activity
20132026
most citedA 3D Dust Map Based on Gaia, Pan-STARRS 1 and 2MASS

1.3k citations · 3.7k across the 45 of their papers we have counts for

collaborators
Showing 2020Show all

6 papers · 1 filter

astro-ph.GA2020★ 16 cited

The Cloud Factory II: Gravoturbulent Kinematics of Resolved Molecular Clouds in a Galactic Potential

Andres F. Izquierdo, Rowan J. Smith, Simon C. O. Glover +6

We present a statistical analysis of the gravoturbulent velocity fluctuations in molecular cloud complexes extracted from our "Cloud Factory" galactic-scale ISM simulation suite. F…

astro-ph.GA2020★ 22 cited

Constraining the Distance to the North Polar Spur with Gaia DR2

Kaustav K. Das, Catherine Zucker, Joshua S. Speagle +3

The North Polar Spur (NPS) is one of the largest structures observed in the Milky Way in both the radio and soft x-rays. While several predictions have been made regarding the orig…

astro-ph.IM2020★ 1 cited

A Prospective ISRO-CfA Himalayan Sub-millimeter-wave Observatory Initiative

T. K. Sridharan, Shmuel Bialy, Raymond Blundell +20

The Smithsonian Astrophysical Observatory (SAO), a member of the Center for Astrophysics | Harvard and Smithsonian, is in discussions with the Space Applications Centre (SAC) of th…

astro-ph.GA2020★ 13 cited

Data-Driven Stellar Models

Gregory M. Green, Hans-Walter Rix, Leon Tschesche +7

We develop a data-driven model to map stellar parameters (effective temperature, surface gravity and metallicity) accurately and precisely to broad-band stellar photometry. This mo…

astro-ph.GA2020★ 169 cited

A Galactic-scale gas wave in the Solar Neighborhood

João Alves, Catherine Zucker, Alyssa A. Goodman +6

For the past 150 years, the prevailing view of the local Interstellar Medium (ISM) was based on a peculiarity known as the Gould's Belt, an expanding ring of young stars, gas, and…

astro-ph.GA2020★ 230 cited

A Compendium of Distances to Molecular Clouds in the Star Formation Handbook

Catherine Zucker, Joshua S. Speagle, Edward F. Schlafly +4

Accurate distances to local molecular clouds are critical for understanding the star and planet formation process, yet distance measurements are often obtained inhomogeneously on a…