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Record W4405032760 · doi:10.3847/1538-4357/ad991d

An Enigmatic PeVatron in an Area around H <scp>ii</scp> Region G35.6−0.5

2025· article· en· W4405032760 on OpenAlexfundno aff
Z. Cao, F Aharonian, Axikegu, Yuting Bai, Yiwang Bao, D. Bastieri, Xiao-Jun Bi, Y.J Bi, W Bian, A.V Bukevich, Qin Cao, Weiling Cao, Zhe Cao, J. F. Chang, A.M Chen, Bingqiu Chen, E.S Chen, Hua-Xing Chen, Liang Chen, Lin Chen, Long Chen, M.J Chen, M.L Chen, Qin Chen, Shengyong Chen, Shaw H. Chen, S. Z. Chen, T. L. Chen, Yang Chen, Na Cheng, Y.D Cheng, Micheline C. Chu, Maxwell Cui, S. W. Cui, X.H Cui, Y. D. Cui, B. Z. Dai, Zi-Gao Dai, Danzengluobu Danzengluobu, X.Q Dong, K. K. Duan, Junhui Fan, Yi-Zhong Fan, Fang Ji, J. Fang, Kun Fang, C. Feng, Hua Feng, L. Feng, Shuo Feng, X.T Feng, Y. Feng, Y. L. Feng, S. Gabici, Bo Gao, C. D. Gao, Q. Gao, Wei Gao, M. M. Ge, T.T Ge, Li‐Sheng Geng, Gwenael Giacinti, G. Gong, Q. B. Gou, M. H. Gu, Fulai Guo, Jia Guo, Xu Guo, Y. Q. Guo, Yong Guo, Y. A. Han, O. A. Hannuksela, M Hasan, H. H. He, H. N. He, Jiangbiao He, Y. He, Y. K. Hor, Bowen Hou, Changbo Hou, X. T. Hou, H. B. Hu, Q. Hu, S. C. Hu, C. Huang, D.H Huang, T.Q Huang, Weidong Huang, X. T. Huang, X.Y Huang, Yongbo Huang, Yanyi Huang, X. L. Ji, H.Y Jia, Ke Jia, Hongbing Jiang, K. Jiang, Xiaojun Jiang, Z.J Jiang, Min Jin, M. M. Kang, I. Karpikov, D. Khangulyan, D. Kuleshov, K. Kurinov, Bing Li, C.M Li, Cheng Li, Cong Li, Duo Li, Li Fei, Haibo Li, Hancheng Li, Jian Li, Jie Li, Kai Li, Shaoquan Li, W.L Li, X.R. Li, Xin Li, Yuze Li, Zhe Li, Zhuo Li, En‐Wei Liang, Yun-Feng Liang, S.J Lin, Yun Liu, C Liu, Dantong Liu, D. Liu, Haiqing Liu, H.D Liu, Jie Liu, J.L Liu, M. Liu, Rui Liu, S.M Liu, Y. Liu, Yu‐Rong Liu, Quantian Luo, Yi Luo, H.K Lv, B.Q Ma, L.L Ma, Xinhua Ma, J. R. Mao, W. Mitthumsiri, Haowei Mu, Y. C. Nan, A. Neronov, K.C.Y Ng, L.J Ou, P. Pattarakijwanich, Z. Y. Pei, J.C Qi, Ming Qi, Bing-Qiang Qiao, J. J. Qin, Ahmed Raza, D. Ruffolo, A. Sáiz, M. A. Saeed, D. Semikoz, Lu Shao, O. Shchegolev, X.D Sheng, Fengchun Shu, H. C. Song, Yu.V Stenkin, V. I. Stepanov, Yanjing Su, D.X Sun, Q. N. Sun, X.N Sun, Zhifeng Sun, J. Takata, P. H. T. Tam, Q.W Tang, Ryan W. Tang, Z.B Tang, W. W. Tian, L.H Wan, C. Wang, C.B Wang, G.W Wang, Haigang Wang, H.H Wang, Jincheng Wang, Kai Wang, L.P Wang, L.Y Wang, Ping Wang, Ruikang K. Wang, Weiyang Wang, X.G. Wang, Xuefeng Wang, Yi Wang, Y.D Wang, Yun-Jiang Wang, Z.H. Wang, Z.X Wang, Zhen Wang, Z. Wang, D. M. Wei, Jun-Jie Wei, Yujie Wei, T. Wen, Chen Wu, H. R. Wu, Qi Wu, Sheng Wu, X.F Wu, Yong Wu, Shao-Qiang Xi, Jing Xia, G. M. Xiang, D. X. Xiao, G. Xiao, Y. Xin, Yi Xing, D.R Xiong, D.L Xu, R.F Xu, Rui Xu, Weiwei Xu, L. Xue, D.H Yan, Jing‐Zhi Yan, Ting Yan, Chul Woo Yang, C. Y. Yang, Fan Yang, Fang Yang, Lili Yang, Mo Yang, Ruizhi Yang, W.X Yang, Y. Yao, Z. G. Yao, L. Q. Yin, N. Yin, X. H. You, Z. Y. You, Yi Yu, Hui Yue, Houdun Zeng, T. X. Zeng, Wen Zeng, M. Zha, Bin‐Bin Zhang, Fengming Zhang, Hua Zhang, H.M Zhang, Hengyun Zhang, J.L Zhang, Li Zhang, Peng Zhang, P.P Zhang, Rui Zhang, Shengbai Zhang, S.R Zhang, S.S Zhang, Xiao Zhang, X.P Zhang, Y.F Zhang, Yi Zhang, Yong Zhang, Bo Zhao, J. Zhao, Lei Zhao, S. P. Zhao, Xinsheng Zhao, F. Zheng, Bo Zhou, H. Zhou, J. N. Zhou, Mingfei Zhou, Ping Zhou, Ruijie Zhou, X. X. Zhou, Baohua Zhu, C. G. Zhu, F. R. Zhu, Hao Zhu, Kejun Zhu, Yuan-Chuan Zou, X. Zuo

