diff --git a/FGRP1_discoveries.html b/FGRP1_discoveries.html
index 50c0f4c11e258ec810c2ac1bd964e023b6ddb32d..0ecbb325383b64486011c6af28266a85f26c0420 100644
--- a/FGRP1_discoveries.html
+++ b/FGRP1_discoveries.html
@@ -167,6 +167,10 @@ gamma-ray emission as a function of pulsar rotation phase and resolve the pulse
                         </table>
                         <br>
                       </td>
+                      <td colspan="1" rowspan="2" style="vertical-align: top;" width="460">
+                        <img style="width: 250px;" alt="J1653" src="img/fhist-J1653-0158.png">
+                        <img style="width: 196px; height: 373px;" alt="J1653" src="img/tvsph-J1653-0158.png">
+                      </td>
                     </tr>
                     <tr>
                       <td style="vertical-align: top;">
@@ -174,6 +178,14 @@ gamma-ray emission as a function of pulsar rotation phase and resolve the pulse
                         <a href="https://einsteinathome.org/show_user.php?userid=726200">Hapsburg (Taiwan)</a> and <a href="https://einsteinathome.org/show_user.php?userid=947071">TGWakko (USA)</a><br><br>
                         <b>Survey:</b><br>
                         FGRPB1<br><br>
+                        <b>Selected pulsar parameters:</b><br>
+                        Right ascension: 16:53<br>
+                        Declination: -01:58<br>
+                        Spin frequency: 508.21 Hz<br>
+                        First frequency derivate: -6.20 x 10<sup>-16</sup> Hz/s<br>
+                        Orbital period: 75 min<br>
+                        Characteristic age: 37 Gyrs<br>
+                        Spin-down power: 4.4 x 10<sup>33</sup> erg/s<br>
                       </td>
                     </tr>
                   </tbody>
@@ -197,6 +209,10 @@ gamma-ray emission as a function of pulsar rotation phase and resolve the pulse
                         </table>
                         <br>
                       </td>
+                      <td colspan="1" rowspan="2" style="vertical-align: top;" width="460">
+                        <img style="width: 250px;" alt="J2039" src="img/fhist-J2039-5617.png">
+                        <img style="width: 196px; height: 373px;" alt="J2039" src="img/tvsph-J2039-5617.png">
+                      </td>
                     </tr>
                     <tr>
                       <td style="vertical-align: top;">
@@ -204,6 +220,14 @@ gamma-ray emission as a function of pulsar rotation phase and resolve the pulse
                         <a href="https://einsteinathome.org/show_user.php?userid=578159">jbencin (USA)</a> and <a href="https://einsteinathome.org/show_user.php?userid=635570">Peter</a><br><br>
                         <b>Survey:</b><br>
                         FGRPB1<br><br>
+                        <b>Selected pulsar parameters:</b><br>
+                        Right ascension: 20:39<br>
+                        Declination: -56:17<br>
+                        Spin frequency: 377.23 Hz<br>
+                        First frequency derivate: -2.02 x 10<sup>-15</sup> Hz/s<br>
+                        Orbital period: 5.3 h<br>
+                        Characteristic age: 4 Gyrs<br>
+                        Spin-down power: 2.5 x 10<sup>34</sup> erg/s<br>
                       </td>
                     </tr>
                   </tbody>
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