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185 results on '"Le Brun V."'

1. Euclid preparation: XXXVIII. Spectroscopy of active galactic nuclei with NISP.

Author

Euclid Collaboration, Lusso, E., Fotopoulou, S., Selwood, M., Allevato, V., Calderone, G., Mancini, C., Mignoli, M., Scodeggio, M., Bisigello, L., Feltre, A., Ricci, F., La Franca, F., Vergani, D., Gabarra, L., Le Brun, V., Maiorano, E., Palazzi, E., Moresco, M., and Zamorani, G.

Subjects
DISTRIBUTION (Probability theory), BLACK holes, ACTIVE galactic nuclei, REDSHIFT, SUPERMASSIVE black holes, ASTROPHYSICS, SPECTROMETRY, GALAXY clusters
Abstract

The statistical distribution and evolution of key properties of active galactic nuclei (AGN), such as their accretion rate, mass, and spin, remains a subject of open debate in astrophysics. The ESA Euclid space mission, launched on July 1 2023, promises a breakthrough in this field. We create detailed mock catalogues of AGN spectra from the rest-frame near-infrared down to the ultraviolet – including emission lines – to simulate what Euclid will observe for both obscured (type 2) and unobscured (type 1) AGN. We concentrate on the red grisms of the NISP instrument, which will be used for the wide-field survey, opening a new window for spectroscopic AGN studies in the near-infrared. We quantify the efficiency in the redshift determination as well as in retrieving the emission line flux of the Hα+[N II] complex, as Euclid is mainly focused on this emission line, given that it is expected to be the brightest one in the probed redshift range. Spectroscopic redshifts are measured for 83% of the simulated AGN in the interval where the Hα is visible (i.e. 0.89 <  z <  1.83 at a line flux of > 2 × 10−16 erg s−1 cm−2, encompassing the peak of AGN activity at z ≃ 1 − 1.5) within the spectral coverage of the red grism. Outside this redshift range, the measurement efficiency decreases significantly. Overall, a spectroscopic redshift iscorrectly determined for about 90% of type 2 AGN down to an emission line flux of roughly 3 × 10−16 erg s−1 cm−2, and for type 1 AGN down to 8.5 × 10−16 erg s−1 cm−2. Recovered values for black hole mass show a small offset with respect to the input values by about 10%, but the agreement is good overall. With such a high spectroscopic coverage at z <  2, we will be able to measure AGN demography, scaling relations, and clustering from the epoch of the peak of AGN activity down to the present-day Universe for hundreds of thousands of AGN with homogeneous spectroscopic information. [ABSTRACT FROM AUTHOR]

Published
2024
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2. Metal content of the circumgalactic medium around star-forming galaxies at z ∼ 2.6 as revealed by the VIMOS Ultra-Deep Survey

Author

Méndez-Hernández, H., primary, Cassata, P., additional, Ibar, E., additional, Amorín, R., additional, Aravena, M., additional, Bardelli, S., additional, Cucciati, O., additional, Garilli, B., additional, Giavalisco, M., additional, Guaita, L., additional, Hathi, N., additional, Koekemoer, A., additional, Le Brun, V., additional, Lemaux, B. C., additional, Maccagni, D., additional, Ribeiro, B., additional, Tasca, L., additional, Tejos, N., additional, Thomas, R., additional, Tresse, L., additional, Vergani, D., additional, Zamorani, G., additional, and Zucca, E., additional

Published
2022
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3. Less and more IGM-transmitted galaxies from z ∼ 2.7 to z ∼ 6 from VANDELS and VUDS

Author

Thomas, R., primary, Pentericci, L., additional, Le Fèvre, O., additional, Koekemoer, A. M., additional, Castellano, M., additional, Cimatti, A., additional, Fontanot, F., additional, Gargiulo, A., additional, Garilli, B., additional, Talia, M., additional, Amorín, R., additional, Bardelli, S., additional, Cristiani, S., additional, Cresci, G., additional, Franco, M., additional, Fynbo, J. P. U., additional, Hathi, N. P., additional, Hibon, P., additional, Khusanova, Y., additional, Le Brun, V., additional, Lemaux, B. C., additional, Mannucci, F., additional, Schaerer, D., additional, Zamorani, G., additional, and Zucca, E., additional

Published
2021
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4. UV and Lyα luminosity functions of galaxies and star formation rate density at the end of HI reionization from the VIMOS UltraDeep Survey (VUDS)

Author

Khusanova, Y., primary, Le Fèvre, O., additional, Cassata, P., additional, Cucciati, O., additional, Lemaux, B. C., additional, Tasca, L. A. M., additional, Thomas, R., additional, Garilli, B., additional, Le Brun, V., additional, Maccagni, D., additional, Pentericci, L., additional, Zamorani, G., additional, Amorín, R., additional, Bardelli, S., additional, Castellano, M., additional, Cassarà, L. P., additional, Cimatti, A., additional, Giavalisco, M., additional, Hathi, N. P., additional, Ilbert, O., additional, Koekemoer, A. M., additional, Marchi, F., additional, Pforr, J., additional, Ribeiro, B., additional, Schaerer, D., additional, Tresse, L., additional, Vergani, D., additional, and Zucca, E., additional

Published
2020
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5. The VIMOS Public Extragalactic Redshift Survey (VIPERS)

Author

Gargiulo, A., primary, Cucciati, O., additional, Garilli, B., additional, Scodeggio, M., additional, Bolzonella, M., additional, Zamorani, G., additional, De Lucia, G., additional, Krywult, J., additional, Guzzo, L., additional, Granett, B. R., additional, de la Torre, S., additional, Abbas, U., additional, Adami, C., additional, Arnouts, S., additional, Bottini, D., additional, Cappi, A., additional, Franzetti, P., additional, Fritz, A., additional, Haines, C., additional, Hawken, A. J., additional, Iovino, A., additional, Le Brun, V., additional, Le Fèvre, O., additional, Maccagni, D., additional, Małek, K., additional, Marulli, F., additional, Moutard, T., additional, Polletta, M., additional, Pollo, A., additional, Tasca, L. A. M., additional, Tojeiro, R., additional, Vergani, D., additional, Zanichelli, A., additional, Bel, J., additional, Branchini, E., additional, Coupon, J., additional, Ilbert, O., additional, Moscardini, L., additional, and Peacock, J. A., additional

Published
2019
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6. 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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7. 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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8. The VIMOS Public Extragalactic Redshift Survey (VIPERS)

