References
D72  (2011):  Masiero, J.R., Mainzer, A.K., Grav, T., Bauer, J.M., Cutri, R.M., Dailey, J., Eisenhardt, P.R.M., McMillan, R.S., Spahr, T.B., Skrutskie, M.F., Tholen, D., Walker, R.G., Wright, E.L., DeBaun, E., Elsbury, D., Gautier, IV, T., Gomillion, S., Wilkins, A., 2011. Main Belt Asteroids with WISE/NEOWISE. I. Preliminary Albedos and Diameters. Astrophysical Journal 741, 68. 
Mass estimates
Notes (N):
1: This estimate is discarded for the average mass (and derived density) calculation in Carry (2012).
2: This estimate is discarded for the average mass (and derived density) calculation in SiMDA (catalog).
3: This estimate is an average of individual solutions listed before under the same reference (e.g. M125).
PheMu : Mutual eclipsing phenomena in binary systems.

EVM mass average M = (9.270 ± 3.090) × 10^{14} kg (ΔM/M = 33%, SNR = 3.0)
Derived bulk density ρ = (1.64 ± 0.55) g/cm^{3} (Δρ/ρ = 33%, SNR = 3.0)

References
M79  (2009):  Kryszczyńska, A., Colas, F., Descamps, P., Bartczak, P., Polińska, M., Kwiatkowski, T., Lecacheux, J., Hirsch, R., Fagas, M., Kamiński, K., Michałowski, T., Marciniak, A., 2009. New binary asteroid 809 Lundia. I. Photometry and modelling. Astronomy and Astrophysics 501, 769–776. 
 