A dataset provided by the European Space Agency

Name OT1_dmarrone_1
Title SPIRE Spectroscopy of the Brightest High-Redshift Submillimeter Galaxies
URL

http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342224208&instrument_name=PACS&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342224208&instrument_name=SPIRE&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342224209&instrument_name=SPIRE&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342224209&instrument_name=PACS&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342231989&instrument_name=SPIRE&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342231989&instrument_name=PACS&product_level=LEVEL0&compress=true
DOI https://doi.org/10.5270/esa-s6d9wie
Author marrone, d.
Description The South Pole Telescope has conducted a large survey of the southern sky atmillimeter wavelengths and discovered a population of high-redshiftstrongly-lensed dusty star forming galaxies. Both the lensing and thelong wavelength selection biases these sources to the highest redshiftand their apparent luminosity makes them the most best possiblecandidates for SPIRE FTS spectroscopy. By combining the uniquecapabilities of SPT as a survey machine and Herschel as a followupspectroscopy machine, we propose to obtain spectra for five of thebrightest lensed sources in the sky. These observations will open anew astrophysical window into the study of young star forminggalaxies. The ratios of far-IR lines will provide ground-breakingphysical information about this earliest stage of galaxy evolution,including the best measures of how star formation is proceeding, dustemission and absorption properties, the detailed physics of the ISM,and also the quantitative contribution of the emission that comes fromblack hole accretion in an obscured AGN for these high redshiftsources.
Publication
  • SPT 0538-50: Physical Conditions in the Interstellar Medium of a Strongly Lensed Dusty Star-forming Galaxy at z = 2.8 | Bothwell M. S. et al. | The Astrophysical Journal Volume 779 Issue 1 article id. 67 15 pp. (2013). | 779 | 10.1088\\/0004-637X\\/779\\/1\\/67 | 2013ApJ...779...67B | http://adsabs.harvard.edu/abs/2013ApJ...779...67B
  • Search for candidate strongly lensed dusty galaxies in the Planck satellite catalogues | Trombetti T. et al. | Astronomy and Astrophysics | null | null | 2021A&A...653A.151T |
  • Stellar Masses and Star Formation Rates of Lensed, Dusty, Star-forming Galaxies from the SPT Survey | Ma Jingzhe et al. | The Astrophysical Journal Volume 812 Issue 1 article id. 88 16 pp. (2015). | 812 | 10.1088\\/0004-637X\\/812\\/1\\/88 | 2015ApJ...812...88M | http://adsabs.harvard.edu/abs/2015ApJ...812...88M
Instrument SPIRE_SpireSpectrometer_, PACS_PacsPhoto_largeScan
Temporal Coverage 2011-07-14T23:28:44Z/2011-11-08T11:17:38Z
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 2012-05-08T07:28:26Z
Keywords Herschel, HSC, submillimetre, far-infrared, HIFI, PACS, SPIRE
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, marrone et al., 2012, 'SPIRE Spectroscopy of the Brightest High-Redshift Submillimeter Galaxies', SPG v14.2.0, European Space Agency, https://doi.org/10.5270/esa-s6d9wie