very Large Array. The CO emission is extended on a spatial scale of 2\'\'. This extension could...

Young massive stars in the ISOGAL survey II. The catalogue of bright YSO candidates (2002)

Felli, M., Testi, L., Schuller, F., Omont, A.

The 7 and 15 um observations of selected fields in the Galactic Plane obtained with ISOCAM during the ISOGAL program offer an unique possibility to search for previously unknown YSOs, undetected by...

86 GHz SiO maser survey of late-type stars in the Inner Galaxy. I. Observational data (2002)

Messineo, M., Habing, H. J., Sjouwerman, L. O., Omont, A., Menten, K. M.

We present 86 GHz (v = 1, J = 2 -1) SiO maser line observations with the IRAM 30-m telescope of a sample of 441 late-type stars in the Inner Galaxy (-4 degr < l < +30 degr). These stars were selected...

A 1.2mm MAMBO/IRAM-30m Study of Dust Emission from optically luminous z~2 Quasars (2002)

Omont, A., Beelen, A., Bertoldi, F., Cox, P., Carilli, C., Priddey, R. S., ...

We report 250GHz (1.2mm) observations of redshift 1.8 < z < 2.8 optically luminous (M_B < -27.0), radio quiet quasars using the Max-Planck Millimeter Bolometer (MAMBO) array at the IRAM 30-metre...

Infrared stellar populations in the central parts of the Milky Way galaxy (2002)

Van Loon, Jacco Th., Gilmore, G. F., Omont, A., Glass, I. S., Messineo, M., ...

Near- and mid-IR survey data from DENIS and ISOGAL are used to investigate the structure and formation history of the inner 10 degree (1.4 kpc) of the Milky Way galaxy. Synthetic bolometric...

Low resolution spectroscopy of ISOGAL sources: Search for early-type stars with infrared excess (2002)

Schultheis, M., Parthasarathy, M., Omont, A., Cohen, M., Ganesh, S., Sevre, F., ...

An analysis of low resolution spectra and infared data of 29 ISOGAL-DENIS sources with mid-IR excess is presented. Eight ISOGAL sources from our sample with 7-15 micron excess are found to be B and...

CO and Dust in PSS2322+1944 at a redshift of 4.12 (2002)

Cox, P., Omont, A., Djorgovski, S. G., Bertoldi, F., Pety, J., Carilli, C. L., ...

Using the IRAM interferometer we have detected J=4-3 and 5-4 CO line emission toward the radio quiet quasar PSS2322+1944. At a redshift of z_CO=4.1199 this is the fourth and strongest detection of CO...

Imaging low order CO emission from the z=4.12 QSO PSS 2322+1944 (2002)

Carilli, C., Cox, P., Bertoldi, F., Menten, K. M., Omont, A.

We present observations of CO 1-0 and CO 2-1 emission from the z = 4.12 QSO PSS 2322+1944 using the Very Large Array. The CO emission is extended on a spatial scale of 2\'\'. This extension could...

Young massive stars in the ISOGAL survey II. The catalogue of bright YSO candidates (2002)

Felli, M., Testi, L., Schuller, F., Omont, A.

The 7 and 15 um observations of selected fields in the Galactic Plane obtained with ISOCAM during the ISOGAL program offer an unique possibility to search for previously unknown YSOs, undetected by...

86 GHz SiO maser survey of late-type stars in the Inner Galaxy. I. Observational data (2002)

Messineo, M., Habing, H. J., Sjouwerman, L. O., Omont, A., Menten, K. M.

We present 86 GHz (v = 1, J = 2 -1) SiO maser line observations with the IRAM 30-m telescope of a sample of 441 late-type stars in the Inner Galaxy (-4 degr < l < +30 degr). These stars were selected...

A 1.2mm MAMBO/IRAM-30m Study of Dust Emission from optically luminous z~2 Quasars (2002)

Omont, A., Beelen, A., Bertoldi, F., Cox, P., Carilli, C., Priddey, R. S., ...

We report 250GHz (1.2mm) observations of redshift 1.8 < z < 2.8 optically luminous (M_B < -27.0), radio quiet quasars using the Max-Planck Millimeter Bolometer (MAMBO) array at the IRAM 30-metre...

