J/ApJS/259/37 IDEOS. II. Observables in the 5.4-36µm range (Spoon+, 2022)
The Infrared Database of Extragalactic Observables from Spitzer.
II. The database and diagnostic power of crystalline silicate features in galaxy
spectra.
Spoon H.W.W., Hernan-Caballero A., Rupke D., Waters L.B.F.M.,
Lebouteiller V., Tielens A.G.G.M., Loredo T., Su Y., Viola V.
<Astrophys. J. Suppl. Ser., 259, 37 (2022)>
=2022ApJS..259...37S 2022ApJS..259...37S
ADC_Keywords: Galaxies, IR; Spectra, infrared; Redshifts; Equivalent widths
Keywords: Infrared galaxies ; Starburst galaxies ; Active galaxies ;
Interstellar medium ; Silicate grains ;
Polycyclic aromatic hydrocarbons ; Astrochemistry ;
Galaxy spectroscopy ; LINER galaxies ;
Ultraluminous infrared galaxies ; Dust continuum emission
Abstract:
We present the Infrared Database of Extragalactic Observables from
Spitzer (IDEOS), a homogeneous, publicly available, database of
77 fitted mid-infrared observables in the 5.4-36µm range,
comprising measurements for 3335 galaxies observed in the
low-resolution staring mode of the Infrared Spectrometer on board the
Spitzer Space Telescope. Among the included observables are polycyclic
aromatic hydrocarbon fluxes and their equivalent widths, the strength
of the 9.8µm silicate feature, emission-line fluxes, solid-state
features, rest-frame continuum fluxes, synthetic photometry, and a
mid-infrared spectral classification. The IDEOS spectra were selected
from the Cornell Atlas of Spitzer-IRS Sources. To our surprise, we
have detected at a >95% confidence level crystalline silicates in the
spectra of 786 IDEOS galaxies. The detections range from single-band
detections to detections of all fitted crystalline bands (16, 19, 23,
28, and 33µm). We find the strength of the crystalline silicate
bands to correlate with the amorphous silicate strength and the change
from an emission to an absorption feature to occur at higher
obscuration as the wavelength of the crystalline silicate band is
longer. These observed characteristics are consistent with an origin
for the amorphous and crystalline silicate features in a centrally
heated dust geometry, either an edge-on disk or a cocoon. We find the
23 and 33µm crystalline silicate bands to be well suited to
classify the obscuration level of galactic nuclei, even in the
presence of strong circumnuclear star formation. Based on our
detection statistics, we conclude that crystalline silicates are a
common component of the interstellar medium of galactic nuclei.
Description:
The Infrared Database of Extragalactic Observables from Spitzer
(IDEOS) builds on the publication-quality IRS spectra in the Combined
Atlas of Sources with Spitzer IRS Spectra (CASSIS) repository.
