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http://hdl.handle.net/20.500.12386/31890
Titolo: | The VANDELS ESO public spectroscopic survey. Final data release of 2087 spectra and spectroscopic measurements | Autori: | GARILLI, BIANCA MARIA ROSA McLure, R. PENTERICCI, Laura FRANZETTI, PAOLO GARGIULO, ADRIANA Carnall, A. CUCCIATI, Olga IOVINO, Angela Amorin, R. BOLZONELLA, MICOL BONGIORNO, ANGELA CASTELLANO, MARCO Cimatti, A. Cirasuolo, M. Cullen, F. Dunlop, J. Elbaz, D. Finkelstein, S. FONTANA, Adriano FONTANOT, Fabio FUMANA, Marco Guaita, L. Hartley, W. Jarvis, M. Juneau, S. Maccagni, D. McLeod, D. Nandra, K. Pompei, E. POZZETTI, Lucia SCODEGGIO, MARCO Talia, M. Calabrò, A. CRESCI, GIOVANNI Fynbo, J. P. U. Hathi, N. P. Hibon, P. Koekemoer, A. M. MAGLIOCCHETTI, MANUELA Salvato, M. VIETRI, GIUSTINA Zamorani, G. Almaini, O. Balestra, I. BARDELLI, Sandro Begley, R. Brammer, G. Bell, E. F. Bowler, R. A. A. Brusa, M. Buitrago, F. Caputi, C. Cassata, P. Charlot, S. Citro, A. CRISTIANI, Stefano Curtis-Lake, E. Dickinson, M. FAZIO, GIACOMO Ferguson, H. C. FIORE, Fabrizio Franco, M. Georgakakis, A. Giavalisco, M. GRAZIAN, Andrea Hamadouche, M. Jung, I. Kim, S. Khusanova, Y. Le Fèvre, O. LONGHETTI, Marcella Lotz, J. MANNUCCI, FILIPPO Maltby, D. Matsuoka, K. Mendez-Hernandez, H. Mendez-Abreu, J. MIGNOLI, Marco Moresco, M. NONINO, Mario Pannella, M. Papovich, C. Popesso, P. Roberts-Borsani, G. Rosario, D. J. Saldana-Lopez, A. SANTINI, Paola SAXENA, AAYUSH Schaerer, D. Schreiber, C. Stark, D. Tasca, L. A. M. Thomas, R. VANZELLA, Eros Wild, V. Williams, C. ZUCCA, Elena |
Data pubblicazione: | 2021 | Rivista: | ASTRONOMY & ASTROPHYSICS | Numero: | 647 | Da pagina:: | A150 | Abstract: | VANDELS is an ESO Public Spectroscopic Survey designed to build a sample of high-signal-to-noise ratio, medium-resolution spectra of galaxies at redshifts between 1 and 6.5. Here we present the final Public Data Release of the VANDELS Survey, comprising 2087 redshift measurements. We provide a detailed description of sample selection, observations, and data reduction procedures. The final catalogue reaches a target selection completeness of 40% at i<SUB>AB</SUB> = 25. The high signal-to-noise ratio of the spectra (above 7 in 80% of the spectra) and the dispersion of 2.5 Å allowed us to measure redshifts with high precision, the redshift measurement success rate reaching almost 100%. Together with the redshift catalogue and the reduced spectra, we also provide optical mid-infrared photometry and physical parameters derived through fitting the spectral energy distribution. The observed galaxy sample comprises both passive and star forming galaxies covering a stellar mass range of 8.3 < Log(M<SUB>*</SUB>/M<SUB>⊙</SUB>) < 11.7. <P />This paper, which presents the final data release of the final high-redshift VIMOS survey, is dedicated to the memory of Olivier Le Fèvre, PI of the VIMOS instrument, world renowned expert of extragalactic spectroscopy and a pioneer in spectroscopy of the distant Universe. <P />All catalogues and spectra are accessible through the survey database (<A href="http://vandels.inaf.it">http://vandels.inaf.it</A>) where all information can be queried interactively, and via the ESO Archive (<A href="https://www.eso.org/qi/">https://www.eso.org/qi/</A>). | URI: | http://hdl.handle.net/20.500.12386/31890 | URL: | https://www.aanda.org/articles/aa/full_html/2021/03/aa40059-20/aa40059-20.html http://arxiv.org/abs/2101.07645v1 |
ISSN: | 0004-6361 | DOI: | 10.1051/0004-6361/202040059 | Bibcode ADS: | 2021A&A...647A.150G | Fulltext: | open |
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