(55637) 2002 UX25 (Greek Wikipedia)

Analysis of information sources in references of the Wikipedia article "(55637) 2002 UX25" in Greek language version.

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69^th place

279^th place

18^th place

57^th place

9,017^th place

7,806^th place

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low place

arxiv.org

S. Fornasier, E. Lellouch, T. Müller, P. Santos-Sanz, P. Panuzzo, C. Kiss, T. Lim, M. Mommert, D. Bockelée-Morvan, E. Vilenius, J. Stansberry, G.P. Tozzi, S. Mottola, A. Delsanti, J. Crovisier, R. Duffard, F. Henry, P. Lacerda, A. Barucci, A. Gicquel (2013). «TNOs are Cool: A survey of the trans-Neptunian region. VIII. Combined Herschel PACS and SPIRE observations of 9 bright targets at 70--500 micron».
arXiv:1305.0449v2
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John Stansberry, Will Grundy, Mike Brown, Dale Cruikshank, John Spencer, David Trilling, Jean-Luc Margot (2007). «Physical Properties of Kuiper Belt and Centaur Objects: Constraints from Spitzer Space Telescope».
arXiv:astro-ph/0702538
[astro-ph]
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Brown, M. E. (2013). «The Density of Mid-sized Kuiper Belt Object 2002 UX25 and the Formation of the Dwarf Planets». Astrophysical Journal Letters 778 (2). doi:10.1088/2041-8205/778/2/L34. http://adsabs.harvard.edu/abs/2013ApJ...778L..34B.
Rousselot, P.; Petit, J.-M.; Poulet, F.; Sergeev, A. Photometric study of Centaur (60558) 2000 EC98 and trans-neptunian object (55637) 2002 UX25 at different phase angles, Icarus, 176, (2005) pp. 478–491.Abstract.