- ID:
- ivo://org.gavo.dc/zcosmos/q/ssa
- Title:
- zCosmos Bright Spectroscopic Observations DR2
- Short Name:
- zCosmos SSAP
- Date:
- 23 Mar 2022 13:13:07
- Publisher:
- The GAVO DC team
- Description:
- The zCOSMOS redshift survey used 600h on the VIMOS spectrograph spread over five observing seasons (2005-2009) to obtain spectra of about 20,000 galaxies selected to have Iab < 22.5 across the full 1.7 deg2 of the COSMOS field. This part, "zCOSMOS-bright", was designed to yield a high and fairly uniform sampling rate (about 70%), with a high success rate in measuring redshifts (approaching 100% at 0.5 < z < 0.8), and with sufficient velocity accuracy (about 100 km/s) to efficiently map the environments of galaxies down to the scale of galaxy groups out to redshifts z ~ 1.
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- WFAU, Institute for Astronomy, University of Edinburgh50
- The GAVO DC team28
- The CeSAM VO team15
- Stellar Department of Astronomical Institute of the Academy of Sciences of the Czech Republic10
- Centro de Estudios de Física del Cosmos de Aragón (CEFCA)4
- Mullard Space Science Laboratory4
- Paris Astronomical Data Centre4
- Leibniz Institute for Astrophysics Potsdam (AIP)3
- INAF2
- The staff at the ArVO Data Center2
- Copyright © 2015-2023 Javalambre Photometric Local Universe Survey. All Rights Reserved.3
- If you use GDS data, please cite :bibcode:`2015AN....336..590H`.2
- When publishing research making use of this service, please acknowledge: "The TheoSSA service (http://dc.g-vo.org/theossa) used to retrieve theoretical spectra for this paper was constructed as part of the activities of the German Astrophysical Virtual Observatory."2
- Guoshoujing Telescope (the Large Sky Area Multi-Object Fiber Spectroscopic Telescope LAMOST) is a National Major Scientific Project built by the Chinese Academy of Sciences. Funding for the project has been provided by the National Development and Reform Commission. LAMOST is operated and managed by the National Astronomical Observatories, Chinese Academy of Sciences. Please also see the `LAMOST Data Policy`_. .. _LAMOST Data Policy: http://dr.lamost.org/ucenter/doc/lssdp2
- If you use this data, please acknowledge: "This research made use of Flash/Heros data served through the GAVO data center". Thanks.2
- CALIFA asks you to acknowledge: "This study uses data provided by the Calar Alto Legacy Integral Field Area (CALIFA) survey (http://califa.caha.es/)." "Based on observations collected at the Centro Astronómico Hispano Alemán (CAHA) at Calar Alto, operated jointly by the Max-Planck-Institut fűr Astronomie and the Instituto de Astrofísica de Andalucía (CSIC)." and to cite both of :bibcode:`2014A&A...569A...1W` and :bibcode:`2012A&A...538A...8S`1
- If you use public Gaia DR2 data in a paper, please take note of `ESAC's guide`_ on how to acknowledge and cite it. .. _ESAC's guide: http://gea.esac.esa.int/archive/documentation/GDR2/Miscellaneous/sec_credit_and_citation_instructions/1
- If you use this data, please reference Kaufer, A., et al: Commissioning FEROS, the new high-resolution spectrograph at La-Silla, :bibcode:`1999Msngr..95....8K`.1
- Copyright © 2018-2023 Javalambre Physics of the Accelerating Universe Astrophysical Survey. All Rights Reserved.1
- Data in this service is licensed under the `Creative Commons Attribution 4.0 License <http://creativecommons.org/licenses/by/4.0/>`_ .. image:: /static/img/ccby.png :alt: [CC-BY] 1
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