(Cherenkov Telescope Array : CTA) (Large-Sized Telescope : LST) 2f CTA CTA CTA CTA-Japan LST CTA CTA 3 20 GeV 100 TeV 20 GeV 1000 GeV LST 23 m 23 m 1.
|
|
- えいじろう みやまる
- 7 years ago
- Views:
Transcription
1 CTA - 2f ( 27 ) 14NM160L
2 (Cherenkov Telescope Array : CTA) (Large-Sized Telescope : LST) 2f CTA CTA CTA CTA-Japan LST CTA CTA 3 20 GeV 100 TeV 20 GeV 1000 GeV LST 23 m 23 m 1.51 m m 58.4 m 28 m LST CTA LST f (28 m 29.2 m) 80 % (D80) Pixel 50 mm 1/ mm ( 0.03 ) 2f 2f 2 (2f) 2f LED ON OFF 2f 5 6
3 1 mm 2f 1 mm 1f 0.5 mm 2f 2f 300 nm 550 nm 85 % 470 nm LED 2f 90 % 89.4 % 93.3 % 5 % 2f 2
4 1 Introduction Cherenkov Telescope Array, CTA CTA CTA CTA-Japan Large-Sized Telescope (LST) LST LST LST LST f f f f f f
5 : Cd f Phase Measuring Deflectometry (PMD) LED A High Dynamic Range (HDR) 112 B 2f 117 C 134 2
6 1.1 [1] [2] [2] [2] π 0 [2] [2] [3] [3] [4] [5] CORSIKA [9] [5] ( ) ( ) [10] CTA [11] CTA ( ) MAGIC ( ) H.E.S.S. ( ) [12] "Kifune plot" X VHE [12] CTA 3 [13] [12] Large-Sized Telescope (LST) ( / CTA ) Large-Sized Telescope (LST) [14] MAGIC AMC [15] CTA [16] CMOS [17] [12] CTA PMT (R ) PMT [18] [19] cold slump [12] [10]
7 2.20 [20] [14] [21] [21] [10] f pixel [10] [10] D80 [10] D LED [10] No.70 (1/5 ) No.70 (1 ) No.70 (3.2 ) No.70 (1 ) USB PC LED f No.75 D No No No.76 D No No ON OFF LED SUPERSTAR PAR LED f
8 3.39 2f ( No.70) D Cd D80 Cd D80 ( : )[10] D80 ( : ) Cd33 ( : ) No No No No No LED : OSB5XNE3C1S LED LED : CC1000EH LED LED LED r No.70 D PC NewLens (S55-250mm F4-5.6 IS STM) OldLens (EF-S55-250mm F4-5.6 IS II) D80 ( : ) Cd33 ( : ) D80 ( : ) Cd33 ( : ) f PMD (No.70) f PMD (No.75) f PMD (No.77) f PMD (No.81) f
9 LED LED LED 60 m LED 60 m m m LED (ON BG) LED (1) (2) LED ( ) LED (2f ) f (1) (2) A.1 1/ A A.3 HDR A.4 HDR A.5 (1/5 3.2 ) HDR A.6 ( ) Y = 1480 ( ) A.7 ( ) Y = 1480 ( ) A B.1 R B.2 D B.3 R vs D B.4 No B.5 No B.6 No B.7 No B.8 No
10 B.9 No B.10 No B.11 No B.12 No B.13 No C.1 EF-S55-250mm F4-5.6 IS C.2 EF-S55-250mm F4-5.6 IS C.3 EF-S55-250mm F4-5.6 IS STM C.4 EF-S55-250mm F4-5.6 IS STM C.5 EF-S55-250mm F4-5.6 IS STM
11 Large-Sized Telescope (LST) LST f [10] D D No.70 No.75 (No.73 ) R D f D80 ( No.75) D80 ( No.75) OFF D80 ( No.70) D D D D No f PMD (LED) No LED LED (12 3 ) LED (12 4 ) LED (12 3 ) LED (12 4 (1)) LED (12 4 (2)) LED (12 4 (3)) LED ( ) Fitting
12 B.1 2f LST
13 1 Introduction Victor Franz Hess 90 % 9 % 1 % ev 1.2 kev X TeV (= ev) 1.1: [1] 10
14 1.2.1 E /E 1.2: [2] 1.3: [2] 10 GeV MeV γ 1.4: [2] 11
15 π 0 π 0 p + p p + p + π 0 + π + + π π 0 γ + γ (1.1) π s 2 π MeV(π 0 ) 1.5: π 0 [2] ( ) 2 1.6: - [2] 12
16 GeV ( ) ( 83 MeV) 1.7: [3] 13
17 2 1.8: [3] 14
18 1.3.2 (c/n) ( 1.9) c n βc θ cos θ = 1/(βn) n 300 nm β 1/n E E m e c 2 / 1 1/n 2 = 21 MeV (m e : ) λ2 ( ) 1 dλ N = 2πα 1 λ 1 (βn(λ)) 2 λ 2 α 1/137 λ 1 λ 2 1 TeV ( 1.10) 1 m : [4] 1.10: [5] 15
19 TeV : MAGIC [6] VERITAS [7] H.E.S.S. [8] 16
20 1.4.1 (Imaging Air Cherenkov Technique : IACT) : CORSIKA [9] : : ( ) 17
21 : [5] : ( ) ( ) [10] 18
22 2 Cherenkov Telescope Array, CTA 2.1 CTA TeV Cherenkov Telescope Array (CTA) ( 2.1) 3 H.E.S.S, MAGIC, VERITAS (1 m Crab erg s 1 cm 2 ) 20 GeV 100 TeV ( 2.2) : CTA [11] 2.2: CTA ( ) MAGIC ( ) H.E.S.S. ( ) [12] CTA GeV Active Galactic Nuclei (AGN) (GRB : Gamma-Ray Burst) Extragalactic Background Light (EBL) 100 GeV 10 TeV 19
23 10 TeV 100 CTA 1000 ( 2.3) 2.3: "Kifune plot" X VHE [12] CTA CTA 23 m Large-Sized Telescope (LST) 12 m Midium-Sized Telescope (MST) 4 m Small-Sized Telescope (SST) 3 ( 2.4) ( 2.5) CTA 20 GeV 100 TeV CTA-Japan 100 CTA-Japan PHYS ( ) MC ( ) FPI (Focal Plane Instrument/ ) ELEC ( ) MIR ( ) CAL ( ) Large-Sized Telescope (LST) CTA CTA-Japan 15 % 20
24 2.4: CTA 3 [13] :LST :MST :SST 2.1: LST MST SST 23 m m 4.3 m 20 GeV - 1 TeV 100 GeV - 10 TeV 5 TeV TeV Parabolic Davies-Cotton Davies-Cotton or or Schwarzschild-Couder Schwarzschild-Couder 368 m m 2 37 m 2 28 m 15 m 7 m : [12] 21
25 2.2 Large-Sized Telescope (LST) CTA-Japan Large-Sized Telescope (LST) ( 2.6) LST LST LST 1600 Active Mirror Control (AMC) 2.6: Large-Sized Telescope (LST) ( / CTA ) LST LST ( 2.7) 23 m 368 m m 2 MAGIC 240 m p.e. 100 p.e. MAGIC 50 p.e. 50 GeV LST GeV 30 GeV LST 20 GeV 1 TeV follow up follow up 22
26 CTA CTA LST LST 2.7: Large-Sized Telescope (LST) 2.2: Large-Sized Telescope (LST) (D) 23 m 368 m 2 (f) 28 m (f/d = 1.2) Parabolic m Pixel 50 mm < 100 t 180 /20 s Active Mirror Control System (AMC) 23
27 2.2.2 LST LST 198 ( 2.8) 1.51 m AMC : [14] :Active Mirror Control (AMC) LST (Active Mirror Control : AMC) MAGIC ( 2.9) ( 2.10) MAGIC AMC CTA CMOS ( 2.11) 2.8 CMOS LST 24
28 2.9: MAGIC AMC [15] 2.10: CTA [16] 2.11: CMOS [17] 25
29 2.2.3 LST LST ( 2.12) (PMT) ( 2.13) PMT CCD PMT ( 2.14) 1 1 Pixel ( 50 mm 0.1 ) PMT 7 1 PMT ( 2.15) LST 2000 PMT : [12] 2500 kg 2.13: CTA PMT (R ) CTA-Japan 26
