Estimación del tamaño de la BLR usando la emisión de rayos X de alta energía

ilustraciones, gráficas, tablas

Autores:: Perdomo Rodríguez, Martha Morelia

Tipo de recurso:

Fecha de publicación:: 2022

Institución:: Universidad Nacional de Colombia

Repositorio:: Universidad Nacional de Colombia

Idioma:: spa

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repository_id_str
dc.title.spa.fl_str_mv	Estimación del tamaño de la BLR usando la emisión de rayos X de alta energía
dc.title.translated.eng.fl_str_mv	BLR size estimation using high-energy X-ray emission
title	Estimación del tamaño de la BLR usando la emisión de rayos X de alta energía
spellingShingle	Estimación del tamaño de la BLR usando la emisión de rayos X de alta energía 520 - Astronomía y ciencias afines Galaxias Galaxias:activas Galaxias: nucleo Cuasares:líneas de emisión Galaxias:Seyfert Galaxias: rayos X Galaxies:active Galaxies: nuclei Quasars:emission lines Galaxies:Seyfert Galaxies: X rays
title_short	Estimación del tamaño de la BLR usando la emisión de rayos X de alta energía
title_full	Estimación del tamaño de la BLR usando la emisión de rayos X de alta energía
title_fullStr	Estimación del tamaño de la BLR usando la emisión de rayos X de alta energía
title_full_unstemmed	Estimación del tamaño de la BLR usando la emisión de rayos X de alta energía
title_sort	Estimación del tamaño de la BLR usando la emisión de rayos X de alta energía
dc.creator.fl_str_mv	Perdomo Rodríguez, Martha Morelia
dc.contributor.advisor.none.fl_str_mv	Higuera Garzón, Mario Armando
dc.contributor.author.none.fl_str_mv	Perdomo Rodríguez, Martha Morelia
dc.subject.ddc.spa.fl_str_mv	520 - Astronomía y ciencias afines
topic	520 - Astronomía y ciencias afines Galaxias Galaxias:activas Galaxias: nucleo Cuasares:líneas de emisión Galaxias:Seyfert Galaxias: rayos X Galaxies:active Galaxies: nuclei Quasars:emission lines Galaxies:Seyfert Galaxies: X rays
dc.subject.proposal.spa.fl_str_mv	Galaxias Galaxias:activas Galaxias: nucleo Cuasares:líneas de emisión Galaxias:Seyfert Galaxias: rayos X
dc.subject.proposal.eng.fl_str_mv	Galaxies:active Galaxies: nuclei Quasars:emission lines Galaxies:Seyfert Galaxies: X rays
description	ilustraciones, gráficas, tablas
publishDate	2022
dc.date.accessioned.none.fl_str_mv	2022-08-12T13:34:55Z
dc.date.available.none.fl_str_mv	2022-08-12T13:34:55Z
dc.date.issued.none.fl_str_mv	2022-06-24
dc.type.spa.fl_str_mv	Trabajo de grado - Maestría
dc.type.driver.spa.fl_str_mv	info:eu-repo/semantics/masterThesis
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dc.identifier.instname.spa.fl_str_mv	Universidad Nacional de Colombia
dc.identifier.reponame.spa.fl_str_mv	Repositorio Institucional Universidad Nacional de Colombia
dc.identifier.repourl.spa.fl_str_mv	https://repositorio.unal.edu.co/
url	https://repositorio.unal.edu.co/handle/unal/81862 https://repositorio.unal.edu.co/
identifier_str_mv	Universidad Nacional de Colombia Repositorio Institucional Universidad Nacional de Colombia
dc.language.iso.spa.fl_str_mv	spa
language	spa
