Social isolation recruits amygdala-cortical circuitry to escalate alcohol drinking

Kavli Affiliate: Kay Tye | Authors: Reesha Patel, Makenzie Patarino, Kelly Kim, Rachelle Pamintuan, Felix Taschbach, Hao Li, Christopher Lee, Aniek van Hoek, Rogelio Castro, Christian Cazares, Ray Miranda, Caroline Jia, Jeremy Delahanty, Kanha Batra, Laurel Keyes, Avraham Libster, Romy W. Wichmann, Talmo Pereira, Marcus Benna and Kay M. Tye | Summary: How do social […]


Continue.. Social isolation recruits amygdala-cortical circuitry to escalate alcohol drinking

Highly Significant Detection of X-Ray Polarization from the Brightest Accreting Neutron Star Sco X-1

Kavli Affiliate: Nicola Omodei | First 5 Authors: Fabio La Monaca, Alessandro Di Marco, Juri Poutanen, Matteo Bachetti, Sara E. Motta | Summary: The Imaging X-ray Polarimetry Explorer (IXPE) measured with high significance the X-ray polarization of the brightest Z-source Scorpius X-1, resulting in the nominal 2-8 keV energy band in a polarization degree of […]


Continue.. Highly Significant Detection of X-Ray Polarization from the Brightest Accreting Neutron Star Sco X-1

Highly Significant Detection of X-Ray Polarization from the Brightest Accreting Neutron Star Sco X-1

Kavli Affiliate: Herman L. Marshall | First 5 Authors: Fabio La Monaca, Alessandro Di Marco, Juri Poutanen, Matteo Bachetti, Sara E. Motta | Summary: The Imaging X-ray Polarimetry Explorer measured with high significance the X-ray polarization of the brightest Z-source Sco X-1, resulting in the nominal 2-8 keV energy band in a polarization degree of […]


Continue.. Highly Significant Detection of X-Ray Polarization from the Brightest Accreting Neutron Star Sco X-1

Extragalactic Magnetism with SOFIA (SALSA Legacy Program). VII. A Tomographic View of Far-infrared and Radio Polarimetric Observations through MHD Simulations of Galaxies

Kavli Affiliate: Susan E. Clark | First 5 Authors: Sergio Martin-Alvarez, Enrique Lopez-Rodriguez, Tara Dacunha, Susan E. Clark, Alejandro S. Borlaff | Summary: The structure of magnetic fields in galaxies remains poorly constrained, despite the importance of magnetism in the evolution of galaxies. Radio synchrotron and far-infrared (FIR) polarization and polarimetric observations are the best […]


Continue.. Extragalactic Magnetism with SOFIA (SALSA Legacy Program). VII. A Tomographic View of Far-infrared and Radio Polarimetric Observations through MHD Simulations of Galaxies

Extragalactic Magnetism with SOFIA (SALSA Legacy Program). VII. A tomographic view of far infrared and radio polarimetric observations through MHD simulations of galaxies

Kavli Affiliate: Susan E. Clark | First 5 Authors: Sergio Martin-Alvarez, Enrique Lopez-Rodriguez, Tara Dacunha, Susan E. Clark, Alejandro S. Borlaff | Summary: The structure of magnetic fields in galaxies remains poorly constrained, despite the importance of magnetism in the evolution of galaxies. Radio synchrotron and far-infrared dust polarization (FIR) polarimetric observations are the best […]


Continue.. Extragalactic Magnetism with SOFIA (SALSA Legacy Program). VII. A tomographic view of far infrared and radio polarimetric observations through MHD simulations of galaxies

Modeling the Morphology of Fast Radio Bursts and Radio Pulsars with fitburst

Kavli Affiliate: Kiyoshi W. Masui | First 5 Authors: Emmanuel Fonseca, Ziggy Pleunis, Daniela Breitman, Ketan R. Sand, Bikash Kharel | Summary: We present a framework for modeling astrophysical pulses from radio pulsars and fast radio bursts (FRBs). This framework, called fitburst, generates synthetic representations of dynamic spectra that are functions of several physical and […]


Continue.. Modeling the Morphology of Fast Radio Bursts and Radio Pulsars with fitburst

Modeling the Morphology of Fast Radio Bursts and Radio Pulsars with fitburst

Kavli Affiliate: Kiyoshi W. Masui | First 5 Authors: Emmanuel Fonseca, Ziggy Pleunis, Daniela Breitman, Ketan R. Sand, Bikash Kharel | Summary: We present a framework for modeling astrophysical pulses from radio pulsars and fast radio bursts (FRBs). This framework, called fitburst, generates synthetic representations of dynamic spectra that are functions of several physical and […]


Continue.. Modeling the Morphology of Fast Radio Bursts and Radio Pulsars with fitburst