Search catalogue
J/MNRAS/392/1265 Faint red galaxies in Coma cluster spectroscopy (Smith+, 2009)
A spectroscopic survey of dwarf galaxies in the Coma cluster: stellar populations, environment and downsizing. Smith R.J., Lucey J.R., Hudson M.J., Allanson S.P., Bridges T.J., Hornschemeier A.E., Marzke R.O., Miller N.A. <Mon. Not. R. Astron. Soc., 392, 1265-1294 (2009)> =2009MNRAS.392.1265S
ADC_Keywords: Clusters, galaxy ; Galaxy catalogs ; Spectroscopy Keywords: galaxies: clusters: individual: Coma - galaxies: dwarf - galaxies: elliptical and lenticular, cD - galaxies: evolution - galaxies: formation Abstract: We investigate the stellar populations in a sample of 89 faint red galaxies in the Coma cluster, using high signal-to-noise ratio (S/N) spectroscopy from the 6.5-m MMT. Our sample is drawn from two 1° fields, one centred on the cluster core and the other located 1° to the south-west of the cluster centre. The target galaxies are mostly 2-4mag fainter than M*; galaxies with these luminosities have been previously studied only using small samples, or at low S/N. For a comparison sample we use published high-S/N data for red-sequence galaxies in the Shapley supercluster. We use state-of-the-art stellar population models (by R. Schiavon, Cat. J/ApJS/171/146) to interpret the absorption-line indices and infer the single-burst-equivalent age and metallicity (Fe/H) for each galaxy, as well as the abundances of the light elements Mg, Ca, C and N. Description: Spectra were obtained at the 6.5-m MMT using the Hectospec fibre-fed spectrograph, in parallel with a redshift survey of faint candidate cluster members (Marzke et al., in preparation). The observations were performed in queue-mode over the period 2007 February-April, mainly within five days of new moon. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file tablee1.dat 291 89 Absorption-line index data for the Coma sample tablee2.dat 92 89 Derived parameters for the Coma dwarf galaxy sample tablee3.dat 95 66 *Stellar population parameters from EZ-AGES for the Shapley sample
Note on tablee3.dat: Other relevant parameters for these galaxies, including the individual line index measurements, were tabulated by Smith et al. (2007, Cat. J/MNRAS/381/1035).
See also: VII/42 : GMP catalogue: galaxies in the Coma cluster (Godwin+ 1983) J/MNRAS/381/1035 : Spectroscopy in Shapley supercluster (Smith+, 2007) Byte-by-byte Description of file: tablee1.dat
Bytes Format Units Label Explanations
1- 4 I4 --- GMP GMP number 6- 7 I2 h RAh Right ascension (J2000) 8 A1 --- --- [:] 9- 10 I2 min RAm Right ascension (J2000) 11 A1 --- --- [:] 12- 15 F4.1 s RAs Right ascension (J2000) 17 A1 --- DE- Declination sign (J2000) 18- 19 I2 deg DEd Declination (J2000) 20 A1 --- --- [:] 21- 22 I2 arcmin DEm Declination (J2000) 23 A1 --- --- [:] 24- 25 I2 arcsec DEs Declination (J2000) 27- 31 F5.2 mag umag SDSS u magnitude 33- 37 F5.2 mag gmag SDSS g magnitude 39- 43 F5.2 mag rmag SDSS r magnitude 45- 49 F5.2 mag imag SDSS i magnitude 51- 55 F5.2 mag zmag SDSS z magnitude 57- 61 F5.2 0.1nm HdA HδA index 63- 66 F4.2 0.1nm e_HdA rms uncertainty on HdA 68- 72 F5.2 0.1nm HdF HδA index 74- 77 F4.2 0.1nm e_HdF rms uncertainty on HdF 79- 84 F6.3 mag CN1 CN1 index 86- 91 F6.3 mag e_CN1 rms uncertainty on CN1 93- 98 F6.3 mag CN2 CN2 index 100-105 F6.3 mag e_CN2 rms uncertainty on CN2 107-111 F5.2 0.1nm Ca4227 Ca4227 index 113-119 F7.2 0.1nm e_Ca4227 rms uncertainty on Ca4227 121-125 F5.2 0.1nm G4300 G4300 index 127-130 F4.2 0.1nm e_G4300 rms uncertainty on G4300 132-136 F5.2 0.1nm HgA HγA index 138-141 F4.2 0.1nm e_HgA rms uncertainty on HgA 143-147 F5.2 0.1nm HgF HγF index 149-152 F4.2 0.1nm e_HgF rms uncertainty on HgF 154-158 F5.2 0.1nm Fe4383 