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1. Obscured AGN at 1.5 < 3.0 from the zCOSMOS-deep Survey

Author: Mignoli, M., primary, Feltre, A., additional, Bongiorno, A., additional, Calura, F., additional, Gilli, R., additional, Vignali, C., additional, Zamorani, G., additional, Lilly, S. J., additional, Le Fèvre, O., additional, Bardelli, S., additional, Bolzonella, M., additional, Bordoloi, R., additional, Le Brun, V., additional, Caputi, K. I., additional, Cimatti, A., additional, Diener, C., additional, Garilli, B., additional, Koekemoer, A. M., additional, Maier, C., additional, Mainieri, V., additional, Peng, Y., additional, Pérez Montero, E., additional, Silverman, J. D., additional, and Zucca, E., additional
Published: 2019
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2. PHIBSS2: survey design and z = 0.5 – 0.8 results

Author: Freundlich, J., primary, Combes, F., additional, Tacconi, L. J., additional, Genzel, R., additional, Garcia-Burillo, S., additional, Neri, R., additional, Contini, T., additional, Bolatto, A., additional, Lilly, S., additional, Salomé, P., additional, Bicalho, I. C., additional, Boissier, J., additional, Boone, F., additional, Bouché, N., additional, Bournaud, F., additional, Burkert, A., additional, Carollo, M., additional, Cooper, M. C., additional, Cox, P., additional, Feruglio, C., additional, Förster Schreiber, N. M., additional, Juneau, S., additional, Lippa, M., additional, Lutz, D., additional, Naab, T., additional, Renzini, A., additional, Saintonge, A., additional, Sternberg, A., additional, Walter, F., additional, Weiner, B., additional, Weiß, A., additional, and Wuyts, S., additional
Published: 2019
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3. The zCOSMOS survey

Author: Zucca E., Bardelli S., Bolzonella M., Zamorani G., Ilbert O., Pozzetti L., Mignoli M., Kova, #269, Lilly S., Tresse L., Tasca L., Cassata P., Halliday C., Vergani D., Caputi K., Carollo C. M., Contini T., Kneib J. P., Le Fèvre O., Mainieri V., Renzini A., Scodeggio M., Bongiorno A., Coppa G., de La Torre S., de Ravel L., Franzetti P., Garilli B., Iovino A., Kampczyk P., Knobel C., Lamareille F., Le Borgne J. F., Le Brun V., Maier C., Pellò R., Peng Y., Perez Montero E., Ricciardelli E., Silverman J. D., Tanaka M., Abbas U., Bottini D., Cappi A., Guzzo L., Koekemoer A. M., Leauthaud A., Maccagni D., Marinoni C., McCracken H. J., Meme, P., Meneux B., Oesch P., Porciani C., Scaramella R., Arnouts S., Aussel H., Capak P., Kartaltepe J., Salvato M., Sanders D., Scoville N., Taniguchi Y., Thompson D., CUCCIATI, OLGA, CIMATTI, ANDREA, MORESCO, MICHELE ENNIO MARIA, INAF - Osservatorio Astronomico di Brera (OAB), Istituto Nazionale di Astrofisica (INAF), INAF - Osservatorio Astronomico di Bologna (OABO), Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO), AUTRES, Laboratoire d'Astrophysique de Marseille (LAM), Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS), INAF - Osservatorio Astrofisico di Arcetri (OAA), University of Chicago, Laboratoire Astrophysique de Toulouse-Tarbes (LATT), Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Centre National de la Recherche Scientifique (CNRS), INAF- Milano, Dipartimento di Fisica, Università degli Studi di Milano-Bicocca = University of Milano-Bicocca (UNIMIB)-Università degli Studi di Milano = University of Milan (UNIMI), Institute of Astronomy [ETH Zürich], Department of Physics [ETH Zürich] (D-PHYS), Eidgenössische Technische Hochschule - Swiss Federal Institute of Technology [Zürich] (ETH Zürich)- Eidgenössische Technische Hochschule - Swiss Federal Institute of Technology [Zürich] (ETH Zürich), Tokai University, Istituto di Astrofisica Spaziale e Fisica cosmica - Bologna (IASF-Bo), Space Telescope Science Institute (STSci), Centre de Physique Théorique - UMR 6207 (CPT), Université de la Méditerranée - Aix-Marseille 2-Université de Provence - Aix-Marseille 1-Université de Toulon (UTLN)-Centre National de la Recherche Scientifique (CNRS), Centre de Physique Théorique - UMR 7332 (CPT), Aix Marseille Université (AMU)-Université de Toulon (UTLN)-Centre National de la Recherche Scientifique (CNRS), Institut d'Astrophysique de Paris (IAP), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Max-Planck-Institut für Astronomie (MPIA), Max-Planck-Gesellschaft, Materials & Process technology, Boeing Company [Chicago], California Institute of Technology (CALTECH), Sea Mammal Research Unit, St Andrews, Astronomy, Zucca E., Bardelli S., Bolzonella M., Zamorani G., Ilbert O., Pozzetti L., Mignoli M., Kova&#269, K., Lilly S., Tresse L., Tasca L., Cassata P., Halliday C., Vergani D., Caputi K., Carollo C. M., Contini T., Kneib J.-P., Le Fèvre O., Mainieri V., Renzini A., Scodeggio M., Bongiorno A., Coppa G., Cucciati O., de La Torre S., de Ravel L., Franzetti P., Garilli B., Iovino A., Kampczyk P., Knobel C., Lamareille F., Le Borgne J.-F., Le Brun V., Maier C., Pellò R., Peng Y., Perez-Montero E., Ricciardelli E., Silverman J. D., Tanaka M., Abbas U., Bottini D., Cappi A., Cimatti A., Guzzo L., Koekemoer A. M., Leauthaud A., Maccagni D., Marinoni C., McCracken H. J., Meme, P., Meneux B., Moresco M., Oesch P., Porciani C., Scaramella R., Arnouts S., Aussel H., Capak P., Kartaltepe J., Salvato M., Sanders D., Scoville N., Taniguchi Y., Thompson D., Università di Bologna, Dipartimento di Astronomia, Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Aix Marseille Université (AMU)-Centre National d'Études Spatiales [Toulouse] (CNES), Centre National de la Recherche Scientifique (CNRS)-Observatoire Midi-Pyrénées (OMP), Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées, Università degli Studi di Milano-Bicocca [Milano] (UNIMIB)-Università degli Studi di Milano [Milano] (UNIMI), Centre National de la Recherche Scientifique (CNRS)-Université de Toulon (UTLN)-Université de Provence - Aix-Marseille 1-Université de la Méditerranée - Aix-Marseille 2, and Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Pierre et Marie Curie - Paris 6 (UPMC)
Subjects: Normalization (statistics), Cosmology and Nongalactic Astrophysics (astro-ph.CO), High density, FOS: Physical sciences, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Surveys, 01 natural sciences, Luminosity, [PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], MORPHOLOGICAL CLASSIFICATION, 1ST EPOCH DATA, 0103 physical sciences, Astrophysics::Solar and Stellar Astrophysics, Density field, FIELD, 10. No inequality, 010303 astronomy & astrophysics, PHOTOMETRIC REDSHIFTS, Astrophysics::Galaxy Astrophysics, galaxies: statistics, Luminosity function (astronomy), Physics, REDSHIFT SURVEY, LEGACY SURVEY, 010308 nuclear & particles physics, Galaxies: evolution, Galaxies: luminosity function, mass function, Galaxies: statistics, Astronomy and Astrophysics, Space and Planetary Science, VLT DEEP SURVEY, B band, Galaxy, galaxies: luminosity function, mass function, COLOR-DENSITY RELATION, galaxies: luminosity function, mass function, DIGITAL SKY SURVEY, galaxies: evolution, Cosmic time, SURVEY COSMOS, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: (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 field are available. The global LF exhibits a brightening of ~0.7 mag in M* from z~0.2 to z~0.9. At low z, late types dominate at faint magnitudes, while the bright end is populated mainly by early types. At higher z, late-type galaxies evolve significantly and, at z~1, the contribution from the various types to the bright end of the LF is comparable. The evolution for early types is in both luminosity and normalization. A similar behaviour is exhibited by late types, but with an opposite trend for the normalization. Studying the role of the environment, we find that the global LF of galaxies in overdense regions has always a brighter M* and a flatter slope. In low density environments, the main contribution to the LF is from blue galaxies, while for high density environments there is an important contribution from red galaxies to the bright end. The differences between the global LF in the two environments are not due to only a difference in the relative numbers of red and blue galaxies, but also to their relative luminosity distributions: the value of M* for both types in underdense regions is always fainter than in overdense environments. The "specular" evolution of late- and early-type galaxies is consistent with a scenario where a part of blue galaxies is transformed in red galaxies with increasing cosmic time, without significant changes in the fraction of intermediate-type galaxies. The bulk of this tranformation in overdense regions probably happened before z~1, while it is still ongoing at lower z in underdense environments., Comment: 18 pages, 10 figures, A&A in press
Published: 2009
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4. Obscured AGN at 1.5 < z < 3.0 from the zCOSMOS-deep Survey: I. Properties of the emitting gas in the narrow-line region.

Author: Mignoli, M., Feltre, A., Bongiorno, A., Calura, F., Gilli, R., Vignali, C., Zamorani, G., Lilly, S. J., Le Fèvre, O., Bardelli, S., Bolzonella, M., Bordoloi, R., Le Brun, V., Caputi, K. I., Cimatti, A., Diener, C., Garilli, B., Koekemoer, A. M., Maier, C., and Mainieri, V.
Subjects: SEYFERT galaxies, STELLAR mass, ACTIVE galactic nuclei, IONIZED gases, GAS distribution, GALAXY spectra
Abstract: Context. The physics and demographics of high-redshift obscured active galactic nuclei (AGN) is still scarcely investigated. New samples of such objects, selected with different techniques, can provide useful insights into their physical properties. Aims. With the goal to determine the properties of the gas in the emitting region of type 2 AGN, in particular, the gas metal content, we exploit predictions from photoionization models, including new parameterizations for the distance of gas distribution from the central source and internal microturbulence in the emitting clouds, to interpret rest-frame UV spectral data. Methods. We selected a sample of 90 obscured (type 2) AGN with 1.45 ≤ z ≤ 3.05 from the zCOSMOS-deep galaxy sample by 5σ detection of the high-ionization C IVλ1549 narrow emission line. This feature in a galaxy spectrum is often associated with nuclear activity, and the selection effectiveness has also been confirmed by diagnostic diagrams based on utraviolet (UV) emission-line ratios. We applied the same selection technique and collected a sample of 102 unobscured (type 1) AGN. Taking advantage of the large amount of multiband data available in the COSMOS field, we investigated the properties of the C IV-selected type 2 AGN, focusing on their host galaxies, X-ray emission, and UV emission lines. Finally, we investigated the physical properties of the ionized gas in the narrow-line region (NLR) of this type 2 AGN sample by combining the analysis of strong UV emission lines with predictions from photoionization models. Results. We find that in order to successfully reproduce the relative intensity of UV emission lines of the selected high-z type 2 AGN, two new ingredients in the photoionization models are fundamental: small inner radii of the NLR (≈90 pc for LAGN = 1045 erg s−1), and the internal dissipative microturbulence of the gas-emitting clouds (with vmicr ≈ 100 km s−1). With these modified models, we compute the gas-phase metallicity of the NLR, and our measurements indicate a statistically significant evolution of the metal content with redshift. Finally, we do not observe a strong relationship between the NLR gas metallicity and the stellar mass of the host galaxy in our C IV-selected type 2 AGN sample. [ABSTRACT FROM AUTHOR]
Published: 2019
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5. Tracking the impact of environment on the galaxy stellar mass function up to z â¼ 1 in the 10 k zCOSMOS sample

