J/AJ/112/1335       Hubble Deep Field observations   (Williams+ 1996)

The Hubble Deep Field observations, data reduction, and galaxy photometry. Williams R.E., Blacker B., Dickinson M., van Dyke Dixon W., Ferguson H.C., Fruchter A.S., Giavalisco M., Gilliland R.L., Heyer I., Katsanis R., Levay Z., Lucas R.A., McElroy D.B., Petro L., Postman M., Adorf H.-M., Hook R.N. <Astron. J. 112, 1335 (1996)> =1996AJ....112.1335W 1996AJ....112.1335W
ADC_Keywords: Galaxies, photometry Mission_Name: HST Abstract: The Hubble Deep Field (HDF) is a Director's Discretionary program on HST in Cycle 5 to image an undistinguished field at high Galactic latitude in four passbands as deeply as reasonably possible. These images provide the most detailed view to date of distant field galaxies and are likely to be important for a wide range of studies in galaxy evolution and cosmology. In order to optimize observing in the time available, a field in the northern continuous viewing zone was selected and images were taken for ten consecutive days, or approximately 150 orbits. Shorter 1-2 orbit images were obtained of the fields immediately adjacent to the primary HDF in order to facilitate spectroscopic follow-up by ground- based telescopes. The observations were made from 1995 December 18-30, and both raw and reduced data have been put in the public domain as a community service. We present a summary of the criteria for selecting the field, the rationale behind the filter selection and observing times in each band, and the strategies for planning the observations to maximize the exposure time while avoiding Earth-scattered light. Data reduction procedures are outlined, and images of the combined frames in each band are presented. Objects detected in these images are listed in a catalog with their basic photometric parameters. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table7.dat 124 3509 Hubble Deep Field source catalog table7.ps 72 10734 PostScript version of table7 tables.fit 2880 78 FITS tables of the complete set of parameters for each galaxy -------------------------------------------------------------------------------- See also: J/AJ/112/359 : Galaxies in the Hubble Deep Field (van den Bergh+ 1996) J/ApJ/453/48 : VI photometry of HST faint field galaxies (Driver+ 1995) Byte-by-byte Description of file: table7.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 14 A14 --- [WBD96] Identification number 17- 22 F6.1 pix Xpos X position (1) 24- 29 F6.1 pix Ypos Y position (1) 31- 32 I2 h RAh [12] Right ascension (J2000) 34- 35 I2 min RAm Right ascension (J2000) 37- 42 F6.3 s RAs Right ascension (J2000) 44 A1 --- DE- [+] Declination sign 45- 46 I2 deg DEd [62] Declination (J2000) 48- 49 I2 arcmin DEm Declination (J2000) 51- 55 F5.2 arcsec DEs Declination (J2000) 57 A1 --- l_mt Limit flag on mt 58- 62 F5.2 mag mt Total magnitude 64 A1 --- l_mi Limit flag on mi 65- 69 F5.2 mag mi Isophotal magnitude 71 A1 --- l_U-B Limit flag on U-B 72- 76 F5.2 mag U-B ? U-B colour index 78 A1 --- l_B-V Limit flag on B-V 79- 83 F5.2 mag B-V ? B-V colour index 85 A1 --- l_V-I Limit flag on V-I 86- 90 F5.2 mag V-I ? V-I colour index 92- 98 F7.2 --- S/N ? Signal-to-noise ratio 101-105 F5.2 arcsec2 area Area 108-111 F4.2 arcsec r1 Unweighted first moment radius 113-116 F4.2 --- b/a Ellipticity 118-120 I3 deg PA Position angle 122-124 A3 --- Flag Flags -------------------------------------------------------------------------------- Note (1): 1 pix = 0.1 arcsec; x increasing from left to right, y increasing from low to top -------------------------------------------------------------------------------- Acknowledgements: Copied on 27-Nov-1996 via FTP from http://www.stsci.edu/ftp/observer/hdf/archive/v2catalog
(End) Francois Ochsenbein [CDS] 27-Nov-1996
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