116P/Wild
Depending on its visual orbit angle, the comet has 2 tails counterwise in these days.
� 2009-03-17 by Bernhard Haeusler, Maidbronn, Germany, comet movement: 0.22"/min., image centered on the stars
3 x 5 min. exposure,
2009-03-17, UT 23:15, 12" SCT
f-7 + CCD ST10XME
14.73 mag, coma: 0'45", tail:1'24" in PA 113�, anti tail: 1'17" in PA
300�
� 2009-03-17 by Bernhard Haeusler, Maidbronn, Germany, image centered on the comet
22 x 5 min. exposure,
2009-03-17, UT 23:15 to UT 01:08, 12" SCT
f-7 + CCD ST10XME
14.73 mag, coma: 0'45", tail:1'24" in PA 113�, anti tail: 1'17" in PA
300�
MPC observation: computed with Astrometrica
COD B82
OBS Bernhard Haeusler
TEL 0.30-m Schmidt-Cassegrain + CCD
NET CMC-14
0116P C2009 03 18.03121 09 20
26.02 +19 58 39.6 14.7 N B82
0116P C2009 03 18.03478 09 20 25.92 +19 58 39.3 14.7 N B82
0116P C2009 03 18.04550 09 20 25.70 +19 58 38.7 14.7 N B82
Gauss curve produced by Astrometrica. The total PSF is using the
aperture circle of 10 x 10 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:
COD B82
OBS Bernhard Haeusler
CATALOG: USNO A2.0 / CMC-14 - BAND: R
10x10 20x20 30x30 40x40 50x50 60x60 SNR SB COD
OBJECT DATE TIME +/-
+/- +/-
+/- +/-
+/- N FWHM CAT
------------ ---------- -------- ----- ----- ----- ----- ----- -----
---- ---- ---
116P
18/03/2009 00:55:13 14.73 14.01 13.68 13.48 13.34 13.24 33.7 19.3 B82
116P
18/03/2009 00:55:13* 0.01 0.01 0.01 0.01 0.01 0.01 5 4.9 CMC
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.
links:
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