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Redshifts of Emission-Line Objects in the Hubble Ultra Deep Field

2007; Institute of Physics; Volume: 134; Issue: 1 Linguagem: Inglês

10.1086/513512

1538-3881

Chun Xu, N. Pirzkal, Sangeeta Malhotra, James E. Rhoads, Bahram Mobasher, E. Daddi, C. Gronwall, Nimish P. Hathi, N. Panagia, Henry C. Ferguson, Anton M. Koekemoer, M. Kümmel, Leonidas A. Moustakas, A. Pasquali, S. di Serego Alighieri, J. Vernet, J. R. Walsh, Rogier A. Windhorst, Haojing Yan,

Stellar, planetary, and galactic studies

We present redshifts for 115 emission line objects in the Hubble Ultra Deep Field (HUDF) identified through the GRism ACS Program for Extragalactic Science (GRAPES) project using the slitless grism spectroscopy mode of the ACS Camera on the Hubble Space Telescope (HST). The sample was selected by an emission line search on all extracted 1-dimensional GRAPES spectra. We identify the emission lines using line wavelength ratios where multiple lines are detected in the grism wavelength range (5800A < lambda < 9600A), and using photometric redshift information where multiple lines are unavailable. We then derive redshifts using the identified lines. Our redshifts are accurate to delta(z) = 0.009, based on both statistical uncertainty estimates and comparison with published ground-based spectra. Over 40% of our sample is fainter than typical magnitude limits for ground-based spectroscopy (with i_{AB}>25 mag). Such emission lines would likely remain undiscovered without our deep survey. The emission line objects fall into 3 categories: 1) Most are low to moderate redshift galaxies (0 < z < 2), including many actively star forming galaxies with strong HII regions; 2) 9 are high redshift (4 < z < 7) Lyman-alpha emitters; and 3) at least 3 are candidate AGNs.