output
19972026
most citedGaia Data Release 2. Summary of the contents and survey properties

8.6k citations

Showing 2017 · astro-ph.GAShow all

82 papers · 2 filters

astro-ph.GA2017★ 69 cited

The TOP-SCOPE survey of Planck Galactic Cold Clumps: Survey overview and results of an exemplar source, PGCC G26.53+0.17

Tie Liu, Kee-Tae Kim, Mika Juvela +11

The low dust temperatures (<14 K) of Planck Galactic Cold Clumps (PGCCs) make them ideal targets to probe the initial conditions and very early phase of star formation. TOP-SCOPE i…

astro-ph.GA2017★ 7 cited

Arp 202: a TDG formed in a parent's extended dark matter halo?

T. C. Scott, P. Lagos, S. Ramya +6

We report on H + [NII] imaging of the Arp 202 interacting pair and its tidal dwarf galaxy (TDG) candidate as well as a GMOS long slit spectrum from the TDG candidate, observed w…

astro-ph.GA2017★ 22 cited

Enhancing the H2O Megamaser Detection Rate Using Optical and Mid-infrared Photometry

C. Y. Kuo, A. Constantin, J. A. Braatz +8

Water megamasers from circumnuclear disks in galaxy centers provide the most accurate measurements of supermassive black hole masses and uniquely probe the sub-parsec accretion pro…

astro-ph.GA2017★ 28 cited

ELUCID V. Lighting dark matter halos with galaxies

Xiaohu Yang, Youcai Zhang, Huiyuan Wang +16

In a recent study, using the distribution of galaxies in the north galactic pole of SDSS DR7 region enclosed in a 500$\mpch$ box, we carried out our ELUCID simulation (Wang et al.…

astro-ph.GA2017★ 1 cited

Current stage of the ATCA follow-up for SPLASH

Hai-Hua Qiao, Andrew J. Walsh, Zhi-Qiang Shen

Four ground-state OH transitions were detected in emission, absorption and maser emission in the Southern Parkes Large-Area Survey in Hydroxyl (SPLASH). We re-observed these OH mas…

astro-ph.GA2017★ 14 cited

Revisiting LS I +61 303 with VLBI astrometry

Y. W. Wu, G. Torricelli-Ciamponi, M. Massi +4

We conducted multi-epoch VLBA phase reference observations of LS I +61 303 in order to study its precessing radio jet. Compared to similar observations in 2006, we find that the ob…