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 | http://adsabs.harvard.edu/abs/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 | http://adsabs.harvard.edu/abs/2015A%26A...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 | http://adsabs.harvard.edu/abs/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
Last Update 2025-01-24
Keywords Herschel, HSC, submillimetre, far-infrared, HIFI, PACS, SPIRE
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, bayliss et al., 2012, 'Far-IR dust properties of a star-bursting ULIRG at the center of the most luminous and strongest cooling flow galaxy known', SPG v14.2.0, European Space Agency, https://doi.org/10.5270/esa-wwlkvib