Author: Bolzonella M., Kova, #269, Pozzetti L., Zucca E., Lilly S. J., Peng Y., Iovino A., Zamorani G., Vergani D., Tasca L. A. M., Lamareille F., Oesch P., Caputi K., Kampczyk P., Bardelli S., Maier C., Abbas U., Knobel C., Scodeggio M., Carollo C. M., Contini T., Kneib J. P., Le Fèvre O., Mainieri V., Renzini A., Bongiorno A., Coppa G., de la Torre S., de Ravel L., Franzetti P., Garilli B., Le Borgne J. F., Le Brun V., Mignoli M., Pelló R., Perez Montero E., Ricciardelli E., Silverman J. D., Tanaka M., Tresse L., Bottini D., Cappi A., Cassata P., Guzzo L., Koekemoer A. M., Leauthaud A., Maccagni D., Marinoni C., McCracken H. J., Memeo P., Meneux B., Porciani C., Scaramella R., Aussel H., Capak P., Halliday C., Ilbert O., Kartaltepe J., Salvato M., Sanders D., Scarlata C., Scoville N., Taniguchi Y., Thompson D., CUCCIATI, OLGA, CIMATTI, ANDREA, Bolzonella M., Kova&#269, K., Pozzetti L., Zucca E., Cucciati O., Lilly S. J., Peng Y., Iovino A., Zamorani G., Vergani D., Tasca L. A. M., Lamareille F., Oesch P., Caputi K., Kampczyk P., Bardelli S., Maier C., Abbas U., Knobel C., Scodeggio M., Carollo C. M., Contini T., Kneib J.-P., Le Fèvre O., Mainieri V., Renzini A., Bongiorno A., Coppa G., de la Torre S., de Ravel L., Franzetti P., Garilli B., Le Borgne J.-F., Le Brun V., Mignoli M., Pelló R., Perez-Montero E., Ricciardelli E., Silverman J. D., Tanaka M., Tresse L., Bottini D., Cappi A., Cassata P., Cimatti A., Guzzo L., Koekemoer A. M., Leauthaud A., Maccagni D., Marinoni C., McCracken H. J., Memeo P., Meneux B., Porciani C., Scaramella R., Aussel H., Capak P., Halliday C., Ilbert O., Kartaltepe J., Salvato M., Sanders D., Scarlata C., Scoville N., Taniguchi Y., Thompson D., INAF - Osservatorio Astronomico di Bologna (OABO), Istituto Nazionale di Astrofisica (INAF), AUTRES, INAF- Milano, Institute of Astronomy [ETH Zürich], Department of Physics [ETH Zürich] (D-PHYS), Eidgenössische Technische Hochschule - Swiss Federal Institute of Technology [Zürich] (ETH Zürich)- Eidgenössische Technische Hochschule - Swiss Federal Institute of Technology [Zürich] (ETH Zürich), INAF - Osservatorio Astronomico di Brera (OAB), Laboratoire d'Astrophysique de Marseille (LAM), Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS), University of Chicago, Laboratoire Astrophysique de Toulouse-Tarbes (LATT), Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Astrophysique de l'Observatoire Midi-Pyrénées (LATT), Human Genetics Center, The University of Texas Health Science Center at Houston (UTHealth), School of Biotechnology and Biomolecular Sciences, University of New South Wales [Sydney] (UNSW), Space Telescope Science Institute (STSci), Centre de Physique Théorique - UMR 6207 (CPT), Université de la Méditerranée - Aix-Marseille 2-Université de Provence - Aix-Marseille 1-Université de Toulon (UTLN)-Centre National de la Recherche Scientifique (CNRS), Centre de Physique Théorique - UMR 7332 (CPT), Aix Marseille Université (AMU)-Université de Toulon (UTLN)-Centre National de la Recherche Scientifique (CNRS), Institut d'Astrophysique de Paris (IAP), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Istituto di Astrofisica Spaziale e Fisica cosmica - Bologna (IASF-Bo), California Institute of Technology (CALTECH), Max-Planck-Institut für Astronomie (MPIA), Max-Planck-Gesellschaft, Materials & Process technology, Boeing Company [Chicago], Sea Mammal Research Unit, St Andrews, Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Aix Marseille Université (AMU)-Centre National d'Études Spatiales [Toulouse] (CNES), Centre National de la Recherche Scientifique (CNRS)-Observatoire Midi-Pyrénées (OMP), Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées, Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS), Centre National de la Recherche Scientifique (CNRS)-Université de Toulon (UTLN)-Université de Provence - Aix-Marseille 1-Université de la Méditerranée - Aix-Marseille 2, and Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Pierre et Marie Curie - Paris 6 (UPMC)
Subjects: Cosmology and Nongalactic Astrophysics (astro-ph.CO), Stellar mass, FOS: Physical sciences, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics, 01 natural sciences, Photometry (optics), [PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], 0103 physical sciences, Galaxy formation and evolution, Density contrast, 010303 astronomy & astrophysics, Astrophysics::Galaxy Astrophysics, Physics, 010308 nuclear & particles physics, Star formation, galaxies: fundamental parameters, Astronomy and Astrophysics, Redshift, Galaxy, Bimodality, galaxies: luminosity function, mass function, Space and Planetary Science, cosmology: observations, galaxies: evolution, galaxies: luminosity function, mass function, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: We study the impact of the environment on the evolution of galaxies in the zCOSMOS 10k sample in the redshift range 0.1, Comment: 17 pages, 11 figures. Version accepted for publication in Astronomy and Astrophysics, including referee's suggestions, a new section with comparison with literature data, and updated references
Published: 2010
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6. Extended Lymanαhaloes around individual high-redshift galaxies revealed by MUSE

Author: Wisotzki, L., primary, Bacon, R., additional, Blaizot, J., additional, Brinchmann, J., additional, Herenz, E. C., additional, Schaye, J., additional, Bouché, N., additional, Cantalupo, S., additional, Contini, T., additional, Carollo, C. M., additional, Caruana, J., additional, Courbot, J.-B., additional, Emsellem, E., additional, Kamann, S., additional, Kerutt, J., additional, Leclercq, F., additional, Lilly, S. J., additional, Patrício, V., additional, Sandin, C., additional, Steinmetz, M., additional, Straka, L. A., additional, Urrutia, T., additional, Verhamme, A., additional, Weilbacher, P. M., additional, and Wendt, M., additional
Published: 2016
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7. Evolution of the specific star formation rate function atz< 1.4 Dissecting the mass-SFR plane in COSMOS and GOODS

Author: Ilbert, O., primary, Arnouts, S., additional, Le Floc’h, E., additional, Aussel, H., additional, Bethermin, M., additional, Capak, P., additional, Hsieh, B.-C., additional, Kajisawa, M., additional, Karim, A., additional, Le Fèvre, O., additional, Lee, N., additional, Lilly, S., additional, McCracken, H. J., additional, Michel-Dansac, L., additional, Moutard, T., additional, Renzini, M. A., additional, Salvato, M., additional, Sanders, D. B., additional, Scoville, N., additional, Sheth, K., additional, Silverman, J. D., additional, Smolčić, V., additional, Taniguchi, Y., additional, and Tresse, L., additional
Published: 2015
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8. Extreme emission-line galaxies out toz~ 1 in zCOSMOS

Author: Amorín, R., primary, Pérez-Montero, E., additional, Contini, T., additional, Vílchez, J. M., additional, Bolzonella, M., additional, Tasca, L. A. M., additional, Lamareille, F., additional, Zamorani, G., additional, Maier, C., additional, Carollo, C. M., additional, Kneib, J.-P., additional, Le Fèvre, O., additional, Lilly, S., additional, Mainieri, V., additional, Renzini, A., additional, Scodeggio, M., additional, Bardelli, S., additional, Bongiorno, A., additional, Caputi, K., additional, Cucciati, O., additional, de la Torre, S., additional, de Ravel, L., additional, Franzetti, P., additional, Garilli, B., additional, Iovino, A., additional, Kampczyk, P., additional, Knobel, C., additional, Kovač, K., additional, Le Borgne, J.-F., additional, Le Brun, V., additional, Mignoli, M., additional, Pellò, R., additional, Peng, Y., additional, Presotto, V., additional, Ricciardelli, E., additional, Silverman, J. D., additional, Tanaka, M., additional, Tresse, L., additional, Vergani, D., additional, and Zucca, E., additional
Published: 2015
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9. Mass-metallicity relation of zCOSMOS galaxies atz≈ 0.7, its dependence on star formation rate, and the existence of massive low-metallicity galaxies

Author: Maier, C., primary, Ziegler, B. L., additional, Lilly, S. J., additional, Contini, T., additional, Pérez-Montero, E., additional, Lamareille, F., additional, Bolzonella, M., additional, and Le Floc’h, E., additional
Published: 2015
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10. Passive galaxies as tracers of cluster environments atz~ 2

Author: Strazzullo, V., primary, Daddi, E., additional, Gobat, R., additional, Garilli, B., additional, Mignoli, M., additional, Valentino, F., additional, Onodera, M., additional, Renzini, A., additional, Cimatti, A., additional, Finoguenov, A., additional, Arimoto, N., additional, Cappellari, M., additional, Carollo, C. M., additional, Feruglio, C., additional, Le Floc’h, E., additional, Lilly, S. J., additional, Maccagni, D., additional, McCracken, H. J., additional, Moresco, M., additional, Pozzetti, L., additional, and Zamorani, G., additional
Published: 2015
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11. The MUSE 3D view of theHubbleDeep Field South

Author: Bacon, R., primary, Brinchmann, J., additional, Richard, J., additional, Contini, T., additional, Drake, A., additional, Franx, M., additional, Tacchella, S., additional, Vernet, J., additional, Wisotzki, L., additional, Blaizot, J., additional, Bouché, N., additional, Bouwens, R., additional, Cantalupo, S., additional, Carollo, C. M., additional, Carton, D., additional, Caruana, J., additional, Clément, B., additional, Dreizler, S., additional, Epinat, B., additional, Guiderdoni, B., additional, Herenz, C., additional, Husser, T.-O., additional, Kamann, S., additional, Kerutt, J., additional, Kollatschny, W., additional, Krajnovic, D., additional, Lilly, S., additional, Martinsson, T., additional, Michel-Dansac, L., additional, Patricio, V., additional, Schaye, J., additional, Shirazi, M., additional, Soto, K., additional, Soucail, G., additional, Steinmetz, M., additional, Urrutia, T., additional, Weilbacher, P., additional, and de Zeeuw, T., additional
Published: 2015
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12. ZCOSMOS 10k-bright spectroscopic sample

