The diverse properties of the most ultraviolet-luminous galaxies discovered by GALEX

Charles G. Hoopes, Timothy M. Heckman, Samir Salim, Mark Seibert, Christy A. Tremonti, David Schiminovich, R. Michael Rich, D. Christopher Martin, Stephane Charlot, Guinevere Kauffmann, Karl Forster, Peter G. Friedman, Patrick Morrissey, Susan G. Neff, Todd Small, Ted K. Wyder, Luciana Bianchi, José Donas, Young Wook Lee, Barry F. MadoreBruno Milliard, Alex S. Szalay, Barry Y. Welsh, Sukyoung K. Yi

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Abstract

We report on the properties of a sample of ultraviolet-luminous galaxies (UVLGs) selected by matching the Galaxy Evolution Explorer (GALEX) All-Sky Imaging and Medium Imaging Surveys with the Sloan Digital Sky Survey third data release. The overlap between these two surveys is roughly 450 deg2. Of 25,362 galaxies (with SDSS spectroscopy) in the range 0.0 < z < 0.3 detected by GALEX, there are 215 galaxies with L > 2 × 1010 L at 1530 Å (observed wavelength). The properties of this population are well correlated with ultraviolet surface brightness. We find that the galaxies with low UV surface brightness are primarily large spiral systems with a mixture of old and young stellar populations, while the high surface brightness galaxies consist primarily of compact starburst systems, with an approximate boundary at a surface brightness of I1530 = 10 8 L kpc-2. The large galaxies appear to be the high-luminosity tail of the galaxy star formation function and owe their large luminosity to their large surface area. In terms of the behavior of surface brightness with luminosity, size with luminosity, the mass-metallicity relation, and other parameters, the compact UVLGs clearly depart from the trends established by the full sample of galaxies. The subset of compact UVLGs with the highest surface brightness (I1530 > 109 L kpc-2; "supercompact UVLGs") have characteristics that are remarkably similar to Lyman break galaxies at higher redshift. They are much more luminous (and thus have much higher star formation rates) than typical local ultraviolet-bright starburst galaxies and blue compact dwarf galaxies. They have metallicities that are systematically lower than normal galaxies of the same stellar mass, indicating that they are less chemically evolved. In all these respects, they are the best local analogs for Lyman break galaxies.

Original languageEnglish
Pages (from-to)441-456
Number of pages16
JournalAstrophysical Journal, Supplement Series
Volume173
Issue number2
DOIs
Publication statusPublished - 2007 Dec 1

Fingerprint

galaxies
brightness
luminosity
young population
surface area
metallicity
spectroscopy
wavelength
compact galaxies
starburst galaxies
dwarf galaxies
star formation rate
stellar mass
set theory
sky
star formation
analogs
trends
wavelengths

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

Hoopes, C. G., Heckman, T. M., Salim, S., Seibert, M., Tremonti, C. A., Schiminovich, D., ... Yi, S. K. (2007). The diverse properties of the most ultraviolet-luminous galaxies discovered by GALEX. Astrophysical Journal, Supplement Series, 173(2), 441-456. https://doi.org/10.1086/516644
Hoopes, Charles G. ; Heckman, Timothy M. ; Salim, Samir ; Seibert, Mark ; Tremonti, Christy A. ; Schiminovich, David ; Rich, R. Michael ; Martin, D. Christopher ; Charlot, Stephane ; Kauffmann, Guinevere ; Forster, Karl ; Friedman, Peter G. ; Morrissey, Patrick ; Neff, Susan G. ; Small, Todd ; Wyder, Ted K. ; Bianchi, Luciana ; Donas, José ; Lee, Young Wook ; Madore, Barry F. ; Milliard, Bruno ; Szalay, Alex S. ; Welsh, Barry Y. ; Yi, Sukyoung K. / The diverse properties of the most ultraviolet-luminous galaxies discovered by GALEX. In: Astrophysical Journal, Supplement Series. 2007 ; Vol. 173, No. 2. pp. 441-456.
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abstract = "We report on the properties of a sample of ultraviolet-luminous galaxies (UVLGs) selected by matching the Galaxy Evolution Explorer (GALEX) All-Sky Imaging and Medium Imaging Surveys with the Sloan Digital Sky Survey third data release. The overlap between these two surveys is roughly 450 deg2. Of 25,362 galaxies (with SDSS spectroscopy) in the range 0.0 < z < 0.3 detected by GALEX, there are 215 galaxies with L > 2 × 1010 L⊙ at 1530 {\AA} (observed wavelength). The properties of this population are well correlated with ultraviolet surface brightness. We find that the galaxies with low UV surface brightness are primarily large spiral systems with a mixture of old and young stellar populations, while the high surface brightness galaxies consist primarily of compact starburst systems, with an approximate boundary at a surface brightness of I1530 = 10 8 L⊙ kpc-2. The large galaxies appear to be the high-luminosity tail of the galaxy star formation function and owe their large luminosity to their large surface area. In terms of the behavior of surface brightness with luminosity, size with luminosity, the mass-metallicity relation, and other parameters, the compact UVLGs clearly depart from the trends established by the full sample of galaxies. The subset of compact UVLGs with the highest surface brightness (I1530 > 109 L ⊙ kpc-2; {"}supercompact UVLGs{"}) have characteristics that are remarkably similar to Lyman break galaxies at higher redshift. They are much more luminous (and thus have much higher star formation rates) than typical local ultraviolet-bright starburst galaxies and blue compact dwarf galaxies. They have metallicities that are systematically lower than normal galaxies of the same stellar mass, indicating that they are less chemically evolved. In all these respects, they are the best local analogs for Lyman break galaxies.",
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Hoopes, CG, Heckman, TM, Salim, S, Seibert, M, Tremonti, CA, Schiminovich, D, Rich, RM, Martin, DC, Charlot, S, Kauffmann, G, Forster, K, Friedman, PG, Morrissey, P, Neff, SG, Small, T, Wyder, TK, Bianchi, L, Donas, J, Lee, YW, Madore, BF, Milliard, B, Szalay, AS, Welsh, BY & Yi, SK 2007, 'The diverse properties of the most ultraviolet-luminous galaxies discovered by GALEX', Astrophysical Journal, Supplement Series, vol. 173, no. 2, pp. 441-456. https://doi.org/10.1086/516644

