J/A+A/591/A130      Dynamic SEDs of southern blazars - DSSB      (Krauss+, 2016)

The TANAMI Multiwavelength Program: Dynamic spectral energy distributions of southern blazars. Krauss F., Wilms J., Kadler M., Ojha R., Schulz R., Trustedt J., Edwards P.G., Stevens J., Ros E., Baumgartner W., Beuchert T., Blanchard J., Buson S., Carpenter B., Dauser T., Falkner S., Gehrels N., Grafe C., Gulyaev S., Hase H., Horiuchi S., Kreikenbohm A., Kreykenbohm I., Langejahn M., Leiter K., Lovell J.E.J., Mueller C., Natusch T., Nesci R., Pursimo T., Phillips C., Ploetz C., Quick J., Tzioumis A.K., Weston S. <Astron. Astrophys. 591, A130 (2016)> =2016A&A...591A.130K 2016A&A...591A.130K (SIMBAD/NED BibCode)
ADC_Keywords: QSOs ; BL Lac objects ; Energy distributions Keywords: galaxies: active - BL Lacertae: general - quasars: general - relativistic processes Abstract: Simultaneous broadband spectral and temporal studies of blazars are an important tool for investigating active galactic nuclei (AGN) jet physics. We study the spectral evolution between quiescent and flaring periods of 22 radio-loud AGN through multiepoch, quasi-simultaneous broadband spectra. For many of these sources these are the first broadband studies. We use a Bayesian block analysis of Fermi/LAT light curves to determine time ranges of constant flux for constructing quasi-simultaneous spectral energy distributions (SEDs). The shapes of the resulting 81 SEDs are described by two logarithmic parabolas and a blackbody spectrum where needed. Description: The Dynamic SEDs of southern blazars catalog is based on a TANAMI multiwavelength project that has been monitoring a sample of 22 radio-loud blazars of the southern sky from radio to gamma-ray wavelengths. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 80 22 Sources used in the SED catalog fit_res.dat 319 81 Fit parameters sp/* . 81 Individual files of fluxes of all SEDs refs.dat 61 25 References -------------------------------------------------------------------------------- Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 2 I2 --- Seq Sequential number 4- 11 A8 --- Name IAU B1950 name 13- 26 A14 --- OName 3FGL association name 28- 39 A12 --- 3FGL 3FGL catalog name (JHHMM.m+DDMM) 41- 46 A6 --- Class Classification 47 A1 --- r_Class Reference for classification, in refs.dat file 49- 53 F5.3 --- z ?=- Redshift 54 A1 --- r_z Reference for redshift, in refs.dat file 56- 63 F8.4 deg RAdeg Right ascension (J2000) 65- 72 F8.4 deg DEdeg Declination (J2000) 73 A1 --- r_Pos Refenrece for position, in refs.dat file 75- 78 F4.2 10+20cm-2 NH Absorbing column (1) 80 I1 --- Nsed number of SEDs -------------------------------------------------------------------------------- Note (1): Absorbing column from (Kalberla et al. 2005A&A...440..775K 2005A&A...440..775K, Cat. VIII/76; Bajaja et al. 2005A&A...440..767B 2005A&A...440..767B, Cat. VII/75). -------------------------------------------------------------------------------- Byte-by-byte Description of file: fit_res.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 8 A8 --- Name IAUB1950 Source designation (HHMM+DDd) 12- 18 A7 --- sed SED state label 22- 29 F8.2 s Tmin MJD start of SED state 33- 40 F8.2 s Tmax MJD end of SED state 44- 51 F8.2 --- nsync Normalization of synchrotron parabola (1) 55- 62 F8.2 --- b_nsync Lower confidence level of normalization (1) 66- 73 F8.2 --- B_nsync Upper confidence level of normalization (1) 78- 81 F4.2 --- async Fit parameter A (photon index) (1) 88- 91 F4.2 --- b_async Lower confidence level of parameter A (1) 98-101 F4.2 --- B_async Upper confidence level of parameter A (1) 106-109 F4.2 --- bsync Fit parameter B (curvature) (1) 116-119 F4.2 --- b_bsync ?=0 Lower confidence level of parameter B (1) 126-129 F4.2 --- B_bsync ?=0 Upper confidence level of parameter B (1) 133-140 E8.3 --- nhe Normalization of high-energy parabola (1) 144-151 E8.3 --- b_nhe Lower confidence level of normalization (1) 155-162 E8.3 --- B_nhe Upper confidence level of normalization (1) 166-169 F4.2 --- ahe Fit parameter A (photon index) of HE parabola (1) 174-177 F4.2 --- b_ahe ?=0 Lower confidence level of parameter A (1) 182-185 F4.2 --- B_ahe ?=0 Upper confidence level of parameter A (1) 189-192 F4.2 --- bhe Fit parameter B (curvature) of HE parabola (1) 197-200 F4.2 --- b_bhe ?=0 Lower confidence level of parameter B (1) 205-208 F4.2 --- B_bhe ?=0 Upper confidence level of parameter B (1) 212-219 E8.3 --- nbb Normalization of blackbody component (1) 223-230 E8.3 --- b_nbb ?=0 Lower confidence level of blackbody normalization (1) 234-241 E8.3 --- B_nbb ?=0 Upper confidence level of blackbody normalization (1) 245-252 E8.3 keV kt Redshifted blackbody temperature (1) 256-263 E8.3 keV b_kt Lower confidence level of blackbody temperature (1) 267-274 E8.3 keV B_kt Upper confidence level of blackbody temperature (1) 278-281 F4.2 10+20cm-2 NH Absorbing column 285-289 F5.2 --- dof Degrees of freedom 294-299 F6.2 --- chir Reduced Chi^2 value 305-308 F4.2 --- lx/ledd X-ray luminosity/Eddington luminosity 314-319 F6.2 --- lbol/ledd Bolometric luminosity/Eddington luminosity -------------------------------------------------------------------------------- Note (1): Note on fit parameters: If confidence level values are given as 0.0, the parameter was frozen in the fit. If the value itself is given as 0.0 the fit component was not used for this fit. -------------------------------------------------------------------------------- Byte-by-byte Description of file: sp/* -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 10 E10.5 Hz bFreq Lower frequency bin 14- 23 E10.5 Hz BFreq Upper frequency bin 27- 36 E10.5 mW/m2 Flux Flux value in given bin 40- 49 E10.5 mW/m2 e_Flux ? Uncertainty of flux value in given bin -------------------------------------------------------------------------------- Byte-by-byte Description of file: refs.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1 A1 --- Ref Reference code 3- 21 A19 --- BibCode BibCode 23- 42 A20 --- Aut Author's name 44- 61 A18 --- Com Comments -------------------------------------------------------------------------------- Acknowledgements: Felicia Krauss, Felicia.Krauss(at)fau.de
(End) Felicia Krauss [FAU], Patricia Vannier [CDS] 31-May-2016
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