activity
20152026
most citedThe Disk Substructures at High Angular Resolution Project (DSHARP): I. Motivation, Sample, Calibration, and Overview

1.1k citations · 7.1k across the 103 of their papers we have counts for

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Showing astro-ph.GAShow all

6 papers · 1 filter

astro-ph.GA2021★ 143 cited

Molecules with ALMA at Planet-forming Scales (MAPS) IV: Emission Surfaces and Vertical Distribution of Molecules

Charles J. Law, Richard Teague, Ryan A. Loomis +32

The Molecules with ALMA at Planet-forming Scales (MAPS) Large Program provides a unique opportunity to study the vertical distribution of gas, chemistry, and temperature in the pro…

astro-ph.GA2021★ 1 cited

Molecules with ALMA at Planet-forming Scales (MAPS) XII: Inferring the C/O and S/H ratios in Protoplanetary Disks with Sulfur Molecules

Romane Le Gal, Karin I. Öberg, Richard Teague +24

Sulfur-bearing molecules play an important role in prebiotic chemistry and planet habitability. They are also proposed probes of chemical ages, elemental C/O ratio, and grain chemi…

astro-ph.GA2021★ 21 cited

An ALMA Survey of Chemistry in Disks around M4-M5 Stars

Jamila Pegues, Karin I. Oberg, Jennifer B. Bergner +10

M-stars are the most common hosts of planetary systems in the Galaxy. Protoplanetary disks around M-stars thus offer a prime opportunity to study the chemistry of planet-forming en…

astro-ph.GA2017★ 49 cited

H2CO distribution and formation in the TW Hya disk

Karin I. Oberg, Viviana V. Guzman, Christopher J. Merchantz +8

H2CO is one of the most readily detected organic molecules in protoplanetary disks. Yet its distribution and dominant formation pathway(s) remain largely unconstrained. To address…

astro-ph.GA2017★ 54 cited

Nitrogen Fractionation in Protoplanetary Disks from the H13CN/HC15N Ratio

V. V. Guzmán, K. I. Öberg, J. Huang +2

Nitrogen fractionation is commonly used to assess the thermal history of Solar System volatiles. With ALMA it is for the first time possible to directly measure 14N/15N ratios in c…

astro-ph.GA2016★ 24 cited

Constraining the size of the carrier of the 5797.1 diffuse interstellar band

Jane Huang, Takeshi Oka

The diffuse interstellar band (DIB) at 5797.1 Å is simulated based on three premises: (1) The carrier of the DIB is polar as concluded by T. Oka et al. from the anomalous spectrum…