X-ray and multiwavelength polarization of Mrk 501 from 2022 to 2023

We present multiwavelength polarization measurements of the luminous blazar Mrk~501 over a 14-month period. The 2--8 keV X-ray polarization was measured with the Imaging X-ray Polarimetry Explorer (IXPE) with six 100-ks observations spanning from 2022 March to 2023 April. Each IXPE observation was a...

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Veröffentlicht in:arXiv.org 2024-07
Hauptverfasser: Chen, Chien-Ting J, Liodakis, Ioannis, Kim, Dawoon E, Laura Di Gesu, Alessandro Di Marco, Negro, Michela, Marscher, Alan P, Wu, Kinwah, Agudo, Iván, Poutanen, Juri, Mizuno, Tsunefumi, Kouch, Pouya M, Lindfors, Elina, Grishina, Tatiana S, Kopatskaya, Evgenia N, Larionova, Elena G, Troitsky, Ivan S, Vasilyev, Andrey A, Zhovtan, Alexey V, Aceituno, Francisco José, Bonnoli, Giacomo, Casanova, Víctor, Escudero, Juan, Agís-González, Beatriz, Husillos, César, Jorge Otero Santos, Myserlis, Ioannis, Gurwell, Mark, Keating, Garrett, Kang, Sincheol, Sang-Sung, Lee, Sang-Hyun, Kim, Cheong, Whee Yeon, Hyeon-Woo, Jeong, Song, Chanwoo, Kagitani, Masato, Kravtsov, Vadim, Nitindala, Anagha P, Sakanoi, Takeshi, Imazawa, Ryo, Kawabata, Koji S, Uemura, Makoto, Akitaya, Hiroshi, Casadio, Carolina, Sievers, Albrecht, Antonelli, Lucio Angelo, Bachetti, Matteo, Baumgartner, Wayne H, Bianchi, Stefano, Bongiorno, Stephen D, Bonino, Raffaella, Capitanio, Fiamma, Costa, Enrico, Ettore Del Monte, Doroshenko, Victor, Dovčiak, Michal, Enoto, Teruaki, Evangelista, Yuri, Fabiani, Sergio, Ferrazzoli, Riccardo, Garcia, Javier A, Gunji, Shuichi, Hayashida, Kiyoshi, Heyl, Jeremy, Iwakiri, Wataru, Kislat, Fabian, Kolodziejczak, Jeffery J, Krawczynski, Henric, Latronico, Luca, Manfreda, Alberto, Marinucci, Andrea, Marshall, Herman L, Mitsuishi, Ikuyuki, C -Y Ng, O'Dell, Stephen L, Omodei, Nicola, Oppedisano, Chiara, Papitto, Alessandro, Abel Lawrence Peirson, Perri, Matteo, Pesce-Rollins, Melissa, Pilia, Maura, Possenti, Andrea, Puccetti, Simonetta, Ramsey, Brian D, Ratheesh, Ajay, Roberts, Oliver J, Romani, Roger W, Slane, Patrick, Swartz, Douglas A, Tamagawa, Toru, Tavecchio, Fabrizio, Taverna, Roberto, Tawara, Yuzuru, Tennant, Allyn F, Tsygankov, Sergey S, Turolla, Roberto, Vink, Jacco, Weisskopf, Martin C, Xie, Fei
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creator Chen, Chien-Ting J
Liodakis, Ioannis
Kim, Dawoon E
Laura Di Gesu
Alessandro Di Marco
Negro, Michela
Marscher, Alan P
Wu, Kinwah
Agudo, Iván
Poutanen, Juri
Mizuno, Tsunefumi
Kouch, Pouya M
Lindfors, Elina
Grishina, Tatiana S
Kopatskaya, Evgenia N
Larionova, Elena G
Troitsky, Ivan S
Vasilyev, Andrey A
Zhovtan, Alexey V
Aceituno, Francisco José
Bonnoli, Giacomo
Casanova, Víctor
Escudero, Juan
Agís-González, Beatriz
Husillos, César
Jorge Otero Santos
Myserlis, Ioannis
Gurwell, Mark
Keating, Garrett
Kang, Sincheol
Sang-Sung, Lee
Sang-Hyun, Kim
Cheong, Whee Yeon
Hyeon-Woo, Jeong
Song, Chanwoo
Kagitani, Masato
Kravtsov, Vadim
Nitindala, Anagha P
Sakanoi, Takeshi
Imazawa, Ryo
Kawabata, Koji S
Uemura, Makoto
Akitaya, Hiroshi
Casadio, Carolina
Sievers, Albrecht
Antonelli, Lucio Angelo
Bachetti, Matteo
Baumgartner, Wayne H
Bianchi, Stefano
Bongiorno, Stephen D
Bonino, Raffaella
Capitanio, Fiamma
Costa, Enrico
Ettore Del Monte
Doroshenko, Victor
Dovčiak, Michal
Enoto, Teruaki
Evangelista, Yuri
Fabiani, Sergio
Ferrazzoli, Riccardo
Garcia, Javier A
Gunji, Shuichi
Hayashida, Kiyoshi
Heyl, Jeremy
Iwakiri, Wataru
Kislat, Fabian
Kolodziejczak, Jeffery J
Krawczynski, Henric
Latronico, Luca
Manfreda, Alberto
