activity
19992020
most citedHigh-excitation CO in a quasar host galaxy at z=6.42

197 citations · 919 across the 21 of their papers we have counts for

collaborators

18 papers

astro-ph.GA2020★ 29 cited

The Megamaser Cosmology Project. XI. A geometric distance to CGCG 074-064

D. W. Pesce, J. A. Braatz, M. J. Reid +6

As part of the survey component of the Megamaser Cosmology Project, we have discovered a disk megamaser system in the galaxy CGCG 074-064. Using the GBT and the VLA, we have obtain…

astro-ph.GA2019★ 19 cited

Star Formation Efficiencies at Giant Molecular Cloud Scales in the Molecular Disk of the Elliptical Galaxy NGC 5128 (Centaurus A)

D. Espada, S. Verley, R. E. Miura +15

We present ALMA CO(1-0) observations toward the dust lane of the nearest elliptical and radio galaxy, NGC 5128 (Centaurus A), with high angular resolution ( 1 arcsec, or 18 p…

astro-ph.GA2019★ 20 cited

Accretion disk versus jet orientation in HO megamaser galaxies

F. Kamali, C. Henkel, S. Koyama +10

An essential part of the paradigm describing active galactic nuclei is the alignment between the radio jet and the associated rotation axis of the sub-pc sized accretion disks. Bec…

astro-ph.GA2018★ 27 cited

The Serpens filament: at the onset of slightly supercritical collapse

Y. Gong, G. ~X. Li, R. ~Q. Mao +5

The Serpens filament, as one of the nearest infrared dark clouds, is regarded as a pristine filament at a very early evolutionary stage of star formation. In order to study its mol…

astro-ph.SR2017★ 14 cited

SiS in the circumstellar envelope of IRC +10126: maser and quasi-thermal emission

Y. Gong, C. Henkel, J. Ott +6

We present new Effelsberg-100 m, ATCA, and VLA observations of rotational SiS transitions in the circumstellar envelope (CSE) of IRC +10216. Thanks to the high angular resolution a…

astro-ph.GA2015★ 22 cited

New candidates for extremely metal-poor emission-line galaxies in the SDSS/BOSS DR10

N. G. Guseva, Y. I. Izotov, K. J. Fricke +1

We present a spectroscopic study of eight extremely low-metallicity candidate emission-line galaxies with oxygen abundances possibly below 12 +log O/H = 7.35. These galaxies were s…