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Comet 46P/WIRTANEN- 21 nov. 2018

Astrometry for Minor Planet Center


COD G39

CON F.-J. Hambsch, ROAD  , San Pedro de Atacama, Chile, Oude Bleken 12, 2400 Mol, Belgium

OBS F.-J.Hambsch, E.Bryssinck

MEA E.Bryssinck

TEL 0.4-m f/6.8 astrograph + CCD

ACK MPCReport file updated 2018.11.21 19:46:04

NET CMC-15

0046P         C2018 11 21.21903 02 12 47.64 -28 56 12.8          12.9 R      G39

0046P         C2018 11 21.22051 02 12 47.81 -28 56 10.2          12.9 R      G39

0046P         C2018 11 21.22199 02 12 47.77 -28 56 05.5          12.9 R      G39

0046P         C2018 11 21.22347 02 12 47.90 -28 56 02.2          13.0 R      G39

0046P         C2018 11 21.22495 02 12 48.33 -28 55 59.0          12.9 R      G39

0046P         C2018 11 21.22644 02 12 48.09 -28 55 56.1          12.9 R      G39

----- end -----

Photometry data from FOCAS-II


COD G39

CON ROAD - Remote Observatory Atacama Desert , San Pedro de Atacama, Chile

CATALOG: USNO A2.0 / CMC 14-15 - BAND: R


                                   10x10  20x20  30x30  40x40  50x50  60x60   SNR   SB   COD

COMET         UTC                    +/-    +/-    +/-    +/-    +/-    +/-     N  FWHM  CAT

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

46P           21/11/2018 05:21:48  12.53  11.61  11.10  10.76  10.50  10.29  35.6  17.7  G39

46P           21/11/2018 05:21:48*  0.00   0.01   0.00   0.00   0.00   0.00     5   3.4  CMC


                                                                     AFRHO         LOG

COMET         UTC                   DELTA    r    BOX "   MAG   RSR    CM    +/-  AFRHO  OBS

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

46P           21/11/2018 05:21:48    0.17   1.10  164.68   9.00   36     81     2  1.909  G39


FoCAs 3.53

www.astrosurf.com/cometas-obs

es.groups.yahoo.com/group/Cometas_Obs

Af(rho) data obtained from filtered images (CARA Approuch) are available,


please send a request to the CARA-coordinator if you are interested in these data

Afρ data  according CARA approach

Afρ vs. radius distance to core (with R-Bessel ) filter