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<!--
//==============================================================================
// tableTools.html
//
// Copyright (C) 2010-2013 Tobias Toll and Thomas Ullrich
//
// This file is part of Sartre version: 1.1
//
// This program is free software: you can redistribute it and/or modify
// it under the terms of the GNU General Public License as published by
// the Free Software Foundation.
// This program is distributed in the hope that it will be useful,
// but without any warranty; without even the implied warranty of
// merchantability or fitness for a particular purpose. See the
// GNU General Public License for more details.
// You should have received a copy of the GNU General Public License
// along with this program. If not, see <http://www.gnu.org/licenses/>.
//
// Author: Thomas Ullrich
// Last update:
//
$Date: 2013-01-14 16:47:38 -0500 (Mon, 14 Jan 2013) $
//
$Author: thomas.ullrich@bnl.gov $
//==============================================================================
-->
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>
<
title
>
Sartre - What's new?
</
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>
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Home
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Overview
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What's New?
</
h1
>
<
h3
>
Version 1.1
</
h3
>
<
p
>
Due to continuous numerical issues in calculating the logarithmic
derivative of the amplitude along
<
em
>
x
</
em
>
(typically called
λ
)
that is needed to calculate the skewedness and real amplitude corrections
we decided to create
lambda lookup tables and include them in the
<
code
>
tables/
</
code
>
directory.
λ
is
derived from the referring ep table (also when running eA). If the
kinematic range is not sufficient, that is if the amplitude table
range used is larger than that of the
λ
table, we fallback
to calculating the value on the fly from the referring ep table.
If the latter is not large enough corrections are switched off. In
any case the user is informed about what is happening. One side effect
of this change is that event generation with corrections
<
em
>
on
</
em
>
became
generally faster.
</
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Last Update:
<!-- #BeginDate format:Am1 -->
May 29, 2013
<!-- #EndDate -->
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></
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>
</
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html
>
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