阋卫一 (Chinese Wikipedia)

Analysis of information sources in references of the Wikipedia article "阋卫一" in Chinese language version.

refsWebsite

Global rank Chinese rank

13web.archive.org

1^st place

5harvard.edu

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57^th place

3arxiv.org

69^th place

254^th place

3doi.org

2^nd place

23^rd place

2nih.gov

4^th place

5^th place

2abc.net.au

139^th place

367^th place

2skytonight.com

low place

2caltech.edu

887^th place

966^th place

1johnstonsarchive.net

9,017^th place

7,655^th place

1upmc.fr

low place

1arizona.edu

1,592^nd place

1,417^th place

1pluggd.tv

low place

abc.net.au

Zabarenko, D. Planet Xena has moon called Gabrielle. Australian Broadcasting Corporation. 2005-10-03 [2008-03-09]. （原始内容存档于2017-04-08）.
Ingham, R. 'Tenth planet' Xena bigger than Pluto. Australian Broadcasting Corporation. 2006-02-02 [2008-03-09]. （原始内容存档于2016-06-03）.

arizona.edu

lpl.arizona.edu

Tidal Evolution of Dysnomia, Satellite of the Dwarf Planet Eris By Richard Greenberga,* and Rory Barnesa (PDF). [2013-11-02]. （原始内容存档 (PDF)于2013-11-03）.

arxiv.org

Brown, M. E.; et al.. Satellites of the Largest Kuiper Belt Objects (PDF). Astrophysical Journal Letters. 2006, 639 (1): L43 [2011-10-19]. Bibcode:2006ApJ...639L..43B. arXiv:astro-ph/0510029 . doi:10.1086/501524. （原始内容存档 (PDF)于2018-09-28）.
Santos-Sanz, P.; et al.. "TNOs are Cool": A Survey of the Transneptunian Region IV. Size/albedo characterization of 15 scattered disk and detached objects observed with Herschel Space Observatory-PACS. 2012. arXiv:1202.1481  [astro-ph.EP].
米高·布朗; et al. 最大柯伊伯带天體的衛星（Satellites of the largest Kuiper belt objects） (PDF). Astrophys.J. 2006, 639 (L43) [2006-09-14].
arXiv:astro-ph/0510029
. （原始内容存档 (PDF)于2019-07-13）.

caltech.edu

web.gps.caltech.edu

Brown, M. E.; et al.. Satellites of the Largest Kuiper Belt Objects (PDF). Astrophysical Journal Letters. 2006, 639 (1): L43 [2011-10-19]. Bibcode:2006ApJ...639L..43B. arXiv:astro-ph/0510029 . doi:10.1086/501524. （原始内容存档 (PDF)于2018-09-28）.

gps.caltech.edu

Brown, M. E. Dysnomia, the moon of Eris. Caltech. 2007-06-14 [2011-07-03]. （原始内容存档于2013-12-26）.

doi.org

Brown, M. E.; et al.. Satellites of the Largest Kuiper Belt Objects (PDF). Astrophysical Journal Letters. 2006, 639 (1): L43 [2011-10-19]. Bibcode:2006ApJ...639L..43B. arXiv:astro-ph/0510029 . doi:10.1086/501524. （原始内容存档 (PDF)于2018-09-28）.
Brown, M. E.; Schaller, E. L. The Mass of Dwarf Planet Eris. Science. 2007, 316 (5831): 1585. Bibcode:2007Sci...316.1585B. PMID 17569855. doi:10.1126/science.1139415.
Sicardy, B.; et al.. A Pluto-like radius and a high albedo for the dwarf planet Eris from an occultation (PDF). Nature. 2011, 478 (7370): 493–496 [2013-11-02]. Bibcode:2011Natur.478..493S. PMID 22031441. doi:10.1038/nature10550. （原始内容存档 (PDF)于2013-11-04）.

harvard.edu

ui.adsabs.harvard.edu

Brown, M. E.; et al.. Satellites of the Largest Kuiper Belt Objects (PDF). Astrophysical Journal Letters. 2006, 639 (1): L43 [2011-10-19]. Bibcode:2006ApJ...639L..43B. arXiv:astro-ph/0510029 . doi:10.1086/501524. （原始内容存档 (PDF)于2018-09-28）.
Brown, M. E.; Schaller, E. L. The Mass of Dwarf Planet Eris. Science. 2007, 316 (5831): 1585. Bibcode:2007Sci...316.1585B. PMID 17569855. doi:10.1126/science.1139415.
Sicardy, B.; et al.. A Pluto-like radius and a high albedo for the dwarf planet Eris from an occultation (PDF). Nature. 2011, 478 (7370): 493–496 [2013-11-02]. Bibcode:2011Natur.478..493S. PMID 22031441. doi:10.1038/nature10550. （原始内容存档 (PDF)于2013-11-04）.

