J/MNRAS/458/3083    Abell 3888 galaxies redshifts            (Shakouri+, 2016)

An optical analysis of the merging cluster Abell 3888. Shakouri S., Johnston-Hollitt M., Dehghan S. <Mon. Not. R. Astron. Soc., 458, 3083-3098 (2016)> =2016MNRAS.458.3083S 2016MNRAS.458.3083S (SIMBAD/NED BibCode)
ADC_Keywords: Clusters, galaxy ; Galaxy catalogs; Redshifts Keywords: galaxies: clusters: general - galaxies: clusters: individual: A3888 - galaxies: distances and redshifts Abstract: In this paper we present new AAOmega spectroscopy of 254 galaxies within a 30 arcmin radius around Abell 3888. We combine these data with the existing redshifts measured in a one degree radius around the cluster and performed a substructure analysis. We confirm 71 member galaxies within the core of A3888 and determine a new average redshift and velocity dispersion for the cluster of 0.1535±0.0009 and 1181±197km/s, respectively. The cluster is elongated along an East-West axis and we find the core is bimodal along this axis with two subgroups of 26 and 41 members detected. Our results suggest that A3888 is a merging system putting to rest the previous conjecture about the morphological status of the cluster derived from X-ray observations. In addition to the results on A3888 we also present six newly detected galaxy overdensities in the field, three of which we classify as new galaxy clusters. Description: Our new observations of the cluster A3888 were taken on the 2013 May 9 and 10 with the AAT in service mode. We present 254 new redshifts in the region of A3888. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 96 254 Details of the objects observed with the AAOmega tablea1.dat 51 48 Details of the galaxies of detected galaxy clusters (Structures 6-8) -------------------------------------------------------------------------------- Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 2 I2 h RAh Right ascension (J2000) 4- 5 I2 min RAm Right ascension (J2000) 7- 11 F5.2 s RAs Right ascension (J2000) 13 A1 --- DE- Declination sign (J2000) 14- 15 I2 deg DEd Declination (J2000) 17- 18 I2 arcmin DEm Declination (J2000) 20- 24 F5.2 arcsec DEs Declination (J2000) 26- 32 F7.5 --- z Redshift 34- 40 F7.5 --- e_z rms uncertainty on z 42 I1 --- q_z [3/5] Redshift quality flag (1) 44- 90 A47 --- Lines Spectral lines detected 92- 96 F5.2 mag Bmag Blue magnitude from the SuperCOSMOS catalogue -------------------------------------------------------------------------------- Note (1): Redshift quality flag as follows: 3 = likely reliable 4 = very reliable (both H and K absorption lines present) 5 = very reliable (H and K and at least one of the other absorption line (Mg, Na, G, Hδ) present) -------------------------------------------------------------------------------- Byte-by-byte Description of file: tablea1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1 I1 --- Struc [6/8] Structure number 3- 18 A16 --- Name Name of the structure (SJD JHHMM.m+DDMM) 20- 21 I2 h RAh Right ascension (J2000) 23- 24 I2 min RAm Right ascension (J2000) 26- 30 F5.2 s RAs Right ascension (J2000) 32 A1 --- DE- Declination sign (J2000) 33- 34 I2 deg DEd Declination (J2000) 36- 37 I2 arcmin DEm Declination (J2000) 39- 43 F5.2 arcsec DEs Declination (J2000) 45- 51 F7.5 --- z Redshift -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Patricia Vannier [CDS] 17-Feb-2017
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