The PHANGS-MUSE survey. Probing the chemo-dynamical evolution of disc galaxies
學年 110
學期 2
出版(發表)日期 2022-03-28
作品名稱 The PHANGS-MUSE survey. Probing the chemo-dynamical evolution of disc galaxies
著者 Eric Emsellem; Eva Schinnerer; Francesco Santoro; Francesco Belfiore; Ismael Pessa; Rebecca McElroy; Guillermo A. Blanc; Enrico Congiu; Brent Groves; I. -Ting Ho; Kathryn Kreckel; Alessandro Razza; Patricia Sanchez-Blazquez; Oleg Egorov; Chris Faesi; Ralf S. Klessen; Adam K. Leroy; Sharon Meidt; Miguel Querejeta; Erik Rosolowsky; Fabian Scheuermann; Gagandeep S. Anand; Ashley T. Barnes; Ivana Bešlić; Frank Bigiel; Médéric Boquien; Yixian Cao; Mélanie Chevance; Daniel A. Dale; Cosima Eibensteiner; Simon C. O. Glover; Kathryn Grasha; Jonathan D. Henshaw; Annie Hughes; Eric W. Koch; J. M. Diederik Kruijssen; Janice Lee; Daizhong Liu; Hsi-An Pan; Jérôme Pety; Toshiki Saito; Karin M. Sandstrom; Andreas Schruba; Jiayi Sun; David A. Thilker; Antonio Usero; Elizabeth J. Watkins; and Thomas G. Williams
著錄名稱、卷期、頁數 Astronomy & Astrophysics 659, p.47
摘要 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.
關鍵字 galaxies: spiral;galaxies: star formation;surveys;techniques: imaging spectroscopy;ISM: general;stars: kinematics and dynamics
語言 en_US
ISSN 2329-1273;2329-1265
期刊性質 國外
收錄於 SCI
國別 USA
出版型式 ,電子版,紙本

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