这篇文章首次提出对于磁化中子星加热的极度明亮的超新星，因为晚期存在较强的伽马射线与X射线泄露，将比不考虑这些泄露的情形暗。文章投出八天，编辑部就初步接受文章，按照审稿人意见，小修了几处，被正式接受。

ApJ96936R2 Decision Letter

November 18, 2014

Nanjing University
School of Astronomy and Space Science
22 Hankou Road, Nanjing 210093, Jiangsu Province, CHINA
Nanjing, Jiangsu 210093
China

Title: Superluminous Supernovae Powered by Magnetars: Late-time Lightcurves and Hard Emission Leakage, ApJ96936R2

I am happy to report that the above paper is accepted for publication in The Astrophysical Journal.

I am sending the accepted version to the ApJ editorial office. Correspondence concerning the logistical aspects of publishing this manuscript should be directed to apj@apj.usask.ca. If you have any additional questions concerning the scientific content of your manuscript, please direct them to me.

Sincerely,
Luigi Stella
Scientific Editor
The Astrophysical Journal
apjse@xx-xxxx.xxxx.xx

祝贺shanqin！

与这篇论文同时完成的还有另一篇同样篇幅的论文，尚未投稿，正准备投到ApJ，实际上这篇即将投出的文章的结果更早得出，但是我觉得另外一篇更加基础与重要，所以先修改投出哪一篇。

手上这篇只需要加几句比较强的结论就可以投到ApJ了。希望也能像之前那篇那么顺利。

第三篇已经初步完成结果，等第二篇投出后，立即开始写，争取元旦前投到ApJ或者AA（《天文学与天体物理学》，法）。

祝贺！

祝贺小王！

九年前来客栈，是小王
现在重新注册，是老王

恭喜贺喜！老小王前段时间还失落过一阵，现在终究还是雄起了。加油！

恭喜！继续加油！