MACS0416.1-2403

MACS J0416.1-2403是一個紅移值 z=0.397 的星系團，位於波江座^[1]。200 kpc範圍內質量為太陽的160兆倍。如果它的半徑是950 kpc，總質量則是太陽的1.15 x 10¹⁵倍^[2]。該星系團由大質量星系團巡天（英語：MAssive Cluster Survey）發現（Massive Cluster Survey, MACS）^[3][4]。該星系團可使位於它後方遠處的星系產生重力透鏡效應，使一個星系產生多個影像^[5][6]。

哈勃太空望遠鏡拍攝的星系團MCS J0416.1–2403。

參考資料

1. Colour image of galaxy cluster MCS J0416.1–2403. ESA/Hubble. 24 July 2014 [6 September 2015]. （原始內容存檔於2020-10-25）.
2. Jauzac, Mathilde; Eric Jullo; Dominique Eckert; Harald Ebeling; Johan Richard; Marceau Limousin; et al. Hubble Frontier Fields: The Geometry and Dynamics of the Massive Galaxy Cluster Merger MACSJ0416.1-2403. arXiv. 23 June 2014 [25 July 2014]. （原始內容存檔於2019-09-30）.
3. Mann, Andrew; Harald Ebeling. X-ray-optical classification of cluster mergers and the evolution of the cluster merger fraction. March 2012 [2015-09-06]. （原始內容存檔於2018-08-08）.
4. Ebeling, Harald; Alastair Edge; J. Patrick Henry. MACS: A Quest for the Most Massive Galaxy Clusters in the Universe. June 2001 [3 February 2015]. （原始內容存檔於2019-03-30）.
5. Diego, Jose M. Free Form Lensing Implications for the Collision of Dark Matter and Gas in the Frontier Fields Cluster MACSJ0416.1-2403. 4 June 2014 [2015-09-06]. （原始內容存檔於2018-08-08）.
6. New mass map of a distant galaxy cluster is the most precise yet. 24 July 2014 [25 July 2014]. （原始內容存檔於2019-08-24）.