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The evolving SFR-M_star relation and sSFR since z~5 from the VUDS spectroscopic survey

L. Tasca, O. Fevre, N. Hathi, D. Schaerer, O. Ilbert, G. Zamorani, B. Lemaux, P. Cassata, B. Garilli, V. Brun, D. Maccagni, L. Pentericci, R. Thomas, E. Vanzella, E. Zucca, R. Amorin, S. Bardelli, L. Cassara, M. Castellano, A. Cimatti, O. Cucciati, A. Durkalec, A. Fontana, M. Giavalisco, A. Grazian, S. Paltani, B. Ribeiro, M. Scodeggio, V. Sommariva, M. Talia, L. Tresse, D. Vergani, P. Capak, S. Charlot, T. Contini, J. Cuby, S. de la Torre, J. Dunlop, S. Fotopoulou, A. Koekemoer, C. Lopez-Sanjuan, Y. Mellier, J. Pforr, M. Salvato, N. Scoville, Y. Taniguchi, и P. Wang. (2014)cite arxiv:1411.5687Comment: 10 pages, 4 figures, submitted to A&A.

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COSMOS2020: A panchromatic view of the Universe to $z\sim10$ from two complementary catalogsJ. Weaver, O. Kauffmann, O. Ilbert, H. McCracken, A. Moneti, S. Toft, G. Brammer, M. Shuntov, I. Davidzon, B. Hsieh и 47 other автор(ы). (2021)cite arxiv:2110.13923Comment: 39 pages, 21 figures, accepted for publication in The Astrophysical Journal Supplement Series. Production of IRAC mosaics are presented in Moneti et al. "Euclid Preparation: XVIII. Cosmic Dawn Survey. Spitzer observations of the Euclid deep fields and calibration fields" which has been posted simultaneously. Catalogs can be accessed online now at https://cosmos2020.calet.org.The Evolution of ISM Mass Probed by Dust Emission -- ALMA Observations at z = 0.3 to 2N. Scoville, H. Aussel, K. Sheth, K. Scott, D. Sanders, R. Ivison, A. Pope, P. Capak, P. Bout, S. Manohar и 2 other автор(ы). (2014)cite arxiv:1401.2987Comment: Accepted ApJ 1/13/2014.Dust-obscured star formation and the contribution of galaxies escaping UV/optical color selections at z~2L. Riguccini, E. Floc'h, O. Ilbert, H. Aussel, M. Salvato, P. Capak, H. McCracken, J. Kartaltepe, D. Sanders, и N. Scoville. (2011)cite arxiv:1106.0498Comment: Accepted for publication in A&A. 16 pages, 13 figures.The evolving SFR-M_star relation and sSFR since z~5 from the VUDS spectroscopic surveyL. Tasca, O. Fevre, N. Hathi, D. Schaerer, O. Ilbert, G. Zamorani, B. Lemaux, P. Cassata, B. Garilli, V. Brun и 37 other автор(ы). (2014)cite arxiv:1411.5687Comment: 10 pages, 4 figures, submitted to A&A.The COSMOS2015 Catalog: Exploring the 1<z<6 Universe with half a million galaxiesC. Laigle, H. McCracken, O. Ilbert, B. Hsieh, I. Davidzon, P. Capak, G. Hasinger, J. Silverman, C. Pichon, J. Coupon и 27 other автор(ы). (2016)cite arxiv:1604.02350Comment: Accepted for publication in ApJ.The VIMOS Ultra-Deep Survey: ~10,000 galaxies with spectroscopic redshifts to study galaxy assembly at early epochs 2<z<~6O. Fevre, L. Tasca, P. Cassata, B. Garilli, V. Brun, D. Maccagni, L. Pentericci, R. Thomas, E. Vanzella, G. Zamorani и 35 other автор(ы). (2014)cite arxiv:1403.3938Comment: 43 pages, 30 figures, submitted to A&A.ISM Masses and Star Formation at z = 1 to 6 ALMA Observations of Dust Continuum in 180 Galaxies in COSMOSN. Scoville, K. Sheth, H. Aussel, P. Bout, P. Capak, A. Bongiorno, C. Casey, L. Murchikova, J. Koda, A. Pope и 5 other автор(ы). (2015)cite arxiv:1505.02159Comment: submitted ApJ Letters.The Interstellar Medium In Galaxies Seen A Billion Years After The Big BangP. Capak, C. Carilli, G. Jones, C. Casey, D. Riechers, K. Sheth, C. Carollo, O. Ilbert, A. Karim, O. LeFevre и 4 other автор(ы). (2015)cite arxiv:1503.07596Comment: Submitted to Nature, under review after referee report. 22 pages, 4 figures, 4 Extended Data Figures, 5 Extended Data tables.Spectroscopic observation of Ly$\alpha$ emitters at z~7.7 and implications on re-ionizationA. Faisst, P. Capak, C. Carollo, C. Scarlata, и N. Scoville. (2014)cite arxiv:1402.3604Comment: 11 pages, 6 figures, 2 tables, submitted to ApJ.Evolution of the specific Star Formation Rate Function at z<1.4 - Dissecting the mass-SFR plane in COSMOS and GOODSO. Ilbert, S. Arnouts, E. Floc'h, H. Aussel, H. Bethermin, P. Capak, B. Hsieh, M. Kajisawa, O. Fevre, N. Lee и 12 other автор(ы). (2014)cite arxiv:1410.4875Comment: 24 pages, 15 figures, 3 tables, submitted to A&A, comments are welcome.

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