Imaging low-order CO emission from the z = 4.12 quasi-stellar object PSS J2322+1944 (2002)

Carilli, C. L., Cox, P., Bertoldi, F., Menten, K. M., Omont, A., Djorgovski, S. G., ...

We present observations of CO (1-0) and CO (2-1) emission from the z = 4.12 quasi-stellar object (QSO) PSS J2322+1944 using the Very Large Array.(1) The CO emission is extended on a spatial scale of...

CO and dust in PSS 2322+1944 at a redshift of 4.12 (2002)

Cox, P., Omont, A., Djorgovski, S. G., Bertoldi, F., Pety, J., Carilli, C. L., ...

Using the IRAM interferometer we have detected J=4-->3 and 5-- >4 CO line emission toward the radio quiet quasar PSS 2322+1944. At a redshift of z(CO)=4.1199 this is the fourth and strongest...

86 GHz SiO maser survey of late-type stars in the Inner Galaxy - I. Observational data (2002)

Messineo, M., Habing, H. J., Sjouwerman, L. O., Omont, A., Menten, K. M.

We present 86 GHz (v = 1; J = 2 --> 1) SiO maser line observations with the IRAM 30-m telescope of a sample of 441 late-type stars in the Inner Galaxy ( -4degrees < 1 < +30degrees). These stars were...

The hydrodynamical structure of circumstellar envelopes around low mass-loss rate, low outflow velocity AGB stars (2002)

Winters, J. M., Le Bertre, T., Nyman, L. A., Omont, A., Jeong, K. S.

Recent hydrodynamical models (Winters et al. 2000b) allow the existence of pulsating, large velocity amplitude Asymptotic Giant Branch (AGB) stars with tenuous dusty circumstellar shells, which...

A 1.2mm MAMBO/IRAM-30m Survey of Dust Emission from the Highest Redshift PSS Quasars (2001)

Omont, A., Cox, P., Bertoldi, F., McMahon, R. G., Carilli, C., Isaak, K. G.

We report 250 GHz (1.2mm) observations of redshift > 3.8 quasars from the Palomar Sky Survey (PSS) sample, using the Max-Planck Millimetre Bolometer (MAMBO) array at the IRAM 30-metre telescope....

Radio Observations of Infrared Luminous High Redshift QSOs (2001)

Carilli, C. L., Bertoldi, F., Omont, A., Cox, P., McMahon, R. G., Isaak, K. G.

We present Very Large Array (VLA) observations at 1.4 GHz and 5 GHz of a sample of 12 Quasi-stellar Objects (QSOs) at z = 3.99 to 4.46. The sources were selected as the brightest sources at 250 GHz...

Mm/submm observations of symbiotic binary stars: implications for the mass loss and mass exchange (2001)

Mikolajewska, J., Ivison, R. J., Omont, A.

We discuss mm/submm spectra of a sample of symbiotic binary systems, and compare them with popular models proposed to account for their radio emission. We find that radio emission from quiescent...

Mass-Losing Semiregular Variable Stars in Baade's Windows (2001)

Alard, C., Blommaert, J., Cesarsky, C., Epchtein, N., Felli, M., Fouque, P., ...

By cross-correlating the results of two recent large-scale surveys, the general properties of a well defined sample of semi-regular variable stars have been determined. ISOGAL mid-infrared photometry...

A 1.2mm MAMBO/IRAM-30m Survey of Dust Emission from the Highest Redshift PSS Quasars (2001)

Omont, A., Cox, P., Bertoldi, F., McMahon, R. G., Carilli, C., Isaak, K. G.

We report 250 GHz (1.2mm) observations of redshift > 3.8 quasars from the Palomar Sky Survey (PSS) sample, using the Max-Planck Millimetre Bolometer (MAMBO) array at the IRAM 30-metre telescope....

Mass-Losing Semiregular Variable Stars in Baade's Windows (2001)

Alard, C., Blommaert, J., Cesarsky, C., Epchtein, N., Felli, M., Fouque, P., ...

By cross-correlating the results of two recent large-scale surveys, the general properties of a well defined sample of semi-regular variable stars have been determined. ISOGAL mid-infrared photometry...

