X 20, 1 1 HETE-2 Swift CCD GRB CCD CCD CCD

Size: px
Start display at page:

Download "X 20, 1 1 HETE-2 Swift CCD GRB CCD CCD CCD"

Transcription

1 CCD 04RP

2 X 20, 1 1 HETE-2 Swift CCD GRB CCD CCD CCD

3 GRB GRB WIDGET CCD CCD CCD CCD CCD ST-9XE CCD CCD CCD CCD dark frame dark count

4 4.2.2 dark count dark count hot pixel dead pixel hot pixel dead pixel light count linearity CCD CCD

5 1.1 BATSE GRB030329/SN2003dh GRB SN2003dh BeppoSAX GRB X GRB ROTSE CGRO BATSE 1234 GRB (T 90 ) GRB ( ) TAROT( 25cm) GRB ( ) GRB(z=6.3)[14] GRB (I-band ) X (0.5-10ev ) light curve prompt emission afterglow [14] ROTSE-III( 45cm) 19 VLT( 8m) GRB X light curve X

6 2.1 X ( ) GRB WIDGET cm Schmidt GCN WIDGET Shnidt follow-up follow-up CCD ST-9XE MEADE LX ST-9XE Interline Frame transfer Full frame transfer CCD CCDOPS dark frame dark count log(adu) 1/T dark count dark count dark frame dark count hot pixel [ ] 60[sec] hot pixel [ ] 2[sec]

7 4.15 light count linearity CCD CCD CCD

8 1 (GRB) erg VELA BATSE 1 GRB 2 - X BeppoSAX GRB GRB GRB GRB 6

9 1.1: BATSE HETE-2 HETE-2 GRB HETE-2 GRB X GRB GRB 2004 Swift GRB Swift Short GRB GRB 1 GLAST MAXI 7

10 GRB 20 GRB 1.2: GRB030329/SN2003dh GRB SN2003dh 1.2 GRB X BeppoSAX GRB GRB BeppoSAX X X X (t 1 ) 8

11 1.3: BeppoSAX GRB X 8 3 GRB GRB Swift X X Swift 100 GRB

12 図 1.4: GRB の可視光残光 左はバースト当日 右は 8 日後 1.3 可視光フラッシュ 可視光フラッシュは GRB で初めて捉えられた これはバースト 発生後 急激に明るくなる現象である GRB では バースト発生 後 22 秒から観測が始まり その約 50 秒後に約 9 等級に増光し その後急 激に減光した その後の観測からこの GRB は z = 1.6 という高赤方偏 移で起こったことが明らかとなった この可視光フラッシュは 観測例が 少なく どのバーストでも起きることなのかは はっきりとしていない GRB は バーストの中でも明るい方であったが バーストの明る さと可視光フラッシュの相関も不明である 観測データが少ないため こ の現象については 発生直後からの連続した観測が重要であり 今後の観 測体制の充実に期待される 1.4 ガンマ線バーストの種類と起源天体 ガンマ線バーストの継続時間は 図 1.6 で示されるように 2 つに種類 に分けられる 一般に 継続時間 2 秒以上のものを Long GRB 2 秒以下 のものを Short GRB と呼んでいる この中で詳細な観測が進んでいるのは Long GRB である Short GRB は 継続時間が 2 秒と短く 検出される光子数も Long GRB に比べ 相 対的に少ないからである このため 残光が捉えにくく 起源や母銀河も 分からなかった また BeppoSAX は Short GRB を検出しにくい装置 であったため Short GRB の研究が進むには 観測装置の進歩を待たね ばならなかった Short GRB の残光は Swift 衛星により GRB050509B で初めて捉えら 10

13 1.5: ROTSE GRB GRB Long GRB 1 Ic (hypernova) Long GRB GRB 1 Short GRB 100 Short GRB 11

14 1.6: CGRO BATSE 1234 GRB (T 90 ) 2 2 X (X-Ray Flash) (X (X-Ray Rich GRB) ) X 1.7: GRB ( ) 12

15 GRB GRB 2 GRB GRB :51:44(UT) Swift/BAT TAROT(25cm) 5 z = 6.29 GRB 1.8: TAROT( 25cm) GRB ( 1.9: GRB (Iband ) X (0.5-10ev ) ) light curve prompt emission GRB(z=6.3)[14] afterglow [14] GRB z = GRB 20 GRB Schmidt (105cm)

16 1.10: ROTSE-III( 45cm) : GRB X VLT( 8m) light curve X GRB GRB GRB 14

17 2 2.1 WIDGET 105cm Schmidt GRB X Swift X GRB X GRB X GRB HETE-2 BeppoSAX 5 6 HETE-2 Swift 15

