Broz, M.; Morbidelli, A.; Bottke, W. F.; Rozehnal, J.; Vokrouhlický, D.; Nesvorný, D. (March 2013). "Constraining the cometary flux through the asteroid belt during the late heavy bombardment". Astronomy and Astrophysics. 551: 16. arXiv:1301.6221. Bibcode:2013A&A...551A.117B. doi:10.1051/0004-6361/201219296.
Pravec (2012) web: 3 rotational light-curves constructed in January, February and March 2012, gave a rotation period 11.131 hours (for all three lightcurves) with a brightness amplitude of 0.55, 0.64 and 0.66 in magnitude, respectively. Summary figures for (14627) Emilkowalski at LCDB and at Ondrejov Asteroid Photometry Project
Broz, M.; Morbidelli, A.; Bottke, W. F.; Rozehnal, J.; Vokrouhlický, D.; Nesvorný, D. (March 2013). "Constraining the cometary flux through the asteroid belt during the late heavy bombardment". Astronomy and Astrophysics. 551: 16. arXiv:1301.6221. Bibcode:2013A&A...551A.117B. doi:10.1051/0004-6361/201219296.
Broz, M.; Morbidelli, A.; Bottke, W. F.; Rozehnal, J.; Vokrouhlický, D.; Nesvorný, D. (March 2013). "Constraining the cometary flux through the asteroid belt during the late heavy bombardment". Astronomy and Astrophysics. 551: 16. arXiv:1301.6221. Bibcode:2013A&A...551A.117B. doi:10.1051/0004-6361/201219296.
Pravec (2012) web: 3 rotational light-curves constructed in January, February and March 2012, gave a rotation period 11.131 hours (for all three lightcurves) with a brightness amplitude of 0.55, 0.64 and 0.66 in magnitude, respectively. Summary figures for (14627) Emilkowalski at LCDB and at Ondrejov Asteroid Photometry Project