C/2010 G1 (Boattini)
I could confirm this comet in the night of discovery on the NEO confirmation page:
"the object is clearly cometary with a coma of 2 arc
minutes and with an elongated area of 1'15" in PA237.
8 images, 1 min. exp. time each, SCT-12" f-5.65 taken at 2010 04 05.82632 -
05.83184"
� 2010-04-05 by Bernhard Haeusler, Maidbronn, Germany frozen on comet
35 min. exposure,
2010-04-05 UT 19:49, 12" SCT
f-5.65 + CCD ST10XME
15.88 mag, coma: 2', tail: 1'15" in PA237
MPC observation: computed with Astrometrica
COD B82
OBS Bernhard Haeusler
TEL 0.30-m Schmidt-Cassegrain + CCD
NET CMC-14
RG14C6D C2010 04 05.82632 04 11 13.55 +27 09 03.8 16.2 N B82
RG14C6D C2010 04 05.82789 04 11 13.83 +27 09 00.9 16.0 N B82
RG14C6D C2010 04 05.82948 04 11 14.22 +27 08 56.1 16.0 N B82
RG14C6D C2010 04 05.83184 04 11 14.67 +27 08 52.2 16.1 N B82
RG14C6D C2010 04 05.83738 04 11 15.89 +27 08 36.8 16.1 N B82
RG14C6D C2010 04 05.84132 04 11 16.69 +27 08 27.1 16.1 N B82
RG14C6D C2010 04 05.84527 04 11 17.39 +27 08 16.9 16.1 N B82
RG14C6D C2010 04 05.84920 04 11 18.21 +27 08 06.4 16.0 N B82
RG14C6D C2010 04 05.85315 04 11 19.02 +27 07 56.2 16.1 N B82
RG14C6D C2010 04 05.85710 04 11 19.71 +27 07 45.9 16.1 N B82
Gauss curve produced by Astrometrica. The total PSF is using the
aperture circle of 3 x 3 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
------------ ---------- --------
----- ----- ----- ----- ----- -----
---- ---- ---
RG14C6D 05/04/2010
19:53:52 15.88 14.92 14.40 14.07 13.81 13.58 5.5 18.1 B82
RG14C6D 05/04/2010 19:53:52* 0.05
0.02 0.04 0.05 0.05 0.06 8 4.2 CMC
RG14C6D 05/04/2010 20:17:10 15.88
14.95 14.47 14.15 13.92 13.73 6.7 18.0 B82
RG14C6D 05/04/2010 20:17:10* 0.05
0.04 0.04 0.07 0.07 0.09 7 4.8 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.
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