SlideShare a Scribd company logo
1 of 13
Download to read offline
T. Fujii (ICRR), M. Malacari, J. Albury, J.A. Bellido, J. Farmer, A. Galimova, P. Horvath,
M. Hrabovsky, D. Mandat, A. Matalon, J.N. Matthews, M. Merolle, X. Ni, L. Nozka,
M. Palatka, M. Pech, P. Privitera, P. Schovanek, S.B. Thomas, P. Travnicek
72 2017 3 17
http://www.fast-project.org
FAST 4
FAST
TA
Credit: Max Malacari
EUSO-TA
Fine pixelated camera
Low-cost and simplified/optimized FD
Too expensive to cover a huge area
2
Single or few pixels and smaller optics
Fluorescence detector Array of Single-pixel Telescopes
Segmented mirror telescope
Variable angles of elevation – steps.
15 deg 45 deg
✦ > 1019.5 eV
✦ (30,000 km2, 10×Auger or TA×4) ⇒
FAST
3
✦ EUSO-TA 1
✦
✦
✦ Astroparticle Physics, 74 (2016) 64-72
✦
✦ FAST (
FAST )
(Xmax)
EUSO-TA
telescope
+ FAST camera
Fig. 12. A 1018
eV shower simultaneously detected by the TA FD and the FAST protot
superimposed (see Fig. 11). In (b), the corresponding FADC trace recorded by the FAS
Fig. 6. FADC signal recorded for a YAP light pulse. It is used to monitor the relative gain
of the PMT.
Fig. 7. Variation of the YAP signal during a seven hour data taking run.
70 T. Fujii et al. / Astroparticle Physics 74 (2016) 64–72
Vertical Laser
~1019.3 eV
Cosmic Ray
~1018.0 eV
FAST - progress in design and construction
UV Plexiglass Segmented primary mirror8 inch PMT camera
(2 x 2)
1m2 aperture
FOV = 25°x 25°
variable
tilt
Joint Laboratory of Optics Olomouc – Malargue November 2015
Prototype - October 2015
15°
45°
4Joint Laboratory of Optics in Olomouc, Czech Republic
FAST
UV band-pass
filter
5
FAST
2016 10
http://www.fast-project.org
Produced by D. Mandat and M. Malacari
FAST (2016 10 )
6
FAST
7
✦ (TA)
✦ 10 MHz, 80 µs
✦ TA 21
km
Time (100 ns)
0 100 200 300 400 500 600 700 800
-30
-20
Time (100 ns)
0 100 200 300 400 500 600 700 800
-30
-20
Time (100 ns)
0 100 200 300 400 500 600 700 800
/(100ns)p.e.N
-20
-10
0
10
20
30
PMT 2
Time (100 ns)
0 100 200 300 400 500 600 700 800
/(100ns)p.e.N
-20
-10
0
10
20
30
40
PMT 4
80 µs
100
( )
()
FAST
8
✦ : 62194 events
:
PMT 1 PMT 3
PMT 2 PMT 4
: 2016 10 5
Time (100 ns)
0 100 200 300 400 500 600 700 800
/(100ns)p.e.N
-30
-20
-10
0
10
20
30
40
PMT 1
Time (100 ns)
0 100 200 300 400 500 600 700 800
/(100ns)p.e.N
-30
-20
-10
0
10
20
30
PMT 3
Time (100 ns)
0 100 200 300 400 500 600 700 800
/(100ns)p.e.N
-20
-10
0
10
20
30
PMT 2
Time (100 ns)
0 100 200 300 400 500 600 700 800
/(100ns)p.e.N
-20
-10
0
10
20
30
40
PMT 4
Time (100 ns)
0 100 200 300 400 500 600 700 800
/(100ns)p.e.N
-20
0
20
40
60
80
100
PMT 1
Time (100 ns)
0 100 200 300 400 500 600 700 800
/(100ns)p.e.N
-30
-20
-10
0
10
20
30
40
PMT 3
Time (100 ns)
0 100 200 300 400 500 600 700 800
/(100ns)p.e.N
-20
0
20
40
60
80
100
120
140
PMT 2
Time (100 ns)
0 100 200 300 400 500 600 700 800
/(100ns)p.e.N
-20
-10
0
10
20
30
40
PMT 4
[]
Time (100 ns)
0 100 200 300 400 500 600 700 800
/(100ns)p.e.N
0
200
400
600
800
1000
1200
PMT 1
Time (100 ns)
0 100 200 300 400 500 600 700 800
/(100ns)p.e.N
0
200
400
600
800
1000
PMT 3
Time (100 ns)
0 100 200 300 400 500 600 700 800
/(100ns)p.e.N
0
200
400
600
800
1000
PMT 2
Time (100 ns)
0 100 200 300 400 500 600 700 800
/(100ns)p.e.N
0
200
400
600
800
1000
PMT 4
: 2016 10 5
9
✦ ->PMT -> (>35 µs)-> ->2 PMT
✦ 62194 -> 4290 -> 3950 -> 389 -> 90 events
Event 387: log10(E(eV)): 18.68, Zen: 61.0◦
, Azi: 63.3◦
,
Core(11.86, -11.50), Rp: 3.52, Psi: 42.8◦
, Xmax: 1113 g/cm2
FoV(1407 - 1769), Date: 20161005, Time: 06:07:38.800548560
Event 388: log10(E(eV)): 17.96, Zen: 38.8◦
, Azi: -19.6◦
,
Core(8.90, -17.03), Rp: 9.44, Psi: 82.6◦
, Xmax: 768 g/cm2
FoV(498 - 1017), Date: 20161005, Time: 06:30:06.947113522
Event 389: log10(E(eV)): 17.83, Zen: 4.7◦
, Azi: 115.2◦
,
Core(14.23, -5.41), Rp: 7.18, Psi: 86.7◦
, Xmax: 656 g/cm2
FoV(473 - 850), Date: 20161005, Time: 06:35:10.462924009
Event 393: log10(E(eV)): 18.14, Zen: 31.6◦
, Azi: 2.8◦
,
Core(6.02, -6.69), Rp: 11.96, Psi: 102.1◦
, Xmax: 762 g/cm2
FoV(373 - 991), Date: 20161005, Time: 06:51:48.292842002
Event 394: log10(E(eV)): 18.69, Zen: 61.2◦
, Azi: -9.4◦
,
Core(9.58, -20.15), Rp: 9.27, Psi: 57.3◦
, Xmax: 1021 g/cm2
FoV(829 - 1221), Date: 20161005, Time: 06:53:27.011365323
Event 395: log10(E(eV)): 18.26, Zen: 17.7◦
, Azi: -82.0◦
,
Core(13.53, -2.14), Rp: 10.39, Psi: 98.2◦
, Xmax: 769 g/cm2
FoV(303 - 890), Date: 20161005, Time: 06:53:43.909532618
10
Time (100 ns)
0 100 200 300 400 500 600 700 800
/(100ns)p.e.N
-40
-20
0
20
40
60
PMT 1
Time (100 ns)
0 100 200 300 400 500 600 700 800
/(100ns)p.e.N
-20
-10
0
10
20
30
40
PMT 3
Time (100 ns)
0 100 200 300 400 500 600 700 800
/(100ns)p.e.N
-40
-30
-20
-10
0
10
20
30
40
50
PMT 2
Time (100 ns)
0 100 200 300 400 500 600 700 800
/(100ns)p.e.N
-30
-20
-10
0
10
20
30
40
PMT 4
2016/10/05 06:37:49.525424540
Time (100 ns)
0 100 200 300 400 500 600 700 800
/(100ns)p.e.N
0
500
1000
1500
2000
PMT 1
Time (100 ns)
0 100 200 300 400 500 600 700 800
/(100ns)p.e.N
0
50
100
150
200
250
300
350
PMT 3
Time (100 ns)
0 100 200 300 400 500 600 700 800
/(100ns)p.e.N
0
200
400
600
800
1000
PMT 2
Time (100 ns)
0 100 200 300 400 500 600 700 800
/(100ns)p.e.N
0
50
100
150
200
250
300
PMT 4
2016/10/05 10:25:50.781802380
TAFD
logE = 18.08
Rp = 2.40 km
Too
close
11
Time (100 ns)
0 100 200 300 400 500 600 700 800
/(100ns)p.e.N
-30
-20
-10
0
10
20
30
40
50
60
PMT 1
Time (100 ns)
0 100 200 300 400 500 600 700 800
/(100ns)p.e.N
0
50
100
150
200
PMT 3
Time (100 ns)
0 100 200 300 400 500 600 700 800
/(100ns)p.e.N
-20
0
20
40
60
80
PMT 2
Time (100 ns)
0 100 200 300 400 500 600 700 800
/(100ns)p.e.N
-20
0
20
40
60
80
100
120
PMT 4
Time (100 ns)
0 100 200 300 400 500 600 700 800
/(100ns)p.e.N
-50
0
50
100
150
200
PMT 1
Time (100 ns)
0 100 200 300 400 500 600 700 800
/(100ns)p.e.N
-30
-20
-10
0
10
20
30
40
PMT 3
Time (100 ns)
0 100 200 300 400 500 600 700 800
/(100ns)p.e.N
-20
0
20
40
60
80
PMT 2
Time (100 ns)
0 100 200 300 400 500 600 700 800
/(100ns)p.e.N
-20
-10
0
10
20
PMT 4
Time (100 ns)
0 100 200 300 400 500 600 700 800
/(100ns)p.e.N
0
50
100
150
200
250
300
350
PMT 1
Time (100 ns)
0 100 200 300 400 500 600 700 800
/(100ns)p.e.N
-20
0
20
40
60
80
PMT 3
Time (100 ns)
0 100 200 300 400 500 600 700 800
/(100ns)p.e.N
-20
-10
0
10
20
30
PMT 2
Time (100 ns)
0 100 200 300 400 500 600 700 800
/(100ns)p.e.N
-20
-10
0
10
20
30
40
50
PMT 4
Time (100 ns)
0 100 200 300 400 500 600 700 800
/(100ns)p.e.N
0
50
100
150
200
PMT 1
Time (100 ns)
0 100 200 300 400 500 600 700 800
/(100ns)p.e.N
-20
0
20
40
60
80
100
120
PMT 3
Time (100 ns)
0 100 200 300 400 500 600 700 800
/(100ns)p.e.N
-20
0
20
40
60
80
100
PMT 2
Time (100 ns)
0 100 200 300 400 500 600 700 800
/(100ns)p.e.N
-20
0
20
40
60
80
PMT 4
128
18
Time (100 ns)
0 100 200 300 400 500 600 700 800
/(100ns)p.e.N
0
5
10
15
20
12
✦ 21 km
284
✦
✦ (
)
✦
✦ PMT
✦ PMT
( )
✦
( )
Sum
PMT 1
PMT 3
PMT 2
PMT 4
( )
Simulation
(Preliminary)
Data
11
Optical simulation status
FAST Simulation - example
- PSF (7.5deg diagonal) aperture input 0.5W 0.43W/PMT1, <0.001W/PMT234 (eff: 86%)
10
Optical simulation status
- axis): aperture input 0.5W 4x0.04W/PMT (eff: 32%)
FAST Simulation - example
13
✦ Fluorescence detector Array of Single-pixel Telescopes (FAST)
✦
✦ FAST
✦ 2016 10 2017 1
✦ 128 18
✦ 21 km
✦
✦ 2017 1 25 GPS
✦
✦ 2017 6 FAST GPS DAQ
✦ http://www.fast-project.org

