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J/AJ/119/1562       gri photometry of 48 galaxy clusters    (Margoniner+, 2000)

Photometric properties of 48 clusters of galaxies. I. The Butcher-Oemler effect Margoniner V. E., de Carvalho R. R. <Astron. J. 119, 1562 (2000)> =2000AJ....119.1562M
ADC_Keywords: Clusters, galaxy ; Photometry, CCD Keywords: galaxies: clusters: general - galaxies: evolution - galaxies: fundamental parameters - galaxies: photometry Abstract: We present gri CCD photometry of 44 Abell clusters and four cluster candidates. Twenty-one clusters in our sample have spectroscopic redshifts. Fitting a relation between mean g, r, and i magnitudes and redshift for this subsample, we have calculated photometric redshifts for the remainder with an estimated accuracy of approximately 0.03. The resulting redshift range for the sample is 0.03 < z < 0.38. Color-magnitude diagrams are presented for the complete sample and used to study evolution of the galaxy population in the cluster environment. Description: We obtained CCD images of 48 clusters in four runs between 1997 March and 1998 November. All data were taken with the Tek 2K-3 detector at the Cassegrain focus of the 0.9 m telescope at the Cerro Tololo Inter-American Observatory (CTIO). The CCD has 2048x2048 pixels, each pixel covering 0.396'', corresponding to a field of approximately 13.5x13.5 or about 0.5-6.7 Mpc at z=0.03-0.38 (H0 = 67 km.s-1.Mpc-1). We observed 44 Abell clusters and four cluster candidates detected in POSS-II (Second Palomar Sky Survey; Gal et al. 2000AJ....119...12G) photographic plates. The images were taken through the g, r and i filters of the Thuan & Gunn (1976PASP...88..543T) photometric system, with effective wavelengths and widths of 5118 and 900 Å for g, 6798 and 1000 Å for r, and 8100 and 1500 Å for i. The exposure times varied between 15-60 minutes in the g band, 10-20 minutes in the r band, and 10-15 minutes in the i band. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table3.dat 74 19492 Galaxy catalogs and gri photometry
See also: VII/110 : Rich Clusters of Galaxies (Abell+ 1989) J/A+AS/103/245 : Gunn gri photometry of Clusters of Galaxies (Molinari+ 1994) J/A+AS/119/391 : Gunn photometry of seven clusters of galaxies (Molinari+ 1996) Byte-by-byte Description of file: table3.dat
Bytes Format Units Label Explanations
1- 10 A10 --- Name Galaxy name 12- 15 I4 yr Obs.Y Year of observation 17- 19 A3 "month" Obs.M Month of observation 21- 22 I2 d Obs.D Day of observation 26- 27 I2 h RAh Right Ascension (J2000) 29- 30 I2 min RAm Right Ascension (J2000) 32- 36 F5.2 s RAs Right Ascension (J2000) 40 A1 --- DE- Sign of the Declination (J2000) 41 I1 deg DEd Declination (J2000) 43- 44 I2 arcmin DEm Declination (J2000) 46- 50 F5.2 arcsec DEs Declination (J2000) 54- 58 F5.2 mag gmag The g band aperture magnitude 62- 66 F5.2 mag rmag The r band aperture magnitude 70- 74 F5.2 mag imag The i band aperture magnitude
History: From AJ electronic edition
(End) Greg Schwarz [AAS] 18-Apr-2000
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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