REVIEW 3 major objections 2 minor 142 references
EuraGovExam packs over 8,000 real civil-service exam questions into single images and shows that even leading vision-language models reach only about 86 percent accuracy.
Reviewed by Pith at T0; open to challenge. T0 means a machine referee read the full paper against a public rubric. the ladder, T0–T4 →
T0 review · grok-4.5
2026-07-13 17:06 UTC pith:SDJDJZKK
load-bearing objection Abstract pitches a useful real-exam VLM benchmark, but the supplied full text is an unrelated GRB afterglow paper, so none of the claims can be checked. the 3 major comments →
EuraGovExam: A Multilingual Multimodal Benchmark from Real-World Civil Service Exams
The pith
A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.
Core claim
Real civil-service exams from five Eurasian regions, when rendered as single images that contain the entire problem and require only a standardized answer format, form a stringent test of vision-language models; even the best systems achieve only roughly 86 percent accuracy and thereby expose concrete limits in layout parsing, multilingual typography, and culturally grounded reasoning.
What carries the argument
The single-image protocol: every item embeds problem statement, answer choices, and visual elements inside one high-resolution scan, accompanied solely by a minimal standardized instruction for answer formatting. This design eliminates external text and forces end-to-end visual-linguistic processing.
Load-bearing premise
That an 86 percent accuracy ceiling on this particular set of scanned multiple-choice exams under the single-image minimal-instruction setup reliably diagnoses general vision-language-model shortcomings rather than reflecting OCR artifacts, answer-key noise, or the specific sampling of domains and languages.
What would settle it
A controlled re-evaluation in which the identical questions are supplied as clean, machine-readable text (or as images with perfect OCR) and the same models then exceed 95 percent accuracy would show that the reported difficulty is largely an artifact of scanning and layout rather than of deeper reasoning limits.
If this is right
- Model developers gain a public, culturally diverse testbed that stresses layout, typography, and cross-lingual document understanding under realistic public-sector constraints.
- E-governance and automated exam-grading systems can use the same items to quantify and improve handling of authentic scanned forms and multilingual tables.
- Future VLM training or fine-tuning regimes that close the gap to human-level performance on EuraGovExam would demonstrate progress on high-stakes image-grounded reasoning.
- The 17-domain, five-region composition supplies a ready template for constructing parallel benchmarks in additional languages or administrative traditions.
Where Pith is reading between the lines
- Because the benchmark preserves original exam layouts, residual model errors are likely to cluster around table reading, multi-column parsing, and mixed-script typography—suggesting targeted pre-training on form-like documents could yield outsized gains.
- The cultural and linguistic spread implies that gains measured solely on English-centric VQA suites may overstate readiness for real public-sector deployment outside those languages.
- If the 86 percent ceiling persists after stronger OCR pipelines are applied, the residual gap would isolate genuine multi-hop and domain-knowledge failures rather than pure perception failures.
Editorial analysis
A structured set of objections, weighed in public.
Referee Report
Summary. The submission abstract presents EuraGovExam as a new multilingual multimodal VLM benchmark of >8,000 high-resolution scanned multiple-choice items drawn from real civil-service exams in South Korea, Japan, Taiwan, India, and the EU, spanning 17 domains. Items are rendered as single images containing the full question, choices, and visual elements, with only a minimal answer-format instruction, so that models must perform layout-aware, cross-lingual reasoning from pixels. The abstract reports that even state-of-the-art VLMs reach only ~86% accuracy and claims the resource sets a new standard for high-stakes, culturally realistic evaluation. The body of the supplied manuscript, however, is an unrelated astrophysics paper on forward- and reverse-shock afterglow emission from two-component GRB jets modeled with VegasAfterglow; none of the claimed dataset construction, annotation, leakage controls, model list, scoring protocol, or error analysis for EuraGovExam appears.
Significance. A carefully constructed, single-image, real-exam benchmark covering multiple Eurasian languages and administrative domains would be a valuable diagnostic for layout, OCR, and cross-lingual reasoning limits of current VLMs and would have clear applications in e-governance and exam preparation. Because the full methods, data, and results for EuraGovExam are absent from the supplied manuscript, that potential significance cannot be evaluated or credited.
major comments (3)
- The full manuscript text supplied under paper_id 2603.27223 is the unrelated GRB afterglow study (VegasAfterglow, ISM/wind FS/RS light curves, arXiv:2603.27225). No sections, tables, figures, or appendices describe EuraGovExam dataset construction, answer-key provenance, OCR/layout pipeline, train/test splits, leakage controls, model list, prompting protocol, or the 86% SOTA result. The central empirical claim therefore cannot be verified from the materials provided.
