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The VHE SED modelling of Markarian 501 in 2009

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The VHE SED modelling of Markarian 501 in 2009

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dc.contributor.author Sahu, S. es_ES
dc.contributor.author López Fortín, C. E. es_ES
dc.contributor.author Iglesias Martínez, M. E. es_ES
dc.contributor.author Nagataki, S. es_ES
dc.contributor.author Fernández de Córdoba, Pedro es_ES
dc.date.accessioned 2021-05-28T03:32:30Z
dc.date.available 2021-05-28T03:32:30Z
dc.date.issued 2020-02 es_ES
dc.identifier.issn 0035-8711 es_ES
dc.identifier.uri http://hdl.handle.net/10251/166896
dc.description.abstract [EN] The high energy blazar, Markarian 501 was observed as a part of multi-instrument and multiwavelength campaign spanning the whole electromagnetic spectrum for 4.5 months during March 15 to August 1, 2009. On May 1, Whipple 10 m telescope observed a very strong gamma-ray flare in a time interval of about 0.5 h. Apart from this flare, high state and low state emissions were also observed by Whipple, VERITAS and MAGIC telescopes. Using the photohadronic model and accounting for the absorption of the extragalactic background light to these very high energy gamma-rays, excellent fits are obtained for the observed spectra. We have shown that the intrinsic spectrum for low state emission is flat, however, for high and very high states this is a power-law with slowly increasing exponent. es_ES
dc.description.sponsorship The work of SS is partially supported by DGAPA-UNAM(Mexico) Project No. IN103019. SN is partially supported by 'JSPS Grantsin-Aid for Scientific Research KAKENHI (A) 19H00693', 'Pioneering Program of RIKEN for Evolution of Matter in the Universe (r-EMU)', and 'Interdisciplinary Theoretical and Mathematical Sciences Program of RIKEN'. SS is also thankful to Japan Society for the Promotion of Science (JSPS) for the invitational fellow program. es_ES
dc.language Inglés es_ES
dc.publisher Oxford University Press es_ES
dc.relation.ispartof Monthly Notices of the Royal Astronomical Society es_ES
dc.rights Reserva de todos los derechos es_ES
dc.subject Astroparticle physics es_ES
dc.subject BL Lacertae objects: general es_ES
dc.subject Gamma-rays: galaxies es_ES
dc.subject.classification MATEMATICA APLICADA es_ES
dc.title The VHE SED modelling of Markarian 501 in 2009 es_ES
dc.type Artículo es_ES
dc.identifier.doi 10.1093/mnras/staa023 es_ES
dc.relation.projectID info:eu-repo/grantAgreement/UNAM//IN103019/MX/Conexión entre rayos gamma y neutrinos de alta energía: una perspectiva astrofísica./ es_ES
dc.relation.projectID info:eu-repo/grantAgreement/MEXT//19H00693/ es_ES
dc.rights.accessRights Abierto es_ES
dc.contributor.affiliation Universitat Politècnica de València. Departamento de Matemática Aplicada - Departament de Matemàtica Aplicada es_ES
dc.description.bibliographicCitation Sahu, S.; López Fortín, CE.; Iglesias Martínez, ME.; Nagataki, S.; Fernández De Córdoba, P. (2020). The VHE SED modelling of Markarian 501 in 2009. Monthly Notices of the Royal Astronomical Society. 492(2):2261-2267. https://doi.org/10.1093/mnras/staa023 es_ES
dc.description.accrualMethod S es_ES
dc.relation.publisherversion https://doi.org/10.1093/mnras/staa023 es_ES
