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Journal of High Energy Astrophysics
基本信息
期刊名称 Journal of High Energy Astrophysics
J HIGH ENERGY ASTROP
期刊ISSN 2214-4048
期刊官方网站 https://www.journals.elsevier.com/journal-of-high-energy-astrophysics
是否OA
出版商 Elsevier BV
出版周期
始发年份
年文章数 9
最新影响因子 3.8(2022)  scijournal影响因子  greensci影响因子
中科院SCI期刊分区
大类学科 小类学科 Top 综述
地学天文4区 ASTRONOMY & ASTROPHYSICS 天文与天体物理4区
CiteScore
CiteScore排名 CiteScore SJR SNIP
学科 排名 百分位 2.61 1.365 0.640
Physics and Astronomy
Astronomy and Astrophysics
25 / 76 67%
补充信息
自引率 0.00%
H-index 11
SCI收录状况 Science Citation Index Expanded
官方审稿时间
网友分享审稿时间 数据统计中,敬请期待。
PubMed Central (PML) http://www.ncbi.nlm.nih.gov/nlmcatalog?term=2214-4048%5BISSN%5D
投稿指南
期刊投稿网址 https://www.evise.com/profile/#/JHEAP/login
收稿范围

Driven by observations conducted with unprecedented experimental facilities and satellites, the last few years have brought a plethora of historic results at the high-energy end of the electromagnetic spectrum. These appeal to new theoretical efforts and multi-frequency investigations, which are altogether leading to a burst of new ideas, problems, and research directions.
High-energy astrophysics, a research field that connects astronomy, cosmology and particle physics, will continue to expand in the next decades with an increasing rate, additionally boosted by the forthcoming improvements in experimental detection precision.
The Journal of High Energy Astrophysics (JHEAp) is the first astrophysical journal that focuses on the study of highly energetic phenomena.
Pivoting on this general topic, and in the belief that boundaries in astronomy are naturally fading, JHEAp seeks the most impacting and scientifically sound papers, those generally crossing specialization fields and attracting the interest of astronomers at any wavelength.
The journal welcomes manuscripts on theoretical models, simulations, and observations of highly energetic astrophysical objects both in our Galaxy and beyond. Among those, black holes at all scales, neutron stars, pulsars and their nebula, binaries, novae and supernovae, their remnants, active galaxies, and clusters are just a few examples. The journal will consider research across the whole electromagnetic spectrum, as well as research using various messengers, such as gravitational waves or neutrinos. Effects of high-energy phenomena on cosmology and star-formation, results from dedicated surveys expanding the knowledge of extreme environments, and astrophysical implications of dark matter are also welcomed topics.
The journal adopts the commonly used single blind peer review system, during which the reviewer names are kept anonymous while the author or collaboration name is disclosed to the reviewers. In addition, the journal will introduce the possibility for papers to be refereed in a double blind process, in order to ensure and promote quality. A dedicated reviewer pool, an active Editorial Board, a fast and traceable online submission procedure, and appropriate reviewer incentives will further ensure a rapid and strict peer reviewing process.
JHEAp has no page charges and has a delayed open access model. All color figures are free for the online version and a selection of printed color figures costs may be waived at the Editor's discretion. JHEAp will be indexed in all major systems such as Scopus and the SAO/NASA Astrophysics Data System (ADS).

收录体裁
Original research papers, reviews, special issue papers
投稿指南 https://www.elsevier.com/journals/journal-of-high-energy-astrophysics/2214-4048/guide-for-authors
投稿模板
参考文献格式 https://www.elsevier.com/journals/journal-of-high-energy-astrophysics/2214-4048/guide-for-authors
编辑信息
Editor-in-Chief
Institute of Space Sciences, Barcelona, Spain 
Associate Editors
North-West University, South Africa 
INAF-Istituto Nazionale di Astrofisica, Milano, Italy 

Michael Carini

Western Kentucky University, Kentucky, USA 
The University of Hong Kong, Hong Kong 
Università degli Studi di Milano-Bicocca, Milano, Italy 
Nagoya University, Nagoya, Japan 
Leopold-Franzens-Universität Innsbruck, Innsbruck, Austria  Gamma-ray astrophysics, cosmic ray physics (sub-UHECR), multi-messenger astronomy, multi-waveband identification
University of Nevada at Las Vegas, Las Vegas, Nevada, USA 
Chinese Academy of Sciences (CAS), Beijing, China  High energy astrophysics, including compact objects, relativistic outflows, gamma-ray bursts, and AGNs, data analysis methodology and space instrumentation


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