activity
20042019
most citedCfA3: 185 Type Ia Supernova Light Curves from the CfA

524 citations · 1.7k across the 19 of their papers we have counts for

collaborators

19 papers

astro-ph.GA2019★ 4 cited

Evidence for disc regulation in the lowest-mass stars of the young stellar cluster NGC 2264

Santiago Orcajo, Lucas A. Cieza, Roberto Gamen +1

In the pre-main-sequence stage, star-disc interactions have been shown to remove stellar angular momentum and regulate the rotation periods of stars with M2 and earlier spectral ty…

astro-ph.EP2018★ 45 cited

A universal spin-mass relation for brown dwarfs and planets

Aleks Scholz, Keavin Moore, Ray Jayawardhana +3

While brown dwarfs show similarities with stars in their early life, their spin evolution is much more akin to that of planets. We have used lightcurves from the K2 mission to meas…

astro-ph.GA2015★ 303 cited

Young Stellar Objects in the Gould Belt

Michael M. Dunham, Lori E. Allen, Neal J. Evans +14

We present the full catalog of Young Stellar Objects (YSOs) identified in the 18 molecular clouds surveyed by the Spitzer Space Telescope "cores to disks" (c2d) and "Gould Belt" (G…

astro-ph.SR2014★ 33 cited

Near Infrared Spectroscopy of Young Brown Dwarfs in Upper Scorpius

P. Dawson, A. Scholz, T. P. Ray +3

Spectroscopic follow-up is a pre-requisite for studies of the formation and early evolution of brown dwarfs. Here we present IRTF/SpeX near-infrared spectroscopy of 30 candidate me…

astro-ph.GA2014★ 30 cited

The Spitzer Survey of Interstellar Clouds in the Gould Belt. VI. The Auriga-California Molecular Cloud observed with IRAC and MIPS

Hannah Broekhoven-Fiene, Brenda C. Matthews, Paul M. Harvey +15

We present observations of the Auriga-California Molecular Cloud (AMC) at 3.6, 4.5, 5.8, 8.0, 24, 70 and 160 micron observed with the IRAC and MIPS detectors as part of the Spitzer…

astro-ph.GA2013★ 110 cited

The Luminosities of Protostars in the Spitzer c2d and Gould Belt Legacy Clouds

Michael M. Dunham, Hector G. Arce, Lori E. Allen +14

Motivated by the long-standing "luminosity problem" in low-mass star formation whereby protostars are underluminous compared to theoretical expectations, we identify 230 protostars…