I am currently studying magnetic interactions between young stars and their surrounding disks. Theories of low-mass star formation suggest these interactions govern the physics of mass accretion and angular momentum transfer in the youngest stars. To study this complex and time-dependent phenomenon, I analyze photometry and spectroscopy at wavelengths stretching from visual light to the radio, using dedicated observations in concert with data from large survey projects.
I also study low-mass stars at later ages; I am carrying out a census of stars in the local galactic neighborhood, and tracing the properties and evolution of stellar magnetic fields over time. I am currently preparing a new description of my research program, but a slightly outdated (almost two years old!) copy of my research statement is still available.
PDF Version |PS Version
(Last update: Aug. 2007)
Covey, K. R., Ivezic, Z., et al. 2007 (18 total authors), Stellar SEDs from 0.3-2.5 Microns: Tracing the Stellar Locus and Searching for Color Outliers in SDSS and 2MASS, Astronomical Journal, in press
ADS | astro-ph | full resolution PDF | full resolution PS
Covey, K. R., Greene, T. P., Doppmann, G. W., & Lada, C. J. 2006, The Radial Velocity Distribution of Class I and Flat-Spectrum Protostars, Astronomical Journal, 131, 512
ADS | PDF | PS
Covey, K. R., Greene, T. P., Doppmann, G. W., & Lada, C. J. 2005, The Angular Momentum Content and Evolution of Class I and Flat-Spectrum Protostars, Astronomical Journal, 129, 2765
ADS | PDF | PS
ADS Listing (60 abstracts) | astro-ph Listing (19 abstracts)
Resources from Covey et al. 2007: The 'Hammer' spectral typing and analysis software; the `High Quality' sample of SDSS/2MASS matches (superclean.fits); the full sample, with calculated color distances (colordistances.fits); and machine-readable tables of the properties of the median stellar locus (medianlocus.tbl), synthetic SDSS/2MASS photometry of Pickles (1998) spectral standards with solar (SolarPickles.tbl) and non-solar (NonSolarPickles.tbl) metallicites;
Spectra and photometry from Hawley et al. 2002: SDSS M/L spectral templates from Figure 5, as well as the complete spectroscopic sample. Photometry for these objects is also available in three tables (with a generic README file): M0-M8 objects with Early Data Release spectra, objects M9 and later identified by Hawley et al. 2002, and previously known SDSS MLT dwarves.