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Found Pulsars with Diofferncing

The Gamma-ray Large Area Space Telescope has made significant strides in astrophysics by discovering new pulsars. This groundbreaking research includes detailed observations using various viewing periods, such as VP-10 for GEMINGA, VELA, and CRAB pulsars. Through advanced data analysis techniques, including differential measurements and signal-to-noise ratio calculations, researchers like Marcus Ziegler, Bill Atwood, and Brian Baughman have unveiled essential characteristics of pulsars, contributing to our understanding of the universe.

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Found Pulsars with Diofferncing

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  1. Gamma-ray Large Area Space Telescope Found Pulsars with Diofferncing Marcus Ziegler Bill Atwood Brian Baughman Robert Johnson

  2. GEMINGA VP-10 GEMINGA Viewing Period VP-10 epoch = 43946.00 Pulsar_L = 195.13 Pulsar_B = 4.27 R=2 deg around source f0 = 2*4.21775012277 f1 = -0.1952379E-12 (not corrected for) f2 = 0.28E-24 (not corrected for) 1200 events in 2 deg Radius Max_diff 10 000s 26681 Differences S/N for peak 51 Frequencysteps 2E-5 Hz Range in plot +- 2E-2 Hz 2000 Points in Plot Calculation took 5s

  3. VELA VP-7 Crab Viewing Period VP-7 epoch = 51559.319 Pulsar_L = 263.55 Pulsar_B = -2.79 R=2 deg around source f0 = 11.1946499395 f1 = -1.5666E-11 (not corrected for) f2 = 1.028E-21 (not corrected for) 1197 events in 2 deg Radius Max_diff 10 000s 26681 Differences S/N for peak 492 Frequencysteps 2E-5 Hz Range in plot +- 2E-2 Hz 2000 Points in Plot Calculation took 10s

  4. CRAB VP-10 Crab Viewing Period VP10 epoch = 40000.00 Pulsar_L = 184.56 Pulsar_B = -5.78 R=2 deg around source f0 = 30.2253744 f1 = -3.86228E-10 f2 = 1.2426E-20 1166 events in 2 deg Radius Max_diff 100 000s 112682 Differences S/N for peak 86 Frequencysteps 2E-6 Hz Range in plot +- 2E-3 Hz 2000 Points in Plot Calculation took 40s

  5. B1706-44 VP-10 B1706-44 Period VP50 epoch = 50042.00 Pulsar_L = 343.10 Pulsar_B = -2.69 R=2 deg around source f0 = 9.7599781350 f1 = -8.857444E-12 f2 = 173.1E-24 869 events in 2 deg Radius Max_diff 100 000s 60742 Differences S/N for peak 38 Frequencysteps 2E-6 Hz Range in plot +- 2E-3 Hz 2000 Points in Plot Calculation took 25s

  6. B1055-52 VP-0140 B1055.52 Period VP0140 epoch = 43555.6172 Pulsar_L = 285.98 Pulsar_B = 6.65 R=2 deg around source f0 = 5.0733708820 f1 = -1.50149E-13 f2 = NA 628 events in 2 deg Radius Max_diff 1 000 000s 188930 Differences S/N for peak 15.7 Frequencysteps 2E-6 Hz Range in plot +- 2E-3 Hz 2000 Points in Plot

  7. B1951+32 Phase 1234 epoch 49845.00 Phase 1-4 Pulsar_L = 68.77 Pulsar_B = 2.82 r=2 f0 = 25.2964792556 f1 = -3.740159E-12 f2 = 1.462E-23 2939 events in 2 deg Radius Max_diff 500 000s 188930 Differences S/N for peak ~10 Frequencysteps 2E-6 Hz Range in plot +- 5E-3 Hz 5000 Points in Plot

  8. B1509-58 Phase 1234 epoch 48355 Pulsar_L = 320.32 Pulsar_B = -1.16 r=2 f0 = 6.637 f1 = -6.76E-11 f2 = 1.958E-21 Max_diff 1 000 000s Frequencysteps 1E-6 Hz

  9. J1930+1852 Phase 1234 NAME J1930+1852 PSRJ J1930+1852 POSEPOCH 52280.00 GL 54.10 GB 0.27 F0 7.3070012560 F1 -4.00746E-11 Max_diff 100 000s Frequencysteps 2E-6 Hz

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