📣 We're hiring! Seeking a postdoctoral researcher to work on scientific and technical problems related to the Polarization Sky Survey of the Universe’s Magnetism (POSSUM), a new wide-field polarimetry survey on the Australian Square Kilometre Array Pathfinder (ASKAP).
https://uoft.me/postdocradiopol
https://uoft.me/postdocradiopol
November 11, 2025 at 7:00 PM
📣 We're hiring! Seeking a postdoctoral researcher to work on scientific and technical problems related to the Polarization Sky Survey of the Universe’s Magnetism (POSSUM), a new wide-field polarimetry survey on the Australian Square Kilometre Array Pathfinder (ASKAP).
https://uoft.me/postdocradiopol
https://uoft.me/postdocradiopol
Pulsar timing and polarimetry: results and perspectives. Konstantin A. Postnov et. al. https://arxiv.org/abs/2502.00080
February 4, 2025 at 5:34 AM
Pulsar timing and polarimetry: results and perspectives. Konstantin A. Postnov et. al. https://arxiv.org/abs/2502.00080
Jo\~ao Lu\'is Rosa, Nicolas Aimar, Hanna Liis Tamm: Polarimetry imprints of exotic compact objects: solitonic boson stars https://arxiv.org/abs/2504.02472 https://arxiv.org/pdf/2504.02472 https://arxiv.org/html/2504.02472
April 4, 2025 at 6:10 AM
Jo\~ao Lu\'is Rosa, Nicolas Aimar, Hanna Liis Tamm: Polarimetry imprints of exotic compact objects: solitonic boson stars https://arxiv.org/abs/2504.02472 https://arxiv.org/pdf/2504.02472 https://arxiv.org/html/2504.02472
method to probe the structure of X-ray binaries. The Imaging X-ray Polarimetry Explorer observed the High-Mass X-ray Binary Cygnus X-1 and the Low-Mass X-ray Binary Swift J1727.8-1613 in different accretion states: in the hard state and in the soft [2/5 of https://arxiv.org/abs/2504.10981v1]
April 16, 2025 at 6:08 AM
method to probe the structure of X-ray binaries. The Imaging X-ray Polarimetry Explorer observed the High-Mass X-ray Binary Cygnus X-1 and the Low-Mass X-ray Binary Swift J1727.8-1613 in different accretion states: in the hard state and in the soft [2/5 of https://arxiv.org/abs/2504.10981v1]
NASA’s IXPE Obtains First X-ray Polarization Measurement of Magnetar Outburst What happens when the universe’s most magnetic object shines with the power of 1,000 Suns in a matter of seconds? Thanks to NASA’s IXPE (Imaging X-ray Polarimetry Explo...
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Interest | Match | Feed
Origin
www.nasa.gov
June 5, 2025 at 8:32 PM
A new type-1 transition in NGC 1346 revealed by (spectro)polarimetry
https://arxiv.org/pdf/2507.08589
F. Marin, D. Hutsemékers, S. Jorstad.
https://arxiv.org/pdf/2507.08589
F. Marin, D. Hutsemékers, S. Jorstad.
https://arxiv.org/abs/2507.08589
arXiv abstract link
arxiv.org
July 14, 2025 at 4:31 AM
A new type-1 transition in NGC 1346 revealed by (spectro)polarimetry
https://arxiv.org/pdf/2507.08589
F. Marin, D. Hutsemékers, S. Jorstad.
https://arxiv.org/pdf/2507.08589
F. Marin, D. Hutsemékers, S. Jorstad.
Unnati Kashyap, Thomas J. Maccarone, Eliot C. Pattie, Mason Ng, Swati Ravi, Herman L. Marshall: X-ray and radio polarimetry of the neutron star low mass X-ray binary GX 13+1 https://arxiv.org/abs/2508.05763 https://arxiv.org/pdf/2508.05763 https://arxiv.org/html/2508.05763
August 11, 2025 at 6:42 AM
Unnati Kashyap, Thomas J. Maccarone, Eliot C. Pattie, Mason Ng, Swati Ravi, Herman L. Marshall: X-ray and radio polarimetry of the neutron star low mass X-ray binary GX 13+1 https://arxiv.org/abs/2508.05763 https://arxiv.org/pdf/2508.05763 https://arxiv.org/html/2508.05763
The Chinese pulsar timing array data release I. Polarimetry for 56 millisecond pulsars. (replaced) Jiangwei Xu et. al. https://arxiv.org/abs/2502.20820
April 23, 2025 at 1:45 AM
The Chinese pulsar timing array data release I. Polarimetry for 56 millisecond pulsars. (replaced) Jiangwei Xu et. al. https://arxiv.org/abs/2502.20820
At NAM 2025 in Durham @nam25-durham.bsky.social : Thomas Baxter is speaking on "Probing the axial symmetry of gamma-ray burst jets using afterglow polarimetry". Thomas has published in #MNRAS, for example as a co-author on academic.oup.com/mnras/articl...
