Research output: Contribution to journal › Article › peer-review
Testing particle acceleration in blazar jets with continuous high-cadence optical polarization observations. / Liodakis, Ioannis; Kiehlmann, Sebastian; Marscher, Alan P.; Zhang, Haocheng; Blinov, Dmitry; Jorstad, Svetlana G.; Agudo, Iván; Benítez, Erika; Berdyugin, Andrei; Bonnoli, Giacomo; Casadio, Carolina; Chen, Chien-Ting; Chen, Wen-Ping; Ehlert, Steven R.; Escudero, Juan; Grishina, Tatiana S.; Hiriart, David; Hsu, Angela; Imazawa, Ryo; Jermak, Helen E.; Jose, Jincen; Kaaret, Philip; Kopatskaya, Evgenia N.; Lalchand, Bhavana; Larionova, Elena G.; Lindfors, Elina; López, José M.; McCall, Callum; Morozova, Daria A.; Palaiologou, Efthymios; Pandey, Shivangi; Poutanen, Juri; Rakshit, Suvendu; Reig, Pablo; Sasada, Mahito; Savchenko, Sergey S.; Shablovinskaya, Elena; Neha, Sharma; Shrestha, Manisha; Steele, Iain A.; Troitskiy, Ivan S.; Troitskaya, Yulia V.; Uemura, Makoto; Vasilyev, Andrey A.; Weaver, Zachary R.; Wiersema, Klaas; Weisskopf, Martin C.
In: ASTRONOMY & ASTROPHYSICS, Vol. 689, A200, 13.09.2024.Research output: Contribution to journal › Article › peer-review
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TY - JOUR
T1 - Testing particle acceleration in blazar jets with continuous high-cadence optical polarization observations
AU - Liodakis, Ioannis
AU - Kiehlmann, Sebastian
AU - Marscher, Alan P.
AU - Zhang, Haocheng
AU - Blinov, Dmitry
AU - Jorstad, Svetlana G.
AU - Agudo, Iván
AU - Benítez, Erika
AU - Berdyugin, Andrei
AU - Bonnoli, Giacomo
AU - Casadio, Carolina
AU - Chen, Chien-Ting
AU - Chen, Wen-Ping
AU - Ehlert, Steven R.
AU - Escudero, Juan
AU - Grishina, Tatiana S.
AU - Hiriart, David
AU - Hsu, Angela
AU - Imazawa, Ryo
AU - Jermak, Helen E.
AU - Jose, Jincen
AU - Kaaret, Philip
AU - Kopatskaya, Evgenia N.
AU - Lalchand, Bhavana
AU - Larionova, Elena G.
AU - Lindfors, Elina
AU - López, José M.
AU - McCall, Callum
AU - Morozova, Daria A.
AU - Palaiologou, Efthymios
AU - Pandey, Shivangi
AU - Poutanen, Juri
AU - Rakshit, Suvendu
AU - Reig, Pablo
AU - Sasada, Mahito
AU - Savchenko, Sergey S.
AU - Shablovinskaya, Elena
AU - Neha, Sharma
AU - Shrestha, Manisha
AU - Steele, Iain A.
AU - Troitskiy, Ivan S.
AU - Troitskaya, Yulia V.
AU - Uemura, Makoto
AU - Vasilyev, Andrey A.
AU - Weaver, Zachary R.
AU - Wiersema, Klaas
AU - Weisskopf, Martin C.
PY - 2024/9/13
Y1 - 2024/9/13
N2 - Variability can be the pathway to understanding the physical processes in astrophysical jets. However, the high-cadence observations required to test particle acceleration models are still missing. Here we report on the first attempt to produce continuous, $>24$ hour polarization light curves of blazars using telescopes distributed across the globe, following the rotation of the Earth, to avoid the rising Sun. Our campaign involved 16 telescopes in Asia, Europe, and North America. We observed BL Lacertae and CGRaBS J0211+1051 for a combined 685 telescope hours. We find large variations in the polarization degree and angle for both sources on sub-hour timescales as well as a $ rotation of the polarization angle in CGRaBS J0211+1051 in less than two days. We compared our high-cadence observations to particle-in-cell magnetic reconnection and turbulent plasma simulations. We find that although the state-of-the-art simulation frameworks can produce a large fraction of the polarization properties, they do not account for the entirety of the observed polarization behavior in blazar jets.
AB - Variability can be the pathway to understanding the physical processes in astrophysical jets. However, the high-cadence observations required to test particle acceleration models are still missing. Here we report on the first attempt to produce continuous, $>24$ hour polarization light curves of blazars using telescopes distributed across the globe, following the rotation of the Earth, to avoid the rising Sun. Our campaign involved 16 telescopes in Asia, Europe, and North America. We observed BL Lacertae and CGRaBS J0211+1051 for a combined 685 telescope hours. We find large variations in the polarization degree and angle for both sources on sub-hour timescales as well as a $ rotation of the polarization angle in CGRaBS J0211+1051 in less than two days. We compared our high-cadence observations to particle-in-cell magnetic reconnection and turbulent plasma simulations. We find that although the state-of-the-art simulation frameworks can produce a large fraction of the polarization properties, they do not account for the entirety of the observed polarization behavior in blazar jets.
UR - https://www.mendeley.com/catalogue/8f7ab0cb-66e4-3a3c-8ef0-fcb3fec51e29/
U2 - 10.1051/0004-6361/202451037
DO - 10.1051/0004-6361/202451037
M3 - Article
VL - 689
JO - ASTRONOMY & ASTROPHYSICS
JF - ASTRONOMY & ASTROPHYSICS
SN - 0004-6361
M1 - A200
ER -
ID: 124577020