output
20152019
most citedFirst M87 Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole

4.3k citations

51 papers

astro-ph.GA20191.5k cited

First M87 Event Horizon Telescope Results. V. Physical Origin of the Asymmetric Ring

The Event Horizon Telescope Collaboration

The Event Horizon Telescope (EHT) has mapped the central compact radio source of the elliptical galaxy M87 at 1.3 mm with unprecedented angular resolution. Here we consider the phy…

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.HE2019106 cited

The LOFAR Tied-Array All-Sky Survey (LOTAAS): Survey overview and initial pulsar discoveries

S. Sanidas, S. Cooper, C. G. Bassa +20

We present an overview of the LOFAR Tied-Array All-Sky Survey (LOTAAS) for radio pulsars and fast transients. The survey uses the high-band antennas of the LOFAR Superterp, the den…

astro-ph.GA201923 cited

Starburst and post-starburst high-redshift protogalaxies: The feedback impact of high energy cosmic rays

Ellis R. Owen, Kinwah Wu, Xiangyu Jin +2

Quenching of star-formation has been identified in many starburst and post-starburst galaxies, indicating burst-like star-formation histories (SFH) in the primordial Universe. We h…

astro-ph.GA201922 cited

Gemini Imaging of the Host Galaxies of Changing-Look Quasars

Paul J. L. Charlton, John J. Ruan, Daryl Haggard +4

Changing-look quasars are a newly-discovered class of luminous active galactic nuclei that undergo rapid (10 year) transitions between Type 1 and Type 1.9/2, with an asso…

astro-ph.HE201912 cited

The Green Bank North Celestial Cap Pulsar Survey. IV: Four New Timing Solutions

R. J. Aloisi, A. Cruz, L. Daniels +40

We present timing solutions for four pulsars discovered in the Green Bank Northern Celestial Cap (GBNCC) survey. All four pulsars are isolated with spin periods between 0.26s a…