30 2.14: PMT PMT 2.15: PMT [18] 27
31 2.3 LST LST 1.51 m ( 2.16) AMC CMOS 10 cm AMC mm LST 198 CTA 8 LST CTA-Japan : 2.17: [19] 28
32 LST mm AMC CMOS 10 cm LST 50 kgf 50 kgf 80 mm LST 2.7 mm 60 mm 2.7 mm LST 1 Pixel 50 mm 1/ mm 80 % 80 % D80 28 m 29.2 m LST LST 28 m 29.2 m 300 nm 550 nm 85 % CTA 1 % ( ) LST 10 29
33 2.3: LST 1510 mm (flat-flat) Hex < 50 kgf < 80 mm D80 < 16.6 mm at 1f > 85% at nm (> 90% at 400 nm) < 1 %/yr IP66 > cold slump ( 2.18) cold slump 1 INAF (Istituto Nazionale di AstroFisica) MAGIC 100 LST 60 mm ( 2.19) 2.7 mm 65.4 mm 47 kgf 2.18: cold slump [12] 30
34 2.19: [10] 5 (Cr+Al+SiO 2 +HfO 2 +SiO 2 ) ( 2.20) LST 2.8 m 9 m ( 2.21) LST 2.20: [20] 2.21: [14] 31
35 2.3.3 ( 2.22) 5 AMC 2 cm ( 2.23) 2.22: [21] 2.23: [21] 3 32
36 f f f 2f 2f f(focal length) h = R sin θ = (R f) sin 2θ (3.1) θ sin θ θ sin 2θ 2θ (3.1) h Rθ = (R f)2θ R 2f (3.2) R 2f 3.1: [10] 33
37 2f (2f) ( ) 2f 2f f 2f 1/2 2f (D80) 1 f 16.6 mm mm 2f D80 < 16.6 mm at 1f D80 < 33.2 mm at 2f 2f 3.2 LED LED ON OFF LST 56 m 58.4 m : 2f 34
38 LED (ON) (OFF) LED ON LED 2f LED OFF ON OFF D80 1) RAW 2) 3) D80 3 1) RAW RAW (Canon.CR2 ) JPEG RAW RAW dcraw[22] ImageMagick[23] 2 dcraw RAW FITS FITS 2:1:1 CMOS 1 Canon EOS Kiss X5 FITS 5202 pixel 3465 pixel pixel 1732 pixel 4 1 pixel 0.1 mm DS9[24] FITS 3.3: pixel [10] 1500 pixel 1500 pixel 15 cm 15 cm 35
39 2) ON OFF 1:1 OFF ON OFF OFF 200 pixel ON ( 3.4) ON OFF A M m ON OFF I ON,m I OF F,m A A = 1 M M m=1 I ON,m ION,m = I OF F,m I OF F,m (3.3) A OFF n I A,n I A,n = I ON,n A I OF F,n (3.4) 3.4 ON OFF 3.4: [10] 36
40 3) D80 I A,n (x G, y G ) 600 pixel 600 pixel N x G = N I A,n x n n=1 y G = N x n n=1 N I A,n y n n=1 (3.5) N y n n=1 (x G, y G ) r r 100 r 100 I A,100 I A, % I A,80 r 80 D80 4πr 2 dr dr = 1 pixel 80 % I A,80 r 80 r 80 2 D80 ( 3.5) r pixel 750pixel 750 pixel I A,100 ( 3.6) 3.5: D80 [10] 3.6: D80 37
41 3.2 2f 2f ( R) 0.5 m (R±0.5 m) 3 3 ON OFF f LST 28 m 29.2 m 2f 60 m LED 2f 2f 3.1: 2f [10] ( or ) LED(OSRAM : LED SUPERSTAR PAR ) ( ) (Canon : EOS 60D) 1/5, 1, 3.2 s (F ) 6.3 ISO(CMOS ) ( ) 1 (Canon : EF-S55-250mm f/4-5.6 IS II) mm 3.7: LED : (OFF) : (ON) 3.8: [10] 1 FITS 38
42 LED OSRAM LED SUPERSTAR PAR ( 3.7) 5 W 50 W 60 m ( 3.8) pixel Canon EOS 60D EF-S55-250mm f/4-5.6 IS II (F ) 6.3 1/ ISO 100 ISO CMOS ( ) cm LED ( R ) 3 m ON ( 3.9) 3 ON LED OFF ON OFF 0.5 m 3 3.9: 3.9 2f ( 3.10) 39
43 3.10: 2f No.70 No.75 (No.73 ) No.70 3 ( 3.11, 3.12, ) 3.11: No.70 (1/5 ) 40
44 3.12: No.70 (1 ) 3.13: No.70 (3.2 ) 41
45 3.2: D80 [ ] D80 [pixel] 1/ , 3.12, ( ) z ( ) x ( ) y ( ) 3.2 D ( ) D80 1/5 1 1 s D80 (S/N ) D80 3 y No pixel 1500 pixel 1050 pixel 1500 pixel 200 pixel 3.3: D pixel 276 pixel 42
46 3.14: No.70 (1 ) D80 No.70 No : No.70 No.75 (No.73 ) [m] [ ] A D80 [pixel] D80 [mm] 2 No / / / No / / /
47 [m] [ ] A D80 [pixel] D80 [mm] 2 No / / / No / / / No / / / ( R) ( ) D D mm 3.5: R D80 No.70 No.71 No.72 No.74 No.75 R [m] D80 [mm] pixel = 0.1 mm 44
48 D D80 D80 56 m 58.4 m D80 3 ( 3.15) 3.15: 45
49 s A = 1.01 A = % 2 % ON OFF 1 s 0.1 % 0.1 % pixel 2 count 1500 pixel 1500 pixel count A (= 0.1 % ) 60 m 2f 3.3 PC HDR (High Dynamic Range) f PC PC 2f 3 HDR (High Dynamic Range) 2f 46
50 3.3 2f 2f 2f 2f 2f PC PC PC USB PC ( 3.16) PC gphoto2[25] gphoto2 3.16: USB PC 47
51 : : 48
52 f 2f 3.6 2f (LED) LED Lightning EVER MR16 GU10 LED Bulbs (Warm White) LED GU10 E26 ( 3.19) 3.19: LED LED : 30 cm 30 cm 1 cm L Pixel 49
53 Canon EOS Kiss X5 Canon EF-S55-250mm f/4-5.6 IS II Canon ET-60 Canon EOS Kiss X5 Canon EOS 60D ( 3.21) 6 cm 3.21: 3.6: 2f or LED Lightning EVER : MR16 GU10 LED Bulbs (Warm White) : Canon : EOS Kiss X5 Canon : EF-S55-250mm f/4-5.6 IS II Canon : ET-60 BOSCH : GLM 80 (F ISO ) ( 3.1) 50
54 f : 3.23: 1 2f 2f 2 ( 3.24) 5 mm No.75 ( R) 0.5 m (R±0.5 m) 0.1 m 11 51
55 3.24: 2f 3.25: No.75 D : No : No
56 3.25 X Y pixel 80% 2 D80 0 R pixel D80 2 2f : D80 ( No.75) < > R = m < > R = m [ pixel] ON OFF OFF 2 OFF 53
57 20 pixel 2 mm D80 3 D80 LED 2f 5 mm 10 mm D : D80 ( No.75) 5 mm 10 mm [ pixel] 10 mm 14 pixel 20 pixel D : 10 mm 54
58 No No.76 R±0.5 m 0.25 m 5 ( 3.31) 3.29: No.76 D : No : No D m m 0.20 m 0.10 m 2 R±0.45 m 0.15 m 7 55
59 5 ON OFF ON OFF LED ON OFF BG LED : 3.33: ON OFF 56
60 LED ON/OFF LED ON/OFF + LED ON + OFF LED ON + OFF + LED ON + OFF + 3.9: OFF D80 ( No.70) D80 [pixel] A A ON OFF D80 LED ON/OFF 2f LED 10 mm ( R) 0.45 m (R±0.5 m) 0.15 m m ( 0.10 m) ON OFF LED ON/OFF 57
61 3.3.4 (LED) OSRAM LED SUPERSTAR PAR LED LED 5 W 50 W LED 4 mm LED LED : LED SUPERSTAR PAR : : : 3.35: LED cm 3.36: 58
62 3 m 3.37 PC 5 m USB 3.37: f 3.38: 2f 59
63 3.3.5 : No : 2f ( No.70) D80 8 pixel pixel : D80 D mm 3 0.1mm 60
64 f OFF OFF ( 1 ) 2015/5/13 16: /6/17 15: /6/17 20: /8/27 15: /8/27 21: /6/17 22:26 ( ) 3.41: 61
