Access to Astronomical Catalogues

← Click to display the menu
J/ApJ/837/45     2006-2012 Rc-band & 4.8GHz obs. of AO 0235+164     (Fan+, 2017)

Variability and period analysis for BL Lac AO 0235+164. Fan J.H., Kurtanidze O., Liu Y., Liu X., Yang J.H., Richter G.M., Nikolashvili M.G., Kurtanidze S.O., Wang H.T., Sasada M., Zhou A.Y., Lin C., Yuan Y.H., Zhang Y.T., Costantin D. <Astrophys. J., 837, 45-45 (2017)> =2017ApJ...837...45F (SIMBAD/NED BibCode)
ADC_Keywords: BL Lac objects ; Photometry, RI ; Radio continuum Keywords: BL Lacertae objects: individual: A0 0235+164; galaxies: active; galaxies: photometry Abstract: Variability is one of the extreme observational properties of BL Lacertae objects. AO 0235+164 is a well-studied BL Lac throughout all electromagnetic wavebands. In the present work, we show its optical R-band photometric observations carried out during the period from 2006 November to 2012 December using the Ap6E CCD camera attached to the primary focus of the 70cm meniscus telescope at Abastumani Observatory, Georgia. During our monitoring period, it showed a large variation of ΔR=4.88mag (14.19-19.07mag) and a short timescale of ΔTv=73.5minutes. During the period of 2006 December to 2009 November, we made radio observations of the source using the 25m radio telescope at Xinjiang Astronomical Observatory. By adopting a discrete correlation function to the optical and radio observations we found that the optical variation leads a radio variation of 23.2±12.9days. Objects: ---------------------------------------------------------- RA (ICRS) DE Designation(s) ---------------------------------------------------------- 02 38 38.93 +16 36 59.3 AO 0235+164 = QSO B0235+1624 ---------------------------------------------------------- File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table3.dat 28 1207 Observational data for AO 0235+164 with the 70cm meniscus telescope at Abastumani Observatory table4.dat 26 754 Radio observations for AO 0235+164 with the 25m telescope at Xinjiang Astronomical Observatory
See also: J/A+AS/129/577 : AO 0235+164 BVRI photometry (Takalo+ 1998) J/ApJ/537/101 : Optical Study for blazars. I. (Fan+, 2000) J/AJ/122/2055 : UBVRIJHK photometry of AGN field stars (Gonzalez-Perez+, 2001) J/A+A/369/758 : VRI photometry of BL Lac (1997-1999) (Fan+, 2001) J/A+A/445/441 : SED of BL Lacertae objects (Nieppola+, 2006) J/AJ/132/1256 : eim BATC photometry of OJ 287 (Wu+, 2006) J/ApJ/672/40 : AO 0235+164 outburst in 2006 December (Hagen-Thorn+, 2008) J/MNRAS/392/1181 : BV(RI)c photometry of 3C 273 (Dai+, 2009) J/ApJ/716/30 : SED of Fermi bright blazars (Abdo+, 2010) J/ApJS/188/405 : Fermi-LAT first source catalog (1FGL) (Abdo+, 2010) J/ApJ/743/171 : The 2LAC catalog (Ackermann+, 2011) J/ApJS/199/31 : Fermi LAT second source catalog (2FGL) (Nolan+, 2012) J/other/RAA/14.1135 : Doppler factor for a Fermi blazar sample (Fan+, 2014) J/ApJS/213/26 : Optical light curves of PHL1811 and 3C273 (Fan+, 2014) J/ApJ/810/14 : Third catalog of LAT-detected AGNs (3LAC) (Ackermann+, 2015) J/ApJS/218/18 : 2004-2012 BVRI observations of blazar S5 0716+714 (Dai+, 2015) J/MNRAS/453/1562 : CRTS close supermassive black hole binaries (Graham+, 2015) J/ApJS/226/20 : X-ray, opt. & radio SEDs of Fermi blazars (Fan+, 2016) J/A+A/591/A21 : Optical flux behaviour of Fermi blazars (Marchesini+, 2016) J/A+A/587/A112 : Long term R and V band monitoring of AGN (Taris+, 2016) Byte-by-byte Description of file: table3.dat
Bytes Format Units Label Explanations
1- 13 F13.5 d JD Julian Date 15- 21 F7.4 mag Rmag [14/19.1] R band magnitude 23- 28 F6.4 mag e_Rmag [0/0.6] The 1σ uncertainty in Rmag
Byte-by-byte Description of file: table4.dat
Bytes Format Units Label Explanations
1- 12 F12.4 d JD Julian Date 14- 19 F6.4 Jy F4.8 [0.8/5.4] Flux density at 4.8GHz 21- 26 F6.4 Jy e_F4.8 [0.007/0.07] The 1σ uncertainty at F4.8
History: From electronic version of the journal
(End) Prepared by [AAS], Emmanuelle Perret [CDS] 16-Oct-2017
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

catalogue service

© Unistra/CNRS

CDS.SocialNetLogos - Contact