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Cited article:

UY Ursae Majoris: An A-Subtype W UMa System with a Very Large Fill-Out Factor and an Extreme Mass Ratio

Chun-Hwey Kim, Mi-Hwa Song, Jang-Ho Park, et al.
Journal of Astronomy and Space Sciences 36 (4) 265 (2019)
https://doi.org/10.5140/JASS.2019.36.4.265

UBVRcIcANALYSIS OF THE RECENTLY DISCOVERED TOTALLY ECLIPSING EXTREME MASS RATIO BINARY V1853 ORIONIS, AND A STATISTICAL LOOK AT 25 OTHER EXTREME MASS RATIO SOLAR-TYPE CONTACT BINARIES

R. G. Samec, C. M. Labadorf, N. C. Hawkins, D. R. Faulkner and W. Van Hamme
The Astronomical Journal 142 (4) 117 (2011)
https://doi.org/10.1088/0004-6256/142/4/117

LOW MASS RATIO CONTACT BINARY SYSTEMS HN UMa AND II UMa - III

Woo-Baik Lee, Ho-Il Kim, Young-Woon Kang and Kyu-Dong Oh
Journal of Astronomy and Space Sciences 23 (3) 189 (2006)
https://doi.org/10.5140/JASS.2006.23.3.189

The First Photometric Analyses Of Four New Discovered Ew-Type Eclipsing Binaries: GSC 1848-1264, GSC 0804-0118, GSC 0619-0232 And GSC 2936-0478

Y. G. Yang, S. B. Qian, D. J. Gonzalez-rojas and J. Z. Yuan
Astrophysics and Space Science 300 (4) 337 (2005)
https://doi.org/10.1007/s10509-005-4161-4

A Photometric Study of the W UMa-type Eclipsing Binary System GSC 0445-1993

Yuan-Gui Yang, Sheng-Bang Qian and M. D Koppelman
Chinese Journal of Astronomy and Astrophysics 5 (2) 137 (2005)
https://doi.org/10.1088/1009-9271/5/2/003