J/AJ/159/167 AMUSING++ nearby galaxy compilation. I. Sample (Lopez-Coba+, 2020)
The AMUSING++ nearby galaxy compilation.
I. Full sample characterization and galactic-scale outflow selection.
Lopez-Coba C., Sanchez S.F., Anderson J.P., Cruz-Gonzalez I., Galbany L.,
Ruiz-Lara T., Barrera-Ballesteros J.K., Prieto J.L., Kuncarayakti H.
<Astron. J., 159, 167 (2020)>
=2020AJ....159..167L 2020AJ....159..167L
ADC_Keywords: Galaxies, spectra; Active gal. nuclei; Redshifts; Morphology
Stars, masses; Optical; Intergalactic medium; Galaxy catalogs
Keywords: Catalogs ; Interstellar medium ; Galactic winds
Abstract:
We present here the All-weather MUse Supernova Integral-field of
Nearby Galaxies (AMUSING++): the largest compilation of nearby
galaxies observed with the Multi Unit Spectroscopic Explorer (MUSE)
integral-field spectrograph so far. This collection consists of 635
galaxies from different MUSE projects covering the redshift interval
0.0002<z<0.1. The sample and its main properties are characterized and
described here. It includes galaxies of almost all morphological
types, with a good coverage in its color-magnitude diagram, within the
stellar mass range between 108 and 1012M☉, and with properties
resembling those of a diameter-selected sample. The AMUSING++ sample
is, therefore, suitable for studying, with unprecedented detail, the
properties of nearby galaxies at global and local scales, providing us
with more than 50 million individual spectra. We use this compilation
to investigate the presence of galactic outflows. We exploit the use
of combined emission-line images to explore the shape of the different
ionized components and the distribution along classical diagnostic
diagrams to disentangle the different ionizing sources across the
optical extension of each galaxy. We use the cross-correlation
function to estimate the level of symmetry of the emission lines as an
indication of the presence of shocks and/or active galactic nuclei. We
uncovered a total of 54 outflows, comprising ∼8% of the sample. A
large number of the discovered outflows correspond to those driven by
active galactic nuclei (∼60%), suggesting some bias in the selection
of our sample. No clear evidence was found that outflow host galaxies
are highly star-forming, and outflows appear to be found within all
galaxies around the star-formation sequence.
Description:
In the present work, we compile the All-weather MUse Supernova
Integral-field of Nearby Galaxies ("AMUSING++") sample from different
MUSE projects and use this to identify and study galactic outflows at
sub-kiloparsec scales over a large number of different galaxies.
The Multi Unit Spectroscopic Explorer (MUSE) instrument provides a
wide field of view (FoV) of 1'x1', with a spatial sampling of
0.2"x0.2" per pixel, thus, the spatial resolution is seeing limited.
MUSE covers the whole optical range from 4750 to 9300Å, with a
spectral sampling of 1.25Å, and a full width at half maximum (FWHM)
that depends slightly on the wavelength, being ∼2.4Å at the red
part of the spectrum (at 7500Å).
We selected galaxies observed with MUSE (FWHM∼1") from the European
Southern Observatory (ESO) archive, acquired until 2018-August with
redshifts below z<0.1. See Section 2 for further explanations.
