Küppers, M.; Mottola, S.; Lowry, S. C.; A'Hearn, M. F.; Barbieri, C.; Barucci, M. A.; et al. (January 2007). "Determination of the light curve of the Rosetta target asteroid (2867) Steins by the OSIRIS cameras onboard Rosetta". Astronomy and Astrophysics. 462 (1): L13 –L16. arXiv:astro-ph/0612097. Bibcode:2007A&A...462L..13K. doi:10.1051/0004-6361:20066694. S2CID14097820.
Küppers, M.; Mottola, S.; Lowry, S. C.; A'Hearn, M. F.; Barbieri, C.; Barucci, M. A.; et al. (January 2007). "Determination of the light curve of the Rosetta target asteroid (2867) Steins by the OSIRIS cameras onboard Rosetta". Astronomy and Astrophysics. 462 (1): L13 –L16. arXiv:astro-ph/0612097. Bibcode:2007A&A...462L..13K. doi:10.1051/0004-6361:20066694. S2CID14097820.
Mainzer, A. K.; Bauer, J. M.; Cutri, R. M.; Grav, T.; Kramer, E. A.; Masiero, J. R.; et al. (June 2016). "NEOWISE Diameters and Albedos V1.0". NASA Planetary Data System: EAR-A-COMPIL-5-NEOWISEDIAM-V1.0. Bibcode:2016PDSS..247.....M. Retrieved 31 August 2018.
Weissman, Paul R.; Lowry, Stephen C.; Choi, Young-Jun (August 2005). "CCD Photometry of Asteroid 2867 Steins: Flyby Target of the Rosetta Mission". American Astronomical Society. 37: 644. Bibcode:2005DPS....37.1528W.
Küppers, M.; Mottola, S.; Lowry, S. C.; A'Hearn, M. F.; Barbieri, C.; Barucci, M. A.; et al. (January 2007). "Determination of the light curve of the Rosetta target asteroid (2867) Steins by the OSIRIS cameras onboard Rosetta". Astronomy and Astrophysics. 462 (1): L13 –L16. arXiv:astro-ph/0612097. Bibcode:2007A&A...462L..13K. doi:10.1051/0004-6361:20066694. S2CID14097820.
Warner, Brian D. (September 2004). "Lightcurve analysis for numbered asteroids 301, 380, 2867, 8373, 25143, and 31368". The Minor Planet Bulletin. 31 (3): 67–70. Bibcode:2004MPBu...31...67W. ISSN1052-8091.
Lightcurve plot of 2867 Steins, Palmer Divide Observatory by B. D. Warner (2004). Rotation period of 6.05±0.01 hours with a brightness amplitude of 0.30 mag. Quality code is 3-. Summary figures for (2867) Šteins at the LCDB.
Lightcurve plot of 2867 Steins, Palmer Divide Observatory by B. D. Warner (2004). Rotation period of 6.05±0.01 hours with a brightness amplitude of 0.30 mag. Quality code is 3-. Summary figures for (2867) Šteins at the LCDB.
Mainzer, A. K.; Bauer, J. M.; Cutri, R. M.; Grav, T.; Kramer, E. A.; Masiero, J. R.; et al. (June 2016). "NEOWISE Diameters and Albedos V1.0". NASA Planetary Data System: EAR-A-COMPIL-5-NEOWISEDIAM-V1.0. Bibcode:2016PDSS..247.....M. Retrieved 31 August 2018.
Küppers, M.; Mottola, S.; Lowry, S. C.; A'Hearn, M. F.; Barbieri, C.; Barucci, M. A.; et al. (January 2007). "Determination of the light curve of the Rosetta target asteroid (2867) Steins by the OSIRIS cameras onboard Rosetta". Astronomy and Astrophysics. 462 (1): L13 –L16. arXiv:astro-ph/0612097. Bibcode:2007A&A...462L..13K. doi:10.1051/0004-6361:20066694. S2CID14097820.
"Target: Steins". IAU–Working Group for Planetary System Nomenclature (WGPSN). Archived from the original on 3 October 2018. Retrieved 14 September 2015.
"Target: Steins". IAU–Working Group for Planetary System Nomenclature (WGPSN). Archived from the original on 3 October 2018. Retrieved 14 September 2015.
Warner, Brian D. (September 2004). "Lightcurve analysis for numbered asteroids 301, 380, 2867, 8373, 25143, and 31368". The Minor Planet Bulletin. 31 (3): 67–70. Bibcode:2004MPBu...31...67W. ISSN1052-8091.