More Related Content

What's hot

Fluorescence detector Array of Single-pixel Telescopes (FAST) project
Fluorescence detector Array of Single-pixel Telescopes (FAST) projectFluorescence detector Array of Single-pixel Telescopes (FAST) project
Fluorescence detector Array of Single-pixel Telescopes (FAST) projectToshihiro FUJII
 
A Conceptual Design for a Large Ground Array of Fluorescence Detectors
A Conceptual Design for a Large Ground Array of Fluorescence DetectorsA Conceptual Design for a Large Ground Array of Fluorescence Detectors
A Conceptual Design for a Large Ground Array of Fluorescence DetectorsToshihiro FUJII
 
Future Prospects on UHECR and UHE Photon
Future Prospects on UHECR and UHE PhotonFuture Prospects on UHECR and UHE Photon
Future Prospects on UHECR and UHE PhotonToshihiro FUJII
 
The FAST Project - Next Generation UHECR Observatory -
The FAST Project - Next Generation UHECR Observatory -The FAST Project - Next Generation UHECR Observatory -
The FAST Project - Next Generation UHECR Observatory -Toshihiro FUJII
 
FAST実験6:新型大気蛍光望遠鏡による観測報告とピエールオージェ観測所への設置計画
FAST実験6:新型大気蛍光望遠鏡による観測報告とピエールオージェ観測所への設置計画FAST実験6:新型大気蛍光望遠鏡による観測報告とピエールオージェ観測所への設置計画
FAST実験6:新型大気蛍光望遠鏡による観測報告とピエールオージェ観測所への設置計画Toshihiro FUJII
 
Talents up grazioli cesare_20_05_2013
Talents up grazioli cesare_20_05_2013Talents up grazioli cesare_20_05_2013
Talents up grazioli cesare_20_05_2013AREA Science Park
 