18 2.1: X ( ) 2.2: GRB X Swift GRB 16

19 2.2 GRB GRB GRB 2.1 GRB 1.5 GRB ( ) GRB TAROT ( ) 25cm GRB050904,GRB060111B ROTSE-III ( ) 45cm GRB050401,GRB MASTER ( ) 20cm GRB RAPTOR ( ) 40cm 4 4 GRB041219A,GRB050820A REM ( ) 60cm GRB : GRB WIDGET WIDGET(WIDefild telescope for GRB Early Timing) WIDGET Swift/BAT /6 WIDGET follow-up 17

20 2.3: WIDGET 2.4: 105cm Schmidt 2.3 GRB GCN(The Gamma-ray bursts Coordination Network) 3 GRB GRB WIDGET Schmidt GRB precursor BAT GRB GCN Swift Schmidt 18

21 2.5: GCN 2.6: WIDGET Shnidt follow-up follow-up

22 2.4 MEADE LX90-30 CCD SBIG ST-9XE PC CCD GRB CCD PC WIDGET [mm] [mm] f/ /sec 2.2: MEADE LX : CCD ST-9XE 2.8: MEADE LX

23 3 CCD CCD CCD 3.1 CCD CCD Charge Coupled Device (pixel) 1 2 CCD CCD CCD CCD 1 ST-9XE 600[nm] 67 CCD ST-9XE 3.1 CCD Si Si 1.14[eV] ( [eV], [nm]) [nm] CCD CCD pn p n n p 21

24 3.1: ST-9XE CCD CCD ( ) 4. 22

25 ( ) CCD CCD Interline (IL ) : Interline Frame trnsfer(ft )

26 Full frame transfer(fft ) FT FT CCD Full frame transfer CCD AD 16bit ADU(Analog to Degital Unit) 3.3: Frame transfer 3.4: Full frame transfer 3.2 CCD CCD Boltzmann exp( E g /2k B T ) CCD CCD 24

27 1 3.3 CCD CCD CCD 5 1. CCD CCD CCD

28 3.4 CCD ST-9XE CCD ST-9XE ST-9XE CCD Kodak KAF-0261E-NABG TI TC mm 262,144 pixel µ 4e/pixel 0 A/D 16bit A/D Gain 2.2e /ADU 15e RMS AD 420,000 pixel/sec FFT 1[sec] : ST-9XE 26

29 4 CCD CCD CCD CCD 4.1 CCD 3.2 CCD CCD CCD ST-9XE 4.1 CCD USB CCDOPS Windows ( 4.2) CCD CCD CCD ( 3.1) 27

30 4.1: 4.2: CCD CC- DOPS [ ] [ ] [ ] : CCD CCD CCD 28

31 CCD CCD CCD [ ] [ ] : CCD

32 30 20 temperature vs time temperature [ time [sec] 0-5 temperature vs time temperature [ time [min] 4.3: 30

33 1000 log(time) vs 1/T (set point -5[ log(time) vs 1/T (set point -10[ -10 log(time) [sec] 100 log(time) [sec] /T [/K] /T [/K] 1000 log(time) vs 1/T (set point -15[ log(time) vs 1/T (set point -20[ -20 log(time) [sec] log(time) [sec] /T [/K] /T [/K] 4.4: [ ] [sec 1 ] ± ± ± ± : 31

34 4.5: dark frame 4.2 dark frame dark frame dark frame dark frame dark count bias frame 0 bias bias AD 0 bais bias count light frame light count dark frame dark count bias count light frame dark frame bias frame bias dark count light frame dark frame dark count dark count CCD 32

35 dark count [ADU] dark count vs temperature (integral time 60) f(x)= exp(0.060x) g(x)= exp(0.071x) mean stddev temperature [ 4.6: 60 dark count dark count dark frame IRAF imcombain 10 dark count 60 dark count dark count CCD Boltzmann exp( E g /2k B T ) CCD CCD dark count 33

36 logadu vs 1/T (integral time 60[sec]) mean stddv log(dark count) [ADU] /T [/K] 4.7: log(adu) 1/T log(adu) E g 1.6[eV] dark count CCD 1 1 count ,90,120,180,300 dark frame dark count count IRAF dark count 4.8 5, 10, dark count dark count 4.8 dark count 34

37 dark count 1 dark count count [ADU/sec] Gain 2.2 [e /ADU] 4.4. [ ] dark current [e /sec/pixel] ± ± ± : 35

38 dark count vs integral time dark count [ADU] f(x)=3.073x g(x)=1.821x h(x)=1.103x dark count f(x)=1.811x integral time [sec] dark count vs integral time ( dark count [ADU] integral time [sec] 4.8: dark count 36

