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J/A+A/414/825       Mid-infrared spectroscopy of LINERs      (Satyapal+, 2004)

A joint mid-infrared spectroscopic and X-ray imaging investigation of LINER galaxies. Satyapal S., Sambruna R.M., Dudik R.P. <Astron. Astrophys. 414, 825 (2004)> =2004A&A...414..825S
ADC_Keywords: Galaxies, IR ; X-ray sources ; Spectroscopy Keywords: galaxies: starburst - X-rays: galaxies - infrared: galaxies Abstract: We present a comprehensive comparative high resolution mid-IR spectroscopic and X-ray imaging investigation of LINERs using archival observations from the ISO-SWS and the Chandra Advanced CCD Imaging Spectrometer. Although the sample is heterogeneous and incomplete, this is the first comprehensive study of the mid-infrared fine structure line emission of LINERs. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1.dat 82 42 The ISO-SWS and Chandra sample table2.dat 155 24 Observed fine structure line fluxes and upper limits
See also: J/other/RMxAA/35.187 : Multifrequency catalog of LINERs (Carrillo+, 1999) Byte-by-byte Description of file: table1.dat
Bytes Format Units Label Explanations
1- 15 A15 --- Name Common galaxy name 17- 19 A3 --- OName Other name of the galaxy 21- 37 A17 --- Obs Observed by Chandra, SWS or LWS 39- 44 F6.2 Mpc Dist Distance (for H0=75km/s/Mpc unless otherwise noted in n_Dist) 45 A1 --- n_Dist [a-g] References for Dist (1) 47- 58 A12 --- MType Hubble type 60- 63 F4.1 [solLum] logLFIR ? Far-infrared luminosity (2) 65 A1 --- l_LFIR/LB Limit flag on LFIR/LB 66- 71 F6.2 --- LFIR/LB ? Far-infrared to B luminosities ratio (3) 73- 75 A3 --- BroadHa [yes ] LINERs with broad Hα emission 77- 81 F5.3 10+22cm-2 NH Hydrogen column density
Note (1): References: a: Stanek et al. (1998ApJ...503L.131S) b: Puche et al. (1988A&A...206...89P) c: Tully et al. (1988AJ.....96...73T) d: Guainazzi (2000A&A...364L..80G) e: Ho et al. (2001ApJ...549L..51H) f: Wilson & Yang (2001, AAS 33, 1530) g: Feldmeier et al. (1997, Cat. J/ApJ/479/231) Note (2): Far-infrared luminosity corresponds to the 40-500um wavelength interval and were calculated using the IRAS 60 and 100um fluxes according to the prescription: LFIR=1.26*10-14(2.58f60+f100) in W/m2 (Sanders & Mirabel, 1996ARA&A..34..749S) Note (3): LB: B magnitude see Carrillo et al. (1999, J/other/RMxAA/35.187)
Byte-by-byte Description of file: table2.dat
Bytes Format Units Label Explanations
