681 citations · 4.2k across the 111 of their papers we have counts for
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SDSS-IV MaNGA: Identification of active galactic nuclei in optical integral field unit surveys
Dominika Wylezalek, Nadia L. Zakamska, Jenny E. Greene +5
In this paper, we investigate 2727 galaxies observed by MaNGA as of June 2016 to develop spatially resolved techniques for identifying signatures of active galactic nuclei (AGN). W…
SDSS-IV MaNGA: Evidence of the importance of AGN feedback in low-mass galaxies
Samantha J. Penny, Karen L. Masters, Rebecca Smethurst +15
We present new evidence for AGN feedback in a subset of 69 quenched low-mass galaxies ( M, ) selected from the first t…
The first 62 AGN observed with SDSS-IV MaNGA - I: their characterization and definition of a control sample
Sandro B. Rembold, Jáderson S. Shimoia, Thaisa Storchi-Bergmann +16
We report the characterization of the first MaNGA Active Galactic Nuclei (AGN) hosts in the Fifth Product Launch (MPL-5) and the definition of a control sample of non-active g…
The Fourteenth Data Release of the Sloan Digital Sky Survey: First Spectroscopic Data from the extended Baryon Oscillation Spectroscopic Survey and from the second phase of the Apache Point Observatory Galactic Evolution Experiment
Bela Abolfathi, D. S. Aguado, Gabriela Aguilar +344
The fourth generation of the Sloan Digital Sky Survey (SDSS-IV) has been in operation since July 2014. This paper describes the second data release from this phase, and the fourtee…
Are we seeing accretion flows in a 250kpc-sized Ly-alpha halo at z=3?
J. Vernet, M. D. Lehnert, C. De Breuck +8
Using MUSE on the ESO-VLT, we obtained a 4 hour exposure of the z=3.12 radio galaxy MRC0316-257. We detect features down to ~10^-19 erg/s/cm^2/arcsec^2 with the highest surface bri…
The implications of the surprising existence of a large, massive CO disk in a distant protocluster
H. Dannerbauer, M. D. Lehnert, B. H. C. Emonts +18
It is not yet known if the properties of molecular gas in distant protocluster galaxies are significantly affected by their environment as galaxies are in local clusters. Through a…