Infrared Values (ravedr6.dr6_irfm)
The table has 517055 rows, 6 columns.
dr6_irfm is a table of stellar atmospheric parameters as derived by pipeline IRFM
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; and 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.
|rave_obs_id||char||meta.id||Unique Identifier for RAVE objects, Observation Date, Fieldname, Fibernumber|
|teff_irfm||double||phys.temperature.effective||K||Effective temperature from infrared flux method|
|K||Error of effective temperature from infrared flux method|
|rad_irfm||double||phys.angSize||mas||Angular diameter from infrared flux method|
|mas||Error of angular diameter from infrared flux method|
|method_irfm||char||meta.flag||Indicator of the method for deriving the given values|