Author

Vergani, D., primary, Garilli, B., additional, Polletta, M., additional, Franzetti, P., additional, Scodeggio, M., additional, Zamorani, G., additional, Haines, C. P., additional, Bolzonella, M., additional, Guzzo, L., additional, Granett, B. R., additional, de la Torre, S., additional, Abbas, U., additional, Adami, C., additional, Bottini, D., additional, Cappi, A., additional, Cucciati, O., additional, Davidzon, I., additional, De Lucia, G., additional, Fritz, A., additional, Gargiulo, A., additional, Hawken, A. J., additional, Iovino, A., additional, Krywult, J., additional, Le Brun, V., additional, Le Fèvre, O., additional, Maccagni, D., additional, Małek, K., additional, Marulli, F., additional, Pollo, A., additional, Tasca, L. A. M., additional, Tojeiro, R., additional, Zanichelli, A., additional, Arnouts, S., additional, Bel, J., additional, Branchini, E., additional, Coupon, J., additional, Ilbert, O., additional, Moutard, T., additional, and Moscardini, L., additional

Published
2018
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9. The progeny of a cosmic titan: a massive multi-component proto-supercluster in formation at z = 2.45 in VUDS

Author

Cucciati, O., primary, Lemaux, B. C., additional, Zamorani, G., additional, Le Fèvre, O., additional, Tasca, L. A. M., additional, Hathi, N. P., additional, Lee, K.-G., additional, Bardelli, S., additional, Cassata, P., additional, Garilli, B., additional, Le Brun, V., additional, Maccagni, D., additional, Pentericci, L., additional, Thomas, R., additional, Vanzella, E., additional, Zucca, E., additional, Lubin, L. M., additional, Amorin, R., additional, Cassarà, L. P., additional, Cimatti, A., additional, Talia, M., additional, Vergani, D., additional, Koekemoer, A., additional, Pforr, J., additional, and Salvato, M., additional

Published
2018
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10. The VIMOS Public Extragalactic Redshift Survey (VIPERS)

Author

Mohammad, F. G., primary, Bianchi, D., additional, Percival, W. J., additional, de la Torre, S., additional, Guzzo, L., additional, Granett, B. R., additional, Branchini, E., additional, Bolzonella, M., additional, Garilli, B., additional, Scodeggio, M., additional, Abbas, U., additional, Adami, C., additional, Bel, J., additional, Bottini, D., additional, Cappi, A., additional, Cucciati, O., additional, Davidzon, I., additional, Franzetti, P., additional, Fritz, A., additional, Iovino, A., additional, Krywult, J., additional, Le Brun, V., additional, Le Fèvre, O., additional, Małek, K., additional, Marulli, F., additional, Polletta, M., additional, Pollo, A., additional, Tasca, L. A. M., additional, Tojeiro, R., additional, Vergani, D., additional, Zanichelli, A., additional, Arnouts, S., additional, Coupon, J., additional, De Lucia, G., additional, Ilbert, O., additional, Moscardini, L., additional, and Moutard, T., additional

Published
2018
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11. The VIMOS Public Extragalactic Redshift Survey (VIPERS)

Author

Siudek, M., primary, Małek, K., additional, Pollo, A., additional, Krakowski, T., additional, Iovino, A., additional, Scodeggio, M., additional, Moutard, T., additional, Zamorani, G., additional, Guzzo, L., additional, Garilli, B., additional, Granett, B. R., additional, Bolzonella, M., additional, de la Torre, S., additional, Abbas, U., additional, Adami, C., additional, Bottini, D., additional, Cappi, A., additional, Cucciati, O., additional, Davidzon, I., additional, Franzetti, P., additional, Fritz, A., additional, Krywult, J., additional, Le Brun, V., additional, Le Fèvre, O., additional, Maccagni, D., additional, Marulli, F., additional, Polletta, M., additional, Tasca, L. A.M., additional, Tojeiro, R., additional, Vergani, D., additional, Zanichelli, A., additional, Arnouts, S., additional, Bel, J., additional, Branchini, E., additional, Coupon, J., additional, De Lucia, G., additional, Ilbert, O., additional, Haines, C. P., additional, Moscardini, L., additional, and Takeuchi, T. T., additional

Published
2018
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13. The VIMOS Public Extragalactic Redshift Survey (VIPERS)

Author

Scodeggio, M., primary, Guzzo, L., additional, Garilli, B., additional, Granett, B. R., additional, Bolzonella, M., additional, de la Torre, S., additional, Abbas, U., additional, Adami, C., additional, Arnouts, S., additional, Bottini, D., additional, Cappi, A., additional, Coupon, J., additional, Cucciati, O., additional, Davidzon, I., additional, Franzetti, P., additional, Fritz, A., additional, Iovino, A., additional, Krywult, J., additional, Le Brun, V., additional, Le Fèvre, O., additional, Maccagni, D., additional, Małek, K., additional, Marchetti, A., additional, Marulli, F., additional, Polletta, M., additional, Pollo, A., additional, Tasca, L. A. M., additional, Tojeiro, R., additional, Vergani, D., additional, Zanichelli, A., additional, Bel, J., additional, Branchini, E., additional, De Lucia, G., additional, Ilbert, O., additional, McCracken, H. J., additional, Moutard, T., additional, Peacock, J. A., additional, Zamorani, G., additional, Burden, A., additional, Fumana, M., additional, Jullo, E., additional, Marinoni, C., additional, Mellier, Y., additional, Moscardini, L., additional, and Percival, W. J., additional

Published
2018
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14. The VIMOS Public Extragalactic Redshift Survey (VIPERS)

Author

de la Torre, S., primary, Jullo, E., additional, Giocoli, C., additional, Pezzotta, A., additional, Bel, J., additional, Granett, B. R., additional, Guzzo, L., additional, Garilli, B., additional, Scodeggio, M., additional, Bolzonella, M., additional, Abbas, U., additional, Adami, C., additional, Bottini, D., additional, Cappi, A., additional, Cucciati, O., additional, Davidzon, I., additional, Franzetti, P., additional, Fritz, A., additional, Iovino, A., additional, Krywult, J., additional, Le Brun, V., additional, Le Fèvre, O., additional, Maccagni, D., additional, Małek, K., additional, Marulli, F., additional, Polletta, M., additional, Pollo, A., additional, Tasca, L. A. M., additional, Tojeiro, R., additional, Vergani, D., additional, Zanichelli, A., additional, Arnouts, S., additional, Branchini, E., additional, Coupon, J., additional, De Lucia, G., additional, Ilbert, O., additional, Moutard, T., additional, Moscardini, L., additional, Peacock, J. A., additional, Metcalf, R. B., additional, Prada, F., additional, and Yepes, G., additional

Published
2017
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15. The VIMOS Public Extragalactic Redshift Survey

