Keck deimos spectroscopy of a GALEX UV-selected sample from the Medium Imaging Survey

Ryan P. Mallery, R. Michael Rich, Samir Salim, Todd Small, Stephane Charlot, Mark Seibert, Ted Wyder, Tom A. Barlow, Karl Forster, Peter G. Friedman, D. Christopher Martin, Patrick Morrissey, Susan G. Neff, David Schiminovich, Luciana Bianchi, José Donas, Timothy M. Heckman, Young Wook Lee, Barry F. Madore, Bruno MilliardAlex S. Szalay, Barry Y. Welsh, Sukyoung Yi

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Abstract

We report results from a pilot program to obtain spectroscopy for objects detected in the Galaxy Evolution Explorer (GALEX) Medium Imaging Survey (MIS). Our study examines the properties of galaxies detected by GALEX fainter than the Sloan Digital Sky Survey (SDSS) spectroscopic survey. This is the first study to extend the techniques of Salim and coworkers to estimate stellar masses, star formation rates (SFRs), and the b (star formation history) parameter for star-forming galaxies out to z ∼ 0.7. We obtain redshifts for 50 GALEXMlS sources reaching NUV = 23.9 (AB mag) having counterparts in the SDSS Data Release 4 (DR4). Of our sample, 43 are star-forming galaxies with z < 0.7,3 have emission-line ratios indicative of active galactic nuclei with z < 0.7, and 4 objects with z > 1 are QSOs, 3 of which are not previously cataloged. We compare our sample to a much larger sample of ∼50,000 matched GALEX/SGSS galaxies with SDSS spectroscopy; while our survey is shallow, the optical counterparts to our sources reach ∼3 mag fainter in SDSS r than the SDSS spectroscopic sample. We use emission-line diagnostics for the galaxies to determine that the sample contains mostly star-forming galaxies. The galaxies in the sample populate the blue sequence in the NUV - r versus Mr color-magnitude diagram. The derived stellar masses of the galaxies range from 108 to 1011 M, and derived SFRs are between 10-1 and 102 M yr-1. Our sample has SFRs, luminosities, and velocity dispersions that are similar to the samples of faint compact blue galaxies studied previously in the same redshift range by Koo and collaborators, Guzmán and collaborators, and Phillips and collaborators. However, our sample is ∼2 mag fainter in surface brightness than the compact blue galaxies. We find that the star formation histories for a majority of the galaxies are consistent with a recent starburst within the last 100 Myr.

Original languageEnglish
Pages (from-to)471-481
Number of pages11
JournalAstrophysical Journal, Supplement Series
Volume173
Issue number2
DOIs
Publication statusPublished - 2007 Dec 1

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Deimos
spectroscopy
galaxies
star formation rate
stellar mass
stars
history
star formation
histories
diagram
color-magnitude diagram

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

Mallery, Ryan P. ; Rich, R. Michael ; Salim, Samir ; Small, Todd ; Charlot, Stephane ; Seibert, Mark ; Wyder, Ted ; Barlow, Tom A. ; Forster, Karl ; Friedman, Peter G. ; Martin, D. Christopher ; Morrissey, Patrick ; Neff, Susan G. ; Schiminovich, David ; Bianchi, Luciana ; Donas, José ; Heckman, Timothy M. ; Lee, Young Wook ; Madore, Barry F. ; Milliard, Bruno ; Szalay, Alex S. ; Welsh, Barry Y. ; Yi, Sukyoung. / Keck deimos spectroscopy of a GALEX UV-selected sample from the Medium Imaging Survey. In: Astrophysical Journal, Supplement Series. 2007 ; Vol. 173, No. 2. pp. 471-481.
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Mallery, RP, Rich, RM, Salim, S, Small, T, Charlot, S, Seibert, M, Wyder, T, Barlow, TA, Forster, K, Friedman, PG, Martin, DC, Morrissey, P, Neff, SG, Schiminovich, D, Bianchi, L, Donas, J, Heckman, TM, Lee, YW, Madore, BF, Milliard, B, Szalay, AS, Welsh, BY & Yi, S 2007, 'Keck deimos spectroscopy of a GALEX UV-selected sample from the Medium Imaging Survey', Astrophysical Journal, Supplement Series, vol. 173, no. 2, pp. 471-481. https://doi.org/10.1086/516638

Keck deimos spectroscopy of a GALEX UV-selected sample from the Medium Imaging Survey. / Mallery, Ryan P.; Rich, R. Michael; Salim, Samir; Small, Todd; Charlot, Stephane; Seibert, Mark; Wyder, Ted; Barlow, Tom A.; Forster, Karl; Friedman, Peter G.; Martin, D. Christopher; Morrissey, Patrick; Neff, Susan G.; Schiminovich, David; Bianchi, Luciana; Donas, José; Heckman, Timothy M.; Lee, Young Wook; Madore, Barry F.; Milliard, Bruno; Szalay, Alex S.; Welsh, Barry Y.; Yi, Sukyoung.

In: Astrophysical Journal, Supplement Series, Vol. 173, No. 2, 01.12.2007, p. 471-481.

Research output: Contribution to journalArticle

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AU - Rich, R. Michael

AU - Salim, Samir

AU - Small, Todd

AU - Charlot, Stephane

AU - Seibert, Mark

AU - Wyder, Ted

AU - Barlow, Tom A.

AU - Forster, Karl

AU - Friedman, Peter G.

AU - Martin, D. Christopher

AU - Morrissey, Patrick

AU - Neff, Susan G.

AU - Schiminovich, David

AU - Bianchi, Luciana

AU - Donas, José

AU - Heckman, Timothy M.

AU - Lee, Young Wook

AU - Madore, Barry F.

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AU - Yi, Sukyoung

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N2 - We report results from a pilot program to obtain spectroscopy for objects detected in the Galaxy Evolution Explorer (GALEX) Medium Imaging Survey (MIS). Our study examines the properties of galaxies detected by GALEX fainter than the Sloan Digital Sky Survey (SDSS) spectroscopic survey. This is the first study to extend the techniques of Salim and coworkers to estimate stellar masses, star formation rates (SFRs), and the b (star formation history) parameter for star-forming galaxies out to z ∼ 0.7. We obtain redshifts for 50 GALEXMlS sources reaching NUV = 23.9 (AB mag) having counterparts in the SDSS Data Release 4 (DR4). Of our sample, 43 are star-forming galaxies with z < 0.7,3 have emission-line ratios indicative of active galactic nuclei with z < 0.7, and 4 objects with z > 1 are QSOs, 3 of which are not previously cataloged. We compare our sample to a much larger sample of ∼50,000 matched GALEX/SGSS galaxies with SDSS spectroscopy; while our survey is shallow, the optical counterparts to our sources reach ∼3 mag fainter in SDSS r than the SDSS spectroscopic sample. We use emission-line diagnostics for the galaxies to determine that the sample contains mostly star-forming galaxies. The galaxies in the sample populate the blue sequence in the NUV - r versus Mr color-magnitude diagram. The derived stellar masses of the galaxies range from 108 to 1011 M⊙, and derived SFRs are between 10-1 and 102 M⊙ yr-1. Our sample has SFRs, luminosities, and velocity dispersions that are similar to the samples of faint compact blue galaxies studied previously in the same redshift range by Koo and collaborators, Guzmán and collaborators, and Phillips and collaborators. However, our sample is ∼2 mag fainter in surface brightness than the compact blue galaxies. We find that the star formation histories for a majority of the galaxies are consistent with a recent starburst within the last 100 Myr.

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