J/MNRAS/481/3497 JINGLE, Survey overview and first results (Saintonge+, 2018)
JINGLE, a JCMT legacy survey of dust and gas for galaxy evolution studies.
I. Survey overview and first results.
Saintonge A., Wilson C.D., Xiao T., Lin L., Hwang H.S., Tosaki T.,
Bureau M., Cigan P.J., Clark C.J.R., Clements D.L., De Looze I.,
Dharmawardena T., Gao Y., Gear W.K., Greenslade J., Lamperti I., Lee J.C.,
Li C., Michalowski M.J., Mok A., Pan H.-A., Sansom A.E., Sargent M.,
Smith M.W.L., Williams T., Yang C., Zhu M., Accurso G., Barmby P.,
Brinks E., Bourne N., Brown T., Chung A., Chung E.J., Cibinel A.,
Coppin K., Davies J., Davis T.A., Eales S., Fanciullo L., Fang T., Gao Y.,
Glass D.H.W., Gomez H.L., Greve T., He J., Ho L.C., Huang F., Jeong H.,
Jiang X., Jiao Q., Kemper F., Kim J.H., Kim M., Kim T., Ko J., Kong X.,
Lacaille K., Lacey C.G., Lee B., Lee J.H., Lee W.-K., Masters K., Oh S.-H.,
Papadopoulos P., Park C., Park S.-J., Parsons H., Rowlands K., Scicluna P.,
Scudder J.M., Sethuram R., Serjeant S., Shao Y., Sheen Y.-K., Shi Y.,
Shim H., Smith C.M.A., Spekkens K., Tsai A.-L., Verma A., Urquhart S.,
Violino G., Viti S., Wake D., Wang J., Wouterloot J., Yang Y., Yim K.,
Yuan F., Zheng Z.
<Mon. Not. R. Astron. Soc., 481, 3497-3519 (2018)>
=2018MNRAS.481.3497S 2018MNRAS.481.3497S (SIMBAD/NED BibCode)
ADC_Keywords: Interstellar medium ; Galaxies, photometry ; Surveys
Keywords: ISM: general - galaxies: evolution - galaxies: ISM -
galaxies: photometry
Abstract:
JINGLE is a new JCMT legacy survey designed to systematically study
the cold interstellar medium of galaxies in the local Universe. As
part of the survey we perform 850µm continuum measurements with
SCUBA-2 for a representative sample of 193 Herschel-selected galaxies
with M*> 109M☉, as well as integrated CO(2-1) line fluxes with
RxA3m for a subset of 90 of these galaxies. The sample is selected
from fields covered by the Herschel-ATLAS survey that are also
targeted by the MaNGA optical integral-field spectroscopic survey. The
new JCMT observations combined with the multiwavelength ancillary data
will allow for the robust characterization of the properties of dust
in the nearby Universe, and the benchmarking of scaling relations
between dust, gas, and global galaxy properties. In this paper we give
an overview of the survey objectives and details about the sample
selection and JCMT observations, present a consistent 30-band
UV-to-FIR photometric catalogue with derived properties, and introduce
the JINGLE Main Data Release. Science highlights include the
non-linearity of the relation between 850µm luminosity and CO line
luminosity (logLCO(2-1)=1.372logL850-1.376), and the serendipitous
discovery of candidate z>6 galaxies.
Description:
JINGLE is a SCUBA-2 survey at 850µm of 193 galaxies, with about half
of the galaxies also being observed in the CO J=2-1 line [hereafter,
CO(2-1)] using the RxA3m instrument. The sample consists of
Herschel-detected galaxies probing the star formation main sequence
above M*=109M☉. Amongst several other data products, the JCMT
observations importantly provide total, integrated molecular gas
masses through the CO(2-1) line measurements as well as accurate
dust masses from the modelling of the 850µm and other infrared
photometric points.