Author: Moresco, M., Pozzetti, L., Cimatti, A., Zamorani, G., Mignoli, M., Di Cesare, S., Bolzonella, M., Zucca, E., Lilly, S., Kovač, K., Scodeggio, M., Cassata, P., Tasca, L., Vergani, D., Halliday, C., Carollo, M., Contini, T., Kneib, J. -P., Le Févre, O., Mainieri, V., Renzini, A., Bardelli, S., Bongiorno, A., Caputi, K., Coppa, G., Cucciati, O., De La Torre, S., De Ravel, L., Franzetti, P., Garilli, B., Iovino, A., Kampczyk, P., Knobel, C., Lamareille, F., Le Borgne, J. -F., Le Brun, V., Maier, C., Pellò, R., Peng, Y., Perez Montero, E., Ricciardelli, E., Silverman, J. D., Tanaka, M., Tresse, L., Abbas, U., Bottini, D., Cappi, A., Guzzo, L., Koekemoer, A. M., Leauthaud, A., Maccagni, D., Marinoni, C., Mccracken, H. J., Memeo, P., Meneux, B., Nair, P., Oesch, P., Porciani, C., Scaramella, R., Scarlata, C., and Scoville, N.
Subjects: surveys, Space and Planetary Science, galaxies: evolution, galaxies: fundamental parameters, galaxies: statistics, Astronomy and Astrophysics
Published: 2010

13. The zCOSMOS redshift survey: evolution of the light in bulges and discs sincez~ 0.8

Author: Tasca, L. A. M., primary, Tresse, L., additional, Le Fèvre, O., additional, Ilbert, O., additional, Lilly, S. J., additional, Zamorani, G., additional, López-Sanjuan, C., additional, Ho, L. C., additional, Bardelli, S., additional, Cattaneo, A., additional, Cucciati, O., additional, Farrah, D., additional, Iovino, A., additional, Koekemoer, A. M., additional, Liu, C. T., additional, Massey, R., additional, Renzini, A., additional, Taniguchi, Y., additional, Welikala, N., additional, Zucca, E., additional, Carollo, C. M., additional, Contini, T., additional, Kneib, J.-P., additional, Mainieri, V., additional, Scodeggio, M., additional, Bolzonella, M., additional, Bongiorno, A., additional, Caputi, K., additional, de la Torre, S., additional, Franzetti, P., additional, Garilli, B., additional, Guzzo, L., additional, Kampczyk, P., additional, Knobel, C., additional, Kovač, K., additional, Lamareille, F., additional, Le Borgne, J.-F., additional, Le Brun, V., additional, Maier, C., additional, Mignoli, M., additional, Pello, R., additional, Peng, Y., additional, Perez Montero, E., additional, Rich, R. M., additional, Tanaka, M., additional, Vergani, D., additional, Bordoloi, R., additional, Cappi, A., additional, Cimatti, A., additional, Coppa, G., additional, McCracken, H. J., additional, Moresco, M., additional, Pozzetti, L., additional, Sanders, D., additional, and Sheth, K., additional
Published: 2014
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14. The mean star-forming properties of QSO host galaxies

Author: Rosario, D. J., primary, Trakhtenbrot, B., additional, Lutz, D., additional, Netzer, H., additional, Trump, J. R., additional, Silverman, J. D., additional, Schramm, M., additional, Lusso, E., additional, Berta, S., additional, Bongiorno, A., additional, Brusa, M., additional, Förster-Schreiber, N. M., additional, Genzel, R., additional, Lilly, S., additional, Magnelli, B., additional, Mainieri, V., additional, Maiolino, R., additional, Merloni, A., additional, Mignoli, M., additional, Nordon, R., additional, Popesso, P., additional, Salvato, M., additional, Santini, P., additional, Tacconi, L. J., additional, and Zamorani, G., additional
Published: 2013
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15. Deep Galaxy survey at 6.75µm with the ISO satellite

Author: Flores, H., Hammer, F., Désert, F. X., Césarsky, C., Thuan, T., Crampton, D., Eales, Stephen Anthony, Le Fèvre, O., Lilly, S. J., Omont, A., and Elbaz, D.
Subjects: QB
Abstract: Deep 6.75µm mid-IR ISOCAM observations were obtained from the Canada-France Redshift Survey (CFRS) 1415+52 field with the Infrared Space Observatory. The identification of the sources with optical counterparts is described in detail, and a classification scheme is devised which depends on the S/N of the detection and the inverse probability of chance coincidence. 83% of the 54ISOCAMsources are identified with IAB 1 of the 44 S6:75µm > 150µJy sources which are non-stellar (7 ”spectroscopic” and 3 ”photometric” stars excluded).
Published: 1999

16. Spot the difference

Author: Moresco, M., primary, Pozzetti, L., additional, Cimatti, A., additional, Zamorani, G., additional, Bolzonella, M., additional, Lamareille, F., additional, Mignoli, M., additional, Zucca, E., additional, Lilly, S. J., additional, Carollo, C. M., additional, Contini, T., additional, Kneib, J.-P., additional, Le Fèvre, O., additional, Mainieri, V., additional, Renzini, A., additional, Scodeggio, M., additional, Bardelli, S., additional, Bongiorno, A., additional, Caputi, K., additional, Cucciati, O., additional, de la Torre, S., additional, de Ravel, L., additional, Franzetti, P., additional, Garilli, B., additional, Iovino, A., additional, Kampczyk, P., additional, Knobel, C., additional, Kovač, K., additional, Le Borgne, J.-F., additional, Le Brun, V., additional, Maier, C., additional, Pelló, R., additional, Peng, Y., additional, Perez-Montero, E., additional, Presotto, V., additional, Silverman, J. D., additional, Tanaka, M., additional, Tasca, L., additional, Tresse, L., additional, Vergani, D., additional, Barnes, L., additional, Bordoloi, R., additional, Cappi, A., additional, Diener, C., additional, Koekemoer, A. M., additional, Le Floc’h, E., additional, López-Sanjuan, C., additional, McCracken, H. J., additional, Nair, P., additional, Oesch, P., additional, Scarlata, C., additional, Scoville, N., additional, and Welikala, N., additional
Published: 2013
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17. Mass assembly in quiescent and star-forming galaxies sincez≃ 4 from UltraVISTA

Author: Ilbert, O., primary, McCracken, H. J., additional, Le Fèvre, O., additional, Capak, P., additional, Dunlop, J., additional, Karim, A., additional, Renzini, M. A., additional, Caputi, K., additional, Boissier, S., additional, Arnouts, S., additional, Aussel, H., additional, Comparat, J., additional, Guo, Q., additional, Hudelot, P., additional, Kartaltepe, J., additional, Kneib, J. P., additional, Krogager, J. K., additional, Le Floc’h, E., additional, Lilly, S., additional, Mellier, Y., additional, Milvang-Jensen, B., additional, Moutard, T., additional, Onodera, M., additional, Richard, J., additional, Salvato, M., additional, Sanders, D. B., additional, Scoville, N., additional, Silverman, J. D., additional, Taniguchi, Y., additional, Tasca, L., additional, Thomas, R., additional, Toft, S., additional, Tresse, L., additional, Vergani, D., additional, Wolk, M., additional, and Zirm, A., additional
Published: 2013
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18. Obscured AGN atz ~ 1 from the zCOSMOS-Bright Survey

Author: Mignoli, M., primary, Vignali, C., additional, Gilli, R., additional, Comastri, A., additional, Zamorani, G., additional, Bolzonella, M., additional, Bongiorno, A., additional, Lamareille, F., additional, Nair, P., additional, Pozzetti, L., additional, Lilly, S. J., additional, Carollo, C. M., additional, Contini, T., additional, Kneib, J.-P., additional, Le Fèvre, O., additional, Mainieri, V., additional, Renzini, A., additional, Scodeggio, M., additional, Bardelli, S., additional, Caputi, K., additional, Cucciati, O., additional, de la Torre, S., additional, de Ravel, L., additional, Franzetti, P., additional, Garilli, B., additional, Iovino, A., additional, Kampczyk, P., additional, Knobel, C., additional, Kovač, K., additional, Le Borgne, J.-F., additional, Le Brun, V., additional, Maier, C., additional, Pellò, R., additional, Peng, Y., additional, Perez Montero, E., additional, Presotto, V., additional, Silverman, J. D., additional, Tanaka, M., additional, Tasca, L., additional, Tresse, L., additional, Vergani, D., additional, Zucca, E., additional, Bordoloi, R., additional, Cappi, A., additional, Cimatti, A., additional, Koekemoer, A. M., additional, McCracken, H. J., additional, Moresco, M., additional, and Welikala, N., additional
Published: 2013
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19. Investigating the relationship between AGN activity and stellar mass in zCOSMOS galaxies at 0 < z < 1 using emission-line diagnostic diagrams

Author: Vitale, M., primary, Mignoli, M., additional, Cimatti, A., additional, Lilly, S. J., additional, Carollo, C. M., additional, Contini, T., additional, Kneib, J.-P., additional, Le Fevre, O., additional, Mainieri, V., additional, Renzini, A., additional, Scodeggio, M., additional, Zamorani, G., additional, Bardelli, S., additional, Barnes, L., additional, Bolzonella, M., additional, Bongiorno, A., additional, Bordoloi, R., additional, Bschorr, T. J., additional, Cappi, A., additional, Caputi, K., additional, Coppa, G., additional, Cucciati, O., additional, de la Torre, S., additional, de Ravel, L., additional, Franzetti, P., additional, Garilli, B., additional, Iovino, A., additional, Kampczyk, P., additional, Knobel, C., additional, Koekemoer, A. M., additional, Kovač, K., additional, Lamareille, F., additional, Le Borgne, J.-F., additional, Le Brun, V., additional, López-Sanjuan, C., additional, Maier, C., additional, McCracken, H. J., additional, Moresco, M., additional, Nair, P., additional, Oesch, P. A., additional, Pello, R., additional, Peng, Y., additional, Pérez Montero, E., additional, Pozzetti, L., additional, Presotto, V., additional, Silverman, J., additional, Tanaka, M., additional, Tasca, L., additional, Tresse, L., additional, Vergani, D., additional, Welikala, N., additional, and Zucca, E., additional
Published: 2013
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20. The cosmic evolution of oxygen and nitrogen abundances in star-forming galaxies over the past 10 Gyr

