This catalogue provides details of accreting neutron stars that are thermonuclear burst oscillation sources.  It includes the source name, the burst oscillation frequency, and references (with NASA Astrophysical Data System links) for the burst oscillation discovery paper(s).  It includes all sources where the burst oscillation detection is considered to be robust, and is an updated version of Table 1 in <a href="https://ui.adsabs.harvard.edu/abs/2012ARA%26A..50..609W" rel="external">Watts 2012</a>. Second (confirmation) references are given for sources where the initial discovery rested on a single burst. It does not include tentative detections (see Table 2 of <a href="https://ui.adsabs.harvard.edu/abs/2012ARA%26A..50..609W" rel="external">Watts 2012</a>).
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<table cellpadding=5 border=2>
          <tr>
          <td class="head" width="500"> Source </td>
          <td class="head">Frequency (Hz) </td>
          <td class="head">Discovery paper(s) </td>
          </tr>
          
          
            <tr>
            <td> <strong>Persistent accretion-powered pulsars with burst oscillations</strong> </td>
            <td>  </td>
            <td>  </td>
	    </tr>
          
          <tr>
            <td> SAX J1808.4-3658 </td>
            <td> 401 </td>
            <td> 
               <a href="https://ui.adsabs.harvard.edu/abs/2003Natur.424...42C">Chakrabarty et al. 2003</a> 
              </td>
	    </tr>
	   
	   <tr>
	   <td> IGR J17498-2921 </td>
	   <td> 401 </td>
	   <td> 
	   <a href="https://ui.adsabs.harvard.edu/abs/2011ATel.3568....1L">Linares et al. 2011</a>;
	   <a href="https://ui.adsabs.harvard.edu/abs/2012MNRAS.422.2351C">Chakraborty &amp; Bhattacharyya 2012</a>
           </td>
	   </tr>
	   
           <tr>
	   <td> XTE J1814-338 </td>
	   <td>  314 </td>
	   <td> 
	   <a href="https://ui.adsabs.harvard.edu/abs/2003ApJ...596L..67S">Strohmayer et al. 2003</a>
           </td>
	   </tr>
	   
	   <tr>
	   <td> IGR J18245-2452 </td>
	   <td>  254 </td>
	   <td> 
	   <a href="https://ui.adsabs.harvard.edu/abs/2013ATel.5068....1P">Patruno 2013</a>;
	   <a href="https://ui.adsabs.harvard.edu/abs/2013Natur.501..517P">Papitto et al. 2013</a>
           </td>
	   </tr>

	   
	   <tr>
	   <td>IGR J17511-3057  </td>
	   <td>  245</td>
	   <td> 
	   <a href="https://ui.adsabs.harvard.edu/abs/2010MNRAS.409.1136A">Altamirano et al. 2010</a>
           </td>
	   </tr>
	   
	   <tr>
	   <td>IGR J17480-2446 </td>
	   <td> 11 </td>
	   <td> 
	   <a href="https://ui.adsabs.harvard.edu/abs/2011ApJ...740L...8C">Cavecchi et al. 2011</a>
           </td>
	   </tr>
	   
	   <tr>
	   <td> <strong>Intermittent accretion-powered pulsars with burst oscillations</strong> </td>
	   <td>  </td>
	   <td>  </td>
	   </tr>
	   
	    <tr>
	   <td> Aql X-1 </td>
	   <td>  550 </td>
	   <td> 
	   <a href="https://ui.adsabs.harvard.edu/abs/1998ApJ...495L...9Z">Zhang et al. 1998</a>
           </td>
	   </tr>
	   
	   <tr>
	   <td> HETE J1900.1-2455 </td>
	   <td> 377 </td>
	   <td> 
	   <a href="https://ui.adsabs.harvard.edu/abs/2009ApJ...698L.174W">Watts et al. 2009</a>
           </td>
	   </tr>
	   
