A dataset provided by the European Space Agency

Name OT1_ttakagi_1
Title A deep PACS survey of AKARI-Deep field south: Revealing the connection between AGN and star formation
URL

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DOI 10.5270/esa-dhi5w7l
Author takagi, t.
Description We propose a deep PACS imaging survey of a prestigious far-IR survey field, AKARI-Deep field south, which has the lowest cirrus background in the sky and has been observed with most of the major IR and submm telescopes, such as AKARI, Spitzer-MIPS, BLAST and Herschel-HerMES, covering 7-12 deg^2. We also conducted one of the widest and deepest millimetre survey using ASTE-AzTEC within this field, covering 0.25 deg^2. Although there are many (sub)mm survey fields in different parts of the sky, ADF-S has a unique data set from AKARI-IRC at 2.4, 3.2, 4.1, 7, 11, 15 micron, i.e. filling the wavelength gap between Spitzer-IRAC 8 micron and MIPS 24 micron. We utilize this comprehensive mid-IR coverage to identify obscured AGNs and derive the bolometric AGN luminosity, based on the type-independent X-ray-to-mid-IR luminosity relation. PACS photometry is necessary to derive accurate star formation rate (SFR) in starburst-AGN composite system. We investigate the relative importance of AGN in SMGs and other mid-IR selected ULIRGs, as a function of SFR, stellar mass, and redshift. Ultimately, we will determine the role of AGN in galaxy formation and the regulation mechanism for co-evolution of stellar mass assembly and central black hole. Also, deep PACS images allow us to identify millimeter-selected SMGs at very high redshifts, which will be prime targets of ALMA.
Publication The Spitzer-IRAC-MIPS Extragalactic Survey (SIMES). II. Enhanced Nuclear Accretion Rate in Galaxy Groups at z ∼ 0.2 . Baronchelli I. et al. . The Astrophysical Journal, Volume 857, Issue 1, article id. 64, 23 pp. (2018). . 857 . 10.3847\/1538-4357\/aab78b . 2018ApJ...857...64B ,
Instrument PACS_PacsPhoto_largeScan
Temporal Coverage 2011-10-04T01:39:49Z/2012-03-14T14:19:14Z
Version SPG v14.2.0
Mission Description Herschel was launched on 14 May 2009! It is the fourth 'cornerstone' mission in the ESA science programme. With a 3.5 m Cassegrain telescope it is the largest space telescope ever launched. It is performing photometry and spectroscopy in approximately the 55-671 µm range, bridging the gap between earlier infrared space missions and groundbased facilities.
Creator Contact https://support.cosmos.esa.int/herschel/
Date Published 2012-09-14T12:21:31Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2012-09-14T12:21:31Z, OT1_ttakagi_1, SPG v14.2.0. https://doi.org/10.5270/esa-dhi5w7l