- Abstract claim that SOTA VLMs achieve only 86% accuracy and thereby diagnose genuine layout/cross-lingual limits: without the evaluation section, model list, scoring rules, or error analysis (OCR vs. reasoning failures), it is impossible to determine whether the figure is an artifact of scan quality, answer-key errors, domain sampling, or prompt format. This is load-bearing for the 'new standard' assertion.
- Abstract design claim that every item is a single image with only minimal formatting instructions: the manuscript contains no protocol, example images, or ablation showing that performance is limited by layout-aware reasoning rather than ordinary OCR or language coverage. The diagnostic power of the benchmark therefore remains unsubstantiated.
minor comments (2)
- Title, abstract, and arXiv identifier (2603.27223, cs.CV) do not match the body text (astro-ph.HE GRB afterglow paper). This metadata mismatch must be resolved before any scientific review can proceed.
- If the intended EuraGovExam manuscript exists, it should be supplied in full so that dataset statistics, annotation quality, and evaluation tables can be examined.
Circularity Check
No circularity: self-contained numerical parameter study of two-component jet afterglows with independent analytical scalings.
full rationale
The manuscript is a systematic exploration of forward- and reverse-shock afterglow light curves from two-component (core+wing) jets using the external VegasAfterglow code plus newly derived analytical scalings (Appendix A). Parameters (energies, Lorentz factors, opening angles, engine duration, density profiles) are varied one-at-a-time from a stated default table; resulting multi-band light curves and critical frequencies are reported and compared to the independent scalings. No quantity is fitted to data and then re-presented as a prediction; no uniqueness theorem or ansatz is imported via self-citation to force the central claims; the derivations of pre-peak slopes, peak-time ratios R(t_peak), peak-flux ratios R(F_ u,peak), and Doppler corrections a( heta) stand on standard blast-wave hydrodynamics and synchrotron formulae that do not presuppose the numerical outcomes. The paper therefore contains no self-definitional loops, fitted-input-as-prediction steps, or load-bearing self-citation chains. Score 0 is the correct, expected outcome for this class of modeling paper.
Axiom & Free-Parameter Ledger
free parameters (2)
- Reported SOTA accuracy (~86%)
- Dataset size and domain mix (8,000+ items, 17 domains, 5 regions)
axioms (3)
- domain assumption Embedding full question content in a single image with only minimal answer-format instructions is a valid and superior stress test of layout-aware cross-lingual VLM reasoning versus text-extracted or multi-channel setups.
- domain assumption Real civil-service exam documents from KR/JP/TW/IN/EU are representative high-stakes public-sector assessments for evaluating cultural realism and linguistic diversity.
- ad hoc to paper Multiple-choice accuracy on this set diagnoses general limitations of current VLMs in multilingual image-grounded settings.
invented entities (1)
-
EuraGovExam benchmark
no independent evidence
read the original abstract
We present EuraGovExam, a multilingual and multimodal benchmark sourced from real-world civil service examinations across five representative Eurasian regions: South Korea, Japan, Taiwan, India, and the European Union. Designed to reflect the authentic complexity of public-sector assessments, the dataset contains over 8,000 high-resolution scanned multiple-choice questions covering 17 diverse academic and administrative domains. Unlike existing benchmarks, EuraGovExam embeds all question content--including problem statements, answer choices, and visual elements--within a single image, providing only a minimal standardized instruction for answer formatting. This design demands that models perform layout-aware, cross-lingual reasoning directly from visual input. All items are drawn from real exam documents, preserving rich visual structures such as tables, multilingual typography, and form-like layouts. Evaluation results show that even state-of-the-art vision-language models (VLMs) achieve only 86% accuracy, underscoring the benchmark's difficulty and its power to diagnose the limitations of current models. By emphasizing cultural realism, visual complexity, and linguistic diversity, EuraGovExam establishes a new standard for evaluating VLMs in high-stakes, multilingual, image-grounded settings. It also supports practical applications in e-governance, public-sector document analysis, and equitable exam preparation.
Reference graph
Works this paper leans on
-
[1]
(A10) becomes Rs < R∆ < RΓ < R N ,(A11) which means that the reverse shock crosses the shell be- fore the deceleration begins [109]
ISM: Thin-Shell FS In the thin-shell regime, the ordering of the radii in Eq. (A10) becomes Rs < R∆ < RΓ < R N ,(A11) which means that the reverse shock crosses the shell be- fore the deceleration begins [109]. Consequently, the Lorentz factor stays constant untilt dec, after which it decays as follows: Γ∝ ( Γ0, t < t dec E1/8t−3/8, t > t dec ,(A12) where...
