Evidence map›Paper›PMID 41499505›Full record

ArticleScience advances2026

First submillimeter lights from Dome A: Tracing the carbon cycle in the feedback of massive stars.

Yan Gong, Jiaqiang Zhong, Yuan Ren, Yilong Zhang, Daizhong Liu, Yiping Ao, Qijun Yao, Wen Zhang, Wei Miao, Zhenhui Lin and 31 more

Abstract read
PubMed Full text at PMC Publisher
In one paragraph

Article in Science advances, 2026. The graph could read no effect estimate from its abstract, so it casts no vote on the map. Not yet cited in PubMed.

0numbers the graph read from it
0cells of the map it votes in
0citing papers in PubMed
–field-weighted citation impact
1 · What the graph read from it

What it found

Each row is one number read from the abstract, on the scale the paper reported it, with its interval. Left of the dashed line favours the treatment, right favours the comparator. Under each row is the sentence it came from. New to these charts? A ten-minute tutorial.

The abstract states no effect estimate the extractor could read, or names no intervention and outcome on the map, so this paper lights no cell and moves no belief. It is still indexed, cited and linked below.

2 · The registry

The trial behind it

Trials whose registry record cites this paper, or whose number appears in the abstract. A trial that started after this paper was published is citing it as background, not reporting it.

Neither the registry nor the abstract names a trial number. If this is a trial report, that itself is worth knowing.

3 · Its place in the literature

Who cites it

0 citing papers in PubMed.

No citing paper in PubMed yet.

4 · The record

Corrections and comments

PubMed lists nothing against this paper. Absence here is not a guarantee, only a check that was made.

5 · Who and what money

Authors and funding

41 authors.

