Homogeneous Photometry. III. A Star Catalog for the Open Cluster NGC 6791

139 citations recorded by the source corpus.

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

MESA ISOCHRONES AND STELLAR TRACKS (MIST). I. SOLAR-SCALED MODELS (2016, unknown): “The Brogaard et al. (2012) sample consists of photometry from Stetson et al. (2003) that has been empirically corrected for differential reddening effects.”
The age of the oldest Open Clusters (2003, methodology): “We used E(B − V ) = 0.15±0.02 (Twarog et al. 1997), [Fe/H]=0.40±0.06 (G00), and employed the same field dwarf sample and method as for the other OCs; the cluster MS CMD is from the new photometry by Stetson et al. (2003).”
REDDENING AND EXTINCTION TOWARD THE GALACTIC BULGE FROM OGLE-III: THE INNER MILKY WAY'S RV ∼ 2.5 EXTINCTION CURVE (2012, methodology): “For the open cluster NGC 6791, we use the photometric catalog of Stetson et al. (2003), which was updated for the work of Brogaard et al. (2012) and now includes corrections for differential reddening.”
The Dartmouth Stellar Evolution Database (2008, methodology): “Carney et al. (2005) combined JHK photometry of NGC 6791 with optical data from Stetson et al. (2003).”
A REVISED EFFECTIVE TEMPERATURE SCALE FOR THE KEPLER INPUT CATALOG (2011, methodology): “To identify blended sources in the KIC, we further performed a test using the separation index (Stetson et al. 2003), which is defined as the logarithmic ratio of the surface brightness of a star to the summed brightness from all neighboring stars (see also An et al. 2008).”