-
[2]
After that, the shocked ejecta gradually adjusts to the BM solution
ISM: Thin-Shell RS The blastwave dynamics is the same as in the thin-shell FS case during the shock-crossing phase. After that, the shocked ejecta gradually adjusts to the BM solution. The analytical expressions detailed below represent the standard scaling laws for thin-shell RS emission, derived under the assumption that the shock reaches mildly relativ...
-
[3]
(A10) are or- dered in reverse [6]: Rs > R∆ > RΓ > R N .(A35) The reverse shock becomes relativistic early, which causes the blastwave to decelerate during the shock-crossing phase
ISM: Thick-Shell FS In the thick-shell case, the radii in Eq. (A10) are or- dered in reverse [6]: Rs > R∆ > RΓ > R N .(A35) The reverse shock becomes relativistic early, which causes the blastwave to decelerate during the shock-crossing phase. The deceleration radiusR Γ is no longer relevant. The blastwave decelerates as Γ∝ ( Γ0ξ3/4 0 t−1/4, t < t × E1/8 ...
-
[4]
ISM: Thick-Shell RS In this case, the RS becomes relativistic early. The blastwave decelerates as γ3 ∼ Γ0ξ3/4 0√ 2 × ( (t/t×)−1/4, t < t × (t/t×)−7/16, t > t × ,(A47) The scalings laws for the thick-shell RS are given as Fν,max ∝E 5/4 ISOΓ−1 0 × ( t−5/4 × t1/2, t < t × t11/48 × t−47/48, t > t × ,(A48) νm ∝Γ 2 0 × ( 1, t < t × t73/48 × t−73/48, t > t × ,(A...
-
[5]
Since the algebra is analogous, we do not repeat it here
Wind The derivations in a wind-like medium follows the same procedure as in the ISM case: one combines the dynami- cal evolution of the shocked regions with the time depen- dence of the critical frequencies to obtain the flux scalings in a particular spectram segment of interest. Since the algebra is analogous, we do not repeat it here. Instead, we summar...
-
[6]
M. J. Rees and P. Meszaros, Relativistic fireballs - Energy conversion and time-scales., MNRAS258, 41 (1992)
1992
-
[7]
Piran, Gamma-ray bursts and the fireball model, Phys
T. Piran, Gamma-ray bursts and the fireball model, Phys. Rep.314, 575 (1999), arXiv:astro-ph/9810256 [astro-ph]
Pith/arXiv arXiv 1999
-
[8]
M. J. Rees and P. Meszaros, Unsteady Outflow Mod- els for Cosmological Gamma-Ray Bursts, ApJ430, L93 (1994), arXiv:astro-ph/9404038 [astro-ph]
Pith/arXiv arXiv 1994
-
[9]
S. Kobayashi, T. Piran, and R. Sari, Can Internal Shocks Produce the Variability in Gamma-Ray Bursts?, ApJ490, 92 (1997), arXiv:astro-ph/9705013 [astro-ph]
Pith/arXiv arXiv 1997
-
[10]
T. Piran, The physics of gamma-ray bursts, Re- views of Modern Physics76, 1143 (2004), arXiv:astro- ph/0405503 [astro-ph]
arXiv 2004
-
[11]
R. Sari and T. Piran, Hydrodynamic Timescales and Temporal Structure of Gamma-Ray Bursts, ApJ455, L143 (1995), arXiv:astro-ph/9508081 [astro-ph]
Pith/arXiv arXiv 1995
-
[12]
Meszaros and M
P. Meszaros and M. J. Rees, Relativistic Fireballs and Their Impact on External Matter: Models for Cosmo- logical Gamma-Ray Bursts, ApJ405, 278 (1993)
1993
-
[13]
S. Kobayashi, T. Piran, and R. Sari, Hydrodynamics of a Relativistic Fireball: The Complete Evolution, ApJ 513, 669 (1999), arXiv:astro-ph/9803217 [astro-ph]
Pith/arXiv arXiv 1999
-
[14]
P. M´ esz´ aros and M. J. Rees, Optical and Long- Wavelength Afterglow from Gamma-Ray Bursts, ApJ 476, 232 (1997), arXiv:astro-ph/9606043 [astro-ph]
Pith/arXiv arXiv 1997
-
[15]
R. Sari, T. Piran, and R. Narayan, Spectra and Light Curves of Gamma-Ray Burst Afterglows, ApJ497, L17 (1998), arXiv:astro-ph/9712005 [astro-ph]
Pith/arXiv arXiv 1998
-
[16]
R. Sari and T. Piran, Predictions for the Very Early Afterglow and the Optical Flash, ApJ520, 641 (1999), arXiv:astro-ph/9901338 [astro-ph]
Pith/arXiv arXiv 1999
-
[17]
B. Zhang, S. Kobayashi, and P. M´ esz´ aros, Gamma-Ray Burst Early Optical Afterglows: Implications for the Initial Lorentz Factor and the Central Engine, ApJ595, 950 (2003), arXiv:astro-ph/0302525 [astro-ph]
Pith/arXiv arXiv 2003
-
[18]
B. Zhang, Y. Z. Fan, J. Dyks, S. Kobayashi, 25 P. M´ esz´ aros, D. N. Burrows, J. A. Nousek, and N. Gehrels, Physical Processes Shaping Gamma-Ray Burst X-Ray Afterglow Light Curves: Theoretical Im- plications from the Swift X-Ray Telescope Observations, ApJ642, 354 (2006), arXiv:astro-ph/0508321 [astro- ph]
Pith/arXiv arXiv 2006
-
[19]
V. Lipunov, V. Kornilov, E. Gorbovskoy, N. Shatskij, D. Kuvshinov, N. Tyurina, A. Belinski, A. Krylov, P. Balanutsa, V. Chazov, A. Kuznetsov, P. Kortunov, A. Sankovich, A. Tlatov, A. Parkhomenko, V. Krushin- sky, I. Zalozhnyh, A. Popov, T. Kopytova, K. Ivanov, S. Yazev, and V. Yurkov, Master Robotic Net, Advances in Astronomy2010, 349171 (2010), arXiv:090...
