J/A+AS/146/141      Intensive monitoring of OJ 287           (Pursimo+, 2000)

Intensive monitoring of OJ 287. Pursimo T., Takalo L.O., Sillanpaeae A., Kidger M., Lehto H.J., Heidt J., Charles P.A., Aller H., Aller M., Beckmann V., Benitez E., Bock H., Boltwood P., Borgeest U., De Diego J.A., De Francesco G., Dietrich M., Dultzin-Hacyan D., Efimov YU., Fiorucci M., Ghisellini G., Gonzalez-perez J.N., Hanski M., Heinaemaeki P., Honeycutt R.K., Hughes P., Karlamaa K., Katajainen S., Knee L.B.G., Kurtanidze O.M., Kuemmel M., Kuehl D., Lainela M., Lanteri L., Von Linde J., Laehteenmaeki A., Maesano M., Mahoney T., Marchenko S., Marscher A., Massaro E., Montagni F., Nesci R., Nikolashvili M., Nilsson K., Nurmi P., Pietilae H., Poyner G., Raiteri C.M., Rekola R., Richter G.M., Riehokainen A., Robertson J.W., Rodriguez-Espinoza J.M., Sadun A., Shakhovskoy N., Schramm K.J., Schramm T., Sobrito G., Teerikorpi P., Teraesranta H., Tornikoski M., Tosti G., Turner G.W., Valtaoja E., Valtonen M., Villata M., Wagner S.J., Webb J., Weneit W., Wiren S. <Astron. Astrophys. Suppl. Ser., 146, 141-155 (2000)> =2000A&AS..146..141P 2000A&AS..146..141P (SIMBAD/NED BibCode)
ADC_Keywords: BL Lac objects ; Photometry; Polarization; Radio continuum Keywords: BL Lac objects - OJ 287 - photometry Abstract: We present intensive optical, infrared, and radio monitoring observations of the BL Lac object OJ 287, taken between the years 1993-1998. Two large optical outbursts were detected at the predicted times in November 1994 and December 1995. The detection of these outbursts supports the binary black hole model for OJ 287. Optical and radio polarisation observations show large variability in the degree of polarisation and position angle, very similar to those observed during the 1983/84 outburst in OJ 287. The polarisation position angles show very similar behaviour during these observations, indicating that, at least, the magnetic field orientations in radio and optical bands are related in OJ 287. Optical and infrared light curves show continuous variability in time scales ranging from tens of minutes to years. In the radio bands we have observed some of the lowest ever measured flux levels. During the first optical outburst in November 1994 the observed radio flux was very low, but during the second optical outburst radio bands also showed high flux levels. This is a puzzling observation, which can hopefully be used for discriminating between different outburst models. On top of the large outbursts OJ 287 has displayed flaring activity in time scales from days to weeks and shorter time scale flickering. Description: We present intensive optical, infrared, and radio monitoring observations of the BL Lac object OJ 287, taken between the years 1993-1998. Most of the optical observations were taken using CCD-cameras and the data were reduced using standard procedures, i.e. bias and flat field corrections. For these data differential photometry was performed using calibration stars (4,10,11) from (Smith et al. 1985AJ.....90.1184S 1985AJ.....90.1184S) or Fiorucci & Tosti (1996A&AS..116..403F 1996A&AS..116..403F, Cat. J/A+AS/116/403). All the optical polarisation observations were made using similar UBVRI photopolarimeter both at Crimea and at the NOT. The infrared data were collected mostly at the 1.5m Carlos Sanchez telescope on Tenerife, using a single channel CVF-photometer with some additional data from UKIRT. The radio data are nightly averages collected within radio monitoring programs at Michigan, Metsahovi, and SEST, with frequencies from 4.8 to 230GHz. Small amount of UV data was obtained with the IUE-satellite during the first outburst. In addition we provide visual brightness estimates from amateur astronomers. Objects: ------------------------------------------------ RA (2000) DE Designation(s) ------------------------------------------------ 08 54 48.87 +20 06 30.6 OJ 287 = OHIO J 287 ------------------------------------------------ File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 36 9888 Optical observations of OJ 287 table2.dat 35 242 NIR observations of OJ 287 table3.dat 38 1245 Radio flux density 5-375GHz observations of OJ 287 table4.dat 37 7 IUE UV observations of OJ 287 table5.dat 53 437 Optical polarimetry observations of OJ 287 table6.dat 56 526 Radio polarimetry observations of OJ 287 table7.dat 35 134 Visual brightness estimates of OJ 287 -------------------------------------------------------------------------------- See also: J/A+AS/129/569 : BVRI photometry of OJ 287 (Jia Guibin+ 1998) J/AJ/132/1256 : eim BATC photometry of OJ 287 (Wu+, 2006) J/MNRAS/385/823 : UBVRI light curves of OJ 287 (Zheng+, 2008) J/MNRAS/402/2087 : Optical polarization of OJ 287 in 2005-2009 (Villforth+, 