65 3.42: 3.10: Mean RMS count RMS 6.82 count CMOS count 50 count count 1/4 62
66 3.3.7 Cd33 Constant diameter (Cd) Phase Measuring Deflectometry (PMD) 2f PMD PMD PMD PMD 2013 [10] Cd33 Constant diameter D80 33 mm Cd33 Cd33 2f 33 mm 3.43: Cd r 100 ( 750 pixel) D80 Cd33 Cd33 D80 ( 3.44) 63
67 3.44: D80 Cd33 D80 [mm] Cd33 [%] 2f D80 (r 100 ) 80 % Cd33 64
68 D80 Cd33 D80 Cd 33 A D80 Cd33 [10] 3.45 A 0.1 % D80 23 pixel = 2.3 mm 3.45: D80 ( : )[10] : D80 ( : ) 65
69 3.47: Cd33 ( : ) 3.46 D % 10 pixel 1 mm 1 mm 3.46 D80 D80 2 Cd33 D LST 2f 2f 6 No.70 No.85 (No.73 ) No.70 No : No.70 No.71 No.72 No.74 No.75 R ( ) [m] D80 ( ) [mm] R (Fit) [m] D80 (Fit) [mm]
70 No : No.70 67
71 No : No.71 68
72 No : No.72 69
73 No : No.74 70
74 No : No.75 71
75 3.4 2f 2f 4 2f PMD (LED) LED LED SUPERSTAR PAR LED LED LED 2700 K 300 nm 550 nm LED LED 4 LED OptoSupply OSB5XNE3C1S ( 3.53) LED 470 nm 3 W LED 60 m 3.54 LED LED LED : LED : OSB5XNE3C1S 3.54: LED 72
76 LED 3.54 LED LED 3.54 LED LED CC1000EH ( 3.55) 3.55: LED : CC1000EH LED LED DC LED DC ( 3.57) LED 4 mm ( 3.56) 3.56: LED LED LED ON/OFF DC ON/OFF mm 73
77 3.57: LED 3.58: 3.59: 3.60: LED 74
78 Canon EOS Kiss X5 Canon EOS 8000D CMOS Canon EOS 8000D CMOS Canon EOS Kiss X mm(aps-c ) D80 Canon EF-S55-250mm F4-5.6 IS II Canon EF-S55-250mm F4-5.6 IS STM Canon EF-S55-250mm F4-5.6 IS II 250 mm 0.31 Canon EF-S55-250mm F4-5.6 IS STM 250 mm mm 14 % 17 % ( 3.61) f : :Canon EF-S55-250mm F4-5.6 IS II :Canon EF-S55-250mm F4-5.6 IS STM 75
79 nm LED LED CMOS r pixel 2000 pixel 700 pixel 700 pixel r pixel 3.62: r 100 : r 100 : r r 100 r
80 pixel : f No D No.70 7 (EOS 8000D + EF-S55-250mm F4-5.6 IS STM) (EOS Kiss X5 + EF-S55-250mm F4-5.6 IS II) No LED D mm 0.94 mm 7 No
81 3.12: D80 D80 [mm] D80 [mm] [mm] No No No No : No.70 D80 D80 1mm r D80 ( 3.65) r
82 3.65: 3.13: D80 D80 [mm] D80 [mm] [mm] ( [mm]) No (-0.37) No (-0.19) No (-0.19) No (-0.37) r mm r 100 r 100 D mm D80 No.70 No EOS 8000D EOS Kiss X NewCamera EOS 8000D OldCamera EOS Kiss X5 NewLens EF-S55-250mm F4-5.6 IS STM OldLens EF- S55-250mm F4-5.6 IS II NewCamera OldCamera NewLens OldLens 79
83 3.14: D80 Camera NewCamera OldCamera Lens NewLens OldLens NewLens OldLens No.70 D80 [mm] Scale(1 mm =) [pixel] No.77 D80 [mm] Scale(1 mm =) [pixel] f 1 mm No.70 No.77 No.77 NewCamera NewLens 0.4 mm D80 D80 NewLens OldLens D80 4 mm CMOS 1 pixel 4 mm 3.66 PC PC : PC 80
84 3.67: NewLens (S55-250mm F4-5.6 IS STM) 3.68: OldLens (EF-S55-250mm F4-5.6 IS II) 81
85 RAW dcraw ImageMagick FITS FITS ds : 1 NewLens 0.7 % OldLens 2.2 % D : D80 Camera NewCamera OldCamera Lens NewLens OldLens NewLens OldLens No.70 D80 [mm] Scale(1 mm =) [pixel] No.77 D80 [mm] Scale(1 mm =) [pixel] No.77 NewCamera 0.1 mm NewCamera OldCamera 0.5 mm r
86 : D80 ( : ) 3.71: Cd33 ( : ) A 0.1 % +0.1 % D80 8 pixel 10 pixel A 2047 D80 A A
87 M A m=1 = (I ON,m ) M m=1 (I OF F,m ) (3.6) A 3.4 I A,n = (I ON,n ) A (I OF F,n ) (3.7) 3.7 D : D80 ( : ) 3.73: Cd33 ( : ) D80 50 % D80 6 pixel 1 mm 84
88 f 1 5 2f 2f No : 3.16: No.70, /06/18 23:45 : LED Old,Old /06/ Old,Old /10/15 17:00 Old,Old /12/03 18:35 2f Old,Old /12/09 22:17 New,New 85
89 3.4.5 Phase Measuring Deflectometry (PMD) PMD 2f R PMD 0.07 m 0.28 m PMD 2f 2f D80 1 mm 1 mm PMD 2f 3.17: 2f PMD 2f PMD D80 [mm] R [m] D80 [mm] R [m] D80 [mm] R [m] ( ) ( ) (Fit) (Fit) No No No No : 2f PMD (No.70) 86
90 3.76: 2f PMD (No.75) 3.77: 2f PMD (No.77) 3.78: 2f PMD (No.81) 87
91 4 4.1 CTA LST 300 nm 550 nm 85 % LST 90 % 1.51 m 2f 2f 4.1 2f LED 2f 2f 2f 4.1: 2f 88
92 f LED Canon EOS Kiss X5 + Canon EF-S55-250mm F4-5.6 IS II (LED) (LED) ON OFF pixel 1 pixel : 4.1: (LED) ON OFF ON OFF Ave σ Ave σ Ave ± σ ± ± ± ± ± [ count/pixel] 89
93 2f No.70 2f r 100 ( 750 pixel) 2f count = 2f r 100 1pixel (4.1) mm mm 2 ( 4.3) 4.3: 1 mm = pixel pixel pixel : No.70 [count/pixel] [%] ± ± ± ± ± ±
94 4.2 LED 10 % LED 30 1/ LED LED LED LED 470 nm 470 nm LED S/N LED cm LED 55 cm 2f LED LED : LED 91
95 4.5: LED 4.6: LED LED % LED % LED LED 92
96 60 m LED 60 m S 6 60 m LED m LED LED : LED 60 m 4.8: LED 60 m LED LED 1 pixel
97 ( ) LED count/pixel count/pixel count/pixel 2 count LED LED 10 count S/N LED S/N 60 m LED 60 m LED ( EOS Kiss X5) 56 m LED LED 10 OFF : 60 m 60 m 7 LED LED
98 4.10: 60 m LED (ON BG) 4.3: LED [min] LED (ON-BG) [count/pixel] ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± count/pixel 60 m 60 2 count 10 count % 95
99 4.3.2 LED LED LED 2 LED LED : LED (12 3 ) ON OFF ON OFF Ave σ Ave σ Ave ± σ ± ± ± ± [ count/pixel] 4.5: LED (12 4 ) ON OFF ON OFF Ave σ Ave σ Ave ± σ ± ± ± ± ± [ count/pixel] 96
100 2 LED LED 4.11 LED A 1 cm ( ) ( ) 2 C A 1cm LED 1 ( 4.17) 4.11: LED f LED ( 4.15) ON 4 OFF(BG) 2 (4 ) Ave σ BG(1) BG(2) [ count/pixel] 4.6: LED (12 3 ) 4.12: (1) 97
