VI photometry and spectroscopy in h+{chi} Per (Currie+, 2010)

Details VI photometry and spectroscopy in h+{chi} Per (Currie+, 2010) VI photometry and spectroscopy in h+{chi} Per (Currie+, 2010)

Apr 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010ycat..21860191c&link_type=abstract

VizieR On-line Data Catalog: J/ApJS/186/191. Originally published in: 2010ApJS..186..191C

Physics

Associations: Stellar, Photometry: Vri, Spectra: Infrared Spectral Types, Clusters: Open

Scientific paper

Optical VI photometry of h and {chi} Persei were taken with the Mosaic Imager at the 4m Mayall telescope at the Kitt Peak National Observatory on 2006 October 13-16 and 27-30. We acquired low-resolution optical spectroscopy of Two Micron All Sky Survey (2MASS)-detected stars within 1deg2 of the cluster centers. For faint stars, we used the multiobject, fiber-fed spectrograph Hectospec on the 6.5m MMT. Brighter stars were observed with the fiber-fed spectrograph Hydra on the 3.5m WIYN telescope at Kitt Peak National Observatory and single-slit FAST spectrograph on the 1.5m Tillinghast telescope at the Fred Lawrence Whipple Observatory.
(4 data files).

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