XMMU J134736.6+173403: an eclipsing LMXB in quiescence or a peculiar AGN? (2008)
Carpano, S., Altieri, B., King, A. R., Nucita, A., Leisy, P.
Aims. We report the discovery of a peculiar object observed serendipitously with XMM-Newton. We present its timing and spectral properties and investigate its optical counterpart. Methods. The light...
The first XMM-Newton slew survey catalogue: XMMSL1 (2008)
Saxton, R. D., Read, A. M., Esquej, P., Freyberg, M. J., Altieri, B., Bermejo, D.
We report on the production of a large area, shallow, sky survey, from XMM-Newton slews. The great collecting area of the mirrors coupled with the high quantum efficiency of the EPIC detectors have...
The first XMM-Newton slew survey catalogue: XMMSL1 (2008)
Saxton, R. D., Read, A. M., Esquej, P., Freyberg, M. J., Altieri, B., Bermejo, D.
The XMM-Newton medium-energy X-ray 'all-sky' survey (2008)
Saxton, R. D., Read, A. M., Freyberg, M. J., Esquej, P., Altieri, B.
Pacaud, F, Pierre, M, Adami, C, Altieri, B, Andreon, S, Chiappetti, L, ...
We present a sample of 29 galaxy clusters from the XMM-LSS survey over an area of some 5 deg(2) out to a redshift of z = 1.05. The sample clusters, which represent about half of the X-ray clusters...
ISO Observations of Seyfert Galaxies (2007)
B. Schulz, J. Clavel, B. Altieri, P. Barr, P. Claes, A. Heras, ...
Abstract. A list of 41 Active Galactic Nuclei (AGN) drawn from the CfA sample has been observed with the ISO satellite. The data set consists of 2.5-11.6 m low resolution (3000 km/s) spectra and...
Iso Soc Vilspa, K. Leech, B. Altieri, P. Claes, R. Laureijs, E. L. Martin, ...
. Teide 1 and Calar 3 are unique objects in being the first solitary Brown Dwarfs discovered. This point deserves stressing - they are not companions to other objects (in fact they are distant from...
Iso Data, B. Schulz, J. Clavel, B. Altieri, P. Barr, P. Claes, ...
We present low resolution spectrophotometric and imaging ISO observations of a sample of 58 AGN's over the 2.5--11.6 ¯m range. The data strongly support unification schemes and set new...
Design and Implementation of CIA, the ISOCAM Interactive Analysis System (2007)
S. Ott, Ott Abergel, B. Altieri, J-l. Augueres, H. Aussel, J-p. Bernard, ...
. This paper presents an overview of the Interactive Analysis System for ISOCAM (CIA). 10 With this system ISOCAM data can be analysed for calibration and engineering purposes, the ISOCAM pipeline...
The Infrared Spectrum Of Comet Hale-Bopp As Seen By The Infrared Space Observatory (2007)
K. Leech, J. Crovisier, T. Y. Brooke, M. S. Hanner, B. Altieri, ...
. Spectra of comet C/1995 O1 (Hale-Bopp) were obtained with the Infrared Space Observatory (ISO) at medium resolution with the grating spectrometer in the photometer (PHT-S) and/or at high resolution...
Iso Mid-Infrared Observations Of Abell 370 (2007)
Metcalfe Altieri Aussel, L. Metcalfe, B. Altieri, H. Aussel, A. Biviano, B. Mc Breen, ...
We report on the mid-IR imaging at 7 and 10 ¯m of the galaxy cluster Abell 370, obtained with the ISOCAM instrument onboard ESA's Infrared Space Observatory (ISO), as part of an ongoing program...
Ultimate Sensitivity With Isocam (2007)
Altieri Metcalfe And, B. Altieri, L. Metcalfe, J. Blommaert, D. Elbaz, ...
. We discuss the instrumental factors which constrain the sensitivity limits of the mid-infrared camera (ISOCAM) of ESA's Infrared Space Observatory (ISO). The observing strategy judged to be...
S. Ott, R. Gastaud, S. Guest, M. Delaney, B. Altieri, B. Ali, ...
. The ISOCAM Interactive Analysis System (CIA) is used to calibrate and to perform the astronomical data processing of ISOCAM, the infrared camera on board the Infrared Space Observatory (ISO). 1 ISO...
