output
19962026
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 2016 · astro-ph.GAShow all

41 papers · 2 filters

astro-ph.GA2016★ 53 cited

Carbon monoxide in an extremely metal-poor galaxy

Yong Shi, Junzhi Wang, Zhi-Yu Zhang +4

Extremely metal-poor galaxies with metallicity below 10% of the solar value in the local universe are the best analogues to investigating the interstellar medium at a quasi-primiti…

astro-ph.GA2016★ 32 cited

Dense gas in low-metallicity galaxies

J. Braine, Y. Shimajiri, P. André +4

Stars form out of the densest parts of molecular clouds. Far-IR emission can be used to estimate the Star Formation Rate (SFR) and high dipole moment molecules, typically HCN, trac…

astro-ph.GA2016★ 55 cited

AGN-Host Connection at 0.5 < z < 2.5: A rapid evolution of AGN fraction in red galaxies during the last 10 Gyr

Tao Wang, D. Elbaz, D. M. Alexander +13

We explore the dependence of the incidence of moderate-luminosity ( erg s) AGNs and the distribution of their accretion rates on host color at 0.5 <…

astro-ph.GA2016★ 3 cited

Deep CFHT Y-band imaging of VVDS-F22 field: I. data products and photometric redshifts

Dezi Liu, Jinyi Yang, Shuo Yuan +5

We present our deep -band imaging data of a two square degree field within the F22 region of the VIMOS VLT Deep Survey. The observations were conducted using the WIRCam instrume…

astro-ph.GA2016★ 23 cited

Dense Gas in the Outer Spiral Arm of M51

Hao Chen, Jonathan Braine, Yu Gao +2

There is a linear relation between the mass of dense gas, traced by the HCN(1-0) luminosity, and the star formation rate (SFR), traced by the far-infrared luminosity. Recent observ…

astro-ph.GA2016★ 12 cited

The quenched mass portion of star-forming galaxies and the origin of the star formation sequence slope

Zhizheng Pan, Xian Zhong Zheng, Xu Kong

Observationally, a massive disk galaxy can harbor a bulge component that is comparably inactive as a quiescent galaxy (QG). It has been speculated that the quenched component conta…