dc.description.upvformatpinicio 2261 es_ES
dc.description.upvformatpfin 2267 es_ES
dc.type.version info:eu-repo/semantics/publishedVersion es_ES
dc.description.volume 492 es_ES
dc.description.issue 2 es_ES
dc.relation.pasarela S\399835 es_ES
dc.contributor.funder Universidad Nacional Autónoma de México es_ES
dc.contributor.funder Japan Society for the Promotion of Science es_ES
dc.contributor.funder Ministry of Education, Culture, Sports, Science and Technology, Japón es_ES
dc.description.references Abdo, A. A., Ackermann, M., Ajello, M., Asano, K., Baldini, L., Ballet, J., … Bechtol, K. (2009). FERMIDISCOVERY OF GAMMA-RAY EMISSION FROM NGC 1275. The Astrophysical Journal, 699(1), 31-39. doi:10.1088/0004-637x/699/1/31 es_ES
dc.description.references Acciari, V. A., Arlen, T., Aune, T., Beilicke, M., Benbow, W., Böttcher, M., … Bugaev, V. (2011). SPECTRAL ENERGY DISTRIBUTION OF MARKARIAN 501: QUIESCENT STATE VERSUS EXTREME OUTBURST. The Astrophysical Journal, 729(1), 2. doi:10.1088/0004-637x/729/1/2 es_ES
dc.description.references Aharonian, F. A., Akhperjanian, A. G., Barrio, J. A., Bernlöhr, K., Bolz, O., Börst, H., … Denninghoff, S. (2001). Reanalysis of the high energy cutoff of the 1997 Mkn 501 TeV energy spectrum. Astronomy & Astrophysics, 366(1), 62-67. doi:10.1051/0004-6361:20000098 es_ES
dc.description.references Ahnen, M. L., Ansoldi, S., Antonelli, L. A., Antoranz, P., Babic, A., Banerjee, B., … Becerra González, J. (2017). Multiband variability studies and novel broadband SED modeling of Mrk 501 in 2009. Astronomy & Astrophysics, 603, A31. doi:10.1051/0004-6361/201629540 es_ES
dc.description.references Aliu, E., Archambault, S., Archer, A., Arlen, T., Aune, T., Barnacka, A., … Berger, K. (2016). Very high energy outburst of Markarian 501 in May 2009. Astronomy & Astrophysics, 594, A76. doi:10.1051/0004-6361/201628744 es_ES
dc.description.references Baring, M. G., Böttcher, M., & Summerlin, E. J. (2016). Probing acceleration and turbulence at relativistic shocks in blazar jets. Monthly Notices of the Royal Astronomical Society, 464(4), 4875-4894. doi:10.1093/mnras/stw2344 es_ES
dc.description.references Cao, G., & Wang, J. (2014). THE HADRONIC ORIGIN OF THE HARD GAMMA-RAY SPECTRUM FROM BLAZAR 1ES 1101-232. The Astrophysical Journal, 783(2), 108. doi:10.1088/0004-637x/783/2/108 es_ES
dc.description.references Dermer, C. D., & Schlickeiser, R. (1993). Model for the High-Energy Emission from Blazars. The Astrophysical Journal, 416, 458. doi:10.1086/173251 es_ES
dc.description.references Domínguez, A., Finke, J. D., Prada, F., Primack, J. R., Kitaura, F. S., Siana, B., & Paneque, D. (2013). DETECTION OF THE COSMIC γ-RAY HORIZON FROM MULTIWAVELENGTH OBSERVATIONS OF BLAZARS. The Astrophysical Journal, 770(1), 77. doi:10.1088/0004-637x/770/1/77 es_ES
dc.description.references Franceschini, A., Rodighiero, G., & Vaccari, M. (2008). Extragalactic optical-infrared background radiation, its time evolution and the cosmic photon-photon opacity. Astronomy & Astrophysics, 487(3), 837-852. doi:10.1051/0004-6361:200809691 es_ES
dc.description.references Ghisellini, G., Celotti, A., Fossati, G., Maraschi, L., & Comastri, A. (1998). A theoretical unifying scheme for gamma-ray bright blazars. Monthly Notices of the Royal Astronomical Society, 301(2), 451-468. doi:10.1046/j.1365-8711.1998.02032.x es_ES
