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Landolt BV and Sloan g’r’i’ photometry of 358,963 RAVE stars Ulisse Munari and Arne Henden
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Landolt BV and Sloan gri photometry of 358,963 RAVE stars Ulisse Munari and Arne Henden.

Mar 27, 2015

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Page 1: Landolt BV and Sloan gri photometry of 358,963 RAVE stars Ulisse Munari and Arne Henden.

Landolt BV and Sloan g’r’i’

photometry of 358,963 RAVE stars

Ulisse Munari and Arne Henden

Page 2: Landolt BV and Sloan gri photometry of 358,963 RAVE stars Ulisse Munari and Arne Henden.

239 ,102 RAVE stars have a Tycho-2 counterpart

377 ,807 stars have a match

in DENIS

Page 3: Landolt BV and Sloan gri photometry of 358,963 RAVE stars Ulisse Munari and Arne Henden.

399 ,443 RAVE stars have a2MASS counterpart

err(J)=0.023

err(H)=0.032

err(K)=0.026

Page 4: Landolt BV and Sloan gri photometry of 358,963 RAVE stars Ulisse Munari and Arne Henden.

G0 main sequence dwarfRAVE

to date, 358,963 RAVE stars have been observed by APASS on at least 2 distinct epochs in the Landolt B,V and Sloan g’r’i’ bands.

median of internal errors of the mean on RAVE stars:

0.013 0.011 0.012 0.013 0.018 mag

Page 5: Landolt BV and Sloan gri photometry of 358,963 RAVE stars Ulisse Munari and Arne Henden.

on average 3.7 epochs

target 6 epochs

Page 6: Landolt BV and Sloan gri photometry of 358,963 RAVE stars Ulisse Munari and Arne Henden.

median 0.274 arcsec

Page 7: Landolt BV and Sloan gri photometry of 358,963 RAVE stars Ulisse Munari and Arne Henden.

Landolt (1983, 1992) primary standards

Page 8: Landolt BV and Sloan gri photometry of 358,963 RAVE stars Ulisse Munari and Arne Henden.

Henden and Munari (2000, 2001, 2006) seconday Landolt standards

Page 9: Landolt BV and Sloan gri photometry of 358,963 RAVE stars Ulisse Munari and Arne Henden.

Smith et al. (2002) secondary SLOAN standards

Page 10: Landolt BV and Sloan gri photometry of 358,963 RAVE stars Ulisse Munari and Arne Henden.

Mermilloid (1992)

Page 11: Landolt BV and Sloan gri photometry of 358,963 RAVE stars Ulisse Munari and Arne Henden.

Hartman et al. (2008)

Page 12: Landolt BV and Sloan gri photometry of 358,963 RAVE stars Ulisse Munari and Arne Henden.
Page 13: Landolt BV and Sloan gri photometry of 358,963 RAVE stars Ulisse Munari and Arne Henden.
Page 14: Landolt BV and Sloan gri photometry of 358,963 RAVE stars Ulisse Munari and Arne Henden.
Page 15: Landolt BV and Sloan gri photometry of 358,963 RAVE stars Ulisse Munari and Arne Henden.
Page 16: Landolt BV and Sloan gri photometry of 358,963 RAVE stars Ulisse Munari and Arne Henden.
Page 17: Landolt BV and Sloan gri photometry of 358,963 RAVE stars Ulisse Munari and Arne Henden.

- BVgri support photometry from APASS now available for 358,963 RAVE stars (and counting)

- median value for the error of the means about 0.013 mag

- no offset/trend and rms=0.025 on Landolt/Sloan photometric standards, about the same as 2MASS JHKs data

- rms of derived photometric temperatures 250 K

- no significant offset with Greg/Jon spectroscopic temperatures from high res APO Echelle observations of 571 well distributed RAVE stars

SUMMARY

- extention toward V=7.5 stars started (essential for accessing the bulk of spectroscopic calibrators)

- inclusion of z’Y band will start soon

- pilot survey of 100 sq.deg in u’ band completed

- analysis of APASS data of PASTEL stars not yet completed but so far promising