Fe4383 index 160-163 F4.2 0.1nm e_Fe4383 rms uncertainty on Fe4383 165-169 F5.2 0.1nm Ca4455 Ca4455 index 171-174 F4.2 0.1nm e_Ca4455 rms uncertainty on Ca4455 176-180 F5.2 0.1nm Fe4531 Fe4531 index 182-185 F4.2 0.1nm e_Fe4531 rms uncertainty on Fe4531 187-191 F5.2 0.1nm Fe4668 Fe4668 index 193-196 F4.2 0.1nm e_Fe4668 rms uncertainty on Fe4668 198-202 F5.2 0.1nm Hb Hβ index 204-207 F4.2 0.1nm e_Hb rms uncertainty on Hb 209-213 F5.2 0.1nm Fe5015 Fe5015 index 215-221 F7.2 0.1nm e_Fe5015 rms uncertainty on Fe5015 223-227 F5.2 0.1nm Mgb Mgb5177 index 229-232 F4.2 0.1nm e_Mgb rms uncertainty on Mgb 234-239 F6.3 mag Mg1 Mg1 index 241-245 F5.3 mag e_Mg1 rms uncertainty on Mg1 247-252 F6.3 mag Mg2 Mg2 index 254-258 F5.3 mag e_Mg2 rms uncertainty on Mg2 260-264 F5.2 0.1nm Fe5270 Fe5270 index 266-269 F4.2 0.1nm e_Fe5270 rms uncertainty on Fe5270 271-275 F5.2 0.1nm Fe5335 Fe5335 index 277-280 F4.2 0.1nm e_Fe5335 rms uncertainty on Fe5335 282-286 F5.2 0.1nm Fe5406 ?=- Fe5406 index 288-291 F4.2 0.1nm e_Fe5406 ?=- rms uncertainty on Fe5406
Byte-by-byte Description of file: tablee2.dat
Bytes Format Units Label Explanations
1- 4 I4 --- GMP GMP number 5 A1 --- n_GMP [ab] Pecularity on galaxy (1) 7- 10 F4.2 [solLum] logL Luminosity (2) 12- 16 F5.3 [km/s] log.sig ?=- Velocity dispersion from literature compilation 18- 19 I2 --- S/N Signal-to-noise ratio (3) 21- 24 I4 km/s cz Heliocentric velocity 26- 29 F4.1 Gyr tSSP ? SSP-equivalent age (G1) 31- 33 F3.1 Gyr E_tSSP ? Error on tSSP (upper limit) 35- 37 F3.1 Gyr e_tSSP ? Error on tSSP (lower limit) 39- 43 F5.2 [Sun] [Fe/H] ? Abundance [Fe/H] 45- 48 F4.2 [Sun] e_[Fe/H] ? rms uncertainty on [Fe/H] 50- 54 F5.2 [Sun] [Mg/Fe] ? Abundance [Mg/Fe] 56- 59 F4.2 [Sun] e_[Mg/Fe] ? rms uncertainty on [Mg/Fe] 61- 65 F5.2 [Sun] [C/Fe] ? Abundance [C/Fe] 67- 70 F4.2 [Sun] e_[C/Fe] ? rms uncertainty on [C/Fe] 72- 76 F5.2 [Sun] [N/Fe] ? Abundance [N/Fe] 78- 81 F4.2 [Sun] e_[N/Fe] ? rms uncertainty on [N/Fe] 83- 87 F5.2 [Sun] [Ca/Fe] ? Abundance [Ca/Fe] 89- 92 F4.2 [Sun] e_[Ca/Fe] ? rms uncertainty on [Ca/Fe]
Note (1): Note as follows: a = Galaxy with emission lines b = Other galaxy with failed EZ-AGES fits (see details in Appendix D) Note (2): Luminosity based on the SDSS Petrosian magnitude and include the corrections described in Section 2.2. Note (3): S/N is per angstrom, averaged over 4400-5400Å in the rest frame
Byte-by-byte Description of file: tablee3.dat
Bytes Format Units Label Explanations
1- 15 A15 --- Name Galaxy name (HHMMSS.s+DDMMSS) (1) 17- 21 F5.2 [solLum] logL Luminosity (2) 23- 27 F5.3 [km/s] log.sig ?=- Velocity dispersion from literature compilation 29- 32 F4.1 Gyr tSSP ? SSP-equivalent age (G1) 34- 36 F3.1 Gyr E_tSSP ? Error on tSSP (upper limit) 38- 40 F3.1 Gyr e_tSSP ? Error on tSSP (lower limit) 42- 46 F5.2 [Sun] [Fe/H] ? Abundance [Fe/H] 48- 51 F4.2 [Sun] e_[Fe/H] ? rms uncertainty on [Fe/H] 53- 57 F5.2 [Sun] [Mg/Fe] ? Abundance [Mg/Fe] 59- 62 F4.2 [Sun] e_[Mg/Fe] ? rms uncertainty on [Mg/Fe] 64- 68 F5.2 [Sun] [C/Fe] ? Abundance [C/Fe] 70- 73 F4.2 [Sun] e_[C/Fe] ? rms uncertainty on [C/Fe] 75- 79 F5.2 [Sun] [N/Fe] ? Abundance [N/Fe] 81- 84 F4.2 [Sun] e_[N/Fe] ? rms uncertainty on [N/Fe] 86- 90 F5.2 [Sun] [Ca/Fe] ? Abundance [Ca/Fe] 92- 95 F4.2 [Sun] e_[Ca/Fe] ? rms uncertainty on [Ca/Fe]
Note (1): NFP galaxies except 132350.3-313519. Note (2): Luminosity based on the SDSS Petrosian magnitude and include the corrections described in Section 2.2.
Global Notes: Note (G1): the age with the Simple Stellar Population model is estimated from Hβ and metal lines as in Section 3.
History: From electronic version of the journal
(End) Patricia Vannier [CDS] 17-Aug-2009
| 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 |
© UDS/CNRS