activity
19952018
most citedLate-Type Stars in M31. I.: A Photometric Study of AGB Stars and Metallicity Gradients.

71 citations · 167 across the 7 of their papers we have counts for

collaborators

6 papers

astro-ph.IM2018

Sex-Disaggregated Systematics in Canadian Time Allocation Committee Telescope Proposal Reviews

Kristine Spekkens, Nicholas Cofie, Dennis R. Crabtree

Recent studies have shown that the proposal peer review processes employed by a variety of organizations to allocate astronomical telescope time produce outcomes that are systemati…

astro-ph.IM2014★ 3 cited

The Gemini Observatory Fast Turnaround Program

R. E. Mason, S. Cote, M. Kissler-Patig +4

Gemini's Fast Turnaround program is intended to greatly decrease the time from having an idea to acquiring the supporting data. The scheme will offer monthly proposal submission op…

astro-ph2004★ 35 cited

Carbon Stars and other Luminous Stellar Populations in M33

J. F. Rowe, H. B. Richer, J. P. Brewer +1

The M33 galaxy is a nearby, relatively metal-poor, late-type spiral. Its proximity and almost face-on inclination means that it projects over a large area on the sky, making it an…

astro-ph2001★ 5 cited

The Effectiveness of the Canada-France-Hawaii Telescope

Dennis R. Crabtree, Elizabeth P. Bryson

We have investigated the productivity and impact of the Canada-France-Hawaii Telescope (CFHT) during its twenty-year history. CFHT has maintained a database of refereed publication…

astro-ph1996★ 18 cited

Globular Clusters in NGC 1275

Denise Kaisler, William E. Harris, Dennis R. Crabtree +1

We present the results of a deep photometric study of the outer halo of NGC 1275, the highly active cD galaxy at the center of the Perseus cluster. We find a modest excess of faint…

astro-ph1995★ 71 cited

Late-Type Stars in M31. I.: A Photometric Study of AGB Stars and Metallicity Gradients.

J. P. Brewer, H. B. Richer, D. R. Crabtree

We have imaged five 7\arcmin \x 7\arcmin\ fields in M31 spanning galactocentric radii from 4 to 32 kpc along the SW-major axis. The fields were observed through two broad-band (\V\…