Author

Hawken, A. J., primary, Granett, B. R., additional, Iovino, A., additional, Guzzo, L., additional, Peacock, J. A., additional, de la Torre, S., additional, Garilli, B., additional, Bolzonella, M., additional, Scodeggio, M., additional, Abbas, U., additional, Adami, C., additional, Bottini, D., additional, Cappi, A., additional, Cucciati, O., additional, Davidzon, I., additional, Fritz, A., additional, Franzetti, P., additional, Krywult, J., additional, Le Brun, V., additional, Le Fèvre, O., additional, Maccagni, D., additional, Małek, K., additional, Marulli, F., additional, Polletta, M., additional, Pollo, A., additional, Tasca, L. A. M., additional, Tojeiro, R., additional, Vergani, D., additional, Zanichelli, A., additional, Arnouts, S., additional, Bel, J., additional, Branchini, E., additional, De Lucia, G., additional, Ilbert, O., additional, Moscardini, L., additional, and Percival, W. J., additional

Published
2017
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16. The VIMOS Public Extragalactic Redshift Survey (VIPERS)

Author

Gargiulo, A., primary, Bolzonella, M., additional, Scodeggio, M., additional, Krywult, J., additional, De Lucia, G., additional, Guzzo, L., additional, Garilli, B., additional, Granett, B. R., additional, de la Torre, S., additional, Abbas, U., additional, Adami, C., additional, Arnouts, S., additional, Bottini, D., additional, Cappi, A., additional, Cucciati, O., additional, Davidzon, I., additional, Franzetti, P., additional, Fritz, A., additional, Haines, C., additional, Hawken, A. J., additional, Iovino, A., additional, Le Brun, V., additional, Le Fèvre, O., additional, Maccagni, D., additional, Małek, K., additional, Marulli, F., additional, Moutard, T., additional, Polletta, M., additional, Pollo, A., additional, Tasca, L. A. M., additional, Tojeiro, R., additional, Vergani, D., additional, Zanichelli, A., additional, Zamorani, G., additional, Bel, J., additional, Branchini, E., additional, Coupon, J., additional, Ilbert, O., additional, Moscardini, L., additional, and Peacock, J. A., additional

Published
2017
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17. The VIMOS Ultra Deep Survey

Author

Guaita, L., primary, Talia, M., additional, Pentericci, L., additional, Verhamme, A., additional, Cassata, P., additional, Lemaux, B. C., additional, Orlitova, I., additional, Ribeiro, B., additional, Schaerer, D., additional, Zamorani, G., additional, Garilli, B., additional, Le Brun, V., additional, Le Fèvre, O., additional, Maccagni, D., additional, Tasca, L. A. M., additional, Thomas, R., additional, Vanzella, E., additional, Zucca, E., additional, Amorin, R., additional, Bardelli, S., additional, Castellano, M., additional, Grazian, A., additional, Hathi, N. P., additional, Koekemoer, A., additional, and Marchi, F., additional

Published
2017
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18. The VIMOS Public Extragalactic Redshift Survey (VIPERS)

Author

Haines, C. P., primary, Iovino, A., additional, Krywult, J., additional, Guzzo, L., additional, Davidzon, I., additional, Bolzonella, M., additional, Garilli, B., additional, Scodeggio, M., additional, Granett, B. R., additional, de la Torre, S., additional, De Lucia, G., additional, Abbas, U., additional, Adami, C., additional, Arnouts, S., additional, Bottini, D., additional, Cappi, A., additional, Cucciati, O., additional, Franzetti, P., additional, Fritz, A., additional, Gargiulo, A., additional, Le Brun, V., additional, Le Fèvre, O., additional, Maccagni, D., additional, Małek, K., additional, Marulli, F., additional, Moutard, T., additional, Polletta, M., additional, Pollo, A., additional, Tasca, L. A. M., additional, Tojeiro, R., additional, Vergani, D., additional, Zanichelli, A., additional, Zamorani, G., additional, Bel, J., additional, Branchini, E., additional, Coupon, J., additional, Ilbert, O., additional, Moscardini, L., additional, Peacock, J. A., additional, and Siudek, M., additional

Published
2017
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19. The VIMOS Public Extragalactic Redshift Survey (VIPERS)

Author

Moresco, M., primary, Marulli, F., additional, Moscardini, L., additional, Branchini, E., additional, Cappi, A., additional, Davidzon, I., additional, Granett, B. R., additional, de la Torre, S., additional, Guzzo, L., additional, Abbas, U., additional, Adami, C., additional, Arnouts, S., additional, Bel, J., additional, Bolzonella, M., additional, Bottini, D., additional, Carbone, C., additional, Coupon, J., additional, Cucciati, O., additional, De Lucia, G., additional, Franzetti, P., additional, Fritz, A., additional, Fumana, M., additional, Garilli, B., additional, Ilbert, O., additional, Iovino, A., additional, Krywult, J., additional, Le Brun, V., additional, Le Fèvre, O., additional, Małek, K., additional, McCracken, H. J., additional, Polletta, M., additional, Pollo, A., additional, Scodeggio, M., additional, Tasca, L. A. M., additional, Tojeiro, R., additional, Vergani, D., additional, and Zanichelli, A., additional

Published
2017
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20. The VIMOS Public Extragalactic Redshift Survey (VIPERS)

Author

Pezzotta, A., primary, de la Torre, S., additional, Bel, J., additional, Granett, B. R., additional, Guzzo, L., additional, Peacock, J. A., additional, Garilli, B., additional, Scodeggio, M., additional, Bolzonella, M., additional, Abbas, U., additional, Adami, C., additional, Bottini, D., additional, Cappi, A., additional, Cucciati, O., additional, Davidzon, I., additional, Franzetti, P., additional, Fritz, A., additional, Iovino, A., additional, Krywult, J., additional, Le Brun, V., additional, Le Fèvre, O., additional, Maccagni, D., additional, Małek, K., additional, Marulli, F., additional, Polletta, M., additional, Pollo, A., additional, Tasca, L. A. M., additional, Tojeiro, R., additional, Vergani, D., additional, Zanichelli, A., additional, Arnouts, S., additional, Branchini, E., additional, Coupon, J., additional, De Lucia, G., additional, Koda, J., additional, Ilbert, O., additional, Mohammad, F., additional, Moutard, T., additional, and Moscardini, L., additional

Published
2017
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21. The extended epoch of galaxy formation: Age dating of ~3600 galaxies with 2 < z< 6.5 in the VIMOS Ultra-Deep Survey

