The 2-850 micron SED of starforming galaxies

Simple item page
dc.creatorSajina, Anna
dc.creatorScott, Douglas
dc.creatorDennefeld, Michel
dc.creatorDole, Herve
dc.creatorLacy, Mark
dc.creatorLagache, Guilaine
dc.date2004-12-15
dc.date.accessioned2026-07-07T02:16:18Z
dc.date.available2026-07-07T02:16:18Z
dc.descriptionWe present preliminary results on a study of the 2--850 micron SEDs of a sample of 30 FIRBACK galaxies selected at 170 micron. These sources are representative of the brightest ~10% of the Cosmic Infrared Background. They are a mixture of mostly local (z<~0.3) starforming galaxies, and a tail of ULIGs that extend up to z~1, and are likely to be a similar population to faint SCUBA sources. We use archival Spitzer IRAC and MIPS data to extend the spectral coverage to the mid-IR regime, resulting in an unprecended (for this redshift range) census of their infrared SEDs. This allows us to study in far greater detail this important population linking the near-IR stellar emission with PAH and thermal dust emission. We do this using a Markov Chain Monte Carlo method, which easily allows for the inclusion of ~6 free parameters, as well as an estimate of parameter uncertainties and correlations.
dc.description5 pages, 3 figures. Proceeding for the conference "Starbursts: From 30 Doradus to Lyman Break Galaxies", held in Cambridge (UK) in September, 2004
dc.identifierhttps://arxiv.org/abs/astro-ph/0412394
dc.identifierhttp://arxiv.org/abs/astro-ph/0412394
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/8736
dc.subjectAstrophysics
dc.titleThe 2-850 micron SED of starforming galaxies
dc.typetext

Files

Collections

arXiv