M. Pesce-Rollins

5 ta ish

National Institute for Nuclear Physics, Pisa Division

1. Polarized x-rays constrain the disk-jet geometry in the black hole x-ray binary Cygnus X-1

   H. Krawczynski, Fabio Muleri, Michal Dovčiak +97

   Maqola20226 iqtibos

   ABIABI:AkademIndex/2026.other.394312

2. The enhanced X-ray Timing and Polarimetry mission—eXTP for launch in 2030

   Shuang‐Nan Zhang, Andrea Santangelo, Yupeng Xu +97

   MaqolaOAOchiq kirishAstrophysical Phenomena and ObservationsScience China Physics Mechanics and Astronomy20254 iqtibos

   ABIABI:AkademIndex/2025.article.000056

3. MINUTE-TIMESCALE >100 MeV γ-RAY VARIABILITY DURING THE GIANT OUTBURST OF QUASAR 3C 279 OBSERVED BY FERMI-LAT IN 2015 JUNE

   M. Ackermann, Richard Anantua, Katsuaki Asano +97

   MaqolaOAOchiq kirish20163 iqtibos

   ABIABI:AkademIndex/2026.other.058052

4. The Fermi-LAT Lightcurve Repository*

   S. Abdollahi, M. Ajello, L. Baldini +97

   Maqola20232 iqtibos

   ABIABI:AkademIndex/2026.other.254979

5. X-Ray Polarization of the Black Hole X-Ray Binary 4U 1630–47 Challenges the Standard Thin Accretion Disk Scenario

   Ajay Ratheesh, Michal Dovčiak, H. Krawczynski +97

   Maqola20242 iqtibos

   ABIABI:AkademIndex/2026.other.756238