Pith/arXiv arXiv 2010
-
[20]
A. Burd, M. Cwiok, H. Czyrkowski, R. Dabrowski, W. Dominik, M. Grajda, M. Husejko, M. Jegier, A. Kalicki, G. Kasprowicz, K. Kierzkowski, K. Krupska, K. Kwiecinska, L. Mankiewicz, K. Nawrocki, B. Pilecki, L. W. Piotrowski, K. Pozniak, R. Romaniuk, R. Salan- ski, M. Sokolowski, D. Szczygiel, G. Wrochna, and W. Zabolotny, Pi of the Sky - all-sky, real-time s...
Pith/arXiv arXiv 2005
-
[21]
W. T. Vestrand, J. A. Wren, P. R. Wozniak, R. Aptekar, S. Golentskii, V. Pal’Shin, T. Sakamoto, R. R. White, S. Evans, D. Casperson, and E. Fenimore, Energy in- put and response from prompt and early optical after- glow emission inγ-ray bursts, Nature442, 172 (2006), arXiv:astro-ph/0605472 [astro-ph]
Pith/arXiv arXiv 2006
-
[22]
A. Klotz, M. Bo¨ er, J. L. Atteia, and B. Gendre, Early Optical Observations of Gamma-Ray Bursts by the TAROT Telescopes: Period 2001-2008, AJ137, 4100 (2009), arXiv:0902.0898 [astro-ph.HE]
Pith/arXiv arXiv 2001
-
[23]
T. Komesh, B. Grossan, Z. Maksut, E. Abdikamalov, M. Krugov, and G. F. Smoot, Evolution of the after- glow optical spectral shape of GRB 201015A in the first hour: evidence for dust destruction, MNRAS520, 6104 (2023), arXiv:2211.03029 [astro-ph.HE]
Pith/arXiv arXiv 2023
-
[24]
Abdullayev, T
Z. Abdullayev, T. Komesh, B. Grossan, E. Abdika- malov, Z. Maksut, M. Krugov, S. Myrzakul, D. Tu- iakbayeva, and A. Kostangeldinova, Early-Time Opti- cal Spectral Shape Measurements of GRB 200925B,Re- vista Mexicana de Astronomia y Astrofisica Conference Series, Revista Mexicana de Astronomia y Astrofisica Conference Series,59, 109 (2025)
2025
-
[25]
C. Akerlof, R. Balsano, S. Barthelmy, J. Bloch, P. But- terworth, D. Casperson, T. Cline, S. Fletcher, F. Fron- tera, G. Gisler, J. Heise, J. Hills, R. Kehoe, B. Lee, S. Marshall, T. McKay, R. Miller, L. Piro, W. Pried- horsky, J. Szymanski, and J. Wren, Observation of con- temporaneous optical radiation from aγ-ray burst, Na- ture398, 400 (1999), arXiv:a...
Pith/arXiv arXiv 1999
-
[26]
J. Wei, B. Cordier, S. Antier, P. Antilogus, J. L. At- teia, A. Bajat, S. Basa, V. Beckmann, M. G. Bernar- dini, S. Boissier, L. Bouchet, V. Burwitz, A. Claret, Z. G. Dai, F. Daigne, J. Deng, D. Dornic, H. Feng, T. Foglizzo, H. Gao, N. Gehrels, O. Godet, A. Gold- wurm, F. Gonzalez, L. Gosset, D. G¨ otz, C. Gouiffes, F. Grise, A. Gros, J. Guilet, X. Han, M...
