H. Inami, R. Bacon, J. Brinchmann, J. Richard, T. Contini, S. Conseil, S. Hamer, M. Akhlaghi, N. Bouchť, B. Clement, G Desprez, A. Drake, T. Hashimoto, F. Leclercq, M. Maseda, L. Michel-Dansac, M. Paalvast, L. Tresse, E. Ventou, W. Kollatschny, L. A. Boogaard, H. Finley, R. A. Marino, J. Schaye, L. Wisotzki
We have conducted a two-layered spectroscopic survey (1' x 1' ultra deep and 3' x 3' deep regions) in the Hubble Ultra Deep Field (HUDF) with the Multi Unit Spectroscopic Explorer (MUSE). The combination of a large field of view, high sensitivity, and wide wavelength coverage provides an order of magnitude improvement in spectroscopically confirmed redshifts in the HUDF; i.e., 1206 secure spectroscopic redshifts for HST continuum selected objects, which corresponds to 15% of the total (7904). The redshift distribution extends well beyond z > 3 and to HST/F775W magnitudes as faint as approximate to 30 mag (AB, 1 sigma). In addition, 132 secure redshifts were obtained for sources with no HST counterparts that were discovered in the MUSE data cubes by a blind search for emission-line features. In total, we present 1338 high quality redshifts, which is a factor of eight increase compared with the previously known spectroscopic redshifts in the same field. We assessed redshifts mainly with the spectral features [O II] at z < 1.5 (473 objects) and Ly alpha at 2.9 < z < 6.7 (692 objects). With respect to F775W magnitude, a 50% completeness is reached at 26.5 mag for ultra deep and 25.5 mag for deep fields, and the completeness remains greater than or similar to 20% up to 28-29 mag and approximate to 27 mag, respectively. We used the determined redshifts to test continuum color selection (dropout) diagrams of high-z galaxies. The selection condition for F336W dropouts successfully captures approximate to 80% of the targeted z similar to 2.7 galaxies. However, for higher redshift selections (F435W, F606W, and F775W dropouts), the success rates decrease to approximate to 20-40%. We empirically redefine the selection boundaries to make an attempt to improve them to approximate to 60%. The revised boundaries allow bluer colors that capture Ly alpha emitters with high Ly alpha equivalent widths falling in the broadbands used for the color-color selection. Along with this paper, we release the redshift and line flux catalog.
galaxies: high-redshift; galaxies: formation; galaxies: evolution; catalogs; surveys; Astrophysics - Astrophysics of Galaxies
Astronomy and Astrophysics
Volume 608, Article Number 2