dc.relation.references.spa.fl_str_mv	[Abdo, 2010] Abdo, A. (2010). The frst catalogue of active galactic nuclei detected by the fermi large area telescope. Astrophysical Journal, 715:429–457 [Akritas and Bershady, 1996] Akritas and Bershady (1996). Linear regression for astronomical data with measurement errors and intrinsic scatter. Astrophysical Journal, 470:706–714 [Beckmann and Schrader, 2012] Beckmann and Schrader (2012). Active Galactic Nuclei. Wiley-VCH, Weinheim [Bennert and Wilson, 2004] Bennert, N., F. H. S. Y. and Wilson, A. (2004). Comparing agn broad and narrow line regions, in the interplay among black holes, stars and ism in galactic nuclei. IAU Symposium, 222:307–309 [Bentz Misty C. Williams Peter R. and Tommaso, 2021] Bentz Misty C. Williams Peter R., Street Rachel, O. C. A. V. M. and Tommaso, T. (2021). A detailed view of the broad-line region in ngc 3783 from velocity resolved reverberation mapping. Astrophysical Journal, 920:112–123 [Boggs Paul and Robert, 1987] Boggs Paul, B. R. and Robert, S. (1987). A stable and efcient algorithm for nonlinear orthogonal distance regression. Society for Industrial and Applied Mathematics, 8:1052–1078 [Bradley, 1998] Bradley, P. (1998). On uncertainties in cross-correlation lags and the reality of wavelength-dependent continuum lags in active galactic nuclei. Astronomical Society of the Pacifc, 110:660–670. [Cruz de Oliveira and Fernandes de Aguiar, 2013] Cruz de Oliveira, E. and Fernandes de Aguiar, P. (2013). Least squares regression with errors in both variables: Case studies. Quim Nova, 36:885–889 [Czerny Bozena and Vladimir, 2017] Czerny Bozena, Li Yang-Rong, S. K. H. P. S. W. C. and Vladimir, K. (2017). Self consistent model of the broad line region. Frontiers in Astronomy and Space Sciences, 4:1–5 [Edelson and Krolik, 1988] Edelson and Krolik (1988). The discrete correlation function: a new method for analyzing unevenly sampled variability data. Astrophysical Journal, 333:646–656 [Gaskell and Peterson, 1987] Gaskell and Peterson (1987). The accuracy of cross-correlation estimates of quasar emission-line region sizes. Astrophysical Journal, 65:1–11 [Gaskell and Sparke, 1986] Gaskell, C. M. and Sparke, L. (1986). Line variations in quasars and seyfert galaxies. Astrophysical Journal, 305:175–186 [Hagai, 2020] Hagai, N. (2020). Testing broad line region models with reverberation mapping. Montly Notices of Royal Astronomical Society, 494:1611–1621 [Kaspi, 2000] Kaspi, S. (2000). Reverberation measurements for 17 quasars and the sizemass-luminosity relations in active galactic nuclei. Astrophysical Journal, 533:631–649 [Kaspi, 2005] Kaspi, S. (2005). The relationship between luminosity and broad-line region size in active galactic nuclei. Astrophysical Journal, 629:61–71 [Maoz and Netzer, 1989] Maoz, D. and Netzer, H. (1989). Evaluation of the cross-correlation method and the size of agn emission-line regions. Montly Notices of Royal Astronomical Society, 236:21–29 [Massaro, 2011] Massaro, F. (2011). Large-scale extragalactic jets in the chandra era. i. data reduction and analysis. Astrophysical Journal, 197:1–14. [Morgan C.W. and Falco, 2010] Morgan C.W., Kochanek, C.-M. N. and Falco, E. (2010). The quasar accretion disk size- blackhole relation. Astrophysical Journal, 712:1129–1136 [Netzer, 2006] Netzer, H. (2006). Active galactic nuclei: Basic physics and main components. Lec. Notes. Phys., 693:1–37 [Netzer, 2013] Netzer, H. (2013). The Physics and Evolution of Active Galactic Nuclei. Cambridge University Press, New York [P´erez E. and L., 1988] P´erez E., R. A. and L., D. L. F. (1988). The response of the broad emission line region to ionizating continuum variations-iii an atlas of transfer functions. Astrophysical Journal, 