Author

Thomas, R., primary, Le Fèvre, O., additional, Scodeggio, M., additional, Cassata, P., additional, Garilli, B., additional, Le Brun, V., additional, Lemaux, B. C., additional, Maccagni, D., additional, Pforr, J., additional, Tasca, L. A. M., additional, Zamorani, G., additional, Bardelli, S., additional, Hathi, N. P., additional, Tresse, L., additional, Zucca, E., additional, and Koekemoer, A. M., additional

Published
2017
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22. The VIMOS Public Extragalactic Redshift Survey (VIPERS)

Author

Cucciati, O., primary, Davidzon, I., additional, Bolzonella, M., additional, Granett, B. R., additional, De Lucia, G., additional, Branchini, E., additional, Zamorani, G., additional, Iovino, A., additional, Garilli, B., additional, Guzzo, L., additional, Scodeggio, M., additional, de la Torre, S., additional, Abbas, U., additional, Adami, C., additional, Arnouts, S., additional, Bottini, D., additional, Cappi, A., additional, Franzetti, P., additional, Fritz, A., additional, Krywult, J., additional, Le Brun, V., additional, Le Fèvre, O., additional, Maccagni, D., additional, Małek, K., additional, Marulli, F., additional, Moutard, T., additional, Polletta, M., additional, Pollo, A., additional, Tasca, L. A. M., additional, Tojeiro, R., additional, Vergani, D., additional, Zanichelli, A., additional, Bel, J., additional, Blaizot, J., additional, Coupon, J., additional, Hawken, A., additional, Ilbert, O., additional, Moscardini, L., additional, Peacock, J. A., additional, and Gargiulo, A., additional

Published
2017
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23. New constraints on the average escape fraction of Lyman continuum radiation in z ~ 4 galaxies from the VIMOS Ultra Deep Survey (VUDS)

Author

Marchi, F., primary, Pentericci, L., additional, Guaita, L., additional, Ribeiro, B., additional, Castellano, M., additional, Schaerer, D., additional, Hathi, N. P., additional, Lemaux, B. C., additional, Grazian, A., additional, Le Fèvre, O., additional, Garilli, B., additional, Maccagni, D., additional, Amorin, R., additional, Bardelli, S., additional, Cassata, P., additional, Fontana, A., additional, Koekemoer, A. M., additional, Le Brun, V., additional, Tasca, L. A. M., additional, Thomas, R., additional, Vanzella, E., additional, Zamorani, G., additional, and Zucca, E., additional

Published
2017
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24. The VIMOS Public Extragalactic Redshift Survey (VIPERS)

Author

Rota, S., primary, Granett, B. R., additional, Bel, J., additional, Guzzo, L., additional, Peacock, J. A., additional, Wilson, M. J., additional, Pezzotta, A., additional, de la Torre, S., additional, Garilli, B., additional, Bolzonella, M., additional, Scodeggio, M., additional, Abbas, U., additional, Adami, C., additional, Bottini, D., additional, Cappi, A., additional, Cucciati, O., additional, Davidzon, I., additional, Franzetti, P., additional, Fritz, A., additional, Iovino, A., additional, Krywult, J., additional, Le Brun, V., additional, Le Fèvre, O., additional, Maccagni, D., additional, Małek, K., additional, Marulli, F., additional, Percival, W. J., additional, Polletta, M., additional, Pollo, A., additional, Tasca, L. A. M., additional, Tojeiro, R., additional, Vergani, D., additional, Zanichelli, A., additional, Arnouts, S., additional, Branchini, E., additional, Coupon, J., additional, De Lucia, G., additional, Ilbert, O., additional, Moscardini, L., additional, and Moutard, T., additional

Published
2017
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25. The VIMOS Ultra Deep Survey first data release: Spectra and spectroscopic redshifts of 698 objects up to zspec ~ 6 in CANDELS

Author

Tasca, L. A. M., primary, Le Fèvre, O., additional, Ribeiro, B., additional, Thomas, R., additional, Moreau, C., additional, Cassata, P., additional, Garilli, B., additional, Le Brun, V., additional, Lemaux, B. C., additional, Maccagni, D., additional, Pentericci, L., additional, Schaerer, D., additional, Vanzella, E., additional, Zamorani, G., additional, Zucca, E., additional, Amorin, R., additional, Bardelli, S., additional, Cassarà, L. P., additional, Castellano, M., additional, Cimatti, A., additional, Cucciati, O., additional, Durkalec, A., additional, Fontana, A., additional, Giavalisco, M., additional, Grazian, A., additional, Hathi, N. P., additional, Ilbert, O., additional, Paltani, S., additional, Pforr, J., additional, Scodeggio, M., additional, Sommariva, V., additional, Talia, M., additional, Tresse, L., additional, Vergani, D., additional, Capak, P., additional, Charlot, S., additional, Contini, T., additional, de la Torre, S., additional, Dunlop, J., additional, Fotopoulou, S., additional, Guaita, L., additional, Koekemoer, A., additional, López-Sanjuan, C., additional, Mellier, Y., additional, Salvato, M., additional, Scoville, N., additional, Taniguchi, Y., additional, and Wang, P. W., additional

Published
2017
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26. The VIMOS Public Extragalactic Redshift Survey (VIPERS)

Author

Marchetti, A., primary, Garilli, B., additional, Granett, B. R., additional, Guzzo, L., additional, Iovino, A., additional, Scodeggio, M., additional, Bolzonella, M., additional, de la Torre, S., additional, Abbas, U., additional, Adami, C., additional, Bottini, D., additional, Cappi, A., additional, Cucciati, O., additional, Davidzon, I., additional, Franzetti, P., additional, Fritz, A., additional, Krywult, J., additional, Le Brun, V., additional, Le Fèvre, O., additional, Maccagni, D., additional, Małek, K., additional, Marulli, F., additional, Polletta, M., additional, Pollo, A., additional, Tasca, L. A. M., additional, Tojeiro, R., additional, Vergani, D., additional, Zanichelli, A., additional, Arnouts, S., additional, Bel, J., additional, Branchini, E., additional, Coupon, J., additional, De Lucia, G., additional, Ilbert, O., additional, Moutard, T., additional, Moscardini, L., additional, and Zamorani, G., additional

Published
2017
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27. The VIMOS Public Extragalactic Redshift Survey (VIPERS)