FR3T10-4-IGARSS_Aalto-1_Praks.pptx
FR3T10-4-IGARSS_Aalto-1_Praks.pptxFR3T10-4-IGARSS_Aalto-1_Praks.pptx
FR3T10-4-IGARSS_Aalto-1_Praks.pptxgrssieee
 
Top quark physics at the LHC
Top quark physics at the LHCTop quark physics at the LHC
Top quark physics at the LHCAkira Shibata
 
Slightly fishy - Combining NSOM with SEA TADPOLE
Slightly fishy - Combining NSOM with SEA TADPOLESlightly fishy - Combining NSOM with SEA TADPOLE
Slightly fishy - Combining NSOM with SEA TADPOLEJohanna Trägårdh
 

What's hot (10)

Fluorescence detector Array of Single-pixel Telescopes (FAST) project
Fluorescence detector Array of Single-pixel Telescopes (FAST) projectFluorescence detector Array of Single-pixel Telescopes (FAST) project
Fluorescence detector Array of Single-pixel Telescopes (FAST) project
 
A Conceptual Design for a Large Ground Array of Fluorescence Detectors
A Conceptual Design for a Large Ground Array of Fluorescence DetectorsA Conceptual Design for a Large Ground Array of Fluorescence Detectors
A Conceptual Design for a Large Ground Array of Fluorescence Detectors
 
Future Prospects on UHECR and UHE Photon
Future Prospects on UHECR and UHE PhotonFuture Prospects on UHECR and UHE Photon
Future Prospects on UHECR and UHE Photon
 
The FAST Project - Next Generation UHECR Observatory -
The FAST Project - Next Generation UHECR Observatory -The FAST Project - Next Generation UHECR Observatory -
The FAST Project - Next Generation UHECR Observatory -
 
FAST実験6:新型大気蛍光望遠鏡による観測報告とピエールオージェ観測所への設置計画
FAST実験6:新型大気蛍光望遠鏡による観測報告とピエールオージェ観測所への設置計画FAST実験6:新型大気蛍光望遠鏡による観測報告とピエールオージェ観測所への設置計画
FAST実験6:新型大気蛍光望遠鏡による観測報告とピエールオージェ観測所への設置計画
 
Talents up grazioli cesare_20_05_2013
Talents up grazioli cesare_20_05_2013Talents up grazioli cesare_20_05_2013
Talents up grazioli cesare_20_05_2013
 
FR3T10-4-IGARSS_Aalto-1_Praks.pptx
FR3T10-4-IGARSS_Aalto-1_Praks.pptxFR3T10-4-IGARSS_Aalto-1_Praks.pptx
FR3T10-4-IGARSS_Aalto-1_Praks.pptx
 
Top quark physics at the LHC
Top quark physics at the LHCTop quark physics at the LHC
Top quark physics at the LHC
 
New microsoft-word-document
New microsoft-word-documentNew microsoft-word-document
New microsoft-word-document
 
Slightly fishy - Combining NSOM with SEA TADPOLE
Slightly fishy - Combining NSOM with SEA TADPOLESlightly fishy - Combining NSOM with SEA TADPOLE
Slightly fishy - Combining NSOM with SEA TADPOLE
 

Similar to FAST実験4:大気蛍光望遠鏡による極高エネルギー宇宙線観測報告

First results from the full-scale prototype for the Fluorescence detector Arr...
First results from the full-scale prototype for the Fluorescence detector Arr...First results from the full-scale prototype for the Fluorescence detector Arr...
First results from the full-scale prototype for the Fluorescence detector Arr...Toshihiro FUJII
 
A next-generation ground array for the detection of ultrahigh-energy cosmic r...
A next-generation ground array for the detection of ultrahigh-energy cosmic r...A next-generation ground array for the detection of ultrahigh-energy cosmic r...
A next-generation ground array for the detection of ultrahigh-energy cosmic r...Toshihiro FUJII
 
SPECTRAL-BASED FATIGUE ASSESSMENT OF FSO
SPECTRAL-BASED FATIGUE ASSESSMENT OF FSOSPECTRAL-BASED FATIGUE ASSESSMENT OF FSO
SPECTRAL-BASED FATIGUE ASSESSMENT OF FSOSUMARDIONO .
 
Heated Supersonic Jet Noise
Heated Supersonic Jet NoiseHeated Supersonic Jet Noise
Heated Supersonic Jet NoisePablo Mora
 
Monte Carlo Simulation
Monte Carlo SimulationMonte Carlo Simulation
Monte Carlo SimulationAguinaldo Flor
 
Next-Generation Observatory: Fluorescence detector Array of Single Pixel Tele...
Next-Generation Observatory: Fluorescence detector Array of Single Pixel Tele...Next-Generation Observatory: Fluorescence detector Array of Single Pixel Tele...
Next-Generation Observatory: Fluorescence detector Array of Single Pixel Tele...Toshihiro FUJII
 
Analysis of the Blade Boundary-Layer Flow of a Marine Propeller with RANSE
Analysis of the Blade Boundary-Layer Flow of a Marine Propeller with RANSEAnalysis of the Blade Boundary-Layer Flow of a Marine Propeller with RANSE
Analysis of the Blade Boundary-Layer Flow of a Marine Propeller with RANSEJoão Baltazar
 
Observing ultra-high energy cosmic rays with prototypes of the Fluorescence d...
Observing ultra-high energy cosmic rays with prototypes of the Fluorescence d...Observing ultra-high energy cosmic rays with prototypes of the Fluorescence d...
Observing ultra-high energy cosmic rays with prototypes of the Fluorescence d...Toshihiro FUJII
 
Time-Frequency Representation of Microseismic Signals using the SST
Time-Frequency Representation of Microseismic Signals using the SSTTime-Frequency Representation of Microseismic Signals using the SST
Time-Frequency Representation of Microseismic Signals using the SSTUT Technology
 
FAST実験3:新型大気蛍光望遠鏡の試験観測報告
FAST実験3:新型大気蛍光望遠鏡の試験観測報告FAST実験3:新型大気蛍光望遠鏡の試験観測報告
FAST実験3:新型大気蛍光望遠鏡の試験観測報告Toshihiro FUJII
 
データセンター省エネ化技術トレンド2018
データセンター省エネ化技術トレンド2018データセンター省エネ化技術トレンド2018
データセンター省エネ化技術トレンド2018Tadashi Sugita
 
Nx calrics2019 yano-presentation
Nx calrics2019 yano-presentationNx calrics2019 yano-presentation
Nx calrics2019 yano-presentationShinichiro Yano
 
Iván Brihuega-Probing graphene physics at the atomic scale
Iván Brihuega-Probing graphene physics at the atomic scaleIván Brihuega-Probing graphene physics at the atomic scale
Iván Brihuega-Probing graphene physics at the atomic scaleFundación Ramón Areces
 
The use of a 3-C array for regional monitoring
The use of a 3-C array for regional monitoringThe use of a 3-C array for regional monitoring
The use of a 3-C array for regional monitoringIvan Kitov
 
Trends in Future CommunicationsInternational Workshop - Renato Rabelo
Trends in Future CommunicationsInternational Workshop - Renato RabeloTrends in Future CommunicationsInternational Workshop - Renato Rabelo
Trends in Future CommunicationsInternational Workshop - Renato RabeloCPqD
 

Similar to FAST実験4:大気蛍光望遠鏡による極高エネルギー宇宙線観測報告 (20)

First results from the full-scale prototype for the Fluorescence detector Arr...
First results from the full-scale prototype for the Fluorescence detector Arr...First results from the full-scale prototype for the Fluorescence detector Arr...
First results from the full-scale prototype for the Fluorescence detector Arr...
 