Radio Observations of Infrared Luminous High Redshift QSOs (2001)

Carilli, C. L., Bertoldi, F., Omont, A., Cox, P., McMahon, R. G., Isaak, K. G.

We present Very Large Array (VLA) observations at 1.4 GHz and 5 GHz of a sample of 12 Quasi-stellar Objects (QSOs) at z = 3.99 to 4.46. The sources were selected as the brightest sources at 250 GHz...

A 1.2mm MAMBO/IRAM-30m Survey of Dust Emission from the Highest Redshift PSS Quasars (2001)

Omont, A., Cox, P., Bertoldi, F., McMahon, R. G., Carilli, C., Isaak, K. G.

We report 250 GHz (1.2mm) observations of redshift > 3.8 quasars from the Palomar Sky Survey (PSS) sample, using the Max-Planck Millimetre Bolometer (MAMBO) array at the IRAM 30-metre telescope....

Mass-Losing Semiregular Variable Stars in Baade's Windows (2001)

Alard, C., Blommaert, J., Cesarsky, C., Epchtein, N., Felli, M., Fouque, P., ...

By cross-correlating the results of two recent large-scale surveys, the general properties of a well defined sample of semi-regular variable stars have been determined. ISOGAL mid-infrared photometry...

Radio Observations of Infrared Luminous High Redshift QSOs (2001)

Carilli, C. L., Bertoldi, F., Omont, A., Cox, P., McMahon, R. G., Isaak, K. G.

We present Very Large Array (VLA) observations at 1.4 GHz and 5 GHz of a sample of 12 Quasi-stellar Objects (QSOs) at z = 3.99 to 4.46. The sources were selected as the brightest sources at 250 GHz...

A deep submillimetre survey of the Galactic Centre (2000)

Pierce-Price, D., Richer, J. S., Greaves, J. S., Holland, W. S., Jenness, T., Lasenby, A. N., ...

We present first results from a submillimetre continuum survey of the Galactic Centre `Central Molecular Zone' (CMZ), made with SCUBA on the James Clerk Maxwell Telescope. SCUBA's scan-map mode has...

The DENIS Point Source Catalogue towards the Magellanic Clouds (2000)

Cioni, M-R., Loup, C., Habing, H. J., Fouque', P., Bertin, E., Deul, E., ...

We have compiled the near infrared Point Source Catalogue (PSC) towards the Magellanic Clouds (MCs) extracted from the data obtained with the Deep Near Infrared Survey of the Southern Sky - DENIS...

The DENIS Point Source Catalogue towards the Magellanic Clouds (2000)

Cioni, M-R., Loup, C., Habing, H. J., Fouque', P., Bertin, E., Deul, E., ...

We have compiled the near infrared Point Source Catalogue (PSC) towards the Magellanic Clouds (MCs) extracted from the data obtained with the Deep Near Infrared Survey of the Southern Sky - DENIS...

A deep submillimetre survey of the Galactic Centre (2000)

Pierce-Price, D., Richer, J. S., Greaves, J. S., Holland, W. S., Jenness, T., Lasenby, A. N., ...

We present first results from a submillimetre continuum survey of the Galactic Centre `Central Molecular Zone\' (CMZ), made with SCUBA on the James Clerk Maxwell Telescope. SCUBA\'s scan-map mode has...

The DENIS Point Source Catalogue towards the Magellanic Clouds (2000)

Cioni, M-R., Loup, C., Habing, H. J., Fouque', P., Bertin, E., Deul, E., ...

We have compiled the near infrared Point Source Catalogue (PSC) towards the Magellanic Clouds (MCs) extracted from the data obtained with the Deep Near Infrared Survey of the Southern Sky - DENIS...

A deep submillimetre survey of the Galactic Centre (2000)

Pierce-Price, D., Richer, J. S., Greaves, J. S., Holland, W. S., Jenness, T., Lasenby, A. N., ...

We present first results from a submillimetre continuum survey of the Galactic Centre `Central Molecular Zone\' (CMZ), made with SCUBA on the James Clerk Maxwell Telescope. SCUBA\'s scan-map mode has...