dc.description.references Gliozzi, M., Sambruna, R. M., Jung, I., Krawczynski, H., Horan, D., & Tavecchio, F. (2006). Long‐Term X‐Ray and TeV Variability of Mrk 501. The Astrophysical Journal, 646(1), 61-75. doi:10.1086/504700 es_ES
dc.description.references Katarzyński, K., Sol, H., & Kus, A. (2001). The multifrequency emission of Mrk 501. Astronomy & Astrophysics, 367(3), 809-825. doi:10.1051/0004-6361:20000538 es_ES
dc.description.references Krawczynski, H., Hughes, S. B., Horan, D., Aharonian, F., Aller, M. F., Aller, H., … Schroder, M. (2004). Multiwavelength Observations of Strong Flares from the TeV Blazar 1ES 1959+650. The Astrophysical Journal, 601(1), 151-164. doi:10.1086/380393 es_ES
dc.description.references Sahu, S. (2019). Multi-TeV flaring in nearby high-energy blazars: A photohadronic scenario. Revista Mexicana de Física, 65(4 Jul-Aug), 307-320. doi:10.31349/revmexfis.65.307 es_ES
dc.description.references Sahu, S., Miranda, L. S., & Rajpoot, S. (2016). Multi-TeV flaring from blazars: Markarian 421 as a case study. The European Physical Journal C, 76(3). doi:10.1140/epjc/s10052-016-3975-2 es_ES
dc.description.references Sahu, S., de León, A. R., & Miranda, L. S. (2017). Photohadronic scenario in interpreting the February–March 2014 flare of 1ES 1011+496. The European Physical Journal C, 77(11). doi:10.1140/epjc/s10052-017-5335-2 es_ES
dc.description.references Sahu, S., Yáñez, M. V. L., Miranda, L. S., de León, A. R., & Gupta, V. (2017). EBL effect on the observation of multi-TeV flaring of 2009 from Markarian 501. The European Physical Journal C, 77(1). doi:10.1140/epjc/s10052-016-4592-9 es_ES
dc.description.references Sahu, S., López Fortín, C. E., & Nagataki, S. (2019). Multi-TeV Flaring from High-energy Blazars: An Evidence of the Photohadronic Process. The Astrophysical Journal, 884(1), L17. doi:10.3847/2041-8213/ab43c7 es_ES
dc.description.references Sambruna, R. M., Aharonian, F. A., Krawczynski, H., Akhperjanian, A. G., Barrio, J. A., Bernlohr, K., … Cortina, J. (2000). Correlated Intense X‐Ray and TeV Activity of Markarian 501 in 1998 June. The Astrophysical Journal, 538(1), 127-133. doi:10.1086/309133 es_ES
dc.description.references Sikora, M., Begelman, M. C., & Rees, M. J. (1994). Comptonization of diffuse ambient radiation by a relativistic jet: The source of gamma rays from blazars? The Astrophysical Journal, 421, 153. doi:10.1086/173633 es_ES
dc.description.references Tavecchio, F., Maraschi, L., Pian, E., Chiappetti, L., Celotti, A., Fossati, G., … Djannati‐Atai, A. (2001). Theoretical Implications from the Spectral Evolution of Markarian 501 Observed withBeppoSAX. The Astrophysical Journal, 554(2), 725-733. doi:10.1086/321394 es_ES
dc.description.references Urry, C. M., & Padovani, P. (1995). Unified Schemes for Radio-Loud Active Galactic Nuclei. Publications of the Astronomical Society of the Pacific, 107, 803. doi:10.1086/133630 es_ES
dc.description.references Zdziarski, A. A., & Böttcher, M. (2015). Hadronic models of blazars require a change of the accretion paradigm. Monthly Notices of the Royal Astronomical Society: Letters, 450(1), L21-L25. doi:10.1093/mnrasl/slv039 es_ES


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