1- 15 A15 --- Name Galaxy name 19 A1 --- l_[SIV] Limit flag on [SIV] 20- 23 F4.2 10-20W/cm2 [SIV] ? [SIV] line flux (1) 25- 28 F4.2 10-20W/cm2 e_[SIV] ? rms uncertainty on [SIV] 29 A1 --- n_[SIV] [3] Note on [SIV] (2) 32 A1 --- l_[NeII] Limit flag on [NeIII] 33- 38 F6.2 10-20W/cm2 [NeII] ? [NeII] line flux (1) 40- 43 F4.2 10-20W/cm2 e_[NeII] ? rms uncertainty on [NeII] 44 A1 --- n_[NeII] [abc3] Note on [NeII] (2) 48 A1 --- l_[NeV] Limit flag on [NeV] 49- 52 F4.2 10-20W/cm2 [NeV] ? [NeV] line flux (1) 54- 57 F4.2 10-20W/cm2 e_[NeV] ? rms uncertainty on [NeV] 58 A1 --- n_[NeV] [cd3] Note on [NeV] (2) 60 A1 --- l_[NeIII] Limit flag on [NeIII] 61- 65 F5.2 10-20W/cm2 [NeIII] ? [NeIII] line flux (1) 67- 70 F4.2 10-20W/cm2 e_[NeIII] ? rms uncertainty on [NeIII] 71 A1 --- n_[NeIII] [3abd] Note on [NeIII] (2) 74 A1 --- l_[SIII] Limit flag on [SIII] 75- 79 F5.2 10-20W/cm2 [SIII] ? [SIII] line flux (1) 81- 84 F4.2 10-20W/cm2 e_[SIII] ? rms uncertainty on [SIII] 85 A1 --- n_[SIII] [bc3] Note on [SIII] (2) 87 A1 --- l_[OIV] Limit flag on [OIV] 88- 92 F5.3 10-20W/cm2 [OIV] ? [OIV] line flux (1) 94- 97 F4.2 10-20W/cm2 e_[OIV] ? rms uncertainty on [OIV] 99 A1 --- n_[OIV] [3dc] Note on [OIV] (2) 102 A1 --- l_[FeII] Limit flag on [FeIII] 103-107 F5.2 10-20W/cm2 [FeII] ? [FeII] line flux (1) 109-112 F4.2 10-20W/cm2 e_[FeII] ? rms uncertainty on [FeII] 113 A1 --- n_[FeII] [3] Note on [FeII] (2) 115 A1 --- l_[SIII]2 Limit flag on [SIII]2 116-120 F5.2 10-20W/cm2 [SIII]2 ? [SIII]2 line flux (1) 122-125 F4.2 10-20W/cm2 e_[SIII]2 ? rms uncertainty on [SIII]2 126 A1 --- n_[SIII]2 [cb3] Note on [SIII]2 (2) 128 A1 --- l_[SiII] Limit flag on [SiII] 129-134 F6.2 10-20W/cm2 [SiII] ? [SiII] line flux (1) 136-139 F4.2 10-20W/cm2 e_[SiII] ? rms uncertainty on [SiII] 140 A1 --- n_[SiII] [3c] Note on [SiII] (2) 142 A1 --- l_[NeIII]2 Limit flag on [NeIII]2 143-147 F5.2 10-20W/cm2 [NeIII]2 ? [NeIII]2 line flux (1) 149-152 F4.2 10-20W/cm2 e_[NeIII]2 ? rms uncertainty on [NeIII]2 154 A1 --- n_[NeIII]2 [3] Note on [NeIII]2 (2)
Note (1): Definitions: [SIV] : lambda=10.5um; Eion=34.8eV, Aperture2=14x20arcsec2 [NeII] : lambda=12.8um; Eion=21.6eV, Aperture2=14x27arcsec2 [NeV] : lambda=14.3um; Eion=97.1eV, Aperture2=14x27arcsec2 [NeIII] : lambda=15.5um; Eion=41.0eV, Aperture2=14x27arcsec2 [SIII] : lambda=18.7um; Eion=23.3eV, Aperture2=14x27arcsec2 [OIV] : lambda=25.9um; Eion=54.9eV, Aperture2=14x20arcsec2 [FeII] : lambda=26.0um; Eion= 7.9eV, Aperture2=14x27arcsec2 [SIII]2 : lambda=33.5um; Eion=23.3eV, Aperture2=20x33arcsec2 [SiII] : lambda=38.4um; Eion= 8.2eV, Aperture2=20x33arcsec2 [NeIII]2 : lambda=36.0um; Eion=41.0eV, Aperture2=20x33arcsec2 where EIon is lower ionization potential of the stage leading to the transition Note (2): Notes and references: 3: upper limits correspond to 3 values. References: Flux data for these objects were taken from a: Thornley et al. (2000ApJ...539..641T) b: Sugai & Malkan (2000ApJ...529..219S) c: Genzel et al. (1998ApJ...498..579G) d: Prieto & Viegas (2000ApJ...532..238P).
History: From electronic version of the journal
(End) Patricia Bauer [CDS] 27-Jan-2004
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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