-
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 database of lightmeter measurements is made available under the Open
Database License: http://opendatacommons.org/licenses/odbl/1.0/.
Any rights
in individual contents of the database are licensed under the Database
Contents License: http://opendatacommons.org/licenses/dbcl/1.0/1
-
katkat data 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]
The individual catalogs may have other
licensing or copyright schemes, but in general a sound citation
practice should be all right -- even more so since most of the
individual authors are either dead or retired.1
- 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
- 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 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 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
- ARIHIP 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
- Any problems encountered while accessing the data, please contact
zhanghailong@xao.ac.cn. Thanks.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
- H.E.S.S. collaboration, 2018.
The data and documentation is publicly released by the H.E.S.S.
collaboration as a contribution to the ongoing efforts to define a
common open format for data level 3 of imaging atmospheric Cherenkov
telescopes (IACTs) and IACT open-source science tool development, to
enlarge the community involved in IACT data analysis.
No scientific publications may be derived from the data. Using the
data for new claims about the astrophysical sources is not permitted.
When using this data, please include the following attribution:
"This work made use of data from the H.E.S.S. DL3 public test data
release 1 (HESS DL3 DR1, H.E.S.S. collaboration, 2018)".
Alternatively, use the following shorter version, e.g. for
presentations:
"HESS DL3 DR1, H.E.S.S. collaboration".
These terms of use must be included in all copies in full or part of
the data.1
- If this table has been useful to you, please acknowledge: This
research has benefitted from the M, L, and T dwarf compendium housed
at DwarfArchives.org and maintained by Chris Gelino, Davy Kirkpatrick,
and Adam Burgasser.1
- If you use
this data, please
acknowledge: "This work made use of the HDAP which was produced at
Landessternwarte Heidelberg-Königstuhl under grant No. 00.071.2005
of the Klaus-Tschira-Foundation."
The data in this service was calibrated using Astrometry.net,
:bibcode:`2010AJ....139.1782L`.1
- If you use the data or software distributed here, please reference
2012MNRAS.424.2316P. This research was funded in part by SFB 881 "The
Milky Way Galaxy".1