J/ApJS/95/1                Atlas of Quasar Energy Distributions (Elvis+ 1994)

Atlas of Quasar Energy Distributions Elvis M., Wilkes B.J., McDowell J.C., Green R.F., Bechtold J., Willner S.P., Oey M.S., Polomski E., Cutri R. <Astrophys. J. Suppl. Ser. 95, 1 (1994)> =1994ApJS...95....1E 1994ApJS...95....1E
ADC_Keywords: QSOs ; Radio sources ; X-ray sources ; Ultraviolet ; Infrared sources Keywords: atlases - galaxies: photometry - quasars: general Abstract: We present an atlas of the spectral energy distributions (SEDs) of normal, non-blazar, quasars over the whole available range (radio to 10 keV X-rays) of the electromagnetic spectrum. The primary (UVSX) sample includes 47 quasars for which the spectral energy distributions include X-ray spectral indices and UV data. Of these, 29 are radio quiet, and 18 are radio loud. The SEDs are presented both in figures and in tabular form, with additional tabular material published on CD-ROM. Previously unpublished observational data for a second set of quasars excluded from the primary sample are also tabulated. The effects of host galaxy starlight contamination and foreground extinction on the UVSX sample are considered and the sample is used to investigate the range of SED properties. Of course, the properties we derive are influenced strongly by the selection effects induced by quasar discovery techniques. We derive the mean energy distribution (MED) for radio-loud and radio-quiet objects and present the bolometric corrections derived from it. We note, however, that the dispersion about this mean is large (∼one decade for both the infrared and ultraviolet components when the MED is normalized at the near-infrared inflection). At least part of the dispersion in the ultraviolet may be due to time variability, but this is unlikely to be important in the infrared. The existence of such a large dispersion indicates that the MED reflects only some of the properties of quasars and so should be used only with caution. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table3a 107 53 Adopted X-ray power-law fits table3b 75 20 Observational details for new X-ray power-law fits table3.tex 92 225 LaTeX version of table3 tablea1 15 46 Adopted continuum bands tablea2 55 3401 IUE continuum bands tablea3 49 572 Optical continuum measurements tablea4 17 41 Adopted extinction law tablea5 15 155 Starlight Template tableb1 120 4791 Observed energy distribution table6 102 141 Near-infrared photometry table6.tex 86 505 LaTeX version of table6 table9 99 134 Radio fluxes table9.tex 80 322 LaTeX version of table9 table10 48 46 Millimeter fluxes table10.tex 69 106 LaTeX version of table10 table11 22 13 Magnitude scale zero points table11.tex 59 61 LaTeX version of table11 table12 36 37 Adopted host galaxy parameters table12.tex 75 99 LaTeX version of table12 -------------------------------------------------------------------------------- Byte-by-byte Description of file: table3a -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 2- 10 A9 --- Name Quasar name 12 A1 --- l_F0.2 Limit flag for F2 flux 13- 17 F5.2 uJy F0.2 ? Flux at 0.2 KeV 19- 21 F3.1 uJy E_F0.2 ? Error in F2 flux (upper limit) 24- 26 F3.1 uJy e_F0.2 ? Error in F2 flux (lower limit) 28- 32 F5.2 --- alpha10 Energy