Dear Colleagues,

A new list of targets is below.  The two highest priority targets for
northern hemisphere observers are the two returning binaries, (1717) Arlon
and (17260) 2000 JQ5.  Other worked targets that need more data, suitable
for nights when (1717) and (17260) are worked by others or unworkable 
(e.g., due to a proximity to a bright star, or for southern hemisphere 
observers), are (1830) Pogson, (3576) Galina, (35107) 1991 VH, and 
(11072) Hiraoka.  Ok, there is enough binary or other worked targets for 
northern hemisphere observers, but not so many for southern hemisphere ones,
so I add below several new targets around equator that are suitable for 
David and Julian if they don't work any of the other above, higher priority
targets.

Enjoy.

This list of targets is also available on
http://www.asu.cas.cz/~asteroid/binastphotsurvey_listoftargets20081102.txt

Clear Skies,

Petr Pravec

Object                       V    Dec  Elo   Mot Bga   H    q    a     Arc

0. Worked objects:
(1830)    Pogson            15.9   -6  136v  0.1 -64  12.4 2.06 2.19  25opp
                        Monitoring evolution of mutual events would be good,
                        see ephemeris on the binast-webtool.
(1865)    Cerberus          17.0    6v 148v  0.9 -57  16.8 0.58 1.08  16opp
                        YORP detection candidate, low accuracy data 
                        acceptable.
(3576)    Galina            16.2    1  143v  0.1 -60  13.1 2.08 2.39  14opp
                        Couple full night sessions with errors 0.01 mag 
                        needed to nail it down.
(35107)   1991 VH           16.6  -51   92   0.2 -20  16.9 0.97 1.14   4opp
                        Observations for the return NEA binary from the 
                        southern hemispehre would be useful.

Object                       V    Dec  Elo   Mot Bga   H    q    a     Arc  Hrev        P              Ampl  U
1. Returning binaries
(1717)    Arlon             14.7   32  152^  0.2 -15  12.3 1.91 2.20  21opp 12.3       5.1484          0.08  3 B
                        P_orb = 117.0 h, P_1 = 5.148 h, P_2 = 18.23 h
                        Coverage of full P_orb is needed to reveal whether
                        there occur events in the current geometry.
(17260)   2000 JQ58         16.7   17  142^  0.1 -14  14.0 1.80 2.20   7opp 14.0       3.1285          0.15  3 B
                        P_orb = 14.757 h, D_2/D_1 = 0.26

2. Returning "prime suspects", to be followed up on their 2nd (3rd, ...) apparitions
(11072)   Hiraoka           17.0    4  168   0.3 -50  13.5 2.11 2.39   9opp 13.5       4.7512          0.36  3

3. Paired asteroids (errors <0.05 mag needed):
                       
4. New targets
(4262)    1989 CO           15.8    4  165^  0.3 -44  13.2 1.80 2.30  11opp
(4265)    Kani              14.7    6  171   0.2 -48  12.8 1.94 2.43  13opp
(4935)    Maslachkova       15.2    5  167   0.2 -45  13.6 1.88 2.19  11opp
(15291)   1991 VO1          16.0    6  169^  0.3 -44  14.0 1.98 2.26   7opp
(18401)   1992 WE4          15.8    4  165^  0.3 -45  13.4 2.06 2.53   7opp
(30214)   2000 GS125        16.2    1  166   0.3 -51  14.0 1.98 2.30  10opp
(34155)   2000 QJ22         15.2   -5  155   0.2 -47  13.3 1.81 2.43  12opp
(37559)   1985 UR           16.1    5  162^  0.3 -40  14.1 1.95 2.44   7opp
(38926)   2000 SH226        16.2    5  162^  0.2 -40  14.2 1.93 2.52   7opp

Note: The ephemerides were computed for 2008-11-02
      ^/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:
(1830)
(1865)
(3576)
(35107)
(1717)
(17260)
(11072)
(4262)
(4265)
(4935)
(15291)
(18401)
(30214)
(34155)
(37559)
(38926)