L. Metcalfe, B. Altieri, B. McBreen, J-p. Kneib, M. Delaney, A. Biviano, ...
We present imaging results and source counts from an ISOCAM deep and ultra-deep cosmological survey through gravitationally lensing clusters of galaxies at 7¯m and 15¯m. A total area of about 53...
The XMM-Large scale structure catalogue: X-ray sources and associated optical data. Version I (2007)
Pierre, M, Chiappetti, L, Pacaud, F, Gueguen, A, Libbrecht, C, Altieri, B, ...
Following the presentation of the XMM-Large Scale Structure (XMM-LSS) survey X-ray source detection package by Pacaud et al., we provide the source lists for the first surveyed 5.5 deg(2). The...
Pacaud, F., Pierre, M., Adami, C., Altieri, B., Andreon, S., Chiappetti, L., ...
We present a sample of 29 galaxy clusters from the XMM-LSS survey over an area of some 5deg2 out to a redshift of z=1.05. The sample clusters, which represent about half of the X-ray clusters...
The XMM-LSS catalogue: X-ray sources and associated optical data. Version I (2007)
Pierre, M., Chiappetti, L., Pacaud, F., Gueguen, A., Libbrecht, C., Altieri, B., ...
Following the presentation of the XMM-LSS X-ray source detection package by Pacaud et al., we provide the source lists for the first 5.5 surveyed square degrees. The catalogues pertain to the [0.5-2]...
The XMM-LSS Survey: A well controlled X-ray cluster sample over the D1 CFHTLS area (2007)
Pierre, M., Pacaud, F., Willis, J. P., Andreon, S., Valtchanov, I., ...
We present the XMM-LSS cluster catalogue corresponding to the CFHTLS D1 area. The list contains 13 spectroscopically confirmed, X-ray selected galaxy clusters over 0.8 deg2 to a redshift of unity and...
Candidate tidal disruption events from the XMM-Newton slew survey (2007)
Esquei, P., Saxton, R. D., Freyberg, M. J., Read, A. M., Altieri, B., Sanchez-Portal, M., ...
Candidate tidal disruption events from the XMM-Newton Slew Survey (2006)
Esquej, P., Saxton, R. D., Freyberg, M. J., Read, A. M., Altieri, B., Sanchez-Portal, M., ...
In recent years, giant amplitude X-ray flares have been observed from a handful of non-active galaxies. The most plausible scenario of these unusual phenomena is tidal disruption of a star by a...
The XMM Large-Scale Structure survey: the X-ray pipeline and survey selection function (2006)
Pacaud, F, Pierre, M, Refregier, A, Gueguen, A, Starck, JL, Valtchanov, I, ...
We present the X-ray pipeline developed for the purpose of the cluster search in the XMM Large-Scale Structure (XMM-LSS) survey. It is based on a two-stage procedure via a dedicated handling of the...
Pierre, M, Pacaud, F, Duc, PA, Willis, JP, Andreon, S, Valtchanov, I, ...
We present the XMM Large-Scale Structure Survey (XMM-LSS) cluster catalogue corresponding to the Canada-France-Hawaii Telescope Legacy Survey D1 area. The list contains 13 spectroscopically...
XMM-LSS discovery of a z = 1.22 galaxy cluster (2006)
Bremer, M. N., Valtchanov, I., Willis, J., Altieri, B., Andreon, S., Duc, P. A., ...
We present details of the discovery of XLSS J022303.0−043622, a z= 1.2 cluster of galaxies. This cluster was identified from its X-ray properties and selected as a z > 1 candidate from its...
XMM-LSS discovery of a z=1.22 galaxy cluster (2006)
Bremer, M. N., Valtchanov, I., Willis, J. P., Altieri, B., Andreon, S., Duc, P. A, ...
We present details of the discovery of XLSSJ022303.0-043622, a z=1.2 cluster of galaxies. This cluster was identified from its X-ray properties and selected as a z>1 candidate from its...
The XMM-LSS Survey: A well controlled X-ray cluster sample over the D1 CFHTLS area (2006)
Pierre, M., Pacaud, F., Willis, J. P., Andreon, S., Valtchanov, I., ...
We present the XMM-LSS cluster catalogue corresponding to the CFHTLS D1 area. The list contains 13 spectroscopically confirmed, X-ray selected galaxy clusters over 0.8 deg2 to a redshift of unity and...
