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J/A+A/357/839       AGN 2.5-11um spectroscopy                (Clavel+, 2000)

2.5-11 micron spectroscopy and imaging of AGNs. Implication for unification schemes Clavel J., Schulz B., Altieri B., Barr P., Claes P., Heras A., Leech K., Metcalfe L., Salama A. <Astron. Astrophys. 357, 839 (2000)> =2000A&A...357..839C
ADC_Keywords: Active gal. nuclei ; Galaxies, IR ; Spectroscopy Keywords: galaxies: active - infrared: galaxies - galaxies: Seyfert Description: We present observations over the 2.5-11µm range, with the ISOPHOT-S spectrometer and the ISOCAM imaging camera, of a sample of 57 AGNs and one non-active SB galaxy. The sample is about equally divided into type I (≤1.5; 28 sources) and type II (>1.5; 29 sources) objects. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table2.dat 41 59 6.75 and 9.63µm ISOCAM (CAM) & ISOPHOT (PHT) fluxes table3.dat 91 14 Fluxes and dimensions of extended sources table4.dat 70 58 Continuum and PAH band fluxes table5.dat 77 58 PAH band flux tables.tex 119 411 LaTeX version of the tables
See also: J/A+AS/70/95 : Warm IRAS sources. I. AGN candidates (de Grijp+ 1987) Byte-by-byte Description of file: table2.dat
Bytes Format Units Label Explanations
1- 13 A13 --- TARGET Target name 15- 18 I4 mJy CAM(6.75um) ? ISOCAM 6.75µm nuclear flux 20- 22 I3 mJy PHT(6.75um) ? ISOPHOT 6.75µm nuclear flux 23- 24 A2 --- n_PHT(6.75um) [NA ] NA: not analysed 26- 28 I3 mJy CAM(9.63um) ? ISOCAM 9.63µm nuclear flux 30- 32 I3 mJy PHT(9.63um) ? ISOPHOT 9.63µm nuclear flux 33- 34 A2 --- n_PHT(9.63um) [NA ] NA: not analysed 36- 39 F4.1 100pc/arcsec l10 Dimension in kiloparsec at the source corresponding to an angular separation of 10 arcsec on the sky 41 A1 --- Note [E] E: Extended source
Byte-by-byte Description of file: table3.dat
Bytes Format Units Label Explanations
1- 13 A13 --- TARGET Target name 15- 17 I3 mJy Nucl(6.75um) ? Nuclear flux at 6.75µm 19- 22 I4 mJy 24x24(6.75um) Flux in a 24"x24" aperture equivalent to that of the PHT spectrometer on-board ISO at 6.75µm 24- 27 I4 mJy Tot(6.75um) Total flux integrated over the full extent of the source at 6.75µm 29- 31 I3 mJy Nucl(9.63um) ? Nuclear flux at 9.63µm 33- 35 I3 mJy 24x24(9.63um) Flux in a 24"x24" aperture equivalent to that of the PHT spectrometer on-board ISO at 9.63µm 37- 40 I4 mJy Tot(9.63um) Total flux integrated over the full extent of the source at 9.63µm 42- 45 F4.1 arcsec FWHM Full Width at Half Maximum 47- 91 A45 --- Com Comments
Byte-by-byte Description of file: table4.dat
Bytes Format Units Label Explanations
1- 13 A13 --- TARGET Target name 15- 17 A3 --- MType Seyfert class 19- 23 F5.2 --- Sp+Index Continuum spectral index 25- 29 F5.1 mJy F(7um) Continumm flux at 7um 31- 32 A2 --- l_F(3.3um) [≤ ] Limit flag on F(3.3um) 33- 37 F5.3 10-15W/m2 F(3.3um) Flux of the 3.3um PAH emission band 39- 43 F5.3 10-15W/m2 e_F(3.3um) ? rms uncertainty on F3.3um 45- 46 A2 --- l_EW(3.3um) [≤ ] Limit flag on EW(3.3um) 47- 51 F5.3 um EW(3.3um) Equivalent width of the 3.3um PAH emission band 53- 58 F6.3 10-15W/m2 F(6.2um) Flux of the 6.2um PAH emission band 60- 64 F5.3 10-15W/m2 e_F(6.2um) rms uncertainty on F6.2 66- 70 F5.3 um EW(6.2um) Equivalent width of the 6.2um PAH emission band
Byte-by-byte Description of file: table5.dat
Bytes Format Units Label Explanations
1- 13 A13 --- TARGET Target name 15- 17 A3 --- MType Seyfert class 19- 24 F6.3 10-15W/m2 F(7.7um) Flux of the 7.7um PAH emission band 26- 30 F5.3 10-15W/m2 e_F(7.7um) rms uncertainty on F(7.7um) 32- 36 F5.3 um EW(7.7um) Equivalent width of the 7.7um PAH emission band 38- 43 F6.3 10-15W/m2 F(8.6um) Flux of the 8.6um PAH emission band 45- 49 F5.3 10-15W/m2 e_F(8.6um) rms uncertainty on F(8.6um) 51- 56 F6.3 um EW(8.6um) Equivalent width of the 8.6um PAH emission band 58- 64 F7.3 10-15W/m2 F(PAH) Total flux of the PAH emission band at 3.3, 6.2, 7.7 and 8.6um 66- 70 F5.3 10-15W/m2 e_F(PAH) rms uncertainty on F(PAH) 72- 77 F6.3 um EW(PAH) Total equivalent width of the PAH emission band at 3.3, 6.2, 7.7 and 8.6um
Acknowledgements: Jean Clavel
(End) Patricia Bauer CDS 21-Mar-2000
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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