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Yıl: 2023 Cilt: 47 Sayı: 3 Sayfa Aralığı: 124 - 129 Metin Dili: İngilizce DOI: 10.55730/1300-0101.2742 İndeks Tarihi: 14-03-2024

Short-term optical variability of 4C 29.45

Öz:
We observed the flat-spectrum radio quasar 4C 29.45 in the BVRI optical bands for 39 nights from February 2022 to July 2022 with the T60 telescope at T ̈UB ̇ITAK National Observatory (TUG) in Turkey. In this study, we aimed to study flux, color, and spectral variability on short timescales. The object was in an active (bright) phase with an average optical R-band brightness of 14.7 mag and was variable in the BVRI bands throughout the monitoring period. We analyzed the flux variability during our observation period, and the variability amplitudes in V, R, and I bands were determined to be 220% , 208% , and 209% , respectively. Optical spectral energy distributions of 4C 29.45 were derived from the observational data of 33 nights, indicating spectral indices ranging from 1.032 to 1.573. We found modest correlations between optical light curves, and between R-band light curve and spectral indices, suggesting that the time lag ranges from several hours to days. Investigation on relation between spectral and color indices versus R-band magnitude revealed achromatic trend during the bright phase of 4C 29.45 in the first half of 2022. Our periodicity search suggested that the periodicity would be larger than 100 days, and no significant signal for periodicity was found for short timescales.
Anahtar Kelime: AGN blazar flux variability

Belge Türü: Makale Makale Türü: Araştırma Makalesi Erişim Türü: Erişime Açık
  • [1] C. M. Urry and P. Padovani, “Unified schemes for radio-loud active galactic nuclei,” Publications of the Astronomical Society of the Pacific 107 (1995) 803.
  • [2] S. J. Wagner and Witzel A., “Intraday Variability in Quasars and BL LAC Objects,” Annual Review of Astronomy and Astrophysics 33 (1995) 163.
  • [3] M. J. Valtonen, H. J. Lehto, K. Nilsson, J. Heidt and L. O. Takalo et al., “A massive binary black-hole system in OJ 287 and a test of general relativity,” Nature 452 (2008) 851.
  • [4] G. Z. Xie, S. B. Zhou, K. H. Li, H. Dai, L. E. Chen and L. Ma “CCD photometric studies of rapid variability in eight blazars,” Monthly Notices of the Royal Astronomical Society 348 (2004) 831.
  • [5] A. C. Gupta, J. H. Fan, J. M. Bai and S. J. Wagner, “Optical Intra-day Variability in Blazars,” The Astronomical Journal 135 (2008) 1384.
  • [6] A. Agarwal, A. Pandey, A. ̈Ozd ̈onmez, E. Ege, Das A. Kumar and V. Karakulak, “Characterizing the Optical Nature of the Blazar S5 1803+784 during Its 2020 Flare,” The Astrophysical Journal 933 (2022) 42.
  • [7] A. P. Marscher and J. P. Travis, “Synchrotron self-Compton interpretation of multiwaveband observations of gamma-ray bright blazars,” Astronomy and Astrophysics Supplement Series 120 (1996) 537.
  • [8] P. J. Wiita, “Accretion Disk Models for Rapid Variability,” Astronomical Society of the Pacific Conference Series 110 (1996) 42.
  • [9] P. Schneider and A. Weiss, “A gravitational lens origin for AGN-variability?,” Astronomy and Astrophysics 171 (1987) 49.
  • [10] C. M. Raiteri, M. Villata, J. A. Acosta-Pulido, I. Agudo, A. A. Arkharov et al., “Blazar spectral variability as explained by a twisted inhomogeneous jet,” Nature 552 (1997) 374.
  • [11] S. Ciprini, G. Tosti, C. M. Raiteri, M. Villata, M. A. Ibrahimov et al., “Optical variability of the BL Lacertae object GC 0109+224: Multiband behaviour and time scales from a 7-years monitoring campaign,” Astronomy and Astrophysics 400 (2003) 487.
  • [12] A. Agarwal, A. C. Gupta, “Multiband optical variability studies of BL Lacertae,” Monthly Notices of the Royal Astronomical Society 450 (2015) 541.
