/ftp/cats/III/283



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III/283                 RAVE 6th data release                 (Steinmetz+, 2020)
The following files can be converted to FITS (extension .fit or fit.gz)
	master.dat aux.dat obs.dat class.dat repeats.dat madera.dat irfm.dat
	bdasp.dat gaugmad.dat gaugbda.dat cdrmad.dat cdrbdasp.dat
	orbits.dat orbedr3.dat xgaia2.dat xgaiae3.dat xmatch.dat spectra.dat
	fields.dat seismic.dat cnn.dat
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Query from: http://vizier.cds.unistra.fr/viz-bin/VizieR?-source=III/283
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drwxr-xr-x 259 cats archive 8192 Dec 5 19:00 [Up] drwxr-xr-x 6 cats archive 4096 Jan 13 2023 [TAR file] -rw-r--r-- 1 cats archive 681 Dec 19 2022 .message -r--r--r-- 1 cats archive 68489 Oct 21 2021 ReadMe -rw-r--r-- 1 cats archive 2850 Oct 21 2021 +footg5.gif -rw-r--r-- 1 cats archive 50942 Oct 21 2021 +footg8.gif -r--r--r-- 1 cats archive 22619832 Sep 22 2021 aux.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 60283677 Sep 23 2021 bdasp.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 14727219 Sep 23 2021 cdrbdasp.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 14646247 Sep 23 2021 cdrmad.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 7159698 Sep 23 2021 class.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 55775890 Oct 1 2021 cnn.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 302408 Sep 30 2021 fields.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 22907698 Sep 23 2021 gaugbda.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 23484025 Sep 23 2021 gaugmad.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html] drwxr-xr-x 2 cats archive 25276416 Sep 29 2021 img -r--r--r-- 1 cats archive 7168826 Sep 23 2021 irfm.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 19087022 Sep 23 2021 madera.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 25466646 Oct 21 2021 master.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html] -rw-r--r-- 1 cats archive 81905146 Oct 21 2021 master_temp -r--r--r-- 1 cats archive 24110271 Oct 1 2021 obs.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 239005656 Sep 27 2021 orbedr3.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 234882111 Sep 27 2021 orbits.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 5414473 Oct 1 2021 seismic.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html] drwxr-xr-x 2 cats archive 25149440 Sep 29 2021 sp -r--r--r-- 1 cats archive 5781247 Oct 1 2021 spectra.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 95298651 Sep 27 2021 xgaia2.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 66809071 Sep 27 2021 xgaiae3.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 36819626 Sep 28 2021 xmatch.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe : III/283 RAVE 6th data release (Steinmetz+, 2020) ================================================================================ The sixth data release of the Radial Velocity Experiment (RAVE). I. Survey description, spectra, and radial velocities. II. Stellar atmospheric parameters, chemical abundances, and distances. Steinmetz M., Matijevic G., Enke H., Zwitter T., Guiglion G., McMillan P.J., Kordopatis G., Valentini M., Chiappini C., Casagrande L., Wojno J., Anguiano B., Bienayme O., Bijaoui A., Binney J., Burton D., Cass P., de Laverny P., Fiegert K., Freeman K., Fulbright J.P., Gibson B.K., Gilmore G., Grebel E.K., Helmi A., Kunder A., Munari U., Navarro J.F., Parker Q., Ruchti G.R., Recio-Blanco A., Reid W., Seabroke G.M., Siviero A., Siebert A., Stupar M., Watson F., Williams M.E.K., Wyse R.F.G., Anders F., Antoja T., Birko D., Bland-Hawthorn J., Bossini D., Garcia R.A., Carrillo I., Chaplin W.J., Elsworth Y., Famaey B., Gerhard O., Jofre P., Just A., Mathur S., Miglio A., Minchev I., Monari G., Mosser B., Ritter A., Rodrigues T.S., Scholz R.