See Section 2.
File Summary:
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FileName Lrecl Records Explanations
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ReadMe 80 . This file
table6.dat 1713 3559 IDEOS observables
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See also:
J/PASP/119/994 : MIPS 24um calibrators (Engelbracht+, 2007)
J/ApJ/656/770 : Mid-IR spectrum of star-forming galaxies (Smith+, 2007)
J/ApJS/184/230 : Spitzer high-res. MIR spectral atlas (Bernard-Salas+, 2009)
J/ApJS/182/628 : Spitzer quasar and ULIRG evolution study (Veilleux+, 2009)
J/ApJ/723/993 : Spatial extent of (U)LIRGs in MIR. I. (Diaz-Santos+, 2010)
J/MNRAS/427/3209 : Galactic and MC O-AGBs and RSGs stars (Jones+, 2012)
J/ApJ/803/109 : Spitzer/IRS AGN sp. decomposition (Hernan-Caballero+, 2015)
J/MNRAS/455/1796 : IDEOS redshift catalogue (Hernan-Caballero+, 2016)
J/A+A/607/A43 : NGC 4418/VV 655 HI images (Varenius+, 2017)
J/A+A/630/A143 : Magnesium & Si K-edges cross sections (Rogantini+, 2019)
J/A+A/627/A16 : Si K-edge dust absorption cross sections (Zeegers+, 2019)
J/ApJ/905/55 : Bright-PAH galaxies from AKARI & Spitzer (Lai+, 2020)
http://cassis.sirtf.com/ : Combined Atlas of Sources with Spitzer IRS Spectra
http://ideos.astro.cornell.edu/ : IDEOS home page
Byte-by-byte Description of file: table6.dat
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 11 A11 --- Name IDEOS identifier
13- 44 A32 --- Galaxy NED galaxy identifier
46- 54 F9.5 deg RAdeg Right Ascension (J2000) (3)
56- 64 F9.5 deg DEdeg [-87/86.4] Declination (J2000) (3)
66- 73 F8.5 --- z [-0.00016/6.42] Redshift (Paper I;
Hernan-Caballero+,
2016, J/MNRAS/455/1796)
75- 78 A4 --- IRCl Mid-infrared classification (1)
80 A1 --- l_FPAH6.2 Limit on FPAH6.2
82- 90 E9.3 W/m2 FPAH6.2 [3.7e-19/8e-14]? Integrated 6.2um
PAH flux: spline-method
92- 100 E9.3 W/m2 e_FPAH6.2 [3e-19/1.4e-15]? Error in FPAH6.2
102 A1 --- l_EWPAH6.2 Limit on PAH62EQW
104- 109 F6.4 um EWPAH6.2 [0.0009/1.7]? Equivalent width of
the 6.2 micron PAH flux:
spline-method
111- 116 F6.4 um e_EWPAH6.2 [0.0004/0.4]? Error in EWPAH6.2
118 A1 --- l_FPAH11.2 Limit on FPAH11.2
120- 128 E9.3 W/m2 FPAH11.2 [5e-19/6.2e-14]? Integrated 11.2um
PAH flux: spline-method
130- 138 E9.3 W/m2 e_FPAH11.2 [3e-19/1.3e-15]? Error in FPAH11.2
140 A1 --- l_EWPAH11.2 Limit on PAH11EQW
142- 147 F6.4 um EWPAH11.2 [0.0019/2.5]? Equivalent width of
the 11.2 micron PAH flux:
spline-method
149- 154 F6.4 um e_EWPAH11.2 [0.0005/1.8]? Error in EWPAH11.2
156 A1 --- l_FPAH12.7 Limit on FPAH12.7
158- 166 E9.3 W/m2 FPAH12.7 [8e-19/3.1e-14]? Integrated 12.7um
PAH flux: spline-method
168- 176 E9.3 W/m2 e_FPAH12.7 [5e-19/1.6e-15]? Error in FPAH12.7