Prompt periodicity in the GRB 211211A precursor: black-hole or magnetar engine?
ABSTRACT. The merger origin long GRB 211211A was a class (re-)defining event. A precursor was identified with a $\sim 1$ s separation from the main burst,
academic.oup.com
July 10, 2025 at 4:35 PM
At NAM 2025 in Durham @nam25-durham.bsky.social : Thomas Baxter is speaking on "Probing the axial symmetry of gamma-ray burst jets using afterglow polarimetry". Thomas has published in #MNRAS, for example as a co-author on academic.oup.com/mnras/articl...
Gamma-Ray Burst Polarimetry with the POLAR and POLAR-2 missions
https://arxiv.org/pdf/2509.06601
Nicolas De Angelis et al.
https://arxiv.org/pdf/2509.06601
Nicolas De Angelis et al.
https://arxiv.org/abs/2509.06601
arXiv abstract link
arxiv.org
September 9, 2025 at 4:33 AM
Gamma-Ray Burst Polarimetry with the POLAR and POLAR-2 missions
https://arxiv.org/pdf/2509.06601
Nicolas De Angelis et al.
https://arxiv.org/pdf/2509.06601
Nicolas De Angelis et al.
Photon-starved polarimetry via functional classical shadows
https://arxiv.org/pdf/2509.19547
Matteo Rosati, Miranda Parisi, Linda Sansoni, Eleonora Stefanutti, Andrea Chiuri, Marco Barbieri.
https://arxiv.org/pdf/2509.19547
Matteo Rosati, Miranda Parisi, Linda Sansoni, Eleonora Stefanutti, Andrea Chiuri, Marco Barbieri.
https://arxiv.org/abs/2509.19547
arXiv abstract link
arxiv.org
September 25, 2025 at 6:59 AM
Photon-starved polarimetry via functional classical shadows
https://arxiv.org/pdf/2509.19547
Matteo Rosati, Miranda Parisi, Linda Sansoni, Eleonora Stefanutti, Andrea Chiuri, Marco Barbieri.
https://arxiv.org/pdf/2509.19547
Matteo Rosati, Miranda Parisi, Linda Sansoni, Eleonora Stefanutti, Andrea Chiuri, Marco Barbieri.
The Mineralogical Connection Between M- and K-type Asteroids as Indicated by Polarimetry
https://arxiv.org/pdf/2506.14210
Joseph R. Masiero, Yuna G. Kwon, Elena Selmi, Manaswi Kondapally.
https://arxiv.org/pdf/2506.14210
Joseph R. Masiero, Yuna G. Kwon, Elena Selmi, Manaswi Kondapally.
https://arxiv.org/abs/2506.14210
arXiv abstract link
arxiv.org
June 18, 2025 at 4:33 AM
The Mineralogical Connection Between M- and K-type Asteroids as Indicated by Polarimetry
https://arxiv.org/pdf/2506.14210
Joseph R. Masiero, Yuna G. Kwon, Elena Selmi, Manaswi Kondapally.
https://arxiv.org/pdf/2506.14210
Joseph R. Masiero, Yuna G. Kwon, Elena Selmi, Manaswi Kondapally.
ALMA polarimetry of radio-quiet AGNs. E. Shablovinskaia et. al. https://arxiv.org/abs/2506.05973
June 9, 2025 at 5:08 AM
ALMA polarimetry of radio-quiet AGNs. E. Shablovinskaia et. al. https://arxiv.org/abs/2506.05973
Lisa W. Li, Phillip H. H. Oakley, Rebecca N. Schindhelm, Sean G. Sellers, Roberto Casini, Noah A. Rubin: Metasurface-Enabled Astronomical Polarimetry https://arxiv.org/abs/2506.06245 https://arxiv.org/pdf/2506.06245 https://arxiv.org/html/2506.06245
June 9, 2025 at 6:15 AM
Lisa W. Li, Phillip H. H. Oakley, Rebecca N. Schindhelm, Sean G. Sellers, Roberto Casini, Noah A. Rubin: Metasurface-Enabled Astronomical Polarimetry https://arxiv.org/abs/2506.06245 https://arxiv.org/pdf/2506.06245 https://arxiv.org/html/2506.06245
Osservata per la prima volta – con l’Imaging X-ray Polarimetry Explorer #Ixpe – la #polarizzazione di una #magnetar dopo una fase di attivazione. A guidare lo studio, pubblicato oggi su #ApJL, Michela Rigoselli dell’Inaf di Milano.