The XMM Large Scale Structure survey: The X-ray pipeline and survey selection function (2006)
Pacaud, F., Pierre, M., Refregier, A., Gueguen, A., Valtchanov, I., ...
We present the X-ray pipeline developed for the purpose of the cluster search in the XMM-LSS survey. It is based on a two-stage procedure via a dedicated handling of the Poisson nature of the signal:...
Coia, D., Metcalfe, L., McBreen, B., Biviano, A., Smail, I., Altieri, B., ...
The massive cluster of galaxies Abell 2219 (z = 0.228) was observed at 14.3 $\mu$m with the Infrared Space Observatory and results were published by Barvainis et al. (1999). These observations have...
The XMM-LSS survey. Survey design and first results (2006)
Pierre, M., Valtchanov, I., Altieri, B., Andreon, S., Bolzonella, M., Bremer, M., ...
We have designed a medium deep large area X-ray survey with XMM - the XMM Large Scale Structure survey, XMM-LSS - with the scope of extending the cosmological tests attempted using ROSAT cluster...
Sluse, D, Claeskens, J-F, Altieri, B, Cabanac, R A, Garcet, O, Hutsemekers, Damien, ...
Aims.RXS J113155.4-123155 (z=0.66) is a quadruply imaged lensed quasar with a resolved Einstein Ring. The goal of this paper is to provide a full characterization of this system, and more...
Sluse, D, Claeskens, J*-F, Altieri, B, Cabanac, R A, Garcet, O, Hutsemekers, Damien, ...
Aims.RXS J113155.4-123155 (z=0.66) is a quadruply imaged lensed quasar with a resolved Einstein Ring. The goal of this paper is to provide a full characterization of this system, and more...
The XMM-Newton slew survey: a wide-angle survey in the 0.2-12KeV band (2006)
Freyberg, M. J., Altieri, B., Bermejo, D., Esquej, M. P., Lazaro, V., Read, A. M., ...
Status of the XMM-Newton cross-calibration with SASV6.5.0 (2006)
Stuhlinger, M., Altieri, B., Esquej, M. P., Kirsch, M. G. F., Metcalfe, L., Pollock, A. M. T., ...
The XMM-Newton slew survey towards the XMMSL1 catalogue (2006)
Esquej, M. P., Altieri, B., Bermejo, D., Freyberg, M. J., Lazaro, V., Read, A. M., ...
Extended sources in the XMM-Newton slew survey (2006)
Lazaro, V., Saxton, R., Read, A. M., Esquej, M. P., Freyberg, M. J., Altieri, B., ...
Sluse, D., Altieri, B., Cabanac, R. A., Garcet, O., Hutsemékers, D., ...
(abridged) Aims: RXS J113155.4-123155 (z=0.66) is a quadruply imaged lensed quasar with a resolved Einstein Ring. The goal of this paper is to provide a full characterization of this system, and more...
The XMM-Newton Slew Survey: a wide-angle survey in the 0.2 - 12 keV band (2005)
Freyberg, M. J., Altieri, B., Bermejo, D., Esquej, M. P., Lazaro, V., Read, A. M., ...
The scientific data collected during slews of the XMM-Newton satellite are used to construct a slew survey catalogue. This comprises of the order of 4000 sources detected in the EPIC-pn 0.2-12 keV...
The XMM-Newton Slew Survey: towards the XMMSL1 catalogue (2005)
Esquej, M. P., Altieri, B., Bermejo, D., Freyberg, M. J., Lazaro, V., Read, A. M., ...
The XMM-Newton satellite is the most sensitive X-ray observatory flown to date due to the great collecting area of its mirrors coupled with the high quantum efficiency of the EPIC detectors. It...
Status of the XMM-Newton cross-calibration with SASv6.5.0 (2005)
Stuhlinger, M., Altieri, B., Baskill, D., Dennerl, K., Esquej, M. P., Freyberg, M., ...
Further achievements of the XMM-Newton cross-calibration - XMM internal as well as with other X-ray missions - are presented. We explain the major changes in the new version SASv6.5 of the XMM-Newton...
Coia, D., Metcalfe, L., Mcbreen, B., Biviano, A., Altieri, B., Ott, S., ...
Observations of the core of the massive cluster Cl 0024+1654, at a redshift z=0.39, were obtained with the Infrared Space Observatory using ISOCAM at 6.7 mum and 14.3 mum (hereafter 15 mum). Thirty...
