J/AJ/132/1729    Hubble Ultra Deep Field BVI-dropout sources   (Beckwith+, 2006)

The Hubble Ultra Deep Field. Beckwith S.V.W., Stiavelli M., Koekemoer A.M., Caldwell J.A.R., Ferguson H.C., Hook R., Lucas R.A., Bergeron L.E., Corbin M., Jogee S., Panagia N., Robberto M., Royle P., Somerville R.S., Sosey M. <Astron. J., 132, 1729-1755 (2006)> =2006AJ....132.1729B 2006AJ....132.1729B
ADC_Keywords: Surveys ; Galaxies, photometry ; Photometry, HST Keywords: astronomical data bases: miscellaneous - early universe - galaxies: evolution - galaxies: high-redshift Abstract: This paper presents the Hubble Ultra Deep Field (HUDF), a 1 million secs exposure of an 11arcmin2 region in the southern sky with the Advanced Camera for Surveys on the Hubble Space Telescope using Director's Discretionary Time. The exposure time was divided among four filters, F435W (B435), F606W (V606), F775W (i775), and F850LP (z850), to give approximately uniform limiting magnitudes mAB∼29 for point sources. The image contains at least 10000 objects, presented here as a catalog, the vast majority of which are galaxies. Visual inspection of the images shows few if any galaxies at redshifts greater than ∼4 that resemble present-day spiral or elliptical galaxies. The image reinforces the conclusion from the original Hubble Deep Field that galaxies evolved strongly during the first few billion years in the infancy of the universe. Using the Lyman break dropout method to derive samples of galaxies at redshifts between 4 and 7, it is possible to study the apparent evolution of the galaxy luminosity function and number density. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table6.dat 75 504 B435-dropout sources table7.dat 75 204 V606-dropout sources table8.dat 75 54 i775-dropout sources -------------------------------------------------------------------------------- See also: II/258 : Hubble Ultra Deep Field Catalog (UDF) (STScI, 2004) Byte-by-byte Description of file: table6.dat table7.dat table8.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 5 I5 --- UDF The STScI identification number, Cat. II/258 (1) 7- 14 F8.5 deg RAdeg Right Ascension in decimal degrees (J2000) 16- 24 F9.5 deg DEdeg Declination in decimal degrees (J2000) 26- 30 F5.3 arcsec r50 Radius containing 50% of the flux 32- 36 F5.2 mag Bmag ? The B (F435W) band magnitude 38- 42 F5.2 mag e_Bmag ? The 1σ error in Bmag 44- 48 F5.2 mag Vmag ? The V (F606W) band magnitude 50- 53 F4.2 mag e_Vmag ? The 1σ error in Vmag 55- 59 F5.2 mag imag ? The i (F775W) band magnitude 61- 64 F4.2 mag e_imag ? The 1σ error in imag 66- 70 F5.2 mag zmag The z (F850LP) band magnitude 72- 75 F4.2 mag e_zmag The 1σ error in zmag -------------------------------------------------------------------------------- Note (1): UDF number of table8.dat corresponds to UDF number of file udf-z.dat in Cat. II/258, and are identified as UDF 3NNNN in Simbad, (i.e, in table8.dat, "UDF = 229" is "UDF 30229 in Simbad) -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Greg Schwarz [AAS], Patricia Vannier [CDS] 26-Sep-2008
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line