A next-generation ground array for the detection of ultrahigh-energy cosmic r...
A next-generation ground array for the detection of ultrahigh-energy cosmic r...A next-generation ground array for the detection of ultrahigh-energy cosmic r...
A next-generation ground array for the detection of ultrahigh-energy cosmic r...
 
SPECTRAL-BASED FATIGUE ASSESSMENT OF FSO
SPECTRAL-BASED FATIGUE ASSESSMENT OF FSOSPECTRAL-BASED FATIGUE ASSESSMENT OF FSO
SPECTRAL-BASED FATIGUE ASSESSMENT OF FSO
 
Heated Supersonic Jet Noise
Heated Supersonic Jet NoiseHeated Supersonic Jet Noise
Heated Supersonic Jet Noise
 
Monte Carlo Simulation
Monte Carlo SimulationMonte Carlo Simulation
Monte Carlo Simulation
 
Next-Generation Observatory: Fluorescence detector Array of Single Pixel Tele...
Next-Generation Observatory: Fluorescence detector Array of Single Pixel Tele...Next-Generation Observatory: Fluorescence detector Array of Single Pixel Tele...
Next-Generation Observatory: Fluorescence detector Array of Single Pixel Tele...
 
Laser drivenplasma
Laser drivenplasmaLaser drivenplasma
Laser drivenplasma
 
Analysis of the Blade Boundary-Layer Flow of a Marine Propeller with RANSE
Analysis of the Blade Boundary-Layer Flow of a Marine Propeller with RANSEAnalysis of the Blade Boundary-Layer Flow of a Marine Propeller with RANSE
Analysis of the Blade Boundary-Layer Flow of a Marine Propeller with RANSE
 
Observing ultra-high energy cosmic rays with prototypes of the Fluorescence d...
Observing ultra-high energy cosmic rays with prototypes of the Fluorescence d...Observing ultra-high energy cosmic rays with prototypes of the Fluorescence d...
Observing ultra-high energy cosmic rays with prototypes of the Fluorescence d...
 
Time-Frequency Representation of Microseismic Signals using the SST
Time-Frequency Representation of Microseismic Signals using the SSTTime-Frequency Representation of Microseismic Signals using the SST
Time-Frequency Representation of Microseismic Signals using the SST
 
FAST実験3:新型大気蛍光望遠鏡の試験観測報告
FAST実験3:新型大気蛍光望遠鏡の試験観測報告FAST実験3:新型大気蛍光望遠鏡の試験観測報告
FAST実験3:新型大気蛍光望遠鏡の試験観測報告
 
sm ch2 open akan.pdf
sm ch2 open akan.pdfsm ch2 open akan.pdf
sm ch2 open akan.pdf
 
データセンター省エネ化技術トレンド2018
データセンター省エネ化技術トレンド2018データセンター省エネ化技術トレンド2018
データセンター省エネ化技術トレンド2018
 
Nx calrics2019 yano-presentation
Nx calrics2019 yano-presentationNx calrics2019 yano-presentation
Nx calrics2019 yano-presentation
 
Iván Brihuega-Probing graphene physics at the atomic scale
Iván Brihuega-Probing graphene physics at the atomic scaleIván Brihuega-Probing graphene physics at the atomic scale
Iván Brihuega-Probing graphene physics at the atomic scale
 
Advantage of HRAM
Advantage of HRAMAdvantage of HRAM
Advantage of HRAM
 
The use of a 3-C array for regional monitoring
The use of a 3-C array for regional monitoringThe use of a 3-C array for regional monitoring
The use of a 3-C array for regional monitoring
 
PGS_ActiveFleet_2017_1Q
PGS_ActiveFleet_2017_1QPGS_ActiveFleet_2017_1Q
PGS_ActiveFleet_2017_1Q
 
Aofd farid
Aofd faridAofd farid
Aofd farid
 
Trends in Future CommunicationsInternational Workshop - Renato Rabelo
Trends in Future CommunicationsInternational Workshop - Renato RabeloTrends in Future CommunicationsInternational Workshop - Renato Rabelo
Trends in Future CommunicationsInternational Workshop - Renato Rabelo
 

More from Toshihiro FUJII

FAST実験17: FASTミニアレイ建設に向けた進捗報告(日本物理学会2024年春季大会)
FAST実験17: FASTミニアレイ建設に向けた進捗報告(日本物理学会2024年春季大会)FAST実験17: FASTミニアレイ建設に向けた進捗報告(日本物理学会2024年春季大会)
FAST実験17: FASTミニアレイ建設に向けた進捗報告(日本物理学会2024年春季大会)Toshihiro FUJII
 
FAST実験14:新型大気蛍光望遠鏡による南北半球での極高エネルギー宇宙線観測と自立稼働へ向けた開発研究
FAST実験14:新型大気蛍光望遠鏡による南北半球での極高エネルギー宇宙線観測と自立稼働へ向けた開発研究FAST実験14:新型大気蛍光望遠鏡による南北半球での極高エネルギー宇宙線観測と自立稼働へ向けた開発研究
FAST実験14:新型大気蛍光望遠鏡による南北半球での極高エネルギー宇宙線観測と自立稼働へ向けた開発研究Toshihiro FUJII
 
20220906_FAST_JPS_nagasawa.pdf
20220906_FAST_JPS_nagasawa.pdf20220906_FAST_JPS_nagasawa.pdf
20220906_FAST_JPS_nagasawa.pdfToshihiro FUJII
 
Atmospheric monitoring with the Fluorescence detector Array of Single-pixel T...
Atmospheric monitoring with the Fluorescence detector Array of Single-pixel T...Atmospheric monitoring with the Fluorescence detector Array of Single-pixel T...
Atmospheric monitoring with the Fluorescence detector Array of Single-pixel T...Toshihiro FUJII
 
