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AA1730027009.pdf265.26 kB
titleFar Infrared Properties of UV Selected Galaxies from z=4 to z=1.5: Unveiling Obscured Star Formation
Author(eng)Buat, Veronique; Heinis, Sebastien; The HerMES team
Author Affiliation(eng)Aix-Marseille Universite; Aix-Marseille Universite : University of Maryland
Issue Date2018-03-09
PublisherJapan Aerospace Exploration Agency (JAXA)
宇宙航空研究開発機構(JAXA)
Publication titleJAXA Special Publication: Proceedings of the SPICA Science Conference from Exoplanets to Distant Galaxies: SPICA's New Window on the Cool Universe
宇宙航空研究開発機構特別資料
VolumeJAXA-SP-17-010E
Start page49
End page51
Publication date2018-03-09
Languageeng
AbstractWe report on our recent results about the IR properties of FUV selected samples from the COSMOS field at z= 4, 3 and 1.5. The measurements are obtained by stacking at 250, 250 and 500 microns in the Her schel/SPIRE images. Almost no galaxy is detected individually and the stacking is performed as a function of FUV luminosity and stellar mass. We are able to reconstruct the average relation between dust attenuation and stellar mass and the so-called main sequence (star formation rate-stellar mass relation) of galaxies. Implications on star formation histories of galaxies are discussed. We investigate the future impact of SAFARI/SPICA in the study of distant FUV selected galaxies.
DescriptionMeeting Information: SPICA Science Conference from Exoplanets to Distant Galaxies: SPICA's New Window on the Cool Universe (June 18-21, 2013. Ito Hall, the University of Tokyo), Bunkyou-ku, Tokyo, Japan
Physical characteristics: Original contains color illustrations
形態: カラー図版あり
Document TypeConference Paper
JAXA Category特別資料
NASA Subject CategoryAstronomy
ISSN(online)2433-2232
SHI-NOAA1730027009
Report NoJAXA-SP-17-010E
URIhttps://repository.exst.jaxa.jp/dspace/handle/a-is/877802


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