cbat.eps.harvard.edu

Green, D. W. E. S/2005 (2003 UB₃₁₃) 1. IAU Circular. 2005-10-04, 8610 [2012-01-12]. （原始内容存档于2018-11-04）.
Green, D. W. E. (134340) Pluto, (136199) Eris, and (136199) Eris I (Dysnomia). IAU Circular. 2006-09-13, 8747 [2012-01-12]. （原始内容存档 (PDF)于2007-02-05）.

johnstonsarchive.net

Johnston, W. R. (136199) Eris and Dysnomia. Johnston's Archive. 2008-12-30 [2012-04-12]. （原始内容存档于2018-10-22）.

nih.gov

ncbi.nlm.nih.gov

Brown, M. E.; Schaller, E. L. The Mass of Dwarf Planet Eris. Science. 2007, 316 (5831): 1585. Bibcode:2007Sci...316.1585B. PMID 17569855. doi:10.1126/science.1139415.
Sicardy, B.; et al.. A Pluto-like radius and a high albedo for the dwarf planet Eris from an occultation (PDF). Nature. 2011, 478 (7370): 493–496 [2013-11-02]. Bibcode:2011Natur.478..493S. PMID 22031441. doi:10.1038/nature10550. （原始内容存档 (PDF)于2013-11-04）.

pluggd.tv

Julia Sweeney and Michael E. Brown. Hammer Conversations: KCET podcast. 42 min 12 sec. 2007 [2008-06-28]. （原始内容存档于2008-06-26）.

skytonight.com

Tytell, D. All Hail Eris and Dysnomia. Sky & Telescope. 2006-09-14 [2006-12-30]. （原始内容存档于2006-10-19）.
米高·布朗有關迪絲諾美亞名字的解釋. [2006-09-15]. （原始内容存档于2006-10-19）.

upmc.fr

hal.upmc.fr

Sicardy, B.; et al.. A Pluto-like radius and a high albedo for the dwarf planet Eris from an occultation (PDF). Nature. 2011, 478 (7370): 493–496 [2013-11-02]. Bibcode:2011Natur.478..493S. PMID 22031441. doi:10.1038/nature10550. （原始内容存档 (PDF)于2013-11-04）.

web.archive.org

Brown, M. E.; et al.. Satellites of the Largest Kuiper Belt Objects (PDF). Astrophysical Journal Letters. 2006, 639 (1): L43 [2011-10-19]. Bibcode:2006ApJ...639L..43B. arXiv:astro-ph/0510029 . doi:10.1086/501524. （原始内容存档 (PDF)于2018-09-28）.
Johnston, W. R. (136199) Eris and Dysnomia. Johnston's Archive. 2008-12-30 [2012-04-12]. （原始内容存档于2018-10-22）.
Brown, M. E. Dysnomia, the moon of Eris. Caltech. 2007-06-14 [2011-07-03]. （原始内容存档于2013-12-26）.
Green, D. W. E. S/2005 (2003 UB₃₁₃) 1. IAU Circular. 2005-10-04, 8610 [2012-01-12]. （原始内容存档于2018-11-04）.
Green, D. W. E. (134340) Pluto, (136199) Eris, and (136199) Eris I (Dysnomia). IAU Circular. 2006-09-13, 8747 [2012-01-12]. （原始内容存档 (PDF)于2007-02-05）.
Zabarenko, D. Planet Xena has moon called Gabrielle. Australian Broadcasting Corporation. 2005-10-03 [2008-03-09]. （原始内容存档于2017-04-08）.
Ingham, R. 'Tenth planet' Xena bigger than Pluto. Australian Broadcasting Corporation. 2006-02-02 [2008-03-09]. （原始内容存档于2016-06-03）.
Sicardy, B.; et al.. A Pluto-like radius and a high albedo for the dwarf planet Eris from an occultation (PDF). Nature. 2011, 478 (7370): 493–496 [2013-11-02]. Bibcode:2011Natur.478..493S. PMID 22031441. doi:10.1038/nature10550. （原始内容存档 (PDF)于2013-11-04）.
米高·布朗; et al. 最大柯伊伯带天體的衛星（Satellites of the largest Kuiper belt objects） (PDF). Astrophys.J. 2006, 639 (L43) [2006-09-14].
arXiv:astro-ph/0510029
. （原始内容存档 (PDF)于2019-07-13）.
Tidal Evolution of Dysnomia, Satellite of the Dwarf Planet Eris By Richard Greenberga,* and Rory Barnesa (PDF). [2013-11-02]. （原始内容存档 (PDF)于2013-11-03）.
Tytell, D. All Hail Eris and Dysnomia. Sky & Telescope. 2006-09-14 [2006-12-30]. （原始内容存档于2006-10-19）.
米高·布朗有關迪絲諾美亞名字的解釋. [2006-09-15]. （原始内容存档于2006-10-19）.
Julia Sweeney and Michael E. Brown. Hammer Conversations: KCET podcast. 42 min 12 sec. 2007 [2008-06-28]. （原始内容存档于2008-06-26）.