H. Aussel

Publication List Details

Period

1996 - 2009

Number

163

Co-Authors

The Build-Up of the Hubble Sequence in the COSMOS Field (2009)

Oesch, P. A., Carollo, C. M., Feldmann, R., Hahn, O., Lilly, S. J., Sargent, M. T., ...

We use ~8,600 >5e10 Msol COSMOS galaxies to study how the morphological mix of massive ellipticals, bulge-dominated disks, intermediate-bulge disks, bulge-less disks and irregular galaxies evolves...

Spitzer 70 and 160 μm Observations of the COSMOS Field (2009)

Frayer, D. T., Sanders, D. B., Surace, J. A., Aussel, H., Salvato, M., Le Floc'h, E., ...

We present Spitzer 70 and 160 μm observations of the COSMOS Spitzer survey (S-COSMOS). The data processing techniques are discussed for the publicly released products consisting of images and source...

The optical spectra of Spitzer 24 micron galaxies in the COSMOS field: II. Faint infrared sources in the zCOSMOS-bright 10k catalogue (2009)

Caputi, K. I., Lilly, S. J., Aussel, H., Floc'h, E. Le, Sanders, D., Maier, C., ...

We have used the zCOSMOS-bright 10k sample to identify 3244 Spitzer/MIPS 24-micron-selected galaxies with 0.06< S(24um)< 0.50 mJy and I(AB)

The COSMOS-WIRCam near-infrared imaging survey: I: BzK selected passive and star forming galaxy candidates at z>1.4 (2009)

McCracken, H. J., Capak, P., Salvato, M., Aussel, H., Thompson, D., Daddi, E., ...

(abridged) We present a new near-infrared survey covering the 2 deg sq COSMOS field. Combining our survey with Subaru B and z images we construct a deep, wide-field optical-infrared catalogue. At Ks

Spectroscopy of luminous z>7 galaxy candidates and sources of contamination in z>7 galaxy searches (2009)

Capak, P., Mobasher, B., Scoville, N. Z., McCracken, H., Ilbert, O., Salvato, M., ...

We present three bright z dropout candidates selected from deep Near-Infrared (NIR) imaging of the COSMOS 2 square degree field. All three objects match the 0.8-8um colors of other published z>7...

The zCOSMOS survey: the role of the environment in the evolution of the luminosity function of different galaxy types (2009)

Zucca, E., Bardelli, S., Bolzonella, M., Zamorani, G., Ilbert, O., Pozzetti, L., ...

(Abridged) We studied the evolution in the B band luminosity function to z~1 in the zCOSMOS 10k sample, for which both accurate galaxy classifications and a detailed description of the local density...

Deep Spitzer 24mic COSMOS imaging -- I. The evolution of luminous dusty galaxies - Confronting the models (2009)

Floc'h, E. Le, Aussel, H., Ilbert, O., Riguccini, L., Frayer, D., Salvato, M., ...

We present the first results obtained from the identification of ~30,000 sources in the 24mic observations of the COSMOS field at S24>~80muJy. Using accurate photo-z's and extrapolations of the...

Stellar and Total Baryon Mass Fractions in Groups and Clusters Since Redshift 1 (2009)

Giodini, S., Pierini, D., Finoguenov, A., Pratt, G. W., Boehringer, H., Leauthaud, A., ...

We investigate if the discrepancy between estimates of the total baryon mass fraction obtained from observations of the cosmic microwave background (CMB) and of galaxy groups/clusters persists when a...

High-redshift elliptical galaxies: are they (all) really compact? (2009)

Mancini, C., Daddi, E., Renzini, A., Salmi, F., McCracken, H. J., Cimatti, A., ...

We investigate the properties of 12 ultra-massive passively evolving early type galaxies (ETGs) at z_phot>1.4 in the COSMOS 2 deg^2 field. These 12 ETGs were selected as pBzKs, have accurate 1.4

Designing future dark energy space missions. I. Building realistic galaxy spectro-photometric catalogs and their first applications (2009)

Jouvel, S., Ilbert, O., Bernstein, G., Arnouts, S., Dahlen, T., ...

Context. Future dark energy space missions such as JDEM and EUCLID are being designed to survey the galaxy population to trace the geometry of the universe and the growth of structure, which both...

Hubble Space Telescope/Advanced Camera for Surveys Morphology of Lyα Emitters at Redshift 5.7 in the COSMOS Field (2009)

Taniguchi, Y., Murayama, T., Scoville, N. Z., Sasaki, S. S., Nagao, T., Shioya, Y., ...

We present detailed morphological properties of Lyα emitters (LAEs) at z ≈ 5.7 in the COSMOS field based on Hubble Space Telescope Advanced Camera for Surveys (ACS) data. The ACS imaging in the...

Environmental Effects on the Star Formation Activity in Galaxies at z ≃ 1.2 in the COSMOS Field (2009)

Ideue, Y., Nagao, T., Taniguchi, Y., Shioya, Y., Saito, T., Murayama, T., ...

We investigate the relation between the star formation activity in galaxies and environment at z ≃ 1.2 in the Cosmic Evolution Survey field, using the fraction of [O II] emitters and the local...

Tracking the impact of environment on the Galaxy Stellar Mass Function up to z~1 in the 10k zCOSMOS sample (2009)

Bolzonella, M., Kovac, K., Pozzetti, L., Zucca, E., Cucciati, O., Lilly, S. J., ...

We study the impact of the environment on the evolution of galaxies in the zCOSMOS 10k sample in the redshift range 0.1

Star Formation and Dust Obscuration at z ≈ 2: Galaxies at the Dawn of Downsizing (2009)

Pannella, M., Carilli, C. L., Daddi, E., McCracken, H. J., Owen, F. N., Renzini, A., ...

We present first results of a study aimed to constrain the star formation rate (SFR) and dust content of galaxies at z ≈ 2. We use a sample of BzK-selected star-forming galaxies, drawn from the...