Pith/arXiv arXiv 2016
-
[27]
W. Yuan, C. Zhang, Y. Chen, and Z. Ling, The Einstein Probe Mission, inHandbook of X-ray and Gamma-ray Astrophysics, edited by C. Bambi and A. Sangangelo (2022) p. 86
2022
-
[28]
J. A. Nousek, C. Kouveliotou, D. Grupe, K. L. Page, J. Granot, E. Ramirez-Ruiz, S. K. Patel, D. N. Burrows, V. Mangano, S. Barthelmy, A. P. Beardmore, S. Cam- pana, M. Capalbi, G. Chincarini, G. Cusumano, A. D. Falcone, N. Gehrels, P. Giommi, M. R. Goad, O. Godet, C. P. Hurkett, J. A. Kennea, A. Moretti, P. T. O’Brien, J. P. Osborne, P. Romano, G. Tagliaf...
Pith/arXiv arXiv 2006
-
[29]
X.-G. Wang, B. Zhang, E.-W. Liang, H. Gao, L. Li, C.- M. Deng, S.-M. Qin, Q.-W. Tang, D. A. Kann, F. Ryde, and P. Kumar, How Bad or Good Are the External For- ward Shock Afterglow Models of Gamma-Ray Bursts?, ApJS219, 9 (2015), arXiv:1503.03193 [astro-ph.HE]
Pith/arXiv arXiv 2015
-
[30]
S.-X. Yi, M. Du, and T. Liu, Statistical Analyses of the Energies of X-Ray Plateaus and Flares in Gamma-Ray Bursts, ApJ924, 69 (2022), arXiv:2111.01041 [astro- ph.HE]
Pith/arXiv arXiv 2022
-
[31]
M. Busmann, B. O’Connor, J. Sommer, D. Gruen, P. Beniamini, R. Gill, M. J. Moss, A. Palmese, A. Riffeser, Y.-H. Yang, E. Troja, S. Dichiara, R. Ricci, N. Klingler, C. G¨ ossl, L. Hu, A. Rau, C. Ries, G. Ryan, M. Schmidt, M. Yadav, and G. R. Zeimann, The cu- rious case of EP241021a: Unraveling the mystery of its exceptional rebrightening, A&A701, A225 (202...
arXiv 2025
-
[32]
D. Akl, S. Antier, H. Koehn, P. T. H. Pang, J. J. Geng, R. Gill, E. Abdikamalov, C. Adami, V. Aivazyan, L. Almeida, S. Alshamsi, C. Andrade, Q. Andr´ e, C. Angulo-Valdez, J.-L. Atteia, K. Barkaoui, S. Basa, R. L. Becerra, P. Bendjoya, D. Berdikhan, E. Bernaud, S. Boissier, S. Brunier, A. Y. Burdanov, N. R. Butler, J. Chen, F. Colas, W. Corradi, M. W. Coug...
Pith/arXiv arXiv 2026
-
[33]
Liang, L
E.-W. Liang, L. Li, H. Gao, B. Zhang, Y.-F. Liang, X.- F. Wu, S.-X. Yi, Z.-G. Dai, Q.-W. Tang, J.-M. Chen, H.-J. L¨ u, J. Zhang, R.-J. Lu, L.-Z. L¨ u, and J.-Y. Wei, A comprehensive study of gamma-ray burst optical emis- sion. ii. afterglow onset and late re-brightening compo- nents, The Astrophysical Journal774, 13 (2013)
2013
-
[34]
M. Nardini, J. Greiner, T. Kr¨ uhler, S. Klose, R. Filgas, A. Nicuesa Guelbenzu, F. Olivares, A. Rau, A. Rossi, A. Updike, J. Elliott, P. Afonso, and C. Clemens, After- glow rebrightenings as a signature of a long-lasting cen- tral engine: the case of grb 100814a, Astronomy & As- trophysics562, 10.1051/0004-6361/201321525 (2014)
-
[35]
R. Sari and P. M´ esz´ aros, Impulsive and Varying Injec- tion in Gamma-Ray Burst Afterglows, ApJ535, L33 (2000), arXiv:astro-ph/0003406 [astro-ph]
Pith/arXiv arXiv 2000
-
[36]
B. Zhang and P. M´ esz´ aros, Gamma-Ray Bursts with Continuous Energy Injection and Their Afterglow Sig- nature, ApJ566, 712 (2002), arXiv:astro-ph/0108402 [astro-ph]
Pith/arXiv arXiv 2002
-
[37]
A. Panaitescu, P. M´ esz´ aros, N. Gehrels, D. Bur- rows, and J. Nousek, Analysis of the X-ray emission of nine Swift afterglows, MNRAS366, 1357 (2006), arXiv:astro-ph/0508340 [astro-ph]
Pith/arXiv arXiv 2006
-
[38]
T. Laskar, E. Berger, R. Margutti, D. Perley, B. A. Zauderer, R. Sari, and W.-f. Fong, Energy Injection in Gamma-Ray Burst Afterglows, ApJ814, 1 (2015), arXiv:1504.03702 [astro-ph.HE]
Pith/arXiv arXiv 2015
-
[39]
C. Angulo-Valdez, R. L. Becerra, R. Gill, N. Globus, W. H. Lee, D. L´ opez-C´ amara, C. Mihalenko, E. M. M´ endez, R. Ricci, K. Siellez, A. M. Watson, M. Yadav, Y.-H. Yang, D. Akl, S. Antier, J.-L. Atteia, S. Basa, N. R. Butler, S. Dichiara, D. Dornic, J.-G. Ducoin, F. Fortin, L. Garc´ ıa-Garc´ ıa, K. O. L´ opez, F. Mag- nani, B. O’Connor, M. Pereyra, N. ...