Asymptotic giant branch stars in the ISOGAL survey (2000)

Ojha, D. K, Omont, A, Simon, G, Blommaert, J

We present and analyse the data of a field at 1 = 0o, b = +1o from the ISOGAL survey of selected areas of the inner Galactic bulge at 15 and 7 ?m. In combination with IJKs data from the near-infrared...

Spectroscopic observations of first ISOGAL sources (2000)

Ojha, D. K, Sivarani, T, Parthasarathy, M, Omont, A, Ganesh, S, Simon, G

Infrared Space Observatory Galactic (ISOGAL) survey at 7 and 15 μm of ~ 22 deg2 of the inner galactic disk and bulge, has detected several hundred thousand sources. Combining ISOGAL survey with I,...

The DENIS Point Source Catalogue towards the Magellanic Clouds. (2000)

Cioni, M-R.L., Loup, C., Habing, H.J., Fouque, P., Bertin, E., Deul, E., ...

Original article can be found at: http://www.aanda.org/ Copyright The European Southern Observatory DOI: 10.1051/aas:2000210

DENIS and ISOGAL properties of variable star candidates in the Galactic Bulge (2000)

M. Schultheis, S. Ganesh, I. S. Glass, A. Omont, R. Ortiz, G. Simon, ...

. Repeated DENIS observations (summer 1996 & 1998) in the J (1.25 m) and the K S (2.15 m) bands are used to look for variable stars. We present two catalogues of 1000 probable variables in an...

2.4 - 197 micron spectroscopy of OH/IR stars: The IR characteristics of circumstellar dust in O-rich environments (1999)

Sylvester, R. J., Kemper, F., Barlow, M. J., De Jong, T., ...

Infrared spectra of a number of evolved O-rich stars have been obtained with the Short- and Long- Wavelength spectrometers on board the Infrared Space Observatory. The very broad wavelength coverage...

Interstellar extinction towards the inner Galactic Bulge (1999)

Schultheis, M., Ganesh, S., Simon, G., Omont, A., Alard, C., Borsenberger, J., ...

DENIS observations in the J (1.2 micron) and K_S (2.15 micron) bands together with isochrones calculated for the RGB and AGB phase are used to draw an extinction map of the inner Galactic Bulge. The...

CO(4-3) and dust emission in two powerful high-z radio galaxies, and CO lines at high redshifts (1999)

Papadopoulos, Padeli P., Rottgering, H. J. A., Van Der Werf, P. P., Guilloteau, S., Omont, A., ...

We report the detection of sub-mm emission from dust at 850 microns and of the 12CO J=4-3 line in the two distant powerful radio galaxies 4C 60.07 (z=3.79) and 6C 1909+722 (z=3.53). In the case of 4C...

ISOGAL-DENIS detection of red giants with weak mass loss in the Galactic Bulge (1999)

Omont, A., Ganesh, S., Alard, C., Caillaud, B., Copet, E., ...

The ISOGAL project is a survey of the stellar populations, structure, and recent star formation history of the inner disk and bulge of the Galaxy. ISOGAL combines 15 and 7micron ISOCAM observations...

ISOGAL Survey of Baade's Windows in the Mid-infrared (1999)

Glass, I. S, Ganesh, S., Alard, C., Gilmore, G., Evans, T. Lloyd, ...

The ISOGAL mid-infrared survey of areas close to the Galactic Plane aims to determine their stellar content and its possible bearing on the history of the Galaxy. The NGC6522 and Sgr I Baade's...

CO lines in high redshift galaxies: perspective for future mm instruments (1999)

Combes, F., Maoli, R., Omont, A.

Nearly 10 high redshift (z>2) starburst galaxies have recently been detected in the CO lines, revealing the early presence in the universe of objects with large amounts of already-enriched molecular...

CO lines in high redshift galaxies: perspective for future mm instruments (1999)

Combes, F., Maoli, R., Omont, A.

Nearly 10 high redshift (z>2) starburst galaxies have recently been detected in the CO lines, revealing the early presence in the universe of objects with large amounts of already-enriched molecular...

ISOGAL Survey of Baade\'s Windows in the Mid-infrared (1999)

Glass, I. S, Ganesh, S., Alard, C., Gilmore, G., Evans, T. Lloyd, ...

