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HI-MaNGA: HI Followup for the MaNGA Survey

Research output: Contribution to journalArticle

  • Karen L. Masters
  • David V. Stark
  • Zachary J. Pace
  • Frederika Phipps
  • Wiphu Rujopakarn
  • Nattida Samanso
  • Emily Harrington
  • José R. Sánchez-Gallego
  • Vladimir Avila-Reese
  • Matthew Bershady
  • Brian Cherinka
  • Catherine E. Fielder
  • Daniel Finnegan
  • Rogemar A. Riffel
  • Kate Rowlands
  • Shoaib Shamsi
  • Lucy Newnham
  • Anne-Marie Weijmans
  • Catherine A. Witherspoon
We present the HI-MaNGA programme of HI follow-up for the Mapping Nearby Galaxies at Apache Point Observatory (MaNGA) survey. MaNGA, which is part of the Fourth phase of the Sloan Digital Sky Surveys (SDSS-IV), is in the process of obtaining integral field unit (IFU) spectroscopy for a sample of ~10,000 nearby galaxies. We give an overview of the HI 21cm radio follow-up observing plans and progress and present data for the first 331 galaxies observed in the 2016 observing season at the Robert C. Bryd Green Bank Telescope (GBT). We also provide a cross match of the current MaNGA (DR15) sample with publicly available HI data from the Arecibo Legacy Fast Arecibo L-band Feed Array (ALFALFA) survey. The addition of HI data to the MaNGA data set will strengthen the survey's ability to address several of its key science goals that relate to the gas content of galaxies, while also increasing the legacy of this survey for all extragalactic science.
Original languageEnglish
Pages (from-to)3396-3405
Number of pages10
JournalMonthly Notices of the Royal Astronomical Society
Volume488
Issue number3
Early online date10 Jul 2019
DOIs
Publication statusPublished - 1 Sep 2019

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    Rights statement: This article has been accepted for publication in MNRAS © 2019 The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.

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