178 A1 --- l_EWPAH12.7 Limit on EWPAH12.7
180- 187 F8.6 um EWPAH12.7 [0.0024/7]? Equivalent width of the
12.7 micron PAH flux: spline-method
189- 196 F8.6 um e_EWPAH12.7 [0.0006/0.5]? Error in EWPAH12.7
198 A1 --- l_FPAH6.2Drude Limit on FPAH6.2Drude
200- 208 E9.3 W/m2 FPAH6.2Drude [0/1.2e-13]? Integrated 6.2 micron
PAH flux: decomposition-method
210- 218 E9.3 W/m2 e_FPAH6.2Drude [0/8.6e-16]? Error in FPAH6.2Drude
220 A1 --- l_EWPAH6.2Drude Limit on EWPAH6.2Drude
222- 230 F9.6 um EWPAH6.2Drude [0/54]? Equivalent width of the
6.2um PAH flux:
decomposition-method
232- 239 F8.6 um e_EWPAH6.2Drude [0]? Error in EWPAH6.2Drude
(always "0.000000" or blank)
241 A1 --- l_FPAH7.7Drude Limit on FPAH7.7Drude
243- 251 E9.3 W/m2 FPAH7.7Drude [0/4.7e-13]? Integrated 7.7 micron
PAH flux: decomposition-method
253- 261 E9.3 W/m2 e_FPAH7.7Drude [0/6.3e-15]? Error in FPAH7.7Drude
263 A1 --- l_EWPAH7.7Drude Limit on EWPAH7.7Drude
265- 273 F9.6 um EWPAH7.7Drude [0/62]? Equivalent width of the
7.7um PAH flux:
decomposition-method
275- 282 F8.6 um e_EWPAH7.7Drude [0]? Error in EWPAH7.7Drude
(always "0.000000" or blank)
284 A1 --- l_FPAH11.2Drude Limit on FPAH11.2Drude
286- 294 E9.3 W/m2 FPAH11.2Drude [0/9e-14]? Integrated 11.2 micron
PAH flux: decomposition-method
296- 304 E9.3 W/m2 e_FPAH11.2Drude [0/1.3e-15]? Error in FPAH11.2Drude
306 A1 --- l_EWPAH11.2Drude Limit on EWPAH11.2Drude
308- 316 F9.6 um EWPAH11.2Drude [0/29]? Equivalent width of the
11.2 micron PAH flux:
decomposition-method
318- 325 F8.6 um e_EWPAH11.2Drude [0]? Error in EWPAH11.2Drude
(always "0.000000" or blank)
327 A1 --- l_FPAHTotDrude Limit on FPAHTotDrude
329- 337 E9.3 W/m2 FPAHTotDrude [0/1.1e-12]? Integrated 5-18um PAH
flux: decomposition-method
339- 347 E9.3 W/m2 e_FPAHTotDrude [0/6.6e-15]? Error in FPAHTotDrude
349 A1 --- l_FMIRDrude Limit on FMIRDrude
351- 359 E9.3 W/m2 FMIRDrude [1.4e-17/2.2e-12]? Integrated
5-25um continuum flux:
decomposition-method
361- 369 E9.3 W/m2 e_FMIRDrude [0]? Error in FMIRDrude
(always "0.00e+00" or blank)
371- 378 A8 --- MethDrude Origin of the decomposition method
fluxes ("PAHFit" or "QuestFit")
380 A1 --- l_SilStrength Limit on SilStrength
382- 387 F6.3 --- SilStrength [-4.2/0.9]? Strength of the 9.8um
silicate feature
389- 393 F5.3 --- e_SilStrength [0.001/0.9]? Error in SilStrength
395- 402 A8 --- SilFitType Interpolation method used to create
local continuum: powerlaw or spline
404- 413 A10 --- SilAnchorType Origin of anchors for continuum
interpolation: automatically
chosen, manual choice, or
DEBLENDIRS
415 A1 --- l_Cryst19Strength [N >] Limit on Cryst19Strength (2)
417- 422 F6.3 --- Cryst19Strength [-1.2/-0.004]? Strength of the 19um
crystalline silicate feature