Marinucci, Andrea
Marshall, Herman L
Mitsuishi, Ikuyuki
C -Y Ng
O'Dell, Stephen L
Omodei, Nicola
Oppedisano, Chiara
Papitto, Alessandro
Abel Lawrence Peirson
Perri, Matteo
Pesce-Rollins, Melissa
Pilia, Maura
Possenti, Andrea
Puccetti, Simonetta
Ramsey, Brian D
Ratheesh, Ajay
Roberts, Oliver J
Romani, Roger W
Slane, Patrick
Swartz, Douglas A
Tamagawa, Toru
Tavecchio, Fabrizio
Taverna, Roberto
Tawara, Yuzuru
Tennant, Allyn F
Tsygankov, Sergey S
Turolla, Roberto
Vink, Jacco
Weisskopf, Martin C
Xie, Fei
description We present multiwavelength polarization measurements of the luminous blazar Mrk~501 over a 14-month period. The 2--8 keV X-ray polarization was measured with the Imaging X-ray Polarimetry Explorer (IXPE) with six 100-ks observations spanning from 2022 March to 2023 April. Each IXPE observation was accompanied by simultaneous X-ray data from NuSTAR, Swift/XRT, and/or XMM-Newton. Complementary optical-infrared polarization measurements were also available in the B, V, R, I, and J bands, as were radio polarization measurements from 4.85 GHz to 225.5 GHz. Among the first five IXPE observations, we did not find significant variability in the X-ray polarization degree and angle with IXPE. However, the most recent sixth observation found an elevated polarization degree at \(>3\sigma\) above the average of the other five observations. The optical and radio measurements show no apparent correlations with the X-ray polarization properties. Throughout the six IXPE observations, the X-ray polarization degree remained higher than, or similar to, the R-band optical polarization degree, which remained higher than the radio value. This is consistent with the energy-stratified shock scenario proposed to explain the first two IXPE observations, in which the polarized X-ray, optical, and radio emission arises from different regions.
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The 2--8 keV X-ray polarization was measured with the Imaging X-ray Polarimetry Explorer (IXPE) with six 100-ks observations spanning from 2022 March to 2023 April. Each IXPE observation was accompanied by simultaneous X-ray data from NuSTAR, Swift/XRT, and/or XMM-Newton. Complementary optical-infrared polarization measurements were also available in the B, V, R, I, and J bands, as were radio polarization measurements from 4.85 GHz to 225.5 GHz. Among the first five IXPE observations, we did not find significant variability in the X-ray polarization degree and angle with IXPE. However, the most recent sixth observation found an elevated polarization degree at \(&gt;3\sigma\) above the average of the other five observations. The optical and radio measurements show no apparent correlations with the X-ray polarization properties. Throughout the six IXPE observations, the X-ray polarization degree remained higher than, or similar to, the R-band optical polarization degree, which remained higher than the radio value. This is consistent with the energy-stratified shock scenario proposed to explain the first two IXPE observations, in which the polarized X-ray, optical, and radio emission arises from different regions.</description><identifier>EISSN: 2331-8422</identifier><language>eng</language><publisher>Ithaca: Cornell University Library, arXiv.org</publisher><subject>Optical polarization ; Optical properties ; Radio emission ; X ray imagery ; XMM (spacecraft)</subject><ispartof>arXiv.org, 2024-07</ispartof><rights>2024. This work is published under http://creativecommons.org/licenses/by-sa/4.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.