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J/ApJ/707/890           IR properties of E and S0 galaxies         (Temi+, 2009)

Spitzer observations of passive and star-forming early-type galaxies: an infrared color-color sequence. Temi P., Brighenti F., Mathews W.G. <Astrophys. J., 707, 890-902 (2009)> =2009ApJ...707..890T
ADC_Keywords: Galaxies, IR ; Photometry, infrared Keywords: galaxies: elliptical and lenticular, cD - galaxies: ISM - infrared: galaxies - infrared: ISM Abstract: We describe the infrared properties of a large sample of early-type galaxies, comparing data from the Spitzer archive with Ks-band emission from the Two Micron All Sky Survey. While most representations of this data result in correlations with large scatter, we find a remarkably tight relation among colors formed by ratios of luminosities in Spitzer-Multiband Imaging Photometer bands (24, 70, and 160um) and the Ks band. Remarkably, this correlation among E and S0 galaxies follows that of nearby normal galaxies of all morphological types. Description: The FIR data presented here were obtained with the Multiband Imaging Photometer (MIPS) onboard the Spitzer Space Telescope in three wavebands centered at 24, 70, and 160um. These data, collected from the Spitzer public archive, do not form a homogeneous and uniform data set in terms of image depth and observing mode. Column 2 of Table 1 lists the program identification (ID) and principal investigator (PI) for the various original Spitzer observing programs from which our sample galaxies are selected. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1.dat 140 225 Early type galaxies from the Spitzer archives
See also: VII/233 : The 2MASS Extended sources (IPAC/UMass, 2003-2006) VII/237 : HYPERLEDA. I. Catalog of galaxies (Paturel+, 2003) VII/112 : RC2 Catalogue (de Vaucouleurs+ 1976) J/A+A/497/41 : Average Early-type galaxies NIR spectrum (Cesetti+, 2009) J/MNRAS/393/1467 : Field early-type galaxies at 0.2<z<0.8 (Fritz+, 2009) J/ApJ/689/913 : Fundamental planes of early-type galaxies (La Barbera+, 2008) J/ApJ/666/863 : GOODS MIPS early-type galaxies (Van Der Wel+, 2007) J/MNRAS/367/627 : X-ray/NIR correlation for early-type galaxies (Ellis+, 2006) J/AJ/127/131 : NICMOS early-type galaxies (Stanford+, 2004) J/ApJ/551/111 : HDF early-type and spiral galaxies (Ellis+, 2001) J/ApJS/124/127 : Near IR Imaging of Early-Type Galaxies (Pahre, 1999) J/A+AS/100/583 : IR and Optical Photometry of galaxies (Boisson+ 1993) Byte-by-byte Description of file: table1.dat
Bytes Format Units Label Explanations
1- 7 A7 --- Name Galaxy name 9- 17 A9 --- PI PI of the Spitzer observing program 19- 23 I5 --- PID Number of the Spitzer observing program from which the galaxy has been selected 25- 32 A8 --- MType Morphological type from HyperLeda 34- 37 F4.1 --- TT Morphological numerical T type from de Vaucouleurs (1) 39- 44 F6.2 Mpc Dist Galaxy distance (2) 46- 50 F5.2 [Lsun] logLKs Luminosity in the Ks band (3) 52- 57 F6.3 --- U-V ? U-V color index derived from HyperLeda U-B and B-V colors 59- 62 F4.2 [Msun] logMHI ? Neutral hydrogen mass (4) 64- 67 F4.2 [Msun] logMH2 ? Molecular gas mass (5) 69- 70 A2 --- l_F24 [≤] Limit flag on F24 71- 77 F7.2 mJy F24 ? Spitzer/MIPS 24um flux density 79- 84 F6.2 mJy e_F24 ? F24 uncertainty 86- 87 A2 --- l_F70 [≤] Limit flag on F70 88- 93 E6.3 mJy F70 ? Spitzer/MIPS 70um flux density 95- 99 F5.1 mJy e_F70 ? F70 uncertainty 101-102 A2 --- l_F160 [≤] Limit flag on F160 103-109 F7.1 mJy F160 ? Spitzer/MIPS 160um flux density 111-116 F6.1 mJy e_F160 ? F160 uncertainty 118-119 A2 --- l_logL24 [≤] Limit flag on logL24 120-124 F5.2 [10-7W] logL24 ? Specific luminosity L_lambda_ at 24um (6) 126-127 A2 --- l_logL70 [≤] Limit flag on logL70 128-132 F5.2 [10-7W] logL70 ? Specific luminosity L_lambda_ at 70um (6) 134-135 A2 --- l_logL160 [≤] Limit flag on logL160 136-140 F5.2 [10-7W] logL160 ? Specific luminosity L_lambda_ at 160um (6)
Note (1): De Vaucouleurs numerical type, T correspondence with the Hubble type is defined in RC2 (Cat. VII/112). Data values are taken from the HyperLeda Database (Paturel et al. 2003, Cat. VII/237). Note (2): When available, distances are taken from Tonry et al. 2001ApJ...546..681T, otherwise they are from the NASA Extragalactic Database (NED) and corrected for H0=70km/s/Mpc. Note (3): Luminosities in the Ks band, LKs, have been derived using the flux density FKs published by the 2MASS survey, Skrutskie et al. 2006, Cat. VII/233. Note (4): The neutral hydrogen masses, MHI are taken from these publications: Morganti et al. 2006MNRAS.371..157M; Sage & Welch 2006ApJ...644..850S; di Serego Alighieri et al. 2007A&A...474..851D; Roberts et al. 1991ApJS...75..751R; Huchtmeier (1994A&A...286..389H); Huchtmeier et al. (1995A&A...300..675H); Sadler et al. 2000AJ....119.1180S; Knapp & Raimond 1984A&A...138...77K. Note (5): Molecular gas masses, MH2 are collected from these publications: Combes et al. 2007MNRAS.377.1795C; Young et al. 2009AJ....137.3053Y; Young 2002AJ....124..788Y; Sage et al. 2007ApJ...657..232S; Welch & Sage 2003ApJ...584..260W; Roberts et al. 1991ApJS...75..751R. Note (6): In this paper Lλ represents λLλ in erg/s. This differs from our previous notation in which Lλ represented the Spitzer band width multiplied by the specific luminosity.
History: From electronic version of the journal References: Temi et al. 2007ApJ...666..222T Temi et al. 2008ApJ...672..244T Temi et al. 2009ApJ...695....1T
(End) Emmanuelle Perret [CDS] 02-Jan-2012
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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