101 (1) 2 2 ON OFF(BG) 4 ON OFF ON OFF Ave σ Ave σ Ave ± σ ± ± ± ± ± [ count/pixel] 4.7: LED (12 4 (1)) 4.13: (2) (2) 2 2 ON OFF(BG) 4 ON OFF ON OFF Ave σ Ave σ Ave ± σ ± ± ± ± ± [ count/pixel] 4.8: LED (12 4 (2)) 98
102 (3) 2f ( m) No ON OFF(BG) 1 ON OFF 5 Sum [ count] 4.9: LED (12 4 (3)) 4.14: 4.15: 5 ON OFF 1:1 99
103 2 LED % % 3 LED count LED LED 3 4 (1) 4 (3) (3) 2f 4.18 LED 1 cm (0.85 ) 1.5 % 2 cm (1.7 ) 7 % LED LED LED LED LED 60 m LED 1 pixel 2 3 count ( ) 1pixel 0.5 count (15 %) LED 2f LED 1 cm (0.85 ) 1.5 % 2 cm (1.7 ) 7 % LED 100
104 4.16: 4.17: LED ( ) 4.18: LED (2f ) 101
105 LED LED LED 60 m 60 m m LED LED 1 pixel 2 3 count : 102
106 LED LED 10 % f LED LED : m f ( 4.21) No D
107 pixel LED : 2f 4.22: 4.23: 104
108 4.10: LED ( ) [min] LED (ON-BG) 10 6 [count] ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± ± 0.50 (2.74 ± 0.04) 10 6 count 1 % 15?? LED 60 m LED LED m 5 ON OFF
109 図 4.24: 光量推測試験 図中の赤円で囲った部分にみられる光が床や壁の反射成分が鏡に反射された光であり 光量 安定性再試験のようにスクリーンを 2f 側に置いた場合には反射光が写らないことがわかる 図 4.25: スクリーンから見た床と壁の反射光 図 4.26: 暗幕とダンボール壁による遮光 表 4.11: 光量推測試験の測定位置と光量 測定位置 [m] 光量 [count/pixel] ± ± ± ± ±
110 4.27: (1) 5 Fitting m count/pixel 25 m χ 2 /ndf 25 m Fitting : (2) Fitting χ 2 /ndf m count/pixel Fitting 4.12: Fitting 25 m 25 m m [count/pixel]
111 pixel LED 4.2 r pixel 900 pixel ( 3.4 ) No ON OFF : 10 6 [count] No ± No ± No ± No ± No ± mm = 10.7 pixel : 2f [%] [%] [%] No ± No ± No ± No ± No ± % 5 % 5 % 2f 2f 108
112 93 % 90 % 2f LED LED 5 % 5 % 2f 109
113 5 (Chrenkov Telescope Array : CTA) (Large-Sized Telescope : LST) 2f 2f 2f 2f 5 6 2f 1 mm 2f 1 mm 1f 0.5 mm (D80) 16.6 mm 2f 2f PMD PMD f 2f LST 300 nm 550 nm 85 % 1.51 m 470 nm LED 2f 60 m LED 60 m 110
114 60 m 5 90 % 89.4 % 93.3 % 5 % LED 2f 111
115 A High Dynamic Range (HDR) HDR High Dynamic Range (HDR) Canon CMOS ( ) RAW 2 11 = 11bit = 13.7 bit 3 bit 3 bit HDR CMOS 2f HDR 2f 2f (56 m 58.4 m) D80 S/N 2f S/N 1/ HDR S/N 112
116 HDR LED HDR 1/5 3.2 A.1 A.2 A.1: 1/5 A.2: 3.2 1/5 A A.2 2 HDR HDR 3.2 ( ) ( ) ( A.3) 16 (4 bit) HDR A.4 A.3: HDR 113
117 A.4: HDR D80 16 pixel HDR HDR 1/5 3.2 HDR A.5 A.5: (1/5 3.2 ) HDR 114
118 HDR A.5 A.6: ( ) Y = 1480 ( ) A.6 Y = 1480 dx = +4 pixel dy = 32 pixel HDR A.7 A.7: ( ) Y = 1480 ( ) Y = 1480 A.8 115
119 A.8: A.8 1/ /5 3.2 Y = 1/16X Y = X Fittting Fitting Fitting Y = X HDR HDR LED S/N PC HDR 116
120 B 2f f B.1 B.1 B.13 2f LED 15 D80 R Fit B.1: 2f LST D80 [mm] R [m] D80 [mm] R [m] Cd33 [%] Scale(Ave.) [pixel] ( ) ( ) (Fit) (Fit) (1 mm = ) No /06/18 No /06/16 No /07/15 No /07/15 No /05/26 No /07/15 No /06/26 No /07/16 No /06/25 No /06/25 No /06/26 No /07/16 No /07/16 No /06/25 No /06/26 117
121 B.1: R B.2: D80 B.3: R vs D80 118
122 ( ) No
123 No
124 No
125 No
126 No
127 No.76 B.4: No
128 No.77 B.5: No
129 No.78 B.6: No
130 No.79 B.7: No
131 No.80 B.8: No
132 No.81 B.9: No
133 No.82 B.10: No
134 No.83 B.11: No
135 No.84 B.12: No
136 No.85 B.13: No
137 C f D EF-S55-250mm F4-5.6 IS C.1: EF-S55-250mm F4-5.6 IS C.2 DS9 1 (EF-S55-250mm F4-5.6 IS STM C.4 C.5 ) 134
138 C.2: EF-S55-250mm F4-5.6 IS 1 135
139 EF-S55-250mm F4-5.6 IS STM C.3: EF-S55-250mm F4-5.6 IS STM C.4: EF-S55-250mm F4-5.6 IS STM 1 136
140 C.5: EF-S55-250mm F4-5.6 IS STM 1 137
141 CTA-Japan 1 Fermi 2 2f 2f PMD 2f 2 138
142 CTA-Japan CTA-Japan MIR CTA-Japan CTA-Japan MIR 6 3 µ s 6 No.70 No.75 the 70s 139
143 [1] X [2] Tonello, N., 2006, Study of the VHE -ray emission from the Active Galactic Nucleus 1ES [3] Marcus Wagner, R., 2006, Measurement of Very High Energy Gamma-Ray Emission from Four Blazers Using the MAGIC Telescope and a Comparative Blazar Study [4], 2013, CTA, [5] Völk, H. J., & Bernlöhr, K. 2009, Imaging very high energy gamma-ray telescopes [6] MAGIC [7] VERITAS [8] H.E.S.S. [9] Fruck, C., 2011, A new LIDOR system for the MAGIC telescops and site search instrumentation for CTA [10], 2013, CTA, [11] CTA-Japan [12] CTA-Japan consortium, 2014, Cherenkov Telescope Array [13], 2015, Cherenkov Telescope Array (CTA) (9), 2015 [14] CTA Construction Project, 2015, Large Size Telescope Technical Design Report [15] 140
144 [16], 2015, CTA 101: CTA Active Mirror Control, 2015 [17], 2015, CTA, 2015 [18], 2015, CTA, [19], 2014, CTA, [20], 2012, CTA γi, [21], 2015, CTA 96, 2015 [22] dcraw dcoffin/dcraw/ [23] Image Magick [24] SAO Image DS9 [25] gphoto - gphoto Home [26], 2012, RAW [27] DCRAW
Fermi ( )
Fermi ( ) Outline Introduction Blazar Spectral Energy Distribution (SED) Predictions for the Fermi mission (Prospects for CTA) Summary The Blazar Sequence and the Cosmic Gamma-ray Background Radiation
More informationスライド 1
CTA 報告 18: 全体報告 Masahiro Teshima for CTA-Japan Consortium 観測天体 超新星残骸 連星系 銀河団 Cherenkov Telescope Array 超高エネルギー宇宙ガンマ線の研究 活動銀河核 狙う物理 ガンマ線バースト 宇宙線の起源 銀河系内 系外の高エネルギー天体の研究 赤外 可視背景放射 ( 宇宙の星形成史 ) の研究 暗黒物質対消滅からのガンマ線の探索