The ISOGAL mid-infrared survey of areas close to the Galactic Plane aims to determine their stellar content and its possible bearing on the history of the Galaxy. The NGC6522 and Sgr I Baade\'s...

ISOGAL-DENIS detection of red giants with weak mass loss in the Galactic Bulge (1999)

Omont, A., Ganesh, S., Alard, C., Caillaud, B., Copet, E., ...

The ISOGAL project is a survey of the stellar populations, structure, and recent star formation history of the inner disk and bulge of the Galaxy. ISOGAL combines 15 and 7micron ISOCAM observations...

CO(4-3) and dust emission in two powerful high-z radio galaxies, and CO lines at high redshifts (1999)

Papadopoulos, Padeli P., Rottgering, H. J. A., Van Der Werf, P. P., Guilloteau, S., Omont, A., ...

We report the detection of sub-mm emission from dust at 850 microns and of the 12CO J=4-3 line in the two distant powerful radio galaxies 4C 60.07 (z=3.79) and 6C 1909+722 (z=3.53). In the case of 4C...

Interstellar extinction towards the inner Galactic Bulge (1999)

Schultheis, M., Ganesh, S., Simon, G., Omont, A., Alard, C., Borsenberger, J., ...

DENIS observations in the J (1.2 micron) and K_S (2.15 micron) bands together with isochrones calculated for the RGB and AGB phase are used to draw an extinction map of the inner Galactic Bulge. The...

2.4 - 197 micron spectroscopy of OH/IR stars: The IR characteristics of circumstellar dust in O-rich environments (1999)

Sylvester, R. J., Kemper, F., Barlow, M. J., De Jong, T., ...

Infrared spectra of a number of evolved O-rich stars have been obtained with the Short- and Long- Wavelength spectrometers on board the Infrared Space Observatory. The very broad wavelength coverage...

CO lines in high redshift galaxies: perspective for future mm instruments (1999)

Combes, F., Maoli, R., Omont, A.

Nearly 10 high redshift (z>2) starburst galaxies have recently been detected in the CO lines, revealing the early presence in the universe of objects with large amounts of already-enriched molecular...

ISOGAL Survey of Baade\'s Windows in the Mid-infrared (1999)

Glass, I. S, Ganesh, S., Alard, C., Gilmore, G., Evans, T. Lloyd, ...

The ISOGAL mid-infrared survey of areas close to the Galactic Plane aims to determine their stellar content and its possible bearing on the history of the Galaxy. The NGC6522 and Sgr I Baade\'s...

ISOGAL-DENIS detection of red giants with weak mass loss in the Galactic Bulge (1999)

Omont, A., Ganesh, S., Alard, C., Caillaud, B., Copet, E., ...

The ISOGAL project is a survey of the stellar populations, structure, and recent star formation history of the inner disk and bulge of the Galaxy. ISOGAL combines 15 and 7micron ISOCAM observations...

CO(4-3) and dust emission in two powerful high-z radio galaxies, and CO lines at high redshifts (1999)

Papadopoulos, Padeli P., Rottgering, H. J. A., Van Der Werf, P. P., Guilloteau, S., Omont, A., ...

We report the detection of sub-mm emission from dust at 850 microns and of the 12CO J=4-3 line in the two distant powerful radio galaxies 4C 60.07 (z=3.79) and 6C 1909+722 (z=3.53). In the case of 4C...

Interstellar extinction towards the inner Galactic Bulge (1999)

Schultheis, M., Ganesh, S., Simon, G., Omont, A., Alard, C., Borsenberger, J., ...

DENIS observations in the J (1.2 micron) and K_S (2.15 micron) bands together with isochrones calculated for the RGB and AGB phase are used to draw an extinction map of the inner Galactic Bulge. The...

2.4 - 197 micron spectroscopy of OH/IR stars: The IR characteristics of circumstellar dust in O-rich environments (1999)

Sylvester, R. J., Kemper, F., Barlow, M. J., De Jong, T., ...

Infrared spectra of a number of evolved O-rich stars have been obtained with the Short- and Long- Wavelength spectrometers on board the Infrared Space Observatory. The very broad wavelength coverage...

Deep Galaxy survey at 6.75 micron with the ISO satellite (1998)

Flores, H., Hammer, F., Désert, F. X., Césarsky, C., Thuan, T., Crampton, D., ...