HST/ACS Morphology of Lyman Alpha Emitters at Redshift 5.7 in the COSMOS Field (2009)

Taniguchi, Y., Murayama, T., Scoville, N. Z., Sasaki, S. S., Nagao, T., Shioya, Y., ...

We present detailed morphological properties of Lyman alpha emitters (LAEs) at z~ 5.7 in the COSMOS field, based on {\it Hubble Space Telescope} Advanced Camera for Surveys (ACS) data. The ACS...

Environmental Effects on the Star Formation Activity in Galaxies at z=1.2 in the COSMOS Field (2009)

Ideue, Y., Nagao, T., Taniguchi, Y., Shioya, Y., Saito, T., Murayama, T., ...

We investigate the relation between the star-formation activity in galaxies and environment at z=1.2 in the COSMOS field, using the fraction of [OII] emitters and the local galaxy density. The...

Star formation and dust obscuration at z~2: galaxies at the dawn of downsizing (2009)

Pannella, M., Carilli, C. L., Daddi, E., Cracken, H. J. Mc, Owen, F. N., Renzini, A., ...

We present first results of a study aimed to constrain the star formation rate and dust content of galaxies at z~2. We use a sample of BzK-selected star-forming galaxies, drawn from the COSMOS...

Photometric Properties of Lyα Emitters at z ≈ 4.86 in the COSMOS 2 Square Degree Field (2009)

Shioya, Y., Taniguchi, Y., Sasaki, S. S., Nagao, T., Murayama, T., Saito, T., ...

We present results of a survey for Lyα emitters at z ≈ 4.86 based on optical narrowband (λ_c = 7126 Å, Δλ = 73 Å) and broadband (B, V, r', i', and z') observations of the Cosmic Evolution...

Stellar and total baryon mass fractions in groups and clusters since redshift 1 (2009)

Giodini, S., Pierini, D., Finoguenov, A., Pratt, G. W., Boehringer, H., Leauthaud, A., ...

We investigate if the discrepancy between estimates of the total baryon mass fraction obtained from observations of the cosmic microwave background (CMB) and of galaxy groups/clusters persists when a...

Chasing highly obscured QSOs in the cosmos field (2009)

Fiore, F., Puccetti, S., Brusa, M., Salvato, M., Zamorani, G., Aldcroft, T., ...

A large population of heavily obscured, Compton-thick active galactic nuclei (AGNs) is predicted by AGN synthesis models for the cosmic X-ray background and by the "relic" supermassive black hole...

Galaxy Stellar Mass Assembly between 0.2 (2009)

Ilbert, O., Salvato, M., Floc'h, E. Le, Aussel, H., Capak, P., McCracken, H. J., ...

We follow the galaxy stellar mass assembly by morphological and spectral type in the COSMOS 2-deg^2 field. We derive the stellar mass functions and stellar mass densities from z=2 to z=0.2 using...

Spitzer 70 and 160-micron Observations of the COSMOS Field (2009)

Frayer, D. T., Sanders, D. B., Surace, J. A., Aussel, H., Salvato, M., Floc'h, E. Le, ...

We present Spitzer 70 and 160 micron observations of the COSMOS Spitzer survey (S-COSMOS). The data processing techniques are discussed for the publicly released products consisting of images and...

Designing Future Dark Energy Space Mission: I. Building Realistic Galaxy Spectro-Photometric Catalogs and their first applications (2009)

Jouvel, S., Kneib, J-P., Ilbert, O., Bernstein, G., Arnouts, S., Dahlen, T., ...

Future dark energy space missions such as JDEM and EUCLID are being designed to survey the galaxy population to trace the geometry of the universe and the growth of structure, which both depend on...

Photometric properties of Ly alpha emitters at z=4.86 in the COSMOS 2 square degree field (2009)

Shioya, Y., Taniguchi, Y., Sasaki, S. S., Nagao, T., Murayama, T., Saito, T., ...

We present results of a survey for Ly alpha emitters at z=4.86 based on optical narrowband (lambda_c=7126 angstrom, Delta lambda=73 angstrom) and broadband (B, V, r', i', and z') observations of the...

The close environment of 24 μm galaxies at 0.6 < z < 1.0 in the cosmos field (2009)

Caputi, K. I., Kovač, K., Bolzonella, M., Lilly, S. J., Zamorani, G., Aussel, H., ...

We investigate the close environment of 203 Spitzer 24 μm -selected sources at 0.6 < z < 1.0 using zCOSMOS-bright redshifts and spectra of I < 22.5 AB mag galaxies, over 1.5 deg^2 of the COSMOS...

Photometric Redshift and Classification for the XMM-COSMOS Sources (2009)

Salvato, M., Hasinger, G., Ilbert, O., Zamorani, G., Brusa, M., Scoville, N. Z., ...

We present photometric redshifts and spectral energy distribution (SED) classifications for a sample of 1542 optically identified sources detected with XMM in the COSMOS field. Our template fitting...

Cosmos Photometric Redshifts with 30-Bands for 2-deg^2 (2009)

Ilbert, O., Capak, P., Salvato, M., Aussel, H., McCracken, H. J., Sanders, D. B., ...

We present accurate photometric redshifts (photo-z) in the 2-deg^2 COSMOS field. The redshifts are computed with 30 broad, intermediate, and narrowbands covering the UV (Galaxy Evolution Explorer),...

Photometric redshift and classification for the XMM-COSMOS sources (2008)

Salvato, M., Hasinger, G., Ilbert, O., Zamorani, G., Brusa, M., Scoville, N., ...

We present photometric redshifts and spectral energy distribution (SED) classifications for a sample of 1542 optically identified sources detected with XMM in the COSMOS field. Our template fitting...

COSMOS Photometric Redshifts with 30-bands for 2-deg2 (2008)

Ilbert, O., Capak, P., Salvato, M., Aussel, H., McCracken, H. J., Sanders, D. B., ...

