001     598574
005     20250715173522.0
024 7 _ |a 10.3847/1538-4365/acb059
|2 doi
024 7 _ |a Roy:2023gno
|2 INSPIRETeX
024 7 _ |a inspire:2620690
|2 inspire
024 7 _ |a 0067-0049
|2 ISSN
024 7 _ |a 1538-4365
|2 ISSN
024 7 _ |a arXiv:2301.01944
|2 arXiv
024 7 _ |a 10.3204/PUBDB-2023-06893
|2 datacite_doi
024 7 _ |a altmetric:140864673
|2 altmetric
024 7 _ |a WOS:000937564200001
|2 WOS
024 7 _ |2 openalex
|a openalex:W4321597942
037 _ _ |a PUBDB-2023-06893
041 _ _ |a English
082 _ _ |a 520
088 _ _ |a arXiv:2301.01944
|2 arXiv
100 1 _ |a Roy, Abhradeep
|0 0000-0002-4998-4560
|b 0
|e Corresponding author
245 _ _ |a Study of Variability in Long-term Multiwavelength Optical Lightcurves of Blazar AO 0235+164
260 _ _ |a London
|c 2023
|b Institute of Physics Publ.
336 7 _ |a article
|2 DRIVER
336 7 _ |a Output Types/Journal article
|2 DataCite
336 7 _ |a Journal Article
|b journal
|m journal
|0 PUB:(DE-HGF)16
|s 1700220756_3788312
|2 PUB:(DE-HGF)
336 7 _ |a ARTICLE
|2 BibTeX
336 7 _ |a JOURNAL_ARTICLE
|2 ORCID
336 7 _ |a Journal Article
|0 0
|2 EndNote
500 _ _ |a 27 pages, 10 figures. Accepted for publication in The Astrophysical Journal Supplement Series (ApJS)
520 _ _ |a We present a long-term and intraday variability study of optical multiwaveband (U BV RI) data from the blazar AO 0235+164 collected by various telescopes for ∼44 yr (1975–2019). The blazar was found to be significantly variable over the years in all wave bands with a variation of about 6 mag between its low and active states. The variations in the different wave bands are highly correlated without any time lag. We did not observe any significant trend in color variation with time, but we observed a bluer-when-brighter trend between the B − I color index and the R magnitude. Optical BV R-band spectral energy distributions always show a convex shape. Significant intraday variability was frequently seen in the quasi-simultaneous observations of AO 0235+164 made on 22 nights in the R and V bands by the CASLEO and CAHA telescopes during 1999–2019. We also estimated a central supermassive black hole mass of 7.9 × 10$^{7}$ M $_{⊙}$ by analyzing the broad Mg ii emission line in AO 0235+164's spectrum. We briefly explore the probable physical scenarios responsible for the observed variability.
536 _ _ |a 613 - Matter and Radiation from the Universe (POF4-613)
|0 G:(DE-HGF)POF4-613
|c POF4-613
|f POF IV
|x 0
588 _ _ |a Dataset connected to CrossRef, INSPIRE, Journals: bib-pubdb1.desy.de
693 _ _ |0 EXP:(DE-H253)VERITAS-20170101
|5 EXP:(DE-H253)VERITAS-20170101
|e Very Energetic Radiation Imaging Telescope Array System
|x 0
700 1 _ |a Gupta, Alok C.
|0 0000-0002-9331-4388
|b 1
700 1 _ |a Chitnis, Varsha R.
|0 0000-0001-5046-7504
|b 2
700 1 _ |a Cellone, Sergio A.
|0 0000-0002-3866-2726
|b 3
700 1 _ |a Raiteri, Claudia M.
|0 0000-0003-1784-2784
|b 4
700 1 _ |a Romero, Gustavo E.
|0 0000-0002-5260-1807
|b 5
700 1 _ |a Wiita, Paul J.
|0 0000-0002-1029-3746
|b 6
700 1 _ |a Chatterjee, Anshu
|0 0000-0003-0881-9275
|b 7
700 1 _ |a Combi, Jorge A.
|0 0000-0002-2565-5025
|b 8
700 1 _ |a Liao, Mai
|0 0000-0002-9137-7019
|b 9
700 1 _ |a Sarkar, Arkadipta
|0 P:(DE-H253)PIP1101390
|b 10
700 1 _ |a Villata, Massimo
|0 P:(DE-HGF)0
|b 11
773 _ _ |a 10.3847/1538-4365/acb059
|g Vol. 265, no. 1, p. 14 -
|0 PERI:(DE-600)2006860-8
|n 1
|p 14
|t The astrophysical journal / Supplement series
|v 265
|y 2023
|x 0067-0049
787 0 _ |a Roy, Abhradeep et.al.
