Wikipedia:Featured article candidates/61 Cygni/archive1: Difference between revisions
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:::: It is part of a PDF document. Have you tried reading the [http://fr.arxiv.org/abs/1307.7038 arXiv article] and scrolling down to near the end? [[User:Praemonitus|Praemonitus]] ([[User talk:Praemonitus|talk]]) 21:22, 20 March 2015 (UTC)
:::::I read [http://fr.arxiv.org/pdf/1307.7038v1 it] but it seems to me like there aren't any IR excess as they say much about GJ 581, GJ 667C, and GJ 876 M-dwarfs. GJ 820 has its name only in the table. So should I include in the article that there aren't any IR excess? Plus, I couldn't deduce from them that there are any habitable zones either. -[[User:The Herald|The Herald]] [[User talk:The Herald|<sup style="margin-left:0.5px">''the joy of the LORD''</sup>]][[Special:Contributions/The Herald|<sub style="margin-left:-47.5px">''my strength''</sub>]] 04:27, 21 March 2015 (UTC)
:::::: Yes, the absence of a detectable IR excess is still of interest because it tells the reader something about the state of the system. The reference for the habitability radii is in a separate bullet above. [[User:Praemonitus|Praemonitus]] ([[User talk:Praemonitus|talk]])
Thanks. [[User:Praemonitus|Praemonitus]] ([[User talk:Praemonitus|talk]]) 16:20, 18 March 2015 (UTC)
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