File Summary:
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FileName Lrecl Records Explanations
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ReadMe 80 . This file
table2.dat 95 66 Main properties of the galaxies hosting outflows
found in All-weather MUse Supernova Integral-field
of Nearby Galaxies (AMUSING++)
table3.dat 149 635 Isophotal parameters derived for the AMUSING++
galaxies
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See also:
B/eso : ESO Science Archive Catalog (ESO, 1991-2020)
J/A+A/459/55 : Narrow-band imaging of 5 Seyfert-1 galaxies (Bennert+, 2006)
J/ApJ/716/198 : The DiskMass survey. I. (Bershady+, 2010)
J/ApJ/711/284 : Galaxy Zoo: AGN host galaxies (Schawinski+, 2010)
J/ApJ/709/884 : Role of starburst-AGN composites LIRG mergers (Yuan+, 2010)
J/ApJ/731/120 : Intrinsic SN Ia light curves (Mandel+, 2011)
J/ApJ/746/L22 : Dual AGNs in the nearby Universe (Koss+, 2012)
J/A+A/573/A59 : Gas kinematics in CALIFA survey (Garcia-Lorenzo+, 2015)
J/ApJS/224/38 : SPOGS I Shocked POststarburst Galaxy cand. (Alatalo+, 2016)
J/MNRAS/460/1758 : Optical emission lines, galaxy cluster cores 1 (Hamer+,2016)
J/A+A/594/A36 : CALIFA Survey DR3 list of galaxies (Sanchez+, 2016)
J/MNRAS/466/2570 : Low ionization emission-line regions (Belfiore+, 2017)
J/MNRAS/468/3965 : SAMI Galaxy Survey. Gas surface densities (Federrath+, 2017)
J/A+A/602/A85 : SN 1998bw MUSE datacube (Kruehler+, 2017)
J/A+A/606/A12 : MUSE-Wide survey: 831 emission line galaxies (Herenz+, 2017)
J/A+A/608/A2 : MUSE Hubble Ultra Deep Field Survey. II. (Inami+, 2017)
J/A+A/608/A8 : MUSE Hubble Ultra Deep Field Survey. VIII (Leclercq+, 2017)
J/ApJS/230/1 : Herschel SPIRE/FTS 194-671um survey GOALS LIRGs (Lu+, 2017)
J/AJ/154/86 : MaNGA catalog, DR15 (Wake+, 2017)
J/A+A/612/A19 : Abell 2052 VLT/MUSE datacubes (Balmaverde+, 2018)
J/A+A/614/A94 : ESO 362-G18 datacube (Humire+, 2018)
J/A+A/629/A57 : Supernova ASASSN-14jb light curves and spectra (Meza+, 2019)
J/A+A/622/A146 : MAGNUM survey galaxies images (Mingozzi+, 2019)
J/A+A/623/A122 : Sample of MaNGA galaxies properties (Pilyugin+, 2019)
Byte-by-byte Description of file: table2.dat
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Bytes Format Units Label Explanations
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1- 14 A14 --- ID AMUSING++ identifier
16- 39 A24 --- Gal Galaxy name
41- 46 F6.4 --- z [0.001/0.09] Redshift derived with SSP analysis
48- 52 A5 --- MType ? Hyperleda Hubble type
54- 57 F4.1 deg inc [8.1/81.1] Inclination
59- 63 F5.1 deg PA [1.9/175] Position angle
65- 68 F4.1 arcsec Reff [4.8/96.2] Effective radius
70- 73 F4.1 [Msun] logM [8.8/12] log of stellar mass derived
with SSP analysis
75- 79 F5.2 [Msun/yr] logSFR [-2.18/1.69] log of star formation rate
81- 87 A7 --- Nuc Source of the outflow based on the nuclear
ionization
89- 91 I3 km/s W90 [10/184]? W90 of the absolute value of the
median on the asymmetry map
93- 95 A3 --- Ref References (1)
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Note (1): References as follows:
1 = Bonatto & Pastoriza, 1997ApJ...486..132B 1997ApJ...486..132B; Yuan+, 2010, J/ApJ/709/884
2 = Prieto+, 2016ApJ...830L..32P 2016ApJ...830L..32P
3 = Mingozzi+, 2019, J/A+A/622/A146
4 = Mulchaey+, 1996ApJS..102..309M 1996ApJS..102..309M; Fraquelli+, 2000ApJ...532..867F 2000ApJ...532..867F;
Humire+, 2018, J/A+A/614/A94
5 = Gadotti+, 2019MNRAS.482..506G 2019MNRAS.482..506G
6 = Rich+, 2010ApJ...721..505R 2010ApJ...721..505R, Vogt+, 2013ApJ...768..151V 2013ApJ...768..151V
7 = Barbosa+, 2009MNRAS.396....2B 2009MNRAS.396....2B
8 = Durre & Mould, 2018ApJ...867..149D 2018ApJ...867..149D, 2019ApJ...870...37D 2019ApJ...870...37D
9 = Lopez-Coba+, 2017ApJ...850L..17L 2017ApJ...850L..17L