We present accurate photometric redshifts in the 2-deg2 COSMOS field. The redshifts are computed with 30 broad, intermediate, and narrow bands covering the UV (GALEX), Visible-NIR (Subaru, CFHT,...

The close environment of 24 micron galaxies at 0.6 (2008)

Caputi, K. I., Kovac, K., Bolzonella, M., Lilly, S. J., Zamorani, G., Aussel, H., ...

We investigate the close environment of 203 Spitzer 24 micron-selected sources at 0.6

Spectroscopic confirmation of an extreme starburst at redshift 4.547 (2008)

Capak, Peter, Carilli, C. L., Lee, N., Aldcroft, T., Aussel, H., Schinnerer, E., ...

We report the spectroscopic confirmation of a submillimeter galaxy (SMG) at z = 4.547 with an estimated LIR = (0.5–2.0) x 10¹³ L☉. The spectra, mid-IR, and X-ray properties indicate the...

A new method to separate star-forming from AGN galaxies at intermediate redshift : the submillijansky radio population in the VLA-COSMOS survey (2008)

Smolčić, V., Schinnerer, E., Scodeggio, M., Franzetti, P., Aussel, H., Bondi, M., ...

We explore the properties of the submillijansky radio population at 20 cm by applying a newly developed optical color-based method to separate star-forming (SF) from active galactic nucleus (AGN)...

The optical spectra of 24 μm galaxies in the COSMOS field. I. Spitzer MIPS bright sources in the zCOSMOS-bright 10k catalog (2008)

Caputi, K. I., Lilly, S. J., Aussel, H., Sanders, D., Frayer, D., Le Févre, O., ...

We study zCOSMOS-bright optical spectra for 609 Spitzer MIPS 24 μm-selected galaxies with S_(24) μ m > 0.30 mJy and I < 22.5 (AB mag) over 1.5 deg^2 of the COSMOS field. From emission-line...

Spectroscopic Confirmation Of An Extreme Starburst At Redshift 4.547 (2008)

Capak, Peter, Carilli, C. L., Lee, N., Aldcroft, T., Aussel, H., Schinnerer, E., ...

We report the spectroscopic confirmation of a sub-mm galaxy (SMG) at z=4.547 with an estimated L_IR=0.5-2.0x10^13 L_sun. The spectra, mid-IR, and X-ray properties indicate the bolometric luminosity...

A new method to separate star forming from AGN galaxies at intermediate redshift: The submillijansky radio population in the VLA-COSMOS survey (2008)

Smolcic, V., Schinnerer, E., Scodeggio, M., Franzetti, P., Aussel, H., Bondi, M., ...

We explore the properties of the submillijansky radio population at 20 cm by applying a newly developed optical color-based method to separate star forming (SF) from AGN galaxies at intermediate...

The Hα luminosity function and star formation rate at z ≈ 0.24 in the COSMOS 2 square degree field (2008)

Shioya, Y., Taniguchi, Y., Sasaki, S. S., Nagao, T., Murayama, T., Takahashi, M. I., ...

To derive a new Hα luminosity function and to understand the clustering properties of star-forming galaxies at z≈ 0.24, we have made a narrowband imaging survey for Hα-emitting galaxies in the...

A new method to separate star-forming from AGN galaxies at intermediate redshift. The submillijansky radio population in the VLA-COSMOS survey (2008)

Smolcic, V., Schinnerer, E., Scodeggio, M., Franzetti, P., Aussel, H., Bondi, M., ...

We explore the properties of the submillijansky radio population at 20 cm by applying a newly developed optical color-based method to separate star-forming (SF) from active galactic nucleus (AGN)...

Spectroscopic confirmation of an extreme starburst at redshift 4.547 (2008)

Capak, Peter, Carilli, C. L., Lee, N., Aldcroft, T., Aussel, H., Schinnerer, E., ...

We report the spectroscopic confirmation of a submillimeter galaxy (SMG) at z=4.547 with an estimated LIR = (0.5-2.0) × 1013 Lsolar. The spectra, mid-IR, and X-ray properties indicate the...

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...

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...

From a "Launch Readiness" System to an Astronomical Data Processing System - a Review of Four Years of CIA Development (2007)

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...

A Deep And Ultra-Deep Isocam Cosmological Survey Through Gravitationally Lensing Clusters Of Galaxies (2007)

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...

The H$\alpha$ Luminosity Function and Star Formation Rate at $z \approx 0.24$ in the Cosmos 2 Square-Degree Field (2007)

Shioya, Y., Taniguchi, Y., Sasaki, S. S., Nagao, T., Murayama, T., Takahashi, M. I., ...

To derive a new H$\alpha$ luminosity function and to understand the clustering properties of star-forming galaxies at $z \approx 0.24$, we have made a narrow-band imaging survey for H$\alpha$...

COSBO: The MAMBO 1.2 Millimeter Imaging Survey of the COSMOS Field (2007)

Bertoldi, F., Carilli, C., Aravena, M., Schinnerer, E., Voss, H., Smolcic, V., ...

The inner 20 × 20 arcmin^2 of the COSMOS field was imaged at 250 GHz (1.2 mm) to an rms noise level of ~1 mJy per 11" beam using the Max-Planck Millimeter Bolometer Array (MAMBO-2) at the IRAM 30 m...

Deep GALEX Imaging of the COSMOS HST Field: A First Look at the Morphology of z ~ 0.7 Star-forming Galaxies (2007)

Zamojski, M. A., Schiminovich, D., Rich , R. M., Mobasher, B., Koekemoer, A. M., Capak, P., ...

We present a study of the morphological nature of redshift z ~ 0.7 star-forming galaxies using a combination of HST ACS, GALEX, and ground-based images of the COSMOS field. Our sample consists of...

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 First Release COSMOS Optical and Near-IR Data and Catalog (2007)

Capak, P., Aussel, H., Ajiki, M., McCracken, H. J., Mobasher, B., Scoville, N., ...

