19P/Borrelly


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On May, 18 2009 I could finally take more images of the comet.

here is my image of last night:

 19P/Borrelly � by Bernhard Haeusler, Germany

2009-05-18 by Bernhard Haeusler, Maidbronn, Germany               .gif animation 3.919 KB                                                                                       

80 x 3 min. exposure (240 min. total), 2008-05-18 UT 21:11 to UT 01:22 12" SCT f-6.532 + CCD ST10XME
18.04 mag, coma: 0'09", tail: 6'23" in PA 297�

19P/Borrelly � by Bernhard Haeusler, Germany

enlargement 8 x of the image up.

The night was almost perfect with pretty good seeing and clear view.
Average FWHM: 4.0, weakest star on a 3 minute exposure: 19.4 mag

10 x 10 Box magnitudes measured with FOCAS II:
19P: 18.04  (at May, 07: 17.66), Knot a: 18.30, Knot b: 18.57  

The 10 x 10 box method for photometry is not giving the exact magnitude of a and b condensation.
Knot a seemed to change its magnitude during the four hours session. Knot b was more constant. Maybe they are not real.

Giovanni Sostero and his collegues are observing the larger spot close to the central condensation, both marked with the two red blinking circles.
Unfortunately this spot is too weak for performing any astrometry.


Line profile:

 


MPC observation: computed with Astrometrica

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

NET CMC-14

0019P         C2009 05 18.90568 12 28 35.82 +33 49 51.1          17.9 N      B82
0019P         C2009 05 18.94266 12 28 35.35 +33 49 23.4          17.9 N      B82
0019P         C2009 05 18.94484 12 28 35.35 +33 49 22.5          17.9 N      B82
0019P         C2009 05 18.96008 12 28 35.17 +33 49 10.5          18.0 N      B82
0019P         C2009 05 18.97532 12 28 34.94 +33 48 59.0          18.0 N      B82
0019P         C2009 05 19.02324 12 28 34.30 +33 48 23.8          18.1 N      B82
0019P         C2009 05 19.04284 12 28 34.06 +33 48 09.1          18.2 N      B82
0019P      a  C2009 05 18.94266 12 28 34.96 +33 49 27.3          18.1 N      B82
0019P      a  C2009 05 18.94484 12 28 34.93 +33 49 26.8          18.2 N      B82
0019P      a  C2009 05 19.04936 12 28 33.57 +33 48 12.8          18.6 N      B82
0019P      b  C2009 05 18.94266 12 28 34.25 +33 49 28.6          18.6 N      B82
0019P      b  C2009 05 18.94484 12 28 34.21 +33 49 27.7          18.6 N      B82
0019P      b  C2009 05 19.04936 12 28 32.75 +33 48 14.3          18.5 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).

 

The total PSF of the fragments is using the aperture circle of 3 x 3 pixel around the brightest pixel.


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

19P                18/05/2009 23:43:59 18.04 16.90 16.27 15.88 15.60 15.40 4.0 19.4 B82
19P                18/05/2009 23:43:59* 0.09 0.10 0.10 0.10 0.10 0.14 18 4.0 CMC
19P                18/05/2009 23:29:41 18.30 17.00 16.36 15.98 15.73 15.57 3.4 19.5 B82
19P                18/05/2009 23:29:41* 0.19 0.13 0.06 0.04 0.06 0.08 3 3.8 CMC
19P                18/05/2009 23:29:41 18.57 2.1 19.5 B82
19P                18/05/2009 23:29:41* 0.04 3 3.8 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.


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

 

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