Meanwhile, a short report on my latest asteroid discovery: 2013 GM21, which was published in the DOU MPEC K13-G54 today (Apr 12, 2013: look for object K13G21M).
On April 6th, I was on my own initiative (and successfully) trying to get follow-up observations on three objects (2013 EZ102, 2013 EB103 and 2013 EC103) which Krisztian Sarneczky and I discovered in the Konkoly survey from MPC 461 (the 60-cm Schmidt of Konkoly, HU) mid-March. I was "remotely" using the 81-cm Schulman telescope of the Mt. Lemon Sky Center (MPC G84) for that, one of the telescopes in the SSO Network.
In the images that should (and did) contain 2013 EZ102, I found two other moving objects. Both were unidentified - i.e., they were not in the MPCOrb asteroid database of the IAU Minor Planet Center and could be new discoveries! So they were submitted to the MPC with the temporary designations LaMa515 and LaMa516.
One of these (LaMa515) turned out to have been observed by another observatory just days before, so that one was not a new discovery: the other observatory alas beat me to it.
The second object however, a mag +19.5 to +20 object I temporarily designated LaMa516 moving quite close to 2013 EZ102 in the images, turned out to be truely new: my observations of April 6th were the first! It can be seen in the blink above, which shows you a small part of the April 6th discovery images. 2013 EZ102 is in the images too.
I next obtained new images, based on a very rough search orbit fit, on April 7th, 8th and on April 11th, again using the 81-cm telescope of MPC G84. As a result, it was formally MPEC-ed today by the MPC as 2013 GM21: my second asteroid discovery using a "remote" telescope! And my 69th asteroid discovery in total (and 5th in 2013, the other four being in the Konkoly survey. For a full list of my discoveries see here).
The asteroid is a borderline Maria family main belt asteroid. With H=16.8, it is an estimated 1.5 km large. It has the following orbital elements (source: MPC):
Epoch 2013 Mar. 29.0 TT = JDT 2456380.5 MPC M 351.06235 (2000.0)
n 0.24233744 Peri. 39.90632 a 2.5479390 Node 164.25356 e 0.0734092 Incl. 17.12483
q 2.3608968 T 2456417.38101 JDT
P 4.07 H 16.8
From 13 observations 2013 Apr. 6-11.
As can be seen in the orbital plots, the orbit is well inclined to the ecliptic. I discovered it when it was in opposition and close to perihelion of its orbit, these two factors combining in a maximum brightness for the object. This is basically the same situation as with my earlier discovery 2012 SM58.