The PHANGS-MUSE survey. Probing the chemo-dynamical evolution of disc galaxies - INSU - Institut national des sciences de l'Univers Access content directly
Journal Articles Astronomy and Astrophysics - A&A Year : 2022

The PHANGS-MUSE survey. Probing the chemo-dynamical evolution of disc galaxies

Eva Schinnerer
Francesco Santoro
Francesco Belfiore
Ismael Pessa
  • Function : Author
Rebecca Mcelroy
Guillermo A. Blanc
  • Function : Author
Enrico Congiu
Brent Groves
I. -Ting Ho
  • Function : Author
Kathryn Kreckel
Alessandro Razza
Patricia Sanchez-Blazquez
  • Function : Author
Oleg Egorov
Chris Faesi
  • Function : Author
Ralf S. Klessen
  • Function : Author
Adam K. Leroy
  • Function : Author
Sharon Meidt
Miguel Querejeta
Erik Rosolowsky
Fabian Scheuermann
  • Function : Author
Gagandeep S. Anand
  • Function : Author
Ashley T. Barnes
  • Function : Author
Ivana Bešlić
Frank Bigiel
Médéric Boquien
Yixian Cao
Mélanie Chevance
Daniel A. Dale
  • Function : Author
Cosima Eibensteiner
Simon C. O. Glover
  • Function : Author
Kathryn Grasha
Jonathan D. Henshaw
  • Function : Author
Eric W. Koch
  • Function : Author
J. M. Diederik Kruijssen
  • Function : Author
Janice Lee
Daizhong Liu
Hsi-An Pan
Jérôme Pety
Toshiki Saito
Karin M. Sandstrom
  • Function : Author
Andreas Schruba
  • Function : Author
Jiayi Sun
David A. Thilker
  • Function : Author
Antonio Usero
Elizabeth J. Watkins
  • Function : Author
Thomas G. Williams
  • Function : Author

Abstract

We present the PHANGS-MUSE survey, a programme that uses the MUSE integral field spectrograph at the ESO VLT to map 19 massive (9.4 < log(M/M)< 11.0) nearby (D ≲ 20 Mpc) star-forming disc galaxies. The survey consists of 168 MUSE pointings (1' by 1' each) and a total of nearly 15 × 106 spectra, covering ∼1.5 × 106 independent spectra. PHANGS-MUSE provides the first integral field spectrograph view of star formation across different local environments (including galaxy centres, bars, and spiral arms) in external galaxies at a median resolution of 50 pc, better than the mean inter-cloud distance in the ionised interstellar medium. This `cloud-scale' resolution allows detailed demographics and characterisations of H II regions and other ionised nebulae. PHANGS-MUSE further delivers a unique view on the associated gas and stellar kinematics and provides constraints on the star-formation history. The PHANGS-MUSE survey is complemented by dedicated ALMA CO(2-1) and multi-band HST observations, therefore allowing us to probe the key stages of the star-formation process from molecular clouds to H II regions and star clusters. This paper describes the scientific motivation, sample selection, observational strategy, data reduction, and analysis process of the PHANGS-MUSE survey. We present our bespoke automated data-reduction framework, which is built on the reduction recipes provided by ESO but additionally allows for mosaicking and homogenisation of the point spread function. We further present a detailed quality assessment and a brief illustration of the potential scientific applications of the large set of PHANGS-MUSE data products generated by our data analysis framework. The data cubes and analysis data products described in this paper represent the basis for the first PHANGS-MUSE public data release and are available in the ESO archive and via the Canadian Astronomy Data Centre.
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Dates and versions

insu-03667460 , version 1 (13-05-2022)

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Eric Emsellem, Eva Schinnerer, Francesco Santoro, Francesco Belfiore, Ismael Pessa, et al.. The PHANGS-MUSE survey. Probing the chemo-dynamical evolution of disc galaxies. Astronomy and Astrophysics - A&A, 2022, 659, ⟨10.1051/0004-6361/202141727⟩. ⟨insu-03667460⟩
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