_version_ 1866908908086362112
author Tavecchio, Fabrizio
Kim, Dawoon E.
Emery, Gabriel
Liodakis, Ioannis
Agudo, Iván
Coppi, Paolo
Tagliaferri, Giampiero
Di Gesu, Laura
Sbarrato, Tullia
Ballo, Lucia
Sciaccaluga, Alberto
Ehlert, Steven R.
Bonnoli, Giacomo
Aceituno, Francisco José
Casadio, Carolina
Casanova, Víctor
Donnarumma, Immacolata
Escudero, Juan
Morcuende, Daniel
Otero-Santos, Jorge
Sota, Alfredo
Piirola, Vilppu
Kouch, Pouya M.
Lindfors, Elina
Nilsson, Kari
Myserlis, Ioannis
Gurwell, Mark
Keating, Garrett
Rao, Ramprasad
Angelakis, Emmanouil
Kraus, Alexander
Imazawa, Ryo
Sasada, Mahito
Fukazawa, Yasushi
Kawabata, Koji S.
Uemura, Makoto
Mizuno, Tsunefumi
Nakaoka, Tatsuya
Tochihara, Sumie
Akai, Takahiro
Akitaya, Hiroshi
Bachev, Rumen
Strigachev, Anton
Benke, Petra
Debbrecht, Lena
Eich, Julia
Eppel, Florian
Gokus, Andrea
Hämmerich, Steven
Heßdörfer, Jonas
Kadler, Matthias
Kim, Sanghyun
Kirchner, Dana
Paraschos, Georgios Filippos
Rösch, Florian
Schulga, Wladislaw
author_facet Tavecchio, Fabrizio
Kim, Dawoon E.
Emery, Gabriel
Liodakis, Ioannis
Agudo, Iván
Coppi, Paolo
Tagliaferri, Giampiero
Di Gesu, Laura
Sbarrato, Tullia
Ballo, Lucia
Sciaccaluga, Alberto
Ehlert, Steven R.
Bonnoli, Giacomo
Aceituno, Francisco José
Casadio, Carolina
Casanova, Víctor
Donnarumma, Immacolata
Escudero, Juan
Morcuende, Daniel
Otero-Santos, Jorge
Sota, Alfredo
Piirola, Vilppu
Kouch, Pouya M.
Lindfors, Elina
Nilsson, Kari
Myserlis, Ioannis
Gurwell, Mark
Keating, Garrett
Rao, Ramprasad
Angelakis, Emmanouil
Kraus, Alexander
Imazawa, Ryo
Sasada, Mahito
Fukazawa, Yasushi
Kawabata, Koji S.
Uemura, Makoto
Mizuno, Tsunefumi
Nakaoka, Tatsuya
Tochihara, Sumie
Akai, Takahiro
Akitaya, Hiroshi
Bachev, Rumen
Strigachev, Anton
Benke, Petra
Debbrecht, Lena
Eich, Julia
Eppel, Florian
Gokus, Andrea
Hämmerich, Steven
Heßdörfer, Jonas
Kadler, Matthias
Kim, Sanghyun
Kirchner, Dana
Paraschos, Georgios Filippos
Rösch, Florian
Schulga, Wladislaw
contents Multiwavelength polarimetry is a powerful tool to probe magnetic field and flow geometries in the relativistic jets of blazars. In this respect, particularly interesting are the sources whose synchrotron emission covers a broad range of frequencies, from radio to X-rays, such as the BL Lac objects of the HSP type. Previous measurements including radio, optical and X-ray data show a clear trend, with the degree of polarization increasing with frequency. Here we report radio, optical and X-ray observations ($Swift$, $Nustar$ and $IXPE$) of 1ES 1101-232 and RGB J0710+591, two blazars belonging to the puzzling subclass of extreme BL Lacs (EHBL). For 1ES 1101-232 we found a strong frequency-dependency of the degree of polarization (with a ratio $Π_X/Π_O\simeq 5.2$). For RGB J0710+591, IXPE derived a 1$σ$ upper limit $Π_X<11.6\%$, comparable with the measured optical degree of polarization (average $Π_O\sim 12\%$). We discuss the results in the framework of current interpretations and, in particular, we report an improved version of the stratified shock model that is able to reproduce the observed data of both sources.
format Preprint
id arxiv_https___arxiv_org_abs_2512_19193
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle The IXPE and multifrequency polarimetric view of the extreme blazars 1ES 1101-232 and RGB J0710+591
Tavecchio, Fabrizio
Kim, Dawoon E.
Emery, Gabriel
Liodakis, Ioannis
Agudo, Iván
Coppi, Paolo
Tagliaferri, Giampiero
Di Gesu, Laura
Sbarrato, Tullia
Ballo, Lucia
Sciaccaluga, Alberto
Ehlert, Steven R.
Bonnoli, Giacomo
Aceituno, Francisco José
Casadio, Carolina
Casanova, Víctor
Donnarumma, Immacolata
Escudero, Juan
Morcuende, Daniel
Otero-Santos, Jorge
Sota, Alfredo
Piirola, Vilppu
Kouch, Pouya M.
Lindfors, Elina
Nilsson, Kari
Myserlis, Ioannis
Gurwell, Mark
Keating, Garrett
Rao, Ramprasad
Angelakis, Emmanouil
Kraus, Alexander
Imazawa, Ryo
Sasada, Mahito
Fukazawa, Yasushi
Kawabata, Koji S.
Uemura, Makoto
Mizuno, Tsunefumi
Nakaoka, Tatsuya
Tochihara, Sumie
Akai, Takahiro
Akitaya, Hiroshi
Bachev, Rumen
Strigachev, Anton
Benke, Petra
Debbrecht, Lena
Eich, Julia
Eppel, Florian
Gokus, Andrea
Hämmerich, Steven
Heßdörfer, Jonas
Kadler, Matthias
Kim, Sanghyun
Kirchner, Dana
Paraschos, Georgios Filippos
Rösch, Florian
Schulga, Wladislaw
High Energy Astrophysical Phenomena
Multiwavelength polarimetry is a powerful tool to probe magnetic field and flow geometries in the relativistic jets of blazars. In this respect, particularly interesting are the sources whose synchrotron emission covers a broad range of frequencies, from radio to X-rays, such as the BL Lac objects of the HSP type. Previous measurements including radio, optical and X-ray data show a clear trend, with the degree of polarization increasing with frequency. Here we report radio, optical and X-ray observations ($Swift$, $Nustar$ and $IXPE$) of 1ES 1101-232 and RGB J0710+591, two blazars belonging to the puzzling subclass of extreme BL Lacs (EHBL). For 1ES 1101-232 we found a strong frequency-dependency of the degree of polarization (with a ratio $Π_X/Π_O\simeq 5.2$). For RGB J0710+591, IXPE derived a 1$σ$ upper limit $Π_X<11.6\%$, comparable with the measured optical degree of polarization (average $Π_O\sim 12\%$). We discuss the results in the framework of current interpretations and, in particular, we report an improved version of the stratified shock model that is able to reproduce the observed data of both sources.
title The IXPE and multifrequency polarimetric view of the extreme blazars 1ES 1101-232 and RGB J0710+591
topic High Energy Astrophysical Phenomena
url https://arxiv.org/abs/2512.19193