Future ground arrays for ultrahigh-energy cosmic rays: recent updates and per...
Future ground arrays for ultrahigh-energy cosmic rays: recent updates and per...Future ground arrays for ultrahigh-energy cosmic rays: recent updates and per...
Future ground arrays for ultrahigh-energy cosmic rays: recent updates and per...Toshihiro FUJII
 
大気蛍光望遠鏡による極高エネルギー宇宙線スペクトルの研究
大気蛍光望遠鏡による極高エネルギー宇宙線スペクトルの研究大気蛍光望遠鏡による極高エネルギー宇宙線スペクトルの研究
大気蛍光望遠鏡による極高エネルギー宇宙線スペクトルの研究Toshihiro FUJII
 
FAST実験2:新型大気蛍光望遠鏡の性能評価
FAST実験2:新型大気蛍光望遠鏡の性能評価FAST実験2:新型大気蛍光望遠鏡の性能評価
FAST実験2:新型大気蛍光望遠鏡の性能評価Toshihiro FUJII
 

More from Toshihiro FUJII (7)

FAST実験17: FASTミニアレイ建設に向けた進捗報告(日本物理学会2024年春季大会)
FAST実験17: FASTミニアレイ建設に向けた進捗報告(日本物理学会2024年春季大会)FAST実験17: FASTミニアレイ建設に向けた進捗報告(日本物理学会2024年春季大会)
FAST実験17: FASTミニアレイ建設に向けた進捗報告(日本物理学会2024年春季大会)
 
FAST実験14:新型大気蛍光望遠鏡による南北半球での極高エネルギー宇宙線観測と自立稼働へ向けた開発研究
FAST実験14:新型大気蛍光望遠鏡による南北半球での極高エネルギー宇宙線観測と自立稼働へ向けた開発研究FAST実験14:新型大気蛍光望遠鏡による南北半球での極高エネルギー宇宙線観測と自立稼働へ向けた開発研究
FAST実験14:新型大気蛍光望遠鏡による南北半球での極高エネルギー宇宙線観測と自立稼働へ向けた開発研究
 
20220906_FAST_JPS_nagasawa.pdf
20220906_FAST_JPS_nagasawa.pdf20220906_FAST_JPS_nagasawa.pdf
20220906_FAST_JPS_nagasawa.pdf
 
Atmospheric monitoring with the Fluorescence detector Array of Single-pixel T...
Atmospheric monitoring with the Fluorescence detector Array of Single-pixel T...Atmospheric monitoring with the Fluorescence detector Array of Single-pixel T...
Atmospheric monitoring with the Fluorescence detector Array of Single-pixel T...
 
Future ground arrays for ultrahigh-energy cosmic rays: recent updates and per...
Future ground arrays for ultrahigh-energy cosmic rays: recent updates and per...Future ground arrays for ultrahigh-energy cosmic rays: recent updates and per...
Future ground arrays for ultrahigh-energy cosmic rays: recent updates and per...
 
大気蛍光望遠鏡による極高エネルギー宇宙線スペクトルの研究
大気蛍光望遠鏡による極高エネルギー宇宙線スペクトルの研究大気蛍光望遠鏡による極高エネルギー宇宙線スペクトルの研究
大気蛍光望遠鏡による極高エネルギー宇宙線スペクトルの研究
 
FAST実験2:新型大気蛍光望遠鏡の性能評価
FAST実験2:新型大気蛍光望遠鏡の性能評価FAST実験2:新型大気蛍光望遠鏡の性能評価
FAST実験2:新型大気蛍光望遠鏡の性能評価
 

Recently uploaded

Is RISC-V ready for HPC workload? Maybe?
Is RISC-V ready for HPC workload? Maybe?Is RISC-V ready for HPC workload? Maybe?
Is RISC-V ready for HPC workload? Maybe?Patrick Diehl
 
Behavioral Disorder: Schizophrenia & it's Case Study.pdf
Behavioral Disorder: Schizophrenia & it's Case Study.pdfBehavioral Disorder: Schizophrenia & it's Case Study.pdf
Behavioral Disorder: Schizophrenia & it's Case Study.pdfSELF-EXPLANATORY
 
Welcome to GFDL for Take Your Child To Work Day
Welcome to GFDL for Take Your Child To Work DayWelcome to GFDL for Take Your Child To Work Day
Welcome to GFDL for Take Your Child To Work DayZachary Labe
 
Call Girls in Munirka Delhi 💯Call Us 🔝9953322196🔝 💯Escort.
Call Girls in Munirka Delhi 💯Call Us 🔝9953322196🔝 💯Escort.Call Girls in Munirka Delhi 💯Call Us 🔝9953322196🔝 💯Escort.
Call Girls in Munirka Delhi 💯Call Us 🔝9953322196🔝 💯Escort.aasikanpl
 
Call Girls in Munirka Delhi 💯Call Us 🔝8264348440🔝
Call Girls in Munirka Delhi 💯Call Us 🔝8264348440🔝Call Girls in Munirka Delhi 💯Call Us 🔝8264348440🔝
Call Girls in Munirka Delhi 💯Call Us 🔝8264348440🔝soniya singh
 
Artificial Intelligence In Microbiology by Dr. Prince C P
Artificial Intelligence In Microbiology by Dr. Prince C PArtificial Intelligence In Microbiology by Dr. Prince C P
Artificial Intelligence In Microbiology by Dr. Prince C PPRINCE C P
 
Harmful and Useful Microorganisms Presentation
Harmful and Useful Microorganisms PresentationHarmful and Useful Microorganisms Presentation
Harmful and Useful Microorganisms Presentationtahreemzahra82
 
Call Us ≽ 9953322196 ≼ Call Girls In Lajpat Nagar (Delhi) |
Call Us ≽ 9953322196 ≼ Call Girls In Lajpat Nagar (Delhi) |Call Us ≽ 9953322196 ≼ Call Girls In Lajpat Nagar (Delhi) |
Call Us ≽ 9953322196 ≼ Call Girls In Lajpat Nagar (Delhi) |aasikanpl
 
BIOETHICS IN RECOMBINANT DNA TECHNOLOGY.
BIOETHICS IN RECOMBINANT DNA TECHNOLOGY.BIOETHICS IN RECOMBINANT DNA TECHNOLOGY.
BIOETHICS IN RECOMBINANT DNA TECHNOLOGY.PraveenaKalaiselvan1
 
Call Girls in Aiims Metro Delhi 💯Call Us 🔝9953322196🔝 💯Escort.
Call Girls in Aiims Metro Delhi 💯Call Us 🔝9953322196🔝 💯Escort.Call Girls in Aiims Metro Delhi 💯Call Us 🔝9953322196🔝 💯Escort.
Call Girls in Aiims Metro Delhi 💯Call Us 🔝9953322196🔝 💯Escort.aasikanpl
 
