activity
20042022
most citedThe Eleventh and Twelfth Data Releases of the Sloan Digital Sky Survey: Final Data from SDSS-III

2.5k citations · 6.2k across the 50 of their papers we have counts for

collaborators

51 papers

astro-ph.EP2022★ 37 cited

Mapping Protoplanetary Disk Vertical Structure with CO Isotopologue Line Emission

Charles J. Law, Richard Teague, Karin I. Öberg +21

High spatial resolution observations of CO isotopologue line emission in protoplanetary disks at mid-inclinations (30-75°) allow us to characterize the gas structure in…

astro-ph.EP2022★ 7 cited

Millimeter Dust Emission and Planetary Dynamics in the HD 106906 System

Anna Fehr, A. Meredith Hughes, Rebekah I. Dawson +10

Debris disks are dusty, optically thin structures around main sequence stars. HD 106906AB is a short-period stellar binary, host to a wide separation planet, HD 106906b, and a debr…

astro-ph.EP2022★ 18 cited

Multiwavelength Vertical Structure in the AU Mic Debris Disk: Characterizing the Collisional Cascade

David Vizgan, A. Meredith Hughes, Evan S. Carter +9

Debris disks are scaled-up analogs of the Kuiper Belt in which dust is generated by collisions between planetesimals. In the "collisional cascade" model of debris disks, dust lost…

astro-ph.EP2022

CO Line Emission Surfaces and Vertical Structure in Mid-Inclination Protoplanetary Disks

Charles J. Law, Sage Crystian, Richard Teague +18

High spatial resolution CO observations of mid-inclination (30-75°) protoplanetary disks offer an opportunity to study the vertical distribution of CO emission and temperature. The…

astro-ph.EP2022

Kinematic Structures in Planet-Forming Disks

Christophe Pinte, Richard Teague, Kevin Flaherty +3

The past 5 years have dramatically changed our view of the disks of gas and dust around young stars. Observations with the Atacama Large Millimeter/submillimeter Array (ALMA) and e…

astro-ph.SR2021★ 10 cited

A Deep Search for Five Molecules in the 49 Ceti Debris Disk

Jessica Klusmeyer, A. Meredith Hughes, Luca Matra +9

Surprisingly strong CO emission has been observed from more than a dozen debris disks around nearby main-sequence stars. The origin of this CO is unclear, in particular whether it…