J/ApJ/896/L19   16yr LC of TXS 0506+056 from MASTER networks   (Lipunov+, 2020)

Optical observations reveal strong evidence for high-energy neutrino progenitor. Lipunov V.M., Kornilov V.G., Zhirkov K., Gorbovskoy E., Budnev N.M., Buckley D.A.H., Rebolo R., Serra-Ricart M., Podesta R., Tyurina N.., Gress O., Sergienko Y., Yurkov V., Gabovich A., Balanutsa P., Gorbunov I., Vlasenko D., Balakin F., Topolev V., Pozdnyakov A., Kuznetsov A., Vladimirov V., Chasovnikov A., Kuvshinov D., Grinshpun V., Minkina E., Petkov V.B., Svertilov S.I., Lopez C., Podesta F., Levato H., Tlatov A., Van Soelen B., Razzaque S., Bottcher M. <Astrophys. J., 896, L19 (2020)> =2020ApJ...896L..19L 2020ApJ...896L..19L
ADC_Keywords: BL Lac objects; Photometry; Optical Keywords: Neutrino astronomy ; Blazars ; Active galactic nuclei ; Automated telescopes ; Automatic patrol telescopes ; High energy astrophysics ; Black holes ; Particle astrophysics ; Ultra-high-energy cosmic radiation Abstract: We present the earliest astronomical observation of a high-energy neutrino error box of which the variability was discovered after high-energy-neutrino detection. The one robotic telescope of the MASTER global international networks automatically imaged the error box of the very high-energy-neutrino event IceCube-170922A. Observations were carried out in minutes after the IceCube-170922A neutrino event was detected by the IceCube observatory at the South Pole. MASTER found the blazar TXS 0506+056 to be in the off-state after one minute and then switched to the on-state no later than two hours after the event. The effect is observed at a 50σ significance level. We also present own a unique 16yr light curve of blazar TXS 0506+056 (518 data set). Description: This article was attended by eight sites of the MASTER Global Robotic Network: MASTER-Amur (Blagoveshchensk, Russian Far East), MASTER-Tunka (located near Baykal Lake in Siberia, Russia), MASTER-Vostryakovo (near the Moscow), MASTER-Tavrida (Crimea, Russia), MASTER-Kislovodsk (Caucasus, Russia), MASTER-SAAO (South Africa), MASTER-IAC (Tenerife, Spain), and MASTER-OAFA (Argentina). Objects: --------------------------------------------------------------- RA (ICRS) DE Designation(s) --------------------------------------------------------------- 05 09 25.96 +05 41 35.3 TXS 0506+056 = QSO J0509+0541 05 09.7 +05 43 IceCube-170922A = IceCube-170922A --------------------------------------------------------------- File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 91 517 MASTER-NET photometry of the blazar TXS 0506+056 since 2005 till 2020 years in Clear band -------------------------------------------------------------------------------- See also: B/vsx : AAVSO International Variable Star Index VSX (Watson+, 2006-2014) I/345 : Gaia DR2 (Gaia Collaboration, 2018) J/ApJS/194/29 : Observations of blazars at 15GHz (Richards+, 2011) J/ApJ/742/27 : 15GHz and jet properties of MOJAVE blazars (Lister+, 2011) J/ApJ/748/68 : WISE IR colors of gamma-ray blazars (D'Abrusco+, 2012) J/ApJ/767/14 : MASIV survey III. Optical identifications (Pursimo+, 2013) J/ApJS/212/15 : Polarized NVSS sources SEDs (Farnes+, 2014) J/MNRAS/438/3058 : 15GHz variability of γ-ray blazars (Richards+, 2014) J/MNRAS/450/2658 : RATAN-600 flux densities of 123 blazars (Mufakharov+, 2015) J/other/AstBu/70.264 : Sample of 877 blazars (Mingaliev+, 2015) J/ApJ/810/14 : Third catalog of LAT-detected AGNs (3LAC) (Ackermann+, 2015) J/ApJ/864/84 : Swift follow-up obs. of TXS 0506+056 (Keivani+, 2018) J/ApJ/873/132 : ICRF3 radio-loud quasars with Gaia DR2 data (Makarov+, 2019) J/ApJ/874/43 : MOJAVE. XVII. pc-scale jet kinematics of AGNs (Lister+, 2019) J/ApJ/880/32 : Opt./γ-ray flares for Fermi-LAT blazars (Liodakis+, 2019) J/ApJS/242/5 : 40yr of astrometric VLBI obs. of ICRF sources (Xu+, 2019) J/A+A/650/A83 : Radio flux densities of neutrino associations (Hovatta+, 2021) Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 13 F13.5 d JD [2453676.5/2458940.4] Julian Date 15- 19 F5.2 mag Clrmag [14.1/15.9] Apparent clear band magnitude 21- 24 F4.2 mag e_Clrmag [0.01/0.2] Uncertainty in Clrmag 26- 43 A18 --- Site Observing site identifier (1) 45- 49 F5.2 mag Ref1mag [14.3/14.7] Reference star 1 apparent magnitude 51- 55 F5.2 mag Ref2mag [14.7/15.1] Reference star 2 apparent magnitude 57- 61 F5.2 mag Ref3mag [14.7/15.1] Reference star 3 apparent magnitude 63- 67 F5.2 mag Ref4mag [14.6/15] Reference star 4 apparent magnitude 69- 73 F5.2 mag Ref5mag [14.6/15.1] Reference star 5 apparent magnitude 75- 79 F5.2 mag Ref6mag [14.4/14.9] Reference star 6 apparent magnitude 81- 85 F5.2 mag Ref7mag [15.1/15.8] Reference star 7 apparent magnitude 87- 91 F5.2 mag Ref8mag [14.9/15.5] Reference star 8 apparent magnitude -------------------------------------------------------------------------------- Note (1): Site as follows: MASTER-Amur = Blagoveshchensk, Russian Far East (24 occurrences) MASTER-IAC = Tenerife, Spain (20 occurrences) MASTER-Kislovodsk = Caucasus, Russia (60 occurrences) MASTER-OAFA = Argentina (42 occurrences) MASTER-SAAO = South Africa (212 occurrences) MASTER-Tavrida = Crimea, Russia (53 occurrences) MASTER-Tunka = located near Baykal Lake in Siberia, Russia (24 occurrences) MASTER-Vostryakovo = near the Moscow (82 occurrences) -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Prepared by [AAS], Emmanuelle Perret [CDS] 02-Nov-2021
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