GRB 191016A: A Long Gamma-Ray Burst Detected by TESS
arXiv:2102.11295 · doi:10.3847/1538-4357/abe6a2
Abstract
The TESS exoplanet-hunting mission detected the rising and decaying optical afterglow of GRB 191016A, a long Gamma-Ray Burst (GRB) detected by Swift-BAT but without prompt XRT or UVOT follow-up due to proximity to the moon. The afterglow has a late peak at least 1000 seconds after the BAT trigger, with a brightest-detected TESS datapoint at 2589.7 s post-trigger. The burst was not detected by Fermi-LAT, but was detected by Fermi-GBM without triggering, possibly due to the gradual nature of rising light curve. Using ground-based photometry, we estimate a photometric redshift of . Combined with the high-energy emission and optical peak time derived from TESS, estimates of the bulk Lorentz factor range from . The burst is relatively bright, with a peak optical magnitude in ground-based follow-up of mag. Using published distributions of GRB afterglows and considering the TESS sensitivity and sampling, we estimate that TESS is likely to detect GRB afterglow per year above its magnitude limit.
arXiv comment10 pages, 7 figures. Accepted for publication in the Astrophysical Journal
References in corpus (36)
- Astropy: A Community Python Package for Astronomy
- Gaia Data Release 2. Summary of the contents and survey properties
- The Large Area Telescope on the Fermi Gamma-ray Space Telescope Mission
- The Transiting Exoplanet Survey Satellite
- Binary companions of evolved stars in APOGEE DR14: Search method and catalog of ~5,000 companions
- Spectra and Light Curves of Gamma-Ray Burst Afterglows
- HI4PI: A full-sky HI survey based on EBHIS and GASS
- The Fermi Gamma-Ray Burst Monitor
- The Burst Alert Telescope (BAT) on the Swift MIDEX Mission
- The TESS Input Catalog and Candidate Target List
- Predictions for The Very Early Afterglow and The Optical Flash
- The Afterglows of Swift-era Gamma-Ray Bursts. I. Comparing pre-Swift and Swift era Long/Soft (Type II) GRB Optical Afterglows
- Implications for the Cosmic Reionization from the Optical Afterglow Spectrum of the Gamma-Ray Burst 050904 at z = 6.3
- The prompt energy release of gamma-ray bursts using a cosmological k-correction
- REM observations of GRB 060418 and GRB 060607A: the onset of the afterglow and the initial fireball Lorentz factor determination
- A decade of Gamma-Ray Bursts observed by -LAT: The 2 GRB catalog
- The Swift Burst Analyser I: BAT and XRT spectral and flux evolution of Gamma Ray Bursts
- Short versus Long Gamma-Ray Bursts: spectra, energetics, and luminosities
- X-ray Destruction of Dust Along the Line of Sight to Gamma-Ray Bursts
- A statistical study of gamma-ray burst afterglows measured by the Swift Ultra-violet Optical Telescope
- Bulk Lorentz factors of Gamma-Ray Bursts
- The Earliest Luminous Sources and the Damping Wing of the Gunn-Peterson Trough
- Swift and XMM-Newton Observations of the Extraordinary GRB 060729: An afterglow with a more than 100 days X-ray light curve
- Photometric redshifts for GRB afterglows from GROND and Swift/UVOT
- The bright optical/NIR afterglow of the faint GRB 080710 - Evidence for a jet viewed off axis
- Discovery and Vetting of Exoplanets I: Benchmarking K2 Vetting Tools
- GRB081028 and its late-time afterglow re-brightening
- A Characteristic Dense Environment or Wind Signature in Prompt GRB Afterglows
- Study of GRB light curve decay indices in the afterglow phase
- Investigation of dust attenuation and star formation activity in galaxies hosting GRBs
- The luminous host galaxy, faint supernova and rapid afterglow rebrightening of GRB 100418A
- A Comprehensive Study of Gamma-Ray Burst Optical Emission: III. Brightness Distributions and Luminosity Functions of Optical Afterglows
- A Large Catalogue of Multi-wavelength GRB Afterglows I: Color Evolution And Its Physical Implication
- An Estimation of the Gamma-Ray Burst Afterglow Apparent Optical Brightness Distribution Function
- A Large Catalog of Homogeneous Ultra-Violet/Optical GRB Afterglows: Temporal and Spectral Evolution
- The Vast Potential of Exoplanet Satellites for High-Energy Astrophysics
Cited by in corpus (6)
- GRB 191016A: The onset of the forward shock and evidence of late energy injection
- Polarimetry and Photometry of Gamma-Ray Bursts Afterglows with RINGO3
- GRB 191016A: A highly collimated gamma-ray burst jet with magnetised energy injection
- A Comprehensive Investigation of Gamma-Ray Burst Afterglows Detected by TESS
- Searching for Gravitational-Wave Counterparts using the Transiting Exoplanet Survey Satellite
- Broad-band Spectral Modeling of Prompt Emission from Gamma-Ray Bursts Observed by the Transiting Exoplanet Survey Satellite