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J/ApJ/652/1068   Morphology of cool and warm infrared galaxies   (Rahman+, 2006)

Probing cool and warm infrared galaxies using photometric and structural measures. Rahman N., Helou G., Mazzarella J.M. <Astrophys. J., 652, 1068-1076 (2006)> =2006ApJ...652.1068R
ADC_Keywords: Galaxies, IR ; Morphology ; Photometry, infrared Keywords: galaxies: active - galaxies: general - galaxies: spiral - galaxies: starburst - galaxies: structure Abstract: We have analyzed a sample of nearby cool and warm infrared (IR) galaxies using photometric and structural parameters. The set of measures include far-infrared color [C=log(S60um/S100um)], total IR luminosity (LFIR), radio surface brightness, and radio, near-infrared, and optical sizes. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1.dat 125 213 Complete List of 213 Galaxies: SFGs + LIRGs + ULIRGs
See also: J/AJ/126/1607 : IRAS Revised Bright Galaxy Sample (Sanders+, 2003) Byte-by-byte Description of file: table1.dat
Bytes Format Units Label Explanations
1- 6 A6 --- Class Galaxy class (G1) (1) 8- 10 I3 --- Seq Running sequence number (2) 12- 28 A17 --- Name Common name 30 A1 --- f_Name [cw] (c)ool of (w)arm source 32 A1 --- l_S12 Limit flag on S12um 33- 36 F4.2 Jy S12 IRAS 12 micron flux density 38- 41 F4.2 Jy S25 IRAS 25 micron flux density 43- 48 F6.2 Jy S60 IRAS 60 micron flux density 50- 55 F6.2 Jy S100 IRAS 100 micron flux density 57- 61 F5.1 mJy S1.49 The 1.49 GHz flux density (4) 63- 68 F6.2 Mpc Dist Estimated galaxy distance 70 A1 --- f_Dist [PSV-] Flag on Dist (5) 72- 76 F5.2 solLum LTIR Log of the 8-1000 micron luminosity 78- 82 F5.1 arcsec Bmaj ? The B-band 25mag/arcsec2 major axis (θM) 84- 88 F5.1 arcsec Bmin ? The B-band 25mag/arcsec2 minor axis (θm) 90- 94 F5.1 arcsec Kmaj ? The Ks band 20mag/arcsec2 major axis(θM) 96-100 F5.1 arcsec Rmaj Radio 1.49GHZ major axis (θM) 102-106 F5.1 arcsec Rmin ? Radio 1.49GHZ minor axis (θm) 108 A1 --- u_Rmin [?] Uncertainty flag on RMinAxis 110-113 F4.1 arcsec Res VLA beam 1.49GHz resolution 115-125 A11 --- Morph Galaxy optical morphology (6)
Note (1): Galaxy class as follows: SFGs = Low Luminosity Star Forming Galaxies LIRGs = Luminous Infrared Galaxies ULIRGs = Ultra-Luminous Infrared Galaxies Galaxies identified as [RHM2006] Class Seq, i.e. [RHM2006] SFGs 1 for NGC 4565 Note (2): Galaxies are sorted in the ascending order of FIR color, i.e. galaxy numbered 1 has the lowest FIR color, for all three luminosity classes. Note (4): Peak flux Sp in Condon, Anderson & Helou (1991ApJ...376...95C). Sp in mJy in the VLA map with the beam of VLA map, selected by "the maximum at which the source is resolved" (Wang & Helou, 1992ApJ...398L..33W). * For IRASF12224-0624 (LIRGs) Condon, Anderson & Helou (1991ApJ...376...95C) gives θMm<5arcsec2. We assume θM∼5arcsec. * For IRASF15250+3608 (ULIRGs) Condon, Anderson & Helou (1991ApJ...376...95C) gives θMm<0.3arcsec2. We assume θM∼0.3arcsec. Note (5): The following flags from Revised Bright Galaxy Catalog (RBGS) of Sanders et al. (2003, Cat. J/AJ/126/1607): P = Distance is not computed by correcting the heliocentric redshift using the cosmic attractor model, but comes from a direct primary distance measurement S = A direct secondary distance measurement V = The cosmic attractor flow model places the object within the Virgo Cluster at a distance of 15.3Mpc Note (6): The following 22 SFGs have either disturbed outer envelope or a nearby companion (after visual inspection): NGC5792, UGC12914, NGC5600, NGC5937, NGC3508, NGC4045, NGC5430, NGC3994 NGC5218, NGC0150, NGC1134, NGC1083, NGC0660, NGC5953, NGC4532, NGC5915, NGC0520, NGC2782, NGC5930, NGC2798, NGC3597, NGC1222 The following 15 LIRGs have either disturbed outer envelope or a nearby companion (after visual inspection): NGC5394, NGC5257, UGC04881, MCG+07-23-019, NGC6052, NGC6090, CGCG247-020, NGC5256, NGC7592, IRASF17132+5313, IRASF03359+1523, NGC2623, IIIZw035, NGC0034, CGCG436-030
History: From electronic version of the journal
(End) Greg Schwarz [AAS], Patricia Vannier [CDS] 25-Jul-2008
The document above follows the rules of the Standard Description for Astronomical Catalogues.From this documentation it is possible to generate f77 program to load files into arrays or line by line

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