User: barry.wardell Date: 2016/06/05 05:21 PM

Modified: /about/gallery/ index.php /about/gallery/gw150914/ index.php /about/gallery/tov/ index.php

Log: gallery: remove some unnecessary javascript includes

File Changes:

Directory: /about/gallery/ ==========================

File [modified]: index.php Delta lines: +0 -1 =================================================================== --- about/gallery/index.php 2016-06-05 22:09:53 UTC (rev 1554) +++ about/gallery/index.php 2016-06-05 22:21:46 UTC (rev 1555) @@ -1,6 +1,5 @@ <?php $title='Einstein Toolkit Gallery'; include_once($_SERVER['DOCUMENT_ROOT'].'/global/header.php');?> -<script type="text/javascript" src="/global/jwplayer/jwplayer.js"></script>

<p>This page contains images and movies of example simulations using the Einstein Toolkit, either exclusively or combined with external codes.

Directory: /about/gallery/gw150914/ ===================================

File [modified]: index.php Delta lines: +0 -1 =================================================================== --- about/gallery/gw150914/index.php 2016-06-05 22:09:53 UTC (rev 1554) +++ about/gallery/gw150914/index.php 2016-06-05 22:21:46 UTC (rev 1555) @@ -1,6 +1,5 @@ <?php $title="Gallery: Binary black hole GW150914"; include_once($_SERVER['DOCUMENT_ROOT'].'/global/header.php');?> -<script type="text/javascript" src="/global/jwplayer/jwplayer.js"></script>

<?php $sim_stats = json_decode(file_get_contents("stats.json"), true);

Directory: /about/gallery/tov/ ==============================

File [modified]: index.php Delta lines: +0 -1 =================================================================== --- about/gallery/tov/index.php 2016-06-05 22:09:53 UTC (rev 1554) +++ about/gallery/tov/index.php 2016-06-05 22:21:46 UTC (rev 1555) @@ -1,6 +1,5 @@ <?php $title="Gallery: Single stable neutron star"; include_once($_SERVER['DOCUMENT_ROOT'].'/global/header.php');?> -<script type="text/javascript" src="/global/jwplayer/jwplayer.js"></script>

<p>This simulation shows how to evolve a stable, single neutron star. It uses a TOV solution as initial data and follows the initial (numerical) perturbations, writing the maximum