424- 428 F5.3 --- e_Cryst19Strength [0.002/0.04]? Error in
Cryst19Strength
430 A1 --- l_Cryst23Strength [N >] Limit on Cryst23Strength (2)
432- 437 F6.3 --- Cryst23Strength [-0.3/0.8]? Strength of the 23um
crystalline silicate feature
439- 443 F5.3 --- e_Cryst23Strength [0.003/0.04]? Error in
Cryst23Strength
445 A1 --- l_Cryst28Strength [N >] Limit on Cryst28Strength (2)
447- 452 F6.3 --- Cryst28Strength [-0.06/1.2]? Strength of the 28um
crystalline silicate feature
454- 458 F5.3 --- e_Cryst28Strength [0.003/0.02]? Error in
Cryst28Strength
460 A1 --- l_Cryst33Strength [N >] Limit on Cryst33Strength (2)
462- 467 F6.3 --- Cryst33Strength [-0.07/1.9]? Strength of the 33um
crystalline silicate feature
469- 473 F5.3 --- e_Cryst33Strength [0.004/0.1]? Error in
Cryst33Strength
475- 479 F5.3 --- TauIce [0.015/1.3]? Optical depth of the
6um water ice feature
481- 485 F5.3 --- e_TauIce [0.006/0.3]? Error in TauIce
487- 491 F5.3 --- Tau685 [0.019/1.5]? Optical depth of the
6.85um hydrocarbon feature
493- 497 F5.3 --- e_Tau685 [0.003/0.2]? Error in Tau685
499 A1 --- l_Ar2Flux Limit on Ar2Flux
501- 509 E9.3 W/m2 Ar2Flux [2.4e-19/3.7e-15]? Integrated
6.99um [Ar II] line flux
511- 519 E9.3 W/m2 e_Ar2Flux [9.8e-20/3e-16]? Error in Ar2Flux
521 A1 --- l_Ar3Flux Limit on Ar3Flux
523- 531 E9.3 W/m2 Ar3Flux [3.5e-19/10e-16]? Integrated 8.99um
[Ar III] line flux
533- 541 E9.3 W/m2 e_Ar3Flux [2e-19/2.2e-16]? Error in Ar3Flux
543 A1 --- l_Cl2Flux Limit on Cl2Flux
545- 553 E9.3 W/m2 Cl2Flux [4.4e-19/3.6e-16]? Integrated
14.37um [Cl II] line flux
555- 563 E9.3 W/m2 e_Cl2Flux [4.4e-19/1.6e-16]? Error in Cl2Flux
565 A1 --- l_Fe2Flux Limit on Fe2Flux
567- 575 E9.3 W/m2 Fe2Flux [6e-19/1.4e-15]? Integrated 25.99um
[Fe II] line flux
577- 585 E9.3 W/m2 e_Fe2Flux [1.8e-19/5e-16]? Error in Fe2Flux
587 A1 --- l_H2S0Flux Limit on H2S0Flux
589- 597 E9.3 W/m2 H2S0Flux [6e-19/1.4e-15]? Integrated 28.22um
H_2 0-0 S(0) line flux
599- 607 E9.3 W/m2 e_H2S0Flux [4.3e-19/3e-17]? Error in H2S0Flux
609 A1 --- l_H2S1Flux Limit on H2S1Flux
611- 619 E9.3 W/m2 H2S1Flux [5.5e-19/1.2e-15]? Integrated
17.03um H_2 0-0 S(1) line flux
621- 629 E9.3 W/m2 e_H2S1Flux [3.7e-19/2.3e-16]? Error in
H2S1Flux
631 A1 --- l_H2S2Flux Limit on H2S2Flux
633- 641 E9.3 W/m2 H2S2Flux [4.4e-19/1.1e-15]? Integrated
12.28um H_2 0-0 S(2) line flux
643- 651 E9.3 W/m2 e_H2S2Flux [2e-19/3.2e-16]? Error in H2S2Flux
653 A1 --- l_H2S3Flux Limit on H2S3Flux
655- 663 E9.3 W/m2 H2S3Flux [4e-19/6.2e-16]? Integrated 9.66um
H_2 0-0 S(3) line flux
665- 673 E9.3 W/m2 e_H2S3Flux [1.3e-19/1.4e-16]? Error in
H2S3Flux
675 A1 --- l_H2S5Flux Limit on H2S5Flux
677- 685 E9.3 W/m2 H2S5Flux [1.5e-19/9.7e-16]? Integrated