Extended sources in the XMM-Newton slew survey (2005)
Lazaro, V., Saxton, R., Read, A. M., Esquej, M. P., Freyberg, M. J., Altieri, B., ...
The low background, good spatial resolution and great sensitivity of the EPIC-pn camera on XMM-Newton give useful limits for the detection of extended sources even during the short exposures made...
Willis, JP, Pacaud, F, Valtchanov, I, Pierre, M, Ponman, T, Read, A, ...
We present X-ray and optical spectroscopic observations of 12 galaxy groups and clusters identified within the X-ray Multi-Mirror (XMM) Large-Scale Structure (LSS) survey. Groups and clusters are...
Clavel, J., Schulz, B., Altieri, B., Barr, P., Alloin, D., ...
Mid-infrared images of the Seyfert 1 galaxy Mrk 279 obtained with the ISO satellite are presented together with the results of a one-year monitoring campaign of the 2.5-11.7 micron spectrum....
The XMM-LSS Survey. First high redshift galaxy clusters: relaxed and collapsing systems (2005)
Valtchanov, I., Pierre, M., Willis, J., Santos, S. Dos, Jones, L., Andreon, S., ...
We present five newly found galaxy clusters at z>0.6 from the XMM Large-Scale Structure Survey (XMM-LSS). All five objects are extended X-ray sources in the XMM images. For three of them we have...
Processing challenges in the XMM-Newton slew survey (2005)
Saxton, R., Altieri, B., Read, A., Freyberg, M., Esquej, M. P., Bermejo, D.
The great collecting area of the mirrors coupled with the high quantum efficiency of the EPIC detectors have made XMM-Newton the most sensitive X-ray observatory flown to date. This is particularly...
Arnaud, M., Aghanim, N., Gastaud, R., Neumann, D. M., Lumb, D., Briel, U., ...
We present a temperature map and a temperature profile of the central part (r < 20\' or 1/4 virial radius) of the Coma cluster. We combined 5 overlapping pointings made with XMM/EPIC/MOS and...
Willis, J. P., Pacaud, F., Valtchanov, I., Pierre, M., Ponman, T., Read, A., ...
We present X-ray and optical spectroscopic observations of twelve galaxy groups and clusters identified within the XMM Large-Scale Structure (LSS) survey. Groups and clusters are selected as extended...
The XMM-Newton Slew Survey (2005)
Read, A. M., Saxton, R. D., Esquej, M. P., Freyberg, M. J., Altieri, B.
XMM-Newton, with the huge collecting area of its mirrors and the high quantum efficiency of its EPIC detectors, is the most sensitive X-ray observatory ever flown. This is strikingly evident during...
Batch discovery of nine z~1 clusters using x-ray and K or R,z' images (2005)
Andreon, S., Valtchanov, I., Jones, L. R., Altieri, B., Bremer, M., Willis, J., ...
We present results of an initial search for clusters of galaxies at z~1 and above, using data from 2.9 square degrees of XMM-Newton images. By selecting weak potentially extended X-ray sources with...
Optical and radio observations of a sample of 52 powerful ultra-steep spectrum radio sources (2005)
Ledoux, C., Melnick, J., Giraud, E., Kulkarni, V., Altieri, B.
We present the results of radio (VLA) and optical (ESO/La Silla) imaging of a sample of 52 radio sources having an ultra-steep radio spectrum with $\alpha$ mostly steeper than -1.1 at decimetre...
Optical and radio observations of a sample of 52 powerful ultra-steep spectrum radio sources (2005)
Ledoux, C., Melnick, J., Giraud, E., Kulkarni, V., Altieri, B.
We present the results of radio (VLA) and optical (ESO/La Silla) imaging of a sample of 52 radio sources having an ultra-steep radio spectrum with $\alpha$ mostly steeper than -1.1 at decimetre...
Optical and radio observations of a sample of 52 powerful ultra-steep spectrum radio sources (2005)
Ledoux, C., Melnick, J., Giraud, E., Kulkarni, V., Altieri, B.
We present the results of radio (VLA) and optical (ESO/La Silla) imaging of a sample of 52 radio sources having an ultra-steep radio spectrum with $\alpha$ mostly steeper than -1.1 at decimetre...
The XMM-Newton slew survey (2005)
Read, A.M., Saxton, R.D., Esquej, M.P., Freyberg, M.J., Altieri, B.
