Additional values from the SPARV pipeline (ravedr6.dr6_sparv_aux)

Description

The SPARV pipeline"s additional output is provided in this tab. This additional information such as stellar parameters from matching templates is provided. These data should, if at all, be used with care for further astrophysical applications, as they are subject to complicated biases (see DR4, Section 4.4)

Attribution

Funding for Rave has been provided by:

• the Leibniz Institute for Astrophysics Potsdam (AIP);
• the Australian Astronomical Observatory;
• the Australian National University;
• the Australian Research Council;
• the French National Research Agency;
• the German Research Foundation (SPP 1177 and SFB 881);
• the European Research Council (ERC-StG 240271 Galactica);
• the Istituto Nazionale di Astrofisica at Padova;
• the Johns Hopkins University;
• the National Science Foundation of the USA (AST-0908326);
• the W. M. Keck foundation;
• the Macquarie University;
• the Netherlands Research School for Astronomy;
• the Natural Sciences and Engineering Research Council of Canada;
• the Slovenian Research Agency;
• the Swiss National Science Foundation;
• the Science & Technology FacilitiesCouncil of the UK;
• Opticon;
• Strasbourg Observatory;
• the Universities of Basel, Groningen, Heidelberg and Sydney.

This work has made use of data from the European Space Agency (ESA) mission Gaia (https://www.cosmos.esa.int/gaia), processed by the GaiaData 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.

Columns