</rights><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>776,780</link.rule.ids></links><search><creatorcontrib>Chen, Chien-Ting J</creatorcontrib><creatorcontrib>Liodakis, Ioannis</creatorcontrib><creatorcontrib>Kim, Dawoon E</creatorcontrib><creatorcontrib>Laura Di Gesu</creatorcontrib><creatorcontrib>Alessandro Di Marco</creatorcontrib><creatorcontrib>Negro, Michela</creatorcontrib><creatorcontrib>Marscher, Alan P</creatorcontrib><creatorcontrib>Wu, Kinwah</creatorcontrib><creatorcontrib>Agudo, Iván</creatorcontrib><creatorcontrib>Poutanen, Juri</creatorcontrib><creatorcontrib>Mizuno, Tsunefumi</creatorcontrib><creatorcontrib>Kouch, Pouya 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Fiamma</creatorcontrib><creatorcontrib>Costa, Enrico</creatorcontrib><creatorcontrib>Ettore Del Monte</creatorcontrib><creatorcontrib>Doroshenko, Victor</creatorcontrib><creatorcontrib>Dovčiak, Michal</creatorcontrib><creatorcontrib>Enoto, Teruaki</creatorcontrib><creatorcontrib>Evangelista, Yuri</creatorcontrib><creatorcontrib>Fabiani, Sergio</creatorcontrib><creatorcontrib>Ferrazzoli, Riccardo</creatorcontrib><creatorcontrib>Garcia, Javier A</creatorcontrib><creatorcontrib>Gunji, Shuichi</creatorcontrib><creatorcontrib>Hayashida, Kiyoshi</creatorcontrib><creatorcontrib>Heyl, Jeremy</creatorcontrib><creatorcontrib>Iwakiri, Wataru</creatorcontrib><creatorcontrib>Kislat, Fabian</creatorcontrib><creatorcontrib>Kolodziejczak, Jeffery J</creatorcontrib><creatorcontrib>Krawczynski, Henric</creatorcontrib><creatorcontrib>Latronico, Luca</creatorcontrib><creatorcontrib>Manfreda, Alberto</creatorcontrib><creatorcontrib>Marinucci, Andrea</creatorcontrib><creatorcontrib>Marshall, Herman L</creatorcontrib><creatorcontrib>Mitsuishi, Ikuyuki</creatorcontrib><creatorcontrib>C -Y Ng</creatorcontrib><creatorcontrib>O'Dell, Stephen L</creatorcontrib><creatorcontrib>Omodei, Nicola</creatorcontrib><creatorcontrib>Oppedisano, Chiara</creatorcontrib><creatorcontrib>Papitto, Alessandro</creatorcontrib><creatorcontrib>Abel Lawrence Peirson</creatorcontrib><creatorcontrib>Perri, Matteo</creatorcontrib><creatorcontrib>Pesce-Rollins, Melissa</creatorcontrib><creatorcontrib>Pilia, Maura</creatorcontrib><creatorcontrib>Possenti, Andrea</creatorcontrib><creatorcontrib>Puccetti, Simonetta</creatorcontrib><creatorcontrib>Ramsey, Brian D</creatorcontrib><creatorcontrib>Ratheesh, Ajay</creatorcontrib><creatorcontrib>Roberts, Oliver J</creatorcontrib><creatorcontrib>Romani, Roger W</creatorcontrib><creatorcontrib>Slane, Patrick</creatorcontrib><creatorcontrib>Swartz, Douglas A</creatorcontrib><creatorcontrib>Tamagawa, Toru</creatorcontrib><creatorcontrib>Tavecchio, Fabrizio</creatorcontrib><creatorcontrib>Taverna, Roberto</creatorcontrib><creatorcontrib>Tawara, Yuzuru</creatorcontrib><creatorcontrib>Tennant, Allyn F</creatorcontrib><creatorcontrib>Tsygankov, Sergey S</creatorcontrib><creatorcontrib>Turolla, Roberto</creatorcontrib><creatorcontrib>Vink, Jacco</creatorcontrib><creatorcontrib>Weisskopf, Martin C</creatorcontrib><creatorcontrib>Xie, Fei</creatorcontrib><title>X-ray and multiwavelength polarization of Mrk 501 from 2022 to 2023</title><title>arXiv.org</title><description>We present multiwavelength polarization measurements of the luminous blazar Mrk~501 over a 14-month period. The 2--8 keV X-ray polarization was measured with the Imaging X-ray Polarimetry Explorer (IXPE) with six 100-ks observations spanning from 2022 March to 2023 April. Each IXPE observation was accompanied by simultaneous