marcus ziegler scipp/ucscpulsar meeting dc2 1 fourier transform with differences on simulated and...
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Marcus Ziegler SCIPP/UCSC Pulsar Meeting DC2 1
Fourier Transform with differences on Fourier Transform with differences on Simulated and Real Pulsar DataSimulated and Real Pulsar Data
UPDATE UPDATE
Gamma-ray Large Gamma-ray Large Area Space Area Space TelescopeTelescope
Marcus Ziegler
Bill Atwood
Brian Baughman
Robert Johnson
Marcus Ziegler SCIPP/UCSC Pulsar Meeting DC2 2
Basic IdeaBasic Idea
take only differences with t < max_diff
typical max_diff = 10 000stypical EGRET viewingperiod ~ 1 000 000s
Calculate the Fourier-Transform of the
time differences of the photon arrival times tn.
Marcus Ziegler SCIPP/UCSC Pulsar Meeting DC2 3
Dependence on max_diffDependence on max_diffThe dependence of the signal width on max_diff
-0 .001 -0.0005 0 0.0005 0.0010
0.2
0.4
0.6
0.8
1
FT+differnces
F + f in Hz0
Po
we
r
max_diff = 2000 s
-0. 001 -0.0005 0 0.0005 0.0010
0.2
0.4
0.6
0.8
1
FT+differnces
F + f in Hz0
Pow
er
max_diff = 10000 s
-0. 001 -0.0005 0 0.0005 0.0010
0.2
0.4
0.6
0.8
1
FT+differnces
F + f in Hz0
Pow
er
max_diff = 100000 s
Pulse width ~ 1/max_diff
Simmulated Pulsar at 10Hz
Power RMS off peak is called Noise
Small max_diff+ Small number of differences (fast)+ Coarse stepping in Frequency space (fast)-Large noise (Small S/N ratio)
Large max_diff+ Good S/N ratio- Large number of differences (very slow)
Marcus Ziegler SCIPP/UCSC Pulsar Meeting DC2 4
Blind Search for VELABlind Search for VELAVELA Viewing Period VP 7max_diff 10 000sScan region 1 Hz – 100 Hz
S/N
F in Hz
VELA
S/N
F in Hz
VELA
Number of Photons 1 197Number of differences 22 700Number F trials 2 000 000Calculations 52 800 000 000took 4h 30 min
F0 catalog 11.19888756F0 from search 11.19882249
F1 catalog -0.1557 E-10F1 from search 0.0850 E-10
F0 trials with S/N > 10
Refined search around good F0 candidates
Marcus Ziegler SCIPP/UCSC Pulsar Meeting DC2 5
Blind Search for GEMINGABlind Search for GEMINGAGEMINGA Viewing Period VP 10max_diff 10 000sScan region 1 Hz – 100 Hz
Number of Photons 1 200Number of differences 12 300Number F trials 2 000 000Calculations 2 400 000 000took 3h 30 min
F0 catalog 4.2177501F0 from search 4.2176815
F1 catalog -0.00195 E-10F1 from search -0.00935 E-10
0 20 40 60 80 100
10
20
30
40
50
60
70S/N
F in Hz
0 2 4 6 8 10 12 14 16 18 200
100
200
300
400
500
600
700S/N
F in Hz
F0 trials with S/N > 10
Refined search around good F0 candidates
Marcus Ziegler SCIPP/UCSC Pulsar Meeting DC2 6
The large F1 of CRABThe large F1 of CRAB
Simmulate Pulsar F0 = 10HzF1 = -3.0 E-10
F1 GEMINGA -0.00195 E-10F1 VELA -0.15666 E-10F1 CRAB -3.86228 E-10
Scan in F1 @ 10 Hz, max_diff 10 000s
-F1
Po
wer
-F1
Po
wer
Scan in F1 CRAB max_diff 10 000s
Marcus Ziegler SCIPP/UCSC Pulsar Meeting DC2 7
F0 and F1 Scan for CRABF0 and F1 Scan for CRAB
Scan in F CRAB max_diff 10 000sF1 steps @ 10Hz 0.05 E-10F1 steps @ 30Hz 0.15 E-10
F0 catalog 30.2254F0 from search 29.9493
F1 catalog -3.8623 E-10F1 from search -3.7719 E-10
Epoch CRAB 40000Epoch Search 48393
Calculations took 4d 16h