S5 0014+81 (Chinese Wikipedia)

Analysis of information sources in references of the Wikipedia article "S5 0014+81" in Chinese language version.

refsWebsite

Global rank Chinese rank

18^th place

57^th place

1^st place

2^nd place

23^rd place

887^th place

966^th place

75^th place

140^th place

69^th place

254^th place

arxiv.org

Ghisellini, Gabriele; Foschini, Luigi; Volonteri, Marta; Ghirlanda, Giancarlo; et al. The blazar S5 0014+813: a real or apparent monster?. Monthly Notices of the Royal Astronomical Society. 14 Jul 2009, 399 (1): L24–L28. Bibcode:2009MNRAS.399L..24G. arXiv:0906.0575 . doi:10.1111/j.1745-3933.2009.00716.x. 17:53:24 GMT.

NED results for object S5 0014+81. NASA/IPAC EXTRAGALACTIC DATABASE. [2018-04-21]. （原始内容存档于2017-06-30）.

1.2×1.110⁴¹ watts. Kühr, Helmut; Liebert, James W.; Strittmatter, Peter A.; Schmidt, Gary D.; et al. The most luminous quasar - S5 0014+81. Astrophysical Journal. 15 December 1983 [2018-04-21]. Bibcode:1983ApJ...275L..33K. doi:10.1086/184166. （原始内容存档于2018-06-12）.
Ghisellini, Gabriele; Foschini, Luigi; Volonteri, Marta; Ghirlanda, Giancarlo; et al. The blazar S5 0014+813: a real or apparent monster?. Monthly Notices of the Royal Astronomical Society. 14 Jul 2009, 399 (1): L24–L28. Bibcode:2009MNRAS.399L..24G. arXiv:0906.0575 . doi:10.1111/j.1745-3933.2009.00716.x. 17:53:24 GMT.
Page, Don N. Particle Emission Rates from a Black Hole: Massless Particles from an Uncharged, Nonrotating Hole. Physical Review D. 1976, 13 (2): 198–206. Bibcode:1976PhRvD..13..198P. doi:10.1103/PhysRevD.13.198. See in particular equation (27).

1.2×1.110⁴¹ watts. Kühr, Helmut; Liebert, James W.; Strittmatter, Peter A.; Schmidt, Gary D.; et al. The most luminous quasar - S5 0014+81. Astrophysical Journal. 15 December 1983 [2018-04-21]. Bibcode:1983ApJ...275L..33K. doi:10.1086/184166. （原始内容存档于2018-06-12）.
Ghisellini, Gabriele; Foschini, Luigi; Volonteri, Marta; Ghirlanda, Giancarlo; et al. The blazar S5 0014+813: a real or apparent monster?. Monthly Notices of the Royal Astronomical Society. 14 Jul 2009, 399 (1): L24–L28. Bibcode:2009MNRAS.399L..24G. arXiv:0906.0575 . doi:10.1111/j.1745-3933.2009.00716.x. 17:53:24 GMT.
Page, Don N. Particle Emission Rates from a Black Hole: Massless Particles from an Uncharged, Nonrotating Hole. Physical Review D. 1976, 13 (2): 198–206. Bibcode:1976PhRvD..13..198P. doi:10.1103/PhysRevD.13.198. See in particular equation (27).

1.2×1.110⁴¹ watts. Kühr, Helmut; Liebert, James W.; Strittmatter, Peter A.; Schmidt, Gary D.; et al. The most luminous quasar - S5 0014+81. Astrophysical Journal. 15 December 1983 [2018-04-21]. Bibcode:1983ApJ...275L..33K. doi:10.1086/184166. （原始内容存档于2018-06-12）.

The Milky Way absolute visual magnitude is -20.6. Huchra, John P. The Properties of Galaxies. harvard.edu. Harvard-Smithsonian Center for Astrophysics. 2009 [18 January 2015]. （原始内容存档于2018-09-08）.

Solar luminosity is 3.846×10²⁶ watts. Sun Facts. nasa.gov. 14 January 2015 [2018-04-21]. （原始内容存档于2018-09-08）.

NED results for object S5 0014+81. NASA/IPAC EXTRAGALACTIC DATABASE. [2018-04-21]. （原始内容存档于2017-06-30）.
1.2×1.110⁴¹ watts. Kühr, Helmut; Liebert, James W.; Strittmatter, Peter A.; Schmidt, Gary D.; et al. The most luminous quasar - S5 0014+81. Astrophysical Journal. 15 December 1983 [2018-04-21]. Bibcode:1983ApJ...275L..33K. doi:10.1086/184166. （原始内容存档于2018-06-12）.
Solar luminosity is 3.846×10²⁶ watts. Sun Facts. nasa.gov. 14 January 2015 [2018-04-21]. （原始内容存档于2018-09-08）.
The Milky Way absolute visual magnitude is -20.6. Huchra, John P. The Properties of Galaxies. harvard.edu. Harvard-Smithsonian Center for Astrophysics. 2009 [18 January 2015]. （原始内容存档于2018-09-08）.