More informationE 1 GeV E 10 GeV 1 2, X X , GeV 10 GeV 1 GeV GeV π
169 8555 3 4 1 e-mail: kataoka.jun@waseda.jp 606 8502 e-mail: totani@kuastro.kyoto-u.ac.jp 305 0801 1 1 e-mail: kunihito.ioka@kek.jp 50 5 X 1 10 10 2008 3 2,000 542 2012 9 5 2. 1 3 E 1 GeV E 10 GeV 1 2,
More information( :YITP- W- ) ( ) 1 M1 1 2 3 3 D1 ALMA NGC3256 D1 M1 X M1-2 a1 M2 a2 M1 a3 M1 CTA a4 M1 c1 M2 c2 D2 c3 M2 c4 M2 c5 M1 Gravitational Leptogenesis a2 M1 ( ) Abstract 10 15.5 ev(knee energy) 12 TopB ( )
More information3 3.3. I 3.3.2. [ ] N(µ, σ 2 ) σ 2 (X 1,..., X n ) X := 1 n (X 1 + + X n ): µ X N(µ, σ 2 /n) 1.8.4 Z = X µ σ/ n N(, 1) 1.8.2 < α < 1/2 Φ(z) =.5 α z α
2 2.1. : : 2 : ( ): : ( ): : : : ( ) ( ) ( ) : ( pp.53 6 2.3 2.4 ) : 2.2. ( ). i X i (i = 1, 2,..., n) X 1, X 2,..., X n X i (X 1, X 2,..., X n ) ( ) n (x 1, x 2,..., x n ) (X 1, X 2,..., X n ) : X 1,
More information( ) 09:00 17:40 08: :00 09: :05 10:15 1 ( ) -01 ( 5 ) (10:15 10:25 ) 10:25 11:50 2 ( ) -02 ( 6 ) (11:50 13:00 ) 13:00 1
29 30 2 7 ( ) 09:00 17:40 08:55 31 501 09:00 09:05 31 501 9:05 10:15 1 ( ) -01 ( 5 ) (10:15 10:25 ) 10:25 11:50 2 ( ) -02 ( 6 ) (11:50 13:00 ) 13:00 14:10 1 ( ) -03 ( 5 ) (14:10 14:20 ) 14:20 16:10 2 (
More information5 36 5................................................... 36 5................................................... 36 5.3..............................
9 8 3............................................. 3.......................................... 4.3............................................ 4 5 3 6 3..................................................
More informationチュートリアル:ノンパラメトリックベイズ
{ x,x, L, xn} 2 p( θ, θ, θ, θ, θ, } { 2 3 4 5 θ6 p( p( { x,x, L, N} 2 x { θ, θ2, θ3, θ4, θ5, θ6} K n p( θ θ n N n θ x N + { x,x, L, N} 2 x { θ, θ2, θ3, θ4, θ5, θ6} log p( 6 n logθ F 6 log p( + λ θ F θ
More informationTelescope Array FD SD SD
2009 2010 3 T06MI051 2 4 1-1 4 1-2 5 1-3 Telescope Array 6 1-4 FD 9 1-5 SD 11 1-6 SD 15 1-7 16 17 2-1 17 2-1-1 17 2-1-2 18 2-2 20 2-3 21 2-4 23 2-4-1 23 2-4-2 24 2-5 28 2-5-1 30 2-5-2 31 2-5-3 32 2-5-4
More information第85 回日本感染症学会総会学術集会後抄録(III)
β β α α α µ µ µ µ α α α α γ αβ α γ α α γ α γ µ µ β β β β β β β β β µ β α µ µ µ β β µ µ µ µ µ µ γ γ γ γ γ γ µ α β γ β β µ µ µ µ µ β β µ β β µ α β β µ µµ β µ µ µ µ µ µ λ µ µ β µ µ µ µ µ µ µ µ
More informationuntitled
10 log 10 W W 10 L W = 10 log 10 W 10 12 10 log 10 I I 0 I 0 =10 12 I = P2 ρc = ρcv2 L p = 10 log 10 p 2 p 0 2 = 20 log 10 p p = 20 log p 10 0 2 10 5 L 3 = 10 log 10 10 L 1 /10 +10 L 2 ( /10 ) L 1 =10
More informationAppendix 1. CRC 13 Appendix Appendix LCGT 18 DECIGO 18 XMASS 19 GADZOOKS! 20 NEWAGE(
CRC 22 1 3 2 4 2-1 2-2 2-3 2-4 3 9 3-1 3-2 3-3 3-4 3-5 4 12 Appendix 1. CRC 13 Appendix 2. 14 Appendix 3. 17 LCGT 18 DECIGO 18 XMASS 19 GADZOOKS! 20 NEWAGE( ) 21 22 24 CTA (Cherenkov Telescope Array) 25
More informationJPS2016_Aut_Takahashi_ver4
CTA 111: CTA 7 A B A C D A E F G D H I J K H H J L H I A C B I A J I H A M H D G Dang Viet Tan G Daniela Hadasch A Daniel Mazin A C CTA-Japan A, B, Max-Planck-Inst. fuer Phys. C, D, ISEE E, F, G, H, I,
More information24.15章.微分方程式
m d y dt = F m d y = mg dt V y = dy dt d y dt = d dy dt dt = dv y dt dv y dt = g dv y dt = g dt dt dv y = g dt V y ( t) = gt + C V y ( ) = V y ( ) = C = V y t ( ) = gt V y ( t) = dy dt = gt dy = g t dt
More information[ ] [ ] [ ] [ ] [ ] [ ] ADC
[ ] [ ] [ ] [ ] [ ] [ ] ADC BS1 m1 PMT m2 BS2 PMT1 PMT ADC PMT2 α PMT α α = n ω n n Pn TMath::Poisson(x,[0]) 0.35 0.3 0.25 0.2 0.15 λ 1.5 ω n 2 = ( α 2 ) n n! e α 2 α 2 = λ = λn n! e λ Poisson Pn 0.1
More informationC:/KENAR/0p1.dvi
2{3. 53 2{3 [ ] 4 2 1 2 10,15 m 10,10 m 2 2 54 2 III 1{I U 2.4 U r (2.16 F U F =, du dt du dr > 0 du dr < 0 O r 0 r 2.4: 1 m =1:00 10 kg 1:20 10 kgf 8:0 kgf g =9:8 m=s 2 (a) x N mg 2.5: N 2{3. 55 (b) x
More informationELECTRONIC IMAGING IN ASTRONOMY Detectors and Instrumentation 4 The discovery power of modern astronomoical instruments 5 Instrumentation and dete
ELECTRONIC IMAGING IN ASTRONOMY Detectors and Instrumentation 4 The discovery power of modern astronomoical instruments 5 Instrumentation and detectors 4 2017/4/19 Contents 4.3 Polarization; transverse
More information0.,,., m Euclid m m. 2.., M., M R 2 ψ. ψ,, R 2 M.,, (x 1 (),, x m ()) R m. 2 M, R f. M (x 1,, x m ), f (x 1,, x m ) f(x 1,, x m ). f ( ). x i : M R.,,
2012 10 13 1,,,.,,.,.,,. 2?.,,. 1,, 1. (θ, φ), θ, φ (0, π),, (0, 2π). 1 0.,,., m Euclid m m. 2.., M., M R 2 ψ. ψ,, R 2 M.,, (x 1 (),, x m ()) R m. 2 M, R f. M (x 1,, x m ), f (x 1,, x m ) f(x 1,, x m ).
More informationMuon Muon Muon lif
2005 2005 3 23 1 2 2 2 2.1 Muon.......................................... 2 2.2 Muon........................... 2 2.3................................. 3 2.4 Muon life time.........................................
