Star Formation Rate Determinations

dc.creatorCalzetti, Daniela
dc.date2007-07-03
dc.date.accessioned2026-07-07T08:13:47Z
dc.date.available2026-07-07T08:13:47Z
dc.descriptionI review determinations of star formation rates (SFR) from the ultraviolet to the infrared, in the context of their use for galaxies and galaxy surveys. The mid-infrared SFR indicators have garnered interest in recent years thanks to the Spitzer capabilities and the opportunities offered by the upcoming Herschel Space Telescope. I discuss what we have learned in the mid-infrared from studies of local galaxies combining Spitzer with HST and other data.
dc.description12 pages, 4 figures; to appear in the Proceedings of the conference `Pathways through an Eclectic Universe', J.H. Knapen, T.J. Mahoney, and A. Vazdekis eds., ASP Conference Serries, 2007
dc.identifierhttps://arxiv.org/abs/0707.0467
dc.identifierhttp://arxiv.org/abs/0707.0467
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/132891
dc.subjectAstrophysics
dc.titleStar Formation Rate Determinations
dc.typetext

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