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

被引：93

作者：

Emsellem, Eric ^{[1
,2
]}

Schinnerer, Eva ^{[3
]}

Santoro, Francesco ^{[3
]}

Belfiore, Francesco ^{[4
]}

Pessa, Ismael ^{[3
]}

McElroy, Rebecca ^{[5
]}

Blanc, Guillermo A. ^{[6
,7
]}

Congiu, Enrico ^{[6
]}

Groves, Brent ^{[8
,9
]}

Ho, I-Ting ^{[3
]}

Kreckel, Kathryn ^{[10
]}

Razza, Alessandro ^{[6
]}

Sanchez-Blazquez, Patricia ^{[12
]}

Egorov, Oleg ^{[10
,13
]}

Faesi, Chris ^{[3
]}

Klessen, Ralf S. ^{[14
,15
]}

Leroy, Adam K. ^{[16
]}

Meidt, Sharon ^{[17
]}

Querejeta, Miguel ^{[18
]}

Rosolowsky, Erik ^{[19
]}

Scheuermann, Fabian ^{[10
]}

Anand, Gagandeep S. ^{[20
]}

Barnes, Ashley T. ^{[21
]}

Beslic, Ivana ^{[21
]}

Bigiel, Frank ^{[21
]}

Boquien, Mederic ^{[22
]}

Cao, Yixian ^{[23
]}

Chevance, Melanie ^{[10
]}

Dale, Daniel A. ^{[24
]}

Eibensteiner, Cosima ^{[21
]}

Glover, Simon C. O. ^{[14
]}

Grasha, Kathryn ^{[9
]}

Henshaw, Jonathan D. ^{[3
]}

Hughes, Annie ^{[25
]}

Koch, Eric W. ^{[26
]}

Kruijssen, J. M. Diederik ^{[10
]}

Lee, Janice ^{[11
]}

Liu, Daizhong ^{[27
]}

Pan, Hsi-An ^{[3
]}

Pety, Jerome ^{[28
,29
]}

Saito, Toshiki ^{[3
]}

Sandstrom, Karin M. ^{[30
]}

Schruba, Andreas ^{[27
]}

Sun, Jiayi ^{[16
]}

Thilker, David A. ^{[31
]}

Usero, Antonio ^{[18
]}

Watkins, Elizabeth J. ^{[10
]}

Williams, Thomas G. ^{[3
]}

机构：

[1] European Southern Observ, Karl Schwarzschild Str 2, D-85748 Garching, Germany

[2] Univ Lyon 1, Univ Lyon, ENS Lyon, CNRS,Ctr Rech Astrophys Lyon,UMR5574, F-69230 St Genis Laval, France

[3] Max Planck Inst Astron, Konigstuhl 17, D-69117 Heidelberg, Germany

[4] INAF, Osservatorio Astrofis Arcetri, Largo E Fermi 5, I-50125 Florence, Italy

[5] Univ Sydney, Sch Phys, Sydney Inst Astron, Phys Rd, Darlington, NSW 2006, Australia

[6] Univ Chile, Dept Astron, Santiago, Chile

[7] Observ Carnegie Inst Sci, Pasadena, CA USA

[8] Univ Western Australia, Int Ctr Radio Astron Res, 7 Fairway, Crawley, WA 6009, Australia

[9] Australian Natl Univ, Res Sch Astron & Astrophys, Canberra, ACT 2611, Australia

[10] Heidelberg Univ, Zentrum Astron, Astron Rech Inst, Monchhofstr 12-14, D-69120 Heidelberg, Germany

[11] NSFs NOIRLab, Gemini Observ, 950 N Cherry Ave, Tucson, AZ 85719 USA

[12] Univ Complutense Madrid, Dept Fis Tierra & Astrofis, Madrid 28040, Spain

[13] Lomonosov Moscow State Univ, Sternberg Astron Inst, Univ Sky Pr 13, Moscow 119234, Russia

[14] Heidelberg Univ, Zentrum Astron, Inst Theoret Astrophys, Albert Ueberle Str 2, D-69120 Heidelberg, Germany

[15] Heidelberg Univ, Interdisziplinares Zentrum Wissensch Rechnen, Neuenheimer Feld 205, D-69120 Heidelberg, Germany

[16] Ohio State Univ, Dept Astron, 140 West 18th Ave, Columbus, OH 43210 USA

[17] Univ Ghent, Sterrenkundig Observ, Krijgslaan 281 S9, B-9000 Ghent, Belgium

[18] Observ Astron Nacl IGN, C Alfonso XII 3, Madrid 28014, Spain

[19] Univ Alberta, Dept Phys, Edmonton, AB T6G 2E1, Canada

[20] Univ Hawaii, Inst Astron, 2680 Woodlawn Dr, Honolulu, HI 96822 USA

[21] Univ Bonn, Argelander Inst Astron, Hugel 71, D-53121 Bonn, Germany

[22] Univ Antofagasta, Ctr Astron CITEVA, Ave Angamos 601, Antofagasta, Chile

[23] Aix Marseille Univ, CNRS, CNES, LAM Lab Astrophys Marseille, F-13388 Marseille, France

[24] Univ Wyoming, Dept Phys & Astron, Laramie, WY 82071 USA

[25] Univ Toulouse, UPS OMP, IRAP, F-31028 Toulouse 4, France

[26] Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA

[27] Max Planck Inst Extraterr Phys, Giessenbachstr 1, D-85748 Garching, Germany

[28] Inst Radioastron Millimetr IRAM, 300 Rue Piscine, F-38406 St Martin dHeres, France

[29] PSL Res Univ, Sorbonne Univ, CNRS, LERMA,Observ Paris, F-75014 Paris, France

[30] Univ Calif San Diego, Dept Phys, Ctr Astrophys & Space Sci, 9500 Gilman Dr, La Jolla, CA 92093 USA

[31] Johns Hopkins Univ, Dept Phys & Astron, Baltimore, MD 21218 USA

来源：

ASTRONOMY & ASTROPHYSICS | 2022年 / 659卷

基金：

欧洲研究理事会;

关键词：

galaxies; spiral; star formation; surveys; techniques; imaging spectroscopy; ISM; general; stars; kinematics and dynamics; SDSS-IV MANGA; STAR-FORMATION RATES; DIGITAL SKY SURVEY; EDGE-CALIFA SURVEY; OXYGEN-ABUNDANCE GRADIENT; MOLECULAR GAS PROPERTIES; FORMATION MAIN-SEQUENCE; H-II REGIONS; NEARBY GALAXIES; STELLAR FEEDBACK;

D O I：

10.1051/0004-6361/202141727

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

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-circle dot)< 11.0) nearby (D less than or similar to 20 Mpc) star-forming disc galaxies. The survey consists of 168 MUSE pointings (1 ' by 1 ' each) and a total of nearly 15 x 10(6) spectra, covering similar to 1.5 x 10(6) 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.

引用

页数：47

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