Ixpe svela i segreti di una magnetar attiva
Il satellite Nasa-Asi Ixpe ha osservato per la prima volta la magnetar 1E 1841-045 durante una fase di attivazione, rilevando l’emissione di raggi X polarizzati. Questa scoperta fornisce nuovi indizi ...
www.media.inaf.it
May 28, 2025 at 11:21 AM
Osservata per la prima volta – con l’Imaging X-ray Polarimetry Explorer #Ixpe – la #polarizzazione di una #magnetar dopo una fase di attivazione. A guidare lo studio, pubblicato oggi su #ApJL, Michela Rigoselli dell’Inaf di Milano.
of Cyg X-1 was measured 13 times with the Imaging X-ray Polarimetry Explorer (IXPE), covering both hard and soft spectral states. The X-ray polarization degree (PD) in the hard state was found to be $\approx4.0\%$, roughly twice as high as in the soft [2/6 of https://arxiv.org/abs/2505.03942v1]
May 8, 2025 at 6:07 AM
of Cyg X-1 was measured 13 times with the Imaging X-ray Polarimetry Explorer (IXPE), covering both hard and soft spectral states. The X-ray polarization degree (PD) in the hard state was found to be $\approx4.0\%$, roughly twice as high as in the soft [2/6 of https://arxiv.org/abs/2505.03942v1]
Varpu Ahlberg, Anastasiia Bocharova, Alexandra Veledina: The constraining power of X-ray polarimetry: detailed structure of the intrabinary bow shock in Cygnus X-3 https://arxiv.org/abs/2507.21708 https://arxiv.org/pdf/2507.21708 https://arxiv.org/html/2507.21708
July 30, 2025 at 6:42 AM
Varpu Ahlberg, Anastasiia Bocharova, Alexandra Veledina: The constraining power of X-ray polarimetry: detailed structure of the intrabinary bow shock in Cygnus X-3 https://arxiv.org/abs/2507.21708 https://arxiv.org/pdf/2507.21708 https://arxiv.org/html/2507.21708
X-ray and radio polarimetry of the neutron star low-mass X-ray binary 4U 1728-34. Unnati Kashyap (TTU et. al. https://arxiv.org/abs/2504.14021
June 5, 2025 at 6:07 AM
X-ray and radio polarimetry of the neutron star low-mass X-ray binary 4U 1728-34. Unnati Kashyap (TTU et. al. https://arxiv.org/abs/2504.14021
Nishant Mehrotra, Sandesh Rao Mattu, Robert Calderbank: Instantaneous Polarimetry with Zak-OTFS https://arxiv.org/abs/2508.19185 https://arxiv.org/pdf/2508.19185 https://arxiv.org/html/2508.19185
August 27, 2025 at 6:36 AM
Nishant Mehrotra, Sandesh Rao Mattu, Robert Calderbank: Instantaneous Polarimetry with Zak-OTFS https://arxiv.org/abs/2508.19185 https://arxiv.org/pdf/2508.19185 https://arxiv.org/html/2508.19185
Ieva: Enter the TRANSNEO project, the main goal of which is to obtain photoemtry, spectroscopy, and polarimetry in trans-NEOs.
#EPSCDPS2025 #EPSCDPS
#EPSCDPS2025 #EPSCDPS
September 9, 2025 at 12:11 PM
Ieva: Enter the TRANSNEO project, the main goal of which is to obtain photoemtry, spectroscopy, and polarimetry in trans-NEOs.