Author

Krywult, J., primary, Tasca, L. A. M., additional, Pollo, A., additional, Vergani, D., additional, Bolzonella, M., additional, Davidzon, I., additional, Iovino, A., additional, Gargiulo, A., additional, Haines, C. P., additional, Scodeggio, M., additional, Guzzo, L., additional, Zamorani, G., additional, Garilli, B., additional, Granett, B. R., additional, de la Torre, S., additional, Abbas, U., additional, Adami, C., additional, Bottini, D., additional, Cappi, A., additional, Cucciati, O., additional, Franzetti, P., additional, Fritz, A., additional, Le Brun, V., additional, Le Fèvre, O., additional, Maccagni, D., additional, Małek, K., additional, Marulli, F., additional, Polletta, M., additional, Tojeiro, R., additional, Zanichelli, A., additional, Arnouts, S., additional, Bel, J., additional, Branchini, E., additional, Coupon, J., additional, De Lucia, G., additional, Ilbert, O., additional, McCracken, H. J., additional, Moscardini, L., additional, and Takeuchi, T. T., additional

Published
2017
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28. 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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29. Tracking the impact of environment on the galaxy stellar mass function up to z ∼ 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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30. The evolving star formation rate: MBlack star relation and sSFR since z ≃ 5 from the VUDS spectroscopic survey

Author

Tasca, L. A. M., Le Fèvre, O., Hathi, N. P., Schaerer, D., Ilbert, O., Zamorani, G., Lemaux, B. C., Cassata, P., Garilli, B., Le Brun, V., Maccagni, D., Pentericci, L., Thomas, R., Vanzella, E., Zucca, E., Amorin, R., Bardelli, S., Cassarà, L. P., Castellano, M., Cimatti, A., Cucciati, O., Durkalec, A., Fontana, A., Giavalisco, M., Grazian, A., Paltani, S., Ribeiro, B., Scodeggio, M., Sommariva, V., Talia, M., Tresse, L., Vergani, D., Capak, P., Charlot, S., Contini, T., De La Torre, S., Dunlop, J., Fotopoulou, S., Koekemoer, A., López-Sanjuan, C., Mellier, Y., Pforr, J., Salvato, M., Scoville, N., Taniguchi, Y., and Wang, P. W.

Subjects
galaxies: high-redshift, Space and Planetary Science, galaxies: star formation, galaxies: formation, Astronomy and Astrophysics, galaxies: evolution
Published
2015

31. The VIMOS Public Extragalactic Redshift Survey (VIPERS)

Author

Siudek, M., primary, Małek, K., additional, Scodeggio, M., additional, Garilli, B., additional, Pollo, A., additional, Haines, C. P., additional, Fritz, A., additional, Bolzonella, M., additional, de la Torre, S., additional, Granett, B. R., additional, Guzzo, L., additional, Abbas, U., additional, Adami, C., additional, Bottini, D., additional, Cappi, A., additional, Cucciati, O., additional, De Lucia, G., additional, Davidzon, I., additional, Franzetti, P., additional, Iovino, A., additional, Krywult, J., additional, Le Brun, V., additional, Le Fèvre, O., additional, Maccagni, D., additional, Marchetti, A., additional, Marulli, F., additional, Polletta, M., additional, Tasca, L. A. M., additional, Tojeiro, R., additional, Vergani, D., additional, Zanichelli, A., additional, Arnouts, S., additional, Bel, J., additional, Branchini, E., additional, Ilbert, O., additional, Gargiulo, A., additional, Moscardini, L., additional, Takeuchi, T. T., additional, and Zamorani, G., additional

Published
2017
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32. VIMOS Ultra-Deep Survey (VUDS): IGM transmission towards galaxies with 2.5 < z < 5.5 and the colour selection of high-redshift galaxies

Author

Thomas, R., primary, Le Fèvre, O., additional, Le Brun, V., additional, Cassata, P., additional, Garilli, B., additional, Lemaux, B. C., additional, Maccagni, D., additional, Pentericci, L., additional, Tasca, L. A. M., additional, Zamorani, G., additional, Zucca, E., additional, Amorin, R., additional, Bardelli, S., additional, Cassarà, L., additional, Castellano, M., additional, Cimatti, A., additional, Cucciati, O., additional, Durkalec, A., additional, Fontana, A., additional, Giavalisco, M., additional, Grazian, A., additional, Hathi, N. P., additional, Ilbert, O., additional, Paltani, S., additional, Pforr, J., additional, Ribeiro, B., additional, Schaerer, D., additional, Scodeggio, M., additional, Sommariva, V., additional, Talia, M., additional, Tresse, L., additional, Vanzella, E., additional, Vergani, D., additional, Capak, P., additional, Charlot, S., additional, Contini, T., additional, Cuby, J. G., additional, de la Torre, S., additional, Dunlop, J., additional, Fotopoulou, S., additional, Koekemoer, A., additional, López-Sanjuan, C., additional, Mellier, Y., additional, Salvato, M., additional, Scoville, N., additional, Taniguchi, Y., additional, and Wang, P. W., additional

Published
2017
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33. The VIMOS Public Extragalactic Redshift Survey (VIPERS)

Author

Di Porto, C., primary, Branchini, E., additional, Bel, J., additional, Marulli, F., additional, Bolzonella, M., additional, Cucciati, O., additional, de la Torre, S., additional, Granett, B. R., additional, Guzzo, L., additional, Marinoni, C., additional, Moscardini, L., additional, Abbas, U., additional, Adami, C., additional, Arnouts, S., additional, Bottini, D., additional, Cappi, A., additional, Coupon, J., additional, Davidzon, I., additional, De Lucia, G., additional, Fritz, A., additional, Franzetti, P., additional, Fumana, M., additional, Garilli, B., additional, Ilbert, O., additional, Iovino, A., additional, Krywult, J., additional, Le Brun, V., additional, Le Fèvre, O., additional, Maccagni, D., additional, Małek, K., additional, McCracken, H. J., additional, Paioro, L., additional, Polletta, M., additional, Pollo, A., additional, Scodeggio, M., additional, Tasca, L. A. M., additional, Tojeiro, R., additional, Vergani, D., additional, Zanichelli, A., additional, Burden, A., additional, Marchetti, A., additional, Martizzi, D., additional, Mellier, Y., additional, Nichol, R. C., additional, Peacock, J. A., additional, Percival, W. J., additional, Viel, M., additional, Wolk, M., additional, and Zamorani, G., additional

Published
2016
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34. Effect of the star formation histories on theSFR-M∗relation atz≥ 2

