J/AJ/131/2018     Galaxies with large velocity dispersions     (Bernardi+, 2006)

A search for the most massive galaxies: double trouble? Bernardi M., Sheth R.K., Nichol R.C., Miller C.J., Schlegel D., Frieman J., Schneider D.P., Subbarao M., York D.G., Brinkmann J. <Astron. J., 131, 2018-2034 (2006)> =2006AJ....131.2018B 2006AJ....131.2018B
ADC_Keywords: Galaxies, spectra ; Redshifts ; Velocity dispersion Keywords: galaxies: elliptical and lenticular, cD - galaxies: evolution - galaxies: fundamental parameters - galaxies: photometry - galaxies: stellar content Abstract: We describe the results of a search for galaxies with large (350≥km/s) velocity dispersions. The largest systems we have found appear to be the extremes of the early-type galaxy population: compared to other galaxies with similar luminosities, they have the largest velocity dispersions and the smallest sizes. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 86 57 Physical parameters and median errors of the objects in our sample that are not obvious superpositions table2.dat 66 48 *Physical parameters of the objects in our sample that are almost certainly superpositions -------------------------------------------------------------------------------- Note on table2.dat: For these objects, the measured parameters of the blend are almost certainly not those of the individual components, so the measurement errors are not reported. -------------------------------------------------------------------------------- See also: http://www.sdss.org : SDSS Home Page Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 4 A4 --- --- [SDSS] 6- 23 A18 --- SDSS SDSS name (JHHMMSS.s+DDMMSS.s) 25- 31 F7.5 --- z Redshift 33- 38 F6.2 mag rMAG Absolute r band magnitude 40- 43 F4.2 mag e_rMAG Error in rMAG 45- 48 F4.2 mag g-r Rest-frame model g-r color index 50- 53 F4.2 mag e_g-r Error in g-r 55- 58 F4.2 [kpc] logR r-band size 60- 63 F4.2 [kpc] e_logR Error in logR 65- 67 I3 km/s sigma Aperture-corrected velocity dispersion 69- 70 I2 km/s e_sigma Error in sigma 72- 76 F5.3 mag Mg2 ? Mg2 line strength 78- 82 F5.3 mag e_Mg2 ? Error in Mg2 84- 85 I2 --- S/N Signal-to-noise ratio (1) 86 A1 --- f_S/N [*] Indicates objects for which evidence for superposition is the weakest -------------------------------------------------------------------------------- Note (1): Estimates of Mg2 were only made if S/N≥18. -------------------------------------------------------------------------------- Byte-by-byte Description of file: table2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 4 A4 --- --- [SDSS] 6- 23 A18 --- SDSS SDSS name (JHHMMSS.s+DDMMSS.s) 25- 31 F7.5 --- z Spectroscopic redshift 33- 38 F6.2 mag rMAG Absolute r band magnitude 40- 43 F4.2 mag g-r g-r color index 45- 48 F4.2 [kpc] logR r-band size 50- 53 I4 km/s Delcz ? Line of sight separation between the two components 55- 57 I3 km/s sigma Aperture-corrected velocity dispersion 59- 63 F5.3 mag Mg2 ? Mg2 line strength 65- 66 I2 --- S/N Signal-to-noise ratio -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Marianne Brouty [CDS] 07-Mar-2007
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