activity
20012024
most citedVacuum nonlinear electrodynamic effects in hard emission of pulsars and magnetars

32 citations · 43 across the 9 of their papers we have counts for

collaborators

12 papers

astro-ph.HE2024★ 1 cited

Gamma-ray bursts at extremely small fluence

Vladimir Lipunov, Sergey Svertilov, Vladislav Topolev

In this review we show that the space experiment with gamma-ray detector with sensitivity 2 orders of magnitude higher than existing ones will make it possible to discover up to a…

astro-ph.IM2018★ 3 cited

Observations of Near-Earth Optical Transients with the Lomonosov Space Observatory

V. M. Lipunov, E. S. Gorbovskoy, V. G. Kornilov +8

The results of observations with the MASTER-SHOK robotic wide-field optical cameras onboard the Lomonosov Space Observatory carried out in 2016 are presented. In all, the automated…

astro-ph.HE2017★ 2 cited

First results of the Lomonosov TUS and GRB experiments

S. V. Biktemerova, A. V. Bogomolov, V. V. Bogomolov +39

On April 28, 2016, the Lomonosov satellite, equipped with a number of scientific instruments, was launched into orbit. Here we present briefly some of the results obtained with the…

astro-ph.HE2015

Testing and Performance of UFFO Burst Alert & Trigger Telescope

J. Ripa, M. B. Kim, J. Lee +26

The Ultra-Fast Flash Observatory pathfinder (UFFO-p) is a new space mission dedicated to detect Gamma-Ray Bursts (GRBs) and rapidly follow their afterglows in order to provide earl…

astro-ph.HE2012

Feasibility of a Small, Rapid Optical-to-IR Response, Next Generation Gamma Ray Burst Mission

B. Grossan, G. F. Smoot, V. V. Bogomolov +13

We present motivations for and study feasibility of a small, rapid optical to IR response gamma ray burst (GRB) space observatory. By analyzing existing GRB data, we give realistic…

astro-ph.IM2012★ 4 cited

A next generation Ultra-Fast Flash Observatory (UFFO-100) for IR/optical observations of the rise phase of gamma-ray bursts

B. Grossan, I. H. Park, S. Ahmad +39

The Swift Gamma-ray Burst (GRB) observatory responds to GRB triggers with optical observations in ~ 100 s, but cannot respond faster than ~ 60 s. While some ground-based telescopes…