Deep 6.75um mid-IR ISOCAM observations were obtained of the Canada-France Redshift Survey (CFRS) 1415+52 field with the Infrared Space Observatory. The identification of the sources with optical...

15um ISO observations of a CFRS field: the cosmic SFR as derived from UV, optical, mid-IR and radio photometry (1998)

Flores, H., Hammer, F., Thuan, T., Césarsky, C., Désert, F. X., Omont, A., ...

The CFRS 1452+52 field has been deeply imaged with the Infrared Space Observatory (ISO) using ISOCAM through the LW3 filter (12-18um). Careful data analysis and comparison to deep optical and radio...

The FIRBACK 175 micron Survey (1998)

Clements, David L., Puget, J-L, Lagache, G., Dole, H., Cox, P., Gispert, R., ...

The FIRBACK project is a collaboration of eight institutes aimed at using long wavelength surveys with ISO to uncover the nature of the Cosmic Far-Infrared Background. We have surveyed nearly 4 sq....

Deep Galaxy survey at 6.75 micron with the ISO satellite (1998)

Flores, H., Hammer, F., Désert, F. X., Césarsky, C., Thuan, T., Crampton, D., ...

Deep 6.75um mid-IR ISOCAM observations were obtained of the Canada-France Redshift Survey (CFRS) 1415+52 field with the Infrared Space Observatory. The identification of the sources with optical...

Deep Galaxy survey at 6.75 micron with the ISO satellite (1998)

Flores, H., Hammer, F., Désert, F. X., Césarsky, C., Thuan, T., Crampton, D., ...

Deep 6.75um mid-IR ISOCAM observations were obtained of the Canada-France Redshift Survey (CFRS) 1415+52 field with the Infrared Space Observatory. The identification of the sources with optical...

First ISOCAM images of the Milky Way (1996)

Perault, M, Omont, A, Simon, G, Seguin, P, Ojha, D, Blommaert, Joris; U0037630, ...

ISOGAL is a 15 mu m ISOCAM survey of similar to 12 deg(2) in the Galactic Plane interior to \l\ = 45 degrees. In combination with IJK data from the near-infrared southern sky survey DENIS, the ISO...

On the theory of collisions of atoms in rydberg states with neutral particles (1977)

Omont, A.

The theory of transitions between Rydberg states induced by thermal collisions, and of the broadening and shift of optical lines involving such states, is reconsidered. It is shown that the Fermi...

On the theory of collisions of atoms in rydberg states with neutral particles (1977)

Omont, A.

The theory of transitions between Rydberg states induced by thermal collisions, and of the broadening and shift of optical lines involving such states, is reconsidered. It is shown that the Fermi...

On the theory of collisions of atoms in rydberg states with neutral particles (1977)

Omont, A.

The theory of transitions between Rydberg states induced by thermal collisions, and of the broadening and shift of optical lines involving such states, is reconsidered. It is shown that the Fermi...

Study of Hg* (63 p1)-noble gas collisions in a 200 kG field range (1976)

Gay, J.C., Omont, A.

The study of Hg* (6 3P1)-rare gas collisions in a 200 kG range of magnetic field is reported. The results show that the collisional transfer rates between the m = 0 and the m = ± 1 Zeeman sublevels...

Study of Hg* (63 p1)-noble gas collisions in a 200 kG field range (1976)

Gay, J.C., Omont, A.

The study of Hg* (6 3P1)-rare gas collisions in a 200 kG range of magnetic field is reported. The results show that the collisional transfer rates between the m = 0 and the m = ± 1 Zeeman sublevels...

Study of Hg* (63 p1)-noble gas collisions in a 200 kG field range (1976)

Gay, J.C., Omont, A.

The study of Hg* (6 3P1)-rare gas collisions in a 200 kG range of magnetic field is reported. The results show that the collisional transfer rates between the m = 0 and the m = ± 1 Zeeman sublevels...

Influence d'un écart à la résonance sur les sections efficaces de collisions quasi résonnantes. I. cas d'un système à deux niveaux (1974)

Gay, J.C., Omont, A.

