Detecting Radio AGN Signatures in Red Geysers

Namrata Roy, Kevin Bundy, Edmond Cheung, Wiphu Rujopakarn, Michele Cappellari, Francesco Belfiore, Renbin Yan, Tim Heckman, Matthew Bershady, Jenny Greene, Kyle Westfall, Niv Drory, Kate Rubin, David Law, Kai Zhang, Joseph Gelfand, Dmitry Bizyaev, David Wake, Karen Masters, Daniel ThomasCheng Li, Rogemar A. Riffel

Research output: Contribution to journalArticlepeer-review

17 Scopus citations


A new class of quiescent galaxies harboring possible AGN-driven winds has been discovered using spatially resolved optical spectroscopy from the ongoing SDSS-IV MaNGA survey. These galaxies, termed "red geysers," constitute 5%-10% of the local quiescent population and are characterized by narrow bisymmetric patterns in ionized gas emission features. Cheung et al. argued that these galaxies host large-scale AGN-driven winds that may play a role in suppressing star formation at late times. In this work, we test the hypothesis that AGN activity is ultimately responsible for the red geyser phenomenon. We compare the nuclear radio activity of the red geysers to a matched control sample with similar stellar mass, redshift, rest-frame NUV - r color, axis ratio, and presence of ionized gas. We have used the 1.4 GHz radio continuum data from the VLA FIRST survey to stack the radio flux from the red geyser and control samples. In addition to a three times higher FIRST detection rate, we find that red geysers have a 5σ higher level of average radio flux than control galaxies. After restricting to rest-frame NUV - r color >5 and checking mid-IR WISE photometry, we rule out star formation contamination and conclude that red geysers are associated with more active AGNs. Red geysers and a possibly related class with disturbed Hα emission account for 40% of all radio-detected red galaxies with log (M /M o) < 11.

Original languageEnglish
Article number117
JournalAstrophysical Journal
Issue number2
StatePublished - Dec 20 2018

Bibliographical note

Funding Information:
Funding for the Sloan Digital Sky Survey IV has been provided by the Alfred P. Sloan Foundation, the U.S. Department of Energy Office of Science, and the Participating Institutions. The SDSS-IV acknowledges support and resources from the Center for High-Performance Computing at the University of Utah. The SDSS website is

Funding Information:
NR thanks Professor Puragra Guhathakurta for helpful comments and discussions. RAR acknowledges CNPq and FAPERGS.

Publisher Copyright:
© 2018. The American Astronomical Society. All rights reserved.


  • galaxies: evolution
  • galaxies: formation
  • galaxies: general

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science


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