X-ray data from NuSTAR, Swift/XRT, and/or XMM-Newton. Complementary optical-infrared polarization measurements were also available in the B, V, R, I, and J bands, as were radio polarization measurements from 4.85 GHz to 225.5 GHz. Among the first five IXPE observations, we did not find significant variability in the X-ray polarization degree and angle with IXPE. However, the most recent sixth observation found an elevated polarization degree at \(&gt;3\sigma\) above the average of the other five observations. The optical and radio measurements show no apparent correlations with the X-ray polarization properties. Throughout the six IXPE observations, the X-ray polarization degree remained higher than, or similar to, the R-band optical polarization degree, which remained higher than the radio value. This is consistent with the energy-stratified shock scenario proposed to explain the first two IXPE observations, in which the polarized X-ray, optical, and radio emission arises from different regions.</description><subject>Optical polarization</subject><subject>Optical properties</subject><subject>Radio emission</subject><subject>X ray imagery</subject><subject>XMM (spacecraft)</subject><issn>2331-8422</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2024</creationdate><recordtype>article</recordtype><sourceid>BENPR</sourceid><recordid>eNqNyrEKwjAUQNEgCBbtPzxwLiTvmdrORXFxc3ArAVNtTZOapIp-vQp-gNMZ7p2wBIlEVqwQZywNoeOcY75GKSlh1THz6gnKnqAfTWwf6q6Ntud4gcEZ5duXiq2z4BrY-ytILqDxrgfkiBDdV1qwaaNM0OnPOVtuN4dqlw3e3UYdYt250dtPqokXoiwFyZz-u974bjeb</recordid><startdate>20240715</startdate><enddate>20240715</enddate><creator>Chen, Chien-Ting J</creator><creator>Liodakis, Ioannis</creator><creator>Kim, Dawoon E</creator><creator>Laura Di Gesu</creator><creator>Alessandro Di Marco</creator><creator>Negro, Michela</creator><creator>Marscher, Alan P</creator><creator>Wu, Kinwah</creator><creator>Agudo, Iván</creator><creator>Poutanen, Juri</creator><creator>Mizuno, Tsunefumi</creator><creator>Kouch, Pouya M</creator><creator>Lindfors, Elina</creator><creator>Grishina, Tatiana S</creator><creator>Kopatskaya, Evgenia N</creator><creator>Larionova, Elena G</creator><creator>Troitsky, Ivan S</creator><creator>Vasilyev, Andrey A</creator><creator>Zhovtan, Alexey V</creator><creator>Aceituno, Francisco José</creator><creator>Bonnoli, Giacomo</creator><creator>Casanova, Víctor</creator><creator>Escudero, Juan</creator><creator>Agís-González, Beatriz</creator><creator>Husillos, César</creator><creator>Jorge Otero Santos</creator><creator>Myserlis, Ioannis</creator><creator>Gurwell, Mark</creator><creator>Keating, Garrett</creator><creator>Kang, Sincheol</creator><creator>Sang-Sung, Lee</creator><creator>Sang-Hyun, Kim</creator><creator>Cheong, Whee 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Ioannis ; Kim, Dawoon E ; Laura Di Gesu ; Alessandro Di Marco ; Negro, Michela ; Marscher, Alan P ; Wu, Kinwah ; Agudo, Iván ; Poutanen, Juri ; Mizuno, Tsunefumi ; Kouch, Pouya M ; Lindfors, Elina ; Grishina, Tatiana S ; Kopatskaya, Evgenia N ; Larionova, Elena G ; Troitsky, Ivan S ; Vasilyev, Andrey A ; Zhovtan, Alexey V ; Aceituno, Francisco José ; Bonnoli, Giacomo ; Casanova, Víctor ; Escudero, Juan ; Agís-González, Beatriz ; Husillos, César ; Jorge Otero Santos ; Myserlis, Ioannis ; Gurwell, Mark ; Keating, Garrett ; Kang, Sincheol ; Sang-Sung, Lee ; Sang-Hyun, Kim ; Cheong, Whee Yeon ; Hyeon-Woo, Jeong ; Song, Chanwoo ; Kagitani, Masato ; Kravtsov, Vadim ; Nitindala, Anagha P ; Sakanoi, Takeshi ; Imazawa, Ryo ; Kawabata, Koji