2010) J/AJ/141/65 : BATC ceimo light curves of OJ 287 (Dai+, 2011) J/ApJ/764/5 : BR photometry of 2012 precursor flare in OJ287 (Pihajoki+, 2013) J/A+A/597/A80 : GMVA 86GHz images of OJ 287 (Hodgson+, 2017) J/ApJ/835/275 : OJ 287 flux + polarization during 2016 outburst (Rakshit+, 2017) J/A+A/610/A74 : OJ 287 far-infrared photometry (Kidger+, 2018) J/A+A/619/A88 : High cadence polarization monitoring of OJ287 (Myserlis+, 2018) J/AJ/157/95 : Optical variability of OJ 287 in 2016-2017 (Gupta+, 2019) J/ApJ/862/1 : Rotation reversals in the polarization in OJ 287 (Cohen+, 2018) Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 13 F13.5 d JD Time of observation Julian Date 15 A1 --- l_mag Upper limit flag on mag 16- 21 F6.3 mag mag Instrumental Magnitude 23- 27 F5.3 mag e_mag ?=9.999 Uncertainty in Magnitude (brightness upper limit indicated as 9.99) 30 I1 --- B [1/5] Pass Band identifier (G1) 31- 32 I2 --- O [01/16] Observation identifier (G2) 33 I1 --- Inst [1/6] Magnitude zero point (G3) 36 A1 --- Band [UBVRI] Human readable Passband -------------------------------------------------------------------------------- Byte-by-byte Description of file: table2.dat table7.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 13 F13.5 d JD Time of observation Julian Date 15 A1 --- l_mag Upper limt flag on mag 16- 21 F6.3 mag mag Magnitude 23- 27 F5.3 mag e_mag ?=9.999 Magnitude error (brightness upper limit indicated as 9.999) 30 I1 --- B [6/9] Code For Pass Band or Frequency (G1) 31- 32 I2 --- O [13/99] Origin of Observation (G2) 35 A1 --- Band [JHKE] Human readable Passband -------------------------------------------------------------------------------- Byte-by-byte Description of file: table3.dat table4.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 13 F13.5 d JD Time of observation Julian Date 16- 20 F5.3 Jy Flux Flux density 22- 26 F5.3 Jy e_Flux Flux density error 29- 30 I2 --- B [11/20] Code For Frequency (G1) 31- 32 I2 --- O [10/24] Origin of Observation (G2) 35- 38 A4 --- Band Human readable Frequency (1) -------------------------------------------------------------------------------- Note (1): Human readable Frequency: for table3.dat: 4.8, 8.0, 14.5, 22, 37, 90, 150, 230, 270, 375GHz for table4.dat: LWP -------------------------------------------------------------------------------- Byte-by-byte Description of file: table5.dat table6.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 13 F13.5 d JD Time of observation Julian Date 16- 21 F6.3 % P Degree of linear polarization 23- 27 F5.3 % e_P Error in linear polarization 30- 36 F7.3 deg PA Position Angle 38- 44 F7.3 deg e_PA Error in Position Angle 47- 48 I2 --- B [1/13] Code For Band (G1) 49- 50 I2 --- O [01/21] Origin of Observation (G2) 53- 56 A4 --- Band Human readable Passband (1) -------------------------------------------------------------------------------- Note (1): Human readable Passband: for table5.dat: UBVRI for table6.dat: 4.8, 8.0 or 14.5GHz -------------------------------------------------------------------------------- Global notes: Note (G1): Pass Band identifier as follows: 1 = U 2 = B 3 = V 4 = R 5 = I 6 = J 7 = H 8 = K 9 = Eye estimate 10 = LWP 2500Å 11 = 5 GHz 12 = 8 GHz 13 = 14.5 GHz 14 = 22 GHz 15 = 37 GHz 16 = 90 GHz 17 = 150 GHz 18 = 230 GHz 19 = 270 GHz 20 = 375 GHz Note (G2): Observation identifier code as follows: 1 = Nordic Optical Telescope 2 = Jacobus Kapteyn Telescope 3 = Heidelberg 4 = Torino Observatory 5 = Tuorla Observatory 6 = Calar Alto 7 = Boltwood 8 = IAC-80 10 = Cananea 11 = Lowell Observatory 12 = Rome 13 = Crimea Observatory 14 = San Pedro Martir 15 = RoboScope 16 = Perugia Observatory 18 = Carlos Sanchez Telescope 19 = UKIRT 20 = IUE 21 = Michigan Radio Telescope 22 = Metsahovi Radio Telescope 23 = SEST 24 = Stevens J. A. et al., 1994ApJ...437...91S 1994ApJ...437...91S 90 = Day 91 = Hewitt 92 = Jensen 93 = Kinnunen 94 = Nelson 95 = Poyner 96 = Toone 97 = Vanmunster 98 = Westlund 99 = Worraker Note (G3): Instrumental magnitude zero point code as follows: 1 = CCD photmetry: OJ287 magnitude zero point from field stars 2 = CCD photmetry: Magnitude zero point from Star 10 (Smith et al., 1985AJ.....90.1184S 1985AJ.....90.1184S) 3 = CCD photmetry: Magnitude zero point from Star 4 (Smith et al., 1985AJ.....90.1184S 1985AJ.....90.1184S) 4 = CCD photmetry: Magnitude zero point from Star 11 (Smith et al., 1985AJ.....90.1184S 1985AJ.....90.1184S) 5 = CCD photmetry: Magnitude zero point from Star C2 Fiorucci & Tosti 1996, Cat. J/A+AS/116/403 6 = Photopolarimeter -------------------------------------------------------------------------------- Acknowledgements: Tapio Pursimo, tpursimo(at)not.iac.es
(End) Patricia Vannier [CDS] 08-May-2021
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