Sökning: onr:"swepub:oai:DiVA.org:kth-315345" > Long-term Multiband...
Fältnamn | Indikatorer | Metadata |
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000 | 05102naa a2200481 4500 | |
001 | oai:DiVA.org:kth-315345 | |
003 | SwePub | |
008 | 220704s2022 | |||||||||||000 ||eng| | |
009 | oai:DiVA.org:su-207333 | |
024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-3153452 URI |
024 | 7 | a https://doi.org/10.3847/1538-4365/ac6c2c2 DOI |
024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-2073332 URI |
040 | a (SwePub)kthd (SwePub)su | |
041 | a engb eng | |
042 | 9 SwePub | |
072 | 7 | a ref2 swepub-contenttype |
072 | 7 | a art2 swepub-publicationtype |
100 | 1 | a Gupta, Alok C.u Aryabhatta Res Inst Observat Sci ARIES, Manora Peak 263001, Nainital, India.;Shanghai Frontiers Sci Ctr Gravitat Wave Detect, 800 Dongchuan Rd, Shanghai 200240, Peoples R China.4 aut |
245 | 1 0 | a Long-term Multiband Near-infrared Variability of the Blazar OJ 287 during 2007-2021 |
264 | c 2022-06-17 | |
264 | 1 | b American Astronomical Society,c 2022 |
338 | a print2 rdacarrier | |
500 | a QC 20230404 | |
520 | a We present the most extensive and well-sampled long-term multiband near-infrared (NIR) temporal and spectral variability study of OJ 287, considered to be the best candidate binary supermassive black hole blazar. These observations were made between 2007 December and 2021 November. The source underwent similar to 2-2.5 mag variations in the J, H, and Ks NIR bands. Over these long-term timescales there were no systematic trends in either flux or spectral evolution with time or with the source's flux states. However, on shorter timescales, there are significant variations in flux and spectra indicative of strong changes during different activity states. The NIR spectral energy distributions show diverse facets at each flux state, from the lowest to the highest. The spectra are, in general, consistent with a power-law spectral profile (within 10%) and many of them indicate minor changes (observationally insignificant) in the shift of the peak. The NIR spectra generally steepen during bright phases. We briefly discuss these behaviors in the context of blazar emission scenarios/mechanisms, OJ 287's well-known traditional behavior, and implications for models of the source central engine invoked for its long-term optical semiperiodic variations. | |
650 | 7 | a NATURVETENSKAPx Fysikx Astronomi, astrofysik och kosmologi0 (SwePub)103052 hsv//swe |
650 | 7 | a NATURAL SCIENCESx Physical Sciencesx Astronomy, Astrophysics and Cosmology0 (SwePub)103052 hsv//eng |
700 | 1 | a Kushwaha, Pankaju Aryabhatta Res Inst Observat Sci ARIES, Manora Peak 263001, Nainital, India.;Indian Inst Sci Educ & Res Mohali, Dept Phys Sci, Sect 81, Sas Nagar 140306, Punjab, India.;Chinese Acad Sci, Key Lab Radio Astron, Nanjing 210033, Jiangsu, Peoples R China.4 aut |
700 | 1 | a Carrasco, L.u Inst Nacl Astrofis Opt & Electr, Luis Enrique Erro 1, Puebla 72840, Mexico.4 aut |
700 | 1 | a Xu, Haiguangu Shanghai Frontiers Sci Ctr Gravitat Wave Detect, 800 Dongchuan Rd, Shanghai 200240, Peoples R China.;Shanghai Jiao Tong Univ, Sch Phys & Astron, 800 Dongchuan Rd, Shanghai 200240, Peoples R China.4 aut |
700 | 1 | a Wiita, Paul J.u Coll New Jersey, Dept Phys, 2000 Pennington Rd, Ewing, NJ 08628 USA.4 aut |
700 | 1 | a Escobedo, G.u Inst Nacl Astrofis Opt & Electr, Luis Enrique Erro 1, Puebla 72840, Mexico.4 aut |
700 | 1 | a Porras, A.u Inst Nacl Astrofis Opt & Electr, Luis Enrique Erro 1, Puebla 72840, Mexico.4 aut |
700 | 1 | a Recillas, E.u Inst Nacl Astrofis Opt & Electr, Luis Enrique Erro 1, Puebla 72840, Mexico.4 aut |
700 | 1 | a Mayya, Y. D.u Inst Nacl Astrofis Opt & Electr, Luis Enrique Erro 1, Puebla 72840, Mexico.4 aut |
700 | 1 | a Chavushyan, V.u Inst Nacl Astrofis Opt & Electr, Luis Enrique Erro 1, Puebla 72840, Mexico.4 aut |
700 | 1 | a Villarroel, Beatrizu Stockholms universitet,Nordiska institutet för teoretisk fysik (Nordita),Instituto de Astrofisica de Canarias, Spain,NORDITA, SU;Stockholm Univ, Roslagstullsbacken 23, SE-10691 Stockholm, Sweden.4 aut0 (Swepub:su)bevi1144 |
700 | 1 | a Zhang, Zhongliu Inst Astrofis Canarias, Avda Via Lactea S-N, E-38205 Tenerife, Spain.;Chinese Acad Sci, Shanghai Astron Observ, Shanghai 200030, Peoples R China.4 aut |
710 | 2 | a Aryabhatta Res Inst Observat Sci ARIES, Manora Peak 263001, Nainital, India.;Shanghai Frontiers Sci Ctr Gravitat Wave Detect, 800 Dongchuan Rd, Shanghai 200240, Peoples R China.b Aryabhatta Res Inst Observat Sci ARIES, Manora Peak 263001, Nainital, India.;Indian Inst Sci Educ & Res Mohali, Dept Phys Sci, Sect 81, Sas Nagar 140306, Punjab, India.;Chinese Acad Sci, Key Lab Radio Astron, Nanjing 210033, Jiangsu, Peoples R China.4 org |
773 | 0 | t Astrophysical Journal Supplement Seriesd : American Astronomical Societyg 260:2, s. 39-q 260:2<39-x 0067-0049x 1538-4365 |
856 | 4 | u https://doi.org/10.3847/1538-4365/ac6c2cy Fulltext |
856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-315345 |
856 | 4 8 | u https://doi.org/10.3847/1538-4365/ac6c2c |
856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-207333 |
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