More informationMott散乱によるParity対称性の破れを検証
Mott Parity P2 Mott target Mott Parity Parity Γ = 1 0 0 0 0 1 0 0 0 0 1 0 0 0 0 1 t P P ),,, ( 3 2 1 0 1 γ γ γ γ γ γ ν ν µ µ = = Γ 1 : : : Γ P P P P x x P ν ν µ µ vector axial vector ν ν µ µ γ γ Γ ν γ
More informationAbstruct CANGAROO-III (PhotoMultiplier Tube PMT PMT ) PMT PMT R3479 ND 1 PMT 10 ( 90 ) Woomera PMT PMT (Light Guide LG) LG 0.944±0.023 PMT (4 ch) PMT
CANGAROOIII January 16, 2009 Abstruct CANGAROO-III (PhotoMultiplier Tube PMT PMT ) PMT PMT R3479 ND 1 PMT 10 ( 90 ) Woomera PMT PMT (Light Guide LG) LG 0.944±0.023 PMT (4 ch) PMT R8900U (HPKK) R8900U Bialkali
More information1 2 3
BL01604-103 JA DIGITAL CAMERA X-S1 http://fujifilm.jp/personal/digitalcamera/index.html 1 2 3 y y y y y c a b P S A M C1/C2/C3 E E E B Adv. SP F N h I P O W X Y d ISO Fn1 Fn2 b S I A b X F a K A E A Adv.
More informationuntitled
BELLE TOP 12 1 3 2 BELLE 4 2.1 BELLE........................... 4 2.1.1......................... 4 2.1.2 B B........................ 7 2.1.3 B CP............... 8 2.2 BELLE...................... 9 2.3
More informationB
B09170 5 8 ) ( ) π 0-1 s -1 sr -1 MeV HI Emissivity (3rd quadrant) -3-4 Abdo et al. 009 (6 months, P6V3_DIFFUSE) Local arm interarm Perseus arm and beyond Emissivity (MeV E -5-6 3 4 Energy (MeV) 5 1: 1
More informationIEEE HDD RAID MPI MPU/CPU GPGPU GPU cm I m cm /g I I n/ cm 2 s X n/ cm s cm g/cm
Neutron Visual Sensing Techniques Making Good Use of Computer Science J-PARC CT CT-PET TB IEEE HDD RAID MPI MPU/CPU GPGPU GPU cm I m cm /g I I n/ cm 2 s X n/ cm s cm g/cm cm cm barn cm thn/ cm s n/ cm
More information168 13 Maxwell ( H ds = C S rot H = j + D j + D ) ds (13.5) (13.6) Maxwell Ampère-Maxwell (3) Gauss S B 0 B ds = 0 (13.7) S div B = 0 (13.8) (4) Farad
13 Maxwell Maxwell Ampère Maxwell 13.1 Maxwell Maxwell E D H B ε 0 µ 0 (1) Gauss D = ε 0 E (13.1) B = µ 0 H. (13.2) S D = εe S S D ds = ρ(r)dr (13.3) S V div D = ρ (13.4) ρ S V Coulomb (2) Ampère C H =
More informationLHC ALICE (QGP) QGP QGP QGP QGP ω ϕ J/ψ ALICE s = ev + J/ψ
8 + J/ψ ALICE B597 : : : 9 LHC ALICE (QGP) QGP QGP QGP QGP ω ϕ J/ψ ALICE s = ev + J/ψ 6..................................... 6. (QGP)..................... 6.................................... 6.4..............................
More informationCopyrght 7 Mzuho-DL Fnancal Technology Co., Ltd. All rghts reserved.
766 Copyrght 7 Mzuho-DL Fnancal Technology Co., Ltd. All rghts reserved. Copyrght 7 Mzuho-DL Fnancal Technology Co., Ltd. All rghts reserved. 3 Copyrght 7 Mzuho-DL Fnancal Technology Co., Ltd. All rghts
More informationBethe-Bloch Bethe-Bloch (stopping range) Bethe-Bloch FNAL (Fermi National Accelerator Laboratory) - (SciBooNE ) SciBooNE Bethe-Bloch FNAL - (SciBooNE
21 2 27 Bethe-Bloch Bethe-Bloch (stopping range) Bethe-Bloch FNAL (Fermi National Accelerator Laboratory) - (SciBooNE ) SciBooNE Bethe-Bloch FNAL - (SciBooNE ) Bethe-Bloch 1 0.1..............................
More information204 / CHEMISTRY & CHEMICAL INDUSTRY Vol.69-1 January 2016 047
9 π 046 Vol.69-1 January 2016 204 / CHEMISTRY & CHEMICAL INDUSTRY Vol.69-1 January 2016 047 β γ α / α / 048 Vol.69-1 January 2016 π π π / CHEMISTRY & CHEMICAL INDUSTRY Vol.69-1 January 2016 049 β 050 Vol.69-1
More informationCherenkov Telescope Array Observations of gamma rays in 20 GeV 300 TeV band Cherenkov light from electromagnetic shower produced by interaction of gam
,,,,,, CTA-Japan consortium 2017, September 12 15, 2017 Cherenkov Telescope Array Observations of gamma rays in 20 GeV 300 TeV band Cherenkov light from electromagnetic shower produced by interaction of
More informationhirameki_09.dvi
2009 July 31 1 2009 1 1 e-mail: mtakahas@auecc.aichi-edu.ac.jp 2 SF 2009 7 31 3 1 5 1.1....................... 5 1.2.................................. 6 1.3..................................... 7 1.4...............................
More informationX 20, 1 1 HETE-2 Swift CCD GRB CCD CCD CCD
CCD 04RP019 20 3 7 X 20, 1 1 HETE-2 Swift CCD GRB CCD CCD CCD 1 6 1.1................... 6 1.2................... 8 1.3....................... 10 1.4............. 10 1.5................. 13 2 15 2.1..........................
More informationA B 5 C 9 3.4 7 mm, 89 mm 7/89 = 3.4. π 3 6 π 6 6 = 6 π > 6, π > 3 : π > 3
π 9 3 7 4. π 3................................................. 3.3........................ 3.4 π.................... 4.5..................... 4 7...................... 7..................... 9 3 3. p
More informationMicrosoft PowerPoint - TMTinst_ _summerschool_akiyama
1 2 3 4 5 6 7 8 9 10 590nm 2200nm 0 1.739 1.713 5 1.708 1.682 10 1.678 1.652 0-10 0.061061 0.061061 11 12 13 14 15 16 17 18 19 20 21 22 23 24 25 26 27 28 29 1.0 x1.0 0.5 x0.5 0.2 x0.2 0.1 x0.1 bg/30ms
More information(CN)
ONY CN ( ) (CN) ONY VAIO o-net ony Plaza Edy 1 1 1946 0 1955 CG( ) 1979 3 1986 10 199 3 9.3 1 3000 900 13 4 1988 CB CB ( ME)1989 ( PE) 1993 ME 50 (CE) 1995 1996 (o-net) 1997 001 P P, P P b a + r + r P
More informationスーパーカミオカンデにおける 高エネルギーニュートリノ研究
2009 11 20 Cosmic Ray PD D M P4 ? CR M f M PD MOA M1 ν ν p+p+p+p 4 He +2e - +2ν e MeV e - + p n+ ν e γ e + + e - ν x + ν x p + p, γ + p π + X π µ + ν µ e + ν µ + ν e TeV p + p π + X π µ + ν µ e + ν µ +
More informationx : = : x x
x : = : x x x :1 = 1: x 1 x : = : x x : = : x x : = : x x ( x ) = x = x x = + x x = + + x x = + + + + x = + + + + +L x x :1 = 1: x 1 x ( x 1) = 1 x 2 x =1 x 2 x 1= 0 1± 1+ 4 x = 2 = 1 ± 5 2 x > 1
More information日本分子第4巻2号_10ポスター発表.indd
JSMI Report 62 63 JSMI Report γ JSMI Report 64 β α 65 JSMI Report JSMI Report 66 67 JSMI Report JSMI Report 68 69 JSMI Report JSMI Report 70 71 JSMI Report JSMI Report 72 73 JSMI Report JSMI Report 74
More informationexample2_time.eps
Google (20/08/2 ) ( ) Random Walk & Google Page Rank Agora on Aug. 20 / 67 Introduction ( ) Random Walk & Google Page Rank Agora on Aug. 20 2 / 67 Introduction Google ( ) Random Walk & Google Page Rank
More information3 1 4 1.1......................... 4 1.1.1....................... 4 1.1.2.................. 4 1.1.3 Coulomb potential.............. 5 1.2.............