We present imaging data and photometry for the COSMOS survey in 15 photometric bands between 0.3um and 2.4um. These include data taken on the Subaru 8.3m telescope, the KPNO and CTIO 4m telescopes,...

The angular correlations of galaxies in the COSMOS field (2007)

McCracken, H. J., Peacock, J. A., Guzzo, L., Capak, P., Porciani, C., Scoville, N., ...

We present measurements of the two-point galaxy angular correlation function w(\theta) in the COSMOS field. Independent determinations of w(\theta) as a function of magnitude limit are presented for...

The COSMOS Survey: Hubble Space Telescope / Advanced Camera for Surveys (HST/ACS) Observations and Data Processing (2007)

Koekemoer, A. M., Aussel, H., Calzetti, D., Capak, P., Giavalisco, M., ...

We describe the details of the Hubble Space Telescope (HST) Advanced Camera for Surveys / Wide Field Channel (ACS/WFC) observations of the COSMOS field, including the data calibration and processing...

The [OII]3727 Luminosity function and Star Formation Rate at z~1.2 in the COSMOS 2 Square-degree Field and the Subaru Deep Field (2007)

Takahashi, M. I., Shioya, Y., Taniguchi, Y., Murayama, T., Ajiki, M., Sasaki, S. S., ...

We have carried out a wide-field imaging survey for [OII]3727 emitting galaxies at z~1.2 in the HST COSMOS 2 square degree field using the Suprime-Cam on the Subaru Telescope. The survey covers a sky...

Lyman Alpha Emitters at Redshift 5.7 in the COSMOS Field (2007)

Murayama, T., Taniguchi, Y., Scoville, N. Z., Ajiki, M., Sanders, D. B., Mobasher, B., ...

We present results from a narrow-band optical survey of a contiguous area of 1.95 deg^2, covered by the Cosmic Evolution Survey (COSMOS). Both optical narrow-band (lambda_c = 8150 AA and Delta_lambda...

Deep GALEX Imaging of the HST/COSMOS Field: A First Look at the Morphology of z~0.7 Star-forming Galaxies (2007)

Zamojski, M. A., Schiminovich, D., Rich, R. M., Mobasher, B., Koekemoer, A. M., Capak, P., ...

We present a study of the morphological nature of redshift z~0.7 star-forming galaxies using a combination of HST/ACS, GALEX and ground-based images of the COSMOS field. Our sample consists of 8,146...

The Spitzer Legacy Survey of the HST-ACS 2 sq. deg. COSMOS Field: survey strategy and first analysis (2007)

Sanders, D. B., Salvato, M., Aussel, H., Ilbert, O., Scoville, N., Surace, J. A., ...

The Spitzer-COSMOS survey (S-COSMOS) is a Legacy program (Cycles 2+3) designed to carry out a uniform deep survey of the full 2 sq deg COSMOS field in all seven Spitzer bands (3.6, 4.5, 5.6, 8.0,...

The Cosmic Evolution Survey (COSMOS): a large-scale structure at z=0.73 and the relation of galaxy morphologies to local environment (2007)

Guzzo, L., Cassata, P., Finoguenov, A., Massey, R., Scoville, N. Z., Capak, P., ...

We have identified a large-scale structure at z~0.73 in the COSMOS field, coherently described by the distribution of galaxy photometric redshifts, an ACS weak-lensing convergence map and the...

The redshift evolution of early-type galaxies in COSMOS: Do massive early-type galaxies form by dry mergers? (2007)

Scarlata, C., Carollo, C. M., Lilly, S. J., Feldmann, R., Kampczyk, P., Renzini, A., ...

ABRIDGED: We study the evolution since z~1 of the rest-frame B luminosity function of the early-type galaxies (ETGs) in ~0.7 deg^2 in the COSMOS field. In order to identify ALL progenitors of local...

The Zurich Extragalactic Bayesian Redshift Analyzer (ZEBRA) and its first application: COSMOS (2007)

Feldmann, R., Carollo, C. M., Porciani, C., Lilly, S. J., Capak, P., Taniguchi, Y., ...

We present ZEBRA, the Zurich Extragalactic Bayesian Redshift Analyzer. The current version of ZEBRA combines and extends several of the classical approaches to produce accurate photometric redshifts...

The VLA-COSMOS Survey: II. Source Catalog of the Large Project (2007)

Schinnerer, E., Smolcic, V., Carilli, C. L., Bondi, M., Ciliegi, P., Jahnke, K., ...

The VLA-COSMOS large project is described and its scientific objective is discussed. We present a catalog of ~ 3,600 radio sources found in the 2deg^2 COSMOS field at 1.4 GHz. The observations in the...

The XMM-Newton wide-field survey in the COSMOS field: VI. Statistical properties of clusters of galaxies (2007)

Finoguenov, A., Guzzo, L., Hasinger, G., Scoville, N. Z., Aussel, H., Boehringer, H., ...

We present the results of a search for galaxy clusters in the first 36 XMM-Newton pointings on the COSMOS field. We reach a depth for a total cluster flux in the 0.5-2 keV band of 3x10-15 ergs cm-2...

Photometric Redshifts of Galaxies in COSMOS (2007)

Mobasher, B., Capak, P., Scoville, N. Z., Dahlen, T., Salvato, M., Aussel, H., ...

We measure photometric redshifts and spectral types for galaxies in the COSMOS survey. We use template fitting technique combined with luminosity function priors and with the option to simultaneously...

The redshift evolution of early-type galaxies in COSMOS: Do massive early-type galaxies form by dry mergers? (2007)

Scarlata, C., Carollo, C. M., Lilly, S. J., Feldmann, R., Kampczyk, P., Renzini, A., ...

ABRIDGED: We study the evolution since z~1 of the rest-frame B luminosity function of the early-type galaxies (ETGs) in ~0.7 deg^2 in the COSMOS field. In order to identify ALL progenitors of local...

