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Pulsars

This study presents a comparative analysis of pulsar data from J2037+1911 and J2037+1942. Original GBT data and recently collected data were evaluated to identify trends and anomalies. The known pulsar exhibited strong readings across both datasets, while the candidate pulsar was assumed to be radio frequency interference (RFI). Observations showed an increase in period measurements from original to collected data. Notably, the reduced χ² values slightly decreased for the unknown candidate, but significantly increased for the known pulsar J2037+1942.

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Pulsars

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  1. Pulsars By: Team Taylor Nic, Jurni, Hannah, and Ryan With help from our amazing mentor NATHAN

  2. Original GBT Data

  3. J2037+1911

  4. J2037+1911

  5. 1711+8827

  6. Recently Collected GBT Data

  7. J2037+1942

  8. 1711+8827

  9. Original Pulsar Data: J2037+1942 Recently Collected Pulsar Data: J2037+1942

  10. Original Candidate Data:1711+8827 Recently Collected Candidate Data: 1711+8827

  11. Overall Observations • Known pulsar showed strong readings in both plots • Candidate assumed to be RFI • Period increases in both plots of original to collected. • Reduced χ² decreased slightly in the unknown plot readings • Reduced χ² increased dramatically in the known pulsar, J2037+1942

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