Johnson, H. M.; Wright, C. D. Predicted infrared brightness of stars within 25 parsecs of the sun. Astrophysical Journal Supplement Series (abstract)使用|format=需要含有|url= (帮助). 1983, 53: 643–711. Bibcode:1983ApJS...53..643J. doi:10.1086/190905.引文使用过时参数coauthors (帮助); 使用|accessdate=需要含有|url= (帮助)—see page 673.
Bean, Jacob L.; Benedict, G. Fritz; Endl, Michael. Metallicities of M Dwarf Planet Hosts from Spectral Synthesis. The Astrophysical Journal (abstract)使用|format=需要含有|url= (帮助). 2006, 653 (1): L65–L68. Bibcode:2006ApJ...653L..65B. doi:10.1086/510527.引文使用过时参数coauthors (帮助)—for the metallicity, note that or 44%
Schneider, J. Notes for star GJ 436. The Extrasolar Planets Encyclopaedia. [2008-09-07]. (原始内容存档于2012-05-24).
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Johnson, H. M.; Wright, C. D. Predicted infrared brightness of stars within 25 parsecs of the sun. Astrophysical Journal Supplement Series (abstract)使用|format=需要含有|url= (帮助). 1983, 53: 643–711. Bibcode:1983ApJS...53..643J. doi:10.1086/190905.引文使用过时参数coauthors (帮助); 使用|accessdate=需要含有|url= (帮助)—see page 673.
Bean, Jacob L.; Benedict, G. Fritz; Endl, Michael. Metallicities of M Dwarf Planet Hosts from Spectral Synthesis. The Astrophysical Journal (abstract)使用|format=需要含有|url= (帮助). 2006, 653 (1): L65–L68. Bibcode:2006ApJ...653L..65B. doi:10.1086/510527.引文使用过时参数coauthors (帮助)—for the metallicity, note that or 44%