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20062009
most citedMeasured Metallicities at the Sites of Nearby Broad-Lined Type Ic Supernovae and Implications for the SN-GRB Connection

360 citations · 836 across the 10 of their papers we have counts for

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astro-ph200821 cited

Planets in Stellar Clusters Extensive Search. V. Search for planets and identification of 18 new variable stars in the old open cluster NGC 188

B. J. Mochejska, K. Z. Stanek, D. D. Sasselov +7

We have undertaken a long-term project, Planets in Stellar Clusters Extensive Search (PISCES), to search for transiting planets in open clusters. In this paper we present the resul…

astro-ph200848 cited

Deep MMT Transit Survey of the Open Cluster M37 IV: Limit on the Fraction of Stars With Planets as Small as 0.3 R_J

J. D. Hartman, B. S. Gaudi, M. J. Holman +6

We present the results of a deep (15 ~< r ~< 23), 20 night survey for transiting planets in the intermediate age open cluster M37 (NGC 2099) using the Megacam wide-field mosaic CCD…

astro-ph200846 cited

Outliers from the Mass--Metallicity Relation I: A Sample of Metal-Rich Dwarf Galaxies from SDSS

Molly S. Peeples, Richard W. Pogge, K. Z. Stanek

We have identified a sample of 41 low-mass high--oxygen abundance outliers from the mass--metallicity relation of star-forming galaxies measured by Tremonti et al (2004). These gal…

astro-ph2007142 cited

Deep MMT Transit Survey of the Open Cluster M37 II: Variable Stars

J. D. Hartman, B. S. Gaudi, M. J. Holman +5

We have conducted a deep ($15 \la r \la 23$), 20 night survey for transiting planets in the intermediate age () open cluster M37 (NGC 2099) using the Megacam wi…

astro-ph200759 cited

Deep MMT Transit Survey of the Open Cluster M37 I: Observations and Cluster Parameters

J. D. Hartman, B. S. Gaudi, M. J. Holman +6

We have conducted a deep ($15 \la r \la 23$), 20 night survey for transiting planets in the intermediate age open cluster M37 (NGC 2099) using the Megacam wide-field mosaic CCD cam…

astro-ph2007105 cited

The Future is Now: the Formation of Single Low Mass White Dwarfs in the Solar Neighborhood

Mukremin Kilic, K. Z. Stanek, M. H. Pinsonneault

Low mass helium-core white dwarfs (M < 0.45 Msun) can be produced from interacting binary systems, and traditionally all of them have been attributed to this channel. However, a lo…