J/A+A/561/A33  SDSS star-forming galaxies multi-wavelength study (Izotov+, 2014)

Multi-wavelength study of 14000 star-forming galaxies from the Sloan Digital Sky Survey. Izotov Y.I., Guseva N.G., Fricke K.J., Henkel C. <Astron. Astrophys., 561, A33-33 (2014)> =2014A&A...561A..33I 2014A&A...561A..33I
ADC_Keywords: Galaxies, photometry ; Photometry, SDSS ; Photometry, infrared ; Photometry, ultraviolet Keywords: galaxies: abundances Abstract: We studied a large sample of ∼14000 dwarf star-forming galaxies with strong emission lines. These low-metallicity galaxies with oxygen abundances of 12+logO/H∼7.4-8.5 are selected from the Sloan Digital Sky Survey (SDSS) and distributed in the redshift range of z∼0-0.6. We modelled spectral energy distributions (SED) of all galaxies, which were based on the SDSS spectra in the visible range of 0.38µm-0.92µm and included both the stellar and ionised gas emission. These SEDs were extrapolated to the UV and mid-infrared ranges to cover the wavelength range of 0.1µm-22µm. The SDSS spectroscopic data were supplemented by photometric data from the GALEX, SDSS, 2MASS, WISE, IRAS, and NVSS all-sky surveys. Using these data, we derived global characteristics of the galaxies, such as their element abundances, luminosities, and stellar masses. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table2.dat 108 96 Observed parameters of the galaxies table3.dat 88 96 Derived parameters of the galaxies -------------------------------------------------------------------------------- Byte-by-byte Description of file: table2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1 A1 --- Gr [abc] Group (G1) 3- 12 A10 --- Name Galaxy abbreviated name (JHHMM+DDMM) 14- 15 I2 h RAh Right ascension (J2000) 17- 18 I2 min RAm Right ascension (J2000) 20- 24 F5.2 s RAs Right ascension (J2000) 26 A1 --- DE- Declination sign (J2000) 27- 28 I2 deg DEd Declination (J2000) 30- 31 I2 arcmin DEm Declination (J2000) 33- 37 F5.2 arcsec DEs Declination (J2000) 39- 44 F6.4 --- z Spectroscopic redshift 46- 50 F5.2 mag gmag SDSS g magnitude 52- 56 F5.2 mag FUV ?=- GALEX far-UV magnitude 58- 62 F5.2 mag NUV ?=- GALEX near-UV magnitude 64- 68 F5.2 mag W1mag WISE 3.4um magnitude 70- 74 F5.2 mag W2mag WISE 4.6um magnitude 76- 80 F5.2 mag W3mag WISE 12um magnitude 82 A1 --- l_W4mag Limit flag on W4mag 83- 86 F4.2 mag W4mag WISE 22um magnitude 88-108 A21 --- OName Other names -------------------------------------------------------------------------------- Byte-by-byte Description of file: table3.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1 A1 --- Gr [abc] Group (G1) 3- 12 A10 --- Name Galaxy abbreviated name (JHHMM+DDMM) 14- 17 F4.2 [-] e(O) [7.4/8.6] Oxygen abundance (log(O/H)+12) 19- 21 I3 0.1nm EW(Hb) Rest-frame equivalent width of the Hβ emission line 23- 28 F6.2 mag gMAG Extinction-corrected absolute SDSS g magnitude 30- 34 F5.2 [10-7W] logLHb Log of the aperture- and extinction-corrected Hβ luminosity (in erg/s) 36- 40 F5.2 [10-6W/nm] logLFUV ?=- Log of the extinction-corrected GALEX far-UV luminosity (in erg/s/Å) 42- 46 F5.2 [10-6W/nm] logLNUV ?=- Log of the extinction-corrected GALEX near-UV luminosity (in erg/s/Å) 48- 52 F5.2 [10-6W/nm] logLW1 Log of the extinction-corrected WISE 3.4um luminosity (in erg/s/Å) 54- 58 F5.2 [10-6W/nm] logLW2 Log of the extinction-corrected WISE 4.6um luminosity (in erg/s/Å) 60- 64 F5.2 [10-6W/nm] logLW3 Log of the extinction-corrected WISE 12um luminosity (in erg/s/Å) 66 A1 --- l_logLW4 Limit flag on logLW4 67- 71 F5.2 [10-6W/nm] logLW4 Log of the extinction-corrected WISE 22um luminosity (in erg/s/Å) 73- 77 F5.2 [Msun] logM* Log of the aperture-corrected stellar mass 79- 82 F4.2 [Msun] logMy Log of the aperture-corrected mass of the young stellar population 84- 88 F5.2 Msun/yr SFR Star formation rate (1) -------------------------------------------------------------------------------- Note (1): SFR derived from L(Hα)=2.8L(Hβ) and using relation SFR(M/yr)=4.4x10-42L(Hα)(erg/s) (Kennicutt 1998ARA&A..36..189K 1998ARA&A..36..189K). -------------------------------------------------------------------------------- Note (G1): Groups as follows: a = Galaxies with m(3.4um)-m(4.6um)≥2mag b = Galaxies with 2mag>m(3.4um)-m(4.6um)≥1.5mag c = Representative galaxies with m(3.4um)-m(4.6um)<0.5mag -------------------------------------------------------------------------------- History: 09-May-2014: From electronic version of the journal 23-Nov-2016: Luminosity units in table3 corrected (fluxes units previously indicated), thanks to Genoveva Micheva to notice it and Yuri Izotov to confirm the right units.
(End) Patricia Vannier [CDS] 31-Mar-2014
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