Deep GALEX Imaging of the HST/COSMOS Field: A First Look at the Morphology of z~0.7 Star-forming Galaxies (2007)

Zamojski, M. A., Schiminovich, D., Rich, R. M., Mobasher, B., Koekemoer, A. M., Capak, P., ...

We present a study of the morphological nature of redshift z~0.7 star-forming galaxies using a combination of HST/ACS, GALEX and ground-based images of the COSMOS field. Our sample consists of 8,146...

The Cosmic Evolution Survey (COSMOS): a large-scale structure at z=0.73 and the relation of galaxy morphologies to local environment (2007)

Guzzo, L., Cassata, P., Finoguenov, A., Massey, R., Scoville, N. Z., Capak, P., ...

We have identified a large-scale structure at z~0.73 in the COSMOS field, coherently described by the distribution of galaxy photometric redshifts, an ACS weak-lensing convergence map and the...

The Spitzer Legacy Survey of the HST-ACS 2 sq. deg. COSMOS Field: survey strategy and first analysis (2007)

Sanders, D. B., Salvato, M., Aussel, H., Ilbert, O., Scoville, N., Surace, J. A., ...

The Spitzer-COSMOS survey (S-COSMOS) is a Legacy program (Cycles 2+3) designed to carry out a uniform deep survey of the full 2 sq deg COSMOS field in all seven Spitzer bands (3.6, 4.5, 5.6, 8.0,...

The Cosmic Evolution Survey (COSMOS): Subaru observations of the HST cosmos field (2007)

Taniguchi, Y., Scoville, N., Murayama, T., Sanders, D. B., Mobasher, B., Aussel, H., ...

We present deep optical imaging observations of 2 square degree area, covered by the Cosmic Evolution Survey (COSMOS), made by the prime-focus camera (Supreme-Cam) on the 8.2 m Subaru Telescope....

The [O II] l3727 luminosity function and star formation rate at z~1.2 in the COSMOS 2 square degree field and the Subaru deep field (2007)

Takahashi, M. I., Shioya, Y., Taniguchi, Y., Murayama, T., Ajiki, M., Sasaki, S. S., ...

We have carried out a wide-field imaging survey for [O II] lambda3727 emitting galaxies at z~1.2 in the HST COSMOS 2 square degree field using the Suprime-Cam on the Subaru Telescope. The survey...

The Cosmic Evolution Survey (COSMOS): overview (2007)

Scoville, N., Aussel, H., Brusa, M., Capak, P., Carollo, C. M., Elvis, M., ...

The Cosmic Evolution Survey (COSMOS) is designed to probe the correlated evolution of galaxies, star formation, active galactic nuclei (AGNs), and dark matter (DM) with large-scale structure (LSS)...

Large structures and galaxy evolution in COSMOS at z < 1.1 (2007)

Scoville, N., Aussel, H., Benson, A., Blain, A., Calzetti, D., Capak, P., ...

We present the first identification of large-scale structures (LSSs) at z

COSMOS: Hubble Space Telescope observations (2007)

Scoville, N., Abraham, R. G., Aussel, H., Barnes, J. E., Benson, A., Blain, A. W., ...

The Cosmic Evolution Survey (COSMOS) was initiated with an extensive allocation (590 orbits in Cycles 12-13) using the Hubble Space Telescope (HST) for high-resolution imaging. Here we review the...

The VLA-COSMOS Survey. II. Source catalog of the large project (2007)

Schinnerer, E., Smolcic, V., Carilli, C. L., Bondi, M., Ciliegi, P., Jahnke, K., ...

The VLA-COSMOS Large Project is described and its scientific objective is discussed. We present a catalog of ~3600 radio sources found in the 2 deg2 COSMOS field at 1.4 GHz. The observations in the...

A potential galaxy threshing system in the COSMOS field (2007)

Sasaki, S. S., Taniguchi, Y., Scoville, N., Mobasher, B., Aussel, H., Sanders, D. B., ...

We report on the discovery of a new potential galaxy threshing system in the COSMOS 2 square degree field using the prime-focus camera, Suprime-Cam, on the 8.2 m Subaru Telescope. This system...

S-COSMOS: the Spitzer Legacy survey of the Hubble Space Telescope ACS 2 deg2 COSMOS Field I: survey strategy and first analysis (2007)

Sanders, D. B., Salvato, M., Aussel, H., Ilbert, O., Scoville, N., Surace, J. A., ...

The COSMOS Spitzer survey (S-COSMOS) is a Legacy program (Cycles 2+3) designed to carry out a uniform deep survey of the full 2 deg2 COSMOS field in all seven Spitzer bands (3.6, 4.5, 5.6, 8.0, 24.0,...

The Spitzer Legacy survey of the HST-ACS 2 sq. deg. COSMOS field: survey strategy and first analysis (2007)

Sanders, D. B., Salvato, M., Aussel, H., Ilbert, O., Scoville, N., Surace, J. A., ...

The Spitzer-COSMOS survey (S-COSMOS) is a Legacy program (Cycles 2+3) designed to carry out a uniform deep survey of the full 2 sq deg COSMOS field in all seven Spitzer bands (3.6, 4.5, 5.6, 8.0,...

The stellar content of the COSMOS field as derived from morphological and SED-based star/galaxy separation (2007)

Robin, A. C., Rich, R. M., Aussel, H., Capak, P., Tasca, L. A. M., Jahnke, K., ...

We report on the stellar content of the COSMOS two degree field, as derived from a rigorous star-galaxy separation approach developed for using stellar sources to define the point-spread function...

Lya emitters at redshift 5.7 in the COSMOS field (2007)

Murayama, T., Taniguchi, Y., Scoville, N. Z., Ajiki, M., Sanders, D. B., Mobasher, B., ...

