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J/A+AS/70/95         Warm IRAS sources. I. AGN candidates (de Grijp+ 1987)

Warm IRAS sources. I. A catalogue of AGN candidates from the point source catalog. de Grijp M.H.K., Miley G.K., Lub J. <Astron. Astrophys. Suppl. Ser. 70, 95 (1987)> =1987A&AS...70...95D
ADC_Keywords: Infrared sources ; Active gal. nuclei Keywords: catalogue - Seyferts - infrared radiation Abstract: We have previously shown that a blue (warm) 60 to 25µm infrared colour provides a powerful parameter for discriminating between AGNs and normal galaxies and that the far-IR spectrum is therefore an efficient tool for finding new AGNs (de Grijp et al., 1985Natur.314..140D) Here we present a list of such AGN candidates based on warm IR sources from the IRAS Point Source Catalogue (PSC, Cat. II/125). Identification data and finding charts are also given. In addition the list of warm IRAS sources is supplemented by a compendium of data from the IRAS PSC on detected sources identified with previously known AGNs whose infrared spectra do not bring them within our colour selection criterion File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1.dat 110 565 *IRAS candidate Active Galactic Nuclei table2.dat 110 177 Active galaxies compiled by Veron-Cetty & Veron (1985, See Cat. VII/188), that were not included in table I. table3.dat 110 9 Extragalactic radio sources (Kuhr, 1981A&AS...45..367K) not present in tables I & II dml87.dat 15 565 Actual IRAS names of the objects studied in table1 (added in 2011, see the "History" section below)
Note to table1: Sources were selected on position (high galactic latitude, not in Magellanic and colour (25 to 60µm spectral index between 1.5 and 0.0). All sources satisfying these criteria are included, even when optical identification indicates them to be non-extragalactic objects. See also: II/125 : IRAS catalogue of Point Sources, Version 2.0 (IPAC 1986) J/A+AS/96/389 : Warm IRAS sources. II. (de Grijp+, 1992) J/A+AS/108/61 : Warm IRAS source. IV. (Fehmers+, 1994) VII/188 : Quasars and Active Galactic Nuclei (7th Ed.) (Veron+ 1996) VII/99 : Radial Velocities of Galaxies (Palumbo+ 1986) Byte-by-byte Description of file: table1.dat table2.dat table3.dat
Bytes Format Units Label Explanations
1- 3 I3 --- Seq Sequential number 4 A1 --- m_Seq [nsew] Multiplicity index on Seq 6- 7 I2 h RAh IRAS right ascension (1950) 9- 10 I2 min RAm IRAS right ascension (1950) 12- 15 F4.1 s RAs [0/60] IRAS right ascension (1950) 17 A1 --- DE- IRAS declination sign 18- 19 I2 deg DEd IRAS declination (1950) 21- 22 I2 arcmin DEm IRAS declination (1950) 24- 25 I2 arcsec DEs [0/60] IRAS declination (1950) 27 A1 --- l_a25 Limit flag on a25 28- 32 F5.2 --- a25 ? 25 to 60 µm spectral index 33 A1 --- u_a25 Uncertainty flag on a25 34 A1 --- l_S60 Limit flag on S60 35- 41 F7.2 Jy S60 Flux density at 60µm 42 A1 --- u_S60 Uncertainty flag on S60 45 A1 --- l_a60 Limit flag on a60 46- 50 F5.2 --- a60 ? 60 to 100 µm spectral index 51 A1 --- u_a60 Uncertainty flag on a60 53- 55 A3 --- Class Classification (1) 57- 62 F6.4 --- z ? Redshift (2) 64- 65 I2 --- Cat ? Association Catalogue number (3) 67- 79 A13 --- Source Association source name (3) 81-110 A30 --- Com Comments
Note (1): the classification uses the following abbreviations: BL = BL Lac object S1 = Seyfert 1 (including QSO) S2 = Seyfert 2 S3 = LINER H2 = galaxy with nucleus HII-region PN = planetary nebula RN = reflection nebula DN = galactic dark cloud ST = star LH = local H2 region in the galaxy GAL = galaxy EF = empty field M31 = M31 type Note (2): Redshifts from Veron & Veron (1985, See Cat. VII/188), Palumbo et al. (1983, See Cat. VII/99), de Grijp et al. (1986, A&A, in prep.) Note (3): Matches with published catalogues using the same catalogue numbering convention as given by the IRAS Catalogue (See II/125). The non-standard "ZG" acronym stands for Zwicky's catalog of galaxies (see e.g. cat. VII/190)
Table 4: Objects types identified. -------------------------------------------------- Object type number percentage -------------------------------------------------- stars 77 13.7% planetary nebulae 15 2.7% galactic darks clouds 6 1.1% HII regions 5 0.7% galaxies 443 78.7% doubtful types 17 3.0% Byte-by-byte Description of file: dml87.dat
Bytes Format Units Label Explanations
1- 3 I3 --- Seq Sequential identification, as in table1 6- 15 A10 --- IRAS Actual IRAS-PSC name (Cat. II/125)
History: * 13-May-1997: Prepared via OCR at CDS. * 01-Sep-1997: a list of about 80 errors detected by H. Andernach <heinz(at)cuevano.ugto.mx> have been corrected in the tables. Missing acronyms in column AssSource were also added at CDS. * 09-Jan-2011: file "dml87.txt" supplied by H. Andernach, which contains the actual IRAS names of the sources studied in table1. References: de Grijp et al., Paper II =1992A&AS...96..389D Keel et al., Paper III =1994A&A...283..791K
(End) James Marcout, Patricia Bauer [CDS] 13-May-1997
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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