Yan GongPurple Mountain Observatory and Key Laboratory of Radio Astronomy, Chinese Academy of Sciences, Nanjing 210008, China.ORCID 0000-0002-3866-414X
Jiaqiang ZhongPurple Mountain Observatory and Key Laboratory of Radio Astronomy, Chinese Academy of Sciences, Nanjing 210008, China.ORCID 0000-0002-2019-8291
Yuan RenPurple Mountain Observatory and Key Laboratory of Radio Astronomy, Chinese Academy of Sciences, Nanjing 210008, China.
Yilong ZhangPurple Mountain Observatory and Key Laboratory of Radio Astronomy, Chinese Academy of Sciences, Nanjing 210008, China.ORCID 0000-0002-0738-9528
Daizhong LiuPurple Mountain Observatory and Key Laboratory of Radio Astronomy, Chinese Academy of Sciences, Nanjing 210008, China.ORCID 0000-0001-9773-7479
Yiping AoPurple Mountain Observatory and Key Laboratory of Radio Astronomy, Chinese Academy of Sciences, Nanjing 210008, China.ORCID 0000-0003-3139-2724
Qijun YaoPurple Mountain Observatory and Key Laboratory of Radio Astronomy, Chinese Academy of Sciences, Nanjing 210008, China.
Wen ZhangPurple Mountain Observatory and Key Laboratory of Radio Astronomy, Chinese Academy of Sciences, Nanjing 210008, China.ORCID 0000-0001-6513-5932
Wei MiaoPurple Mountain Observatory and Key Laboratory of Radio Astronomy, Chinese Academy of Sciences, Nanjing 210008, China.ORCID 0000-0001-9062-9061
Zhenhui LinPurple Mountain Observatory and Key Laboratory of Radio Astronomy, Chinese Academy of Sciences, Nanjing 210008, China.ORCID 0009-0002-6559-7859
Wenying DuanPurple Mountain Observatory and Key Laboratory of Radio Astronomy, Chinese Academy of Sciences, Nanjing 210008, China.ORCID 0009-0005-6859-2537
Dong LiuPurple Mountain Observatory and Key Laboratory of Radio Astronomy, Chinese Academy of Sciences, Nanjing 210008, China.ORCID 0000-0002-5032-5650
Kangmin ZhouPurple Mountain Observatory and Key Laboratory of Radio Astronomy, Chinese Academy of Sciences, Nanjing 210008, China.ORCID 0000-0003-1247-1590
Jie LiuPurple Mountain Observatory and Key Laboratory of Radio Astronomy, Chinese Academy of Sciences, Nanjing 210008, China.ORCID 0000-0001-5664-4858
Zheng WangPurple Mountain Observatory and Key Laboratory of Radio Astronomy, Chinese Academy of Sciences, Nanjing 210008, China.
Junda JinPurple Mountain Observatory and Key Laboratory of Radio Astronomy, Chinese Academy of Sciences, Nanjing 210008, China.ORCID 0009-0004-5693-4870
Kun ZhangPurple Mountain Observatory and Key Laboratory of Radio Astronomy, Chinese Academy of Sciences, Nanjing 210008, China.
Feng WuPurple Mountain Observatory and Key Laboratory of Radio Astronomy, Chinese Academy of Sciences, Nanjing 210008, China.
Jinpeng LiPurple Mountain Observatory and Key Laboratory of Radio Astronomy, Chinese Academy of Sciences, Nanjing 210008, China.
Boliang LiuPurple Mountain Observatory and Key Laboratory of Radio Astronomy, Chinese Academy of Sciences, Nanjing 210008, China.
Xuan ZhangPurple Mountain Observatory and Key Laboratory of Radio Astronomy, Chinese Academy of Sciences, Nanjing 210008, China.
Zhengheng LuoPurple Mountain Observatory and Key Laboratory of Radio Astronomy, Chinese Academy of Sciences, Nanjing 210008, China.
Jiameng WangPurple Mountain Observatory and Key Laboratory of Radio Astronomy, Chinese Academy of Sciences, Nanjing 210008, China.
Huiqian HaoThe 54th Research Institute of China Electronics Technology Group Corporation, Shijiazhuang 050081, China.
Xingming LuThe 54th Research Institute of China Electronics Technology Group Corporation, Shijiazhuang 050081, China.
Shaoming XieThe 54th Research Institute of China Electronics Technology Group Corporation, Shijiazhuang 050081, China.
Jia QuanTechnical Institute of Physics and Chemistry, Chinese Academy of Sciences, Beijing 100190, China.
Yanjie LiuTechnical Institute of Physics and Chemistry, Chinese Academy of Sciences, Beijing 100190, China.
Jingtao LiangTechnical Institute of Physics and Chemistry, Chinese Academy of Sciences, Beijing 100190, China.ORCID 0000-0002-7397-4135
Xianjin DengMicrosystem and Terahertz Research Center, China Academy of Engineering Physics, Chengdu, Sichuan 610200, China.
Jun JiangMicrosystem and Terahertz Research Center, China Academy of Engineering Physics, Chengdu, Sichuan 610200, China.
Li LiMicrosystem and Terahertz Research Center, China Academy of Engineering Physics, Chengdu, Sichuan 610200, China.
Liang GuoChangchun Institute of Optics, Fine Mechanics and Physics, Chinese Academy of Sciences, Changchun 130033, China.
Tuo JiPolar Research Institute of China; Key Laboratory for Polar Science, MNR, Shanghai 200136, China.ORCID 0000-0002-9000-4915
Peng JiangPolar Research Institute of China; Key Laboratory for Polar Science, MNR, Shanghai 200136, China.ORCID 0000-0002-5387-7952
Yi ZhangShanghai Key Lab for Astrophysics, Shanghai Normal University, 100 Guilin Road, Shanghai 200234, China.
Chenggang ShuShanghai Key Lab for Astrophysics, Shanghai Normal University, 100 Guilin Road, Shanghai 200234, China.ORCID 0000-0003-1055-2039
Sudeep NeupaneMax-Planck-Institut für Radioastronomie, Auf dem Hügel 69, D-53121 Bonn, Germany.
Ruiqing MaoPurple Mountain Observatory and Key Laboratory of Radio Astronomy, Chinese Academy of Sciences, Nanjing 210008, China.
Shengcai ShiPurple Mountain Observatory and Key Laboratory of Radio Astronomy, Chinese Academy of Sciences, Nanjing 210008, China.
Jing LiPurple Mountain Observatory and Key Laboratory of Radio Astronomy, Chinese Academy of Sciences, Nanjing 210008, China.ORCID 0000-0001-6295-2398

Funding

No grant is acknowledged in the PubMed record.

6 · The paper itself

Abstract

The cycling of carbon between its ionized, atomic, and molecular phases shapes the chemical compositions and physical conditions of the interstellar medium (ISM). However, ground-based studies of the full carbon cycle have been limited by atmospheric absorption. Dome A, the most promising site for submillimeter astronomy, has long resisted successful submillimeter astronomical observations. Using the 60-centimeter Antarctic Terahertz Explorer, we present the first successful CO (4-3) and [CI] ([Formula: see text]) mapping observations of two archetypal triggered massive star-formation regions at Dome A. These data, together with archival [CII], provide the first complete characterization of all three carbon phases in these environments. We find elevated C

Identifiers

PMID41499505
PMCPMC12778048

What Socratic holds

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Read under generation 80e0d062 · epoch 390. Bibliography from PubMed, PubMed Central and OpenAlex; grants from NIH RePORTER; trial links from ClinicalTrials.gov; estimates, votes and beliefs from the Socratic graph.