333:646–656 [Peterson, 2006] Peterson, B. (2006). The broad line region in active galactic nuclei. Lec. Notes. Phys., 693:77–100 [Peterson, 1997] Peterson, B. M. (1997). An Introduction to Active Galactic Nuclei. Cambridge University Press, Cambridge [Peterson, 2004] Peterson, B. M. (2004). Central masses and broad-line region sizes of active galactic nuclei. ii. a homogeneous analysis of a large reverberation-mapping database. Astrophysical Journal, 613:682–699 [Press, 1992] Press, W. (1992). Numerical recipes in C: The art of scientifc computing. Cambridge University Press, Cambridge [Raimundo S.I and A.J., 2019] Raimundo S.I, Pancoast A., V. M. G. M. and A.J., B. (2019). Modelling the agn broad line region using single-epoch spectra-i the case test of arp 151. Montly Notices of Royal Astronomical Society, 489:1899–1918. [Robert, 1993] Robert, A. (1993). Unifed models for active galactic nuclei and quasars. Annual Review Astronomical Astrophysics, 31:473–521 [Shemmer, 2003] Shemmer, O. (2003). Complex optical-x-ray correlations in the narrow-line seyfert 1 galaxy ngc 4051. Royal Astronomical Society, 343:1341–1347. [Soldi, 2014] Soldi, S. (2014). Long-term variability of agn at hard x-rays. Astronomy Astrophysical, 563:1–17 [Soldi., 2014] Soldi., S. (2014). Long-term variability of agn at hard x-rays. Astronomy Astrophysical, A57:1–16. Tremaine, 2002] Tremaine, S. (2002). The slope of the black hole mass versus velocity dispersion correlation. Astrophysical Journal, 574:740–753 [Urry. and Padovani, 1995] Urry., C. and Padovani, P. (1995). Unifed schemes for radio-loud active galactic nuclei. Astronomical Society of the Pacifc, 107:803–846 [Welsh., 1999] Welsh., W. (1999). On the reliability of cross-correlation function lag determinations in active galactic nuclei. Astronomical Society of the Pacifc, 111:1347–1366 [White and Peterson, 1994] White and Peterson (1994). Comments on cross-correlation methodology in variability studies of active galactic nuclei. Astronomical Society of the Pacifc, 106:879–889 [Zhang, 2019] Zhang, Z.-X. (2019). Kinematics of the broad-line region of 3c 273 from a 10 yr reverberation mapping campaign. Astrophysical Journal, 876:1–14
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dc.rights.license.spa.fl_str_mv	Atribución-CompartirIgual 4.0 Internacional
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dc.format.extent.spa.fl_str_mv	xiv, 73 páginas
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dc.publisher.spa.fl_str_mv	Universidad Nacional de Colombia
dc.publisher.program.spa.fl_str_mv	Bogotá - Ciencias - Maestría en Ciencias - Astronomía
dc.publisher.department.spa.fl_str_mv	Observatorio Astronómico Nacional
dc.publisher.faculty.spa.fl_str_mv	Facultad de Ciencias
dc.publisher.place.spa.fl_str_mv	Bogotá, Colombia Bogotá, Colombia
dc.publisher.branch.spa.fl_str_mv	Universidad Nacional de Colombia - Sede Bogotá
institution	Universidad Nacional de Colombia
