Dear Observers, Here is a new list of targets. It would be particularly useful to take data for the returning binary (26471), that could result in obtaining a unique solution for its orbital pole (for our paper Scheirich et al., "Binary asteroid population. 4. Predominance of retrograde orbital poles of binary asteroids.", in preparation). Enjoy! This list of targets is also available at http://www.asu.cas.cz/~asteroid/binastphotsurvey_neosource_targets20160110.txt Fyi, both I and Peter Kusnirak will be away from December 23 to January 3. I may have a limited access so I may process some urgent data during my holidays, but we will resume regular data processing on January 4. Clear Skies, Petr Pravec Object V Dec Elo Mot Bga H q a Arc Hrev P Ampl U 0. Worked objects: (2033) Basilea 14.8 29 169^ 0.3 26 12.9 1.98 2.23 25opp Worked by Don Pray. (3433) Fehrenbach 15.5 27 130v 0.1 -22 12.5 1.95 2.39 23opp New binary, monitoring events would be useful. (4272) Entsuji 16.4 2 100v 0.4 -56 12.8 1.78 2.37 22opp New binary, monitoring events would be useful. (4520) Dovzhenko 16.5 17 127v 0.1 -30 13.1 1.77 2.27 21opp Worked by Joe Pollock. (6148) Ignazgunther 16.1 -20 122v 0.2 -38 13.6 1.74 2.28 16opp Worked by Joe Pollock. (16955) 1998 KU48 15.8 17 145v 0.2 -17 12.5 2.18 2.43 16opp Worked by Julian Oey. (41588) 2000 SC46 14.9 -17 138 0.4 13 13.1 1.59 2.34 14opp Worked by Julian Oey. 1. Returning binaries: (1453) Fennia 15.5 66 136 0.3 30 12.8 1.84 1.90 27opp Return binary, 5th apparition. D_2/D_1 = 0.28, P_orb = 23.00 h (26471) 2000 AS152 16.2 -1 150^ 0.3 23 13.2 1.62 1.92 14opp Return binary, 3rd apparition. Data needed to get a unique orbit solution. D_2/D_1 = 0.36, P_orb = 39.28 h 2. Paired asteroids (errors <= 0.03 mag): 3. Returning "prime suspects", to be followed up on their 2nd (3rd, ...) apparitions (1739) Meyermann 16.4 9 145^ 0.1 41 12.6 1.98 2.26 26opp 12.6 2.8219 0.17 0.22 3 4. New targets: (1770) Schlesinger 15.1 29 166^ 0.2 30 12.0 2.31 2.46 32opp (2535) Hameenlinna 15.2 8 140^ 0.1 45 12.3 2.06 2.24 26opp (3228) Pire 15.4 18 161^ 0.2 32 12.8 2.14 2.46 30opp (7717) Tabeisshi 15.2 25 158^ 0.1 38 13.7 1.76 2.44 19opp (17406) 1987 DO 16.5 19 176^ 0.3 17 14.7 1.96 2.37 14opp (17503) Celestechild 15.5 6 164 0.5 12 14.0 1.72 2.28 16opp (18917) 2000 OG48 16.3 0 151^ 0.2 24 13.8 1.98 2.36 21opp (19496) Josephbarone 16.5 25 176^ 0.3 20 14.5 2.05 2.43 15opp (19711) 1999 TG219 16.4 0 141^ 0.3 35 13.4 1.79 2.35 14opp (22506) 1997 WD8 16.5 18 171^ 0.2 22 14.8 1.92 2.33 15opp (31381) 1998 XW86 16.4 6 160^ 0.3 20 13.6 2.16 2.24 19opp (37586) 1991 BP2 16.0 -4 123^ 0.4 48 13.2 1.86 2.33 13opp (43659) 2002 FJ1 15.5 29 172 0.5 23 14.4 1.75 2.36 13opp (106520) 2000 WA51 16.4 39^ 154 0.5 40 14.8 1.71 2.41 11opp (112493) 2002 PR6 16.2 0 138^ 0.3 38 15.5 1.40 2.12 12opp Note: The ephemerides were computed for 2016-01-10 ^/v means that the value increases/decreases by more than 0.05 mag/day (for V) or by more than 0.5 deg/day for Dec and Elong. The rate of apparent motion (Mot) is in deg/day. Bga is the galactic latitude. Compact listing: (2033) (3433) (4272) (4520) (6148) (16955) (41588) (1453) (26471) (1739) (1770) (2535) (3228) (7717) (17406) (17503) (18917) (19496) (19711) (22506) (31381) (37586) (43659) (106520) (112493)