Evangelista, Y.Y.EvangelistaDel Monte, E.E.Del MonteFeroci, M.M.FerociPittori, CarlottaCarlottaPittoriVerrecchia, FrancescoFrancescoVerrecchiaSantolamazza, P.P.SantolamazzaGiommi, PaoloPaoloGiommi2020-09-172020-09-172009-10-01https://hdl.handle.net/20.500.13025/1293The Astronomer's Telegram, #2238On 9 October 2009 02 57 43 UT SuperAGILE detected a type I X-ray burst from a sky position consistent with the accreting millisecond pulsar HETE J1900.1-2455. The burst was significantly detected only at energies below 28 keV, as typical of type I X-ray bursts in SuperAGILE, due to their soft energy spectrum. The burst profile is double-peaked, with a total duration of about 13 s, similar to previous bursts from this source.X-rayRequest for ObservationsBinariesNeutron StarsTransientshttp://adsabs.harvard.edu/abs/2009ATel.2238....1E2009ATel.2238....1E