index at 1 keV 34- 37 F4.2 --- E_alpha10 ? Error in energy index alpha10 (upper limit) 40- 43 F4.2 --- e_alpha10 ? Error in energy index alpha10 (lower limit) 47- 50 F4.2 uJy F10 Flux at 1 keV or lower limit of the flux if interval 51 A1 --- n_F10 Separation when interval of flux at 1 keV 52- 54 F3.1 uJy F10u ? Upper limit of the flux when interval 56- 59 F4.2 uJy E_F10 ? Error in F10 flux (upper limit) 62- 65 F4.2 uJy e_F10 ? Error in F10 flux (lower limit) 70- 71 I2 --- Ref Reference (1) 73- 76 F4.2 --- alpha40 ? Energy index at 40 keV 78- 81 F4.2 --- E_alpha40 ? Error in energy index alpha40 (upper limit) 84- 87 F4.2 --- e_alpha40 ? Error in energy index alpha40 (lower limit) 92 A1 --- l_F40 Limit flag on F40 flux 93- 96 F4.2 uJy F40 ? Flux at 4 keV or lower limit of the flux if interval 97 A1 --- n_F40 Separation when interval of flux at 4 keV 98-100 F3.1 uJy F40u ? Upper limit of the flux F40 when interval 102-104 F3.1 uJy e_F40 ? rms uncertainty on F40 flux 106-107 I2 --- ref2 ? Reference for F40 flux -------------------------------------------------------------------------------- Note (1): 1) This paper; 2) Wilkes and Elvis (1987ApJ...323..243W 1987ApJ...323..243W) 3) Masnou et al. (1992A&A...253...35M 1992A&A...253...35M) 4) Elvis et al. (1991ApJ...378..537E 1991ApJ...378..537E) 5) Comastri et al. (1992ApJ...384...62C 1992ApJ...384...62C) 6) Turner and Pounds (1989MNRAS.240..833T 1989MNRAS.240..833T) 7) Williams et al. (1992ApJ...389..157W 1992ApJ...389..157W) 8) Ohashi et al. (1992ApJ...398...87O 1992ApJ...398...87O) 9) Della Ceca et al., Cat. VII/181 10) Turner and Pounds (1988MNRAS.232..463T 1988MNRAS.232..463T) 11) Tananbaum et al. (1986ApJ...305...57T 1986ApJ...305...57T) 12) Saxton et al. (1993MNRAS.262...63S 1993MNRAS.262...63S) -------------------------------------------------------------------------------- Byte-by-byte Description of file: table3b -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 9 A9 --- Name Quasar name 11- 15 I5 --- Seq Sequence number 17- 33 A17 --- Date Observation date 35- 39 I5 s Exp Exposure time 41- 44 F4.1 --- Gain Gain 46- 49 A4 --- PHA ? PHA channels 51- 54 I4 --- Counts ? Fit counts 56- 59 F4.2 ct/s Rate ? Count rate 61- 64 F4.2 --- alpha ? Spectral index 66- 70 F5.2 10+20cm-2 NH ? Hydrogen column density 72- 75 F4.1 --- ki2 ? Ki2 (1) -------------------------------------------------------------------------------- Note (1): See Wilkes & Elvis (1987ApJ...323..243W 1987ApJ...323..243W) for details -------------------------------------------------------------------------------- Byte-by-byte Description of file: tablea1 -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 4 I4 0.1nm Lambda Nominal Wavelength 6- 9 I4 0.1nm Range1 Wavelength range (lower value) 10 A1 --- --- [-] Separation flag 11- 14 I4 0.1nm Range2 Wavelength range (upper value) -------------------------------------------------------------------------------- Note: Continuum spectrophotometry has been binned into the rest frame bandpass defined by this table, chosen to avoid strong emission lines as described in the text. Avoiding: 1000-1050 L-beta 1150-1275 L-alpha 1215/NV (20000 km/s) 1375-1450 OIV 1402 1500-1600 CIV 1550 1850-1950 CIII 1909 2700-2900 Mg II 2798 3300-3550 NeV 3426 