Fe muonic atom X 25 5 21 3 1 4 1.1......................... 4 1.1.1....................... 4 1.1.2.................. 4 1.1.3 Coulomb potential.............. 5 1.2.......................... 6 1.2.1...................
More information2 2. : ( Wikipedia ) 2. 3. 2 2. photoelectric effect photoelectron. 2. 3. ν E = hν h ν > ν E = hν hν W = hν
KEK 9,, 20 8 22 8 704 690 9 804 88 3.. 2 2. : ( Wikipedia ) 2. 3. 2 2. photoelectric effect photoelectron. 2. 3. ν E = hν h ν > ν E = hν hν W = hν 2.2. (PMT) 3 2: PMT ( / ) 2.2 (PMT) ν ) 2 2 00 000 PMT
More information1 2 3 P R
BL04700-101 JA DIGITAL CAMERA X-T1 Q Fn http://fujifilm.jp/personal/digitalcamera/index.html http://fujifilm-x.com/x-t1/ 1 2 3 P R y P y P y P y P Q R P V P Q Q Q Fn Fn1 Fn2 Fn3 Fn4 Fn5 Fn6 P S A M M
More informationJ表紙.dpt
250 16 IEC 60730 AA IEC 60065 1985 1989 1989 IEC 60085 1984 IEC 60127 1974 IEC 60161 1965 IEC60227-5 1997 450/750V IEC60245-4 1994 450/750V IEC 60317-0-1 1990 IEC60384-14 1993 14 IEC 60730 IEC61000-2-2
More information一般演題(ポスター)
6 5 13 : 00 14 : 00 A μ 13 : 00 14 : 00 A β β β 13 : 00 14 : 00 A 13 : 00 14 : 00 A 13 : 00 14 : 00 A β 13 : 00 14 : 00 A β 13 : 00 14 : 00 A 13 : 00 14 : 00 A β 13 : 00 14 : 00 A 13 : 00 14 : 00 A
More informationJ表紙.dpt
1 1. 1.1 440V 63A 1 2 3 4 5 6 IEC 61058-1 IEC 61058-2 IEC 61058-2 1.2 1.3 1.4 IEC 60669 IEC 61058-2 1.5 1.6 IEC 60730 2. IEC 61058 1 IEC 60034-1 1996 1 1 1997 2 1999 1 IEC 60038 1983 IEC IEC 60050(151)
More informationboost_sine1_iter4.eps
3 (, 3D ) 2. 2 3.. 3D 3D....,,. a + b = f, a, f. b a (.) b a.: b f (.2), b f., f.2. 2 Y y Q(X,Y,Z) O f o q(x,y) Z X x image plane.2:.2, O, z,. O..2 (X, Y, Z) 3D Q..2 O f, x, y X, Y. Q OQ q, q (x, y). x
More information無印良品 2012 自転車 カタログ
26 897895321,000 140cm 76.0cm 16.0kg H LED 3 263 897896025,000 140cm 76.0cm 16.5kg H 3 LED 20 8978984 8978977 19,800 134cm 73.0cm 15.0kg LED 2620 2620 8486656550 5536207483 14512372,100 8279999840 26 77342561,417
More information1 1 ( ) ( 1.1 1.1.1 60% mm 100 100 60 60% 1.1.2 A B A B A 1
1 21 10 5 1 E-mail: qliu@res.otaru-uc.ac.jp 1 1 ( ) ( 1.1 1.1.1 60% mm 100 100 60 60% 1.1.2 A B A B A 1 B 1.1.3 boy W ID 1 2 3 DI DII DIII OL OL 1.1.4 2 1.1.5 1.1.6 1.1.7 1.1.8 1.2 1.2.1 1. 2. 3 1.2.2
More information03J_sources.key
Radiation Detection & Measurement (1) (2) (3) (4)1 MeV ( ) 10 9 m 10 7 m 10 10 m < 10 18 m X 10 15 m 10 15 m ......... (isotope)...... (isotone)......... (isobar) 1 1 1 0 1 2 1 2 3 99.985% 0.015% ~0% E
More informationuntitled
masato@icrr.u-tokyo.ac.jp 996 Start 997 998 999 000 00 00 003 004 005 006 007 008 SK-I Accident Partial Reconstruction SK-II Full reconstruction ( SK-III ( ),46 (40%) 5,8 (9%),9 (40%) 5MeV 7MeV 4MeV(plan)
More information1 2 2 (Dielecrics) Maxwell ( ) D H
2003.02.13 1 2 2 (Dielecrics) 4 2.1... 4 2.2... 5 2.3... 6 2.4... 6 3 Maxwell ( ) 9 3.1... 9 3.2 D H... 11 3.3... 13 4 14 4.1... 14 4.2... 14 4.3... 17 4.4... 19 5 22 6 THz 24 6.1... 24 6.2... 25 7 26
More informationPowerPoint Presentation
/ 2008/04/04 Ferran Salleras 1 2 40Gb/s 40Gb/s PC QD PC: QD: e.g. PCQD PC/QD 3 CP-ON SP T CP-OFF PC/QD-SMZ T ~ps, 40Gb/s ~100fJ T CP-ON CP-OFF 500µm500µm Photonic Crystal SMZ K. Tajima, JJAP, 1993. Control
More information/...8 ISO D i K UHD JPEG...27 HDMI
Professional ...4...6...8 /...8 ISO...10...11...12 D-...13...14...14...14...15...15...18...21 i...22...24...25...26 4K UHD JPEG...27 HDMI...28 2 ...31...31...31...33 4K UHD...34...36...36...36...37...37...38
More informationCAT. No. 1154b 2008 C-9
T CAT. o. 1154b IS SK µm D K mm & Dmp 1 ea µm d CS mm & Bs K ia & dmp V dp & dmp & Hs 1 mm d & ds & & B2s d2s & Hs & A1s d d B C B2 H A1 SjD d2 H d µm d & dmp & d1mp & dmp V dp 1 mm d d d B & dmp & d1mp
More informationDrift Chamber
Quench Gas Drift Chamber 23 25 1 2 5 2.1 Drift Chamber.............................................. 5 2.2.............................................. 6 2.2.1..............................................
More information3 3 i
00D8102021I 2004 3 3 3 i 1 ------------------------------------------------------------------------------------------------1 2 ---------------------------------------------------------------------------------------2
More informationdvipsj.4131.dvi
7 1 7 : 7.1 3.5 (b) 7 2 7.1 7.2 7.3 7 3 7.2 7.4 7 4 x M = Pw (7.3) ρ M (EI : ) M = EI ρ = w EId2 (7.4) dx 2 ( (7.3) (7.4) ) EI d2 w + Pw =0 (7.5) dx2 P/EI = α 2 (7.5) w = A sin αx + B cos αx 7.5 7.6 :
More informationuntitled
MPPC 18 2 16 MPPC(Multi Pixel Photon Counter), MPPC T2K MPPC T2K (HPK) CPTA, MPPC T2K p,π T2K > 5 10 5 < 1MHz > 15% 200p.e. MIP 5p.e. p/π MPPC HPK MPPC 2 1 MPPC 5 1.1...................................
More informationスライド 1
CTA 開発研究 手嶋政廣 ( 代理発表 戸谷友則 ) for CTA-Japan Consortium CTA 手嶋研究費 170 万 旅費 85 万計 255 万 CTA 戸谷研究費 20 万 旅費 80 万計 100 万 観測天体 超新星残骸 連星系 銀河団 Cherenkov Telescope Array 超高エネルギー宇宙ガンマ線の研究 活動銀河核 ガンマ線バースト 狙うサイエンス 宇宙線の起源
More informationatomic line spectrum emission line absorption line atom proton neutron nuclei electron Z atomic number A mass number neutral atom ion energy
1 22 22.1 atomic line spectrum emission line absorption line atom proton neutronnuclei electron Z atomic number A mass number neutral atom ion energy level ground stateexcited state ionized state 22.2
More information(1) 1.1
1 1 1.1 1.1.1 1.1 ( ) ( ) ( ) { ( ) ( ) { ( ) ( ) { ( ) ( ) { ( ) ( ) { ( ) ( ) ( ) ( ) ( ) 2 1 1.1.2 (1) 1.1 1.1 3 (2) 1.2 4 1 (3) 1.3 ( ) ( ) (4) 1.1 5 (5) ( ) 1.4 6 1 (6) 1.5 (7) ( ) (8) 1.1 7 1.1.3
More informationuntitled
(1) 100 100 60% (2) (3) - 1 - 1 2 3 4 100 200-2 - 1 2 3-3 - 4 5 6 7......... (1) (2) (3) 1) 2) 3) 8(5) - 4 - 0.5 27.3 3 0.05 27.30 4 0.005 Système International d'unités 7218 1 (1) Pas Pas J/molK J/(molK)
More informationΛ (Λ ) Λ (Ge) Hyperball γ ΛN J-PARC Λ dead time J-PARC flash ADC 1 dead time ( ) 1 µsec 3
19 Λ (Λ ) Λ (Ge) Hyperball γ ΛN J-PARC Λ dead time J-PARC flash ADC 1 dead time ( ) 1 µsec 3 1 1 1.1 γ ΛN................. 1 1.2 KEK J-PARC................................ 2 1.2.1 J-PARC....................................