-
[40]
Z. G. Dai and T. Lu, Hydrodynamics of Relativistic Blast Waves in a Density-Jump Medium and Their Emission Signature, ApJ565, L87 (2002), arXiv:astro- ph/0111454 [astro-ph]
arXiv 2002
- [41]
-
[42]
E. Nakar and J. Granot, Smooth light curves from a bumpy ride: relativistic blast wave encounters a density jump, MNRAS380, 1744 (2007), arXiv:astro- ph/0606011 [astro-ph]
arXiv 2007
-
[43]
R. Filgas, J. Greiner, P. Schady, T. Kr¨ uhler, A. C. Updike, S. Klose, M. Nardini, D. A. Kann, A. Rossi, V. Sudilovsky, P. M. J. Afonso, C. Clemens, J. Elliott, A. Nicuesa Guelbenzu, F. Olivares E., and A. Rau, GRB 091127: The cooling break race on magnetic fuel, A&A 535, A57 (2011), arXiv:1109.2810 [astro-ph.HE]
Pith/arXiv arXiv 2011
-
[44]
A. Panaitescu, P. M´ esz´ aros, D. Burrows, J. Nousek, N. Gehrels, P. O’Brien, and R. Willingale, Evidence for chromatic X-ray light-curve breaks in Swift gamma-ray burst afterglows and their theoretical implications, MN- RAS369, 2059 (2006), arXiv:astro-ph/0604105 [astro- ph]
Pith/arXiv arXiv 2059
-
[45]
K. Misra, L. Resmi, D. A. Kann, M. Marongiu, A. Moin, S. Klose, G. Bernardi, A. de Ugarte Postigo, V. K. Jaiswal, S. Schulze, D. A. Perley, A. Ghosh, Dimple, H. Kumar, R. Gupta, M. J. Micha lowski, S. Mart´ ın, A. Cockeram, S. V. Cherukuri, V. Bhalerao, G. E. An- derson, S. B. Pandey, G. C. Anupama, C. C. Th¨ one, S. Barway, M. H. Wieringa, J. P. U. Fynbo...
Pith/arXiv arXiv 2021
-
[46]
G. P. Lamb and S. Kobayashi, Electromagnetic counter- parts to structured jets from gravitational wave detected mergers, MNRAS472, 4953 (2017), arXiv:1706.03000 [astro-ph.HE]
Pith/arXiv arXiv 2017
-
[47]
P. Beniamini, R. Gill, and J. Granot, Robust features of off-axis gamma-ray burst afterglow light curves, MN- RAS515, 555 (2022), arXiv:2204.06008 [astro-ph.HE]
Pith/arXiv arXiv 2022
-
[48]
B. O’Connor, E. Troja, G. Ryan, P. Beniamini, H. van Eerten, J. Granot, S. Dichiara, R. Ricci, V. Lipunov, J. H. Gillanders, R. Gill, M. Moss, S. Anand, I. An- dreoni, R. L. Becerra, D. A. H. Buckley, N. R. Butler, S. B. Cenko, A. Chasovnikov, J. Durbak, C. Francile, E. Hammerstein, A. J. van der Horst, M. M. Kasli- wal, C. Kouveliotou, A. S. Kutyrev, W. ...