6.91um H_2 0-0 S(5) line flux
687- 695 E9.3 W/m2 e_H2S5Flux [1.2e-19/1.2e-16]? Error in
H2S5Flux
697 A1 --- l_H2S7Flux Limit on H2S7Flux
699- 707 E9.3 W/m2 H2S7Flux [3.9e-19/8.7e-16]? Integrated
5.51um H_2 0-0 S(7) line flux
709- 717 E9.3 W/m2 e_H2S7Flux [1e-19/1.2e-16]? Error in H2S7Flux
719 A1 --- l_Ne2Flux Limit on Ne2Flux
721- 729 E9.3 W/m2 Ne2Flux [4.8e-19/2e-14]? Integrated 12.81um
[Ne II] line flux
731- 739 E9.3 W/m2 e_Ne2Flux [1.8e-19/8.8e-16]? Error in Ne2Flux
741 A1 --- l_Ne3-15Flux Limit on Ne3-15Flux
743- 751 E9.3 W/m2 Ne3-15Flux [4.3e-19/3.8e-15]? Integrated
15.56um [Ne III] line flux
753- 761 E9.3 W/m2 e_Ne3-15Flux [1.4e-19/1.2e-16]? Error in
Ne3-15Flux
763 A1 --- l_Ne3-36Flux Limit on Ne3-36Flux
765- 773 E9.3 W/m2 Ne3-36Flux [1.7e-18/4.2e-15]? Integrated
36.01um [Ne III] line flux
775- 783 E9.3 W/m2 e_Ne3-36Flux [1.5e-18/1.8e-16]? Error in
Ne3-36Flux
785 A1 --- l_Ne5-14Flux Limit on Ne5-14Flux
787- 795 E9.3 W/m2 Ne5-14Flux [4e-19/1.2e-15]? Integrated 14.32um
[Ne V] line flux
797- 805 E9.3 W/m2 e_Ne5-14Flux [1.6e-19/1.5e-16]? Error in
Ne5-14Flux
807 A1 --- l_Ne5-24Flux Limit on Ne5-24Flux
809- 817 E9.3 W/m2 Ne5-24Flux [5.9e-19/1.2e-15]? Integrated
24.32um [Ne V] line flux
819- 827 E9.3 W/m2 e_Ne5-24Flux [3.2e-19/9.2e-17]? Error in
Ne5-24Flux
829 A1 --- l_O4Flux Limit on O4Flux
831- 839 E9.3 W/m2 O4Flux [6.2e-19/3e-15]? Integrated 25.89um
[O IV] line flux
841- 849 E9.3 W/m2 e_O4Flux [2e-19/5.6e-14]? Error in O4Flux
851 A1 --- l_S3-18Flux Limit on S3-18Flux
853- 861 E9.3 W/m2 S3-18Flux [6.2e-19/6.7e-15]? Integrated
18.71um [S III] line flux
863- 871 E9.3 W/m2 e_S3-18Flux [2.6e-19/1.5e-16]? Error in
S3-18Flux
873 A1 --- l_S3-33Flux Limit on S3-33Flux
875- 883 E9.3 W/m2 S3-33Flux [1.2e-18/9e-15]? Integrated 33.48um
[S III] line flux
885- 893 E9.3 W/m2 e_S3-33Flux [3.8e-19/4.6e-16]? Error in
S3-33Flux
895 A1 --- l_S4Flux Limit on S4Flux
897- 905 E9.3 W/m2 S4Flux [3.3e-19/2.3e-15]? Integrated
10.51um [S IV] line flux
907- 915 E9.3 W/m2 e_S4Flux [1.5e-19/2.5e-16]? Error in S4Flux
917 A1 --- l_Si2Flux Limit on Si2Flux
919- 927 E9.3 W/m2 Si2Flux [1e-18/2.1e-14]? Integrated 34.82um
[Si II] line flux
929- 937 E9.3 W/m2 e_Si2Flux [5.7e-19/1.4e-15]? Error in Si2Flux
939 A1 --- l_Ar3Ar2Ratio Limit on Ar3Ar2Ratio
941- 948 E8.2 --- Ar3Ar2Ratio [0.012/9.2]? Ratio of the 8.99um
[ArIII] line to the 6.99um [ArII]
line
950- 957 E8.2 --- e_Ar3Ar2Ratio [0.014/4.7]? Error in Ar3Ar2Ratio
959 A1 --- l_Ne3-15Ne2Ratio Limit on Ne3Ne2Ratio
961- 968 E8.2 --- Ne3-15Ne2Ratio [0.004/23]? Ratio of the 15.56um
[NeIII] line to the 12.81um [NeII]
line
970- 977 E8.2 --- e_Ne3-15Ne2Ratio [0.007/16.3]? Error in Ne3Ne2Ratio
979 A1 --- l_Ne5-14Ne2Ratio Limit on Ne5-14Ne2Ratio
