GOTO identification and broadband modelling of the counterpart to the SVOM GRB 250818B
Clicks: 1
ID: 318255
2026
Article Quality & Performance Metrics
Overall Quality
Not rated
Combines reader engagement with the AI quality analysis. This
article has not been analysed, so there is no overall score —
reader engagement is measured and shown alongside.
Reader Engagement
0.0
/100
1 views
0 readers
AI Quality Assessment
Not analyzed
Readership in this journal
Ranked #889 of 913 articles by views in monthly notices of the royal astronomical society
Most read
Least read
Bar heights use a square-root scale. Only the 120 most-read articles are drawn; the journal has 913 in total.
Mint this article as an NFT
Not yet mintedCreate a permanent, verifiable on-chain record of this article on the Scimatic Network. The NFT is held in your Journament account, and you can withdraw it to your own wallet at any time.
5
SUSD
one-off · no wallet required
Abstract
Abstract We present the discovery and multi-wavelength follow-up of 250818B, detected by the Space Variable Objects Monitor (SVOM) and localised by the Gravitational-wave Optical Transient Observer (GOTO). We compile X-ray, optical/NIR, and radio data into broadband light curves and SEDs. Despite being initially reported as short, the public prompt light-curve figure suggests a duration of ~5 s, arguing against a secure short-duration classification. The afterglow is unusually bright relative to short-GRB samples: in X-rays and optical it is broadly consistent with the long-GRB population, while in the radio it is among the most luminous events in the short-GRB comparison sample and remains within the long-GRB range. MeerKAT detects the source at 3.1 GHz, while the Atacama Large Millimeter/submillimeter Array (ALMA) provides deep higher-frequency limits. Keck/LRIS spectroscopy shows continuum and metal absorption (Fe ii, Mg ii, Mg i), giving z = 1.216. Synchrotron forward-shock modelling favours a constant-density medium and refreshed (energy-injection) emission, well described by a two-component jet with core isotropic-equivalent kinetic energy E0 ~ 8 × 1052 erg, ambient number density n0 ~ 12 cm−3, jet half-opening angle θj ≃ 0.13 rad (~7.4○), and electron index p ≃ 1.67. We do not identify a host conclusively: the data admit either a faint LS DR10 galaxy at ~4″ (~34 kpc) as an offset candidate, or a fainter, near-coincident uncatalogued host. 250818B highlights the power of rapid counterpart identification in the SVOM era, while uncertain prompt classification and inconclusive host association still limit progenitor interpretation.
| Reference Key |
openalex_W7165638892
Use this key to autocite in the manuscript while using
SciMatic Manuscript Manager or Thesis Manager
|
|---|---|
| Authors | S Belkin, Gavin P. Lamb, K Ackley, M E Wortley, S McGee, G Schroeder, M Shrestha, B. P. Gompertz, D K Galloway, R Starling, WF Fong, T Laskar, Chang Liu, Alexa C. Gordon, N Pankov, A E Volvach, L N Volvach, A Shein, A Pozanenko, M. Dyer, J. Lyman, K Ulaczyk, D. Steeghs, V. S. Dhillon, P O’Brien, Gavin Ramsay, K Noysena, R Kotak, R. P. Breton, L K Nuttall, D Pollacco, Supachai Awiphan, J. Casares, P Chote, A A Chrimes, R. A. J. Eyles-Ferris, B Godson, P Irawati, D Jarvis, Y Julakanti, L Kelsey, Mark Kennedy, T. Killestein, A Kumar, A Levan, S Littlefair, M. Magee, S Mandhai, D Mata Sánchez, S Mattila, J McCormac, D. E. Mkrtichian, S Moran, J Mullaney, D O’Neill, M. Patel, K Pu, M. Pursiainen, A Sahu, U Sawangwit, E Stanway, Y Sun, Ben Warwick, K. Wiersema |
| Journal | monthly notices of the royal astronomical society |
| Year | 2026 |
| DOI |
10.1093/mnras/stag1193
|
| URL | |
| Keywords | Keywords not found |
Citations
No citations found. To add a citation, contact the admin at info@scimatic.org
Comments
No comments yet. Be the first to comment on this article.