Dear Observers,

I and my collaborators here at Ondrejov and the Charles University Prague 
(David Vokrouhlicky and Josef Durech) extend and intensify our studies of
non-gravitational asteroid evolution processes with photometric observations.
Recently we have been awarded with a grant to run our new project of 
observations with the Danish 1.54-m telescope where we will have 25% of 
observing time since September 2012 to December 2016 (the science 
justification and research tasks of the NEOSource project are available at
http://www.asu.cas.cz/~ppravec/pravec_gacr_b2_c.pdf ).
With the 0.65-m here, we will observe some brighter targets of the project.
As we believe that some of you will be interested to contribute to the
new project as well, we will list brighter NEOSource project targets 
in these monthly lists together with BinAstPhotSurvey targets.  In this
current list below, there are six NEOSource targets for November 
and December.  Of course, there are also several regular BinAstPhotSurvey
targets as well.  Feel free to work on targets for one or both of the 
projects as you like and can.  Enjoy!

This list of targets is also available at
http://www.asu.cas.cz/~asteroid/binastphotsurvey_neosource_targets20111125.txt

Clear Skies,

Petr Pravec

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

0. Worked objects:
(1536)    Pielinen          15.1    4  130v  0.1 -59  12.6 1.77 2.20  28opp
                  Slow rotator, worked by Russ Durkee.
(1573)    Vaisala           14.7   -6  134v  0.2 -67  12.2 1.82 2.37  22opp
                  Slow rotator, worked from Modra.
(1717)    Arlon             15.7    8  121v  0.1 -53  12.3 1.91 2.20  21opp
                  Return binary, covering one last missing orbit phase
                  needed to complete, see the binast-webtool.
(2423)    Ibarruri          15.2   13  139v  0.1 -49  13.2 1.57 2.19  18opp
                  Slow rotator, worked by Russ Durkee, Adrian Galad and
                  Vasilij Chiorny.
(2870)    Haupt             15.4    2  136v  0.1 -60  12.7 1.89 2.39  16opp
                  Slow rotator, worked by Julian Oey.
(4029)    Bridges           17.9   -1  110v  0.1 -57  12.9 2.19 2.53  16opp
                  Return binary, last events coverage for this apparition
                  would be good, errors < 0.03 mag needed.
(5044)    Shestaka          15.6   27  161v  0.2 -30  13.3 2.00 2.24  12opp
                  Worked from Modra.
(5905)    Johnson           17.2  -37  103v  0.3 -79  14.0 1.77 1.91  15opp
                  Return binary, more data needed.
(23225)   2000 WD25         16.2   -8  142v  0.1 -62  14.0 1.79 2.45  14opp
                  Worked by David Higgins.

1. Returning binaries
(3749)    Balam             16.8   21  115^  0.2  33  13.4 1.99 2.24  18opp
                  "Quadruple" system.  NEOSource project.
(4607)    Seilandfarm       16.3   22  142^  0.1   9  13.0 2.22 2.26  14opp
                  D_2/D_1 = 0.30, P_orb = 31.65 h
(175706)  1996 FG3          15.9b  29^ 100^  2.7  52  18.2 0.69 1.05   8opp
                  BYORP target - NEOSource project.

2. Paired asteroids (errors <=0.03 mag needed):
(25884)   2000 SQ4          16.9   23  155v  0.3 -37  14.6 1.80 1.95   9opp

3. YORP objects (errors <=0.05 mag needed) - NEOSource project:
(1620)    Geographos        17.5   50  132^  0.3  24  15.6 0.83 1.25  27opp
                  P = 5.22 h, one lightcurve per lunation sufficient.
(138852)  2000 WN10         17.3f  14^ 165v  2.1 -38  20.1 0.70 1.00  11opp
                  P ~ 4.44 h, one full lightcurve sufficient.

4. Mini-family members (errors <=0.05 mag needed) - NEOSource project:
(6825)    Irvine            17.5   25  114^  0.1  36  13.6 2.13 2.17  16opp
                  P = 3.75 h, one lightcurve per lunation sufficient.
(14627)   Emilkowalski      17.2   38  109^  0.2  46  13.1 2.21 2.60   9opp
                  P ~ 11.13 h, one lightcurve per lunation sufficient.

5. Returning "prime suspects", to be followed up on their 2nd (3rd, ...) apparitions
(1344)    Caubeta           16.5   26  129^  0.1  23  12.8 1.98 2.25  21opp 12.8       3.1220          0.21  3
(1739)    Meyermann         16.0   18  167^  0.3 -16  12.7 1.98 2.26  21opp 12.7       2.8219          0.22  3
(2195)    Tengstrom         15.5   20  122^  0.1  25  12.1 1.99 2.22  22opp 12.1       2.82112    0.17 0.22  3
(3665)    Fitzgerald        16.3    1  159   0.3 -30  13.4 2.20 2.42  17opp 13.41      2.4141          0.08  3

6. New targets
(4826)    Wilhelms          15.7    4  157^  0.3 -22  12.3 1.92 2.38  15opp
(7334)    Sciurus           16.4    9  168   0.3 -33  13.5 2.06 2.41  18opp
(11272)   1988 RK           16.4   -1  159   0.2 -34  13.8 1.98 2.43  14opp
(24475)   2000 VN2          14.7   -2^ 156   0.7 -45  16.1 1.10 1.97   6opp
(39612)   1993 XE1          15.9    1  159   0.5 -42  14.0 1.89 2.36   9opp
(39979)   1998 HT12         15.5    8  166   0.4 -36  13.6 1.85 2.38   8opp
(98129)   2000 SD25         15.6    8  167   0.4 -31  14.1 1.63 2.37   8opp

Note: The ephemerides were computed for 2011-11-25
      ^/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:
(1536)
(1573)
(1717)
(2423)
(2870)
(4029)
(5044)
(5905)
(23225)
(3749)
(4607)
(175706)
(25884)
(1620)
(138852)
(6825)
(14627
(1344)
(1739)
(2195)
(3665)
(4826)
(7334)
(11272)
(24475)
(39612)
(39979)
(98129)