output
19952026
most citedThe Man Behind the Curtain: X-rays Drive the UV through NIR Variability in the 2013 AGN Outburst in NGC 2617

1.9k citations

Showing 2020 · astro-ph.GAShow all

17 papers · 2 filters

astro-ph.GA2020★ 50 cited

Lyman-alpha spectroscopy of extreme [OIII] emitting galaxies at : Implications for Ly visibility and LyC leakage at

Mengtao Tang, Daniel Stark, Jacopo Chevallard +3

Spectroscopic observations of massive galaxies selected to have extremely large [OIII]+H equivalent width (EW Å) have recently revealed large Ly detection ra…

astro-ph.GA2020★ 7 cited

Dorado and its member galaxies. Ha imaging of the group backbone

R. Rampazzo, S. Ciroi, P. Mazzei +9

ABRIDGED: Dorado is a nearby, rich and clumpy galaxy group that extends for several degrees in the Southern Hemisphere. For the first time, we map the Ha distribution as a possible…

astro-ph.GA2020★ 14 cited

The Radio Structure of the Narrow-Line Seyfert 1 Mrk 783 with VLBA and e-MERLIN

E. Congiu, P. Kharb, A. Tarchi +9

In this paper, we present the analysis of new radio and optical observations of the narrow-line Seyfert 1 galaxy Mrk 783. 1.6 GHz observations performed with the e-MERLIN interfero…

astro-ph.GA2020★ 27 cited

The VISCACHA survey -- II. Structure of star clusters in the Magellanic Clouds periphery

J. F. C. Santos, F. F. S. Maia, B. Dias +11

We provide a homogeneous set of structural parameters of 83 star clusters located at the periphery of the Small Magellanic Cloud (SMC) and the Large Magellanic Cloud (LMC). The clu…

astro-ph.GA2020★ 30 cited

The spectroscopic follow-up of the QUBRICS bright quasar survey

K. Boutsia, A. Grazian, G. Calderone +11

We present the results of the spectroscopic follow up of the QUBRICS survey. The selection method is based on a machine learning approach applied to photometric catalogs, covering…

astro-ph.GA2020★ 49 cited

Rest-frame UV spectroscopy of extreme [OIII] emitters at : Toward a high-redshift UV reference sample for JWST

Mengtao Tang, Daniel Stark, Jacopo Chevallard +3

Deep spectroscopy of galaxies in the reionization-era has revealed intense CIII] and CIV line emission (EW Å). In order to interpret the nebular emission emerging at …