Bibliographic record

VenueThe Astrophysical Journal · 2025
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstrophysics and Cosmic Phenomena
Canadian institutionsnot available
FundersNational Key Research and Development Program of ChinaNatural Sciences and Engineering Research Council of CanadaNational Research Council of ThailandNational Science and Technology Development AgencyNational Natural Science Foundation of ChinaEuropean Space AgencyNational Science Foundation
KeywordsPhysicsAstrophysicsCosmic rayObservatorySupernova remnantSpectral indexSupernovaMolecular cloudAstronomySpectral lineStars

Abstract

fetched live from OpenAlex

Abstract Identifying Galactic PeVatrons (PeV particle accelerators) from ultrahigh-energy (UHE, >100 TeV) γ-ray sources plays a crucial role in revealing the origin of Galactic cosmic rays. The UHE source 1LHAASO J1857+0203u is suggested to be associated with HESS J1858+020, which may be attributed to the possible PeVatron candidate supernova remnant (SNR) G35.6−0.4 or H ii region G35.6−0.5. We perform detailed analysis on the very-high-energy and UHE γ-ray emissions toward this region with data from the Large High Altitude Air Shower Observatory (LHAASO). 1LHAASO J1857+0203u is detected with a significance of 11.6σ above 100 TeV, indicating the presence of a PeVatron. It has an extent of ∼0 . ° 18 with a power-law (PL) spectral index of ∼2.5 at 1–25 TeV and pointlike emission with a PL spectral index of ∼3.2 above 25 TeV. Using archival CO and H i data, we identify some molecular and atomic clouds that may be associated with the TeV γ-ray emissions. Our modeling indicates that the TeV γ-ray emissions are unlikely to arise from clouds illuminated by the protons that escaped from SNR G35.6−0.4. In the scenario in which H ii region G35.6−0.5 could accelerate particles to the UHE band, the observed GeV–TeV γ-ray emission could be well explained by a hadronic model with a PL spectral index of ∼2.0 and cutoff energy of ∼450 TeV. However, an origin in an evolved pulsar wind nebula cannot be ruled out.

Fetched live from OpenAlex and de-inverted. Abstracts are not stored in this database: the inverted indexes are 8.6 GB of the frame’s 9.3 GB of text, and the host has 13 GB free.

How this classification was reachedexpand

Full frame machine prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. The Gemma side is a direct model label for every work in the frame, read from the title-only record. The Codex side is a classifier learned from the 10,348 direct Codex labels and calibrated to design-weighted sample rates; fields without enough sample support carry no Codex call. Candidate is the union of the two sides; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels.

metaresearch head score (Codex)0.000
metaresearch head score (Gemma)0.000
Version: metacan-v3-hybrid-931329e0061cValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Observational · Consensus signal: Observational
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.011
Threshold uncertainty score0.023

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0010.000
Science and technology studies0.0000.000
Scholarly communication0.0000.000
Open science0.0000.000
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0020.000

Machine scores (provisional)

The two teacher heads of the student model, read on this work. A score orders the frame for review; it never asserts a category, and the validation status ships verbatim with every row.

Baseline scores from an immature model (maturity gate not passed, 7 training rounds). Scores rank; they never assert a category.

Opus teacher head0.011
GPT teacher head0.241
Teacher spread0.231 · how far apart the two teachers sit on this one work
Validation statusscore_only:v0-immature-baseline · verbatim from the scoring run: score_only means the number may rank works, and no category label ships from it

Classification

machine, unvalidated

Machine predicted; a candidate call from one source (direct Gemma or distilled Codex), not a consensus.

The models applied no category: nothing in the taxonomy fit this work.
Study designObservational
Domainnot available
GenreEmpirical

How this classification was reached, model by model and score by score, is at the end of the page under "How this classification was reached".

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Citations0
Published2025
Admission routes1
Has abstractyes

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