39 4.2.3 dark count dark count dark frame dark count 10 5[sec] 100 dark count dark count [ADU] [ADU] +40, 30 count count stability (-10[ dark count mean 200 dark count number of frame 4.9: dark count 37

40 CCD dark count count dark count 300 dark coumt vs number of frame (-10[ dark count 250 dark count [ADU] number of frame temperature vs number of frame (-10[ -8 dark count -8.5 temperature [ number of frame 4.10: 10 dark frame dark count dark frame 38

41 4.3 hot pixel dead pixel CCD hot pixel,dead pixel hot pixel dead pixel CCD 1pixel hot pixel 4.11: hot pixel hot pixel dark frame 10 60[sec] dark frame fits 199.7[ADU] count 10000[ADU] pixel pixel 1 (x,y)=(433,80) 56455[ADU] 4.13 pixel hot pixel 39

42 pixel histgram (-10[ number of pixel dark count [ADU] 4.12: 10[ ] 60[sec] ST9XE hot pixel 500 pixel 400 y pixel (433,80) x pixel 4.13: hot pixel dead pixel dead pixel light frame 10 2[sec] hot pixel fit 4.14 count dead pixel dead pixel 40

43 1e+06 pixel histgram (-10[ number of pixel light count [ADU] 4.14: -10[ ] 2[sec] 4.4 light count linearity CCD CCD 16bit linearity linearity 10 1 light frame CCD 2 1 count 10000[ADU] 1 pixel 2 count 1000[ADU] light frame dark frame [ADU] linearity count 64000[ADU] linearity 4.15 count 5000[ADU] 41

44 light count linearity light count f(x)=9279x light count [ADU] integral time [sec] light count f(x)=899.6x light linearity date 12/14 light count [ADU] integral time [sec] 4.15: light count linearity 42

45 light frame (LED) linearity [ADU] count 50000[ADU] linearity. 43

46 4.5 CCD CCD CCD ST-9XE CCD CCD CCD 4.17: CCD 4.16: CCD

47 960W CCD CCD CCD CCD CCD CCD CCD CCD CCD , 45

48 4.18: CCD CCD 32 5 dark count 15 dark count Linearity 46

49 dark count light count pixel hot pixel 1 daed pixel CCD : 10 : 20 CCD dark frame ( ) CCD 4.19 CCD CCD 3 12 CCD dark frame light frame WIDGET 47

50 CCD : temp= : temp=10 no -12 yes no yes : 5 : -5 15[min] later : 0 : [min] later : -5 : [min] later light frame 5[sec], 10 yes : -5 : -15 : 0 : -10 no : -10 : [min] later : 5 : -5? temp temp no : 10 : 0 yes dark frame 5[sec], : CCD 48

51 5 CCD GRB 2 CCD 3 49

52 GRB WIDGET 5 50

53 [1] (2001 ) [2] WIDGET (2004 ) [3] CCD GRB (2005 ) [4] (2007 ) [5] GRB (2006 ) [6] [7] CCD [8] [9] Steve B. Howell Handbook of CCD Astronomy [10] M.Boer at al 2006,ApJ [11] A.E.RuIZ-VELASCO at el. 2007,ApJ [12] [13] [14] 51

Recent results from Swift

Recent results from Swift Some recent results from Swift Masaki Mori Goro Sato, presentation for Ph.D. thesis defense (January 2006) P. Jakobsson et al., A&A 447, 897 (2006) N. Kawai et al., astro-ph/0512052 ICRR CANGAROO group

More information

Deep Sky Imager ユーザーズ・マニュアル:基礎編

Deep Sky Imager ユーザーズ・マニュアル:基礎編 Meade Deep Sky Imager - 1 - Copyright 2005 MIC International Co. Ltd, All Rights Reserved. Deep Sky Imager USB DB9RJ11 LX200 #497 CD Deep Sky Imager Autostar Suite CPU Pentium II/400MHz Pentium 4/2GHz

More information

untitled

untitled 13 50 15 6.0 0.25 220 23 92 960 16 16 3.9 3.9 12.8 83.3 7 10 1150 90 1035 1981 1850 4700 4700 15 15 1150 1150 10 12 31 1.5 3.7%(224 ) 1.0 1.5 25.4%(1522 ) 0.7 30.6 1835 ) 0.7 1.0 40.3 (2421 ) 7.3

More information

Akira MIZUTA(KEK) AM, Nagataki, Aoi (ApJ, , 2011) AM + (in prep)

