J/MNRAS/409/1455  Stellar populations of early-type galaxies   (Harrison+, 2010)

The stellar populations of early-type galaxies. I. Observations, line strengths and stellar population parameters. Harrison C.D., Colless M., Kuntschner H., Couch W.J., De Propris R., Pracy M.B. <Mon. Not. R. Astron. Soc., 409, 1455-1469 (2010)> =2010MNRAS.409.1455H 2010MNRAS.409.1455H
ADC_Keywords: Clusters, galaxy ; Galaxies, photometry ; Spectroscopy Keywords: methods: data analysis - galaxies: clusters: general - galaxies: elliptical and lenticular, cD - galaxies: stellar content Abstract: The influence of environment on the formation and evolution of early-type galaxies is, as yet, an unresolved issue. Constraints can be placed on models of early-type galaxy formation and evolution by examining their stellar populations as a function of environment. We present a catalogue of galaxies well suited to such an investigation. The magnitude-limited (bJ≤19.45) sample was drawn from four clusters (Coma, A1139, A3558 and A930 at =0.04) and their surrounds. The catalogue contains luminosities, redshifts, velocity dispersions and Lick line strengths for 416 galaxies, of which 245 are classified as early types. Luminosity-weighted ages, metallicities and α-element abundance ratios have been estimated for 219 of these early types. We also outline the steps necessary for measuring fully calibrated Lick indices and estimating the associated stellar population parameters using up-to-date methods and stellar population models. In a subsequent paper we perform a detailed study of the stellar populations of early-type galaxies in clusters and investigate the effects of environment. Description: Galaxies in the four clusters and three standard stars (HR6159, HR6770 and HR7317) were observed with 2dF during the nights of 2002 April 19-21 using the 300B and 1200V gratings. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file tablea1.dat 90 416 Details of the low-redshift galaxies tablea2.dat 189 416 Line-strengths of the galaxies tablea3.dat 52 416 Stellar population parameters of the galaxies -------------------------------------------------------------------------------- Byte-by-byte Description of file: tablea1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 5 A5 --- Cluster Cluster name 7- 21 A15 --- Name Galaxy name 23- 24 I2 h RAh Right ascension (J2000) 26- 27 I2 min RAm Right ascension (J2000) 29- 33 F5.2 s RAs Right ascension (J2000) 35 A1 --- DE- Declination sign (J2000) 36- 37 I2 deg DEd Declination (J2000) 39- 40 I2 arcmin DEm Declination (J2000) 42- 45 F4.1 arcsec DEs Declination (J2000) 47 A1 --- ET [y/n-] Early-type galaxy ? 49- 53 F5.2 mag bJmag bJ (blue) magnitude 55- 60 F6.2 mag bJMAG Absolute bJ magnitude 62- 66 F5.2 mag rFmag ?=- rF (red) magnitude 68- 73 F6.2 mag rFMAG ?=- Absolute rF magnitude 75- 79 I5 km/s cz Heliocentric spectroscopic redshift 81- 82 I2 km/s e_cz rms uncertainty on cz 84- 86 I3 km/s sigma Velocity dispersion 88- 90 I3 km/s e_sigma rms uncertainty on sigma -------------------------------------------------------------------------------- Byte-by-byte Description of file: tablea2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 15 A15 --- Name Galaxy name 17- 23 F7.4 0.1nm C2 ?=- C2(4668Å) index line strength 25- 31 F7.4 0.1nm Hb ?=- Hβ index line strength 33- 39 F7.4 0.1nm HbG ?=- HβG index (1) 41- 47 F7.4 0.1nm [OIII]1 ?=- [OIII]1 index line strength (1) 49- 55 F7.4 0.1nm [OIII]2 ?=- [OIII]2 index line strength (1) 57- 62 F6.4 0.1nm Fe5015 ?=- Fe5015 index line strength 64- 70 F7.4 mag Mg1 ?=- Mg1 index line strength 72- 77 F6.4 mag Mg2 ?=- Mg2 index line strength 79- 84 F6.4 0.1nm Mgb ?=- Mgb index line strength 86- 91 F6.4 0.1nm Fe5270 ?=- Fe5270 index line strength 93- 98 F6.4 0.1nm Fe5335 ?=- Fe5335 index line strength 100-105 F6.4 0.1nm Fe5406 ?=- Fe5406 index line strength 107-112 F6.4 0.1nm e_C2 ?=- rms uncertainty on C2 (4668Å) 114-119 F6.4 0.1nm e_Hb ?=- rms uncertainty on Hb 121-126 F6.4 0.1nm e_HbG ?=- rms uncertainty on HbaG 128-133 F6.4 0.1nm e_[OIII]1 ?=- rms uncertainty on [OIII]1 135-140 F6.4 0.1nm e_[OIII]2 ?=- rms uncertainty on [OIII]2 142-147 F6.4 0.1nm e_Fe5015 ?=- rms uncertainty on Fe5015 149-154 F6.4 mag e_Mg1 ?=- rms uncertainty on Mg1 156-161 F6.4 mag e_Mg2 ?=- rms uncertainty on Mg2 163-168 F6.4 0.1nm e_Mgb ?=- rms uncertainty on Mgb 170-175 F6.4 0.1nm e_Fe5270 ?=- rms uncertainty on Fe5270 177-182 F6.4 0.1nm e_Fe5335 ?=- rms uncertainty on Fe5335 184-189 F6.4 0.1nm e_Fe5406 ?=- rms uncertainty on Fe5406 -------------------------------------------------------------------------------- Note (1): index defined in Gonzales J.J. 1993, PhD thesis, Univ. California , Santa Cruz (USA) -------------------------------------------------------------------------------- Byte-by-byte Description of file: tablea3.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 15 A15 --- Name Galaxy name 17- 20 F4.1 Gyr Age ?=- Age of stellar population 22- 24 F3.1 Gyr E_Age ?=- Error on Age, upper limit 26- 28 F3.1 Gyr e_Age ?=- Error on Age, lower limit 30- 34 F5.2 [Sun] [Z/H] ?=- Metallicity 36- 39 F4.2 [Sun] e_[Z/H] ?=- rms uncertainty on Metallicity 41- 45 F5.2 [Sun] [a/Fe] ?=- [α/Fe] abundance 47- 50 F4.2 [Sun] e_[a/Fe] ?=- rms uncertainty on [a/Fe] 52 I1 --- N ? Number of indices used to estimate the parameters -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Patricia Vannier [CDS] 07-May-2011
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