144P/Kushida


[upwards] [144p_20090321] [144p_20090319] [144p_20090317] [144p_20090218] [144p_20090217] [144p_20090214] [144p_20090130] [144p_20090104] [144p_20081230] [144p_20081219] [144p_20081217_19]

 144P/Kushida � by Bernhard Haeusler, Germany

2009-02-14 by Bernhard Haeusler, Maidbronn, Germany

4 x 1 min. exposure, 2009-02-14, UT 21:18 to 21:22, 12" SCT  f-7 + CCD ST10XME
14.07 mag, coma: 4'00"


MPC observation: computed with Astrometrica

COD B82
OBS Bernhard Haeusler
TEL 0.30-m Schmidt-Cassegrain + CCD

NET CMC-14

0144P C2009 02 14.88875 04 59 13.86 +16 54 14.0 14.1 N B82
0144P C2009 02 14.88950 04 59 13.97 +16 54 13.9 14.1 N B82
0144P C2009 02 14.89027 04 59 14.07 +16 54 14.0 14.1 N B82
0144P C2009 02 14.89102 04 59 14.21 +16 54 14.1 14.1 N B82


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
------------  ---------- --------  -----  -----  -----  -----  -----  -----  ----  ----  ---

144P              14/02/2009 21:20:53 14.07 13.06 12.54 12.19 11.95 11.76 11.9 18.4 B82
144P              14/02/2009 21:20:53* 0.02 0.03 0.04 0.04 0.04 0.04 5 4.5 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.


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

 

[upwards] [144p_20090321] [144p_20090319] [144p_20090317] [144p_20090218] [144p_20090217] [144p_20090214] [144p_20090130] [144p_20090104] [144p_20081230] [144p_20081219] [144p_20081217_19]

 

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