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spelling	Atribución-CompartirIgual 4.0 Internacionalhttp://creativecommons.org/licenses/by-sa/4.0/info:eu-repo/semantics/openAccesshttp://purl.org/coar/access_right/c_abf2Higuera Garzón, Mario Armandoa12f46c538561a02747286f0cf279f63Perdomo Rodríguez, Martha Morelia79170b48c35b2955865fe3a8efc601ce2022-08-12T13:34:55Z2022-08-12T13:34:55Z2022-06-24https://repositorio.unal.edu.co/handle/unal/81862Universidad Nacional de ColombiaRepositorio Institucional Universidad Nacional de Colombiahttps://repositorio.unal.edu.co/ilustraciones, gráficas, tablasLos mapeos de reverberación han sido la base para encontrar relaciones entre el tamaño de la región de líneas anchas (BLR Broad Line Region por sus siglas en Inglés) y sus luminosidades en las bandas del continuo óptico, ultravioleta, rayos X y líneas de emisión de Balmer. Esta tesis describe y aplicó la técnica del mapeo de reverberación con el fin de conocer la metodología para encontrar el tamaño de la región de líneas anchas, metodología que hace uso de las variaciones correlacionadas entre el continuo y las líneas de emisión [Kaspi, 2000]. Esta tesis partió de la información del tamaño de la región de líneas anchas del grupo de galaxias del trabajo de [Kaspi, 2005] e hizo uso de la base de datos del NED para encontrar datos de luminosidades de estas galaxias en la banda de rayos X duros, con el objetivo de estimar una relación entre el tamaño de la región de líneas anchas y las luminosidades en la banda de rayos X en el rango de 10 keV - 195 KeV, aplicando uno de los métodos de regresión lineal informado en [Kaspi, 2005]. (Texto tomado de la fuente)Reverberation mappings have been the basis for fnding relationships between the size of the broad line region (BLR) and its luminosities in the bands of the optical continuum, ultraviolet, X-rays and Balmer emission lines. This thesis describes and applied the reverberation mapping technique in order to know the methodology to fnd the size of the broad line region, methodology that does use of the correlated variations between the continuum and the emission lines [Kaspi, 2000]. This thesis started from the information on the size of the broad line region of the group of galaxies from the work of [Kaspi, 2005] and made use of the NED database to fnd luminosity data of these galaxies in the hard X-ray band, in order to estimate a relationship between the size of the broad line region and the luminosities in the band of X-rays in the range of 10 keV - 195 KeV, applying one of the regression methods linear reported in [Kaspi, 2005] (Text taken fron the source)MaestríaMagíster en Ciencias - AstronomíaNúcleos Activos de Galaxiasxiv, 73 páginasapplication/pdfspaUniversidad Nacional de ColombiaBogotá - Ciencias - Maestría en Ciencias - AstronomíaObservatorio Astronómico NacionalFacultad de CienciasBogotá, ColombiaBogotá, ColombiaUniversidad Nacional de Colombia - Sede Bogotá520 - Astronomía y ciencias afinesGalaxiasGalaxias:activasGalaxias: nucleoCuasares:líneas de emisiónGalaxias:SeyfertGalaxias: rayos XGalaxies:activeGalaxies: nucleiQuasars:emission linesGalaxies:SeyfertGalaxies: X raysEstimación del tamaño de la BLR usando la emisión de rayos X de alta energíaBLR size estimation using high-energy X-ray emissionTrabajo de grado - Maestríainfo:eu-repo/semantics/masterThesisinfo:eu-repo/semantics/acceptedVersionTexthttp://purl.org/redcol/resource_type/TM[Abdo, 2010] Abdo, A. (2010). The frst catalogue of active galactic nuclei detected by the fermi large area telescope. Astrophysical Journal, 715:429–457[Akritas and Bershady, 1996] Akritas and Bershady (1996). Linear regression for astronomical data with measurement errors and intrinsic scatter. Astrophysical Journal, 470:706–714[Beckmann and Schrader, 2012] Beckmann and Schrader (2012). Active