We present results from a narrowband optical survey of a contiguous area of 1.95 deg2, covered by the Cosmic Evolution Survey (COSMOS). Both optical narrowband (lambdac=8150 Å and Deltalambda=120...

zCOSMOS: a large VLT/VIMOS redshift survey covering 0 < z < 3 in the COSMOS field (2007)

Lilly, S. J., Le Fevre, O., Renzini, A., Zamorani, G., Scodeggio, M., Contini, T., ...

zCOSMOS is a large redshift survey that is being undertaken in the COSMOS field using 600 hours of observation with the VIMOS spectrograph on the 8-m VLT. The survey is designed to characterise the...

The XMM-Newton Wide-Field Survey in the COSMOS field: statistical properties of clusters of galaxies (2007)

Finoguenov, A., Guzzo, L., Hasinger, G., Scoville, N. Z., Aussel, H., Böhringer, H., ...

We present the results of a search for galaxy clusters in the first 36 XMM-Newton pointings on the Cosmic Evolution Survey (COSMOS) field. We reach a depth for a total cluster flux in the 0.5-2 keV...

The first release COSMOS optical and Near-IR data and catalog (2007)

Capak, P., Aussel, H., Ajiki, M., McCracken, H. J., Mobasher, B., Scoville, N., ...

We present imaging data and photometry for the COSMOS survey in 15 photometric bands between 0.3 and 2.4 mum. These include data taken on the Subaru 8.3 m telescope, the KPNO and CTIO 4 m telescopes,...

COSBO: the MAMBO 1.2 millimeter imaging survey of the COSMOS field (2007)

Bertoldi, F., Carilli, C., Aravena, M., Schinnerer, E., Voss, H., Smolcic, V., ...

The inner 20×20 arcmin2 of the COSMOS field was imaged at 250 GHz (1.2 mm) to an rms noise level of ~1 mJy per 11" beam using the Max-Planck Millimeter Bolometer Array (MAMBO-2) at the IRAM 30 m...

Preprint typeset using L ATEX style emulateapj v. 12/01/06 DEEP GALEX IMAGING OF THE HST/COSMOS FIELD: A FIRST LOOK AT THE MORPHOLOGY OF z ∼ 0.7 STAR-FORMING GALAXIES * (2007)

M. A. Zamojski, D. Schiminovich, R. M. Rich, B. Mobasher, A. M. Koekemoer, P. Capak, ...

We present a study of the morphological nature of redshift z ∼ 0.7 star-forming galaxies using a combination of HST/ACS, GALEX and ground-based images of the COSMOS field. Our sample consists of...

The XMM-Newton wide-field survey in the COSMOS field: VI. Statistical properties of clusters of galaxies (2006)

Finoguenov, A., Guzzo, L., Hasinger, G., Scoville, N. Z., Aussel, H., Boehringer, H., ...

We present the results of a search for galaxy clusters in the first 36 XMM-Newton pointings on the COSMOS field. We reach a depth for a total cluster flux in the 0.5-2 keV band of 3x10-15 ergs cm-2...

Large Structures and Galaxy Evolution in COSMOS at z < 1.1 (2006)

Scoville, N., Aussel, H., Benson, A., Blain, A., Calzetti, D., Capak, P., ...

We present the first identification of large-scale structures (LSS) at z $< 1.1$ in the Cosmic Evolution Survey (COSMOS). The structures are identified from adaptive smoothing of galaxy counts in the...

Photometric Redshifts of Galaxies in COSMOS (2006)

Mobasher, B., Capak, P., Scoville, N. Z., Dahlen, T., Salvato, M., Aussel, H., ...

We measure photometric redshifts and spectral types for galaxies in the COSMOS survey. We use template fitting technique combined with luminosity function priors and with the option to simultaneously...

The stellar content of the COSMOS field as derived from morphological and SED based gtar/galaxy Separation (2006)

Robin, A. C., Rich, R. M., Aussel, H., Capak, P., Tasca, L. A. M., Jahnke, K., ...

We report on the stellar content of the COSMOS two degree field, as derived from a rigorous star/galaxy separation approach developed for using stellar sources to define the point spread function...

A Potential Galaxy Threshing System in the Cosmos Field (2006)

Sasaki, S. S., Taniguchi, Y., Scoville, N., Mobasher, B., Aussel, H., Sanders, D. B., ...

We report on the discovery of a new potential galaxy threshing system in the COSMOS 2 square degree field using the prime-focus camera, Suprime-Cam, on the 8.2 m Subaru Telescope. This system...

The Cosmic Evolution Survey (COSMOS) -- Overview (2006)

Scoville, N., Aussel, H., Brusa, M., Capak, P., Carollo, C. M., Elvis, M., ...

The Cosmic Evolution Survey (COSMOS) is designed to probe the correlated evolution of galaxies, star formation, active galactic nuclei (AGN) and dark matter (DM) with large-scale structure (LSS) over...

The VLA-COSMOS Survey: II. Source Catalog of the Large Project (2006)

Schinnerer, E., Smolcic, V., Carilli, C. L., Bondi, M., Ciliegi, P., Jahnke, K., ...

The VLA-COSMOS large project is described and its scientific objective is discussed. We present a catalog of ~ 3,600 radio sources found in the 2deg^2 COSMOS field at 1.4 GHz. The observations in the...

The Cosmic Evolution Survey (COSMOS): Subaru Observations of the HST COSMOS Field (2006)

Taniguchi, Y., Scoville, N., Murayama, T., Sanders, D. B., Mobasher, B., Aussel, H., ...

We present deep optical imaging observations of 2 square degree area, covered by the Cosmic Evolution Survey (COSMOS), made by the prime-focus Camera (Supreme-Cam) on the 8.2m Subaru Telescope....

COSMOS morphological classification with ZEST (the Zurich Estimator of Structural Types) and the evolution since z=1 of the Luminosity Function of early-, disk-, and irregular galaxies (2006)

Scarlata, C., Carollo, C. M., Lilly, S. J., Sargent, M. T., Feldmann, R., Kampczyk, P., ...