3650-3750 [OIII] 3727 3850-4450 Ne II 3869, 3968, H delta 4101, H gamma 4340 4650-5100 H Beta 4861 OIII 6250-6850 OI 6300, Halpha 6562 -------------------------------------------------------------------------------- Byte-by-byte Description of file: tablea2 -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 9 A9 --- Name QSO name 11- 15 A5 --- Obs Observation date, written "MM/YY" 17- 24 A8 --- Exp1 First exposure 26- 33 A8 --- Exp2 Second exposure 35- 38 I4 0.1nm Lambda Lambda (rest) 40- 44 F5.2 [Hz] log(nu) Observed frequency 46- 50 F5.2 [Jy.Hz] log(nuFnu) ? Flux in the observed frame 52- 55 F4.2 [Jy.Hz] e_log(nuFnu) ? rms uncertainty on log(nuFnu) -------------------------------------------------------------------------------- Byte-by-byte Description of file: tablea3 -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 9 A9 --- Name QSO name 11- 18 A8 --- Date Observation date 20- 27 A8 --- Exp Exposure 29- 32 I4 nm Lambda Lambda (rest) 34- 38 F5.2 [Hz] log(nu) Observed frequency 40- 44 F5.2 [Jy.Hz] log(nuFnu) ? Flux in the observed frame 46- 49 F4.2 [Jy.Hz] e_log(nuFnu) ? rms uncertainty on log(nuFnu) -------------------------------------------------------------------------------- Byte-by-byte Description of file: tablea4 -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 4 A4 --- Ref Extinction law reference (1) 6- 11 F6.3 [Hz] log(nu) Frequency 13- 17 F5.3 --- R(nu) Extinction relative to extinction at V (A(nu)/A(V)) -------------------------------------------------------------------------------- Note (1): RL85: Rieke and Lebofsky 1985 SM79: Savage and Mathis 1979 -------------------------------------------------------------------------------- Byte-by-byte Description of file: tablea5 -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 6 F6.3 [Hz] log(nu) Frequency 8- 13 F6.3 [Hz.solLum] log(nuLnu) Energy distribution of starlight template used for host galaxy subtraction, normalized at V -------------------------------------------------------------------------------- Byte-by-byte Description of file: tableb1 -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 9 A9 --- Name Quasar name 11- 15 F5.2 [Hz] log(nu0) Frequency nu0 18- 22 F5.2 [Hz] log(nu1) Frequency nu1 25- 29 F5.2 [Hz] log(nu2) Frequency nu2 31 A1 --- l_log(nuFnu) Limit flag on log(nuFnu) 32- 36 F5.2 [Jy.Hz] log(nuFnu) Flux 42- 45 F4.2 [Jy.Hz] E_log(nuFnu) ? Error on lognuFnu (upper limit) 51- 54 F4.2 [Jy.Hz] e_log(nuFnu) ? Error on lognuFnu (lower limit) 61- 68 A8 --- Date Observation date "DD/MM/YY" partially filled 73- 78 F6.1 arcsec Aper ? Aperture 80- 86 A7 --- Filt Filter or detector 89-103 A15 --- Inst Intrument or telescope 106-120 A15 --- Ref References -------------------------------------------------------------------------------- Byte-by-byte Description of file: table6 -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 9 A9 --- Name Quasar name 11- 15 F5.2 mag Jmag ? J (1.24um) magnitude 16 A1 --- u_Jmag Uncertainty flag on J magnitude 17- 20 F4.2 mag e_Jmag ? rms uncertainty on J magnitude 23- 27 F5.2 mag Hmag ? H (1.63um) magnitude 28 A1 --- u_Hmag Uncertainty flag on H magnitude 29- 32 F4.2 mag e_Hmag ? rms uncertainty on H magnitude 35- 39 F5.2 mag Kmag ? K (2.19um) magnitude 40 A1 --- u_Kmag Uncertainty flag on K magnitude 41- 45 F5.3 mag e_Kmag ? rms uncertainty on K magnitude 47 A1 --- l_3.4mag limit flag on 3.4um magnitude 49- 53 F5.2 mag 3.4mag ? 