activity
20142026
most citedA Census of Young Stars and Brown Dwarfs in IC 348 and NGC 1333

117 citations · 1k across the 22 of their papers we have counts for

collaborators
Showing astro-ph.SRShow all

16 papers · 1 filter

astro-ph.SR2024

Extending the ALMA Census of Circumstellar Disks in the Upper Scorpius OB Association

John M. Carpenter, Taran L. Esplin, Kevin L. Luhman +2

We present ALMA Band 7 continuum (340 GHz) and CO J=3-2 observations for an extended sample of disks in the Upper Scorpius OB Association (Upper Sco, age ~ 10 Myr). The targets wer…

astro-ph.SR2021★ 29 cited

A Census of Stars and Disks in Corona Australis

Taran Esplin, Kevin Luhman

We have performed a census of the young stellar populations near the Corona Australis molecular cloud using photometric and kinematic data from several sources, particularly Gaia E…

astro-ph.SR2020★ 109 cited

Refining the Census of the Upper Scorpius Association with Gaia

K. L. Luhman, T. L. Esplin

We have refined the census of stars and brown dwarfs in the Upper Sco association (~10 Myr, ~145 pc) by 1) updating the selection of candidate members from our previous survey to i…

astro-ph.SR2020★ 45 cited

A Survey for New Stars and Brown Dwarfs in the Ophiuchus Star-forming Complex

T. L. Esplin, K. L. Luhman

We have performed a survey for new members of the Ophiuchus cloud complex using high-precision astrometry from the second data release of Gaia, proper motions measured with multi-e…

astro-ph.SR2019★ 87 cited

A Survey for New Members of Taurus from Stellar to Planetary Masses

T. Esplin, K. Luhman

We present a large sample of new members of the Taurus star-forming region that extend from stellar to planetary masses. To identify candidate members at substellar masses, we have…

astro-ph.SR2019★ 9 cited

Near-Infrared Variability of Low Mass Stars in IC 1396A and TR 37

Huan Y. A. Meng, G. H. Rieke, Jinyoung Serena Kim +5

We have monitored nearly a square degree in IC 1396A/Tr 37 over 21 epochs extending over 2014 - 2016 for sources variable in the JHK bands. In our data, 65 +\- 8 % of previously id…