981- 988 E8.2 --- Ne5-14Ne2Ratio [0.008/8]? Ratio of the 14.32um
[NeV] line to the 12.81um [NeII]
line
990- 997 E8.2 --- e_Ne5-14Ne2Ratio [0.008/2.1]? Error in
Ne5-14Ne2Ratio
999 A1 --- l_Ne5-24Ne2Ratio Limit on Ne5-24Ne2Ratio
1001- 1008 E8.2 --- Ne5-24Ne2Ratio [0.024/7.6]? Ratio of the 24.32um
[NeV] line to the 12.81um [NeII]
line
1010- 1017 E8.2 --- e_Ne5-24Ne2Ratio [0.016/2.1]? Error in
Ne5-24Ne2Ratio
1019 A1 --- l_O4Ne2Ratio Limit on O4Ne2Ratio
1021- 1028 E8.2 --- O4Ne2Ratio [0.02/37]? Ratio of the 25.89um
[OIV] line to the 12.81um [NeII]
line
1030- 1037 E8.2 --- e_O4Ne2Ratio [0.01/120]? Error in O4Ne2Ratio
1039 A1 --- l_O4S3-33Ratio Limit on O4S3-33Ratio
1041- 1048 E8.2 --- O4S3-33Ratio [0.027/9]? Ratio of the 25.89um
[OIV] line to the 33.48um [SIII]
line
1050- 1057 E8.2 --- e_O4S3-33Ratio [0.016/183]? Error in O4S3-33Ratio
1059 A1 --- l_O4S3-18Ratio Limit on O4S3-18Ratio
1061- 1068 E8.2 --- O4S3-18Ratio [0.03/29]? Ratio of the 25.89um
[OIV] line to the 18.71um [SIII]
line
1070- 1077 E8.2 --- e_O4S3-18Ratio [0.02/191]? Error in O4S3-18Ratio
1079 A1 --- l_S3-33S3-18Ratio Limit on S3-33S3-18Ratio
1081- 1088 E8.2 --- S3-33S3-18Ratio [0.3/33.2]? Ratio of the 33.48um
[SIII] line to the 18.71um [SIII]
line
1090- 1097 E8.2 --- e_S3-33S3-18Ratio [0.04/8.4]? Error in
S3-33S3-18Ratio
1099 A1 --- l_S4S3-18Ratio Limit on S4S3-18Ratio
1101- 1108 E8.2 --- S4S3-18Ratio [0.007/5.6]? Ratio of the 10.51um
[SIV] line to the 18.71um [SIII]
line
1110- 1117 E8.2 --- e_S4S3-18Ratio [0.013/1.3]? Error in S4S3-18Ratio
1119 A1 --- l_Si2S3-33Ratio Limit on Si2S3-33Ratio
1121- 1128 E8.2 --- Si2S3-33Ratio [0.23/11.6]? Ratio of the 34.82um
[SiII] line to the 33.48um [SIII]
line
1130- 1137 E8.2 --- e_Si2S3-33Ratio [0.02/2]? Error in Si2S3-33Ratio
1139- 1147 E9.3 mJy IRAC8Flux [0.14/6221]? Synthetic Spitzer IRAC
8um photometry
1149- 1157 E9.3 mJy e_IRAC8Flux [0.007/7]? Error in IRAC8Flux
1159- 1167 E9.3 mJy IRS15Flux [0.2/4582]? Synthetic Spitzer IRS
blue peak-up photometry
1169- 1177 E9.3 mJy e_IRS15Flux [0.016/3.5]? Error in IRS15Flux
1179- 1187 E9.3 mJy IRS22Flux [0.3/12770]? Synthetic Spitzer IRS
red peak-up photometry
1189- 1197 E9.3 mJy e_IRS22Flux [0.02/7.7]? Error in IRS22Flux
1199- 1207 E9.3 mJy MIPS24Flux [0.26/13870]? Synthetic Spitzer
MIPS 24um photometry
1209- 1217 E9.3 mJy e_MIPS24Flux [0.02/10.1]? Error in MIPS24Flux
1219- 1227 E9.3 mJy MIRI56Flux [0.046/3243]? Synthetic JWST MIRI
F560W photometry
1229- 1237 E9.3 mJy e_MIRI56Flux [0.007/8.2]? Error in MIRI56Flux
1239- 1247 E9.3 mJy MIRI77Flux [0.12/6606]? Synthetic JWST MIRI
F770W photometry
1249- 1257 E9.3 mJy e_MIRI77Flux [0.01/9.2]? Error in MIRI77Flux
1259- 1267 E9.3 mJy MIRI10Flux [0.06/4348]? Synthetic JWST MIRI
