diff --git a/FGRP1_discoveries.html b/FGRP1_discoveries.html
index a104694e0c6b30e0c6904f5bc578829d8f3abadd..bb201d497be4a5f3ce50ab1f1a54a65bb5dfcc72 100644
--- a/FGRP1_discoveries.html
+++ b/FGRP1_discoveries.html
@@ -48,15 +48,15 @@ gamma-ray pulsars discovered by our Einstein@Home volunteers to 18. You can find
 plots of all the new discoveries below!</p>
 
 <p>Currently we are 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. <br>
-As always, we are extremely grateful to all of our volunteers, especially those whose computers
+  present these in a series of papers in the near future. </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>
 
-<p>Timeline of <i>Fermi</i>-LAT Blind-Search Pulsar Discoveries</p>
 <img style="width: 500px;" alt="Timeline" src="img/psrs_vs_time.png">
 <br>
-<p>The above plot illustrates the number of gamma-ray pulsars discovered in blind searches using NASA's Fermi Gamma-ray Space Telescope as a function of time (when the discoveries were published). Since the launch of the Fermi satellite in 2008, it has continuously scanning the entire sky and thus is providing an ever increasing data set. In principle, having more data available allows us to do more sensitive pulsar searches. However, at the time, the computational cost increases also rapidly with the longer data time spans. Thus, as the graphics shows, over the last few years the only new such discoveries were made with Einstein@Home, owing to the massive collective computing power provided by the Einstein@Home volunteers.</p>
+<p>The above plot illustrates the number of gamma-ray pulsars discovered in blind searches using NASA's Fermi Gamma-ray Space Telescope as a function of time (when the discoveries were published). Since the Fermi satellite was launched in 2008, it has been continuously scanning the entire sky and thus is providing an ever increasing data set. In principle, having more data available allows us to do more sensitive pulsar searches. However, at the same time, the computational cost also increases rapidly with the longer data time spans. Thus, as the graphic shows, over the last few years the only new such discoveries were made with Einstein@Home, thanks to the massive collective computing power provided by the Einstein@Home volunteers.</p>
 <br>
 
 
diff --git a/img/psrs_vs_time.png b/img/psrs_vs_time.png
index 292a217cca51dc12a0c05ca4b9d31ae5ec135364..d59a3e271d64431ab9ed0af8c09fa15c38115662 100644
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