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 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 1998ApJ...503L.131S) b: Puche et al. (1988A&A...206...89P 1988A&A...206...89P) c: Tully et al. (1988AJ.....96...73T 1988AJ.....96...73T) d: Guainazzi (2000A&A...364L..80G 2000A&A...364L..80G) e: Ho et al. (2001ApJ...549L..51H 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 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 2000ApJ...539..641T) b: Sugai & Malkan (2000ApJ...529..219S 2000ApJ...529..219S) c: Genzel et al. (1998ApJ...498..579G 1998ApJ...498..579G) d: Prieto & Viegas (2000ApJ...532..238P 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