-
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 Swift-XRT
VOEvent alerts produced from transient detections resulting from observations with the NASA Neil Gehrels Swift Observatory and the X-ray Telescope. Events should be reported... -
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... -
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... -
FRB 20121102A parameters of the NRT bursts
The origin(s) of fast radio bursts (FRBs), mysterious radio bursts coming from extragalactic distances, remains unknown. Multiwavelength observations are arguably the only way... -
Gamma-ray burst redshifts
We here propose a new model-independent technique to overcome the circularity problem affecting the use of gamma-ray bursts (GRBs) as distance indicators through the use of... -
Model for subphotospheric dissipation in GRBs
It has been suggested that the prompt emission in gamma-ray bursts (GRBs) could be described by radiation from the photosphere in a hot fireball. Such models must be tested by... -
Metals, depletion, and dimming: decrypting dust
Dust plays a pivotal role in the chemical enrichment of the interstellar medium. In the era of mid-/high-resolution spectra and multiband spectral energy distributions, testing... -
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... -
GRBs data
The detections of some long gamma-ray bursts (LGRBs) relevant to mergers of neutron star (NS)-NS or black hole (BH)-NS, as well as some short gamma-ray bursts (SGRBs) probably... -
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... -
Identifying GRBs from the Fermi/GBM TTE data
To investigate gamma-ray bursts (GRBs) in depth, it is crucial to develop an effective method for identifying GRBs accurately. Current criteria, e.g., onboard blind search,... -
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... -
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,... -
Rest-frame parameters of short and long GRBs
The intrinsic statistical properties and correlations of short gamma-ray bursts (SGRBs) have not been fully determined, due to the limitations of observations. In this paper, we...
