C/2007 Q3 (Siding Spring)

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C/2007 Q3 (Siding Spring) � by Bernhard Haeusler, Germany

2010-04-22 by Bernhard Haeusler, Maidbronn, Germany                                          animation 10 x 5 minutes

C/2007 Q3 (Siding Spring) � by Bernhard Haeusler, Germany

2010-04-22 by Bernhard Haeusler, Maidbronn, Germany                                                       frozen on comet

10 x 5 min. exposure, 2010-04-22 UT 01:39, 12" SCT  f-5.65 + CCD ST10XME
12.47 mag (60*60 box), coma: 1'38", tail: 16' in PA 251

MPC observation: computed with Astrometrica

OBS Bernhard Haeusler
TEL 0.30-m Schmidt-Cassegrain + CCD


CK07Q030 C2010 04 22.07067 15 08 30.45 +63 28 30.1 14.4 N B82
CK07Q030 C2010 04 22.07424 15 08 30.25 +63 28 31.1 14.3 N B82
CK07Q030 C2010 04 22.07782 15 08 30.06 +63 28 32.3 14.4 N B82


Gauss curve produced by Astrometrica. The total PSF is using the aperture circle of 15 x 15 pixel around the brightest pixel.
You see the Gauss curve right as the computed ideal line and the real pixels contributed around the ideal line.
The Fit RMS is the deviation from the ideal line (inlay under the Gauss curve).

Photometry computed with FOCAS II, using the Multibox method:

OBS Bernhard Haeusler

                                                         10x10  20x20  30x30  40x40  50x50  60x60   SNR   SB  COD
OBJECT        DATE          TIME          +/-       +/-       +/-       +/-       +/-      +/-  N  FWHM  CAT
------------  ----------      --------     -----  -----  -----  -----  -----  -----  ----  ----  ---

C/2007 Q3    22/04/2010 01:46:55 14.35 13.62 13.27 13.04 12.87 12.74 55.6 19.6 B82
C/2007 Q3    22/04/2010 01:46:55* 0.00 0.01 0.01 0.00 0.00 0.00 3 3.9 USN

FoCAs II - 07/01/2009-b

FOCAS II is a tool for photometry on the base of data coming from Astrometrica. Focas is basically using the .LOG file of Astrometrica.

Explanation of the FOCAS II table headings:

Object, date and time are self-explaining.
10x10, 20x20 ... 60x60 are the measured magnitudes according to the aperture sizes of photometry in arc sec (rectancle).
SNR is the  Signal-to-noise ratio for aperture photometry (calculator).
SB is the magnitude of the faintest star on the image matching with the used star catalogue. This is not the faintest star of the image!
COD is the MPC Code of the observatory.

second line:
+/- are the precisions of the measurements.
N is the number of the used images for the measurements.
FWHM is the Full-Width Half-Maximum of the total PSF: Measure of the seeing.
CAT is the used star catalog in Astrometrica.

Focas II is using the .log file of Astrometrica and is computing the photometry under different apertures (10x10 ... 60x60).
The graphs are showing the astrometric precision of the images.


http://astrosurf.com/cometas-obs/index_i.htm Visual and CCD Observations and images from the "Cometas Obs" mailing list, using the Focas II format

es.groups.yahoo.com/group/Cometas_Obs The Spanish comet observation group in Yahoo

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Copyright: The author of NEO Planner and all sites of this web is Bernhard Haeusler, Dettelbach, Germany, all rights reserved