The diverse properties of the most ultraviolet-luminous galaxies discovered by GALEX. / Hoopes, Charles G.; Heckman, Timothy M.; Salim, Samir; Seibert, Mark; Tremonti, Christy A.; Schiminovich, David; Rich, R. Michael; Martin, D. Christopher; Charlot, Stephane; Kauffmann, Guinevere; Forster, Karl; Friedman, Peter G.; Morrissey, Patrick; Neff, Susan G.; Small, Todd; Wyder, Ted K.; Bianchi, Luciana; Donas, José; Lee, Young Wook; Madore, Barry F.; Milliard, Bruno; Szalay, Alex S.; Welsh, Barry Y.; Yi, Sukyoung K.

In: Astrophysical Journal, Supplement Series, Vol. 173, No. 2, 01.12.2007, p. 441-456.

Research output: Contribution to journalArticle

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AU - Hoopes, Charles G.

AU - Heckman, Timothy M.

AU - Salim, Samir

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AU - Schiminovich, David

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AU - Kauffmann, Guinevere

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AU - Donas, José

AU - Lee, Young Wook

AU - Madore, Barry F.

AU - Milliard, Bruno

AU - Szalay, Alex S.

AU - Welsh, Barry Y.

AU - Yi, Sukyoung K.

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N2 - We report on the properties of a sample of ultraviolet-luminous galaxies (UVLGs) selected by matching the Galaxy Evolution Explorer (GALEX) All-Sky Imaging and Medium Imaging Surveys with the Sloan Digital Sky Survey third data release. The overlap between these two surveys is roughly 450 deg2. Of 25,362 galaxies (with SDSS spectroscopy) in the range 0.0 < z < 0.3 detected by GALEX, there are 215 galaxies with L > 2 × 1010 L⊙ at 1530 Å (observed wavelength). The properties of this population are well correlated with ultraviolet surface brightness. We find that the galaxies with low UV surface brightness are primarily large spiral systems with a mixture of old and young stellar populations, while the high surface brightness galaxies consist primarily of compact starburst systems, with an approximate boundary at a surface brightness of I1530 = 10 8 L⊙ kpc-2. The large galaxies appear to be the high-luminosity tail of the galaxy star formation function and owe their large luminosity to their large surface area. In terms of the behavior of surface brightness with luminosity, size with luminosity, the mass-metallicity relation, and other parameters, the compact UVLGs clearly depart from the trends established by the full sample of galaxies. The subset of compact UVLGs with the highest surface brightness (I1530 > 109 L ⊙ kpc-2; "supercompact UVLGs") have characteristics that are remarkably similar to Lyman break galaxies at higher redshift. They are much more luminous (and thus have much higher star formation rates) than typical local ultraviolet-bright starburst galaxies and blue compact dwarf galaxies. They have metallicities that are systematically lower than normal galaxies of the same stellar mass, indicating that they are less chemically evolved. In all these respects, they are the best local analogs for Lyman break galaxies.

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Hoopes CG, Heckman TM, Salim S, Seibert M, Tremonti CA, Schiminovich D et al. The diverse properties of the most ultraviolet-luminous galaxies discovered by GALEX. Astrophysical Journal, Supplement Series. 2007 Dec 1;173(2):441-456. https://doi.org/10.1086/516644