3.4um magnitude (Deltaλ=0.2um) 54 A1 --- u_3.4mag Uncertainty flag on 3.4um magnitude 55- 58 F4.2 mag e_3.4mag ? rms uncertainty on 3.4mag or error upper limit if e(3.4mag)l not blank 61- 64 F4.2 mag e(3.4mag)l ? Error in 3.4mag (lower limit) 67- 71 F5.2 mag L'mag ? L' (3.79um) magnitude 73- 76 F4.2 mag e_L'mag ? rms uncertainty on L' magnitude 78- 88 A11 --- Date Observation date 90- 98 A9 --- Tel Telescope 100-101 I2 arcsec Beam Beam size 102 A1 --- Note [ac ] When a, a 5" aperture was used for the 3.4um band measurement. When c: possible clouds, uncertainties believed adequate -------------------------------------------------------------------------------- Byte-by-byte Description of file: table9 -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 9 A9 --- Name Quasar name 11 A1 --- l_Nu Limit flag on nu 12- 19 F8.2 GHz Nu ? Frequency 20 A1 --- l_Score Limit flag on Score 21- 28 F8.2 mJy Score ? Core flux (1) 32- 38 F7.2 mJy e_Score ? rms uncertainty on Score 41 A1 --- l_Sext Limit flag on Sext 42- 49 F8.2 mJy Sext ? Extended flux (1) 53- 58 F6.2 mJy e_Sext ? rms uncertainty on Sext 60- 64 A5 --- Date Observation date "MM/YY" (2) 65 A1 --- u_Date [?] Uncertainty flag on year of observation 71- 75 A5 --- Tel Telescope (3) 82- 83 A2 --- l_Res Limite flag on resolution 85- 91 F7.2 arcsec Res ? Resolution 93 A1 --- u_Res [?] Uncertainty flag on resolution 98- 99 I2 --- Ref References (4) -------------------------------------------------------------------------------- Note (1): The division of fluxes into core and extended is arbitrary when only low-resolution observations are available. In such case the presence of a flux in the 'core' column indicates we have chosen to use it in the construction of the energy distribution. Note (2): MM/YY for a month of observation YY for a year of observation YY-YY for several years of observation Note (3): Telescope acronyms are: FCRAO: Five College Radio Astronomy Observatory, MA GB: Green Bank 300 foot telescope NRAO: NRAO Green Bank Interferometer, WVA OVRO: Owens Valley Radio Observatory, CA PKS: Parkes 64-m DSN telescope, NSW, Australia VLA: Very Large Array, NM VLBI: Goldstone and Madrid DSN telescopes WSRT: Westerbork Synthesis Radio Telescope, Netherlands. Note (4): 1: Kellerman et al. (1989AJ.....98.1195K 1989AJ.....98.1195K) 2: I. Gioia, private communication 3: Gower and Hutchings (1984AJ.....89.1658G 1984AJ.....89.1658G) 4: Unger et al. (1987MNRAS.228..521U 1987MNRAS.228..521U) 5: Preston et al. (1985AJ.....90.1599) 6: Feigelson, Isobe and Kembhavi (1984AJ.....89.1464F 1984AJ.....89.1464F) 7: Rudnick, Sitko, and Stein (1984AJ.....89..753R 1984AJ.....89..753R) 8: Miley and Hartsuijker (1978A+AS...34..129M 1978A+AS...34..129M) 9: Price and Milne (1965AuJPh..18..329P 1965AuJPh..18..329P) 10: Pooley and Henbest (1974MNRAS.169..477P 1974MNRAS.169..477P) 11: Perley (1982AJ.....87..859P 1982AJ.....87..859P) 12: Spencer et al. (1989MNRAS.240..657S 1989MNRAS.240..657S) 13: Swarup, Sinha, and Hilldrup (1984MNRAS.208..813S 1984MNRAS.208..813S) 14: Wills (1979ApJS...39..291W 1979ApJS...39..291W) 15: Owen, Porcas and Neff (1978AJ.....83.1009O 1978AJ.....83.1009O) 16: Hintzen, Ulvestad and Owen (1983AJ.....88..709H 1983AJ.....88..709H) 17: Antonucci and Barvainis (1988ApJ...325L..21A 1988ApJ...325L..21A) 18: Hutchings and Gower (1985AJ.....90..405H 1985AJ.....90..405H) 19: Shimmins and Bolton (1981AuJPh..34..471S 1981AuJPh..34..471S) 20: Bolton and Butler (1975AuJPA..34...33B 1975AuJPA..34...33B) 21: Wills (1975AuJPS..38....1W 1975AuJPS..38....1W) 22: Ekers (1969AuJPS...7....1E 1969AuJPS...7....1E) 23: Shimmins and Bolton (1972AuJPS..23....1S 1972AuJPS..23....1S) 24: Shimmins and Bolton (1972AuJPS..26....1S 1972AuJPS..26....1S) 25: Meurs and Wilson (1981A+AS...45...99M 1981A+AS...45...99M) 26: Edelson (1987ApJ...313..651E 1987ApJ...313..651E) 27: Gregory and Condon (1991) Cat. VIII/14 28: White and Becker Cat. J/MNRAS/251/330 29: Wright et al. Cat. J/MNRAS/251/330 30: Jagers et al. (1982A+A...105..279J 1982A+A...105..279J) 31: Bolton et al. (1971AuJPh..24..889B 1971AuJPh..24..889B) 32: Shimmins et al. (1966AuJPh..19..837S 1966AuJPh..19..837S) 33: Barvainis and Antonucci (1989ApJS...70..257B 1989ApJS...70..257B) -------------------------------------------------------------------------------- Byte-by-byte Description of file: table10 -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 9 A9 --- Name Quasar name 11- 14 F4.2 mm lambda Line 15 A1 --- l_S Limit flag on flux 16- 23 F8.2 mJy S Flux at lambda 24- 29 F6.1 mJy e_S ? rms uncertainty on flux 31- 34 I4 yr Date Obsercation date 40- 44 A5 --- Tel Telescope 47- 48 I2 --- Ref References (1) -------------------------------------------------------------------------------- Note (1): 1) Antonucci, Barvainis and Alloin (1990) (1990ApJ...353..416A 1990ApJ...353..416A) 2) Barvainis and Antonucci (1989) (1989ApJS...70..257B 1989ApJS...70..257B) 3) Chini, Kreysa and Biermann (1989) (1989A&A...219...87C 1989A&A...219...87C) 4) Clegg, et al. (1983) (1983ApJ...273...58C 1983ApJ...273...58C) 5) Edelson, Malkan and Rieke (1987) (1987ApJ...321..233E 1987ApJ...321..233E) 6) Engargiola et al. (1988) (1988ApJ...332L..19E 1988ApJ...332L..19E) 7) Ennis, Neguebauer and Werner (1982) (1982ApJ...262..460E 1982ApJ...262..460E) 8) Landau, Epstein and Rather (1980) 9) Owen, et al. (1978) 10) Owen and Puschell (1982) 11) Robson, et al. (1985) (1985MNRAS.213..355R 1985MNRAS.213..355R) 12) Steppe, et al. (1988) (1988A&AS...75..317S 1988A&AS...75..317S) -------------------------------------------------------------------------------- Byte-by-byte Description of file: table11 -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 3 A3 --- Band Band 6- 10 F5.2 um Lambda Reference lambda 12- 17 F6.1 Jy Zeropt1 Zero point (Vega) (1) 19- 22 I4 Jy Zeropt2 Zero point (alpha = 1) (1) -------------------------------------------------------------------------------- Note (1): The zero points correspond to a system in which the magnitude of Vega is exactly zero. Values are given for an object with the same spectrum as Vega and for an object with a flat energy distribution (power-law spectrum Fν of slope unity) -------------------------------------------------------------------------------- Byte-by-byte Description of file: table12 -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 9 A9 --- Name Object name 11- 15 F5.2 [solLum] logL H band luminosity (1) 17- 20 F4.2 [solLum] E_logL Error in logL (upper limit) 22- 25 F4.2 [solLum] e_logL Error in logL (lower limit) 27- 31 F5.2 kpc Rad Half-light radius (1) 33 I1 --- Ref References (2) -------------------------------------------------------------------------------- Note (1): Adopted luminosities and half light radii for host galaxies, derived as discussed in the text. Note (2): No spatial information was available for objects marked with reference (0), and they have been assigned the median luminosity of the remainder of the sample. 1: Boroson, Oke and Green (1982) (1982ApJ...263...32B 1982ApJ...263...32B) 2: Gehren et al. (1984) (1984ApJ...278...11G 1984ApJ...278...11G) 3: Smith et al. (1986) (1986ApJ...306...64S 1986ApJ...306...64S) 4: Boroson and Oke (1984) (1984ApJ...281..535B 1984ApJ...281..535B) 5: McAlary et al. (1983) (1983ApJS...52..341M 1983ApJS...52..341M) 6: Neugebauer et al. (1985) (1985ApJ...298..275N 1985ApJ...298..275N) 7: Yee and Green (1987) (1987AJ.....94..618Y 1987AJ.....94..618Y) 8: Hutchings, Crampton and Campbell (1984) (1984ApJ...280...41H 1984ApJ...280...41H) 9: Griersmith and Visvanathan (1979) (1979A&A....79..329G 1979A&A....79..329G) -------------------------------------------------------------------------------- References: Antonucci and Barvainis, 1988 Apj 325, 21 =1988ApJ...325L..21A 1988ApJ...325L..21A Antonucci et al. 1990, ApJ 353, 416 =1990ApJ...353..416A 1990ApJ...353..416A Barvainis and Antonucci, 1989, ApJS 70, 257 =1989ApJS...70..257B 1989ApJS...70..257B Bolton and Butler, 1975, Aust. J. Phys. Supl. 34, 33 =1975AuJPA..34...33B 1975AuJPA..34...33B Bolton et al., 1971, Aust. J. Phys. 24, 889 =1971AuJPh..24..889B 1971AuJPh..24..889B Boroson and Oke, 1984, ApJ 281, 535 =1984ApJ...281..535B 1984ApJ...281..535B Boroson, Oke and Green, 1982, ApJ 263, 32 =1982ApJ...263...32B 1982ApJ...263...32B Chini, Kreysa and Biermann, 1989, A&A 219, 87 =1989A&A...219...87C 1989A&A...219...87C Clegg, et al., 1983, ApJ 273, 58 =1983ApJ...273...58C 1983ApJ...273...58C Comastri et al., 1992, ApJ 384, 62 =1992ApJ...384...62C 1992ApJ...384...62C Della Ceca et al., 1990, ApJS 72, 471 =Cat. VII/181 Edelson, 1987, ApJ 313, 651 =1987ApJ...313..651E 1987ApJ...313..651E Edelson, Malkan and Rieke, 1987, ApJ 321, 233 =1987ApJ...321..233E 1987ApJ...321..233E Ekers, 1969, Aust. J. Phys. Supl. 7, 1 =1969AuJPS...7....1E 1969AuJPS...7....1E Elvis et al., 1991, ApJ 378, 537 =1991ApJ...378..537E 1991ApJ...378..537E Engargiola et al., 1988, ApJ 332, 19 =1988ApJ...332L..19E 1988ApJ...332L..19E Ennis et al. 1982, ApJ 262, 460 =1982ApJ...262..460E 1982ApJ...262..460E Feigelson et al., 1984, AJ 89, 1464 =1984AJ.....89.1464F 1984AJ.....89.1464F Gehren et al., 1984, ApJ 278, 11 =1984ApJ...278...11G 1984ApJ...278...11G Gower and Hutchings, 1984, AJ 89, 1658 =1984AJ.....89.1658G 1984AJ.....89.1658G Gregory and Condon, 1991, ApJS 95, 1011 =Cat. VIII/14 Griersmith and Visvanathan, 1979, A&A 79, 329 =1979A&A....79..329G 1979A&A....79..329G Hintzen, Ulvestad and Owen, 1983, AJ 88, 709 =1983AJ.....88..709H 1983AJ.....88..709H Hutchings and Gower, 1985, AJ 90, 405 =1985AJ.....90..405H 1985AJ.....90..405H Hutchings et al.. 1984, ApJ 280, 41 =1984ApJ...280...41H 