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).
在用前所未有的实验设备和卫星进行的观测的推动下，过去几年在电磁频谱的高能端带来了大量的历史结果。这些都需要新的理论努力和多频率的调查，这将导致一系列新的想法、问题和研究方向。高能天体物理学是一个连接天文学、宇宙学和粒子物理学的研究领域，在未来几十年内将继续以越来越快的速度扩展，此外，实验探测精度的提高也将推动这一领域的发展。《高能天体物理学杂志》（JHEPA）是第一本专注于高能现象研究的天体物理学杂志。围绕这一总体主题，并相信天文学的边界自然正在消失，JHEPA寻求最具影响力和科学性的论文，这些论文通常跨越专业领域，并吸引天文学家在任何波长的兴趣。该杂志欢迎有关我们银河系和其他星系中高能天体的理论模型、模拟和观测的手稿。其中，各种尺度的黑洞、中子星、脉冲星及其星云、双星、新星和超新星、它们的残骸、活动星系和星团只是几个例子。该杂志将考虑对整个电磁频谱的研究，以及使用各种信使的研究，如引力波或中微子。高能现象对宇宙学和恒星形成的影响，扩大极端环境知识的专门调查结果，以及暗物质的天体物理影响也受到欢迎。期刊采用常用的单盲同行评审制度，评审人姓名匿名，作者或协作人姓名向评审人公开。此外，该期刊还将介绍在双盲流程中引用论文的可能性，以确保和提高质量。一个专门的评审员库、一个活跃的编辑委员会、一个快速和可追踪的在线提交程序以及适当的评审员激励措施将进一步确保快速和严格的同行评审过程。JHEAP没有页面费用，并且有一个延迟的开放访问模型。所有颜色数字免费提供在线版本，编辑可自行决定免除印刷颜色数字的费用。jheap将在所有主要系统中建立索引，如scopus和sao/nasa天体物理数据系统（ADS）。
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