Health and cleanliness of the XMM-Newton science payload since launch (2005)
Kirsch, M. G., Abbey, A., Altieri, B., Baskill, D., Dennerl, K., Van Dooren, J., ...
XMM-Newton (cross-)calibration (2005)
Esquej, M. P., Saxton, R. D., Kirsch, M. G. F., Altieri, B., Freyberg, M. J., Haberl, F., ...
Optical and radio observations of a sample of 52 powerful ultra-steep spectrum radio sources (2005)
Ledoux, C., Melnick, J., Giraud, E., Kulkarni, V., Altieri, B.
We present the results of radio (VLA) and optical (ESO/La Silla) imaging of a sample of 52 radio sources having an ultra-steep radio spectrum with $\alpha$ mostly steeper than -1.1 at decimetre...
Optical and radio observations of a sample of 52 powerful ultra-steep spectrum radio sources (2005)
Ledoux, C., Melnick, J., Giraud, E., Kulkarni, V., Altieri, B.
We present the results of radio (VLA) and optical (ESO/La Silla) imaging of a sample of 52 radio sources having an ultra-steep radio spectrum with $\alpha$ mostly steeper than -1.1 at decimetre...
Coia, D., Metcalfe, L., McBreen, B., Biviano, A., Smail, I., Altieri, B., ...
The massive cluster of galaxies Abell 2219 (z = 0.228) was observed at 14.3 $\mu$m with the Infrared Space Observatory and results were published by Barvainis et al. (1999). These observations have...
The XMM-LSS survey - First high redshift galaxy clusters: Relaxed and collapsing systems (2004)
Valtchanov, I, Pierre, M, Willis, J, Dos Santos, S, Jones, L, Andreon, S, ...
We present five newly found galaxy clusters at z > 0.6 from the XMM Large-Scale Structure Survey (XMM-LSS). All five objects are extended X-ray sources in the XMM images. For three of them we have...
In-orbit performance of the EPIC-MOS detectors on XMM-Newton (2004)
Sembay, S., Abbey, A., Altieri, B., Ambrosi, R., Baskill, D., Ferrando, P., ...
XMM-Newton was launched into space on a highly eccentric 48 hour orbit on December 10th 1999. XMM-Newton is now in its fifth year of operation and has been an outstanding success, observing the...
XMM-Newton (cross)-calibration (2004)
Kirsch, M. G. F., Altieri, B., Chen, B., Haberl, F., Metcalfe, L., Pollock, A. M. T., ...
ESA's large X-ray space observatory XMM-Newton is in its fifth year of operations. We give a general overview of the status of calibration of the five X-ray instruments and the Optical Monitor. A...
ISOCAM Observations of Intermediate-redshift Galaxy Clusters at 7 and 15 microns (2004)
Perez-Martinez, R., Metcalfe, L., Coia, D., Biviano, A., McBreen, B., Altieri, B., ...
The gravitationally lensing clusters A370, A2218, A1689 and CL0024+1654 were observed with the Infrared Space Observatory (ISO) using ISOCAM at 6.7 and 14.3 microns (hereafter 7 and 15 microns...
Biviano, A., Metcalfe, L., McBreen, B., Altieri, B., Coia, D., Kessler, M. F., ...
We observed the cluster Abell 2218 (z=0.175), with ISOCAM on board the Infrared Space Observatory, using two filters with reference wavelengths of 6.7 and 14.3 microns. We detected 67 extragalactic...
Clusters of galaxies in the mid-infrared (2004)
Biviano, A., Metcalfe, L., Coia, D., McBreen, B., Altieri, B., Perez-Martinez, R., ...
We describe the results of observations of galaxy clusters conducted with ISOCAM on-board the Infrared Space Observatory. Our research is aimed at understanding the processes driving galaxy evolution...
Coia, D., Metcalfe, L., Mcbreen, B., Biviano, A., Altieri, B., Ott, S., ...
Observations of the core of the massive cluster Cl 0024+1654, at a redshift z=0.39, were obtained with the Infrared Space Observatory using ISOCAM at 6.7 mum and 14.3 mum (hereafter 15 mum). Thirty...
The XMM-LSS survey. Survey design and first results (2004)
Pierre, M., Valtchanov, I., Altieri, B., Andreon, S., Bolzonella, M., Bremer, M., ...
We have designed a medium deep large area X-ray survey with XMM - the XMM Large Scale Structure survey, XMM-LSS - with the scope of extending the cosmological tests attempted using ROSAT cluster...