Galactic Nuclei. Wiley-VCH, Weinheim[Bennert and Wilson, 2004] Bennert, N., F. H. S. Y. and Wilson, A. (2004). Comparing agn broad and narrow line regions, in the interplay among black holes, stars and ism in galactic nuclei. IAU Symposium, 222:307–309[Bentz Misty C. Williams Peter R. and Tommaso, 2021] Bentz Misty C. Williams Peter R., Street Rachel, O. C. A. V. M. and Tommaso, T. (2021). A detailed view of the broad-line region in ngc 3783 from velocity resolved reverberation mapping. Astrophysical Journal, 920:112–123[Boggs Paul and Robert, 1987] Boggs Paul, B. R. and Robert, S. (1987). A stable and efcient algorithm for nonlinear orthogonal distance regression. Society for Industrial and Applied Mathematics, 8:1052–1078[Bradley, 1998] Bradley, P. (1998). On uncertainties in cross-correlation lags and the reality of wavelength-dependent continuum lags in active galactic nuclei. Astronomical Society of the Pacifc, 110:660–670.[Cruz de Oliveira and Fernandes de Aguiar, 2013] Cruz de Oliveira, E. and Fernandes de Aguiar, P. (2013). Least squares regression with errors in both variables: Case studies. Quim Nova, 36:885–889[Czerny Bozena and Vladimir, 2017] Czerny Bozena, Li Yang-Rong, S. K. H. P. S. W. C. and Vladimir, K. (2017). Self consistent model of the broad line region. Frontiers in Astronomy and Space Sciences, 4:1–5[Edelson and Krolik, 1988] Edelson and Krolik (1988). The discrete correlation function: a new method for analyzing unevenly sampled variability data. Astrophysical Journal, 333:646–656[Gaskell and Peterson, 1987] Gaskell and Peterson (1987). The accuracy of cross-correlation estimates of quasar emission-line region sizes. Astrophysical Journal, 65:1–11[Gaskell and Sparke, 1986] Gaskell, C. M. and Sparke, L. (1986). Line variations in quasars and seyfert galaxies. Astrophysical Journal, 305:175–186[Hagai, 2020] Hagai, N. (2020). Testing broad line region models with reverberation mapping. Montly Notices of Royal Astronomical Society, 494:1611–1621[Kaspi, 2000] Kaspi, S. (2000). Reverberation measurements for 17 quasars and the sizemass-luminosity relations in active galactic nuclei. Astrophysical Journal, 533:631–649[Kaspi, 2005] Kaspi, S. (2005). The relationship between luminosity and broad-line region size in active galactic nuclei. Astrophysical Journal, 629:61–71[Maoz and Netzer, 1989] Maoz, D. and Netzer, H. (1989). Evaluation of the cross-correlation method and the size of agn emission-line regions. Montly Notices of Royal Astronomical Society, 236:21–29[Massaro, 2011] Massaro, F. (2011). Large-scale extragalactic jets in the chandra era. i. data reduction and analysis. Astrophysical Journal, 197:1–14.[Morgan C.W. and Falco, 2010] Morgan C.W., Kochanek, C.-M. N. and Falco, E. (2010). The quasar accretion disk size- blackhole relation. Astrophysical Journal, 712:1129–1136[Netzer, 2006] Netzer, H. (2006). Active galactic nuclei: Basic physics and main components. Lec. Notes. Phys., 693:1–37[Netzer, 2013] Netzer, H. (2013). The Physics and Evolution of Active Galactic Nuclei. Cambridge University Press, New York[P´erez E. and L., 1988] P´erez E., R. A. and L., D. L. F. (1988). The response of the broad emission line region to ionizating continuum variations-iii an atlas of transfer functions. Astrophysical Journal, 333:646–656[Peterson, 2006] Peterson, B. (2006). The broad line region in active galactic