A dataset provided by the European Space Agency

Name OT2_lyan_4
Title Investigate the Physical Nature of An Extraordinarily Far-IR bright Galaxy Discovered by WISE


DOI 10.5270/esa-sc11oyo
Author yan, l.
Description We request a total of 5.3 hours of Herschel PACS and SPIRE time to investigate the physical nature of an extraordinarily far-IR bright system discovered by the WISE data. This object was first selected to have an extremely red mid-IR SED, very bright at 22micron (38mJy) and not detected at WISE 3.4 and 4.5 micron. At the WISE 12micron position, we found it has IRAS far-IR emission, (600+-59)mJy & (855+-170)mJy at 60 and 100 micron respectively (2. beam). A small 350 micron map, taken with the CSO SHARCII under an exceptionally good weather condition, has detected a 32mJy source at the WISE position. The large discrepancy between fluxes at IRAS 100 micron and CSO 350 micron is intriguing. We propose to clarify the nature of this system --- whether a single or a group of far-IR bright sources --- by utilizing Herschel.s high spatial resolution and fast mapping speed. The Herschel photometry, together with the Keck spectra, will allow us to determine the full IR SEDs and the physical parameters such as IR luminositie, SFR and star formation efficiecy. In addition, the deep Keck LRIS spectrum of the galaxy closest to the WISE 12 micron position has found an emission line object at redshift of 0.593, and the Keck NIRC2 K-band Adaptive Optics image shows an extended, disk like galaxy. At z=0.593, the strong IRAS far-IR emission implies very high L(FIR), in the range of (2.1-10)e+12Lsun, with the lower limit set by considering only 1-4 of the IRAS fluxes. We propose to obtain SPIRE FTS spectroscopy to measure [CII]158um line. At this redshift, this line can only be observed by Herschel, and is outside the ALMA wavelength window. With the measured [CII]-to-L(FIR) ratio, we can constraint the molecular gas mass of Source A by utilizing the correlation between [CII]-to-L(FIR) and L(FIR)-M(H2). Even with null detection, our observation will provide meaningful constraint on the ISM properties of this ULIRG.
Instrument SPIRE_SpireSpectrometer_, PACS_PacsPhoto_largeScan, SPIRE_SpirePhoto_small
Temporal Coverage 2012-06-10T15:26:41Z/2013-01-12T20:55:00Z
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 ┬Ám range, bridging the gap between earlier infrared space missions and groundbased facilities.
Creator Contact https://support.cosmos.esa.int/herschel/
Date Published 2013-07-12T16:20:44Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2013-07-12T16:20:44Z, OT2_lyan_4, SPG v14.2.0. https://doi.org/10.5270/esa-sc11oyo