Call Girls In Nihal Vihar Delhi ❤️8860477959 Looking Escorts In 24/7 Delhi NCR
Call Girls In Nihal Vihar Delhi ❤️8860477959 Looking Escorts In 24/7 Delhi NCRCall Girls In Nihal Vihar Delhi ❤️8860477959 Looking Escorts In 24/7 Delhi NCR
Call Girls In Nihal Vihar Delhi ❤️8860477959 Looking Escorts In 24/7 Delhi NCRlizamodels9
 
LIGHT-PHENOMENA-BY-CABUALDIONALDOPANOGANCADIENTE-CONDEZA (1).pptx
LIGHT-PHENOMENA-BY-CABUALDIONALDOPANOGANCADIENTE-CONDEZA (1).pptxLIGHT-PHENOMENA-BY-CABUALDIONALDOPANOGANCADIENTE-CONDEZA (1).pptx
LIGHT-PHENOMENA-BY-CABUALDIONALDOPANOGANCADIENTE-CONDEZA (1).pptxmalonesandreagweneth
 
Spermiogenesis or Spermateleosis or metamorphosis of spermatid
Spermiogenesis or Spermateleosis or metamorphosis of spermatidSpermiogenesis or Spermateleosis or metamorphosis of spermatid
Spermiogenesis or Spermateleosis or metamorphosis of spermatidSarthak Sekhar Mondal
 
zoogeography of pakistan.pptx fauna of Pakistan
zoogeography of pakistan.pptx fauna of Pakistanzoogeography of pakistan.pptx fauna of Pakistan
zoogeography of pakistan.pptx fauna of Pakistanzohaibmir069
 
insect anatomy and insect body wall and their physiology
insect anatomy and insect body wall and their  physiologyinsect anatomy and insect body wall and their  physiology
insect anatomy and insect body wall and their physiologyDrAnita Sharma
 
Forest laws, Indian forest laws, why they are important
Forest laws, Indian forest laws, why they are importantForest laws, Indian forest laws, why they are important
Forest laws, Indian forest laws, why they are importantadityabhardwaj282
 
Best Call Girls In Sector 29 Gurgaon❤️8860477959 EscorTs Service In 24/7 Delh...
Best Call Girls In Sector 29 Gurgaon❤️8860477959 EscorTs Service In 24/7 Delh...Best Call Girls In Sector 29 Gurgaon❤️8860477959 EscorTs Service In 24/7 Delh...
Best Call Girls In Sector 29 Gurgaon❤️8860477959 EscorTs Service In 24/7 Delh...lizamodels9
 

Recently uploaded (20)

Is RISC-V ready for HPC workload? Maybe?
Is RISC-V ready for HPC workload? Maybe?Is RISC-V ready for HPC workload? Maybe?
Is RISC-V ready for HPC workload? Maybe?
 
Behavioral Disorder: Schizophrenia & it's Case Study.pdf
Behavioral Disorder: Schizophrenia & it's Case Study.pdfBehavioral Disorder: Schizophrenia & it's Case Study.pdf
Behavioral Disorder: Schizophrenia & it's Case Study.pdf
 
Welcome to GFDL for Take Your Child To Work Day
Welcome to GFDL for Take Your Child To Work DayWelcome to GFDL for Take Your Child To Work Day
Welcome to GFDL for Take Your Child To Work Day
 
Call Girls in Munirka Delhi 💯Call Us 🔝9953322196🔝 💯Escort.
Call Girls in Munirka Delhi 💯Call Us 🔝9953322196🔝 💯Escort.Call Girls in Munirka Delhi 💯Call Us 🔝9953322196🔝 💯Escort.
Call Girls in Munirka Delhi 💯Call Us 🔝9953322196🔝 💯Escort.
 
Volatile Oils Pharmacognosy And Phytochemistry -I
Volatile Oils Pharmacognosy And Phytochemistry -IVolatile Oils Pharmacognosy And Phytochemistry -I
Volatile Oils Pharmacognosy And Phytochemistry -I
 
Call Girls in Munirka Delhi 💯Call Us 🔝8264348440🔝
Call Girls in Munirka Delhi 💯Call Us 🔝8264348440🔝Call Girls in Munirka Delhi 💯Call Us 🔝8264348440🔝
Call Girls in Munirka Delhi 💯Call Us 🔝8264348440🔝
 
Artificial Intelligence In Microbiology by Dr. Prince C P
Artificial Intelligence In Microbiology by Dr. Prince C PArtificial Intelligence In Microbiology by Dr. Prince C P
Artificial Intelligence In Microbiology by Dr. Prince C P
 
Harmful and Useful Microorganisms Presentation
Harmful and Useful Microorganisms PresentationHarmful and Useful Microorganisms Presentation
Harmful and Useful Microorganisms Presentation
 
Call Us ≽ 9953322196 ≼ Call Girls In Lajpat Nagar (Delhi) |
Call Us ≽ 9953322196 ≼ Call Girls In Lajpat Nagar (Delhi) |Call Us ≽ 9953322196 ≼ Call Girls In Lajpat Nagar (Delhi) |
Call Us ≽ 9953322196 ≼ Call Girls In Lajpat Nagar (Delhi) |
 
BIOETHICS IN RECOMBINANT DNA TECHNOLOGY.
BIOETHICS IN RECOMBINANT DNA TECHNOLOGY.BIOETHICS IN RECOMBINANT DNA TECHNOLOGY.
BIOETHICS IN RECOMBINANT DNA TECHNOLOGY.
 
Call Girls in Aiims Metro Delhi 💯Call Us 🔝9953322196🔝 💯Escort.
Call Girls in Aiims Metro Delhi 💯Call Us 🔝9953322196🔝 💯Escort.Call Girls in Aiims Metro Delhi 💯Call Us 🔝9953322196🔝 💯Escort.
Call Girls in Aiims Metro Delhi 💯Call Us 🔝9953322196🔝 💯Escort.
 
