Masiero, Joseph R.; Grav, T.; Mainzer, A. K.; Nugent, C. R.; Bauer, J. M.; Stevenson, R.; et al. (August 2014). "Main-belt Asteroids with WISE/NEOWISE: Near-infrared Albedos". The Astrophysical Journal. 791 (2): 11. arXiv:1406.6645. Bibcode:2014ApJ...791..121M. doi:10.1088/0004-637X/791/2/121.
Marciniak, A.; Bartczak, P.; Müller, T.; Sanabria, J. J.; Alí-Lagoa, V.; Antonini, P.; et al. (2018). "Photometric survey, modelling, and scaling of long-period and low-amplitude asteroids". Astronomy & Astrophysics. 610: A7. arXiv:1711.01893. doi:10.1051/0004-6361/201731479.
Masiero, Joseph R.; Grav, T.; Mainzer, A. K.; Nugent, C. R.; Bauer, J. M.; Stevenson, R.; et al. (August 2014). "Main-belt Asteroids with WISE/NEOWISE: Near-infrared Albedos". The Astrophysical Journal. 791 (2): 11. arXiv:1406.6645. Bibcode:2014ApJ...791..121M. doi:10.1088/0004-637X/791/2/121.
Masiero, Joseph R.; Grav, T.; Mainzer, A. K.; Nugent, C. R.; Bauer, J. M.; Stevenson, R.; et al. (August 2014). "Main-belt Asteroids with WISE/NEOWISE: Near-infrared Albedos". The Astrophysical Journal. 791 (2): 11. arXiv:1406.6645. Bibcode:2014ApJ...791..121M. doi:10.1088/0004-637X/791/2/121.
Lightcurve plot of (932) Hooveria, Palmer Divide Observatory, Brian Warner (2010). Rotation period 39.1±0.1 hours with a brightness amplitude of 0.22±0.02 mag. Quality code of 2+. Summary figures for (932) Hooveria at the LCDB
Lightcurve plot of (932) Hooveria, Palmer Divide Observatory, Brian Warner (2010). Rotation period 39.1±0.1 hours with a brightness amplitude of 0.22±0.02 mag. Quality code of 2+. Summary figures for (932) Hooveria at the LCDB