1984ApJ...280...41H Gioia I., private communication Jagers et al., 1982 A&A 105, 279 =1982A+A...105..279J 1982A+A...105..279J Kellerman et al., 1989, AJ 98, 1195 =1989AJ.....98.1195K 1989AJ.....98.1195K Landau, Epstein and Rather, 1980 AJ 85, 363 =1980AJ.....85..363L 1980AJ.....85..363L Masnou et al., 1992, A&A 253, 35 =1992A&A...253...35M 1992A&A...253...35M McAlary et al., 1983, ApJS 52, 341 =1983ApJS...52..341M 1983ApJS...52..341M Meurs and Wilson, 1981, A&AS 45, 99 =1981A+AS...45...99M 1981A+AS...45...99M Miley and Hartsuijker, 1978, A&AS 34, 129 =1978A+AS...34..129M 1978A+AS...34..129M Neugebauer et al., 1985, ApJ 298, 275 =1985ApJ...298..275N 1985ApJ...298..275N Ohashi et al., 1992, ApJ 398, 87 =1992ApJ...398...87O 1992ApJ...398...87O Owen and Puschell, 1982, AJ 87, 595 =1982AJ.....87..595O 1982AJ.....87..595O Owen, Porcas and Neff, 1978, AJ 83, 1009 =1978AJ.....83.1009O 1978AJ.....83.1009O Perley, 1982, AJ 87, 859 =1982AJ.....87..859P 1982AJ.....87..859P Pooley and Henbest, 1974, MNRAS 169, 477 =1974MNRAS.169..477P 1974MNRAS.169..477P Preston et al., 1985, AJ 90, 1599 =1985AJ.....90.1599P 1985AJ.....90.1599P Price and Milne, 1965, Aust. J. Phys. 18, 329 =1965AuJPh..18..329P 1965AuJPh..18..329P Rieke G.H. & Lebofsky M.J. 1985, ApJ, 288, 618 =1985ApJ...288..618R 1985ApJ...288..618R Robson, et al., 1985, MNRAS 213, 355 =1985MNRAS.213..355R 1985MNRAS.213..355R Rudnick, Sitko, and Stein, 1984, AJ 89, 753 =1984AJ.....89..753R 1984AJ.....89..753R Savage and Mathis 1979, ARA&A 17, 73 =1979ARA&A..17...73S 1979ARA&A..17...73S Saxton et al., 1993, MNRAS 262, 63 =1993MNRAS.262...63S 1993MNRAS.262...63S Shimmins & Bolton, 1972a, Aust. J. Phys. Ap. S. 23, 1 =1972AuJPS..23....1S 1972AuJPS..23....1S Shimmins & Bolton, 1972b, Aust. J. Phys. Ap. S. 26, 1 =1972AuJPS..26....1S 1972AuJPS..26....1S Shimmins & Bolton, 1981, Aust. J. Phys. 34, 471 =1972AuJPh..34..471S 1972AuJPh..34..471S Shimmins et al., 1966, Aust. J. Phys. 19, 837 =1966AuJPh..19..837S 1966AuJPh..19..837S Smith et al., 1986, ApJ 306, 64 =1986ApJ...306...64S 1986ApJ...306...64S Spencer et al., 1989, MNRAS 240, 657 =1989MNRAS.240..657S 1989MNRAS.240..657S Steppe, et al., 1988, A&AS 75, 317 =1988A&AS...75..317S 1988A&AS...75..317S Swarup et al., 1984, MNRAS 208, 813 =1984MNRAS.208..813S 1984MNRAS.208..813S Tananbaum et al., 1986, ApJ 305, 57 =1986ApJ...305...57T 1986ApJ...305...57T Turner and Pounds, 1988, MNRAS 232, 463 =1988MNRAS.232..463T 1988MNRAS.232..463T Turner and Pounds, 1989, MNRAS 240, 833 =1989MNRAS.240..833T 1989MNRAS.240..833T Unger et al., 1987, MNRAS 228, 521 =1987MNRAS.228..521U 1987MNRAS.228..521U White and Becker, 1992, ApJs 79, 331 =Cat. VIII/17 Wilkes and Elvis, 1987, ApJ 323, 243 =1987ApJ...323..243W 1987ApJ...323..243W Williams et al., 1992, ApJ 389, 157 =1992ApJ...389..157W 1992ApJ...389..157W Wills, 1975, Aust. J. Phys. Ap. Suppl. 38, 1 =1975AuJPS..38....1W 1975AuJPS..38....1W Wills, 1979, ApJS 39, 291 =1979ApJS...39..291W 1979ApJS...39..291W Wright et al., 1991, MNRAS 251, 330 =Cat. J/MNRAS/251/330 Yee and Green, 1987, AJ 94, 618 =1987AJ.....94..618Y 1987AJ.....94..618Y Origin: AAS CD-ROM series, Volume 3, 1995 Lee Brotzman [ADS] 13-Nov-94
(End) [CDS] 22-Feb-1996
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