VizieR Online Data Catalog: Hβ to N2 line fluxes of nearby galaxies (Brown+, 2017)

Journal article (2018)

Authors

M. J. I. Brown

J. Moustakas

E. Da Cunha

M. Imanishi

Lee Armus

B.R. Brandl Universiteit Leiden

J. Peek Civil Engineering & Geosciences

R. C. Kennicutt

N. J. Bonne

H. T. Intema

F. de Gasperin

M. Boquien

T. H. Jarrett

M. E. Cluver

J. D T Smith

Affiliation

External organisation

Galaxies: spectra Photometry: SDSS Radio continuum Stars: distances

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Published Date

2018

Language

English

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Affiliation

External organisation

Abstract

Our parent sample is star-forming galaxies with optical drift-scan spectrophotometry from Moustakas & Kennicutt (2006, J/ApJS/164/81) and Moustakas+ (2010, J/ApJS/190/233) that also have Sloan Digital Sky Survey III optical imaging (SDSS-III; Aihara+ 2011ApJS..193...29A). All of the galaxies in the sample have imaging at ultraviolet, optical, near-infrared, and mid-infrared wavelengths, taken from GALEX, the Swift UV/Optical Monitor Telescope, the Sloan Digital Sky Survey III (SDSS-III), the Two Micron All Sky Survey (2MASS), the Spitzer Space Telescope, and/or the Wide-field Infrared Space Explorer (WISE). Radio-continuum flux densities at 1.4GHz and 150MHz were determined using multiple sets of archival data. Our principal source of 1.4GHz flux densities is the NRAO VLA Sky Survey (NVSS, Condon+, 1998, VIII/65). Our principal source of 150MHz flux densities is the TIFR GMRT Sky Survey (TGSS), which has an angular resolution of ~25". We used the first alternative data release of the TGSS (TGSS ADR1; Intema+ 2017, J/A+A/598/A78). (1 data file).