activity
20222024
most citedDeciphering the ~18 TeV photons from GRB 221009A

19 citations · 28 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.HE2024★ 2 cited

Redshift constrain of BL Lac PKS 1424+240

Sarira Sahu, D. I. Páez-Sánchez, B. Medina-Carrillo +3

In the period between 2009 and 2015, several very high-energy (VHE GeV) gamma-ray flaring events from the BL Lac object PKS 1424+240 were observed by the Cerenkov telescope…

astro-ph.HE2024★ 3 cited

TeV afterglow from GRB 221009A: photohadronic origin?

Sarira Sahu, B. Medina-Carrillo, D. I. Páez-Sánchez +2

Gamma-ray burst (GRB), GRB 221009A, a long-duration GRB, was observed simultaneously by the Water Cherenkov Detector Array (WCDA) and the Kilometer Squared Array (KM2A) of the Larg…

astro-ph.HE2023★ 1 cited

A photohadronic interpretation of the H.E.S.S. afterglow observations from GRB 221009A

Sarira Sahu, B. Medina-Carrillo, D. I. Páez-Sánchez +2

The High Energy Stereoscopic System (H.E.S.S.) started observing the extremely powerful long-duration gamma-ray burst, GRB 221009A, after 53 hours of the triggering event. The H.E.…

astro-ph.HE2023★ 2 cited

Constraining the redshift of BL Lac VER J0521+211

Sarira Sahu, B. Medina-Carrillo, G. Sánchez-Colón +1

Observation of several very high energy (VHE) flaring events of the BL Lac object VER J0521+211 were reported by the VERITAS and MAGIC collaborations between 2009 and 2014. The red…

astro-ph.HE2022★ 19 cited

Deciphering the ~18 TeV photons from GRB 221009A

Sarira Sahu, B. Medina-Carrillo, G. Sánchez-Colón +1

On 9 October, 2022, an extremely powerful gamma-ray burst, GRB 221009A, was detected by several instruments. Despite being obstructed by the Milky Way galaxy, its afterglow outburs…

astro-ph.HE2022★ 1 cited

Very high energy emission mechanism in the extreme blazar PGC 2402248

B. Medina-Carrillo, Sarira Sahu, G. Sánchez-Colón +1

Extreme high-frequency peaked BL Lacs (EHBLs) are characterized by a synchrotron peak frequency exceeding Hz and a second peak that can be in the energy range of few GeVs…