To achieve our science goals, we need to observe a statistically
significant galaxy sample and obtain homogeneous data products with
the JCMT, making use of both RxA3m and SCUBA-2. We also require the
following ancillary multiwavelength data products: Herschel photometry
to combine with the JCMT 850µm fluxes to derive accurate dust
masses, temperatures, and emissivities; optical integral field
spectroscopy (IFS) to derive spatially resolved (i.e. gradients)
stellar and ionized gas properties, including metallicities; HI
observations (at the minimum integrated measurements, but ideally
resolved maps) to quantify atomic gas masses within the same physical
region of the galaxies as the CO and dust measurements.
File Summary:
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FileName Lrecl Records Explanations
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ReadMe 80 . This file
table2.dat 510 193 JINGLE sample catalog
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Byte-by-byte Description of file: table2.dat
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Bytes Format Units Label Explanations
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1- 24 A24 --- SDSS SDSS Name (SDSS JHHMMSS.ss+DDMMSS.s)
26- 34 A9 --- JINGLE Jingle catalog ID (JINGLENNN)
36- 38 I3 --- IDNUM Jingle catalog number
40- 59 A20 --- SDSSID 5-part SDSS ID
61- 79 I19 --- ObjID SDSS Unique Object Identifier
81- 99 I19 --- SpecObjID SDSS Spectroscopic Object Identifier
101-104 I4 --- Plate SDSS Spectroscopic Plate ID
106-110 I5 --- MJD SDSS Spectroscopic MJD ID
112-114 I3 --- Fiber SDSS Spectroscopic Fiber ID
116-125 F10.6 deg RAdeg Right ascension (J2000)
127-135 F9.6 deg DEdeg Declination (J2000)
137-143 F7.5 --- z SDSS spectroscopic redshift
145-151 F7.5 --- e_z Error on z
153-160 F8.4 Mpc Dist Luminosity distance (Ωm=0.3,
ΩL=0.7, H0=70km/s/Mpc)
162-163 I2 --- AGNclass BPT-based AGN classification (1)
165-176 F12.8 --- [N2/Ha] ?=-99 NII(6583)/Hα emission line
ratio
178-189 F12.8 --- [O3/Hb] ?=-99 OIII(5006)/Hβ emission line
ratio
191-200 F10.6 --- N2PP04 ?=-99 12+log(O/H) from N2/Ha (2)
202-211 F10.6 --- O3N2PP04 ?=-99 12+logO/H from N2/Ha and
O3/Hb (2)
213-220 F8.6 --- MZR 12+logO/H from MZR, Kewley & Ellison
(2008ApJ...681.1183K 2008ApJ...681.1183K), PP04
calibration, using the MAGPHYS stellar
mass (MstarMAG)
222-227 F6.3 [Msun] MstarMGC Star mass from MAGPHYS and CAAPR
photometry
229-234 F6.4 [Msun] e_MstarMGC Error on MstarMAG
236-244 F9.6 [Msun] MstarGRA Star mass from GRASIL and CAAPR
photometry
246-255 F10.6 [Msun] MstarWISE Star mass from CAAPR WISE 3.6µm
(assuming M/L=0.47)
257-266 F10.6 [Msun] e_MstarWISE ?=-99 Error on MstarWISE
268-276 F9.6 [Msun] MstarMPA Star mass from MPA/JHU catalog
278-285 F8.6 [Msun] e_MstarMPA Error on MstarMPA
287-296 F10.6 [Msun] MstarBC03 Star mass from SDSS DR10, Wisconsin
method
298-307 F10.6 [Msun] e_MstarBC03 ?=-99 Error on MstarBC03
309-316 F8.6 [Msun/kpc2] logmu Stellar mass surface density (3)
318-325 F8.6 --- Cindex Concentration index (ratio of r-band
Petrosian r90 and r50) (4)
327-334 F8.6 --- b/a b/a from SDSS 2D exponential fit in
r-band
336-343 F8.5 deg Incl Disc inclination
345-353 F9.6 kpc PerRad SDSS r-band Petrosian radius
355-362 F8.6 kpc r50 SDSS r-band Petrosian R50
364 I1 --- Morph Galaxy morphology from Galaxy Zoo
(2011MNRAS.410..166L 2011MNRAS.410..166L,
Cat. J/MNRAS/410/166) or Choi
(2010JKAS...43..191C 2010JKAS...43..191C) (5)
366-367 I2 --- Morphjin ?=-9 JINGLE consensus morphology
comparing classifications from NED,
Tempel, Kuminski and Galaxy Zoo +
visual inspection for galaxies where
these four sources were
inconsistent (5)
369-370 I2 --- MorphTemp Morphology from Tempel et al.