  • [13] G. Ghisellin , M. Villata, C. M. Raiteri, S. Bosio, G. de Francesco et al., “Optical-IUE observations of the gamma-ray loud BL Lacertae object S5 0716+714: data and interpretation,” Astronomy and Astrophysics 327 (1997) 61.
  • [14] M. Villata, C. M. Raiteri, O. M. Kurtanidze, M. G. Nikolashvili, M. A. Ibrahimov et al., “The WEBT BL Lacertae Campaign 2000,”Astronomy and Astrophysics 390 (2002) 407.
  • [15] B. Rani, A. C. Gupta, A. Strigachev, R. Bachev, P. J. Wiita et al., “Short-term flux and colour variations in low-energy peaked blazars,” Monthly Notices of the Royal Astronomical Society 404 (2010) 1992.
  • [16] A. Agarwal, S. A. Cellone, I. Andruchow, L. Mammana, M. Singh et al., “Multiband optical variability of 3C 279 on diverse time-scales,” Monthly Notices of the Royal Astronomical Society 488 (2019) 4093.
  • [17] M. Villata, C. M. Raiteri, T. J. Balonek, M. F. Aller, S. G Jorstad et al., “The unprecedented optical outburst of the quasar 3C 454.3,” Astronomy and Astrophysics 453 (2006) 817.
  • [18] M.-F. Gu, Y. L. Ai, “The optical variability of flat-spectrum radio quasars in the SDSS stripe 82 region,” Astronomy and Astrophysics 528 (2011) A95.
  • [19] A. Agarwal, B. Mihov, I. Andruchow, S. A. Cellone, G. C. Anupama et al., “Multi-band behaviour of the TeV blazar PG 1553+113 in optical range on diverse timescales,” Astronomy and Astrophysics 645 (2021) A137.
  • [20] A. C. Gupta, A. Agarwal, J. Bhagwan, A. Strigachev, R. Bachev et al., “Multiband optical variability of three TeV blazars on diverse time-scales,” Monthly Notices of the Royal Astronomical Society 458 (2016) 1127.
  • [21] J. C. Isler, C. M. Urry, P. Coppi, C. Bailyn, M. Brady et al., “A Consolidated Framework of the Color Variability in Blazars: Long-term Optical/Near-infrared Observations of 3C 279,” The Astrophysical Journal 844 (2017) 107.
  • [22] V. Negi, R. Joshi, K. Chand, H. Chand, P. Wiita et al., “Optical flux and colour variability of blazars in the ZTF survey,” Monthly Notices of the Royal Astronomical Society 510 (2022) 1791.
  • [23] K. K. Ghosh, B. D. Ramsey, A. C. Sadun and S. Soundararajaperumal, “Optical Variability of Blazars,” The Astrophysical Journal Supplement Series 127 (2000) 11.
  • [24] C. S. Stalin, Gopal-Krishna, R. Sagar, P. J. Wiita, V. Mohan, A. K. Pandey, “Multiband optical monitoring of the blazars S5 0716+714 and BL Lacertae,” Monthly Notices of the Royal Astronomical Society 366 (2006)1337.
  • [25] M. B ̈ottcher, S. Basu, M. Joshi, M. Villata, A. Arai et al., “The WEBT Campaign on the Blazar 3C 279 in 2006,” The Astrophysical Journal 670 (2007) 968.
  • [26] H. Poon, J. H. Fan and J. N. Fu, “The Optical Microvariability and Spectral Changes of the BL Lacertae object S5 0716+714,” The Astrophysical Journal Supplement Series 185 (2009) 511.
  • [27] B. J. Wills, J. T. Pollock, H. D. Aller, M. F. Aller, T. J. Balonek et al., “The QSO 1156+295: a multifrequency study of recent activity,” The Astrophysical Journal 274 (1983) 62.
  • [28] B. J. Wills, D. Wills, M. Breger, R. R. J. Antonucci and R. Barvainis, “A Survey for High Optical Polarization in Quasars with Core-dominant Radio Structure: Is There a Beamed Optical Continuum?,” The Astrophysical Journal 398 (1992) 454.
