Dear all,
I've sent measurement published in DOU 2006-E48. Precovery was made with the
great help of G. Forti and M. Tombelli:
COD 644
OBS Foglia S., Forti G., Tombelli M.
NET UCAC 2
K04V17D C2002 02 16.44933 09 53 22.96 +05 12 42.7 21.7 V
644
K04V17D C2002 02 16.45593 09 53 22.28 +05 12 46.3 21.9 V
644
K04V17D C2002 02 16.46212 09 53 21.68 +05 12 49.6 21.5 V
644
I really don't know who sent measurement published in today's DOU and it seems
that my observations disappear in the 2004 VD17 observations block...
Perhaps my data was difficult to measure but I've not seen any other possible
moving object around the previous data in the SkyMorph image of 2002 02 16
Later I'll try to see again that images.
Sincerely
Sergio Foglia
---------- Initial Header -----------
From : mpml@yahoogroups.com
To : mpml@yahoogroups.com
Cc :
Date : Mon, 13 Mar 2006 05:25:26 -0700
Subject : RE: {MPML} 2004 VD17 Precovery
> Yesterdays DOU had three measurements
>
> K04V17D C2002 02 16.44933 09 53 22.96 +05 12 42.7 21.7 V
EE048644
> K04V17D C2002 02 16.45593 09 53 22.28 +05 12 46.3 21.9 V
EE048644
> K04V17D C2002 02 16.46212 09 53 21.68 +05 12 49.6 21.5 V
EE048644
>
> Which appear to have been re-measured (and stacked) and submitted with the
March 2002 measurements today.
>
> Either way someone appears to have put some work in on these, I am waiting to
see what the Monitors make of VD17 with these added.
>
> David
>
> -----Original Message-----
> From: mpml@yahoogroups.com [mailto:mpml@yahoogroups.com] On Behalf Of Reiner
M. Stoss
> Sent: Monday, March 13, 2006 4:54 AM
> To: mpml@yahoogroups.com
> Subject: Re: {MPML} 2004 VD17 Precovery
>
> David Dixon wrote:
> > Congratulations to someone on the 2002 precovery of 2004 VD17 from #644.
>
> Rob Matson wrote on Thu, 9 Feb 2006:
> ---
> I have a pair of candidate points to experimentally add to the
> 2004 VD17 solution:
>
> COD 644
> CON [matsonr@...]
> OBS E. F. Helin, S. Pravdo, K. Lawrence, K. Kuluhiwa, M. Hicks, R. Thicksten
MEA R. Matson NET USNO-A2.0 TEL 1.2-m Schmidt + CCD TYP
> NEO
>
> K04V17D C2002 02 16.45593 09 53 22.37 +05 12 46.6 644
> K04V17D C2002 03 06.18111 09 25 09.31 +07 54 36.6 21.8 R 644
>
> These are stack-and-tracked triplets and are too questionable to send to MPC.
But I was curious what effect they would have on the
> impact probability if they ~are~ real.
> ---
>
> Today's DOU shows:
> ---
> K04V17D VC2002 02 16.45513 09 53 22.52 +05 12 45.8
EE049644
> K04V17D VC2002 02 16.46912 09 53 21.11 +05 12 52.5
EE049644
> K04V17D VC2002 03 14.21997 09 14 21.33 +09 04 02.8
EE049644
> K04V17D VC2002 03 14.24102 09 14 19.74 +09 04 12.2 20.6 R
EE049644
> K04V17D VC2002 03 15.16442 09 13 13.50 +09 11 42.8
EE049644
> ---
>
> It looks like the 2002 02 16 images were measured without stacking. So someone
must have got access to the original not-compressed
> images. The compressed ones in SkyMorph do *not* show anything on the single
frames and hardly something on the stack that Rob did.
>
> I haven't checked the 2002 03 14/15 images. Anyone?
>
> Reiner
>
>
>
>
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