IR and UV Galaxies at z=0.6 --- Evolution of Dust Attenuation and Stellar Mass

@inproceedings{Xu2007IRAU,
  title={IR and UV Galaxies at z=0.6 --- Evolution of Dust Attenuation and Stellar Mass},
  author={C. Xu and D. Shupe and V. Buat and M. Rowan-Robinson and J. Iglesias-P'aramo and T. Takeuchi and T. Barlow and T. Conrow and F. Fang and K. Forster and P. Friedman and E. Gonzales-Solares and C. Lonsdale and D. Martin and P. Morrissey and S. Neff and D. Schiminovich and M. Seibert and T. Small and G. Smith and J. Surace and T. Wyder},
  year={2007}
}
  • C. Xu, D. Shupe, +19 authors T. Wyder
  • Published 2007
  • Physics
  • We study dust attenuation and stellar mass of z ~ 0.6 star-forming galaxies using new SWIRE observations in IR and GALEX observations in UV. Two samples are selected from the SWIRE and GALEX source catalogs in the SWIRE/GALEX field ELAIS-N1-00 (Ω = 0.8 deg^2). The UV-selected sample has 600 galaxies with photometric redshift (hereafter photo-z) 0.5 ≤ z ≤ 0.7 and NUV ≤ 23.5 (corresponding to L_(FUV) ≥ 10^(9.6) L_☉). The IR-selected sample contains 430 galaxies with f_(24 μm) ≥ 0.2 mJy (L_(dust… CONTINUE READING
    12 Citations

    Figures and Tables from this paper.

    Dust attenuation up to z ≃ 2 in the AKARI North Ecliptic Pole Deep Field
    Dust properties of Lyman-break galaxies at z ~ 3
    • 11
    • Highly Influenced
    • PDF
    The Local Universe as Seen in the Far-Infrared and Far-Ultraviolet: A Global Point of View of the Local Recent Star Formation
    • 78
    • PDF

    References

    SHOWING 1-10 OF 59 REFERENCES
    Luminosity functions for galaxies and quasars in the Spitzer Wide-area Infrared Extragalactic Legacy Survey
    • 88
    • PDF
    Ultraviolet and Far-Infrared-selected Star-forming Galaxies at z = 0: Differences and Overlaps
    • 12
    • PDF
    Dust Attenuation in the Nearby Universe: A Comparison between Galaxies Selected in the Ultraviolet and in the Far-Infrared
    • 263
    • PDF
    Star formation in the nearby universe: The ultraviolet and infrared points of view
    • 106
    • PDF
    The properties of ultraviolet-luminous galaxies at the current epoch
    • 130
    • PDF