10 = Falcke+, 1998ApJ...502..199F 1998ApJ...502..199F
11 = Venturi+, 2018agn..confE..50V
12 = Poggianti+, 2019MNRAS.482.4466P 2019MNRAS.482.4466P
13 = Lopez-Coba+, 2019MNRAS.482.4032L 2019MNRAS.482.4032L
14 = Rafanelli & Marziani+, 1992AJ....103..743R 1992AJ....103..743R
15 = Rich+, 2015ApJS..221...28R 2015ApJS..221...28R
16 = Muller-Sanchez+, 2018Natur.556..345M 2018Natur.556..345M; Treister+, 2018ApJ...854...83T 2018ApJ...854...83T
17 = Rich+, 2011ApJ...734...87R 2011ApJ...734...87R
18 = Bik+, 2015A&A...576L..13B 2015A&A...576L..13B
19 = Powell+, 2018A&A...618A..27P 2018A&A...618A..27P
20 = Husemann+, 2019A&A...627A..53H 2019A&A...627A..53H
21 = Menacho+, 2019MNRAS.487.3183M 2019MNRAS.487.3183M
22 = Venturi+, 2017FrASS...4...46V 2017FrASS...4...46V
23 = Dahlem+, 1997A&A...320..731D 1997A&A...320..731D
24 = Heckman+, 2015ApJ...809..147H 2015ApJ...809..147H
25 = Davies+, 2014MNRAS.444.3961D 2014MNRAS.444.3961D
26 = Farage+, 2012ApJ...747...28F 2012ApJ...747...28F; Canning+, 2013MNRAS.435.1108C 2013MNRAS.435.1108C;
Olivares+, 2019A&A...631A..22O 2019A&A...631A..22O
27 = Donahue+, 2007AJ....134...14D 2007AJ....134...14D
28 = Balmaverde+, 2018, J/A+A/612/A19
29 = Jarvis, 1990A&A...240L...8J 1990A&A...240L...8J; Sparks+, 1993ApJ...413..531S 1993ApJ...413..531S;
Gavazzi+, 2000A&A...361....1G 2000A&A...361....1G
30 = Bower+, 1997ApJ...483L..33B 1997ApJ...483L..33B
31 = Storchi-Bergmann & Bonatto, 1991MNRAS.250..138S 1991MNRAS.250..138S
32 = Prieto+, 1993MNRAS.263...10P 1993MNRAS.263...10P
33 = Solorzano-Inarrea & Tadhunter, 2003MNRAS.340..705S 2003MNRAS.340..705S
34 = Monreal-Ibero+, 2010A&A...517A..28M 2010A&A...517A..28M
35 = Edwards+, 2009MNRAS.396.1953E 2009MNRAS.396.1953E
36 = McDonald+, 2011ApJ...731...33M 2011ApJ...731...33M
37 = Santoro+, 2015A&A...575L...4S 2015A&A...575L...4S
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Byte-by-byte Description of file: table3.dat
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Bytes Format Units Label Explanations
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1- 3 I3 --- Seq [0/634] Running sequence number
5- 27 A23 --- ID AMUSING++ identifier
29- 56 A28 --- Gal Galaxy name
58- 59 I2 h RAh [0/23] Hour of Right Ascension (J2000)
61- 62 I2 min RAm Minute of Right Ascension (J2000)
64- 69 F6.3 s RAs Second of Right Ascension (J2000)
71 A1 --- DE- Sign of the Declination (J2000)
72- 73 I2 deg DEd Degree of Declination (J2000)
75- 76 I2 arcmin DEm Arcminute of Declination (J2000)
78- 83 F6.3 arcsec DEs Arcsecond of Declination (J2000)
85- 90 F6.4 --- z [0.0002/0.2] Redshift derived with the SSP
analysis
92- 96 F5.3 kpc/arcsec Scale [0.004/3.3] Angular scale
98-101 A4 --- MType Hyperleda Hubble type
103-109 F7.4 [Msun/yr] logSFR [-7.9/2.4] Integrated star formation rate
111-115 F5.2 [Msun] logM [4.7/12.81] Integrated stellar mass
117-120 F4.1 deg inc [0/85] Inclination
122-126 F5.1 deg PA [0/180] Position Angle
128-131 F4.1 arcsec Reff [0/65.1] Effective radius
133-137 F5.2 --- r1 [-1/1]? First correlation coefficient (1)
139-143 F5.2 --- r2 [-0.8/1]? Second correlation coefficient (1)
145-149 F5.1 km/s Vel [0/786]? Velocity difference (2)
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Note (1): Correlation coefficients between σ and the log[NII]/Hα
ratio for spaxels lying bellow and above the
Kewley+, 2001ApJ...556..121K 2001ApJ...556..121K curve.
Note (2): W90 of the difference between the gas and stellar kinematics for
spaxels lying above the Kewley+, 2001ApJ...556..121K 2001ApJ...556..121K curve.
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History:
From electronic version of the journal
(End) Prepared by [AAS], Coralie Fix [CDS], 18-May-2020