Author: Pérez-Montero, E., primary, Contini, T., additional, Lamareille, F., additional, Maier, C., additional, Carollo, C. M., additional, Kneib, J.-P., additional, Le Fèvre, O., additional, Lilly, S., additional, Mainieri, V., additional, Renzini, A., additional, Scodeggio, M., additional, Zamorani, G., additional, Bardelli, S., additional, Bolzonella, M., additional, Bongiorno, A., additional, Caputi, K., additional, Cucciati, O., additional, de la Torre, S., additional, de Ravel, L., additional, Franzetti, P., additional, Garilli, B., additional, Iovino, A., additional, Kampczyk, P., additional, Knobel, C., additional, Kovač, K., additional, Le Borgne, J.-F., additional, Le Brun, V., additional, Mignoli, M., additional, Pellò, R., additional, Peng, Y., additional, Presotto, V., additional, Ricciardelli, E., additional, Silverman, J. D., additional, Tanaka, M., additional, Tasca, L. A. M., additional, Tresse, L., additional, Vergani, D., additional, and Zucca, E., additional
Published: 2012
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21. Millimeter imaging of submillimeter galaxies in the COSMOS field: redshift distribution

Author: Smolčić, V., primary, Aravena, M., additional, Navarrete, F., additional, Schinnerer, E., additional, Riechers, D. A., additional, Bertoldi, F., additional, Feruglio, C., additional, Finoguenov, A., additional, Salvato, M., additional, Sargent, M., additional, McCracken, H. J., additional, Albrecht, M., additional, Karim, A., additional, Capak, P., additional, Carilli, C. L., additional, Cappelluti, N., additional, Elvis, M., additional, Ilbert, O., additional, Kartaltepe, J., additional, Lilly, S., additional, Sanders, D., additional, Sheth, K., additional, Scoville, N. Z., additional, and Taniguchi, Y., additional
Published: 2012
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22. The dominant role of mergers in the size evolution of massive early-type galaxies sincez ~ 1

Author: López-Sanjuan, C., primary, Le Fèvre, O., additional, Ilbert, O., additional, Tasca, L. A. M., additional, Bridge, C., additional, Cucciati, O., additional, Kampczyk, P., additional, Pozzetti, L., additional, Xu, C. K., additional, Carollo, C. M., additional, Contini, T., additional, Kneib, J.-P., additional, Lilly, S. J., additional, Mainieri, V., additional, Renzini, A., additional, Sanders, D., additional, Scodeggio, M., additional, Scoville, N. Z., additional, Taniguchi, Y., additional, Zamorani, G., additional, Aussel, H., additional, Bardelli, S., additional, Bolzonella, M., additional, Bongiorno, A., additional, Capak, P., additional, Caputi, K., additional, de la Torre, S., additional, de Ravel, L., additional, Franzetti, P., additional, Garilli, B., additional, Iovino, A., additional, Knobel, C., additional, Kovač, K., additional, Lamareille, F., additional, Le Borgne, J.-F., additional, Le Brun, V., additional, Le Floc’h, E., additional, Maier, C., additional, McCracken, H. J., additional, Mignoli, M., additional, Pelló, R., additional, Peng, Y., additional, Pérez-Montero, E., additional, Presotto, V., additional, Ricciardelli, E., additional, Salvato, M., additional, Silverman, J. D., additional, Tanaka, M., additional, Tresse, L., additional, Vergani, D., additional, Zucca, E., additional, Barnes, L., additional, Bordoloi, R., additional, Cappi, A., additional, Cimatti, A., additional, Coppa, G., additional, Koekemoer, A., additional, Liu, C. T., additional, Moresco, M., additional, Nair, P., additional, Oesch, P., additional, Schawinski, K., additional, and Welikala, N., additional
Published: 2012
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23. A journey from the outskirts to the cores of groups

Author: Presotto, V., primary, Iovino, A., additional, Scodeggio, M., additional, Cucciati, O., additional, Knobel, C., additional, Bolzonella, M., additional, Oesch, P., additional, Finoguenov, A., additional, Tanaka, M., additional, Kovač, K., additional, Peng, Y., additional, Zamorani, G., additional, Bardelli, S., additional, Pozzetti, L., additional, Kampczyk, P., additional, López-Sanjuan, C., additional, Vergani, D., additional, Zucca, E., additional, Tasca, L. A. M., additional, Carollo, C. M., additional, Contini, T., additional, Kneib, J.-P., additional, Le Fèvre, O., additional, Lilly, S., additional, Mainieri, V., additional, Renzini, A., additional, Bongiorno, A., additional, Caputi, K., additional, de la Torre, S., additional, de Ravel, L., additional, Franzetti, P., additional, Garilli, B., additional, Lamareille, F., additional, Le Borgne, J.-F., additional, Le Brun, V., additional, Maier, C., additional, Mignoli, M., additional, Pellò, R., additional, Perez-Montero, E., additional, Ricciardelli, E., additional, Silverman, J. D., additional, Tresse, L., additional, Barnes, L., additional, Bordoloi, R., additional, Cappi, A., additional, Cimatti, A., additional, Coppa, G., additional, Koekemoer, A. M., additional, McCracken, H. J., additional, Moresco, M., additional, Nair, P., additional, and Welikala, N., additional
Published: 2012
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24. The galaxy stellar mass function of X-ray detected groups

Author: Giodini, S., primary, Finoguenov, A., additional, Pierini, D., additional, Zamorani, G., additional, Ilbert, O., additional, Lilly, S., additional, Peng, Y., additional, Scoville, N., additional, and Tanaka, M., additional
Published: 2012
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25. Black hole accretion and host galaxies of obscured quasars in XMM-COSMOS

Author: Mainieri, V., primary, Bongiorno, A., additional, Merloni, A., additional, Aller, M., additional, Carollo, M., additional, Iwasawa, K., additional, Koekemoer, A. M., additional, Mignoli, M., additional, Silverman, J. D., additional, Bolzonella, M., additional, Brusa, M., additional, Comastri, A., additional, Gilli, R., additional, Halliday, C., additional, Ilbert, O., additional, Lusso, E., additional, Salvato, M., additional, Vignali, C., additional, Zamorani, G., additional, Contini, T., additional, Kneib, J.-P., additional, Le Fèvre, O., additional, Lilly, S., additional, Renzini, A., additional, Scodeggio, M., additional, Balestra, I., additional, Bardelli, S., additional, Caputi, K., additional, Coppa, G., additional, Cucciati, O., additional, de la Torre, S., additional, de Ravel, L., additional, Franzetti, P., additional, Garilli, B., additional, Iovino, A., additional, Kampczyk, P., additional, Knobel, C., additional, Kovač, K., additional, Lamareille, F., additional, Le Borgne, J.-F., additional, Le Brun, V., additional, Maier, C., additional, Nair, P., additional, Pello, R., additional, Peng, Y., additional, Perez Montero, E., additional, Pozzetti, L., additional, Ricciardelli, E., additional, Tanaka, M., additional, Tasca, L., additional, Tresse, L., additional, Vergani, D., additional, Zucca, E., additional, Aussel, H., additional, Capak, P., additional, Cappelluti, N., additional, Elvis, M., additional, Fiore, F., additional, Hasinger, G., additional, Impey, C., additional, Le Floc’h, E., additional, Scoville, N., additional, Taniguchi, Y., additional, and Trump, J., additional
Published: 2011
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26. The bimodality of the 10k zCOSMOS-bright galaxies up toz ~ 1: a new statistical and portable classification based on optical galaxy properties

Author: Coppa, G., primary, Mignoli, M., additional, Zamorani, G., additional, Bardelli, S., additional, Lilly, S. J., additional, Bolzonella, M., additional, Scodeggio, M., additional, Vergani, D., additional, Nair, P., additional, Pozzetti, L., additional, Cimatti, A., additional, Zucca, E., additional, Carollo, C. M., additional, Contini, T., additional, Le Fèvre, O., additional, Renzini, A., additional, Mainieri, V., additional, Bongiorno, A., additional, Caputi, K. I., additional, Cucciati, O., additional, de la Torre, S., additional, de Ravel, L., additional, Franzetti, P., additional, Garilli, B., additional, Memeo, P., additional, Iovino, A., additional, Kampczyk, P., additional, Kneib, J.-P., additional, Knobel, C., additional, Koekemoer, A. M., additional, Kovač, K., additional, Lamareille, F., additional, le Borgne, J.-F., additional, le Brun, V., additional, Maier, C., additional, Pellò, R., additional, Peng, Y., additional, Perez-Montero, E., additional, Ricciardelli, E., additional, Scarlata, C., additional, Silverman, J. D., additional, Tanaka, M., additional, Tasca, L., additional, Tresse, L., additional, Abbas, U., additional, Bottini, D., additional, Capak, P., additional, Cappi, A., additional, Cassata, P., additional, Fumana, M., additional, Guzzo, L., additional, Leauthaud, A., additional, Maccagni, D., additional, Marinoni, C., additional, Meneux, B., additional, Oesch, P., additional, Porciani, C., additional, Scaramella, R., additional, and Scoville, N., additional
Published: 2011
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27. zCOSMOS 10k-bright spectroscopic sample

Author: Moresco, M., primary, Pozzetti, L., additional, Cimatti, A., additional, Zamorani, G., additional, Mignoli, M., additional, Di Cesare, S., additional, Bolzonella, M., additional, Zucca, E., additional, Lilly, S., additional, Kovač, K., additional, Scodeggio, M., additional, Cassata, P., additional, Tasca, L., additional, Vergani, D., additional, Halliday, C., additional, Carollo, M., additional, Contini, T., additional, Kneib, J.-P., additional, Le Févre, O., additional, Mainieri, V., additional, Renzini, A., additional, Bardelli, S., additional, Bongiorno, A., additional, Caputi, K., additional, Coppa, G., additional, Cucciati, O., additional, de la Torre, S., additional, de Ravel, L., additional, Franzetti, P., additional, Garilli, B., additional, Iovino, A., additional, Kampczyk, P., additional, Knobel, C., additional, Lamareille, F., additional, Le Borgne, J.-F., additional, Le Brun, V., additional, Maier, C., additional, Pellò, R., additional, Peng, Y., additional, Perez Montero, E., additional, Ricciardelli, E., additional, Silverman, J. D., additional, Tanaka, M., additional, Tresse, L., additional, Abbas, U., additional, Bottini, D., additional, Cappi, A., additional, Guzzo, L., additional, Koekemoer, A. M., additional, Leauthaud, A., additional, Maccagni, D., additional, Marinoni, C., additional, McCracken, H. J., additional, Memeo, P., additional, Meneux, B., additional, Nair, P., additional, Oesch, P., additional, Porciani, C., additional, Scaramella, R., additional, Scarlata, C., additional, and Scoville, N., additional
Published: 2010
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28. Tracking the impact of environment on the galaxy stellar mass function up toz ~ 1 in the 10 k zCOSMOS sample

