J/AJ/138/598        NUV sources in Hubble Ultra Deep Field   (Voyer+, 2009)
The following files can be converted to FITS (extension .fit or fit.gz)
Query from: http://vizier.u-strasbg.fr/viz-bin/VizieR?-source=J/AJ/138/598

drwxr-xr-x 41 cats archive 4096 Feb 26 2012 [Up] drwxr-xr-x 4 cats archive 4096 Dec 7 2015 [TAR file] -rw-r--r-- 1 cats archive 460 Dec 7 2015 .message -r--r--r-- 1 cats archive 5420 Dec 7 2015 ReadMe -rw-r--r-- 1 cats archive 607 Dec 7 2015 +footg5.gif -rw-r--r-- 1 cats archive 2516 Dec 7 2015 +footg8.gif -r--r--r-- 1 cats archive 12576 Feb 12 2012 table1.dat [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe : J/AJ/138/598 NUV sources in Hubble Ultra Deep Field (Voyer+, 2009) ================================================================================ Near-ultraviolet sources in the Hubble Ultra Deep Field: the catalog. Voyer E.N., De Mello D.F., Siana B., Gardner J.P., Quirk C., Teplitz H.I. <Astron. J., 138, 598-605 (2009)> =2009AJ....138..598V ================================================================================ ADC_Keywords: Surveys ; Galaxy catalogs ; Ultraviolet Keywords: galaxies: evolution - galaxies: formation - galaxies: starburst Abstract: The catalog from the first high-resolution U-band image of the Hubble Ultra Deep Field, taken with Hubble's Wide-Field Planetary Camera 2 through the F300W filter, is presented. We detect 96 U-band objects and compare and combine this catalog with a Great Observatories Origins Deep Survey B-selected catalog that provides B, V, i, and z photometry, spectral types, and photometric redshifts. We have also obtained far-ultraviolet (FUV, 1614AA) data with Hubble's Advanced Camera for Surveys Solar Blind Channel (ACS/SBC) and with GALEX. We detected 31 sources with ACS/SBC, 28 with GALEX/FUV, and 45 with GALEX/NUV. The methods of observations, image processing, object identification, catalog preparation, and catalog matching are presented. Description: The U-band observations were obtained with the HST Wide-Field Planetary Camera 2 (WFPC2) in the Cycle 13 HST Treasury proposal (Teplitz, Program 10403). The UDF was imaged in the near-UV (NUV) through the WFPC2/F300W filter (lambdamax=2987AA and deltalambda=740AA) in 12 HST orbits divided into 4 roll angles to compensate for the shape of the WFPC2 chevron and achieve uniform depth. FUV imaging was also obtained in this proposal with HST/ACS Solar Blind Channel (SBC) camera at which time WFPC2 parallel observations were also made. The UDF ACS/SBC images were taken in 50 HST orbits using the long-pass quartz filter (F150LP; lambdaeff=1614AA and FWHM=177AA). The U-band catalog, including U, FUV, B, and BVi postage stamp images of each source, is available online at http://goods.gsfc.nasa.gov/release/UDF_F300W/original/gallery/udf_u_fuv.html

© Université de Strasbourg/CNRS

    • Contact