S ; Uemura, Makoto ; Akitaya, Hiroshi ; Casadio, Carolina ; Sievers, Albrecht ; Antonelli, Lucio Angelo ; Bachetti, Matteo ; Baumgartner, Wayne H ; Bianchi, Stefano ; Bongiorno, Stephen D ; Bonino, Raffaella ; Capitanio, Fiamma ; Costa, Enrico ; Ettore Del Monte ; Doroshenko, Victor ; Dovčiak, Michal ; Enoto, Teruaki ; Evangelista, Yuri ; Fabiani, Sergio ; Ferrazzoli, Riccardo ; Garcia, Javier A ; Gunji, Shuichi ; Hayashida, Kiyoshi ; Heyl, Jeremy ; Iwakiri, Wataru ; Kislat, Fabian ; Kolodziejczak, Jeffery J ; Krawczynski, Henric ; Latronico, Luca ; Manfreda, Alberto ; Marinucci, Andrea ; Marshall, Herman L ; Mitsuishi, Ikuyuki ; C -Y Ng ; O'Dell, Stephen L ; Omodei, Nicola ; Oppedisano, Chiara ; Papitto, Alessandro ; Abel Lawrence Peirson ; Perri, Matteo ; Pesce-Rollins, Melissa ; Pilia, Maura ; Possenti, Andrea ; Puccetti, Simonetta ; Ramsey, Brian D ; Ratheesh, Ajay ; Roberts, Oliver J ; Romani, Roger W ; Slane, Patrick ; Swartz, Douglas A ; Tamagawa, Toru ; Tavecchio, Fabrizio ; Taverna, Roberto ; Tawara, Yuzuru ; Tennant, Allyn F ; Tsygankov, Sergey S ; Turolla, Roberto ; Vink, Jacco ; Weisskopf, Martin C ; Xie, Fei</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-proquest_journals_30819913563</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2024</creationdate><topic>Optical polarization</topic><topic>Optical properties</topic><topic>Radio emission</topic><topic>X ray imagery</topic><topic>XMM (spacecraft)</topic><toplevel>online_resources</toplevel><creatorcontrib>Chen, Chien-Ting J</creatorcontrib><creatorcontrib>Liodakis, Ioannis</creatorcontrib><creatorcontrib>Kim, Dawoon E</creatorcontrib><creatorcontrib>Laura Di Gesu</creatorcontrib><creatorcontrib>Alessandro Di Marco</creatorcontrib><creatorcontrib>Negro, Michela</creatorcontrib><creatorcontrib>Marscher, Alan P</creatorcontrib><creatorcontrib>Wu, Kinwah</creatorcontrib><creatorcontrib>Agudo, Iván</creatorcontrib><creatorcontrib>Poutanen, Juri</creatorcontrib><creatorcontrib>Mizuno, Tsunefumi</creatorcontrib><creatorcontrib>Kouch, Pouya 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Collection</collection><collection>ProQuest Engineering Collection</collection><collection>Engineering Database</collection><collection>Publicly Available Content Database</collection><collection>ProQuest One Academic Eastern Edition (DO NOT USE)</collection><collection>ProQuest One Academic</collection><collection>ProQuest One Academic UKI Edition</collection><collection>ProQuest Central China</collection><collection>Engineering Collection</collection></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Chen, Chien-Ting J</au><au>Liodakis, Ioannis</au><au>Kim, Dawoon E</au><au>Laura Di Gesu</au><au>Alessandro Di Marco</au><au>Negro, Michela</au><au>Marscher, Alan P</au><au>Wu, Kinwah</au><au>Agudo, Iván</au><au>Poutanen, Juri</au><au>Mizuno, Tsunefumi</au><au>Kouch, Pouya M</au><au>Lindfors, Elina</au><au>Grishina, Tatiana S</au><au>Kopatskaya, Evgenia N</au><au>Larionova, Elena G</au><au>Troitsky, Ivan S</au><au>Vasilyev, Andrey A</au><au>Zhovtan, Alexey V</au><au>Aceituno, Francisco José</au><au>Bonnoli, Giacomo</au><au>Casanova, Víctor</au><au>Escudero, Juan</au><au>Agís-González, Beatriz</au><au>Husillos, César</au><au>Jorge Otero Santos</au><au>Myserlis, Ioannis</au><au>Gurwell, Mark</au><au>Keating, Garrett</au><au>Kang, Sincheol</au><au>Sang-Sung, Lee</au><au>Sang-Hyun, Kim</au><au>Cheong, Whee Yeon</au><au>Hyeon-Woo, Jeong</au><au>Song, Chanwoo</au><au>Kagitani, Masato</au><au>Kravtsov, Vadim</au><au>Nitindala, Anagha