  • [29] J. H. Fan, J. Tao, B. C. Qian, A. C. Gupta, Y. Liu et al., “Optical Photometrical Observations and Variability for Quasar 4C 29.45,” Publications of the Astronomical Society of Japan 58 (2006) 797.
  • [30] T. Hovatta, M. Tornikoski, M. Lainela, H. J. Lehto, E. Valtaoja et al., “Statistical analyses of long-term variability of AGN at high radio frequencies,” Astronomy and Astrophysics 469 (2007) 899.
  • [31] T. Savolainen, Y. Y. Kovalev, “Serendipitous VLBI detection of rapid, large-amplitude, intraday variability in QSO 1156+295,” Astronomy and Astrophysics 489 (2008) L33.
  • [32] M. K. Hallum, S. G. Jorstad, V. M. Larionov, A. P. Marscher, M. Joshi et al., “Emission-line Variability during a Nonthermal Outburst in the Gamma-Ray Bright Quasar 1156+295,” The Astrophysical Journal 926 (2022) 180.
  • [33] I. M. McHardy, A. P. Marscher, W. K. Gear, T. Muxlow, H. J. Lehto, R. G. Abraham, “VLBI, MERLIN and VLA observations of the blazar 1156+295 : a bending relativistic jet,” Monthly Notices of the Royal Astronomical Society 246 (1990) 305.
  • [34] D. J. Thompson, D. L. Bertsch, B. L. Dingus, J. A. Esposito, A. Etienne et al., “The Second EGRET Catalog of High-Energy Gamma-Ray Sources,” The Astrophysical Journal Supplement Series 101 (1995) 259.
  • [35] S. G. Jorstad, A. P. Marscher, D. A. Morozova, I. S. Troitsky, I. Agudo et al., “Kinematics of Parsec-scale Jets of Gamma-Ray Blazars at 43 GHz within the VLBA-BU-BLAZAR Program,” The Astrophysical Journal 846 (2017) 98.
  • [36] R. Branly, R. Kilgard, A. Sadun, A. Shcherbanovsky and J. Webb , “Optical Monitoring of AGN Using the SARA Telescope: First Results,” Astronomical Society of the Pacific Conference Series 110 (1996) 170.
  • [37] J. C. Noble and H. R. Miller, “Extreme Optical Microvariability in Three Selected Blazars,” Astronomical Society of the Pacific Conference Series 110 (1996) 30.
  • [38] V. Ramakrishnan, J. Le ́on-Tavares, E. A. Rastorgueva-Foi, K. Wiik, S. G. Jorstad et al., “The connection between the parsec-scale radio jet and γ -ray flares in the blazar 1156+295,” Monthly Notices of the Royal Astronomical Society 445 (2014) 1636.
  • [39] N. Du, M. L. Hulburt, H.-E. H. Choi, R. M. Corcoran, T. J. Balonek, “Bright Optical Flares in Blazars 1156+295 and 1308+326,” The Astronomer’s Telegram (2022) 15441.
  • [40] L. Bradley, B. Sip ̋ocz, T. Robitaille, E. Tollerud, Z. Vin ́ıcius et al., “astropy/photutils: 1.5.0,” Zenodo (2022).
  • [41] P. S. Smith, T. J. Balonek, P. A. Heckert, R. Elston, G. D. Schmidt, “UBVRI field comparison stars for selected active quasars and BL Lacertae objects,” Astronomical Journal 90 (1985) 1184.
  • [42] J. Heidt and S. J. Wagner, “Statistics of optical intraday variability in a complete sample of radio-selected BL Lacertae objects,” Astronomy and Astrophysics 305 (1996) 42.
  • [43] R. A. Edelson, J. H. Krolik, “The Discrete Correlation Function: A New Method for Analyzing Unevenly Sampled Variability Data,” The Astrophysical Journal 333 (1988) 646.
  • [44] A. Pandey, A. C. Gupta, P. J. Wiita, “X-Ray Intraday Variability of Five TeV Blazars with NuSTAR,” The Astrophysical Journal 841 (2017) 123.
