A dataset provided by the European Space Agency

Name OT2_sserje01_2
Title THE HERSCHEL-AKARI NEP DEEP SURVEY: the cosmological history of stellar mass assembly and black hole accretion
URL

http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342239959&instrument_name=SPIRE&product_level=LEVEL0&compress=true

DOI https://doi.org/10.5270/esa-s5duvj7
Author serjeant, s.
Description We propose a far-IR and submm mapping survey of the premier AKARI deep field in the North Ecliptic Pole, in PACS-SPIRE parallel mode. This is the only major deep infrared field not yet covered by Herschel guaranteed or open time key projects. The outstanding and unparalleled continuous mid-IR photometric coverage from AKARI, far better than equivalent Spitzer surveys, enables a wide range of galaxy evolution diagnostics unachievable in any other survey field (including Herschel HerMES-PEP fields), by spanning the wavelengths of redshifted PAH and silicate features and the peak energy output of AGN dust tori. The investment by AKARI in the NEP represents virgul10 percent of the entire pointed observations available throughout the lifetime of AKARI. Our proposal remedies the remarkable omission from Herschel.s legacy surveys of the premier extragalactic deep field from another IR space telescope. We will simultaneously identify and find photometric redshifts for the Herschel point source population, make stacking analysis detections of the galaxies which dominate the submm extragalactic background light as a function of redshift, determine the bolometric power outputs of the galaxies that dominate the submm background, compare the UV-optical-mid-IR continuum-PAH-far-IR-submm-radio star formation rate estimator in the most comprehensive IR survey data set to date, and track the coupled stellar mass assembly and black hole accretion throughout most of the history of the Universe. In OT1 the HOTAC concluded The science output from the proposed survey will be outstanding [.] The panel was convinced that these observations should be done but it since became clear that priority 2 time is very unlikely to be executed, so we request reclassification to priority 1.
Publication The Radio-Far Infrared Correlation in the NEP Deep Field . Barrufet Laia et al. . Publications of The Korean Astronomical Society, vol. 32, issue 1, pp. 267-269 . 32 . 10.5303/PKAS.2017.32.1.267 . 2017PKAS...32..267B ,
A Tale of Two Feedbacks: Star Formation in the Host Galaxies of Radio AGNs . Karouzos Marios et al. . The Astrophysical Journal, Volume 784, Issue 2, article id. 137, 23 pp. (2014). . 784 . 10.1088/0004-637X/784/2/137 . 2014ApJ...784..137K ,
gzK-colour-selected star-forming galaxies in the AKARI NEP-Deep Field . Seo Hyunjong et al. . Monthly Notices of the Royal Astronomical Society . null . null . 2021MNRAS.502.1933S ,
Multiwavelength properties of 850-μm selected sources from the North Ecliptic Pole SCUBA-2 survey . Shim Hyunjin et al. . Monthly Notices of the Royal Astronomical Society . null . null . 2022MNRAS.514.2915S ,
Infrared colours and spectral energy distributions of hard X-ray selected obscured and Compton-thick active galactic nuclei . Kilerci Eser Ece et al. . Monthly Notices of the Royal Astronomical Society . null . null . 2020MNRAS.494.5793K ,
A high redshift population of galaxies at the North Ecliptic Pole. Unveiling the main sequence of dusty galaxies . Barrufet L. et al. . Astronomy and Astrophysics . null . null . 2020A&A...641A.129B ,
AKARI NEP field: Point source catalogs from GALEX and Herschel observations and selection of candidate lensed sub-millimeter galaxies . Burgarella Denis et al. . Publications of the Astronomical Society of Japan, Volume 71, Issue 1, id.12 . 71 . 10.1093/pasj/psy134 . 2019PASJ...71...12B ,
The Herschel-PACS North Ecliptic Pole Survey...
Instrument SPIRE_SpirePhoto_large
Temporal Coverage 2012-03-01T20:50:59Z/2012-03-02T02:58:22Z
Version SPG v14.1.0
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/h®erschel/
Date Published 2012-09-01T20:50:59Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2012, OT2_sserje01_2, SPG v14.1.0. https://doi.org/10.5270/esa-s5duvj7