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J/AJ/123/100        Redshifts of AWM and MKW poor clusters  (Koranyi+, 2002)

Kinematics of AWM and MKW poor clusters. Koranyi D.M., Geller M.J. <Astron. J. 123, 100 (2002)> =2002AJ....123..100K
ADC_Keywords: Clusters, galaxy ; Redshifts ; Equivalent widths Keywords: galaxies: clusters: general - galaxies: distances and redshifts - galaxies: kinematics and dynamics Abstract: We have measured 1365 redshifts to a limiting magnitude of R∼15.5 in 15 AWM/MKW clusters and have collected another 203 from the literature in MKW 4s, MKW 2, and MKW 2s. In AWM 7 we have extended the redshift sample to R∼18 in the cluster center. We have identified 704 cluster members in 17 clusters; 201 are newly identified. We summarize the kinematics and distributions of the cluster galaxies and provide an initial discussion of substructure, mass and luminosity segregation, spectral segregation, velocity-dispersion profiles, and the relation of the central galaxy to global cluster properties. We compute optical mass estimates, which we compare with X-ray mass determinations from the literature. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1.dat 84 1565 Kinematic data for all measured galaxies table2.dat 70 19 Cluster Census
Byte-by-byte Description of file: table1.dat
Bytes Format Units Label Explanations
1- 6 A6 --- Cluster Cluster name 8- 13 A6 --- Clust2 Second name of cluster when two clusters considered (For MKW 2 and MKW 2s only) 15- 16 I2 h RAh Hour of Right Ascension (J2000) (1) 18- 19 I2 min RAm Minute of Right Ascension (J2000) 21- 25 F5.2 s RAs Second of Right Ascension (J2000) 27 A1 --- DE- Sign of the Declination (J2000) 28- 29 I2 deg DEd Degree of Declination (J2000) 31- 32 I2 arcmin DEm Arcminute of Declination (J2000) 34- 37 F4.1 arcsec DEs Arcsecond of Declination (J2000) 39- 43 I5 km/s cz The heliocentric recession velocity 45- 47 I3 km/s e_cz Error in cz 49- 50 A2 --- Type [Em Ab?] Em: emission-line, Ab: absorption-line 52- 56 F5.1 0.1nm EW ? The Halpha equivalent width (2) 58- 62 F5.1 0.1nm e_EW ? Error in EW 64 A1 --- r_cz Source of cz (3) 66- 84 A19 --- Rem Remarks
Note (1): Objects are identified as [KG2002] JHHMMSS.s.ss+DDMMSS.s Note (2): Some galaxies with no measured equivalent widths are classified as Em if the quoted redshift is from an emission-line template (T,M,W), or if the galaxy is listed as having emission in (U,L). Velocity errors (e_cz) for galaxies with emission-line template velocities are boosted by 65km/s in quadrature. Note (3): Source of cz: T = FAST Spectrograph (Fabricant et al., 1998PASP..110...79F) mounted on the 1.5m Tillinghast telescope at the F. L. Whipple Observatory on Mount Hopkins M = MMT Blue Channel spectrograph W = WIYN/Hydra, Hydra multifiber bench spectrograph on the 3.5m WIYN telescope at Kitt Peak U = Updated Zwicky Catalog, UZC; Falco et al., 1999, Cat. J/PASP/111/438 L = Las Campanas Redshift Survey, LCRS; Shectman et al., 1996, Cat. VII/203 N = NED.
Byte-by-byte Description of file: table2.dat
Bytes Format Units Label Explanations
1- 6 A6 --- Cluster Cluster name 7 A1 --- m_Cluster [ab] Multiplicity index on Cluster 9- 11 I3 --- NTot Total number of targets examined 13- 15 I3 --- NCL Number of galaxies in the cluster 17- 19 I3 --- NAb Number of absorption -line galaxies in the cluster 21- 22 I2 --- NEm Number of emission-line galaxies in the cluster 24- 30 F7.1 km/s cz Weighted mean cluster redshift 32- 37 F6.2 mag Mag Absolute magnitude corresponding to 15.5mag at cz 39- 42 F4.2 deg ARad Angular search radius (1) 44- 47 F4.2 Mpc PRad Physical search radius in units of Mpc/h (1) 49- 70 A22 --- Rem Remarks
Note (1): The projected distance from the cD to the most distant galaxy in the region for which we measured a redshift. Conversion from degrees to h-1Mpc uses cz, hence the difference in physical search radius between MKW 7a and MKW 7b, and among MKW 2a, MKW 2b, and MKW 2s. See text for details.
History: From electronic version of the journal
(End) Greg Schwarz [AAS], Patricia Bauer [CDS] 10-Apr-2002
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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