Difference: HPDPDefinitionPage (9 vs. 10)

Revision 102015-06-24 - KatrinaExter

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Herschel Highly Processed Data Product Page

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Long range spectro flat-fielding Manual correction of the flat-fielding drift Yes - level2/2.5 equivalent FITS files No Yes   Must-have, however the aim is to have this as part of the SPG, and only those that still have problems would require manual correction  
Red leak spectral range Run the specific pipeline that deals with red leak region (CalBlock+RSRF) and provide data stand-alone Yes - level2 equivalent FITS files No Yes   Must-have  
High flux source data Very bright sources ought to be reduced with a difference pipeline script Yes - level2/2.5 equivalent FITS files No Yes   Some level of manual reduction may be necessary, but probably are not many such observations  
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Removing background contamination - case 1 chopNod mode Line and continuum Yes - level2/2.5 equivalent FITS files No Yes   Nice to have, depends on how possible it will be to identify these, would be manual reduction  
Removing background contamination - case 2 unchopped mode Line and continuum Yes - level2/2.5 equivalent FITS files No Yes   Nice to have, easier to identify that for chopNod, but would here also be manual reduction  
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Removing background contamination - case 1 chopNod mode Line (and continuum?) Yes - level2/2.5 equivalent FITS files No Yes   Nice to have, depends on how possible it will be to identify these, would be manual reduction  
Removing background contamination - case 2 unchopped mode Line (and continuum?) Yes - level2/2.5 equivalent FITS files No Yes   Nice to have, easier to identify that for chopNod, but would here also be manual reduction  
 
Repair of failed observations Re-run pipeline on observations set to failed Yes - level2/2.5 equivalent FITS files No Yes   Observations that are classed as failed but which will now run in SPG are easy to do and could become standard SPG, for others that require manual reduction they could also become the standard SPG, probably not difficult  
Different wavelength regridding Re-run SPG with different wavelength grid parameter so the fluxes are no dependent and the noise characteristics not changed Yes - level2/2.5 equivalent FITS files No Yes   Has not been discussed by ICC yet, so whether this replaces SPG or is provided as an HPDP or done at all, has not yet been discussed  
Line list catalogue Spectral Feature catalogue No Yes - one file per obsid, and one concatenated file No   dependent on available human resources  
 
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