Author

Cassarà, L. P., primary, Maccagni, D., additional, Garilli, B., additional, Scodeggio, M., additional, Thomas, R., additional, Le Fèvre, O., additional, Zamorani, G., additional, Schaerer, D., additional, Lemaux, B. C., additional, Cassata, P., additional, Le Brun, V., additional, Pentericci, L., additional, Tasca, L. A. M., additional, Vanzella, E., additional, Zucca, E., additional, Amorín, R., additional, Bardelli, S., additional, Castellano, M., additional, Cimatti, A., additional, Cucciati, O., additional, Durkalec, A., additional, Fontana, A., additional, Giavalisco, M., additional, Grazian, A., additional, Hathi, N. P., additional, Ilbert, O., additional, Paltani, S., additional, Ribeiro, B., additional, Sommariva, V., additional, Talia, M., additional, Tresse, L., additional, Vergani, D., additional, Capak, P., additional, Charlot, S., additional, Contini, T., additional, de la Torre, S., additional, Dunlop, J., additional, Fotopoulou, S., additional, Guaita, L., additional, Koekemoer, A., additional, López-Sanjuan, C., additional, Mellier, Y., additional, Pforr, J., additional, Salvato, M., additional, Scoville, N., additional, Taniguchi, Y., additional, and Wang, P. W., additional

Published
2016
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35. The XXL Survey

Author

Pacaud, F., primary, Clerc, N., additional, Giles, P. A., additional, Adami, C., additional, Sadibekova, T., additional, Pierre, M., additional, Maughan, B. J., additional, Lieu, M., additional, Le Fèvre, J. P., additional, Alis, S., additional, Altieri, B., additional, Ardila, F., additional, Baldry, I., additional, Benoist, C., additional, Birkinshaw, M., additional, Chiappetti, L., additional, Démoclès, J., additional, Eckert, D., additional, Evrard, A. E., additional, Faccioli, L., additional, Gastaldello, F., additional, Guennou, L., additional, Horellou, C., additional, Iovino, A., additional, Koulouridis, E., additional, Le Brun, V., additional, Lidman, C., additional, Liske, J., additional, Maurogordato, S., additional, Menanteau, F., additional, Owers, M., additional, Poggianti, B., additional, Pomarède, D., additional, Pompei, E., additional, Ponman, T. J., additional, Rapetti, D., additional, Reiprich, T. H., additional, Smith, G. P., additional, Tuffs, R., additional, Valageas, P., additional, Valtchanov, I., additional, Willis, J. P., additional, and Ziparo, F., additional

Published
2016
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36. The VIMOS Public Extragalactic Redshift Survey (VIPERS)

Author

Bel, J., primary, Branchini, E., additional, Di Porto, C., additional, Cucciati, O., additional, Granett, B. R., additional, Iovino, A., additional, de la Torre, S., additional, Marinoni, C., additional, Guzzo, L., additional, Moscardini, L., additional, Cappi, A., additional, Abbas, U., additional, Adami, C., additional, Arnouts, S., additional, Bolzonella, M., additional, Bottini, D., additional, Coupon, J., additional, Davidzon, I., additional, De Lucia, G., additional, Fritz, A., additional, Franzetti, P., additional, Fumana, M., additional, Garilli, B., additional, Ilbert, O., additional, Krywult, J., additional, Le Brun, V., additional, Le Fèvre, O., additional, Maccagni, D., additional, Małek, K., additional, Marulli, F., additional, McCracken, H. J., additional, Paioro, L., additional, Polletta, M., additional, Pollo, A., additional, Schlagenhaufer, H., additional, Scodeggio, M., additional, Tasca, L. A. M., additional, Tojeiro, R., additional, Vergani, D., additional, Zanichelli, A., additional, Burden, A., additional, Marchetti, A., additional, Mellier, Y., additional, Nichol, R. C., additional, Peacock, J. A., additional, Percival, W. J., additional, Phleps, S., additional, and Wolk, M., additional

Published
2016
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37. The VIMOS Ultra Deep Survey: Lyαemission and stellar populations of star-forming galaxies at 2 < z < 2.5

Author

Hathi, N. P., primary, Le Fèvre, O., additional, Ilbert, O., additional, Cassata, P., additional, Tasca, L. A. M., additional, Lemaux, B. C., additional, Garilli, B., additional, Le Brun, V., additional, Maccagni, D., additional, Pentericci, L., additional, Thomas, R., additional, Vanzella, E., additional, Zamorani, G., additional, Zucca, E., additional, Amorín, R., additional, Bardelli, S., additional, Cassarà, L. P., additional, Castellano, M., additional, Cimatti, A., additional, Cucciati, O., additional, Durkalec, A., additional, Fontana, A., additional, Giavalisco, M., additional, Grazian, A., additional, Guaita, L., additional, Koekemoer, A., additional, Paltani, S., additional, Pforr, J., additional, Ribeiro, B., additional, Schaerer, D., additional, Scodeggio, M., additional, Sommariva, V., additional, Talia, M., additional, Tresse, L., additional, Vergani, D., additional, Capak, P., additional, Charlot, S., additional, Contini, T., additional, Cuby, J. G., additional, de la Torre, S., additional, Dunlop, J., additional, Fotopoulou, S., additional, López-Sanjuan, C., additional, Mellier, Y., additional, Salvato, M., additional, Scoville, N., additional, Taniguchi, Y., additional, and Wang, P. W., additional

Published
2016
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38. Limits on the LyC signal fromz~ 3 sources with secure redshift and HST coverage in the E-CDFS field

Author

Guaita, L., primary, Pentericci, L., additional, Grazian, A., additional, Vanzella, E., additional, Nonino, M., additional, Giavalisco, M., additional, Zamorani, G., additional, Bongiorno, A., additional, Cassata, P., additional, Castellano, M., additional, Garilli, B., additional, Gawiser, E., additional, Le Brun, V., additional, Le Fèvre, O., additional, Lemaux, B. C., additional, Maccagni, D., additional, Merlin, E., additional, Santini, P., additional, Tasca, L. A. M., additional, Thomas, R., additional, Zucca, E., additional, De Barros, S., additional, Hathi, N. P., additional, Amorin, R., additional, Bardelli, S., additional, and Fontana, A., additional

Published
2016
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39. The VIMOS Public Extragalactic Redshift Survey (VIPERS)

Author

Davidzon, I., primary, Cucciati, O., additional, Bolzonella, M., additional, De Lucia, G., additional, Zamorani, G., additional, Arnouts, S., additional, Moutard, T., additional, Ilbert, O., additional, Garilli, B., additional, Scodeggio, M., additional, Guzzo, L., additional, Abbas, U., additional, Adami, C., additional, Bel, J., additional, Bottini, D., additional, Branchini, E., additional, Cappi, A., additional, Coupon, J., additional, de la Torre, S., additional, Di Porto, C., additional, Fritz, A., additional, Franzetti, P., additional, Fumana, M., additional, Granett, B. R., additional, Guennou, L., additional, Iovino, A., additional, Krywult, J., additional, Le Brun, V., additional, Le Fèvre, O., additional, Maccagni, D., additional, Małek, K., additional, Marulli, F., additional, McCracken, H. J., additional, Mellier, Y., additional, Moscardini, L., additional, Polletta, M., additional, Pollo, A., additional, Tasca, L. A. M., additional, Tojeiro, R., additional, Vergani, D., additional, and Zanichelli, A., additional

