A dataset provided by the European Space Agency

Name DDT_bgullber_1
Title Detecting CII emission in zvirgul2.3 lensed SMGs from the South Pole Telescope survey
URL

http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342265811&instrument_name=SPIRE&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342265812&instrument_name=SPIRE&product_level=LEVEL0&compress=true
DOI https://doi.org/10.5270/esa-i7up4t4
Author gullberg, b.
Description With ALMA cycle 0 time we have observed 26 sources selected from the South Pole Telescope (SPT) survey, which covers 2500 deg^2 of sky area. These SPT sources are strongly lensed and the sample includes two of the most distant submm galaxies at z=5.7. The results of these observations reveal an unbiased redshift distribution of our sources peaking at zvirgul 3.5.We have started a follow-up started to observe the CII line in these sources. Combined with low-J CO lines we have already found tentative evidence for evolutionary effects in the ISM properties of our sources. We here propose to observe three SPT sources at 2<z<2.5 which can only be observed with SPIRE/FTS to obtain critical observations in this redshift range, on the low-z side of our redshift distribution. This is our last chance to probe this redshift range in our sample, which is complete at 3<z<5.7. The predicted CII fluxes of our three targets are brighter than published results, ensuring the succes of this proposal and the legacy of Herschel in this field.
Publication
  • The nature of the C II emission in dusty star-forming galaxies from the SPT survey | Gullberg B. et al. | Monthly Notices of the Royal Astronomical Society Volume 449 Issue 3 p.2883-2900 | 449 | 10.1093\\/mnras\\/stv372 | 2015MNRAS.449.2883G | http://adsabs.harvard.edu/abs/2015MNRAS.449.2883G
  • Early Science with the Large Millimeter Telescope: CO and C II Emission in the z = 4.3 AzTEC J095942.9+022938 (COSMOS AzTEC-1) | Yun Min S. et al. | Monthly Notices of the Royal Astronomical Society Volume 454 Issue 4 p.3485-3499 | 454 | 10.1093\\/mnras\\/stv1963 | 2015MNRAS.454.3485Y | http://adsabs.harvard.edu/abs/2015MNRAS.454.3485Y
Instrument SPIRE_SpireSpectrometer_
Temporal Coverage 2013-03-02T18:26:16Z/2013-03-03T02:07:32Z
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 2013-09-02T22:18:20Z
Keywords Herschel, HSC, submillimetre, far-infrared, HIFI, PACS, SPIRE
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, gullberg et al., 2013, 'Detecting SQUARE_BRACKET_OPENCIISQUARE_BRACKET_CLOSE emission in zvirgul2.3 lensed SMGs from the South Pole Telescope survey', SPG v14.1.0, European Space Agency, https://doi.org/10.5270/esa-i7up4t4