The XMM-LSS Survey. First high redshift galaxy clusters: relaxed and collapsing systems (2004)
Valtchanov, I., Pierre, M., Willis, J., Santos, S. Dos, Jones, L., Andreon, S., ...
We present five newly found galaxy clusters at z>0.6 from the XMM Large-Scale Structure Survey (XMM-LSS). All five objects are extended X-ray sources in the XMM images. For three of them we have...
Coia, D., Metcalfe, L., McBreen, B., Biviano, A., Smail, I., Altieri, B., ...
The massive cluster of galaxies Abell 2219 (z = 0.228) was observed at 14.3 $\mu$m with the Infrared Space Observatory and results were published by Barvainis et al. (1999). These observations have...
Coia, D., Metcalfe, L., McBreen, B., Biviano, A., Smail, I., Altieri, B., ...
The massive cluster of galaxies Abell 2219 (z = 0.228) was observed at 14.3 $\mu$m with the Infrared Space Observatory and results were published by Barvainis et al. (1999). These observations have...
Coia, D., Metcalfe, L., Mcbreen, B., Biviano, A., Altieri, B., Ott, S., ...
Observations of the core of the massive cluster Cl 0024+1654, at a redshift z=0.39, were obtained with the Infrared Space Observatory using ISOCAM at 6.7 mum and 14.3 mum (hereafter 15 mum). Thirty...
The XMM-LSS survey. Survey design and first results (2004)
Pierre, M., Valtchanov, I., Altieri, B., Andreon, S., Bolzonella, M., Bremer, M., ...
We have designed a medium deep large area X-ray survey with XMM - the XMM Large Scale Structure survey, XMM-LSS - with the scope of extending the cosmological tests attempted using ROSAT cluster...
The XMM-LSS Survey. First high redshift galaxy clusters: relaxed and collapsing systems (2004)
Valtchanov, I., Pierre, M., Willis, J., Santos, S. Dos, Jones, L., Andreon, S., ...
We present five newly found galaxy clusters at z>0.6 from the XMM Large-Scale Structure Survey (XMM-LSS). All five objects are extended X-ray sources in the XMM images. For three of them we have...
XMM-Newton (cross)-calibration (2004)
Kirsch, M. F. G., Altieri, B., Chen, B., Haberl, F., Metcalfe, L., Pollock, A. M. T., ...
Coia, D., McBreen, B., Metcalfe, L., Biviano, A., Altieri, B., Ott, S., ...
Observations of the core of the massive cluster Cl 0024+1654, at a redshift z=0.39, were obtained with the Infrared Space Observatory using ISOCAM at 6.7 mum and 14.3 mum (hereafter 15 mum). Thirty...
An ISOCAM survey through gravitationally lensing galaxy clusters (2003)
Metcalfe, L., McBreen, B., Altieri, B., Biviano, A., Delaney, M., ...
ISOCAM was used to perform a deep survey through three gravitationally lensing clusters of galaxies. Nearly seventy sq. arcmin were covered over the clusters A370, A2218 and A2390. We present maps...
The XMM-LSS survey. Survey design and first results (2003)
Pierre, M., Valtchanov, I., Altieri, B., Andreon, S., Bolzonella, M., Bremer, M., ...
We have designed a medium deep large area X-ray survey with XMM - the XMM Large Scale Structure survey, XMM-LSS - with the scope of extending the cosmological tests attempted using ROSAT cluster...
The XMM-LSS Survey. First high redshift galaxy clusters: relaxed and collapsing systems (2003)
Valtchanov, I., Pierre, M., Willis, J., Santos, S. Dos, Jones, L., Andreon, S., ...
We present five newly found galaxy clusters at z>0.6 from the XMM Large-Scale Structure Survey (XMM-LSS). All five objects are extended X-ray sources in the XMM images. For three of them we have...
Status of the EPIC/MOS calibration (2002)
Ferrando, P., Abbey, A. F., Altieri, B., Arnaud, M., Bennie, P., Dadina, M., ...
The XMM-Newton observatory has the largest collecting area flown so far for an X-ray imaging system, resulting in a very high sensitivity over a broad spectral range. In order to exploit fully these...
ISO Observations of the dusty quasar BR1202-0725 (2001)
Leech, K. J., Metcalfe, L., Altieri, B.