Published
2016
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40. The Lyman continuum escape fraction of galaxies atz= 3.3 in the VUDS-LBC/COSMOS field

Author

Grazian, A., primary, Giallongo, E., additional, Gerbasi, R., additional, Fiore, F., additional, Fontana, A., additional, Le Fèvre, O., additional, Pentericci, L., additional, Vanzella, E., additional, Zamorani, G., additional, Cassata, P., additional, Garilli, B., additional, Le Brun, V., additional, Maccagni, D., additional, Tasca, L. A. M., additional, Thomas, R., additional, Zucca, E., additional, Amorín, R., additional, Bardelli, S., additional, Cassarà, L. P., additional, Castellano, M., additional, Cimatti, A., additional, Cucciati, O., additional, Durkalec, A., additional, Giavalisco, M., additional, Hathi, N. P., additional, Ilbert, O., additional, Lemaux, B. C., additional, Paltani, S., additional, Ribeiro, B., additional, Schaerer, D., additional, Scodeggio, M., additional, Sommariva, V., additional, Talia, M., additional, Tresse, L., additional, Vergani, D., additional, Bonchi, A., additional, Boutsia, K., additional, Capak, P., additional, Charlot, S., additional, Contini, T., additional, de la Torre, S., additional, Dunlop, J., additional, Fotopoulou, S., additional, Guaita, L., additional, Koekemoer, A., additional, López-Sanjuan, C., additional, Mellier, Y., additional, Merlin, E., additional, Paris, D., additional, Pforr, J., additional, Pilo, S., additional, Santini, P., additional, Scoville, N., additional, Taniguchi, Y., additional, and Wang, P. W., additional

Published
2015
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41. Evolution of clustering length, large-scale bias, and host halo mass at 2 < 5 in the VIMOS Ultra Deep Survey (VUDS)

Author

Durkalec, A., primary, Le Fèvre, O., additional, Pollo, A., additional, de la Torre, S., additional, Cassata, P., additional, Garilli, B., additional, Le Brun, V., additional, Lemaux, B. C., additional, Maccagni, D., additional, Pentericci, L., additional, Tasca, L. A. M., additional, Thomas, R., additional, Vanzella, E., additional, Zamorani, G., additional, Zucca, E., additional, Amorín, R., additional, Bardelli, S., additional, Cassarà, L. P., additional, Castellano, M., additional, Cimatti, A., additional, Cucciati, O., additional, Fontana, A., additional, Giavalisco, M., additional, Grazian, A., additional, Hathi, N. P., additional, Ilbert, O., additional, Paltani, S., additional, Ribeiro, B., additional, Schaerer, D., additional, Scodeggio, M., additional, Sommariva, V., additional, Talia, M., additional, Tresse, L., additional, Vergani, D., additional, Capak, P., additional, Charlot, S., additional, Contini, T., additional, Cuby, J. G., additional, Dunlop, J., additional, Fotopoulou, S., additional, Koekemoer, A., additional, López-Sanjuan, C., additional, Mellier, Y., additional, Pforr, J., additional, Salvato, M., additional, Scoville, N., additional, Taniguchi, Y., additional, and Wang, P. W., additional

Published
2015
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42. The VIMOS Public Extragalactic Redshift Survey

Author

Granett, B. R., primary, Branchini, E., additional, Guzzo, L., additional, Abbas, U., additional, Adami, C., additional, Arnouts, S., additional, Bel, J., additional, Bolzonella, M., additional, Bottini, D., additional, Cappi, A., additional, Coupon, J., additional, Cucciati, O., additional, Davidzon, I., additional, De Lucia, G., additional, de la Torre, S., additional, Fritz, A., additional, Franzetti, P., additional, Fumana, M., additional, Garilli, B., additional, Ilbert, O., additional, Iovino, A., additional, Krywult, J., additional, Le Brun, V., additional, Le Fèvre, O., additional, Maccagni, D., additional, Małek, K., additional, Marulli, F., additional, McCracken, H. J., additional, Polletta, M., additional, Pollo, A., additional, Scodeggio, M., additional, Tasca, L. A. M., additional, Tojeiro, R., additional, Vergani, D., additional, Zanichelli, A., additional, Burden, A., additional, Di Porto, C., additional, Marchetti, A., additional, Marinoni, C., additional, Mellier, Y., additional, Moutard, T., additional, Moscardini, L., additional, Nichol, R. C., additional, Peacock, J. A., additional, Percival, W. J., additional, and Zamorani, G., additional

Published
2015
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43. The evolving star formation rate:M⋆relation and sSFR sincez≃ 5 from the VUDS spectroscopic survey

Author

Tasca, L. A. M., primary, Le Fèvre, O., additional, Hathi, N. P., additional, Schaerer, D., additional, Ilbert, O., additional, Zamorani, G., additional, Lemaux, B. C., additional, Cassata, P., additional, Garilli, B., additional, Le Brun, V., additional, Maccagni, D., additional, Pentericci, L., additional, Thomas, R., additional, Vanzella, E., additional, Zucca, E., additional, Amorin, R., additional, Bardelli, S., additional, Cassarà, L. P., additional, Castellano, M., additional, Cimatti, A., additional, Cucciati, O., additional, Durkalec, A., additional, Fontana, A., additional, Giavalisco, M., additional, Grazian, A., additional, Paltani, S., additional, Ribeiro, B., additional, Scodeggio, M., additional, Sommariva, V., additional, Talia, M., additional, Tresse, L., additional, Vergani, D., additional, Capak, P., additional, Charlot, S., additional, Contini, T., additional, de la Torre, S., additional, Dunlop, J., additional, Fotopoulou, S., additional, Koekemoer, A., additional, López-Sanjuan, C., additional, Mellier, Y., additional, Pforr, J., additional, Salvato, M., additional, Scoville, N., additional, Taniguchi, Y., additional, and Wang, P. W., additional

Published
2015
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44. The VIMOS Public Extragalactic Redshift Survey (VIPERS)

