Added some text about FGRP4, fixed ticks on colorbar for J1057

FGRP1_discoveries.html

@@ -58,6 +58,32 @@ spin-down power is a measure of the total energy emitted by the pulsar. For comp
 Sun outputs roughly 4 x 10<sup>33</sup> erg per second. All pulsars below have a much higher
 spin-down power.</p>
 
+<br>
+<h3>Update: Pulsar Discoveries from FGRP4</h3>
+
+<p>In August 2014, we began the 4<sup>th</sup> Einstein@Home survey for gamma-ray pulsars, or
+"FGRP4". This survey incorporated many new advances that we learned during our previous
+investigation of blind search methods. In addition, we were able to utilised the superior "Pass 8"
+data from the <i>Fermi</i>-LAT team, and search in longer data sets than ever before. In
+combination, these improvements led to FGRP4 being our most sensitive survey to date.</p>
+
+<p>We are very pleased to be able to announce the first set of results from FGRP4. Including the
+discovery of PSR J1906+0722 at the beginning of this survey, these bring the total number of
+gamma-ray pulsars discovered by our Einstein@Home volunteers to 18. You can find the details and
+plots of all the new discoveries below!</p>
+
+<p>We are currently working very hard to study all of the results from FGRP4, and we are hoping to
+present these in a series of papers in the near future. For now, as FGRP4 begins to wind down, we
+are excited to announce the start of our next survey, "FGRPB1". The "B" here stands for "binary";
+for the first time, Einstein@Home will be used to search for gamma-ray pulsars in orbits with
+companion stars, similar to the search which discovered PSR J1311-3430 but on an even larger
+scale.</p>
+
+<p>As always, we are extremely grateful to all of our volunteers, especially those whose computers
+contributed to these new discoveries. To say "we couldn't have done it without you!" would be a terrible
+understatement!</p>
+    
+
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