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Pulsars

Pulsar Search Collaboratory Team Disney Modified Julian Date: 55764 . Pulsars. Introduction . Mission statement: To gain scientific skill in order to detect pulsars from radio data. Radio astronomy is the study of electromagnetic emissions of celestial bodies in the universe.

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Pulsars

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  1. Pulsar Search Collaboratory Team Disney Modified Julian Date: 55764 Pulsars

  2. Introduction • Mission statement: • To gain scientific skill in order to detect pulsars from radio data. • Radio astronomy is the study of electromagnetic emissions of celestial bodies in the universe. • Manmade objects also generate radio signals (RFI).

  3. Onward to Discoveries • Forty-foot Telescope • Object: 3c 295 • Distance: 5.6 billion light years or 1.73 billion pc • RA: 14:09:33 • DEC: 52:26:13 * Actual Jy is 23 Jy 500 Jy ~33 Jy

  4. The Pulsar Evaluation • 15 datasets were analyzed for pulsars • Results of evaluation: • Bodacious RFI and noise • Possible candidates • Known pulsars 00:32 -06:22

  5. Pulsar Candidates 19:21 -16:11 *12:05 -16:08

  6. Known Pulsars *J09:44 -13:54 *J01:08 -14:31

  7. The GBT. • Observing time: 00:30-2:00 • Contribution: Using PYTHON to direct the GBT and to grid data. • Candidates: 19:21-16:11,22:43+69:39,21:07-16:12

  8. GBT Results • Unable to observe all plots • Mainly RFI or noise 19:21 -15:58 21:07 -16:11

  9. Joe Swiggum & Peter Gentile

  10. Conclusion • Observe Period/time • Be Prepared for Problems • Patience is a Virtue • Murphy’s Law • Be thorough in observation and experimentation • Be open to all impossible possibilities

  11. Acknowledgements • Sue Ann Heatherly • Sean Leake and all student mentors • Sarah Scoles • TO ALL TEACHERS! • Duncan and Maura • Ryan Lynch and Peter • The GBT for being the coolest telescope EVER • NRAO for making this possible and tolerating us in our wildest moments 

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