We present mid- and far-IR photometry of the high-redshift (z=4.69) dusty quasar BR1202-0725. The quasar was detected in the near-IR, at a flux level (0.7+/-0.2 mJy) consistent with an average...
Clavel, J., Schulz, B., Altieri, B., Barr, P., Alloin, D., ...
Mid-infrared images of the Seyfert 1 galaxy Mrk 279 obtained with the ISO satellite are presented together with the results of a one-year monitoring campaign of the 2.5-11.7 micron spectrum....
Clavel, J., Schulz, B., Altieri, B., Barr, P., Alloin, D., ...
Mid-infrared images of the Seyfert 1 galaxy Mrk 279 obtained with the ISO satellite are presented together with the results of a one-year monitoring campaign of the 2.5-11.7 micron spectrum....
Clavel, J., Schulz, B., Altieri, B., Barr, P., Alloin, D., ...
Mid-infrared images of the Seyfert 1 galaxy Mrk 279 obtained with the ISO satellite are presented together with the results of a one-year monitoring campaign of the 2.5-11.7 micron spectrum....
XMM-Newton observation of the Lockman Hole; I. The X-ray Data (2000)
Hasinger, G., Altieri, B., Arnaud, M., Barcons, X., Bergeron, J., Brunner, H., ...
We report on the first deep X-ray survey with the XMM-Newton observatory during the performance verification phase. The field of the Lockman Hole, one of the best studied sky areas over a very wide...
Arnaud, M., Aghanim, N., Gastaud, R., Neumann, D. M., Lumb, D., Briel, U., ...
We present a temperature map and a temperature profile of the central part (r < 20' or 1/4 virial radius) of the Coma cluster. We combined 5 overlapping pointings made with XMM/EPIC/MOS and extracted...
Ultimate sensitivity with ISOCAM (2000)
Altieri, B, Metcalfe, L, Blommaert, Joris; U0037630, Elbaz, D, Starck, JL, Aussel, H
We discuss the instrumental factors which constrain the sensitivity limits of the midinfrared camera (ISOCAM) of ESA's Infrared Space Observatory (ISO). The observing strategy judged to be best...
ISO detection of a 60micron source near GRB970508 (2000)
Hanlon, L., Laureijs, R. J., Metcalfe, L., McBreen, B., Altieri, B., Castro-Tirado, A., ...
The Infrared Space Observatory observed the field of the $\gamma$--ray burst GRB 970508 with the CAM and PHT instruments on May 21 and 24, 1997 and with PHT in three filters in November 1997. A...
2.5-11 micron spectroscopy and imaging of AGNs: implication for unification schemes (2000)
Clavel, J., Schulz, B., Altieri, B., Barr, P., Claes, P., Heras, A., ...
We present 2.5-11 micron spectrophotometric & imaging ISO observations of 28 Sf1, 29 Sf2 & 1 normal galaxy. The Sf1 & Sf2 MIR spectra are statistically different: Sf1 have a strong power-law...
ISO detection of a 60 mu m source near GRB 970508 (2000)
Hanlon, L., Laureijs, R.J., Metcalfe, L., McBreen, B., Altieri, B., Castro-Tirado, A.J., ...
Arnaud, M., Aghanim, N., Gastaud, R., Neumann, D. M., Lumb, D., Briel, U., ...
We present a temperature map and a temperature profile of the central part (r < 20\' or 1/4 virial radius) of the Coma cluster. We combined 5 overlapping pointings made with XMM/EPIC/MOS and...
Arnaud, M., Aghanim, N., Gastaud, R., Neumann, D. M., Lumb, D., Briel, U., ...
We present a temperature map and a temperature profile of the central part (r < 20\' or 1/4 virial radius) of the Coma cluster. We combined 5 overlapping pointings made with XMM/EPIC/MOS and...
The infrared spectrum of comet Hale-Bopp as seen by the Infrared Space Observatory. (2000)
Sitko, M. L., Sprague, A. L., Lynch, D. K., Leech, K., Crovisier, J., Bockelee-Morvan, D., ...
An ISOCAM Mid-IR Survey through Gravitationally Lensing Galaxy Clusters (1999)
Biviano, A., Metcalfe, L., Altieri, B., Leech, K., Schulz, B., Kessler, M. F., ...
We present imaging results and source counts from a deep ISOCAM cosmological survey at 15 microns, through gravitationally lensing galaxy clusters. We take advantage of the cluster gravitational...