Author

Cappi, A., primary, Marulli, F., additional, Bel, J., additional, Cucciati, O., additional, Branchini, E., additional, de la Torre, S., additional, Moscardini, L., additional, Bolzonella, M., additional, Guzzo, L., additional, Abbas, U., additional, Adami, C., additional, Arnouts, S., additional, Bottini, D., additional, Coupon, J., additional, Davidzon, I., additional, De Lucia, G., additional, Fritz, A., additional, Franzetti, P., additional, Fumana, M., additional, Garilli, B., additional, Granett, B. R., additional, Ilbert, O., additional, Iovino, A., additional, Krywult, J., additional, Le Brun, V., additional, Le Fèvre, O., additional, Maccagni, D., additional, Małek, K., additional, McCracken, H. J., additional, Paioro, L., additional, Polletta, M., additional, Pollo, A., additional, Scodeggio, M., additional, Tasca, L. A. M., additional, Tojeiro, R., additional, Vergani, D., additional, Zanichelli, A., additional, Burden, A., additional, Di Porto, C., additional, Marchetti, A., additional, Marinoni, C., additional, Mellier, Y., additional, Nichol, R. C., additional, Peacock, J. A., additional, Percival, W. J., additional, Phleps, S., additional, Schimd, C., additional, Schlagenhaufer, H., additional, Wolk, M., additional, and Zamorani, G., additional

Published
2015
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45. 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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46. The VIMOS Ultra-Deep Survey: ~10 000 galaxies with spectroscopic redshifts to study galaxy assembly at early epochs 2

Author

Le Fèvre, O., primary, Tasca, L. A. M., additional, Cassata, P., additional, Garilli, B., additional, Le Brun, V., additional, Maccagni, D., additional, Pentericci, L., additional, Thomas, R., additional, Vanzella, E., additional, Zamorani, G., additional, Zucca, E., additional, Amorin, R., additional, Bardelli, S., additional, Capak, P., additional, Cassarà, L., additional, Castellano, M., additional, Cimatti, A., additional, Cuby, J. G., additional, Cucciati, O., additional, de la Torre, S., additional, Durkalec, A., additional, Fontana, A., additional, Giavalisco, M., additional, Grazian, A., additional, Hathi, N. P., additional, Ilbert, O., additional, Lemaux, B. C., additional, Moreau, C., additional, Paltani, S., additional, Ribeiro, B., additional, Salvato, M., additional, Schaerer, D., additional, Scodeggio, M., additional, Sommariva, V., additional, Talia, M., additional, Taniguchi, Y., additional, Tresse, L., additional, Vergani, D., additional, Wang, P. W., additional, Charlot, S., additional, Contini, T., additional, Fotopoulou, S., additional, López-Sanjuan, C., additional, Mellier, Y., additional, and Scoville, N., additional

Published
2015
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47. Stellar mass to halo mass relation from galaxy clustering in VUDS: a high star formation efficiency atz≃ 3

Author

Durkalec, A., primary, Le Fèvre, O., additional, de la Torre, S., additional, Pollo, A., additional, Cassata, P., additional, Garilli, B., additional, Le Brun, V., additional, Lemaux, B. C., additional, Maccagni, D., additional, Pentericci, L., additional, Tasca, L. A. M., additional, Thomas, R., additional, Vanzella, E., additional, Zamorani, G., additional, Zucca, E., additional, Amorín, R., additional, Bardelli, S., additional, Cassarà, L. P., additional, Castellano, M., additional, Cimatti, A., additional, Cucciati, O., additional, Fontana, A., additional, Giavalisco, M., additional, Grazian, A., additional, Hathi, N. P., additional, Ilbert, O., additional, Paltani, S., additional, Ribeiro, B., additional, Schaerer, D., additional, Scodeggio, M., additional, Sommariva, V., additional, Talia, M., additional, Tresse, L., additional, Vergani, D., additional, Capak, P., additional, Charlot, S., additional, Contini, T., additional, Cuby, J. G., additional, Dunlop, J., additional, Fotopoulou, S., additional, Koekemoer, A., additional, López-Sanjuan, C., additional, Mellier, Y., additional, Pforr, J., additional, Salvato, M., additional, Scoville, N., additional, Taniguchi, Y., additional, and Wang, P. W., additional

Published
2015
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49. 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

50. The extended epoch of galaxy formation: Age dating of ~3600 galaxies with 2 < z < 6.5 in the VIMOS Ultra-Deep Survey.

Author

Thomas, R., Le Fèvre, O., Scodeggio, M., Cassata, P., Garilli, B., Le Brun, V., Lemaux, B. C., Maccagni, D., Pforr, J., Tasca, L. A. M., Zamorani, G., Bardelli, S., Hathi, N. P., Tresse, L., Zucca, E., and Koekemoer, A. M.

Subjects
GALAXY formation, AGE of stars, GALAXIES, STELLAR mass, STAR formation, STELLAR populations
Abstract

In this paper we aim at improving constraints on the epoch of galaxy formation by measuring the ages of 3597 galaxies with reliable spectroscopic redshifts 2 ≤ z ≤ 6:5 in the VIMOS Ultra Deep Survey (VUDS). We derive ages and other physical parameters from the simultaneous fitting with the GOSSIP+ software of observed UV rest-frame spectra and photometric data from the u band up to 4.5 μm using model spectra from composite stellar populations. We perform extensive simulations and conclude that at z ≥ 2 the joint analysis of spectroscopy and photometry, combined with restricted age possibilities when taking the age of the Universe into account, substantially reduces systematic uncertainties and degeneracies in the age derivation; we find that age measurements from this process are reliable. We find that galaxy ages range from very young with a few tens of million years to substantially evolved with ages up to 1.5 Gyr or more. This large age spread is similar for different age definitions including ages corresponding to the last major star formation event, stellar mass-weighted ages, and ages corresponding to the time since the formation of 25% of the stellar mass. We derive the formation redshift zf from the measured ages and find galaxies that may have started forming stars as early as zf ~ 15. We produce the formation redshift function (FzF), the number of galaxies per unit volume formed at a redshift zf, and compare the FzF in increasing observed redshift bins finding a remarkably constant FzF. The FzF is parametrized with (1 + z)ζ, where ζ ≃ 0:58 ± 0:06, indicating a smooth increase of about 2 dex from the earliest redshifts, z ~ 15; to the lowest redshifts of our sample at z ~ 2. Remarkably, this observed increase in the number of forming galaxies is of the same order as the observed rise in the star formation rate density (SFRD). The ratio of the comoving SFRD with the FzF gives an average SFR per galaxy of ~7-17 M⊙=yr at z ~ 4-6, in agreement with the measured SFR for galaxies at these redshifts. From the smooth rise in the FzF we infer that the period of galaxy formation extends all the way from the highest possible formation redshifts that we can probe at z ~ 15 down to redshifts z ~ 2. This indicates that galaxy formation is a continuous process over cosmic time, with a higher number of galaxies forming at the peak in SFRD at z ~ 2 than at earlier epochs. [ABSTRACT FROM AUTHOR]

Published
2017
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