Author: Bolzonella, M., primary, Kovač, K., additional, Pozzetti, L., additional, Zucca, E., additional, Cucciati, O., additional, Lilly, S. J., additional, Peng, Y., additional, Iovino, A., additional, Zamorani, G., additional, Vergani, D., additional, Tasca, L. A. M., additional, Lamareille, F., additional, Oesch, P., additional, Caputi, K., additional, Kampczyk, P., additional, Bardelli, S., additional, Maier, C., additional, Abbas, U., additional, Knobel, C., additional, Scodeggio, M., additional, Carollo, C. M., additional, Contini, T., additional, Kneib, J.-P., additional, Le Fèvre, O., additional, Mainieri, V., additional, Renzini, A., additional, Bongiorno, A., additional, Coppa, G., additional, de la Torre, S., additional, de Ravel, L., additional, Franzetti, P., additional, Garilli, B., additional, Le Borgne, J.-F., additional, Le Brun, V., additional, Mignoli, M., additional, Pelló, R., additional, Perez-Montero, E., additional, Ricciardelli, E., additional, Silverman, J. D., additional, Tanaka, M., additional, Tresse, L., additional, Bottini, D., additional, Cappi, A., additional, Cassata, P., additional, Cimatti, A., additional, Guzzo, L., additional, Koekemoer, A. M., additional, Leauthaud, A., additional, Maccagni, D., additional, Marinoni, C., additional, McCracken, H. J., additional, Memeo, P., additional, Meneux, B., additional, Porciani, C., additional, Scaramella, R., additional, Aussel, H., additional, Capak, P., additional, Halliday, C., additional, Ilbert, O., additional, Kartaltepe, J., additional, Salvato, M., additional, Sanders, D., additional, Scarlata, C., additional, Scoville, N., additional, Taniguchi, Y., additional, and Thompson, D., additional
Published: 2010
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29. The zCOSMOS 10k-sample: the role of galaxy stellar mass in the colour-density relation up toz ~ 1

Author: Cucciati, O., primary, Iovino, A., additional, Kovač, K., additional, Scodeggio, M., additional, Lilly, S. J., additional, Bolzonella, M., additional, Bardelli, S., additional, Vergani, D., additional, Tasca, L. A. M., additional, Zucca, E., additional, Zamorani, G., additional, Pozzetti, L., additional, Knobel, C., additional, Oesch, P., additional, Lamareille, F., additional, Caputi, K., additional, Kampczyk, P., additional, Tresse, L., additional, Maier, C., additional, Carollo, C. M., additional, Contini, T., additional, Kneib, J.-P., additional, Le Fèvre, O., additional, Mainieri, V., additional, Renzini, A., additional, Bongiorno, A., additional, Coppa, G., additional, de la Torre, S., additional, de Ravel, L., additional, Franzetti, P., additional, Garilli, B., additional, Le Borgne, J.-F., additional, Le Brun, V., additional, Mignoli, M., additional, Pellò, R., additional, Peng, Y., additional, Perez-Montero, E., additional, Ricciardelli, E., additional, Silverman, J. D., additional, Tanaka, M., additional, Koekemoer, A. M., additional, Scoville, N., additional, Abbas, U., additional, Bottini, D., additional, Cappi, A., additional, Cassata, P., additional, Cimatti, A., additional, Guzzo, L., additional, Leauthaud, A., additional, Maccagni, D., additional, Marinoni, C., additional, McCracken, H. J., additional, Memeo, P., additional, Meneux, B., additional, Porciani, C., additional, and Scaramella, R., additional
Published: 2010
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30. zCOSMOS – 10k-bright spectroscopic sample

Author: Pozzetti, L., primary, Bolzonella, M., additional, Zucca, E., additional, Zamorani, G., additional, Lilly, S., additional, Renzini, A., additional, Moresco, M., additional, Mignoli, M., additional, Cassata, P., additional, Tasca, L., additional, Lamareille, F., additional, Maier, C., additional, Meneux, B., additional, Halliday, C., additional, Oesch, P., additional, Vergani, D., additional, Caputi, K., additional, Kovač, K., additional, Cimatti, A., additional, Cucciati, O., additional, Iovino, A., additional, Peng, Y., additional, Carollo, M., additional, Contini, T., additional, Kneib, J.-P., additional, Le Févre, O., additional, Mainieri, V., additional, Scodeggio, M., additional, Bardelli, S., additional, Bongiorno, A., additional, Coppa, G., additional, de la Torre, S., additional, de Ravel, L., additional, Franzetti, P., additional, Garilli, B., additional, Kampczyk, P., additional, Knobel, C., additional, Le Borgne, J.-F., additional, Le Brun, V., additional, Pellò, R., additional, Perez Montero, E., additional, Ricciardelli, E., additional, Silverman, J. D., additional, Tanaka, M., additional, Tresse, L., additional, Abbas, U., additional, Bottini, D., additional, Cappi, A., additional, Guzzo, L., additional, Koekemoer, A. M., additional, Leauthaud, A., additional, Maccagni, D., additional, Marinoni, C., additional, McCracken, H. J., additional, Memeo, P., additional, Porciani, C., additional, Scaramella, R., additional, Scarlata, C., additional, and Scoville, N., additional
Published: 2010
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31. Ultraluminous X-ray sources out toz~ 0.3 in the COSMOS field

Author: Mainieri, V., primary, Vignali, C., additional, Merloni, A., additional, Civano, F., additional, Puccetti, S., additional, Brusa, M., additional, Gilli, R., additional, Bolzonella, M., additional, Comastri, A., additional, Zamorani, G., additional, Aller, M., additional, Carollo, M., additional, Scarlata, C., additional, Elvis, M., additional, Aldcroft, T. L., additional, Cappelluti, N., additional, Fabbiano, G., additional, Finoguenov, A., additional, Fiore, F., additional, Fruscione, A., additional, Koekemoer, A. M., additional, Contini, T., additional, Kneib, J.-P., additional, Le Fèvre, O., additional, Lilly, S., additional, Renzini, A., additional, Scodeggio, M., additional, Bardelli, S., additional, Bongiorno, A., additional, Caputi, K., additional, Coppa, G., additional, Cucciati, O., additional, de la Torre, S., additional, de Ravel, L., additional, Franzetti, P., additional, Garilli, B., additional, Iovino, A., additional, Kampczyk, P., additional, Knobel, C., additional, Kovač, K., additional, Lamareille, F., additional, Le Borgne, J.-F., additional, Le Brun, V., additional, Maier, C., additional, Mignoli, M., additional, Pello, R., additional, Peng, Y., additional, Perez Montero, E., additional, Ricciardelli, E., additional, Silverman, J. D., additional, Tanaka, M., additional, Tasca, L., additional, Tresse, L., additional, Vergani, D., additional, Zucca, E., additional, Capak, P., additional, Ilbert, O., additional, Impey, C., additional, Salvato, M., additional, Scoville, N., additional, Taniguchi, Y., additional, and Trump, J., additional
Published: 2010
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32. The X-ray to optical-UV luminosity ratio of X-ray selected type 1 AGN in XMM-COSMOS

Author: Lusso, E., primary, Comastri, A., additional, Vignali, C., additional, Zamorani, G., additional, Brusa, M., additional, Gilli, R., additional, Iwasawa, K., additional, Salvato, M., additional, Civano, F., additional, Elvis, M., additional, Merloni, A., additional, Bongiorno, A., additional, Trump, J. R., additional, Koekemoer, A. M., additional, Schinnerer, E., additional, Le Floc'h, E., additional, Cappelluti, N., additional, Jahnke, K., additional, Sargent, M., additional, Silverman, J., additional, Mainieri, V., additional, Fiore, F., additional, Bolzonella, M., additional, Le Fèvre, O., additional, Garilli, B., additional, Iovino, A., additional, Kneib, J. P., additional, Lamareille, F., additional, Lilly, S., additional, Mignoli, M., additional, Scodeggio, M., additional, and Vergani, D., additional
Published: 2010
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33. The [O iii] emission line luminosity function of optically selected type-2 AGN from zCOSMOS$^{\rm,}$

Author: Bongiorno, A., primary, Mignoli, M., additional, Zamorani, G., additional, Lamareille, F., additional, Lanzuisi, G., additional, Miyaji, T., additional, Bolzonella, M., additional, Carollo, C. M., additional, Contini, T., additional, Kneib, J. P., additional, Le Fèvre, O., additional, Lilly, S. J., additional, Mainieri, V., additional, Renzini, A., additional, Scodeggio, M., additional, Bardelli, S., additional, Brusa, M., additional, Caputi, K., additional, Civano, F., additional, Coppa, G., additional, Cucciati, O., additional, de la Torre, S., additional, de Ravel, L., additional, Franzetti, P., additional, Garilli, B., additional, Halliday, C., additional, Hasinger, G., additional, Koekemoer, A. M., additional, Iovino, A., additional, Kampczyk, P., additional, Knobel, C., additional, Kovač, K., additional, Le Borgne, J. -F., additional, Le Brun, V., additional, Maier, C., additional, Merloni, A., additional, Nair, P., additional, Pello, R., additional, Peng, Y., additional, Perez Montero, E., additional, Ricciardelli, E., additional, Salvato, M., additional, Silverman, J., additional, Tanaka, M., additional, Tasca, L., additional, Tresse, L., additional, Vergani, D., additional, Zucca, E., additional, Abbas, U., additional, Bottini, D., additional, Cappi, A., additional, Cassata, P., additional, Cimatti, A., additional, Guzzo, L., additional, Leauthaud, A., additional, Maccagni, D., additional, Marinoni, C., additional, McCracken, H. J., additional, Memeo, P., additional, Meneux, B., additional, Oesch, P., additional, Porciani, C., additional, Pozzetti, L., additional, and Scaramella, R., additional
Published: 2010
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34. Properties and environment of radio-emitting galaxies in the VLA-zCOSMOS survey

Author: Bardelli, S., primary, Schinnerer, E., additional, Smolčic, V., additional, Zamorani, G., additional, Zucca, E., additional, Mignoli, M., additional, Halliday, C., additional, Kovač, K., additional, Ciliegi, P., additional, Caputi, K., additional, Koekemoer, A. M., additional, Bongiorno, A., additional, Bondi, M., additional, Bolzonella, M., additional, Vergani, D., additional, Pozzetti, L., additional, Carollo, C. M., additional, Contini, T., additional, Kneib, J.-P., additional, Le Fèvre, O., additional, Lilly, S., additional, Mainieri, V., additional, Renzini, A., additional, Scodeggio, M., additional, Coppa, G., additional, Cucciati, O., additional, de la Torre, S., additional, de Ravel, L., additional, Franzetti, P., additional, Garilli, B., additional, Iovino, A., additional, Kampczyk, P., additional, Knobel, C., additional, Lamareille, F., additional, Le Borgne, J.-F., additional, Le Brun, V., additional, Maier, C., additional, Pellò, R., additional, Peng, Y., additional, Perez-Montero, E., additional, Ricciardelli, E., additional, Silverman, J. D., additional, Tanaka, M., additional, Tasca, L., additional, Tresse, L., additional, Abbas, U., additional, Bottini, D., additional, Cappi, A., additional, Cassata, P., additional, Cimatti, A., additional, Guzzo, L., additional, Leauthaud, A., additional, Maccagni, D., additional, Marinoni, C., additional, McCracken, H. J., additional, Memeo, P., additional, Meneux, B., additional, Oesch, P., additional, Porciani, C., additional, Scaramella, R., additional, Capak, P., additional, Sanders, D., additional, Scoville, N., additional, Taniguchi, Y., additional, and Jahnke, K., additional
Published: 2010
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35. The zCOSMOS redshift survey: how group environment alters global downsizing trends

