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PostPosted: Tue Mar 22, 2011 1:58 am 
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Joined: Wed May 17, 2006 7:02 am
Posts: 285
Location: MPE Garching
http://arxiv.org/abs/1103.4055
http://www.sciencemag.org/content/early ... 2.abstract
PAMELA Measurements of Cosmic-ray Proton and Helium Spectra

These data have been added to the database of cosmic-ray measurements available from
http://www.mpe.mpg.de/~aws/propagate.html

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PostPosted: Wed Jul 27, 2011 10:09 am 
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Joined: Mon Jan 19, 2009 9:48 am
Posts: 19
Location: INFN Perugia
strong wrote:
http://arxiv.org/abs/1103.4055
http://www.sciencemag.org/content/early ... 2.abstract
PAMELA Measurements of Cosmic-ray Proton and Helium Spectra

These data have been added to the database of cosmic-ray measurements available from
http://www.mpe.mpg.de/~aws/propagate.html


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PostPosted: Wed Jul 27, 2011 10:11 am 
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Joined: Mon Jan 19, 2009 9:48 am
Posts: 19
Location: INFN Perugia
Ciao,
I see a mis-typing in GCR_data_10.dat, on PAMELA's helium data.
In the point between 10.45 and 11.54 GeV/n (E_mean = 10.98),
the flux value and its errors (low & high) are 3 order of magnitude higher. So:
- 9.76e+02 to be replaced by 9.76e-01.
- 4.0e+01 to be replaced by 4.0e-02.

It is a large deviation and may be important if, e.g., one uses (blindly) the DB data for a chi2 analysis.



strong wrote:
http://arxiv.org/abs/1103.4055
http://www.sciencemag.org/content/early ... 2.abstract
PAMELA Measurements of Cosmic-ray Proton and Helium Spectra

These data have been added to the database of cosmic-ray measurements available from
http://www.mpe.mpg.de/~aws/propagate.html


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PostPosted: Mon Aug 01, 2011 12:52 am 
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Joined: Wed May 17, 2006 7:02 am
Posts: 285
Location: MPE Garching
thanks for spotting and reporting this error, the corrected version is now available : GCR_data_11.dat

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Andy Strong, MPE


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