Call Girls In Nihal Vihar Delhi ❤️8860477959 Looking Escorts In 24/7 Delhi NCR
Call Girls In Nihal Vihar Delhi ❤️8860477959 Looking Escorts In 24/7 Delhi NCRCall Girls In Nihal Vihar Delhi ❤️8860477959 Looking Escorts In 24/7 Delhi NCR
Call Girls In Nihal Vihar Delhi ❤️8860477959 Looking Escorts In 24/7 Delhi NCR
 
Hot Sexy call girls in Moti Nagar,🔝 9953056974 🔝 escort Service
Hot Sexy call girls in  Moti Nagar,🔝 9953056974 🔝 escort ServiceHot Sexy call girls in  Moti Nagar,🔝 9953056974 🔝 escort Service
Hot Sexy call girls in Moti Nagar,🔝 9953056974 🔝 escort Service
 
LIGHT-PHENOMENA-BY-CABUALDIONALDOPANOGANCADIENTE-CONDEZA (1).pptx
LIGHT-PHENOMENA-BY-CABUALDIONALDOPANOGANCADIENTE-CONDEZA (1).pptxLIGHT-PHENOMENA-BY-CABUALDIONALDOPANOGANCADIENTE-CONDEZA (1).pptx
LIGHT-PHENOMENA-BY-CABUALDIONALDOPANOGANCADIENTE-CONDEZA (1).pptx
 
Spermiogenesis or Spermateleosis or metamorphosis of spermatid
Spermiogenesis or Spermateleosis or metamorphosis of spermatidSpermiogenesis or Spermateleosis or metamorphosis of spermatid
Spermiogenesis or Spermateleosis or metamorphosis of spermatid
 
zoogeography of pakistan.pptx fauna of Pakistan
zoogeography of pakistan.pptx fauna of Pakistanzoogeography of pakistan.pptx fauna of Pakistan
zoogeography of pakistan.pptx fauna of Pakistan
 
insect anatomy and insect body wall and their physiology
insect anatomy and insect body wall and their  physiologyinsect anatomy and insect body wall and their  physiology
insect anatomy and insect body wall and their physiology
 
Engler and Prantl system of classification in plant taxonomy
Engler and Prantl system of classification in plant taxonomyEngler and Prantl system of classification in plant taxonomy
Engler and Prantl system of classification in plant taxonomy
 
Forest laws, Indian forest laws, why they are important
Forest laws, Indian forest laws, why they are importantForest laws, Indian forest laws, why they are important
Forest laws, Indian forest laws, why they are important
 
Best Call Girls In Sector 29 Gurgaon❤️8860477959 EscorTs Service In 24/7 Delh...
Best Call Girls In Sector 29 Gurgaon❤️8860477959 EscorTs Service In 24/7 Delh...Best Call Girls In Sector 29 Gurgaon❤️8860477959 EscorTs Service In 24/7 Delh...
Best Call Girls In Sector 29 Gurgaon❤️8860477959 EscorTs Service In 24/7 Delh...
 