Author: Iovino, A., primary, Cucciati, O., additional, Scodeggio, M., additional, Knobel, C., additional, Kovač, K., additional, Lilly, S., additional, Bolzonella, M., additional, Tasca, L. A. M., additional, Zamorani, G., additional, Zucca, E., additional, Caputi, K., additional, Pozzetti, L., additional, Oesch, P., additional, Lamareille, F., additional, Halliday, C., additional, Bardelli, S., additional, Finoguenov, A., additional, Guzzo, L., additional, Kampczyk, P., additional, Maier, C., additional, Tanaka, M., additional, Vergani, D., additional, Carollo, C. M., additional, Contini, T., additional, Kneib, J.-P., additional, Le Fèvre, O., additional, Mainieri, V., additional, Renzini, A., additional, Bongiorno, A., additional, Coppa, G., additional, de la Torre, S., additional, de Ravel, L., additional, Franzetti, P., additional, Garilli, B., additional, Le Borgne, J.-F., additional, Le Brun, V., additional, Mignoli, M., additional, Pellò, R., additional, Peng, Y., additional, Perez-Montero, E., additional, Ricciardelli, E., additional, Silverman, J. D., additional, Tresse, L., additional, Abbas, U., additional, Bottini, D., additional, Cappi, A., additional, Cassata, P., additional, Cimatti, A., additional, Koekemoer, A. M., additional, Leauthaud, A., additional, Maccagni, D., additional, Marinoni, C., additional, McCracken, H. J., additional, Memeo, P., additional, Meneux, B., additional, Porciani, C., additional, Scaramella, R., additional, Schiminovich, D., additional, and Scoville, N., additional
Published: 2009
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36. K+a galaxies in the zCOSMOS survey

Author: Vergani, D., primary, Zamorani, G., additional, Lilly, S., additional, Lamareille, F., additional, Halliday, C., additional, Scodeggio, M., additional, Vignali, C., additional, Ciliegi, P., additional, Bolzonella, M., additional, Bondi, M., additional, Kovač, K., additional, Knobel, C., additional, Zucca, E., additional, Caputi, K., additional, Pozzetti, L., additional, Bardelli, S., additional, Mignoli, M., additional, Iovino, A., additional, Carollo, C. M., additional, Contini, T., additional, Kneib, J.-P., additional, Le Fèvre, O., additional, Mainieri, V., additional, Renzini, A., additional, Bongiorno, A., additional, Coppa, G., additional, Cucciati, O., additional, de la Torre, S., additional, de Ravel, L., additional, Franzetti, P., additional, Garilli, B., additional, Kampczyk, P., additional, Le Borgne, J.-F., additional, Le Brun, V., additional, Maier, C., additional, Pello, R., additional, Peng, Y., additional, Perez Montero, E., additional, Ricciardelli, E., additional, Silverman, J. D., additional, Tanaka, M., additional, Tasca, L., additional, Tresse, L., additional, Abbas, U., additional, Bottini, D., additional, Cappi, A., additional, Cassata, P., additional, Cimatti, A., additional, Guzzo, L., additional, Koekemoer, A. M., additional, Leauthaud, A., additional, Maccagni, D., additional, Marinoni, C., additional, McCracken, H. J., additional, Memeo, P., additional, Meneux, B., additional, Oesch, P., additional, Porciani, C., additional, Scaramella, R., additional, Capak, P., additional, Sanders, D., additional, Scoville, N., additional, and Taniguchi, Y., additional
Published: 2009
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37. The zCOSMOS survey: the role of the environment in the evolution of the luminosity function of different galaxy types

Author: Zucca, E., primary, Bardelli, S., additional, Bolzonella, M., additional, Zamorani, G., additional, Ilbert, O., additional, Pozzetti, L., additional, Mignoli, M., additional, Kovač, K., additional, Lilly, S., additional, Tresse, L., additional, Tasca, L., additional, Cassata, P., additional, Halliday, C., additional, Vergani, D., additional, Caputi, K., additional, Carollo, C. M., additional, Contini, T., additional, Kneib, J.-P., additional, Le Fèvre, O., additional, Mainieri, V., additional, Renzini, A., additional, Scodeggio, M., additional, Bongiorno, A., additional, Coppa, G., additional, Cucciati, O., additional, de la Torre, S., additional, de Ravel, L., additional, Franzetti, P., additional, Garilli, B., additional, Iovino, A., additional, Kampczyk, P., additional, Knobel, C., additional, Lamareille, F., additional, Le Borgne, J.-F., additional, Le Brun, V., additional, Maier, C., additional, Pellò, R., additional, Peng, Y., additional, Perez-Montero, E., additional, Ricciardelli, E., additional, Silverman, J. D., additional, Tanaka, M., additional, Abbas, U., additional, Bottini, D., additional, Cappi, A., additional, Cimatti, A., additional, Guzzo, L., additional, Koekemoer, A. M., additional, Leauthaud, A., additional, Maccagni, D., additional, Marinoni, C., additional, McCracken, H. J., additional, Memeo, P., additional, Meneux, B., additional, Moresco, M., additional, Oesch, P., additional, Porciani, C., additional, Scaramella, R., additional, Arnouts, S., additional, Aussel, H., additional, Capak, P., additional, Kartaltepe, J., additional, Salvato, M., additional, Sanders, D., additional, Scoville, N., additional, Taniguchi, Y., additional, and Thompson, D., additional
Published: 2009
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38. The zCOSMOS survey. The dependence of clustering on luminosity and stellar mass at $z=0.2$–1

Author: Meneux, B., primary, Guzzo, L., additional, de la Torre, S., additional, Porciani, C., additional, Zamorani, G., additional, Abbas, U., additional, Bolzonella, M., additional, Garilli, B., additional, Iovino, A., additional, Pozzetti, L., additional, Zucca, E., additional, Lilly, S. J., additional, Le Fèvre, O., additional, Kneib, J.-P., additional, Carollo, C. M., additional, Contini, T., additional, Mainieri, V., additional, Renzini, A., additional, Scodeggio, M., additional, Bardelli, S., additional, Bongiorno, A., additional, Caputi, K., additional, Coppa, G., additional, Cucciati, O., additional, de Ravel, L., additional, Franzetti, P., additional, Kampczyk, P., additional, Knobel, C., additional, Kovač, K., additional, Lamareille, F., additional, Le Borgne, J.-F., additional, Le Brun, V., additional, Maier, C., additional, Pellò, R., additional, Peng, Y., additional, Perez Montero, E., additional, Ricciardelli, E., additional, Silverman, J. D., additional, Tanaka, M., additional, Tasca, L., additional, Tresse, L., additional, Vergani, D., additional, Bottini, D., additional, Cappi, A., additional, Cimatti, A., additional, Cassata, P., additional, Fumana, M., additional, Koekemoer, A. M., additional, Leauthaud, A., additional, Maccagni, D., additional, Marinoni, C., additional, McCracken, H. J., additional, Memeo, P., additional, Oesch, P., additional, and Scaramella, R., additional
Published: 2009
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39. The zCOSMOS redshift survey: the role of environment and stellar mass in shaping the rise of the morphology-density relation from z ~ 1

Author: Tasca, L. A. M., primary, Kneib, J.-P., additional, Iovino, A., additional, Le Fèvre, O., additional, Kovač, K., additional, Bolzonella, M., additional, Lilly, S. J., additional, Abraham, R. G., additional, Cassata, P., additional, Cucciati, O., additional, Guzzo, L., additional, Tresse, L., additional, Zamorani, G., additional, Capak, P., additional, Garilli, B., additional, Scodeggio, M., additional, Sheth, K., additional, Zucca, E., additional, Carollo, C. M., additional, Contini, T., additional, Mainieri, V., additional, Renzini, A., additional, Bardelli, S., additional, Bongiorno, A., additional, Caputi, K., additional, Coppa, G., additional, de la Torre, S., additional, de Ravel, L., additional, Franzetti, P., additional, Kampczyk, P., additional, Knobel, C., additional, Koekemoer, A. M., additional, Lamareille, F., additional, Le Borgne, J. -F., additional, Le Brun, V., additional, Maier, C., additional, Mignoli, M., additional, Pello, R., additional, Peng, Y., additional, Perez Montero, E., additional, Ricciardelli, E., additional, Silverman, J. D., additional, Vergani, D., additional, Tanaka, M., additional, Abbas, U., additional, Bottini, D., additional, Cappi, A., additional, Cimatti, A., additional, Ilbert, O., additional, Leauthaud, A., additional, Maccagni, D., additional, Marinoni, C., additional, McCracken, H. J., additional, Memeo, P., additional, Meneux, B., additional, Oesch, P., additional, Porciani, C., additional, Pozzetti, L., additional, Scaramella, R., additional, and Scarlata, C., additional
Published: 2009
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40. The spatial clustering of X-ray selected AGN in the XMM-COSMOS field

Author: Gilli, R., primary, Zamorani, G., additional, Miyaji, T., additional, Silverman, J., additional, Brusa, M., additional, Mainieri, V., additional, Cappelluti, N., additional, Daddi, E., additional, Porciani, C., additional, Pozzetti, L., additional, Civano, F., additional, Comastri, A., additional, Finoguenov, A., additional, Fiore, F., additional, Salvato, M., additional, Vignali, C., additional, Hasinger, G., additional, Lilly, S., additional, Impey, C., additional, Trump, J., additional, Capak, P., additional, McCracken, H., additional, Scoville, N., additional, Taniguchi, Y., additional, Carollo, C. M., additional, Contini, T., additional, Kneib, J.-P., additional, Le Fevre, O., additional, Renzini, A., additional, Scodeggio, M., additional, Bardelli, S., additional, Bolzonella, M., additional, Bongiorno, A., additional, Caputi, K., additional, Cimatti, A., additional, Coppa, G., additional, Cucciati, O., additional, de la Torre, S., additional, de Ravel, L., additional, Franzetti, P., additional, Garilli, B., additional, Iovino, A., additional, Kampczyk, P., additional, Knobel, C., additional, Kovač, K., additional, Lamareille, F., additional, Le Borgne, J.-F., additional, Le Brun, V., additional, Maier, C., additional, Mignoli, M., additional, Pellò, R., additional, Peng, Y., additional, Perez Montero, E., additional, Ricciardelli, E., additional, Tanaka, M., additional, Tasca, L., additional, Tresse, L., additional, Vergani, D., additional, Zucca, E., additional, Abbas, U., additional, Bottini, D., additional, Cappi, A., additional, Cassata, P., additional, Fumana, M., additional, Guzzo, L., additional, Leauthaud, A., additional, Maccagni, D., additional, Marinoni, C., additional, Memeo, P., additional, Meneux, B., additional, Oesch, P., additional, Scaramella, R., additional, and Walcher, J., additional
Published: 2008
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41. The zCOSMOS redshift survey: the three-dimensional classification cube and bimodality in galaxy physical properties