F1000W photometry
1269- 1277 E9.3 mJy e_MIRI10Flux [0.004/5.2]? Error in MIRI10Flux
1279- 1287 E9.3 mJy MIRI11Flux [0.08/10160]? Synthetic JWST MIRI
F1130W photometry
1289- 1297 E9.3 mJy e_MIRI11Flux [0.007/11]? Error in MIRI11Flux
1299- 1307 E9.3 mJy MIRI13Flux [0.27/4881]? Synthetic JWST MIRI
F1280W photometry
1309- 1317 E9.3 mJy e_MIRI13Flux [0.01/8.2]? Error in MIRI13Flux
1319- 1327 E9.3 mJy MIRI15Flux [0.05/3965]? Synthetic JWST MIRI
F1500W photometry
1329- 1337 E9.3 mJy e_MIRI15Flux [0.019/4]? Error in MIRI15Flux
1339- 1347 E9.3 mJy MIRI18Flux [0.08/7206]? Synthetic JWST MIRI
F1800W photometry
1349- 1357 E9.3 mJy e_MIRI18Flux [0.02/5.4]? Error in MIRI18Flux
1359- 1367 E9.3 mJy MIRI21Flux [0.14/10400]? Synthetic JWST MIRI
F2100W photometry
1369- 1377 E9.3 mJy e_MIRI21Flux [0.027/8.6]? Error in MIRI21Flux
1379- 1387 E9.3 mJy MIRI25Flux [0.2/16640]? Synthetic JWST MIRI
F2550W photometry
1389- 1397 E9.3 mJy e_MIRI25Flux [0.017/17.1]? Error in MIRI25Flux
1399- 1407 E9.3 mJy WISE12Flux [0.36/3700]? Synthetic WISE band-3
photometry
1409- 1417 E9.3 mJy e_WISE12Flux [0.0099/3.2]? Error in WISE12Flux
1419- 1427 E9.3 mJy WISE22Flux [0.28/13260]? Synthetic WISE band-4
photometry
1429- 1437 E9.3 mJy e_WISE22Flux [0.025/10.5]? Error in WISE22Flux
1439 A1 --- l_F3.7cont Limit on F3.7cont
1441- 1449 E9.3 mJy F3.7cont [0.03/299]? Rest frame continuum
flux density at 3.7um
1451- 1459 E9.3 mJy e_F3.7cont [0.0009/2]? Error in F3.7cont
1461 A1 --- l_F4.2cont Limit on F4.2cont
1463- 1471 E9.3 mJy F4.2cont [0.016/347]? Rest frame continuum
flux density at 4.2um
1473- 1481 E9.3 mJy e_F4.2cont [0.0013/2.6]? Error in F4.2cont
1483 A1 --- l_F5.5cont Limit on F5.5cont
1485- 1493 E9.3 mJy F5.5cont [0.03/3012]? Rest frame continuum
flux density at 5.5um
1495- 1503 E9.3 mJy e_F5.5cont [0.005/23.2]? Error in F5.5cont
1505 A1 --- l_F9.7cont Limit on F9.7cont
1507- 1515 E9.3 mJy F9.7cont [0.028/3381]? Rest frame continuum
flux density at 9.7um
1517- 1525 E9.3 mJy e_F9.7cont [0.008/18]? Error in F9.7cont
1527 A1 --- l_F15cont Limit on F15cont
1529- 1537 E9.3 mJy F15cont [0.1/3615]? Rest frame continuum
flux density at 15um
1539- 1547 E9.3 mJy e_F15cont [0.01/18.3]? Error in F15cont
1549 A1 --- l_F24cont Limit on F24cont
1551- 1559 E9.3 mJy F24cont [0.39/14740]? Rest frame continuum
flux density at 24um
1561- 1569 E9.3 mJy e_F24cont [0.02/58]? Error in F24cont
1571 A1 --- l_F30cont Limit on F30cont
1573- 1581 E9.3 mJy F30cont [0.78/36650]? Rest frame continuum
flux density at 30um
1583- 1591 E9.3 mJy e_F30cont [0.03/204]? Error in F30cont
1593 A1 --- l_C15C55Ratio Limit on C15C55Ratio
1595- 1603 E9.3 --- C15C55Ratio [0.3/59]? Ratio of the rest frame
15um to 5.5um continuum flux
