activity
20062017
most citedA Survey of Local Group Galaxies Currently Forming Stars. I. UBVRI Photometry of Stars in M31 and M33

412 citations · 975 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.SR2017★ 72 cited

The SAGE-Spec Spitzer Legacy program: The life-cycle of dust and gas in the Large Magellanic Cloud. Point source classification III

Olivia C. Jones, Paul M. Woods, F. Kemper +16

The Infrared Spectrograph (IRS) on the {\em Spitzer Space Telescope} observed nearly 800 point sources in the Large Magellanic Cloud (LMC), taking over 1,000 spectra. 197 of these…

astro-ph.GA2010★ 118 cited

The SAGE-Spec Spitzer Legacy program: The life-cycle of dust and gas in the Large Magellanic Cloud. Point source classification I

Paul M. Woods, J. M. Oliveira, F. Kemper +55

We present the classification of 197 point sources observed with the Infrared Spectrograph in the SAGE-Spec Legacy program on the Spitzer Space Telescope. We introduce a decision-t…

astro-ph.GA2010★ 96 cited

The SAGE-Spec Spitzer Legacy program: The life-cycle of dust and gas in the Large Magellanic Cloud

F. Kemper, Paul M. Woods, V. Antoniou +53

The SAGE-Spec Spitzer Legacy program is a spectroscopic follow-up to the SAGE-LMC photometric survey of the Large Magellanic Cloud carried out with the Spitzer Space Telescope. We…

astro-ph.SR2009★ 3 cited

The Physical Properties of Red Supergiants

Emily M. Levesque

Red supergiants (RSGs) are an evolved He-burning phase in the lifetimes of moderately high mass (10 - 25 solar mass) stars. The physical properties of these stars mark them as an i…

astro-ph.SR2009★ 33 cited

Physical Properties of Red Supergiants

Emily Levesque

Red supergiants (RSGs) are a He-burning phase in the evolution of moderately massive stars (10-25 solar masses). For many years, the assumed physical properties of these stars plac…

astro-ph2007★ 2 cited

Physical Properties of Red Supergiants

Philip Massey, Bertrand Plez, Emily M. Levesque +3

Red supergiants (RSGs) are an evolved stage in the life of intermediate massive stars (<25Mo). For many years their location in the H-R diagram was at variance with the evolutionar…