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SUMMARY:keV Dark Matter Searches with the Micro-X Rocket
DTSTART;VALUE=DATE-TIME:20170623T130000Z
DTEND;VALUE=DATE-TIME:20170623T140000Z
DTSTAMP;VALUE=DATE-TIME:20260609T231720Z
UID:indico-event-3023@indico.ific.uv.es
DESCRIPTION:\n    The Micro-X sounding rocket uses a Transition Edge Senso
 r (TES) array to make X-ray observations. The improved energy resolution o
 f TESs compared to traditional space-based detectors brings new precision 
 to both supernova remnant observations and the X-ray search for sterile ne
 utrino dark matter. Current observations disagree over the potential prese
 nce of a 3.5 keV X-ray line consistent with a sterile neutrino interaction
 \, and Micro-X is in a unique position to establish or refute the presence
  of this line. I will present the construction status of the instrument an
 d expectations for flight observations\, with special emphasis given to th
 e prospects of sterile neutrino studies.\n\nhttps://indico.ific.uv.es/even
 t/3023/
LOCATION:IFIC Seminar Room\, 1.1.1
URL:https://indico.ific.uv.es/event/3023/
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