Pith/arXiv arXiv 2023
-
[49]
R. Gill and J. Granot, GRB 221009A afterglow from a shallow angular structured jet, MNRAS524, L78 (2023), arXiv:2304.14331 [astro-ph.HE]
Pith/arXiv arXiv 2023
-
[50]
O. S. Salafia and G. Ghirlanda, The Structure of Gamma Ray Burst Jets, Galaxies10, 93 (2022), arXiv:2206.11088 [astro-ph.HE]
Pith/arXiv arXiv 2022
-
[51]
P. M´ esz´ aros, M. J. Rees, and R. A. M. J. Wijers, Viewing Angle and Environment Effects in Gamma-Ray Bursts: Sources of Afterglow Diversity, ApJ499, 301 (1998), arXiv:astro-ph/9709273 [astro-ph]
Pith/arXiv arXiv 1998
-
[52]
J. Granot, A. Panaitescu, P. Kumar, and S. E. Woosley, Off-Axis Afterglow Emission from Jetted Gamma-Ray Bursts, ApJ570, L61 (2002), arXiv:astro-ph/0201322 [astro-ph]
Pith/arXiv arXiv 2002
- [53]
-
[54]
A. Panaitescu and P. Kumar, The Effect of Angular Structure of Gamma-Ray Burst Outflows on the Af- terglow Emission, ApJ592, 390 (2003), arXiv:astro- ph/0301032 [astro-ph]
arXiv 2003
-
[55]
P. Beniamini, J. Granot, and R. Gill, Afterglow light curves from misaligned structured jets, MNRAS493, 3521 (2020), arXiv:2001.02239 [astro-ph.HE]
Pith/arXiv arXiv 2020
-
[56]
P. Beniamini, R. Duque, F. Daigne, and 27 R. Mochkovitch, X-ray plateaus in gamma-ray bursts’ light curves from jets viewed slightly off-axis, MNRAS 492, 2847 (2020), arXiv:1907.05899 [astro-ph.HE]
Pith/arXiv arXiv 2020
-
[57]
Birenbaum, R
G. Birenbaum, R. Gill, O. Bromberg, P. Beniamini, and J. Granot, Afterglow Linear Polarization Signa- tures from Shallow GRB Jets: Implications for Ener- getic GRBs, ApJ974, 308 (2024)
2024
-
[58]
E. Abdikamalov and P. Beniamini, Reverse and for- ward shock afterglow emission from steep jets viewed off-axis, MNRAS539, 2707 (2025), arXiv:2502.12757 [astro-ph.HE]
Pith/arXiv arXiv 2025
-
[59]
H. Wang, H. Zhou, Y.-Z. Fan, and D.-M. Wei, Forward and Reverse Shock Emission from Relativistic Jets with Arbitrary Angular and Stratified Radial Profiles, ApJ 990, 110 (2025), arXiv:2507.15311 [astro-ph.HE]
Pith/arXiv arXiv 2025
-
[60]
E. Ramirez-Ruiz and N. M. Lloyd-Ronning, Beam mod- els for gamma-ray bursts sources: outflow structure, kinematics and emission mechanisms, New A7, 197 (2002), arXiv:astro-ph/0203447 [astro-ph]
Pith/arXiv arXiv 2002
-
[61]
J. C. McKinney, General relativistic magnetohydrody- namic simulations of the jet formation and large-scale propagation from black hole accretion systems, MNRAS 368, 1561 (2006), arXiv:astro-ph/0603045 [astro-ph]
Pith/arXiv arXiv 2006
-
[62]
S. S. Komissarov, N. Vlahakis, A. K¨ onigl, and M. V. Barkov, Magnetic acceleration of ultrarelativistic jets in gamma-ray burst sources, MNRAS394, 1182 (2009), arXiv:0811.1467 [astro-ph]
Pith/arXiv arXiv 2009
-
[63]
D. K. Desai, L. Combi, D. M. Siegel, and B. D. Metzger, Relativistic jets from millisecond proto- magnetars, arXiv e-prints , arXiv:2601.07918 (2026), arXiv:2601.07918 [astro-ph.HE]
arXiv 2026
-
[64]
B. J. Morsony, D. Lazzati, and M. C. Begelman, Tem- poral and Angular Properties of Gamma-Ray Burst Jets Emerging from Massive Stars, ApJ665, 569 (2007), arXiv:astro-ph/0609254 [astro-ph]
Pith/arXiv arXiv 2007
-
[65]
O. Bromberg, E. Nakar, T. Piran, and R. Sari, The Propagation of Relativistic Jets in External Media, ApJ 740, 100 (2011), arXiv:1107.1326 [astro-ph.HE]
Pith/arXiv arXiv 2011
-
[66]
O. Gottlieb, The Landscape of Collapsar Outflows: Structure, Signatures, and Origins of Einstein Probe Relativistic Supernova Transients, ApJ992, L3 (2025), arXiv:2509.04551 [astro-ph.HE]
