Dear Observers,

A new list of targets is below.  There is one new returning binary, 
1453 Fennia, well before opposition and it should be relatively low burden
on our resources (just a little bit of collaboration may be needed to
cover its 23-h orbital period well).  There is also a few return "prime
suspects" (i.e., asteroids with P and A in the range of asynchronous
binaries, but with no events observed in previous apparitions).
But it looks that you might be interested in attempting new targets, so
I have added several suitable ones.  Enjoy.

This list of targets is also available at
http://www.asu.cas.cz/~asteroid/binastphotsurvey_listoftargets20110104.txt

Clear Skies,

Petr Pravec

Object                       V    Dec  Elo   Mot Bga   H    q    a     Arc  Hrev        P              Ampl  U

0. Worked objects:

1. Returning binaries
(1453)    Fennia            15.9   32  115^  0.1  76  12.8 1.84 1.90  24opp
                          D_2/D_1 = 0.28, P_orb = 22.99 h

2. Returning "prime suspects", to be followed up on their 2nd (3rd, ...) apparitions
(1785)    Wurm              15.6   21  172^  0.3  18  13.2 2.08 2.24  23opp 13.2       3.2693          0.29  3
(2709)    Sagan             16.3   11  143^  0.1  39  13.3 2.04 2.20  16opp 13.3       5.258           0.36  3
(3951)    Zichichi          15.7   11  145^  0.2  37  12.8 1.93 2.34  13opp 12.8       3.3934          0.25  3
(4263)    Abashiri          15.6   24  175^  0.3  16  12.6 1.92 2.23  16opp 12.6       4.8821          0.15  3

3. Paired asteroids (errors <0.05 mag needed):

4. New targets
(1448)    Lindbladia        14.5   32  168^  0.2  22  12.6 1.94 2.37  21opp
(1856)    Ruzena            16.1    7  138^  0.1  40  12.6 2.06 2.24  19opp
(2675)    Tolkien           15.1   27  171^  0.3  20  12.5 1.99 2.21  22opp
(2843)    Yeti              15.1   16  167^  0.2  18  12.8 2.00 2.30  18opp
(3209)    Buchwald          15.9   18  171^  0.3  17  13.6 2.08 2.19  14opp
(3733)    Yoshitomo         15.0   20  167^  0.2  22  13.0 1.94 2.40  16opp
(4205)    David Hughes      15.3   11  160^  0.5  21  14.2 1.47 1.73  15opp
(4822)    Karge             15.5   18  175   0.3  10  13.7 1.83 2.25  13opp
(4971)    Hoshinohiroba     14.9   22  174^  0.2  17  13.1 1.96 2.38  18opp
(5253)    1985 XB           15.6   63^ 137   0.6  35  14.2 1.53 1.97  11opp
(5744)    Yorimasa          16.1    9  150^  0.2  30  13.4 1.91 2.22  18opp
(5802)    1984 HL1          15.0   26  170^  0.2  21  13.1 1.92 2.27  19opp
(5910)    Zatopek           16.0   16  158^  0.2  28  13.6 1.97 2.28  14opp
(5999)    Plescia           16.0   51  134   0.5  51  14.3 1.58 2.28  10opp
(7706)    Mien              16.2   27  173^  0.2  18  14.3 2.00 2.39  13opp
(9014)    Svyatorichter     15.7   32  170   0.3  19  13.6 1.94 2.32  14opp
(14133)   1998 RJ17         16.2    1  157^  0.2  11  14.1 1.87 2.43  11opp
(43891)   1995 SQ1          15.8   45  156^  0.4  27  13.8 1.84 2.37   7opp
(47592)   2000 AO203        16.3    9  159^  0.2  20  13.1 2.13 2.45  12opp
(52266)   Van Flandern      16.0   22  153^  0.3  36  13.7 1.82 2.33  11opp
(69315)   1992 UR2          15.6   62  139   0.2  17  13.6 1.75 2.32   8opp
(79563)   1998 QD70         15.9   13  170   0.3  10  14.2 1.86 2.44   8opp
(129541)  1996 PQ9          16.2   59  139   0.4  12  14.6 1.59 2.27   6opp

Note: The ephemerides were computed for 2011-01-04
      ^/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:
(1453)
(1785)
(2709)
(3951)
(4263)
(1448)
(1856)
(2675)
(2843)
(3209)
(3733)
(4205)
(4822)
(4971)
(5253)
(5744)
(5802)
(5910)
(5999)
(7706)
(9014)
(14133)
(43891)
(47592)
(52266)
(69315)
(79563)
(129541)