J/ApJ/780/34 H_160_-selected catalog of galaxies in the HUDF (Lundgren+, 2014) ================================================================================ Tracing the mass growth and star formation rate evolution of massive galaxies from z~6 to z~1 in the Hubble Ultra-Deep Field. Lundgren B.F., van Dokkum P., Franx M., Labbe I., Trenti M., Bouwens R., Gonzalez V., Illingworth G., Magee D., Oesch P., Stiavelli M. =2014ApJ...780...34L ================================================================================ ADC_Keywords: Galaxy catalogs ; Photometry, HST ; Photometry, infrared ; Redshifts Keywords: galaxies: evolution - galaxies: formation - galaxies: fundamental parameters - galaxies: high-redshift - galaxies: stellar content Abstract: We present an analysis of an H_160_-selected photometric catalog of galaxies in the Hubble Ultra-Deep Field, using imaging from the WFC3/IR camera on the Hubble Space Telescope in combination with archival ultraviolet, optical, and near-infrared imaging. Using these data, we measure the spectral energy distributions of ~1500 galaxies to a limiting H_160_ magnitude of 27.8, from which we fit photometric redshifts and stellar population estimates for all galaxies with well-determined Spitzer IRAC fluxes, allowing for the determination of the cumulative mass function within the range 14. Description: The Hubble Ultra-Deep Field (HUDF; Beckwith et al. 2006, cat. J/AJ/132/1729) is an 11 arcmin2 region of the sky within the GOODS-South field, centered at 3^h^32^m^38.5^s^ -27^d^47'0.0''. The galaxies we examine have been selected from new H_160_-band imaging from the ultra-deep, near-IR WFC3/IR observations in the main HUDF field, part of the 192-orbit HUDF09 program (PI Illingworth: G0 11563). The HUDF09 program includes WFC3/IR images in three filter bands: Y_105_, J_125_, and H_160_. Imaging of the HUDF obtained with the ACS instrument on HST includes observations in four optical filter bands: F435W, F606W, F775W, and F850LP. The observations were obtained in a total of 400 orbits between 2003 September and 2004 January (Beckwith et al. 2006, cat. J/AJ/132/1729). We include deep U-band imaging taken with the VIMOS instrument on the Very Large Telescope's (VLT's) Melipal Unit Telescope at Cerro Paranal Observatory in Chile. These data were obtained by the European Southern Observatory large program 168.A-0485 (PI C. Cesarsky), as part of the Great Observatories Origins Deep Survey (GOODS). The individual frames contributing to the co-added image were obtained in service mode between 2004 August and 2006 October. The K_s_-band photometry in this work has been extracted from a combination of images taken with the Infrared Spectrometer and Array Camera (ISAAC) mounted on the Antu Unit Telescope of the VLT and the PANIC near-IR camera on the 6.5m Magellan telescopes. The VLT/ISAAC exposures were taken in two programs (ESO program 73.A-0764; PI I. Labbe), one consisting of 8hr on the GOODS Chandra Deep Field South and another 15hr exposure in the UDF. Wae include the super-deep observations from the GOODS-S Field, which were obtained using the Infrared Array Camera (IRAC) on the Spitzer Space Telescope taken as part of the Spitzer Legacy Program. We include imaging from channels 1 and 2, which are centered on wavelengths of 3.6{mu}m and 4.5{mu}m, respectively. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table3.dat 304 1553 Photometric catalog -------------------------------------------------------------------------------- See also: B/hst : HST Archived Exposures Catalog (STScI, 2007) II/258 : Hubble Ultra Deep Field Catalog (UDF) (STScI, 2004) J/ApJ/735/86 : NEWFIRM MBS: photometric catalogs (Whitaker+, 2011) J/AJ/135/1624 : PEARS emission-line galaxies (Straughn+, 2008) J/ApJ/682/985 : FIREWORKS photometry of GOODS CDF-S (Wuyts+, 2008) J/ApJ/655/51 : HDFS IRAC observations of 2