New constraints on the star formation histories and dust attenuation of galaxies in the local universe from GALEX

Samir Salim, Stéphane Charlot, R. Michael Rich, Guinevere Kauffmann, Timothy M. Heckman, Tom A. Barlow, Luciana Bianchi, Yong Ik Byun, Jose Donas, Karl Forster, Peter G. Friedman, Patrick N. Jelinsky, Young Wook Lee, Barry F. Madore, Roger F. Malina, D. Christopher Martin, Bruno Milliard, Patrick Morrissey, Susan G. Neff, David SchiminovichMark Seibert, Oswald H.W. Siegmund, Todd Small, Alex S. Szalay, Barry Y. Welsh, Ted K. Wyder

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We derive a variety of physical parameters including star formation rates (SFRs), dust attenuation, and burst mass fractions for 6472 galaxies observed by the Galaxy Evolution Explorer (GALEX) and present in the Sloan Digital Sky Survey Data Release 1 (SDSS DR1) main spectroscopic sample. Parameters are estimated in a statistical way by comparing each observed broadband spectral energy distribution (SED) (two GALEX and five SDSS bands) with an extensive library of model galaxy SEDs, which cover a wide range of star formation histories and include stochastic starbursts. We compare the constraints derived using SDSS bands only with those derived using the combination of SDSS and GALEX photometry. We find that the addition of the GALEX bands leads to significant improvement in the estimation of both the dust optical depth and the star formation rate over timescales of 100 Myr to 1 Gyr in a galaxy. We attain sensitivity to SFRs as low as 10-3 M yr -1, and we find that low levels of star formation (SF) are mostly associated with early-type, red galaxies. The least massive galaxies have ratios of current to past-averaged SF rates (b-parameter) consistent with constant SF over a Hubble time. For late-type galaxies, this ratio on average decreases with mass. We find that b correlates tightly with NUV - r color, implying that the SF history of a galaxy can be constrained on the basis of the NUV - r color alone. The fraction of galaxies that have undergone a significant starburst episode within the last 1 Gyr steeply declines with mass, from ∼20% for galaxies with ∼108 M to ∼5% for ∼1011 M galaxies.

Original languageEnglish
Pages (from-to)L39-L42
JournalAstrophysical Journal
Issue number1 II
Publication statusPublished - 2005 Jan 20


All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

Salim, S., Charlot, S., Rich, R. M., Kauffmann, G., Heckman, T. M., Barlow, T. A., Bianchi, L., Byun, Y. I., Donas, J., Forster, K., Friedman, P. G., Jelinsky, P. N., Lee, Y. W., Madore, B. F., Malina, R. F., Martin, D. C., Milliard, B., Morrissey, P., Neff, S. G., ... Wyder, T. K. (2005). New constraints on the star formation histories and dust attenuation of galaxies in the local universe from GALEX. Astrophysical Journal, 619(1 II), L39-L42.