A dataset provided by the European Space Agency

Name DDT_mbayliss_1
Title Far-IR dust properties of a star-bursting ULIRG at the center of the most luminous and strongest cooling flow galaxy known
URL

http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342245182&instrument_name=PACS&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342245183&instrument_name=PACS&product_level=LEVEL0&compress=true

DOI https://doi.org/10.5270/esa-wwlkvib
Author bayliss, m.
Description We proposed PACS photometry of SPT-CLJ2344-4242. It is the strongest cool core (CC) cluster known and is the only CC to be caught in a rare phase of the CC life-cycle when it is forming stars at a rate comparable to the inferred X-ray cooling rate.
Publication A massive, cooling-flow-induced starburst in the core of a luminous cluster of galaxies . McDonald M. et al. . Nature, Volume 488, Issue 7411, pp. 349-352 (2012). . 488 . 10.1038\/nature11379 . 2012Natur.488..349M ,
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 ,
New XMM-Newton observation of the Phoenix cluster: properties of the cool core . Tozzi P. et al. . Astronomy & Astrophysics, Volume 580, id.A6, 12 pp. . 580 . 10.1051\/0004-6361\/201525745 . 2015A&A...580A...6T ,
BAT AGN Spectroscopic Survey. XI. The Covering Factor of Dust and Gas in Swift/BAT Active Galactic Nuclei . Ichikawa Kohei et al. . The Astrophysical Journal, Volume 870, Issue 1, article id. 31, 16 pp. (2019). . 870 . 10.3847\/1538-4357\/aaef8f . 2019ApJ...870...31I ,
Instrument PACS_PacsPhoto_largeScan
Temporal Coverage 2012-05-01T04:30:00Z/2012-05-01T04:49:37Z
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/h®erschel/
Date Published 2012-11-01T04:40:20Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, bayliss, m., 2012, DDT_mbayliss_1, SPG v14.2.0, European Space Agency, https://doi.org/10.5270/esa-wwlkvib