2009/10/16 Tim Jenness <[log in to unmask]>:
> Fantastic. Works like a charm. Couple of comments:
>
> 1. Could the second line of the history be indented a little?
Done.
> Parameters: FLOW=! FREQ=! [log in to unmask] OUT=@yyy POWER=@power
> MSG_FILTER=! QUIET=!
> Software: /star/bin/smurf/calcnoise
> Group: IN="20090923/00027/s4a20090923_00027_0001,
> 20090923/00027/s4a20090923_00027_0002,
> 20090923/00027/s4a20090923_00027_0003,
>
> like the second line does in the Parameters section.
>
> 2. Kappa please. I have dreamed of seeing the history for something like
> wcsmosaic actually listing all the files that were included in the mosaic.
Done.
> 3. Some extra commas seem to turn up.
>
> Group: SIMPAR=", subname=(s8a,s8b,s8c,s8d), , add_hnoise=0, "
> Group: OBSPAR=", ra=00:00:00.0, dec=00:00:00.0, , lambda=0.85e-3, ,
> mjdaystart=53997.5, , steptime=5.0e-3, , obsmode=heatrun, ,
> flatname=TABLE, , , heatstart=24.2, , heatstep=0.01, , heatnum=150, "
>
> (this is from the SCUBA-2 simulator).
For the moment, I've left these in as blank elements in groups could
in principle be significant.
David
> On Oct 16, 2009, at 7:58 AM, David Berry wrote:
>
>> OK. I've implemented a system to do this. Not quite like I imagined
>> because of limitations caused by fixed-size buffers, etc., and not
>> wanting any direct inter-dependency between NDF and GRP. It involves
>> using the new functions ndgBeggh and ndgEndgh to create a "GRP NDF
>> History" block, within which any uses of kpg1_gtgrp etc are recorded.
>> A new type of NDF event is used to record each NDF to which default
>> history is written, and when ndgEndgh is called, all these NDFs are
>> modified to include the expanded group contents in their history.
>>
>> I've modified cupid_mon.c and smurf_mon.c to use these facilities.
>
>
> --
> Tim Jenness
> Joint Astronomy Centre
>
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