	   <tr>
	   <td><strong> Burst oscillation sources without detectable
accretion-powered pulsations</strong> </td>
	   <td>  </td>
	   <td>  </td>
	   </tr>
	   
	   <tr>
	   <td> 4U 1608-522 </td>
	   <td> 620 </td>
	   <td> 
	   <a href="https://ui.adsabs.harvard.edu/abs/2003HEAD....7.1738H">Hartman et al. 2003</a>; 
   	   <a href="https://ui.adsabs.harvard.edu/abs/2008ApJS..179..360G">Galloway et al. 2008</a>
           </td>
	   </tr>   

	   <tr>
	   <td> SAX J1750.8-2900 </td>
	   <td>601  </td>
	   <td> 
	   <a href="https://ui.adsabs.harvard.edu/abs/2002ApJ...575.1018K">Kaaret et al. 2002</a>;
   	   <a href="https://ui.adsabs.harvard.edu/abs/2008ApJS..179..360G">Galloway et al. 2008</a>
           </td>
	   </tr>   
	   
	   <tr>
	   <td> GRS 1741.9-2853  </td>
	   <td>  589 </td>
	   <td> 
	   <a href="https://ui.adsabs.harvard.edu/abs/1997ApJ...486..355S">Strohmayer et al. 1997</a>
           </td>
	   </tr>   
	   
	   <tr>
	   <td> 4U 1636-536 </td>
	   <td> 581 </td>
	   <td> 
	   <a href="https://ui.adsabs.harvard.edu/abs/1998ApJ...498L.135S">Strohmayer et al. 1998</a>;
	   <a href="https://ui.adsabs.harvard.edu/abs/2002ApJ...577..337S">Strohmayer &amp; Markwardt 2002 (in a superburst) </a>
           </td>
	   </tr>   
	   
	   <tr>
	   <td>  X 1658-298</td>
	   <td>  567</td>
	   <td> 
	   <a href="https://ui.adsabs.harvard.edu/abs/2001ApJ...549L..71W">Wijnands, Strohmayer &amp; Franco 2001</a>
           </td>
	   </tr>   
	   
	   <tr>
	   <td> EXO 0748-676 </td>
	   <td>  552 </td>
	   <td> 
	   <a href="https://ui.adsabs.harvard.edu/abs/2010ApJ...711L.148G">Galloway et al. 2010</a>
           </td>
	   </tr>   
	   
	   <tr>
	   <td> SAX J1810.8-2609 </td>
           <td> 532  </td>
           <td>
           <a href="https://ui.adsabs.harvard.edu/abs/2018ApJ...862L...4B">Bilous et al. 2018</a>
           </td>
           </tr>


	   <tr>
	   <td> KS 1731-260 </td>
	   <td> 524 </td>
	   <td> 
	   <a href="https://ui.adsabs.harvard.edu/abs/1997ApJ...479L.137S">Smith, Morgan &amp; Bradt 1997</a>;
	   <a href="https://ui.adsabs.harvard.edu/abs/2000ApJ...542.1016M">Muno et al. 2000</a>
           </td>
	   </tr>   
	   
	   	   <tr>
	   <td> 4U 1728-34 </td>
	   <td>363  </td>
	   <td> 
	   <a href="https://ui.adsabs.harvard.edu/abs/1996ApJ...469L...9S">Strohmayer et al. 1996</a>
           </td>
	   </tr>   
	   
	   	   <tr>
	   <td>4U 1702-429  </td>
	   <td>329  </td>
	   <td> 
	   <a href="https://ui.adsabs.harvard.edu/abs/1999ApJ...512L.125M">Markwardt, Strohmayer &amp; Swank 1999</a>
           </td>
	   </tr>   
	   
	   	   <tr>
	   <td>IGR J17191-2821  </td>
	   <td>294  </td>
	   <td> 
	   <a href="https://ui.adsabs.harvard.edu/abs/2010MNRAS.401..223A">Altamirano et al. 2010</a>
           </td>
	   </tr>   
	
        </table>
       <br>