Fundamental Transformation Equations Between the u'g'r'i'z' and UBVRCI_C Filter Systems

Details Fundamental Transformation Equations Between the u'g'r'i'z' and UBVRCI_C Filter Systems Fundamental Transformation Equations Between the u'g'r'i'z' and UBVRCI_C Filter Systems

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aas...207.2803a&link_type=abstract

American Astronomical Society Meeting 207, #28.03; Bulletin of the American Astronomical Society, Vol. 37, p.1210

Astronomy and Astrophysics

Astronomy

Scientific paper

Rodgers et al. (2005) showed the UBVRCI_C to u'g'r'i'z' transformation equations are luminosity class dependent. That study developed transformation equations for luminosity class V (main sequence) stars using Landolt (1992) identified equatorial standards with spectroscopically confirmed luminosity classes. Here, we present new data for both luminosity class V and III bright standard stars with known metallicities. These data will be used to develop robust transformation equations for stars of these two luminosity classes.

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