A ring galaxy at z = 1 lensed by the cluster Abell 370 (1999)
Altieri, B., Metcalfe, L., Bézecourt, J., Kneib, J. P., Soucail, G., Borgne, J. F. Le
Published in: Astron. Astrophys. 343 (1999) L70 citations recorded in [Science Citation Index] Abstract: We present a study of a very peculiar object found in the field of the cluster-lens Abell 370....
Metcalfe, L., Altieri, B., McBreen, B., Delaney, M., Biviano, A., ...
We present imaging results and source counts from an ISOCAM deep and ultra-deep cosmological survey through gravitationally lensing clusters of galaxies at 7 and 15 microns. A total area of about 53...
A ring galaxy at z=1 lensed by the cluster Abell 370 (1999)
Soucail, G., Kneib, J. P., Bezecourt, J., Metcalfe, L., Altieri, B., Borgne, J. F. Le
We present a study of a very peculiar object found in the field of the cluster-lens Abell 370. This object displays, in HST imaging, a spectacular morphology comparable to nearby ring-galaxies. From...
Ott, S, Gastaud, R, Guest, S, Delaney, M, Altieri, B, Ali, B, ...
Observations of GRBs with Infrared Space Observatory (1999)
Hanlon, L., Metcalfe, L., Delaney, M., Laureijs, R., McBreen, B., Smith, N., ...
The infrared spectrum of comet Hale-Bopp as seen by the Infrared Space Observatory. (1999)
Leech, K., Crovisier, J., Bockelée-Morvan, D., Brooke, T. Y., Hanner, M. S., Altieri, B., ...
The spectrum of comet Hale-Bopp as seen by ISO. (1999)
Cox, P., Kessler, M. F., Crovisier, J., Leech, K., Bockelée-Morvan, D., Lellouch, E., ...
An ultra-deep ISOCAM observation through a cluster-lens (1999)
B. Altieri, L. Metcalfe, J. P. Kneib, B. Mcbreen, H. Aussel, A. Biviano, ...
. We present results of ultra-deep ISOCAM observations through a cluster-lens at 7¯m and 15¯m with the Infrared Space Observatory (ISO) satellite. These observations reveal a large number of...
An ultra-deep ISOCAM observation through a cluster-lens (1998)
Altieri, B., Metcalfe, L., Kneib, J. P., McBreen, B., Aussel, H., Biviano, A., ...
We present results of ultra-deep ISOCAM observations through a cluster-lens at 7 and 15 micron with the Infrared Space Observatory (ISO) satellite. These observations reveal a large number of...
2.5-12 micron spectrophotometry and imaging of the CfA sample (1998)
Clavel, J., Schulz, B., Altieri, B., Barr, P., Claes, P., Heras, A., ...
We present low resolution spectrophotometric and imaging ISO observations of a sample of 54 AGN's over the 2.5-11 micron range. The observations generally support unification schemes and set new...
ISO Mid-Infrared Observations of Abell 370 (1998)
Metcalfe, L., Altieri, B., Aussel, H., Biviano, A., Breen, B. Mc, Delaney, M., ...
We report on the mid-IR imaging at 7 and 10 microns of the galaxy cluster Abell 370, obtained with the ISOCAM instrument onboard ESA's Infrared Space Observatory (ISO), as part of an ongoing program...
Deep ISOCAM Observations of Abell 2218 (1998)
Altieri, B., Metcalfe, L., Biviano, A., Leech, K., Okumura, K., Schulz, B., ...
We report on the mid-infrared imaging at 5, 7, 10 and 15 microns of the galaxy cluster Abell 2218 obtained with the ISOCAM instrument onboard ESA's Infrared Space Observatory (ISO), as part of an...
NGC5195 - A look into the hot dusty ISM of an interacting SB0 galaxy with ISOCAM (1996)
Boulade, O, Sauvage, M, Altieri, B, Blommaert, Joris; U0037630, Gallais, P, Guest, S, ...
We present broad-band images and a CVF spectrum of NGC5195, the companion of M51. NGC5195 appears as a very strong point source while its spectrum is dominated by the so-called PAH features at 6.2,...
NGC 5195 - A look into the hot dusty ISM of an interacting SB0 galaxy with ISOCAM (1996)
Boulade, O, Sauvage, M, Altieri, B, Blommaert, JADL, Gallais, P, Guest, S, ...