|d 2023
|i IsParent
|0 PUBDB-2023-06969
|r arXiv:2301.01944
|t Study of Variability in Long-term Multiwavelength Optical Lightcurves of Blazar AO 0235+164
856 4 _ |y OpenAccess
|u https://bib-pubdb1.desy.de/record/598574/files/Study%20of%20Variability%20in%20Long-term%20Multiwavelength%20Optical%20Lightcurves%20of%20Blazar%20AO%200235%2B164.pdf
856 4 _ |y OpenAccess
|x pdfa
|u https://bib-pubdb1.desy.de/record/598574/files/Study%20of%20Variability%20in%20Long-term%20Multiwavelength%20Optical%20Lightcurves%20of%20Blazar%20AO%200235%2B164.pdf?subformat=pdfa
909 C O |o oai:bib-pubdb1.desy.de:598574
|p openaire
|p open_access
|p VDB
|p driver
|p dnbdelivery
910 1 _ |a External Institute
|0 I:(DE-HGF)0
|k Extern
|b 0
|6 0000-0002-4998-4560
910 1 _ |a Deutsches Elektronen-Synchrotron
|0 I:(DE-588b)2008985-5
|k DESY
|b 10
|6 P:(DE-H253)PIP1101390
913 1 _ |a DE-HGF
|b Forschungsbereich Materie
|l Matter and the Universe
|1 G:(DE-HGF)POF4-610
|0 G:(DE-HGF)POF4-613
|3 G:(DE-HGF)POF4
|2 G:(DE-HGF)POF4-600
|4 G:(DE-HGF)POF
|v Matter and Radiation from the Universe
|x 0
914 1 _ |y 2023
915 _ _ |a DBCoverage
|0 StatID:(DE-HGF)0200
|2 StatID
|b SCOPUS
|d 2023-10-22
915 _ _ |a Creative Commons Attribution CC BY 4.0
|0 LIC:(DE-HGF)CCBY4
|2 HGFVOC
915 _ _ |a JCR
|0 StatID:(DE-HGF)0100
|2 StatID
|b ASTROPHYS J SUPPL S : 2022
|d 2023-10-22
915 _ _ |a IF >= 5
|0 StatID:(DE-HGF)9905
|2 StatID
|b ASTROPHYS J SUPPL S : 2022
|d 2023-10-22
915 _ _ |a DBCoverage
|0 StatID:(DE-HGF)0501
|2 StatID
|b DOAJ Seal
|d 2023-04-12T14:53:38Z
915 _ _ |a DBCoverage
|0 StatID:(DE-HGF)0500
|2 StatID
|b DOAJ
|d 2023-04-12T14:53:38Z
915 _ _ |a WoS
|0 StatID:(DE-HGF)0113
|2 StatID
|b Science Citation Index Expanded
|d 2023-10-22
915 _ _ |a Fees
|0 StatID:(DE-HGF)0700
|2 StatID
|d 2023-10-22
915 _ _ |a DBCoverage
|0 StatID:(DE-HGF)0150
|2 StatID
|b Web of Science Core Collection
|d 2023-10-22
915 _ _ |a OpenAccess
|0 StatID:(DE-HGF)0510
|2 StatID
915 _ _ |a Peer Review
|0 StatID:(DE-HGF)0030
|2 StatID
|b DOAJ : Peer review, Anonymous peer review, Double anonymous peer review
|d 2023-04-12T14:53:38Z
915 _ _ |a Article Processing Charges
|0 StatID:(DE-HGF)0561
|2 StatID
|d 2023-10-22
915 _ _ |a DBCoverage
|0 StatID:(DE-HGF)1150
|2 StatID
|b Current Contents - Physical, Chemical and Earth Sciences
|d 2023-10-22
915 _ _ |a DBCoverage
|0 StatID:(DE-HGF)0160
|2 StatID
|b Essential Science Indicators
|d 2023-10-22
915 _ _ |a DBCoverage
|0 StatID:(DE-HGF)0199
|2 StatID
|b Clarivate Analytics Master Journal List
|d 2023-10-22
920 1 _ |0 I:(DE-H253)Z_VER-20210408
|k Z_VER
|l VERITAS
|x 0
980 _ _ |a journal
980 _ _ |a VDB
980 _ _ |a UNRESTRICTED
980 _ _ |a I:(DE-H253)Z_VER-20210408
980 1 _ |a FullTexts


LibraryCollectionCLSMajorCLSMinorLanguageAuthor
Marc 21