J/A+AS/130/323 ESO Slice Project (Vettolani+ 1998)
The ESO Slice Project (ESP) galaxy redshift survey: III. The Sample
Vettolani G., Zucca E., Merighi R., Mignoli M., Proust D., Zamorani G.,
Cappi A., Guzzo L., Maccagni D., Ramella M., Stirpe G.M., Blanchard A.,
Cayatte V., Collins C., McGillivray H., Maurogordato S., Scaramella R.,
Balkowski C., Chincarini G., Felenbok P.
<Astron. Astrophys. Suppl. Ser. 130, 323 (1998)>
=1998A&AS..130..323V 1998A&AS..130..323V (SIMBAD/NED BibCode)
ADC_Keywords: Galaxy catalogs ; Surveys ; Radial velocities
Keywords: galaxies: distances and redshifts - cosmology: observations ;
large-scale structure of the Universe
Description:
The ESO Slice Project (ESP) is a galaxy redshift survey in a region
near the South Galactic Pole (see Vettolani et al.,
1997A&A...325..954V 1997A&A...325..954V; Zucca et al., 1997A&A...326..477Z 1997A&A...326..477Z). It extends
over a strip 22(RA)x1(DEC) square degrees, plus a nearby area of 5x1
square degrees, 5 degrees west of the main strip. The right ascension
limits are 22h30m and 01h20m, at a mean declination of -40°15'
(B1950). We have covered this region with a regular grid of adjacent
circular fields, with a diameter of 32arcmin each, corresponding to
the field of view of the multifiber spectrograph OPTOPUS at the 3.6m
ESO telescope. The total solid angle of the spectroscopic survey is
23.2 square degrees. The galaxy catalogue has been extracted from the
Edinburgh-Durham Southern Galaxy catalogue (Heydon-Dumbleton et al.,
1989MNRAS.238..379H 1989MNRAS.238..379H) which has been obtained from COSMOS (MacGillivray
& Stobie, 1984VA.....27..433M 1984VA.....27..433M) scans of SERC J survey plates. The
number of objects in the photometric ESP sample is 4487. The
spectroscopic survey is about 85% complete to the limiting magnitude
bJ=19.4, and consists of 3342 galaxies + 1 QSO with redshift
determination. The ESP survey is intermediate between shallow, wide
angle samples and very deep, one--dimensional pencil beams.
Table 2 lists the fields observed with OPTOPUS and their properties:
the numbers listed in this table can be used to compute the redshift
completeness of each fields, following eq.(2) of the paper. Table 3
provides the catalogue, with galaxies sorted in right ascension.
The catalogue with additional information and updates can also be
found at the following URL: http://boas5.bo.astro.it/~cappi/esokp.html
File Summary:
--------------------------------------------------------------------------------
FileName Lrecl Records Explanations
--------------------------------------------------------------------------------
ReadMe 80 . This file
table2.dat 54 107 OPTOPUS fields
table3.dat 70 4487 Catalogue
--------------------------------------------------------------------------------
See also:
http://boas5.bo.astro.it/~cappi/esokp.html : the database
J/A+A/342/1 : ESO Slice Project. VI. Groups of Galaxies. (Ramella+ 1999)
Byte-by-byte Description of file: table2.dat
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
2- 4 I3 --- Field OPTOPUS field number as in paper
8- 9 I2 h RAh Right ascension (B1950)
11- 12 I2 min RAm Right ascension (B1950)
14- 17 F4.1 s RAs Right ascension (B1950)
21 A1 --- DE- Declination sign
22- 23 I2 deg DEd Declination (B1950)
25- 26 I2 arcmin DEm Declination (B1950)
28- 29 I2 arcsec DEs Declination (B1950)
33- 34 I2 --- Nt No. of objects classified as galaxies in the
photometric catalogue
38- 39 I2 --- Nz No. of measured redshifts
43- 44 I2 --- Nno No. of not observed objects
48- 49 I2 --- Nf No. of failed spectra
53- 54 I2 --- Ns No. of stars
--------------------------------------------------------------------------------
Byte-by-byte Description of file: table3.dat
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
3- 7 I5 --- ESP ESP galaxy number as in paper
10- 12 I3 --- Field OPTOPUS field number as in paper
15- 16 I2 h RAh Right ascension (B1950)
18- 19 I2 min RAm Right ascension (B1950)
21- 24 F4.1 s RAs Right ascension (B1950)
27 A1 --- DE- Declination sign
28- 29 I2 deg DEd Declination (B1950)
31- 32 I2 arcmin DEm Declination (B1950)
34- 35 I2 arcsec DEs Declination (B1950)
38- 42 F5.2 --- bJmag bJ magnitude
45- 49 I5 km/s HRVa ?=0 Heliocentric radial velocity from
absorption lines (1)
51- 53 I3 km/s e_HRVa ?=0 Error on absorption line velocity
55- 59 F5.2 --- R ?=0 R parameter value from cross-correlation
62- 66 I5 km/s HRVe ?=0 Heliocentric radial velocity from
emission lines (1)
68- 70 I3 km/s e_HRVe ?=0 Error on emission line velocity
--------------------------------------------------------------------------------
Note (1): Codes in the velocity column:
-8888 = failed radial velocity measurement
-9999 = stellar spectrum (hence stars misclassified in the EDSGC)
99999 = only for the object #31954, a QSO with z=1.174
--------------------------------------------------------------------------------
Acknowledgements: Elena Zucca
References:
Vettolani et al., Paper I. 1997A&A...325..954V 1997A&A...325..954V
Zucca et al., Paper II. 1997A&A...326..477Z 1997A&A...326..477Z
Cappi et al., Paper IV. 1998A&A...336..445C 1998A&A...336..445C
Scaramella et al. Paper V. 1998A&A...334..404S 1998A&A...334..404S
(End) Patricia Bauer [CDS] 26-Mar-1998