(ABRIDGED) Motivated by the desire to reliably and automatically classify structure of thousands of COSMOS galaxies, we present ZEST, the Zurich Estimator of Structural Types. To classify galaxy...

The Zurich Extragalactic Bayesian Redshift Analyzer and its first application: COSMOS (2006)

Feldmann, R., Carollo, C. M., Porciani, C., Lilly, S. J., Capak, P., Taniguchi, Y., ...

We present the Zurich Extragalactic Bayesian Redshift Analyzer (ZEBRA). The current version of ZEBRA combines and extends several of the classical approaches to produce accurate photometric redshifts...

The Zurich Extragalactic Bayesian Redshift Analyzer (ZEBRA) and its first application: COSMOS (2006)

Feldmann, R., Carollo, C. M., Porciani, C., Lilly, S. J., Capak, P., Taniguchi, Y., ...

We present ZEBRA, the Zurich Extragalactic Bayesian Redshift Analyzer. The current version of ZEBRA combines and extends several of the classical approaches to produce accurate photometric redshifts...

Final analysis of ELAIS 15-$mu$m (Vaccari+, 2005) (2005)

Vaccari, M., Lari, C., Angeretti, L., Fadda, D., Gruppioni, C., Pozzi, F., ...

We present the final analysis of the European Large Area Infrared Space Observatory (ISO) Survey (ELAIS) 15-{mu}m observations, carried out with the ISO Camera (ISOCAM) instrument on board the ISO....

Final analysis of ELAIS 15-mum observations: method, reduction and catalogue (2005)

Vaccari, M., Lari, C., Angeretti, L., Fadda, D., Gruppioni, C., Pozzi, F., ...

We present the final analysis of the European Large Area Infrared Space Observatory (ISO) Survey (ELAIS) 15-mum observations, carried out with the ISO Camera (ISOCAM) instrument on board the ISO. The...

The HST Cosmos Project: Contribution from the Subaru Telescope (2005)

Taniguchi, Yoshiaki, Scoville, N. Z., Sanders, D. B., Mobasher, B., Aussel, H., Capak, P., ...

The Cosmic Evolution Survey (COSMOS) is a Hubble Space Telescope (HST) treasury project.The COSMOS aims to perform a 2 square degree imaging survey of an equatorial field in $I$(F814W) band, using...

Final Analysis of ELAIS 15 $\mu$m Observations : Method, Reduction and Catalogue (2004)

Vaccari, M., Lari, C., Angeretti, L., Fadda, D., Gruppioni, C., Pozzi, F., ...

We present the Final Analysis of the European Large Area ISO Survey (ELAIS) 15 $\mu$m observations, carried out with the ISOCAM instrument on board the Infrared Space Observatory (ISO). The data...

23 High Redshift Supernovae from the IfA Deep Survey: Doubling the SN Sample at z>0.7 (2003)

Barris, Brian J., Tonry, John, Blondin, Stephane, Challis, Peter, Chornock, Ryan, Clocchiatti, Alejandro, ...

We present photometric and spectroscopic observations of 23 high redshift supernovae spanning a range of z=0.34-1.03, 9 of which are unambiguously classified as Type Ia. These supernovae were...

Infrared spectroscopy of faint 15 micron sources in the Hubble Deep Field South: first hints at the properties of the sources of the IR background (2003)

Franceschini, A., Berta, S., Rigopoulou, D., Aussel, H., Cesarsky, C. J., Elbaz, D., ...

We present a spectroscopic analysis of 21 galaxies with z=0.2-1.5 drawn from a 25 sq. arcmin ultra-deep 15 micron ISOCAM survey centered in the HDFS. VLT/ISAAC spectra are reported for 18 sources,...

A Submillimeter and Radio Survey of Gamma-Ray Burst Host Galaxies: A Glimpse into the Future of Star Formation Studies (2002)

Berger, E., Cowie, L. L., Kulkarni, S. R., Frail, D. A., Aussel, H., Barger, A. J.

We present the first comprehensive search for submillimeter and radio emission from the host galaxies of twenty well-localized gamma-ray bursts (GRBs). With the exception of a single source, all...

Kinematics of Galaxies in the Hubble Deep Field South: Discovery of a Very Massive Spiral at z=0.6 (2002)

Rigopoulou, D., Franceschini, A., Aussel, H., Genzel, R., Thatte, N., Cesarsky, C. J.

We report the first results from a study of the internal kinematics, based on spatially resolved H_alpha velocity profiles, of three galaxies at redshift z~0.6 and one at redshift z~0.8, detected by...

The Chandra Deep Field North Survey. XI. X-ray emission from luminous infrared starburst galaxies (2002)

Alexander, D. M., Aussel, H., Bauer, F. E., Brandt, W. N., Hornschemeier, A. E., Vignali, C., ...

Using the 1 Ms Chandra Deep Field North and 15 micron ISOCAM HDF-N surveys we find a tight correlation between the population of strongly evolving starbursts discovered in faint 15 micron ISOCAM...

The Bulk of the Cosmic Infrared Background Resolved by ISOCAM (2002)

Elbaz, D., Cesarsky, C., Chanial, P., Aussel, H., Franceschini, A., Fadda, D., ...

We have computed the 15 microns integrated galaxy light produced by ISOCAM galaxies above a sensitivity limit of 50 microJy. It sets a lower limit to the 15 microns extragalactic background light of...

ISO ELAIS 15{mu}m survey (Lari+, 2001) (2002)

Lari, C., Pozzi, F., Gruppioni, C., Aussel, H., Ciliegi, P., Danese, L., ...

We develop a new data reduction technique for ISOCAM LW data and apply it to the European Large Area ISO Survey (ELAIS) LW3 (15-{mu}m) observations in the southern hemisphere (S1). This method, known...