Author: Mignoli, M., primary, Zamorani, G., additional, Scodeggio, M., additional, Cimatti, A., additional, Halliday, C., additional, Lilly, S. J., additional, Pozzetti, L., additional, Vergani, D., additional, Carollo, C. M., additional, Contini, T., additional, Le Févre, O., additional, Mainieri, V., additional, Renzini, A., additional, Bardelli, S., additional, Bolzonella, M., additional, Bongiorno, A., additional, Caputi, K., additional, Coppa, G., additional, Cucciati, O., additional, de la Torre, S., additional, de Ravel, L., additional, Franzetti, P., additional, Garilli, B., additional, Iovino, A., additional, Kampczyk, P., additional, Kneib, J.-P., additional, Knobel, C., additional, Kovač, K., additional, Lamareille, F., additional, Le Borgne, J.-F., additional, Le Brun, V., additional, Maier, C., additional, Pellò, R., additional, Peng, Y., additional, Perez Montero, E., additional, Ricciardelli, E., additional, Scarlata, C., additional, Silverman, J. D., additional, Tanaka, M., additional, Tasca, L., additional, Tresse, L., additional, Zucca, E., additional, Abbas, U., additional, Bottini, D., additional, Capak, P., additional, Cappi, A., additional, Cassata, P., additional, Fumana, M., additional, Guzzo, L., additional, Leauthaud, A., additional, Maccagni, D., additional, Marinoni, C., additional, McCracken, H. J., additional, Memeo, P., additional, Meneux, B., additional, Oesch, P., additional, Porciani, C., additional, Scaramella, R., additional, and Scoville, N., additional
Published: 2008
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42. Evolution of the specific star formation rate function at z < 1.4 Dissecting the mass-SFR plane in COSMOS and GOODS.

Author: Ilbert, O., Arnouts, S., Le Floc'h, E., Aussel, H., Bethermin, M., Capak, P., Hsieh, B.-C., Kajisawa, M., Karim, A., Le Fèvre, O., Lee, N., Lilly, S., McCracken, H. J., Michel-Dansac, L., Moutard, T., Renzini, M. A., Salvato, M., Sanders, D. B., Scoville, N., and Sheth, K.
Subjects: GALACTIC redshift, STAR formation, STELLAR mass, SEMIANALYTIC sets, DARK matter, GALACTIC evolution, STELLAR luminosity function
Abstract: The relation between the stellar mass (M*) and the star formation rate (SFR) characterizes how the instantaneous star formation is determined by the galaxy past star formation history and by the growth of the dark matter structures. We deconstruct the M*-SFR plane by measuring the specific SFR functions in several stellar mass bins from z = 0.2 out to z = 1.4 (specific SFR = SFR/M*, noted sSFR). Our analysis is primary based on a 24 μm selected catalogue combining the COSMOS and GOODS surveys. We estimate the SFR by combining mid- and far-infrared data for 20500 galaxies. The sSFR functions are derived in four stellar mass bins within the range 9.5 < log(M*/M☉) < 11.5. First, we demonstrate the importance of taking into account selection effects when studying the M*-SFR relation. Secondly, we find a mass-dependent evolution of the median sSFR with redshift varying as sSFR ∞ (1 + z)b, with b increasing from b = 2.88±0.12 to b = 3.78±0.60 between M* = 109.75 M☉ and M* = 1011.1 M☉, respectively. At low masses, this evolution is consistent with the cosmological accretion rate and predictions from semi-analytical models (SAM). This agreement breaks down for more massive galaxies showing the need for a more comprehensive description of the star formation history in massive galaxies. Third, we obtain that the shape of the sSFR function is invariant with time at z < 1.4 but depends on the mass. We observe a broadening of the sSFR function ranging from 0.28 dex at M* = 109.75 M☉ to 0.46 dex at M* = 1011.1 M☉. Such increase in the intrinsic scatter of the M*-SFR relation suggests an increasing diversity of star formation histories (SFHs) as the stellar mass increases. Finally, we find a gradual decline of the sSFR with stellar mass as log10(sSFR) ∞ -0.17M*.We discuss the numerous physical processes, as gas exhaustion in hot gas halos or secular evolution, which can gradually reduce the sSFR and increase the SFH diversity. [ABSTRACT FROM AUTHOR]
Published: 2015
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43. Extreme emission-line galaxies out to z ~ 1 in zCOSMOS.

Author: Amorín, R., Pérez-Montero, E., Contini, T., Vílchez, J. M., Bolzonella, M., Tasca, L. A. M., Lamareille, F., Zamorani, G., Maier, C., Carollo, C. M., Kneib, J.-P., Le Fèvre, O., Lilly, S., Mainieri, V., Renzini, A., Scodeggio, M., Bardelli, S., Bongiorno, A., Caputi, K., and Cucciati, O.
Subjects: EMISSION-line galaxies, GALACTIC evolution, STARBURSTS, GALACTIC redshift, LOW mass stars, STELLAR mass, ASTRONOMICAL photometry
Abstract: Context. The study of large and representative samples of low-metallicity star-forming galaxies at different cosmic epochs is of great interest to the detailed understanding of the assembly history and evolution of low-mass galaxies. Aims. We present a thorough characterization of a large sample of 183 extreme emission-line galaxies (EELGs) at redshift 0.11 ≤ z ≤ 0.93 selected from the 20k zCOSMOS bright survey because of their unusually large emission line equivalent widths. Methods. We use multiwavelength COSMOS photometry, HST-ACS I-band imaging, and optical zCOSMOS spectroscopy to derive the main global properties of star-forming EELGs, such as sizes, stellar masses, star formation rates (SFR), and reliable oxygen abundances using both Â"directÂ" and Â"strong-lineÂ" methods. Results. The EELGs are extremely compact (r50 ~ 1.3 kpc), low-mass (M* ~ 107-1010 M⊙) galaxies forming stars at unusually high specific star formation rates (sSFR = SFR/M* up to 10-7 yr-1) compared to main sequence star-forming galaxies of the same stellar mass and redshift. At rest-frame UV wavelengths, the EELGs are luminous and show high surface brightness and include strong Lya emitters, as revealed by GALEX spectroscopy. We show that zCOSMOS EELGs are high-ionization, low-metallicity systems, with median 12+ log(O/H) = 8.16 Â± 0.21 (0.2 ⊙) including a handful of extremely metal-deficient (<0.1 Z⊙) EELGs. While ~80% of the EELGs show non-axisymmetric morphologies, including clumpy and cometary or tadpole galaxies, we find that ~29% of them show additional low-surface-brightness features, which strongly suggests recent or ongoing interactions. As star-forming dwarfs in the local Universe, EELGs are most often found in relative isolation. While only very few EELGs belong to compact groups, almost one third of them are found in spectroscopically confirmed loose pairs or triplets. Conclusions. The zCOSMOS EELGs are galaxies caught in a transient and probably early period of their evolution, where they are efficiently building up a significant fraction of their present-day stellar mass in an ongoing, galaxy-wide starburst. Therefore, the EELGs constitute an ideal benchmark for comparison studies between low- and high-redshift low-mass star-forming galaxies. [ABSTRACT FROM AUTHOR]
Published: 2015
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44. Mass-metallicity relation of zCOSMOS galaxies at z ≈ 0.7, its dependence on star formation rate, and the existence of massive low-metallicity galaxies.

Author: Maier, C., Ziegler, B. L., Lilly, S. J., Contini, T., Pérez-Montero, E., Lamareille, F., Bolzonella, M., and Le Floc'h, E.
Subjects: STELLAR initial mass function, STELLAR evolution, GALACTIC redshift, GALACTIC evolution, NEAR infrared radiation
Abstract: Aims. The knowledge of the number and physical nature of low-metallicity massive galaxies is crucial for determining and interpreting the mass-metallicity relation (MZR). Methods. Using VLT-ISAAC near-infrared (NIR) spectroscopy of 39 zCOSMOS 0.5 < z < 0.9 galaxies, we have measured Hα and [N II] λ 6584 emission line fluxes for galaxies with [OII] λ 3727, Hβ, and [O III] λ 5007 available from VIMOS optical spectroscopy. The NIR spectroscopy enables us to break the degeneracy of the R23 method to unambiguously derive O/H gas metallicities and star formation rates (SFRs) from extinction-corrected Hα fluxes. Results. We used the position in the D4000 vs. [OIII] λ 5007/Hβ diagram of galaxies with reliable O/Hs from NIR spectroscopy as a benchmark. This enabled us to break the lower or upper branch R23 degeneracy of additional 900 zCOSMOS galaxies at 0.5 < z < 0.9, which do not have measurements of Hα and [NII] λ 6584. Additionally, the Hα-based SFR measurements were used to find the best SFR calibration based on [O II] λ 3727 for the 0.5 < z < 0.9 zCOSMOS galaxies without Hα measurements. With a larger zCOSMOS sample of star-forming galaxies at z ≈ 0.7 with reliable O/H and SFR measurements, we studied the MZR at z ≈ 0.7 and its dependence on (specific) SFR. We find a fraction of 19% of lower mass 9.5 < log (M/M☉) < 10.3 zCOSMOS galaxies that shows a larger evolution of the MZR relation than is found in higher mass galaxies; they are more metal poor at a given mass by a factor of 2-3 than SDSS. This indicates that the low-mass MZR slope steepens at z ≈ 0.7 compared to local galaxies. Many of these galaxies with lower metallicity would be missed by studies that assume upper branch R23 solution for all galaxies. The existence of these metal-poor galaxies at z ≈ 0.7 can be interpreted as the chemical version of galaxy downsizing. Moreover, the sample of zCOSMOS galaxies shows direct evidence that the SFR influences the MZR at these redshifts. The measured metallicities for the zCOSMOS sample broadly agree with the values expected for a non-evolving fundamental metallicity relation. This comparison also reveals that galaxies with lower metallicities and typically higher (specific) SFRs, such as found in our zCOSMOS sample at z ≈ 0.7, agree with the predictions of a non-evolving Z(M, SFR). [ABSTRACT FROM AUTHOR]
Published: 2015
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45. The Canada-France deep fields survey–II: Lyman-break galaxies and galaxy clustering atz $\mathsf{\sim3}$

Author: Foucaud, S., primary, McCracken, H. J., additional, Le Fèvre, O., additional, Arnouts, S., additional, Brodwin, M., additional, Lilly, S. J., additional, Crampton, D., additional, and Mellier, Y., additional
Published: 2003
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46. The Canada-France deep fields survey

Author: McCracken, H. J., primary, Le Fèvre, O., additional, Brodwin, M., additional, Foucaud, S., additional, Lilly, S. J., additional, Crampton, D., additional, and Mellier, Y., additional
Published: 2001
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47. The zCOSMOS redshift survey:evolution of the light in bulges and discs since z ∼ 0.8.