  • [45] V. A. Acciari, S. Ansoldi, L. A. Antonelli, K. Asano, A. Babi ́c et al., “Multiwavelength variability and correlation studies of Mrk 421 during historically low X-ray and γ -ray activity in 2015-2016,” Monthly Notices of the Royal Astronomical Society 504 (2021) 1427.
  • [46] M. Villata, C. M. Raiteri, H. D. Aller, M. F. Aller, H. Ter ̈asranta et al., “The WEBT campaigns on BL Lacertae,” Astronomy and Astrophysics 424 (2004) 497.
  • [47] N. R. Lomb, “Least-squares frequency analysis of unequally spaced data,” Astrophysics and Space Science 39 (1976) 447.
  • [48] J. D. Scargle, “Studies in astronomical time series analysis. II. Statistical aspects of spectral analysis of unevenly spaced data,” The Astrophysical Journal 263 (1982) 835.
  • [49] M. S. Bessell, F. Castelli and B. Plez, “Model atmospheres broad-band colors, bolometric corrections and temperature calibrations for O-M stars,” Astronomy and Astrophysics 333 (1998) 231.
  • [50] M. Sasada, M. Uemura, A. Arai, Y. Fukazawa, K. S. Kawabata et al., “Multiband Photopolarimetric Monitoring of an Outburst of the Blazar 3C 454.3 in 2007,” Publications of the Astronomical Society of Japan 62 (2010) 645.
  • [51] J. Otero-Santos, J. A. Acosta-Pulido, J. Becerra Gonz ́alez, A. Luashvili, N. Castro Segura et al., “A statistical study of the optical spectral variability in gamma-ray blazars,” Monthly Notices of the Royal Astronomical Society 511 (2022) 5611.
APA ÖZDÖNMEZ A (2023). Short-term optical variability of 4C 29.45. , 124 - 129. 10.55730/1300-0101.2742
Chicago ÖZDÖNMEZ Aykut Short-term optical variability of 4C 29.45. (2023): 124 - 129. 10.55730/1300-0101.2742
MLA ÖZDÖNMEZ Aykut Short-term optical variability of 4C 29.45. , 2023, ss.124 - 129. 10.55730/1300-0101.2742
AMA ÖZDÖNMEZ A Short-term optical variability of 4C 29.45. . 2023; 124 - 129. 10.55730/1300-0101.2742
Vancouver ÖZDÖNMEZ A Short-term optical variability of 4C 29.45. . 2023; 124 - 129. 10.55730/1300-0101.2742
IEEE ÖZDÖNMEZ A "Short-term optical variability of 4C 29.45." , ss.124 - 129, 2023. 10.55730/1300-0101.2742
ISNAD ÖZDÖNMEZ, Aykut. "Short-term optical variability of 4C 29.45". (2023), 124-129. https://doi.org/10.55730/1300-0101.2742
APA ÖZDÖNMEZ A (2023). Short-term optical variability of 4C 29.45. Turkish Journal of Physics, 47(3), 124 - 129. 10.55730/1300-0101.2742
Chicago ÖZDÖNMEZ Aykut Short-term optical variability of 4C 29.45. Turkish Journal of Physics 47, no.3 (2023): 124 - 129. 10.55730/1300-0101.2742
MLA ÖZDÖNMEZ Aykut Short-term optical variability of 4C 29.45. Turkish Journal of Physics, vol.47, no.3, 2023, ss.124 - 129. 10.55730/1300-0101.2742
AMA ÖZDÖNMEZ A Short-term optical variability of 4C 29.45. Turkish Journal of Physics. 2023; 47(3): 124 - 129. 10.55730/1300-0101.2742
Vancouver ÖZDÖNMEZ A Short-term optical variability of 4C 29.45. Turkish Journal of Physics. 2023; 47(3): 124 - 129. 10.55730/1300-0101.2742
IEEE ÖZDÖNMEZ A "Short-term optical variability of 4C 29.45." Turkish Journal of Physics, 47, ss.124 - 129, 2023. 10.55730/1300-0101.2742
ISNAD ÖZDÖNMEZ, Aykut. "Short-term optical variability of 4C 29.45". Turkish Journal of Physics 47/3 (2023), 124-129. https://doi.org/10.55730/1300-0101.2742