Kinematics of galaxies in the Hubble Deep Field-South: Discovery of a very massive spiral galaxy at z=0.6 (2002)

Rigopoulou, D., Franceschini, A., Aussel, H., Genzel, R., Thatte, N., Cesarsky, C. J.

We report the first results from a study of the internal kinematics, based on spatially resolved Halpha velocity profiles, of three galaxies at redshift z similar to 0.6 and one at redshift z similar...

A Long-Wavelength View on Galaxy Evolution from Deep Surveys by the Infrared Space Observatory (2001)

Franceschini, A., Aussel, H., Cesarsky, C. J., Elbaz, D., Fadda, D.

We discuss the constraints set on galaxy evolution by data from deep surveys performed in the mid-IR and far-IR with ISO and with mm telescopes at longer wavelengths. These reveal extremely high...

A new method for ISOCAM data reduction - I. Application to the European Large Area ISO Survey Southern Field: method and results (2001)

Lari, C., Pozzi, F., Gruppioni, C., Aussel, H., Ciliegi, P., Danese, L., ...

We develop a new data reduction technique for ISOCAM LW data and apply it to the European Large Area ISO Survey (ELAIS) LW3 (15-mum) observations in the southern hemisphere (S1). This method, known...

A New Method for ISOCAM Data Reduction - I. Application to the European Large Area ISO Survey Southern Field: Method and Results (2001)

Lari, C., Pozzi, F., Gruppioni, C., Aussel, H., Ciliegi, P., Danese, L., ...

We have developed a new data reduction technique for ISOCAM LW data and have applied it to the European Large Area ISO Survey (ELAIS) LW3 (15 micron) observations in the southern hemisphere (S1)....

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...

VLT-ISAAC near-IR Spectroscopy of ISO selected Hubble Deep Field South Galaxies (2000)

Rigopoulou, D., Franceschini, A., Aussel, H., Genzel, R., Cesarsky, C. J., ...

We report the results of near-infrared VLT-ISAAC spectroscopy of a sample of 12 galaxies at z = 0.4-1.4, drawn from the ISOCAM survey of the Hubble Deep Field South. We find that the rest frame...

FIRBACK Source Counts and Cosmological Implications (2000)

Dole, Herve, Gispert, Richard, Lagache, Guilaine, Puget, Jean-Loup, Aussel, H., Bouchet, F. R., ...

FIRBACK is a one of the deepest surveys performed at 170 microns with ISOPHOT onboard ISO, and is aimed at the study of cosmic far infrared background sources. About 300 galaxies are detected in an...

A local infrared perspective to deeper ISO surveys (2000)

Alexander, D. M., Aussel, H.

We present new techniques to produce IRAS 12 micron samples of galaxies and stars. We show that previous IRAS 12 micron samples are incompatible for detailed comparison with ISO surveys and review...

NIR Spectroscopy with the VLT of a sample of ISO selected Hubble Deep Field South Galaxies (1999)

Rigopoulou, D., Franceschini, A., Genzel, R., Aussel, H., Cesarsky, C., ...

A new population of faint galaxies characterized by an extremely high rate of evolution with redshift up to z~1.5 has recently been discovered by ISO. These sources are likely to contribute...

Source Counts from the 15 microns ISOCAM Deep Surveys (1999)

Elbaz, D., Cesarsky, C. J., Fadda, D., Aussel, H., Desert, F. X., Franceschini, A., ...

We present the results of the five mid-IR 15 microns (12-18 microns LW3 band) ISOCAM Guaranteed Time Extragalactic Surveys performed in the regions of the Lockman Hole and Marano Field. The roughly...

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...

Isocam Extragalactic Mid-Infrared Deep Surveys Unveiling Dust-Enshrouded Star Formation In The Universe (1999)

Elbaz, D., Aussel, H., Cesarsky, C. J., Desert, F. X., Fadda, D., Franceschini, A., ...

ISOCAM extragalactic mid-infrared deep surveys have detected a population of strong IR emitters ten times more numerous than expected if there were no evolution from z

FIRBACK Far Infrared Survey with ISO: Data Reduction, Analysis and First Results (1999)

Dole, Herve, Lagache, Guilaine, Puget, Jean-Loup, Gispert, Richard, Aussel, H., Bouchet, F. R., ...

FIRBACK is one of the deepest cosmological surveys performed in the far infrared, using ISOPHOT. We describe this survey, its data reduction and analysis. We present the maps of fields at 175...

A Deep and Ultra-deep ISOCAM Cosmological Survey through Gravitationally Lensing Clusters of Galaxies (1999)

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...

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...

FIRBACK: I. A deep survey at 175 $\mu$m with ISO, preliminary results (1998)

Puget, J. L., Lagache, G., Clements, D. L, Reach, W. T., Aussel, H., Bouchet, F. R, ...

FIRBACK is a deep survey conducted with the ISOPHOT instrument aboard the Infrared Space Observatory (ISO) at an effective wavelength of 175 $\mu$m. We present here results we have obtained on the...

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...

ISOCAM observations of the Hubble Deep Field reduced with the PRETI method (1998)

Aussel, H., Cesarsky, C. J., Elbaz, D.

We have developed a new ISOCAM data reduction technique based on wavelet analysis, especially designed for the detection of faint sources in mid-infrared surveys. This method, the Pattern REcognition...

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....

Isocam deep surveys unveiling star formation in the mid-infrared (1998)

Elbaz, D., Aussel, H., Cesarsky, C. J., Desert, F. X., Fadda, D., Franceschini, A., ...

Before having exhausted the helium in its tank on April 8, 1998, the Infrared Space Observatory had time to perform several complementary surveys at various depths and areas within selected regions...

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...

Source Counts and Background Radiation (1997)

Franceschini, A., Aussel, H., Bressan, A., Cesarsky, C. J., Danese, L., De Zotti, G., ...

Our present understanding of the extragalactic source counts and background radiation at infrared and sub-mm wavelengths is reviewed. Available count data are used to constrain evolutionary models of...