NEO SE36C7A

in 2011

The previously provisional designation SE36C7A before the official confirmation for this NEO now is substituted by designation 2011 CB₆₆.

2011 Mar 06

2011/03/06 16:34:04 UT - 16:48:47 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
     SE36C7A C2011 03 06.69032 11 11 50.25 +42 13 31.8          18.2 R      C42
     SE36C7A C2011 03 06.69160 11 11 50.04 +42 13 31.0          18.3 R      C42
     SE36C7A C2011 03 06.69289 11 11 49.81 +42 13 30.1          18.4 R      C42
     SE36C7A C2011 03 06.69417 11 11 49.63 +42 13 29.4          18.4 R      C42
     SE36C7A C2011 03 06.69545 11 11 49.46 +42 13 28.0          18.4 R      C42
     SE36C7A C2011 03 06.69672 11 11 49.20 +42 13 27.6          18.6 R      C42
     SE36C7A C2011 03 06.69800 11 11 48.95 +42 13 26.6          18.3 R      C42
     SE36C7A C2011 03 06.69926 11 11 48.77 +42 13 25.8          18.2 R      C42
     SE36C7A C2011 03 06.70054 11 11 48.57 +42 13 24.6          18.4 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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