-D., Sharma S., Sysoliatina K. (The Rave collaboration) <Astron. J., 160, 82, 83 (2020) > =2020yCat.3283....0S =2020AJ....160...82S +2020AJ....160...83S ================================================================================ ADC_Keywords: Surveys ; Radial velocities; Milky Way; Stars, fundamental ; Photometry Keywords: Stellar populations - Galaxy stellar content - Milky Way Galaxy - Milky Way dynamics - Surveys - Sky surveys - Catalogs Abstract: The Radial Velocity Experiment (RAVE) is a magnitude-limited (9<I<12) spectroscopic survey of Galactic stars randomly selected in Earth's southern hemisphere. The RAVE medium-resolution spectra (R 7500) cover the Ca-triplet region (8410-8795AA). The sixth and final data release (DR6) is based on 518387 observations of 451783 unique stars. RAVE observations were taken between 2003 April 12 and 2013 April 4. Here we present the genesis, setup, and data reduction of RAVE as well as wavelength-calibrated and flux-normalized spectra and error spectra for all observations in RAVE DR6. Furthermore, we present derived spectral classification and radial velocities for the RAVE targets, complemented by cross-matches with Gaia DR2 and other relevant catalogs. A comparison between internal error estimates, variances derived from stars with more than one observing epoch, and a comparison with radial velocities of Gaia DR2 reveals consistently that 68% of the objects have a velocity accuracy better than 1.4km/s, while 95% of the objects have radial velocities better than 4.0km/s. We present part 2 of the sixth and final Data Release (DR6) of the Radial Velocity Experiment (RAVE), a magnitude-limited (9<I<12) spectroscopic survey of Galactic stars randomly selected in Earth's southern hemisphere. The RAVE medium-resolution spectra (R 7500) cover the Ca triplet region (8410-8795AA) and span the complete time frame from the start of RAVE observations on 2003 April 12 to their completion on 2013 April 4. In the second of two publications, we present the data products derived from 518,387 observations of 451,783 unique stars using a suite of advanced reduction pipelines focusing on stellar atmospheric parameters, in particular purely spectroscopically derived stellar atmospheric parameters (Teff, logg, and the overall metallicity), enhanced stellar atmospheric parameters inferred via a Bayesian pipeline using Gaia DR2 astrometric priors, and asteroseismically calibrated stellar atmospheric parameters for giant stars based on asteroseismic observations for 699 K2 stars. In addition, we provide abundances of the elements Fe, Al, and Ni, as well as an overall [alpha/Fe] ratio obtained using a new pipeline based on the GAUGUIN optimization method that is able to deal with variable signal-to-noise ratios. The RAVE DR6 catalogs are cross-matched with relevant astrometric and photometric catalogs, and are complemented by orbital parameters and effective temperatures based on the infrared flux method. Description: The Radial Velocity Experiment (RAVE) is a magnitude-limited (9<I<12) spectroscopic survey of Galactic stars randomly selected in the southern hemisphere. The RAVE medium resolution spectra (R 7500) cover the Ca-triplet region (8410-8795AA) and span the complete time frame from the start of RAVE observations on 12 April 2003 to their completion on 4 April 2013. Wavelength-calibrated and flux-normalized spectra for 518387 observations of 451783 unique stars are presented. The final data release 6 consists of spectra, error spectra, spectral classification, derived radial velocities, and cross matches with other relevant catalogs. Further data products are using a suite of advanced reduction pipelines focusing on stellar atmospheric parameters, in particular purely spectroscopically derived stellar atmospheric parameters (Teff, logg, and the overall metallicity), enhanced stellar parameters inferred via a Bayesian pipeline using Gaia DR2 astrometric priors, and asteroseismically calibrated stellar parameters for giant stars based on asteroseismic observations for 699 K2 stars. In addition, we provide abundances of the elements Fe, Al, and Ni, as well as an overall [alpha/Fe] ratio obtained using a new pipeline based on the GAUGUIN optimization method that is able to deal with variable signal-to-noise ratios. The Rave DR6 catalogs are cross matched with relevant astrometric and photometric catalogs, and are complemented by orbital parameters and effective temperatures based on the infrared flux method. Acknowledging Rave data in publications: 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 (http://www.cosmos.esa.int/gaia), processed by the GaiaData Processing and Analysis Consortium (DPAC, http://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.