More information(e ) (µ ) (τ ) ( (ν e,e ) e- (ν µ,µ ) µ- (ν τ,τ ) τ- ) ( ) ( ) ( ) (SU(2) ) (W +,Z 0,W ) * 1) [ ] [ ] [ ] ν e ν µ ν τ e µ τ, e R,µ R,τ R (2.1a
1 2 2.1 (e ) (µ ) (τ ) ( (ν e,e ) e- (ν µ,µ ) µ- (ν τ,τ ) τ- ) ( ) ( ) ( ) (SU(2) ) (W +,Z 0,W ) * 1) [ ] [ ] [ ] ν e ν µ ν τ e µ τ, e R,µ R,τ R (2.1a) L ( ) ) * 2) W Z 1/2 ( - ) d u + e + ν e 1 1 0 0
More informationサイバニュース-vol134-CS3.indd
NEWS 2012 WINTER 134 No. F=maF ma m af Contents N, X θ 1,θ 2 θ N 0θ i π/2 X i X 0 Θ i Θ 1 = 2θ 1 Θ 2 = 2(θ 1 θ 2) NX N X 0 Θ N N Θ N = 2{θ 1 θ 2θ 3 θ N } Θ N = 2π A 1A 2B 2B 1 mm 3 α α = π /m A 1A
More information2 X-ray 6 gamma-ray 7 1 17.1 0:38m 0:77m nm 17.2 Hz Hz 1 E p E E = h = ch= (17.2) p = E=c = h=c = h= (17.3) continuum continuous spectrum line spectru
1 17 object 1 observation 17.1 X electromagnetic wave photon 1 = c (17.1) c =3 10 8 ms ;1 m mm = 10 ;3 m m =10 ;6 m nm = 10 ;9 m 1 Hz 17.1 spectrum radio 2 infrared 3 visual light optical light 4 ultraviolet
More informationA13 C A139 A137 A131 A138 V CV FC/SMA 2.51/2.5 MM FF 4 4 5 5 6 A11971 A136 ND A132 1 mm ND1 % 1 %2 6 7 7 A133-9 15 mm 8 A134-9 A135 A135-9 A1127 A1858 A176 A1859 C A11213 C A9865 45V R T 11 15 mm XY XZ
More informationさくらの個別指導 ( さくら教育研究所 ) A AB A B A B A AB AB AB B
1 1.1 1.1.1 1 1 1 1 a a a a C a a = = CD CD a a a a a a = a = = D 1.1 CD D= C = DC C D 1.1 (1) 1 3 4 5 8 7 () 6 (3) 1.1. 3 1.1. a = C = C C C a a + a + + C = a C 1. a a + (1) () (3) b a a a b CD D = D
More information第86回日本感染症学会総会学術集会後抄録(II)
χ μ μ μ μ β β μ μ μ μ β μ μ μ β β β α β β β λ Ι β μ μ β Δ Δ Δ Δ Δ μ μ α φ φ φ α γ φ φ γ φ φ γ γδ φ γδ γ φ φ φ φ φ φ φ φ φ φ φ φ φ α γ γ γ α α α α α γ γ γ γ γ γ γ α γ α γ γ μ μ κ κ α α α β α
More information3-2 PET ( : CYRIC ) ( 0 ) (3-1 ) PET PET [min] 11 C 13 N 15 O 18 F 68 Ga [MeV] [mm] [MeV]
3 PET 3-1 PET 3-1-1 PET PET 1-1 X CT MRI(Magnetic Resonance Imaging) X CT MRI PET 3-1 PET [1] H1 D2 11 C-doxepin 11 C-raclopride PET H1 D2 3-2 PET 0 0 H1 D2 3-1 PET 3-2 PET ( : CYRIC ) ( 0 ) 3-1-2 (3-1
More informationmain.dvi
A 1/4 1 1/ 1/1 1 9 6 (Vergence) (Convergence) (Divergence) ( ) ( ) 97 1) S. Fukushima, M. Takahashi, and H. Yoshikawa: A STUDY ON VR-BASED MUTUAL ADAPTIVE CAI SYSTEM FOR NUCLEAR POWER PLANT, Proc. of FIFTH
More informationTelescope aperture 1.5mφ Telescope length Fit within the H-IIA nose fairing Spatial resolution 0.1" in UV 0.16" in Vis/NIR (Diffraction limit of 1.5mφ
, (NAOJ) (Kyoto U.) Telescope aperture 1.5mφ Telescope length Fit within the H-IIA nose fairing Spatial resolution 0.1" in UV 0.16" in Vis/NIR (Diffraction limit of 1.5mφ at 1µm ) FOV ~200" x 200" to cover
More information2
Rb Rb Rb :10256010 2 3 1 5 1.1....................................... 5 1.2............................................. 5 1.3........................................ 6 2 7 2.1.........................................
More information1 3 1.1 PET..................................... 3 1.1.1......................................... 3 1.1.2 PET................................. 4 1.2..
21 PET 06S2037G 2010 3 1 3 1.1 PET..................................... 3 1.1.1......................................... 3 1.1.2 PET................................. 4 1.2........................................
More information/...8 ISO i K UHD JPEG...28 HDMI K UHD..
Professional Revision 1.0 ...4...6...8 /...8 ISO...10...11...12...13...13...13...14...14...18...22 i...23...24...25...26 4K UHD JPEG...28 HDMI...29...32...32...32...34 4K UHD...35 2 ...37...37...37...38...38...39
More information放射線化学, 97, 29 (2014)
20 5 Absorption spectra of biomolecules over wide energy range are very important to study their radiation effects in terms of the optical approximation proposed by Platzman. Using synchrotron radiation
More informationAF... 4 AF
Professional AF... 4 AF...5... 8...9...10...12...13...16...18...21...22...23...25...25...28...29...30...31 2 35mm...34...35...38...38...41...43...46...46...47...48...49...50...51 RAW...52 RAW...52 RAW...53
More informationCWContinuous Wave CW 1.1.2 XCT(Computed Tomography) MRI Magnetic Resonance Imaging)PET(Positron Emission Tomography) XCT 2
1.1 1.1.1 RadarRadio Detection and Ranging 1960 1 10 1 CWContinuous Wave CW 1.1.2 XCT(Computed Tomography) MRI Magnetic Resonance Imaging)PET(Positron Emission Tomography) XCT 2 3 XCTMRI XCTMRI XCT /10
More information54_2-05-地方会.indd
82 58 59 21 83 84 2 9 4 85 86 1. 87 6 88 89 β 1 90 2 3 p 4 t 5 6 EQ 91 7 8 9 1 10 2 92 11 3 12 13 IT p 14 93 15 16 ACTIVE 17 18 94 p p p 19 20 21 22 95 23 24 25 2 26 β β 96 27 1 28 29 30 97 31 32 33 1
More informationEOS DIGITAL ソフトウェア使用説明書
Canon Utilities ImageBrowser. CameraWindow. RAW Image Task. EOS Capture. PhotoStitch. EOS-D Mark II N EOS-Ds Mark II EOS D EOS Kiss Digital N EOS-D Mark II EOS 0D EOS-Ds EOS-D EOS Kiss Digital EOS 0D EOS
More information