nuclei. Lec. Notes. Phys., 693:77–100[Peterson, 1997] Peterson, B. M. (1997). An Introduction to Active Galactic Nuclei. Cambridge University Press, Cambridge[Peterson, 2004] Peterson, B. M. (2004). Central masses and broad-line region sizes of active galactic nuclei. ii. a homogeneous analysis of a large reverberation-mapping database. Astrophysical Journal, 613:682–699[Press, 1992] Press, W. (1992). Numerical recipes in C: The art of scientifc computing. Cambridge University Press, Cambridge[Raimundo S.I and A.J., 2019] Raimundo S.I, Pancoast A., V. M. G. M. and A.J., B. (2019). Modelling the agn broad line region using single-epoch spectra-i the case test of arp 151. Montly Notices of Royal Astronomical Society, 489:1899–1918.[Robert, 1993] Robert, A. (1993). Unifed models for active galactic nuclei and quasars. Annual Review Astronomical Astrophysics, 31:473–521[Shemmer, 2003] Shemmer, O. (2003). Complex optical-x-ray correlations in the narrow-line seyfert 1 galaxy ngc 4051. Royal Astronomical Society, 343:1341–1347.[Soldi, 2014] Soldi, S. (2014). Long-term variability of agn at hard x-rays. Astronomy Astrophysical, 563:1–17[Soldi., 2014] Soldi., S. (2014). Long-term variability of agn at hard x-rays. Astronomy Astrophysical, A57:1–16.Tremaine, 2002] Tremaine, S. (2002). The slope of the black hole mass versus velocity dispersion correlation. Astrophysical Journal, 574:740–753[Urry. and Padovani, 1995] Urry., C. and Padovani, P. (1995). Unifed schemes for radio-loud active galactic nuclei. Astronomical Society of the Pacifc, 107:803–846[Welsh., 1999] Welsh., W. (1999). On the reliability of cross-correlation function lag determinations in active galactic nuclei. Astronomical Society of the Pacifc, 111:1347–1366[White and Peterson, 1994] White and Peterson (1994). Comments on cross-correlation methodology in variability studies of active galactic nuclei. Astronomical Society of the Pacifc, 106:879–889[Zhang, 2019] Zhang, Z.-X. (2019). Kinematics of the broad-line region of 3c 273 from a 10 yr reverberation mapping campaign. Astrophysical Journal, 876:1–14EstudiantesGrupos comunitariosInvestigadoresMaestrosORIGINAL52048547.2022.pdf52048547.2022.pdfTesis de Maestría en Astronomíaapplication/pdf2434982https://repositorio.unal.edu.co/bitstream/unal/81862/3/52048547.2022.pdfecfd8156036cf4f32c3041e26f8b9296MD53LICENSElicense.txtlicense.txttext/plain; charset=utf-84074https://repositorio.unal.edu.co/bitstream/unal/81862/4/license.txt8153f7789df02f0a4c9e079953658ab2MD54THUMBNAIL52048547.2022.pdf.jpg52048547.2022.pdf.jpgGenerated Thumbnailimage/jpeg4373https://repositorio.unal.edu.co/bitstream/unal/81862/5/52048547.2022.pdf.jpg0e5a263b16bc915ae784f22bb402d053MD55unal/81862oai:repositorio.unal.edu.co:unal/818622024-08-08 23:11:34.636Repositorio Institucional Universidad Nacional de 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EVESURBIFBPUiBMQSBTRUNSRVRBUsONQSBHRU5FUkFMLiAqTEEgVEVTSVMgQSBQVUJMSUNBUiBERUJFIFNFUiBMQSBWRVJTScOTTiBGSU5BTCBBUFJPQkFEQS4gCgpBbCBoYWNlciBjbGljIGVuIGVsIHNpZ3VpZW50ZSBib3TDs24sIHVzdGVkIGluZGljYSBxdWUgZXN0w6EgZGUgYWN1ZXJkbyBjb24gZXN0b3MgdMOpcm1pbm9zLiBTaSB0aWVuZSBhbGd1bmEgZHVkYSBzb2JyZSBsYSBsaWNlbmNpYSwgcG9yIGZhdm9yLCBjb250YWN0ZSBjb24gZWwgYWRtaW5pc3RyYWRvciBkZWwgc2lzdGVtYS4KClVOSVZFUlNJREFEIE5BQ0lPTkFMIERFIENPTE9NQklBIC0gw5psdGltYSBtb2RpZmljYWNpw7NuIDE5LzEwLzIwMjEK

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