-
Photometrical observations of GRB
The database of Gamma Ray Burst (GRB) photometrical observations obtained on defferent telescopes at Fesenkov Astrophysical Institute, Almaty, Kazakhstan. Observations were... -
Associations between short GRBs & FRBs
The physical origin of fast radio bursts (FRBs) is still unclear. However, young magnetars associated with short-duration gamma-ray bursts (SGRBs) have been thought to be... -
Radio-bright/dark GRBs X/radio properties
We analyse two distinct samples of gamma-ray bursts (GRBs), with and without radio afterglow emission. We use an updated sample of 211 GRBs and find, in agreement with previous... -
The gamma/optical flares of 4FGL-DR3 blazars
Using blazar light curves from the optical All-Sky Automated Survey for Supernovae (ASAS-SN) and the {gamma}-ray Fermi-LAT telescope, we performed the most extensive statistical... -
Estimating the peak energy of Swift GRBs
Gamma-ray bursts (GRBs) are among the most energetic explosive phenomena in the universe, and their peak energy (Ep) is a key physical quantity for understanding the prompt... -
GCN VOEvent Streams From Swift-BAT (Burst Alert Telescope)
VOEvent alerts produced from transient detections resulting from observations with the NASA Neil Gehrels Swift Observatory and the Burst Alert Telescope. Events should be... -
GCN VOEvent Streams From Fermi-GBM
VOEvent alerts produced from transient detections resulting from observations with the NASA Fermi Gamma-ray Burst Monitor. Events should be reported within tens to hundreds of... -
GCN VOEvent Streams From Fermi-LAT
description: VOEvent alerts produced from transient detections resulting from observations with the NASA Fermi Large Area Telescope. Events should be reported within tens to of... -
GCN VOEvent Streams From Swift-UVOT
VOEvent alerts produced from transient detections resulting from observations with the NASA Neil Gehrels Swift Observatory and the Ultraviolet Optical Telescope. Events should... -
IR-bright gamma-ray burst host galaxies
We identify and explore the properties of an infrared-bright gamma-ray burst (GRB) host population. Candidate hosts are selected by coincidence with sources in WISE, with... -
AMI 15.7GHz GRB catalogue
We present the Arcminute Microkelvin Imager (AMI) Large Array catalogue of 139 gamma-ray bursts (GRBs). AMI observes at a central frequency of 15.7GHz and is equipped with a... -
Abundance ratio in gamma-ray burst
The distribution of the N/O element abundance ratios calculated by the detailed modelling of different galaxy spectra at z<4 is investigated. Supernova (SN) and long... -
Photometry of the afterglow of GRB 130831A
Gamma-ray bursts (GRBs) are the most luminous explosions in the Universe, yet the nature and physical properties of their energy sources are far from understood. Very important... -
Swift GRBs light curve reconstruction
Gamma-ray bursts (GRBs), as they are observed at high redshift (z=9.4), are vital to cosmological studies and investigating Population III stars. To tackle these studies, we... -
Optical LC fit parameters for 179 GRBs
Gamma-ray bursts (GRBs) are fascinating events due to their panchromatic nature. We study optical plateaus in GRB afterglows via an extended search into archival data. We... -
Insight-HXMT GRB catalog, 2017-2021 obs.
The Hard X-ray Modulation Telescope (Insight-HXMT) is China's first X-ray astronomy satellite. It was launched on 2017 June 15. The anticoincidence CsI detectors of the High... -
2nd cat. of IPN localizations of Konus short GRBs
We present the catalog of InterPlanetary Network (IPN) localizations for 199 short-duration gamma-ray bursts (sGRBs) detected by the Konus-Wind (KW) experiment between 2011... -
The Fermi-LAT long-term transient sources (1FLT)
We present the first Fermi Large Area Telescope (LAT) catalog of long-term {gamma}-ray transient sources (1FLT). This comprises sources that were detected on monthly time... -
Fermi GBM GRBs with multiple pulses
Gamma-ray bursts (GRBs) are highly variable and exhibit strong spectral evolution. In particular, the emission properties vary from pulse to pulse in multipulse bursts. Here we... -
Swift long gamma-ray bursts
The exact relationship between the long gamma-ray burst (LGRB) rate and the cosmic star formation rate (CSFR) is essential for using LGRBs as cosmological probes. In this work,...
