3 papers
astro-ph.GA2012
Converting From 3.6 and 4.5 Micron Fluxes to Stellar Mass
Michael R. Eskew, Dennis F. Zaritsky, Sharon E. Meidt
We use high spatial resolution maps of stellar mass and infrared flux of the Large Magellanic Cloud (LMC) to calibrate a conversion between 3.6 and 4.5 micron fluxes and stellar ma…
astro-ph.GA2011
Nearby Galaxies in More Distant Contexts
Michael Eskew, Dennis Zaritsky
We use published reconstructions of the star formation history (SFH) of the Large Magellanic Cloud (LMC), Small Magellanic Cloud, and NGC 300 from the analysis of resolved stellar…
astro-ph.SR2009
Modeling the System Parameters of 2M1533+3759: A New Longer-Period Low-Mass Eclipsing sdB+dM Binary
B. -Q. For, E. M. Green, G. Fontaine +17
We present new photometric and spectroscopic observations for 2M 1533+3759 (= NSVS 07826147). It has an orbital period of 0.16177042 day, significantly longer than the 2.3--3.0 hou…