FAST実験4:大気蛍光望遠鏡による極高エネルギー宇宙線観測報告

  • 1. T. Fujii (ICRR), M. Malacari, J. Albury, J.A. Bellido, J. Farmer, A. Galimova, P. Horvath, M. Hrabovsky, D. Mandat, A. Matalon, J.N. Matthews, M. Merolle, X. Ni, L. Nozka, M. Palatka, M. Pech, P. Privitera, P. Schovanek, S.B. Thomas, P. Travnicek 72 2017 3 17 http://www.fast-project.org FAST 4 FAST TA Credit: Max Malacari EUSO-TA
  • 2. Fine pixelated camera Low-cost and simplified/optimized FD Too expensive to cover a huge area 2 Single or few pixels and smaller optics Fluorescence detector Array of Single-pixel Telescopes Segmented mirror telescope Variable angles of elevation – steps. 15 deg 45 deg ✦ > 1019.5 eV ✦ (30,000 km2, 10×Auger or TA×4) ⇒
  • 3. FAST 3 ✦ EUSO-TA 1 ✦ ✦ ✦ Astroparticle Physics, 74 (2016) 64-72 ✦ ✦ FAST ( FAST ) (Xmax) EUSO-TA telescope + FAST camera Fig. 12. A 1018 eV shower simultaneously detected by the TA FD and the FAST protot superimposed (see Fig. 11). In (b), the corresponding FADC trace recorded by the FAS Fig. 6. FADC signal recorded for a YAP light pulse. It is used to monitor the relative gain of the PMT. Fig. 7. Variation of the YAP signal during a seven hour data taking run. 70 T. Fujii et al. / Astroparticle Physics 74 (2016) 64–72 Vertical Laser ~1019.3 eV Cosmic Ray ~1018.0 eV
  • 4. FAST - progress in design and construction UV Plexiglass Segmented primary mirror8 inch PMT camera (2 x 2) 1m2 aperture FOV = 25°x 25° variable tilt Joint Laboratory of Optics Olomouc – Malargue November 2015 Prototype - October 2015 15° 45° 4Joint Laboratory of Optics in Olomouc, Czech Republic FAST UV band-pass filter
  • 7. FAST 7 ✦ (TA) ✦ 10 MHz, 80 µs ✦ TA 21 km Time (100 ns) 0 100 200 300 400 500 600 700 800 -30 -20 Time (100 ns) 0 100 200 300 400 500 600 700 800 -30 -20 Time (100 ns) 0 100 200 300 400 500 600 700 800 /(100ns)p.e.N -20 -10 0 10 20 30 PMT 2 Time (100 ns) 0 100 200 300 400 500 600 700 800 /(100ns)p.e.N -20 -10 0 10 20 30 40 PMT 4 80 µs 100 ( ) () FAST
  • 8. 8 ✦ : 62194 events : PMT 1 PMT 3 PMT 2 PMT 4 : 2016 10 5 Time (100 ns) 0 100 200 300 400 500 600 700 800 /(100ns)p.e.N -30 -20 -10 0 10 20 30 40 PMT 1 Time (100 ns) 0 100 200 300 400 500 600 700 800 /(100ns)p.e.N -30 -20 -10 0 10 20 30 PMT 3 Time (100 ns) 0 100 200 300 400 500 600 700 800 /(100ns)p.e.N -20 -10 0 10 20 30 PMT 2 Time (100 ns) 0 100 200 300 400 500 600 700 800 /(100ns)p.e.N -20 -10 0 10 20 30 40 PMT 4 Time (100 ns) 0 100 200 300 400 500 600 700 800 /(100ns)p.e.N -20 0 20 40 60 80 100 PMT 1 Time (100 ns) 0 100 200 300 400 500 600 700 800 /(100ns)p.e.N -30 -20 -10 0 10 20 30 40 PMT 3 Time (100 ns) 0 100 200 300 400 500 600 700 800 /(100ns)p.e.N -20 0 20 40 60 80 100 120 140 PMT 2 Time (100 ns) 0 100 200 300 400 500 600 700 800 /(100ns)p.e.N -20 -10 0 10 20 30 40 PMT 4 [] Time (100 ns) 0 100 200 300 400 500 600 700 800 /(100ns)p.e.N 0 200 400 600 800 1000 1200 PMT 1 Time (100 ns) 0 100 200 300 400 500 600 700 800 /(100ns)p.e.N 0 200 400 600 800 1000 PMT 3 Time (100 ns) 0 100 200 300 400 500 600 700 800 /(100ns)p.e.N 0 200 400 600 800 1000 PMT 2 Time (100 ns) 0 100 200 300 400 500 600 700 800 /(100ns)p.e.N 0 200 400 600 800 1000 PMT 4
  • 9. : 2016 10 5 9 ✦ ->PMT -> (>35 µs)-> ->2 PMT ✦ 62194 -> 4290 -> 3950 -> 389 -> 90 events
  • 10. Event 387: log10(E(eV)): 18.68, Zen: 61.0◦ , Azi: 63.3◦ , Core(11.86, -11.50), Rp: 3.52, Psi: 42.8◦ , Xmax: 1113 g/cm2 FoV(1407 - 1769), Date: 20161005, Time: 06:07:38.800548560 Event 388: log10(E(eV)): 17.96, Zen: 38.8◦ , Azi: -19.6◦ , Core(8.90, -17.03), Rp: 9.44, Psi: 82.6◦ , Xmax: 768 g/cm2 FoV(498 - 1017), Date: 20161005, Time: 06:30:06.947113522 Event 389: log10(E(eV)): 17.83, Zen: 4.7◦ , Azi: 115.2◦ , Core(14.23, -5.41), Rp: 7.18, Psi: 86.7◦ , Xmax: 656 g/cm2 FoV(473 - 850), Date: 20161005, Time: 06:35:10.462924009 Event 393: log10(E(eV)): 18.14, Zen: 31.6◦ , Azi: 2.8◦ , Core(6.02, -6.69), Rp: 11.96, Psi: 102.1◦ , Xmax: 762 g/cm2 FoV(373 - 991), Date: 20161005, Time: 06:51:48.292842002 Event 394: log10(E(eV)): 18.69, Zen: 61.2◦ , Azi: -9.4◦ , Core(9.58, -20.15), Rp: 9.27, Psi: 57.3◦ , Xmax: 1021 g/cm2 FoV(829 - 1221), Date: 20161005, Time: 06:53:27.011365323 Event 395: log10(E(eV)): 18.26, Zen: 17.7◦ , Azi: -82.0◦ , Core(13.53, -2.14), Rp: 10.39, Psi: 98.2◦ , Xmax: 769 g/cm2 FoV(303 - 890), Date: 20161005, Time: 06:53:43.909532618 10 Time (100 ns) 0 100 200 300 400 500 600 700 800 /(100ns)p.e.N -40 -20 0 20 40 60 PMT 1 Time (100 ns) 0 100 200 300 400 500 600 700 800 /(100ns)p.e.N -20 -10 0 10 20 30 40 PMT 3 Time (100 ns) 0 100 200 300 400 500 600 700 800 /(100ns)p.e.N -40 -30 -20 -10 0 10 20 30 40 50 PMT 2 Time (100 ns) 0 100 200 300 400 500 600 700 800 /(100ns)p.e.N -30 -20 -10 0 10 20 30 40 PMT 4 2016/10/05 06:37:49.525424540 Time (100 ns) 0 100 200 300 400 500 600 700 800 /(100ns)p.e.N 0 500 1000 1500 2000 PMT 1 Time (100 ns) 0 100 200 300 400 500 600 700 800 /(100ns)p.e.N 0 50 100 150 200 250 300 350 PMT 3 Time (100 ns) 0 100 200 300 400 500 600 700 800 /(100ns)p.e.N 0 200 400 600 800 1000 PMT 2 Time (100 ns) 0 100 200 300 400 500 600 700 800 /(100ns)p.e.N 0 50 100 150 200 250 300 PMT 4 2016/10/05 10:25:50.781802380 TAFD logE = 18.08 Rp = 2.40 km Too close
  • 11. 11 Time (100 ns) 0 100 200 300 400 500 600 700 800 /(100ns)p.e.N -30 -20 -10 0 10 20 30 40 50 60 PMT 1 Time (100 ns) 0 100 200 300 400 500 600 700 800 /(100ns)p.e.N 0 50 100 150 200 PMT 3 Time (100 ns) 0 100 200 300 400 500 600 700 800 /(100ns)p.e.N -20 0 20 40 60 80 PMT 2 Time (100 ns) 0 100 200 300 400 500 600 700 800 /(100ns)p.e.N -20 0 20 40 60 80 100 120 PMT 4 Time (100 ns) 0 100 200 300 400 500 600 700 800 /(100ns)p.e.N -50 0 50 100 150 200 PMT 1 Time (100 ns) 0 100 200 300 400 500 600 700 800 /(100ns)p.e.N -30 -20 -10 0 10 20 30 40 PMT 3 Time (100 ns) 0 100 200 300 400 500 600 700 800 /(100ns)p.e.N -20 0 20 40 60 80 PMT 2 Time (100 ns) 0 100 200 300 400 500 600 700 800 /(100ns)p.e.N -20 -10 0 10 20 PMT 4 Time (100 ns) 0 100 200 300 400 500 600 700 800 /(100ns)p.e.N 0 50 100 150 200 250 300 350 PMT 1 Time (100 ns) 0 100 200 300 400 500 600 700 800 /(100ns)p.e.N -20 0 20 40 60 80 PMT 3 Time (100 ns) 0 100 200 300 400 500 600 700 800 /(100ns)p.e.N -20 -10 0 10 20 30 PMT 2 Time (100 ns) 0 100 200 300 400 500 600 700 800 /(100ns)p.e.N -20 -10 0 10 20 30 40 50 PMT 4 Time (100 ns) 0 100 200 300 400 500 600 700 800 /(100ns)p.e.N 0 50 100 150 200 PMT 1 Time (100 ns) 0 100 200 300 400 500 600 700 800 /(100ns)p.e.N -20 0 20 40 60 80 100 120 PMT 3 Time (100 ns) 0 100 200 300 400 500 600 700 800 /(100ns)p.e.N -20 0 20 40 60 80 100 PMT 2 Time (100 ns) 0 100 200 300 400 500 600 700 800 /(100ns)p.e.N -20 0 20 40 60 80 PMT 4 128 18
  • 12. Time (100 ns) 0 100 200 300 400 500 600 700 800 /(100ns)p.e.N 0 5 10 15 20 12 ✦ 21 km 284 ✦ ✦ ( ) ✦ ✦ PMT ✦ PMT ( ) ✦ ( ) Sum PMT 1 PMT 3 PMT 2 PMT 4 ( ) Simulation (Preliminary) Data 11 Optical simulation status FAST Simulation - example - PSF (7.5deg diagonal) aperture input 0.5W 0.43W/PMT1, <0.001W/PMT234 (eff: 86%) 10 Optical simulation status - axis): aperture input 0.5W 4x0.04W/PMT (eff: 32%) FAST Simulation - example
  • 13. 13 ✦ Fluorescence detector Array of Single-pixel Telescopes (FAST) ✦ ✦ FAST ✦ 2016 10 2017 1 ✦ 128 18 ✦ 21 km ✦ ✦ 2017 1 25 GPS ✦ ✦ 2017 6 FAST GPS DAQ ✦ http://www.fast-project.org