arXiv 2025
-
[67]
P. C. Duffell and A. I. MacFadyen, From Engine to Af- terglow: Collapsars Naturally Produce Top-heavy Jets and Early-time Plateaus in Gamma-Ray Burst After- glows, ApJ806, 205 (2015), arXiv:1407.8250 [astro- ph.HE]
Pith/arXiv arXiv 2015
-
[68]
A. Tchekhovskoy, J. C. McKinney, and R. Narayan, Simulations of ultrarelativistic magnetodynamic jets from gamma-ray burst engines, MNRAS388, 551 (2008), arXiv:0803.3807 [astro-ph]
Pith/arXiv arXiv 2008
-
[69]
B. Zhang, X. Dai, N. M. Lloyd-Ronning, and P. M´ esz´ aros, Quasi-universal Gaussian Jets: A Unified Picture for Gamma-Ray Bursts and X-Ray Flashes, ApJ 601, L119 (2004), arXiv:astro-ph/0311190 [astro-ph]
Pith/arXiv arXiv 2004
-
[70]
W. Xie, W.-H. Lei, Y.-C. Zou, D.-X. Wang, Q. Wu, and J.-Z. Wang, A two-component jet model based on the Blandford-Znajek and Blandford-Payne processes, Re- search in Astronomy and Astrophysics12, 817 (2012), arXiv:1202.5024 [astro-ph.HE]
Pith/arXiv arXiv 2012
-
[71]
J. Granot, Afterglow Light Curves from Impulsive Rel- ativistic Jets with an Unconventional Structure, ApJ 631, 1022 (2005), arXiv:astro-ph/0504254 [astro-ph]
Pith/arXiv arXiv 2005
-
[72]
F. Peng, A. K¨ onigl, and J. Granot, Two-Component Jet Models of Gamma-Ray Burst Sources, ApJ626, 966 (2005)
2005
-
[73]
H. Pedersen, A. O. Jaunsen, T. Grav, R. Østensen, M. I. Andersen, M. Wold, H. Kristen, A. Broeils, M. N¨ aslund, C. Fransson, M. Lacy, A. J. Castro-Tirado, J. Goros- abel, J. M. Rodr´ ıguez Espinosa, A. M. P´ erez, C. Wolf, R. Fockenbrock, J. Hjorth, P. Muhli, P. Hakala, L. Piro, M. Feroci, E. Costa, L. Nicastro, E. Palazzi, F. Frontera, L. Monaldi, and J...
Pith/arXiv arXiv 1998
-
[74]
D. A. Frail, E. Berger, T. Galama, S. R. Kulkarni, G. H. Moriarty-Schieven, G. G. Pooley, R. Sari, D. S. Shep- herd, G. B. Taylor, and F. Walter, The Enigmatic Ra- dio Afterglow of GRB 991216, ApJ538, L129 (2000), arXiv:astro-ph/0003138 [astro-ph]
Pith/arXiv arXiv 2000
-
[75]
Berger, S
E. Berger, S. R. Kulkarni, G. Pooley, D. A. Frail, V. McIntyre, R. M. Wark, R. Sari, A. M. Soderberg, D. W. Fox, S. Yost, and P. A. Price, A common ori- gin for cosmic explosions inferred from calorimetry of grb030329, Nature426, 154 (2003)
2003
- [76]
-
[77]
Chen, X.-G
L.-J. Chen, X.-G. Wang, Q. Wang, Z.-M. Zhou, W. Zheng, Y.-Z. Chen, and E.-W. Liang, GRB 191221B: The Two-component Jet with Forward and Reverse Shock, ApJ972, 158 (2024)
2024
-
[78]
J. K. Leung, G. E. Anderson, A. J. van der Horst, C. Morley, B. Schneider, F. D. Colle, O. S. Salafia, G. Ghirlanda, S. L. Chastain, A. J. Goodwin, A. Gu- lati, L. Rhodes, S. D. Ryder, A. A. Chrimes, V. D’Elia, M. de Bony de Lavergne, M. D. Pasquale, A. de Ugarte Postigo, D. H. Hartmann, B. P. Gom- pertz, A. J. Levan, T. Murphy, G. P. Rowell, T. D. Russel...
arXiv 2025
-
[79]
Y. Sato, K. Murase, Y. Ohira, S. Inoue, and R. Ya- mazaki, Two-component jet model for the afterglow emission of GRB 201216C and GRB 221009A and impli- cations for jet structure of very-high-energy gamma-ray bursts, Journal of High Energy Astrophysics48, 100415 (2025), arXiv:2502.19051 [astro-ph.HE]
Pith/arXiv arXiv 2025
-
[80]
Y. Sato, K. Obayashi, B. Theodre Zhang, S. J. Tanaka, K. Murase, Y. Ohira, and R. Yamazaki, Synchrotron self-compton emission in the two-component jet model for gamma-ray bursts, Journal of High Energy Astro- physics37, 51 (2023)
2023
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.