NEO SE3615B

in 2011

The previously provisional designation SE3615B before the official confirmation for this NEO now is substituted by designation 2011 EE₁₇. This NEO asteroid is discovered in the course of Catalina Sky Survey on 2011 Mar. 06.199 UT. (MPEC 2011-E38)

2011 Mar 06

2011/03/06 16:00:22 UT - 16:15:02 UT, 14" SCT f/6.9 + QHY9 CCD, BIN 2x2 90 sec x 9 exposure, north up and east left

MPC observation computed with Astrometrica using CMC-14 star catalog in R band:

COD C42
OBS X.Gao, M.-T. Hui
MEA M.-T. Hui
TEL 0.36-m f/6.9 Schmidt-Cassegrain + CCD
NET CMC-14
     SE3615B C2011 03 06.66819 09 40 07.76 -00 20 50.3          17.9 R      C42
     SE3615B C2011 03 06.67201 09 40 07.21 -00 20 22.6          18.2 R      C42
     SE3615B C2011 03 06.67583 09 40 06.59 -00 19 51.8          18.3 R      C42
----- end -----

Gauss curve produced by Astrometrica with CMC-14. The total PSF is using an aperture circle of 5 x 5 pixel around the brightest pixel. We can see the Gauss curve in the right is as the computed ideal line and the real pixels contributed around the ideal line. The Fit RMS, which inlays under the Gauss curve, is the deviation from the ideal line.

Photometry result computed with FOCAS II, which processes images based upon the .LOG file of Astrometrica:

Feel free to e-mail me with any doubts or questions.

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