P</au><au>Sakanoi, Takeshi</au><au>Imazawa, Ryo</au><au>Kawabata, Koji S</au><au>Uemura, Makoto</au><au>Akitaya, Hiroshi</au><au>Casadio, Carolina</au><au>Sievers, Albrecht</au><au>Antonelli, Lucio Angelo</au><au>Bachetti, Matteo</au><au>Baumgartner, Wayne H</au><au>Bianchi, Stefano</au><au>Bongiorno, Stephen D</au><au>Bonino, Raffaella</au><au>Capitanio, Fiamma</au><au>Costa, Enrico</au><au>Ettore Del Monte</au><au>Doroshenko, Victor</au><au>Dovčiak, Michal</au><au>Enoto, Teruaki</au><au>Evangelista, Yuri</au><au>Fabiani, Sergio</au><au>Ferrazzoli, Riccardo</au><au>Garcia, Javier A</au><au>Gunji, Shuichi</au><au>Hayashida, Kiyoshi</au><au>Heyl, Jeremy</au><au>Iwakiri, Wataru</au><au>Kislat, Fabian</au><au>Kolodziejczak, Jeffery J</au><au>Krawczynski, Henric</au><au>Latronico, Luca</au><au>Manfreda, Alberto</au><au>Marinucci, Andrea</au><au>Marshall, Herman L</au><au>Mitsuishi, Ikuyuki</au><au>C -Y Ng</au><au>O'Dell, Stephen L</au><au>Omodei, Nicola</au><au>Oppedisano, Chiara</au><au>Papitto, Alessandro</au><au>Abel Lawrence Peirson</au><au>Perri, Matteo</au><au>Pesce-Rollins, Melissa</au><au>Pilia, Maura</au><au>Possenti, Andrea</au><au>Puccetti, Simonetta</au><au>Ramsey, Brian D</au><au>Ratheesh, Ajay</au><au>Roberts, Oliver J</au><au>Romani, Roger W</au><au>Slane, Patrick</au><au>Swartz, Douglas A</au><au>Tamagawa, Toru</au><au>Tavecchio, Fabrizio</au><au>Taverna, Roberto</au><au>Tawara, Yuzuru</au><au>Tennant, Allyn F</au><au>Tsygankov, Sergey S</au><au>Turolla, Roberto</au><au>Vink, Jacco</au><au>Weisskopf, Martin C</au><au>Xie, Fei</au><format>book</format><genre>document</genre><ristype>GEN</ristype><atitle>X-ray and multiwavelength polarization of Mrk 501 from 2022 to 2023</atitle><jtitle>arXiv.org</jtitle><date>2024-07-15</date><risdate>2024</risdate><eissn>2331-8422</eissn><abstract>We present multiwavelength polarization measurements of the luminous blazar Mrk~501 over a 14-month period. The 2--8 keV X-ray polarization was measured with the Imaging X-ray Polarimetry Explorer (IXPE) with six 100-ks observations spanning from 2022 March to 2023 April. Each IXPE observation was accompanied by simultaneous X-ray data from NuSTAR, Swift/XRT, and/or XMM-Newton. Complementary optical-infrared polarization measurements were also available in the B, V, R, I, and J bands, as were radio polarization measurements from 4.85 GHz to 225.5 GHz. Among the first five IXPE observations, we did not find significant variability in the X-ray polarization degree and angle with IXPE. However, the most recent sixth observation found an elevated polarization degree at \(&gt;3\sigma\) above the average of the other five observations. The optical and radio measurements show no apparent correlations with the X-ray polarization properties. Throughout the six IXPE observations, the X-ray polarization degree remained higher than, or similar to, the R-band optical polarization degree, which remained higher than the radio value. This is consistent with the energy-stratified shock scenario proposed to explain the first two IXPE observations, in which the polarized X-ray, optical, and radio emission arises from different regions.</abstract><cop>Ithaca</cop><pub>Cornell University Library, arXiv.org</pub><oa>free_for_read</oa></addata></record>
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subjects Optical polarization
Optical properties
Radio emission
X ray imagery
XMM (spacecraft)
title X-ray and multiwavelength polarization of Mrk 501 from 2022 to 2023
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