Author: Tasca, L. A. M., Tresse, L., Le Fèvre, O., Ilbert, O., Lilly, S. J., Zamorani, G., López-Sanjuan, C., Ho, L. C., Bardelli, S., Cattaneo, A., Cucciati, O., Farrah, D., Iovino, A., Koekemoer, A. M., Liu, C. T., Massey, R., Renzini, A., Taniguchi, Y., Welikala, N., and Zucca, E.
Subjects: GALACTIC redshift, LUMINESCENCE, GALACTIC bulges, GALACTIC evolution, SPECTRUM analysis, ELLIPTICAL galaxies
Abstract: We studied the chronology of galactic bulge and disc formation by analysing the relative contributions of these components to the B-band rest-frame luminosity density at different epochs. We present the first estimate of the evolution of the fraction of rest-frame B-band light in galactic bulges and discs since redshift z ∼ 0.8. We performed a bulge-to-disc decomposition of HST/ACS images of 3266 galaxies in the zCOSMOS-bright survey with spectroscopic redshifts in the range 0.7 ⩽ z ⩽ 0.9. We find that the fraction of B-band light in bulges and discs is (26 ± 4)% and (74 ± 4)%, respectively. When compared with rest-frame B-band measurements of galaxies in the local Universe in the same mass range (109 M☉ ≲ M ≲ 1011.5 M☉), we find that the B-band light in discs decreases by ∼30% from z ∼ 0.7-0.9 to z ∼ 0, while the light from the bulge increases by ∼30% over the same period of time. We interpret this evolution as the consequence of star formation and mass assembly processes, as well as morphological transformation, which gradually shift stars formed at half the age of the Universe from star-forming late-type/irregular galaxies to earlier types and ultimately into spheroids. [ABSTRACT FROM AUTHOR]
Published: 2014
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48. Spot the difference: Impact of different selection criteria on observed properties of passive galaxies in zCOSMOS-20k sample.

Author: Moresco, M., Pozzetti, L., Cimatti, A., Zamorani, G., Bolzonella, M., Lamareille, F., Mignoli, M., Zucca, E., Lilly, S. J., Carollo, C. M., Contini, T., Kneib, J.-P., Le Fèvre, O., Mainieri, V., Renzini, A., Scodeggio, M., Bardelli, S., Bongiorno, A., Caputi, K., and Cucciati, O.
Subjects: GALACTIC evolution, ASTRONOMICAL observations, STELLAR mass, SPECTRAL energy distribution, EARLY stars
Abstract: Aims. We present the analysis of photometric, spectroscopic, and morphological properties for differently selected samples of passive galaxies up to z = 1 extracted from the zCOSMOS-20k spectroscopic survey. This analysis intends to explore the dependence of galaxy properties on the selection criterion adopted, study the degree of contamination due to star-forming outliers, and provide a comparison between different commonly used selection criteria. This work is a first step to fully investigating the selection effects of passive galaxies for future massive surveys such as Euclid. Methods. We extracted from the zCOSMOS-20k catalog six different samples of passive galaxies, based on morphology (3336 "morphological" early-type galaxies), optical colors (4889 "red-sequence" galaxies and 4882 "red UVJ" galaxies), specific star-formation rate (2937 "quiescent" galaxies), a best fit to the observed spectral energy distribution (2603 "red SED" galaxies), and a criterion that combines morphological, spectroscopic, and photometric information (1530 "red & passive early-type galaxies"). For all the samples, we studied optical and infrared colors, morphological properties, specific star-formation rates (SFRs), and the equivalent widths of the residual emission lines; this analysis was performed as a function of redshift and stellar mass to inspect further possible dependencies. Results. We find that each passive galaxy sample displays a certain level of contamination due to blue/star-forming/nonpassive outliers. The morphological sample is the one that presents the higher percentage of contamination, with ~12-65% (depending on the mass range) of galaxies not located in the red sequence, ~25-80% of galaxies with a specific SFR up to ~25 times higher than the adopted definition of passive, and significant emission lines found in the median stacked spectra, at least for log (M/M☉) < 10.25. The red & passive ETGs sample is the purest, with a percentage of contamination in color <10% for stellar masses log (M/M☉) > 10.25, very limited tails in sSFR, a median value ~20% higher than the chosen passive cut, and equivalent widths of emission lines mostly compatible with no star-formation activity. However, it is also the less economic criterion in terms of information used. Among the other criteria, we found that the best performing are the red SED and the quiescent ones, providing a percentage of contamination only slightly higher than the red & passive ETGs criterion (on average of a factor of ~2) but with absolute values of the properties of contaminants still compatible with a red, passively evolving population. We also find a strong dependence of the contamination on the stellar mass and conclude that, almost irrespective of the adopted selection criteria, a cut at log (M/M☉) > 10.75 provides a significantly purer sample in terms of star-forming contaminants. By studying the restframe color-mass and color-color diagrams, we provided two revised definitions of passive galaxies based on these criteria that better reproduce the observed bimodality in the properties of zCOSMOS-20k galaxies. The analysis of the number densities of the various samples shows evidences of mass-assembly "downsizing", with galaxies at 10.25 < log (M/M☉) < 10.75 increasing their number by a factor ~2-4 from z = 0.6 to z = 0.2, by a factor ~2-3 from z = 1 to z = 0.2 at 10.75 < log (M/M☉) < 11, and by only ~10-50% from z = 1 to z = 0.2 at 11 < log (M/M☉) < 11.5. [ABSTRACT FROM AUTHOR]
Published: 2013
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49. Obscured AGN at z ∼ 1 from the zCOSMOS-Bright Survey.

Author: Mignoli, M., Vignali, C., Gilli, R., Comastri, A., Zamorani, G., Bolzonella, M., Bongiorno, A., Lamareille, F., Nair, P., Pozzetti, L., Lilly, S. J., Carollo, C. M., Contini, T., Kneib, J.-P., Le Fèvre, O., Mainieri, V., Renzini, A., Scodeggio, M., Bardelli, S., and Caputi, K.
Subjects: ACTIVE galactic nuclei, OPTICAL spectroscopy, SEYFERT galaxies, X-ray emission spectroscopy, STELLAR mass, X-ray detection
Abstract: Aims. The application of multi-wavelength selection techniques is essential for obtaining a complete and unbiased census of active galactic nuclei (AGN). We present here a method for selecting z ∼ 1 obscured AGN from optical spectroscopic surveys. Methods. A sample of 94 narrow-line AGN with 0:65 < z < 1:20 was selected from the 20k-Bright zCOSMOS galaxy sample by detection of the high-ionization [Ne v] λ3426 line. The presence of this emission line in a galaxy spectrum is indicative of nuclear activity, although the selection is biased toward low absorbing column densities on narrow-line region or galactic scales. A similar sample of unobscured (type 1 AGN) was collected applying the same analysis to zCOSMOS broad-line objects. This paper presents and compares the optical spectral properties of the two AGN samples. Taking advantage of the large amount of data available in the COSMOS field, the properties of the [Ne v]-selected type 2 AGN were investigated, focusing on their host galaxies, X-ray emission, and optical line-flux ratios. Finally, a previously developed diagnostic, based on the X-ray-to-[Ne v] luminosity ratio, was exploited to search for the more heavily obscured AGN. Results. We found that [Ne v]-selected narrow-line AGN have Seyfert 2-like optical spectra, although their emission line ratios are diluted by a star-forming component. The ACS morphologies and stellar component in the optical spectra indicate a preference for our type 2 AGN to be hosted in early-type spirals with stellar masses greater than 109:5-10 M , on average higher than those of the galaxy parent sample. The fraction of galaxies hosting [Ne v]-selected obscured AGN increases with the stellar mass, reaching a maximum of about 3% at ≈2 × 1011 M . A comparison with other selection techniques at z ∼ 1, namely the line-ratio diagnostics and X-ray detections, shows that the detection of the [Ne v] λ3426 line is an effective method for selecting AGN in the optical band, in particular the most heavily obscured ones, but cannot provide a complete census of type 2 AGN by itself. Finally, the high fraction of [Ne v]-selected type 2 AGN not detected in medium-deep (≈100-200 ks) Chandra observations (67%) is suggestive of the inclusion of Compton-thick (i.e., with NH > 1024 cm-2) sources in our sample. The presence of a population of heavily obscured AGN is corroborated by the X-ray-to-[Ne v] ratio; we estimated, by means of an X-ray stacking technique and simulations, that the Comptonthick fraction in our sample of type 2 AGN is 43 ± 4% (statistical errors only), which agrees well with standard assumptions by XRB synthesis models. [ABSTRACT FROM AUTHOR]
Published: 2013
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50. Mass assembly in quiescent and star-forming galaxies since z ≃ 4 from UltraVISTA.

Author: Ilbert, O., McCracken, H. J., Le Fèvre, O., Capak, P., Dunlop, J., Karim, A., Renzini, M. A., Caputi, K., Boissier, S., Arnouts, S., Aussel, H., Comparat, J., Guo, Q., Hudelot, P., Kartaltepe, J., Kneib, J. P., Krogager, J. K., Le Floc'h, E., Lilly, S., and Mellier, Y.
Subjects: STAR formation, GALAXIES, STELLAR mass, MASS density gradients, REDSHIFT
Abstract: We estimate the galaxy stellar mass function and stellar mass density for star-forming and quiescent galaxies with 0.2 < z < 4. We construct a large, deep (Ks < 24) sample of 220 000 galaxies selected using the new UltraVISTA DR1 data release. Our analysis is based on precise 30-band photometric redshifts. By comparing these photometric redshifts with 10,800 spectroscopic redshifts from the zCOSMOS bright and faint surveys, we find a precision of σΔz/(1+z) = 0.008 at i+ < 22.5 and σΔ/(1+z) = 0.03 at 1.5 < z < 4. We derive the stellar mass function and correct for the Eddington bias. We find a mass-dependent evolution of the global and starforming populations, with the low-mass end of the mass functions evolving more rapidly than the high-mass end. This mass-dependent evolution is a direct consequence of the star formation being "quenched" in galaxies more massive than M ≳ 1010.7-10.9M⊚. For the mass function of the quiescent galaxies, we do not find any significant evolution of the high-mass end at z < 1; however we observe a clear flattening of the faint-end slope. From z ∼ 3 to z ∼ 1, the density of quiescent galaxies increases over the entire mass range. Their comoving stellar mass density increases by 1.6 dex between z ∼ 3 and z ∼ 1 and by less than 0.2 dex at z < 1. We infer the star formation history from the mass density evolution. This inferred star formation history is in excellent agreement with instantaneous star formation rate measurements at z < 1.5, while we find differences of 0.2 dex at z > 1.5 consistent with the expected uncertainties. We also develop a new method to infer the specific star formation rate from the mass function of star-forming galaxies. We find that the specific star formation rate of 1010-10.5M∼ galaxies increases continuously in the redshift range 1 < z < 4. Finally, we compare our results with a semi-analytical model and find that these models overestimate the density of low mass quiescent galaxies by an order of magnitude, while the density of low-mass star-forming galaxies is successfully reproduced. [ABSTRACT FROM AUTHOR]
Published: 2013
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