density
1605- 1613 E9.3 --- e_C15C55Ratio [0.003/11]? Error in C15C55Ratio
1615 A1 --- l_C24C55Ratio Limit on C24C55Ratio
1617- 1625 E9.3 --- C24C55Ratio [0.19/220]? Ratio of the rest frame
24um to 5.5um continuum flux
density
1627- 1635 E9.3 --- e_C24C55Ratio [0.003/43]? Error in C24C55Ratio
1637 A1 --- l_C30C55Ratio Limit on C30C55Ratio
1639- 1647 E9.3 --- C30C55Ratio [0.17/578]? Ratio of the rest frame
30um to 5.5um continuum flux
density
1649- 1657 E9.3 --- e_C30C55Ratio [0.003/75]? Error in C30C55Ratio
1659- 1661 I3 --- SNR66 [1/308]? Continuum S/N at 6.6um
1663- 1665 I3 --- SNR9 [1/557]? Continuum S/N at 9.0um
1667- 1669 I3 --- SNR1125 [1/494]? Continuum S/N at 11.25um
1671- 1673 I3 --- SNR1325 [1/853]? Continuum S/N at 13.25um
1675- 1677 I3 --- SNR14 [1/200]? Continuum S/N at 14.0um
1679- 1681 I3 --- SNR17 [1/674]? Continuum S/N at 17.0um
1683- 1685 I3 --- SNR24 [1/309]? Continuum S/N at 24.0um
1687- 1689 I3 --- SNR30 [1/238]? Continuum S/N at 30.0um
1691- 1695 F5.3 --- SL2SF [0.72/3.8]? Factor by which SL2
spectral segment has been scaled
1697- 1701 F5.3 --- SL1SF [0.78/4.2]? Factor by which SL1
spectral segment has been scaled
1703- 1707 F5.3 --- LL2SF [0.67/2]? Factor by which LL2
spectral segment has been scaled
1709- 1713 F5.3 --- LL1SF [0.64/2]? Factor by which LL1
spectral segment has been scaled
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Note (1): Galaxies in class 1A have a hot-dust-dominated spectrum typical for
AGNs. Galaxies in class 1C have PAH-dominated spectra typical for
starburst galaxies. Galaxies in class 3A have absorption-dominated
spectra typical for centrally heated dust shells or tori. Galaxies in
between these extremes show intermediate properties. See Figure 14 in
Section 8.1.
Note (2): If the values for Cryst19Strength, Cryst23Strength, Cryst28Strength,
and Cryst33Strength are given without errors then they should be interpreted
according to the limit flags (e.g., l_Cryst19Strength, e.g.,
l_Cryst23Strength) as follows:
N = the Cryst##Strength value resides between -Cryst##Strength and
+Cryst##Strength;
> = the Cryst19Strength value resides between Cryst19Strength and zero as
Cryst19Strength is always negative.
Note (3): Position 140.58629 +28.45965 (J2000) for IRAS F10398+3247 has been
corrected at CDS for 160.67006 +32.52528 (J2000) following the SIMBAD,
Paper I (Hernan-Caballero+, 2016, J/MNRAS/455/1796) and NED coordinates.
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History:
From electronic version of the journal
References:
Hernan-Caballero et al. Paper I. 2016MNRAS.455.1796H 2016MNRAS.455.1796H Cat. J/MNRAS/455/1796
(End) Prepared by [AAS], Emmanuelle Perret [CDS] 21-Jun-2022