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II/258              Hubble Ultra Deep Field Catalog (UDF)     (STScI, 2004)

The Hubble Ultra Deep Field Catalog Beckwith S.V.W. <Space Telescope Science Institute (2004)>
ADC_Keywords: Photometry, HST ; Surveys ; Galaxy catalogs Mission_Name: HST Description: The Hubble Ultra Deep Field (PI: Steven V. W. Beckwith) is a 400-orbit Cycle 12 program to image a single field of the Wide Field Camera (WFC) of the Advanced Camera for Surveys (ACS) in four filters: F435W (B), F606W (V), F775W (i), and F850LP (z). The observations took place over 4 months from September 2003 to January 2004 under two program IDs: 9978 and 10086. The observations consist of half-orbit exposures, cycling through each of the filters in a 4-point dither pattern to provide sub-pixel sampling, as well as a larger-scale 3-point line pattern to cover the 2 second of arc gap between the two ACS/WFC chips. The total exposure times are summarized below, with typical exposure times of 1200s for individual images. The AB magnitude zero-points for ACS are current as of March 2004. --------------------------------------------------------------- Number of Number of Total Exp. AB mag. Orbits Exposures Time (s) zero-point --------------------------------------------------------------- B (F435W): 56 112 134880 25.673 V (F606W): 56 112 135320 26.486 i (F775W): 144 288 347110 25.654 z (F850LP): 144 288 346620 24.862 --------------------------------------------------------------- More details are found in the "intro.txt" file, or from the UDF home page. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file intro.txt 68 419 Introduction udf-i.dat 213 10179 The Ultra-Deep Field Catalog from F775W image udf-z.dat 213 7016 The Ultra-Deep Field Catalog from F850LP image
See also: II/253 : Chandra Deep Field South: multi-colour data (Wolf+, 2004) http://cadcwww.hia.nrc.ca/udf/ : Ultra Deep Field High-Level Science Products http://www.stsci.edu/hst/udf : Ultra Deep Field Home Page Byte-by-byte Description of file: udf-i.dat udf-z.dat
Bytes Format Units Label Explanations
3- 7 I5 --- UDF Running number (G1) 11- 17 F7.2 pix Xpos Position of the source (toward East) 20- 26 F7.2 pix Ypos Position of the source (toward North) 29- 39 F11.7 deg RAdeg Right Ascension (J2000) 42- 52 F11.7 deg DEdeg Declination (J2000) 56- 60 F5.1 deg Theta [-90,+90] source orientation "Theta" (counterclockwise from the X-axis = PA-90) 64- 68 F5.3 --- ell Ellipticity (1-b/a) 74- 80 F7.2 pix R50 Half-light radius 83- 88 F6.2 pix FWHM FWHM of a Gaussian fit to each source 93- 96 F4.2 --- Sty Stellarity (1 for point sources, 0 for fully resolved sources) 105-111 F7.4 mag Bmag ?=99.00 AB magnitude in F435W filter (2) 113-119 F7.4 mag e_Bmag ?=99.00 Formal error on Bmag 122-127 F6.1 --- Bs/n Signal to Noise ratio in F435W filter 132-138 F7.4 mag Vmag ?=99.00 AB magnitude in F606W filter (2) 140-146 F7.4 mag e_Vmag ?=99.00 Formal error on Vmag 149-154 F6.1 --- Vs/n Signal to Noise ratio in F606W filter 159-165 F7.4 mag imag ?=99.00 AB magnitude in F775W filter (2) 167-173 F7.4 mag e_imag ?=99.00 Formal error on imag 176-181 F6.1 --- is/n Signal to Noise ratio in F775W filter 186-192 F7.4 mag zmag ?=99.00 AB magnitude in F850LP filter (2) 194-200 F7.4 mag e_zmag ?=99.00 Formal error on zmag 203-208 F6.1 --- zs/n Signal to Noise ratio in F850LP filter 212-213 I2 --- Flags SExtractor flags (1)
Note (1): combination of binary flags with the following meaning: 1 = The object has neighbors, bright and close enough to significantly bias the photometry, or bad pixels 2 = The object was originally blended with another one. 4 = At least one pixel of the object is saturated (or very close to). 8 = The object is truncated (too close to an image boundary). 16 = Object's aperture data are incomplete or corrupted. Note (2): magnitude isophotally matched.
Global Notes: Note (G1): Nomenclature note: Objects in udf-i.dat file are identified as UDF NNNNN in Simbad. Objects in udf-z.dat file are identified as UDF 3NNNN in Simbad, (i.e, in udf-z.dat file, "Seq = 1" is "UDF 30001" in Simbad).
History: From http://cadcwww.hia.nrc.ca/udf/acs-wfc/
(End) Francois Ochsenbein [CDS] 07-May-2005
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

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