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- 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 GDS data, please cite :bibcode:`2015AN....336..590H`.3
- 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/2
- If you use public Gaia DR3 data in a paper, please take note of `ESAC's guide`_ on how to acknowledge and cite it. .. _ESAC's guide: https://gea.esac.esa.int/archive/documentation/GDR3/Miscellaneous/sec_credit_and_citation_instructions/2
- If you use this data, please cite Haschke, R., Grebel, E., Duffau, S., 2011: "New Optical Reddening Maps of the Large and Small Magellanic Clouds", AJ 141, 158, `2011AJ....141..158H <http://adsabs.harvard.edu/abs/2011AJ....141..158H>`_ The photometric data of the red clump is provided by the OGLE collaboration. Part of this research was supported by SFB 881 "The Milky Way System".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
- Please see http://www.sdss.org/collaboration/citing-sdss/ for the authors' requests on how to cite this material.1
- This data essentially is a mirror of http://www.astro.yale.edu/astrom/spm4cat/spm4.html. If you use it, please reference 2011AJ....142...15G.1
- This data is derived from public Gaia DR3 data. Please take note of `ESAC's guide`_ on how to acknowledge and cite Gaia results. .. _ESAC's guide: https://gea.esac.esa.int/archive/documentation/GDR3/Miscellaneous/sec_credit_and_citation_instructions/1
- This work has made use of data from the European Space Agency (ESA) mission `Gaia <https://www.cosmos.esa.int/gaia>`_, processed by the Gaia Data Processing and Analysis Consortium (`DPAC <https://www.cosmos.esa.int/web/gaia/dpac/consortium>`_). Funding for the DPAC has been provided by national institutions, in particular the institutions participating in the Gaia Multilateral Agreement.2
- All publications making use of the RAVE data should refer to the paper given in source.1
- If you use results obtained by this service, please cite the original publication (see source meta) and acknowlege: This work has made use of the sp_ace spectral analysis tool version 1.4.1
- If you use this atlas please cite the Asmus et al. work given under the "source" metadata item.2
- The UCAC4 release paper (in preparation) should be cited whenever UCAC data are utilized.1
- The data files were owned by Xinjiang Astronomical Observatory, and It's managed on a hierarchical basis, some of the data files are available for public download.1
- The data from XAO have been obtained with Xinjiang Nanshan 25M Radio Telescope. And all data are not in the public domain. If you want to use the data for your research, send a request to zhanghailong@xao.ac.cn.2
- The files were owned by FAST. And all data are not in the public domain.1
- This work has made use of data from the European Space Agency (ESA) mission `Gaia <https://www.cosmos.esa.int/gaia>`_, processed by the Gaia `Data Processing and Analysis Consortium (DPAC) <https://www.cosmos.esa.int/web/gaia/dpac/consortium>`_. Funding for the DPAC has been provided by national institutions, in particular the institutions participating in the Gaia Multilateral Agreement.1
- 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."1
- When publishing research making use of this tool, please acknowledge: "The TOSS service (http://dc.g-vo.org/TOSS) used for this paper was constructed as part of the activities of the German Astrophysical Virtual Observatory."1