On étudie, dans le cadre d'une approximation à deux niveaux, l'effet d'un défaut de résonance sur la section efficace de collision dans le cas où le potentiel d'interaction varie en R-3 avec la...

Influence d'un écart à la résonance sur les sections efficaces de collisions quasi résonnantes. I. cas d'un système à deux niveaux (1974)

Gay, J.C., Omont, A.

On étudie, dans le cadre d'une approximation à deux niveaux, l'effet d'un défaut de résonance sur la section efficace de collision dans le cas où le potentiel d'interaction varie en R-3 avec la...

Influence d'un écart à la résonance sur les sections efficaces de collisions quasi résonnantes. I. cas d'un système à deux niveaux (1974)

Gay, J.C., Omont, A.

On étudie, dans le cadre d'une approximation à deux niveaux, l'effet d'un défaut de résonance sur la section efficace de collision dans le cas où le potentiel d'interaction varie en R-3 avec la...

Discussion théorique de l'élargissement par collisions des composantes Zeeman et hyperfines d'une raie optique (1973)

Omont, A.

On compare l'élargissement par collisions des composantes Zeeman d'une raie optique dans la zone (B ∼ 1 T) où leurs différences de fréquence sont beaucoup plus grandes que la largeur des...

Discussion théorique de l'élargissement par collisions des composantes Zeeman et hyperfines d'une raie optique (1973)

Omont, A.

On compare l'élargissement par collisions des composantes Zeeman d'une raie optique dans la zone (B ∼ 1 T) où leurs différences de fréquence sont beaucoup plus grandes que la largeur des...

Discussion théorique de l'élargissement par collisions des composantes Zeeman et hyperfines d'une raie optique (1973)

Omont, A.

On compare l'élargissement par collisions des composantes Zeeman d'une raie optique dans la zone (B ∼ 1 T) où leurs différences de fréquence sont beaucoup plus grandes que la largeur des...

Autoélargissement des courbes de croisement de niveaux observées en rétrodiffusion (niveau 6 3P1 du mercure). (1972)

Dodsworth, B.M., Gay, J.C., Omont, A.

Etude théorique et expérimentale de la largeur des signaux Hanle observés sur la lumière diffusée vers l'arrière par une vapeur de mercure, pour des pressions comprises entre 10-3 et 1 torr....

Autoélargissement des courbes de croisement de niveaux observées en rétrodiffusion (niveau 6 3P1 du mercure). (1972)

Dodsworth, B.M., Gay, J.C., Omont, A.

Etude théorique et expérimentale de la largeur des signaux Hanle observés sur la lumière diffusée vers l'arrière par une vapeur de mercure, pour des pressions comprises entre 10-3 et 1 torr....

Autoélargissement des courbes de croisement de niveaux observées en rétrodiffusion (niveau 6 3P1 du mercure). (1972)

Dodsworth, B.M., Gay, J.C., Omont, A.

Etude théorique et expérimentale de la largeur des signaux Hanle observés sur la lumière diffusée vers l'arrière par une vapeur de mercure, pour des pressions comprises entre 10-3 et 1 torr....

Effet de la dispersion anormale sur les signaux d'effet Hanle observés en diffusion vers l'arrière, sur le niveau 5 1P1 du cadmium (1970)

Crance, M., Omont, A.

Les signaux de croisement de niveaux sont visibles à des pressions de vapeur très élevées sur la lumière de résonance diffusée vers l'arrière dans toutes les directions par une vapeur. Au...

Effet de la dispersion anormale sur les signaux d'effet Hanle observés en diffusion vers l'arrière, sur le niveau 5 1P1 du cadmium (1970)

Crance, M., Omont, A.

Les signaux de croisement de niveaux sont visibles à des pressions de vapeur très élevées sur la lumière de résonance diffusée vers l'arrière dans toutes les directions par une vapeur. Au...

Effet de la dispersion anormale sur les signaux d'effet Hanle observés en diffusion vers l'arrière, sur le niveau 5 1P1 du cadmium (1970)

Crance, M., Omont, A.

Les signaux de croisement de niveaux sont visibles à des pressions de vapeur très élevées sur la lumière de résonance diffusée vers l'arrière dans toutes les directions par une vapeur. Au...