output
20022026
most citedThe Astropy Project: Sustaining and Growing a Community-oriented Open-source Project and the Latest Major Release (v5.0) of the Core Package

5k citations

Showing 2019 · astro-ph.GAShow all

11 papers · 2 filters

astro-ph.GA201941 cited

Probing the full CO spectral line energy distribution (SLED) in the nuclear region of a quasar-starburst system at

Jianan Li, Ran Wang, Dominik Riechers +14

We report Atacama Large Millimeter/submillimeter Array (ALMA) observations of CO , , and and NOrthern Extend…

astro-ph.GA201927 cited

Mass Assembly of Stellar Systems and their Evolution with the SMA (MASSES) -- Full Data Release

Ian W. Stephens, Tyler L. Bourke, Michael M. Dunham +13

We present and release the full dataset for the Mass Assembly of Stellar Systems and their Evolution with the SMA (MASSES) survey. This survey used the Submillimeter Array (SMA) to…

astro-ph.GA201918 cited

The ALMA Spectroscopic Survey in the HUDF: Constraining cumulative CO emission at with power spectrum analysis of ASPECS LP data from 84 to 115 GHz

Bade Uzgil, Chris Carilli, Adam Lidz +12

We present a power spectrum analysis of the ALMA Spectroscopic Survey Large Program (ASPECS LP) data from 84 to 115 GHz. These data predominantly probe small-scale fluctuations ($k…

astro-ph.GA20197 cited

ALMA Band 3 polarimetric follow-up of a complete sample of faint PACO sources

Vincenzo Galluzzi, Giuseppe Puglisi, Sandra Burkutean +17

We present Atacama Large Millimeter/submillimiter Array (ALMA) high sensitivity (mJy) polarimetric observations at GHz (Band 3) of a complete sample of $3…

astro-ph.GA20194.3k cited

First M87 Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole

The Event Horizon Telescope Collaboration

When surrounded by a transparent emission region, black holes are expected to reveal a dark shadow caused by gravitational light bending and photon capture at the event horizon. To…

astro-ph.GA201934 cited

The ALMA-PILS survey: Gas dynamics in IRAS 162932422 and the connection between its two protostars

M. H. D. van der Wiel, S. K. Jacobsen, J. K. Jørgensen +10

[Abridged] The majority of stars form in binary or higher order systems. The Class 0 protostellar system IRAS16293-2422 contains two protostars, 'A' and 'B', separated by ~600 au a…