A dataset provided by the European Space Agency

Name OT2_yshi_3
Title Extremely-metal poor galaxies: mapping dust emission
URL

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http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342255324&instrument_name=SPIRE&product_level=LEVEL0&compress=true
DOI https://doi.org/10.5270/esa-q4fbs1o
Author shi, y.
Description The understanding of the interstellar medium (ISM) and star formationin the low-metallicity environment is crucial to constrain formationof stars and galaxies of the first generation. The local extremelylow-metallicity galaxies (XMPGs) with Z
Publication
  • Spatially resolved dust emission of extremely metal-poor galaxies* | Zhou Luwenjia et al. | Monthly Notices of the Royal Astronomical Society Volume 458 Issue 1 p.772-780 | 458 | 10.1093/mnras/stw345 | 2016MNRAS.458..772Z | http://adsabs.harvard.edu/abs/2016MNRAS.458..772Z
  • Inefficient star formation in extremely metal poor galaxies | Shi Yong et al. | Nature Volume 514 Issue 7522 pp. 335-338 (2014). | 514 | 10.1038/nature13820 | 2014Natur.514..335S | http://adsabs.harvard.edu/abs/2014Natur.514..335S
Instrument PACS_PacsPhoto_largeScan, SPIRE_SpirePhoto_small
Temporal Coverage 2012-04-06T00:34:48Z/2012-11-19T05:55:03Z
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 2013-05-19T04:11:12Z
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, shi et al., 2013, 'Extremely-metal poor galaxies: mapping dust emission', SPG v14.2.0, European Space Agency, https://doi.org/10.5270/esa-q4fbs1o