(2014A&A...566A...1T 2014A&A...566A...1T) (6)
372-377 F6.3 [Msun/yr] SFRMAG SFR from MAGPHYS and CAAPR photometry
379-384 F6.4 [Msun/yr] e_SFRMAG Error on SFRMAG
386-394 F9.6 [Msun/yr] SFRGRA SFR from GRASIL and CAAPR photometry
396-404 F9.6 [Msun/yr] SFRMPA SFR from SDSS MPA/JHU catalog
406-413 F8.6 [Msun/yr] e_SFRMPA Error on SFRMPA
415-424 F10.6 [Msun/yr] SFRIRFUV SFR from WISE 12um + GALEX FUV (CAAPR)
426-435 F10.6 [Msun/yr] e_SFRIRFUV ?=-99.000000 Error on SFRIRFUV
437-445 F9.6 [Msun/yr] SFRFUVCE01 SFR from FUV + LTIR using CE01
templates
447-454 F8.6 [Msun/yr] e_SFRFUVCE01 Error on SFRFUVCE01
456-464 F9.6 [Msun/yr] SFRFUVJRM SFR from FUV + LTIR using JRM templates
466-473 F8.6 [Msun/yr] e_SFRFUVJRM Error on SFRFUVJRM
475-484 F10.6 --- AIRX AIRX (effective UV attenuation) from
CAAPR photometry
486-493 F8.6 mag FUV-Ks ? FUV-Ks colour from CAAPR photometry
495-503 F9.5 [Msun] MHaloTemp Halo mass from Tempel catalog for
galaxies classified as central or
satellite
505-507 I3 --- GroupRank Ranking of the galaxy in its group,
from Tempel
509-510 I2 --- GroupClass [1/3]?=-9 Classification based on
Tempel (1 : isolated, 2 : central,
3 : satellite)
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Note (1): AGN classification as follows:
-1 = Undetermined
0 = Inactive
1 = SFing
2 = Composite
3 = AGN
4 = Seyfert
Note (2): Gas-phase metallicity calculated from optical strong emission lines
measured in the SDSS spectra using the O3N2 calibration of
Pettini & Pagel (2004MNRAS.348L..59P 2004MNRAS.348L..59P, hereafter PP04). In cases where
the emission lines are not all detected or where their excitation is
likely to be influenced by the presence of an AGN, then we use the
value derived from the mass-metallicity relation as derived by
Kewley & Elison (2008ApJ...681.1183K 2008ApJ...681.1183K) to be on the same PP04 scale.
Note (3): Calculated as log(µ*)=log(M*/(2*π*r2)) where M* is from
MAGPHYS and r is the Petrosian half-light radius in the z band in
units of kiloparsec
Note (4): Cindex is a measure of how centrally concentrated the light of the
galaxy is with values above 2.5 indicative of a significant stellar
bulge contribution to the total light
Note (5): Morphology as follows:
1 = spiral
2 = elliptical
Note (6): Morphology from Tempel as follows:
-9 = no data
0 = uncertain
1 = spiral
2 = elliptical
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History:
From electronic version of the journal
(End) Ana Fiallos [CDS] 09-Jun-2022