You can get "Polarized multiwavelength emission from pulsar wind - accretion disk interaction in a transitional millisecond pulsar" from ui.adsabs.harvard.edu/abs/2024arXiv2…

Happy new year to all!

Today we present a comprehensive study of the flaring mode of the transitional millisecond pulsar (tMSP) PSR J1023+0038 during its X-ray sub-luminous state, using strictly simultaneous X-ray, UV, optical, and radio observations. arxiv.org/pdf/2502.06953 (A&A Letters) Institute of Space Sciences (ICE-CSIC)

I have just added information in the website regarding a soon-to-open opportunity to join my group as a Ph.D. student. Please forward to those that might be interested. For details, visit the Join Us link at sites.google.com/view/dft-resea…

We have just released "Identification and characterisation of the gamma-ray counterpart of the transitional pulsar candidate CXOU J110926.4-650224" (A&A, arxiv.org/abs/2502.18073)

We have just released our study on "Upper limits on the gamma-ray emission from the microquasar V4641 Sgr" (ApJ, arxiv.org/abs/2503.16844). No emission found in Fermi-LAT. No correlation between any flares in the gamma-ray light curve and X-ray outbursts.

We have just released '3D MHD simulations of runaway pulsars in core collapse supernova remnants' (A&A Letters, arxiv.org/pdf/2503.21492 These are the first 3D global classical MHD simulation of the CSM around a runaway massive star in the ISM of the Milky Way’s galactic plane.

Our paper 'Galactic transient sources with the Cherenkov Telescope Array Observatory' has been accepted for publication in MNRAS. The article will be available at doi.org/10.1093/mnras/…

We recently released "Fermi-LAT and FAST observation of the gamma-ray binary HESS J0632+057" (JHEAp) arxiv.org/abs/2504.16881 We carried out six deep radio observations. No radio pulsation was detected. Gamma-ray luminosity at the lowest of gamma-ray binaries.

I am glad to share good news: The Fermi Collaboration has just been awarded with the 2025 Giuseppe and Vanna Cocconi Prize of the European Physical Society for outstanding work in particle astrophysics the last 15 years! ESCUELADEESCRITORES CSIC Indomedia Gemilang Institute of Space Sciences (ICE-CSIC)

I wanted to draw attention on our recent Geminga results. Here is a summary in 2 figures (A&A, arxiv.org/abs/2505.21632)

We have just released 'Probing multi-band variability and mode switching in the candidate transitional millisecond pulsar 3FGL J1544.6-1125' (A&A) arxiv.org/abs/2506.20213 Our findings reinforce the mini-pulsar nebula picture for tMSPs in the sub-luminous state.

We have also recently released 'A Systematic Search for MeV-GeV Pulsar Wind Nebulae without Gamma-ray Detected Pulsars' (ApJ arxiv.org/abs/2506.18599 ) We report the analysis of 58 regions, with 9 likely PWN counterparts. This would increase the GeV PWN population from 12 to 21.