NEO SE36C7C
in 2011
- The previously provisional designation
SE36C7C before the official confirmation for this NEO now is substituted by
designation 2011 ED17.
-
- Updated on 2011/03/12
2011 Mar 06
2011/03/06 16:51:55 UT
- 17:06:42 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
SE36C7C C2011 03 06.70220 11 18 42.95 +40 20
52.4 18.7 R
C42
SE36C7C C2011 03 06.70465 11 18 42.77 +40 20 54.8
19.1 R C42
SE36C7C C2011 03 06.70784 11 18 42.58 +40 20 58.7
18.8 R C42
SE36C7C C2011 03 06.71169 11 18 42.43 +40 21 01.5
17.8 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:
-
-
-
Copyright © Man-To
Hui
2011/03/06
Feel free to e-mail
me with any doubts or questions.
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