activity
20012023
most citedThe Host Galaxies and Classification of Active Galactic Nuclei

2.2k citations · 17.4k across the 199 of their papers we have counts for

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Showing 2017 · astro-ph.GAShow all

12 papers · 2 filters

astro-ph.GA2017★ 34 cited

The most ancient spiral galaxy: a 2.6-Gyr-old disk with a tranquil velocity field

Tiantian Yuan, Johan Richard, Anshu Gupta +7

We report an integral-field spectroscopic (IFS) observation of a gravitationally lensed spiral galaxy A1689B11 at redshift . It is the most ancient spiral galaxy discovered…

astro-ph.GA2017★ 102 cited

The SAMI Galaxy Survey: Global stellar populations on the size-mass plane

Nicholas Scott, S. Brough, Scott M. Croom +20

We present an analysis of the global stellar populations of galaxies in the SAMI Galaxy Survey. Our sample consists of 1319 galaxies spanning four orders of magnitude in stellar ma…

astro-ph.GA2017★ 87 cited

The Chemical Evolution Carousel of Spiral Galaxies: Azimuthal Variations of Oxygen Abundance in NGC1365

I-Ting Ho, Mark Seibert, Sharon E. Meidt +9

The spatial distribution of oxygen in the interstellar medium of galaxies is the key to understanding how efficiently metals that are synthesized in massive stars can be redistribu…

astro-ph.GA2017★ 53 cited

Probing the Physics of Narrow Line Regions in Active Galaxies IV: Full data release of The Siding Spring Southern Seyfert Spectroscopic Snapshot Survey (S7)

Adam D. Thomas, Michael A. Dopita, Prajval Shastri +15

We present the second and final data release of the Siding Spring Southern Seyfert Spectroscopic Snapshot Survey (S7). Data are presented for 63 new galaxies not included in the fi…

astro-ph.GA2017★ 78 cited

The SAMI Galaxy Survey: Data Release One with Emission-line Physics Value-Added Products

Andrew W. Green, Scott M. Croom, Nicholas Scott +48

We present the first major release of data from the SAMI Galaxy Survey. This data release focuses on the emission-line physics of galaxies. Data Release One includes data for 772 g…

astro-ph.GA2017★ 112 cited

The Origins of [CII] Emission in Local Star-forming Galaxies

Kevin Croxall, J. D. T. Smith, Eric Pellegrini +17

The [CII] 158um fine-structure line is the brightest emission line observed in local star-forming galaxies. As a major coolant of the gas-phase interstellar medium, [CII] balances…

astro-ph.GA2017★ 5 cited

The SAMI Galaxy Survey: Disk-halo interactions in radio-selected star-forming galaxies

S. K. Leslie, J. J. Bryant, I. -T. Ho +20

In this paper, we compare the radio emission at 1.4 GHz with optical outflow signatures of edge-on galaxies. We report observations of six edge-on star-forming galaxies in the Sydn…

astro-ph.GA2017★ 57 cited

Dissecting Galaxies: Separating Star Formation, Shock Excitation and AGN Activity in the Central Region of NGC 613

Rebecca L. Davies, Brent Groves, Lisa J. Kewley +13

The most rapidly evolving regions of galaxies often display complex optical spectra with emission lines excited by massive stars, shocks and accretion onto supermassive black holes…

astro-ph.GA2017★ 20 cited

Attenuation modified by DIG and dust as seen in M31

Neven Tomicic, Kathryn Kreckel, Brent Groves +5

The spatial distribution of dust in galaxies affects the global attenuation, and hence inferred properties, of galaxies. We trace the spatial distribution of dust in five fields (a…

astro-ph.GA2017★ 61 cited

The Dust Attenuation of Star-forming Galaxies at and Beyond: New Insights from ALMA Observations

Yoshinobu Fudamoto, Pascal A. Oesch, Eva Schinnerer +10

We present results on the dust attenuation of galaxies at redshift by studying the relationship between the UV spectral slope () and the infrared excess (IRX;…

astro-ph.GA2017★ 13 cited

The Survey of Lines in M31 (SLIM): The Drivers of the [CII]/TIR Variation

Maria Julia Kapala, Brent Groves, Karin Sandstrom +7

The ratio of the [CII] 158m emission line over the total infrared emission (TIR) is often used as a proxy for the photoelectric (PE) heating efficiency () of the f…

astro-ph.GA2017★ 29 cited

The SAMI Galaxy Survey: a new method to estimate molecular gas surface densities from star formation rates

Christoph Federrath, Diane M. Salim, Anne M. Medling +16

Stars form in cold molecular clouds. However, molecular gas is difficult to observe because the most abundant molecule (H2) lacks a permanent dipole moment. Rotational transitions…