J/ApJS/159/41 DEEP Groth Strip Survey. I. (Vogt+, 2005)
The DEEP Groth Strip Survey. I. The sample.
Vogt N.P., Koo D.C., Phillips A.C., Wu K., Faber S.M., Willmer C.N.A.,
Simard L., Weiner B.J., Illingworth G.D., Gebhardt K., Gronwall C.,
Guzman R., Im M., Sarajedini V., Groth E.J., Rhodes J., Brunner R.,
Connolly A., Szalay A., Kron R., Blandford R.
<Astrophys. J. Suppl. Ser., 159, 41-59 (2005)>
=2005ApJS..159...41V 2005ApJS..159...41V (SIMBAD/NED BibCode)
ADC_Keywords: Galaxies, photometry ; Photometry, HST
Keywords: cosmology: observations - galaxies: distances and redshifts -
galaxies: evolution - galaxies: formation - galaxies: structure -
surveys
Abstract:
The Deep Extragalactic Exploratory Probe (DEEP) is a multiphase
research program dedicated to the study of the formation and evolution
of galaxies and of large-scale structure in the distant universe. This
paper describes the first five-year phase, denoted DEEP1. A series of
10 DEEP1 papers will discuss a range of scientific topics (e.g., the
study of photometric and spectral properties of a general distant
galaxy survey, the evolution observed in galaxy populations of varied
morphologies). The observational basis for these studies is the Groth
Survey Strip field, a 127arcmin2 region that has been observed with
the Hubble Space Telescope (HST) in both broad I-band and V-band
optical filters and with the Low Resolution Imaging Spectrograph on
the Keck Telescopes. Catalogs of photometric and structural parameters
have been constructed for 11,547 galaxies and stars at magnitudes
brighter than 29, and spectroscopy has been conducted for a
magnitude-color weighted subsample of 818 objects.
File Summary:
--------------------------------------------------------------------------------
FileName Lrecl Records Explanations
--------------------------------------------------------------------------------
ReadMe 80 . This file
table1.dat 111 11547 Catalog of aperture photometry
--------------------------------------------------------------------------------
See also:
J/ApJS/142/1 : DEEP Groth Strip Survey. II. (Simard+, 2002)
J/ApJ/599/1006 : DEEP Groth Strip Survey. VII. (Kobulnicky+, 2003)
J/ApJ/571/136 : DEEP Groth Strip survey. X. (Im+, 2002)
Byte-by-byte Description of file: table1.dat
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 9 A9 --- GSSID The DEEP identification,
DEEP-GSS FFN-XXYYa in Simbad
11- 16 A6 --- Groth The GROTH identification (1)
18- 23 A6 --- Brunner The Brunner identification (2)
25- 32 A8 --- CFRS The CFRS identification (CHH.NNNN),
CFRS HH.NNNN in Simbad (3)
34- 35 I2 h RAh Hour of Right Ascension (J2000)
37- 38 I2 min RAm Minute of Right Ascension (J2000)
40- 45 F6.3 s RAs Second of Right Ascension (J2000)
47 A1 --- DE- Sign of the Declination (J2000)
48- 49 I2 deg DEd Degree of the Declination (J2000)
51- 52 I2 arcmin DEm Arcminute of Declination (J2000)
54- 58 F5.2 arcsec DEs Arcsecond of Declination (J2000)
60- 64 F5.2 mag Vmag ? Inner 1.5" core V606 filter Vega magnitude
66- 70 F5.2 mag Icmag ? Inner 1.5" core I814 filter Vega magnitude
72- 76 F5.2 mag V-Ic ? Inner 1.0" (V606-I814) Vega color index
78- 82 F5.2 mag VmagF ? FOCAS total V606 Vega magnitude
84- 88 F5.2 mag IcmagF ? FOCAS total I814 Vega magnitude
90- 94 F5.2 mag VmagG ? GIM2D total V606 Vega magnitude
96-100 F5.2 mag IcmagG ? GIM2D total I814 Vega magnitude
102-111 A10 --- Code Spectral selection code (4)
--------------------------------------------------------------------------------
Note (1): See Rhodes, Refregier, & Groth (2000ApJ...536...79R 2000ApJ...536...79R).
Note (2): See Brunner, Connolly, & Szalay (1999ApJ...516..563B 1999ApJ...516..563B).
Note (3): See Lilly et al. (1995, Cat. VII/225).
Note (4): Spectral selection code, defined as follows:
zsurvey = Redshift sample
serendip = Companions (on shared slitlet)
disk = Elongated galaxies, I<22.5
align = Mask alignment pointers (mostly stars)
phz = Photometric redshift calibrators
R# = Optical counterparts to known radio sources
morph = Morphologically selected
Group A,B = Members of two small groups on the sky
hiz = Dropout candidates
cfrs = CFRS targets with no redshifts
--------------------------------------------------------------------------------
History:
From electronic version of the journal
References:
Vogt et al., Paper I 2005ApJS..159...41V 2005ApJS..159...41V, this paper
Simard et al., Paper II 2002ApJS..142....1S 2002ApJS..142....1S, Cat. J/ApJS/142/1
Weiner et al., Paper III 2005ApJ...620..595W 2005ApJ...620..595W
Kobulnicky et al., Paper VII 2003ApJ...599.1006K 2003ApJ...599.1006K, Cat. J/ApJ/599/1006
Koo et al., Paper VIII 2005ApJS..157..175K 2005ApJS..157..175K, Cat. J/ApJS/157/175
Gebhardt et al., Paper IX 2003ApJ...597..239G 2003ApJ...597..239G
Im et al. Paper X 2002ApJ...571..136I 2002ApJ...571..136I, Cat. J/ApJ/571/136
Kobulnicky et al., Paper XII 2002AAS...201.5218K 2002AAS...201.5218K
(End) Greg Schwarz [AAS], Marianne Brouty [CDS] 07-Dec-2005