#EPSCDPS2025 #EPSCDPS
#EPSCDPS2025 #EPSCDPS
LAUNCH at 0340 UTC Jan 1 of PSLV-C58 from Satish Dhawan Space Centre carrying the XPoSAT X-ray astronomy satellite, which will attempt X-ray polarimetry in a higher energy band than IXPE
January 1, 2024 at 3:42 AM
LAUNCH at 0340 UTC Jan 1 of PSLV-C58 from Satish Dhawan Space Centre carrying the XPoSAT X-ray astronomy satellite, which will attempt X-ray polarimetry in a higher energy band than IXPE
NASA’s IXPE Imager Reveals Mysteries of Rare Pulsar
An international team of astronomers has uncovered new evidence to explain how pulsing remnants of exploded stars interact with surrounding matter deep in the cosmos, using observations from NASA’s IXPE (Imaging X-ray Polarimetry Explorer) and…
An international team of astronomers has uncovered new evidence to explain how pulsing remnants of exploded stars interact with surrounding matter deep in the cosmos, using observations from NASA’s IXPE (Imaging X-ray Polarimetry Explorer) and…
NASA’s IXPE Imager Reveals Mysteries of Rare Pulsar
An international team of astronomers has uncovered new evidence to explain how pulsing remnants of exploded stars interact with surrounding matter deep in the cosmos, using observations from NASA’s IXPE (Imaging X-ray Polarimetry Explorer) and other telescopes. Scientists based in the U.S., Italy, and Spain, set their sights on a mysterious cosmic duo called PSR J1023+0038, or J1023 for short.
cerebral-overload.com
July 16, 2025 at 9:30 AM
NASA’s IXPE Imager Reveals Mysteries of Rare Pulsar
An international team of astronomers has uncovered new evidence to explain how pulsing remnants of exploded stars interact with surrounding matter deep in the cosmos, using observations from NASA’s IXPE (Imaging X-ray Polarimetry Explorer) and…
An international team of astronomers has uncovered new evidence to explain how pulsing remnants of exploded stars interact with surrounding matter deep in the cosmos, using observations from NASA’s IXPE (Imaging X-ray Polarimetry Explorer) and…
arXiv:2505.00813v1 Announce Type: new
Abstract: We report the first X-ray polarimetric results of the neutron star (NS) low-mass X-ray binary (LMXB) Z-source GX 349+2 using the Imaging X-ray Polarimetry Explorer (IXPE). We discovered that the X-ray [1/4 of https://arxiv.org/abs/2505.00813v1]
Abstract: We report the first X-ray polarimetric results of the neutron star (NS) low-mass X-ray binary (LMXB) Z-source GX 349+2 using the Imaging X-ray Polarimetry Explorer (IXPE). We discovered that the X-ray [1/4 of https://arxiv.org/abs/2505.00813v1]
May 5, 2025 at 6:07 AM
arXiv:2505.00813v1 Announce Type: new
Abstract: We report the first X-ray polarimetric results of the neutron star (NS) low-mass X-ray binary (LMXB) Z-source GX 349+2 using the Imaging X-ray Polarimetry Explorer (IXPE). We discovered that the X-ray [1/4 of https://arxiv.org/abs/2505.00813v1]
Abstract: We report the first X-ray polarimetric results of the neutron star (NS) low-mass X-ray binary (LMXB) Z-source GX 349+2 using the Imaging X-ray Polarimetry Explorer (IXPE). We discovered that the X-ray [1/4 of https://arxiv.org/abs/2505.00813v1]
High-precision broadband linear polarimetry of early-type binaries. V. The Binary System HD 165052 in Open Cluster NGC 6530
https://arxiv.org/pdf/2410.20991
Yasir Abdul Qadir, Andrei V. Berdyugin, Vilppu Piirola, Takeshi Sakanoi, Masato Kagitani, S. V. Berdyugina
https://arxiv.org/pdf/2410.20991
Yasir Abdul Qadir, Andrei V. Berdyugin, Vilppu Piirola, Takeshi Sakanoi, Masato Kagitani, S. V. Berdyugina
High-precision broadband linear polarimetry of early-type binaries. V. The Binary System HD 165052 in Open Cluster NGC 6530
arXiv abstract link
arxiv.org
October 29, 2024 at 3:01 AM
High-precision broadband linear polarimetry of early-type binaries. V. The Binary System HD 165052 in Open Cluster NGC 6530
https://arxiv.org/pdf/2410.20991
Yasir Abdul Qadir, Andrei V. Berdyugin, Vilppu Piirola, Takeshi Sakanoi, Masato Kagitani, S. V. Berdyugina
https://arxiv.org/pdf/2410.20991
Yasir Abdul Qadir, Andrei V. Berdyugin, Vilppu Piirola, Takeshi Sakanoi, Masato Kagitani, S. V. Berdyugina
They should use Spectro-Polarimetry, like us
December 14, 2024 at 2:23 PM
They should use Spectro-Polarimetry, like us