Akira MIZUTA(KEK) AM, Nagataki, Aoi (ApJ, , 2011) AM + (in prep) Akira MIZUTA(KEK) AM, Nagataki, Aoi (ApJ, 732 26, 2011) AM + (in prep) 2011.12.28 GRB GRB. ex. GRB980425/SN1998bw, GRB030329/SN2003dh XRF060218/SN2006aj. GRB091127/SN2009nz XRF100316D/SN2010bh Spectrum

More information

太陽系外惑星探査

太陽系外惑星探査 http://hubblesite.org/newscenter/archive/2001/38/ Terra MODIS http://modarch.gsfc.nasa.gov/ http://www.nasa.gov/home/index.html / 2 Are we alone? Origins Where are they? (Fermi 1950) 3 4 0.5 arcsec 10pc

More information

50cm

50cm 50cm 2005 2 Abstract Gamma-ray bursts (GRBs) are the largest explosions at large distances. The purpose of our study is to observe GRBs and their afterglows to investigate the physical mechanism of GRBs.

More information

DAC121S101/DAC121S101Q 12-Bit Micro Power, RRO Digital-to-Analog Converter (jp)

DAC121S101/DAC121S101Q 12-Bit Micro Power, RRO Digital-to-Analog Converter (jp) DAC121S101 DAC121S101/DAC121S101Q 12-Bit Micro Power, RRO Digital-to-Analog Converter Literature Number: JAJSA89 DAC121S101 12 D/A DAC121S101 12 D/A (DAC) 2.7V 5.5V 3.6V 177 A 30MHz 3 SPI TM QSPI MICROWIRE

More information

0.45m1.00m 1.00m 1.00m 0.33m 0.33m 0.33m 0.45m 1.00m 2

0.45m1.00m 1.00m 1.00m 0.33m 0.33m 0.33m 0.45m 1.00m 2 24 11 10 24 12 10 30 1 0.45m1.00m 1.00m 1.00m 0.33m 0.33m 0.33m 0.45m 1.00m 2 23% 29% 71% 67% 6% 4% n=1525 n=1137 6% +6% -4% -2% 21% 30% 5% 35% 6% 6% 11% 40% 37% 36 172 166 371 213 226 177 54 382 704 216

More information

10 117 5 1 121841 4 15 12 7 27 12 6 31856 8 21 1983-2 - 321899 12 21656 2 45 9 2 131816 4 91812 11 20 1887 461971 11 3 2 161703 11 13 98 3 16201700-3 - 2 35 6 7 8 9 12 13 12 481973 12 2 571982 161703 11

More information

スライド 1

スライド 1 グループ発表天体核研究室 低光度ガンマ線バーストの起源 D2 当真賢二 宇宙ひもを重力レンズで探る D3 須山輝明 2006 年度物理学第二教室教室発表会 @ 第四講義室 天体核研究室の大雑把な研究グループ 天体物理学中村 犬塚 井岡 山田 PD: 町田 石津 三浦 D3: 道越 宇宙論中村 田中 早田 D3: 須山 D2: 横山 D1: 泉 M2: 棚橋 村田 D2: 井上 ( 剛 ) 当真 D1:

More information

Telescope Array FD SD SD

Telescope 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

fma20.PDF

fma20.PDF PZT TSC Measurement for Degraded and Damaged PZT Thin Films Capacitors Prepared by Sputtering. FeRAM MFIS : XRD, TEM : XRF, EDS, EPMA, SIMS : SPM, NDM? DLTS DLTS (TSC) (TSC) fatigue,, ( ) (1) (2) J T TSC

More information

7-1yamazaki.pptx

7-1yamazaki.pptx Suzaku/ASTRO-H Suzaku/ASTRO-H 1. Vela ( Watchman ) (1967 1979): GRB (1969) 2. GINGA (1987 1991): X-ray counterpart GRB (galactic) X-ray burst? 3. BATSE (1991 2000): Galactic origin models!!! 4. BeppoSAX

More information

1 3 1.1 PET..................................... 3 1.1.1......................................... 3 1.1.2 PET................................. 4 1.2..

1 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

ADC121S Bit, ksps, Diff Input, Micro Pwr Sampling ADC (jp)

ADC121S Bit, ksps, Diff Input, Micro Pwr Sampling ADC (jp) ADC121S625 ADC121S625 12-Bit, 50 ksps to 200 ksps, Differential Input, Micro Power Sampling A/D Converter Literature Number: JAJSAB8 ADC121S625 12 50kSPS 200kSPS A/D ADC121S625 50kSPS 200kSPS 12 A/D 500mV

More information

1 158 14 2 8 00225 2 1.... 3 1.1... 4 1.2... 5 2.... 6 2.1...7 2.2... 8 3.... 9 3.1... 10 3.2... 16 4.... 17 4.1... 18 4.2... 20 4.3... 22 5.... 23 5.1... 24 5.2... 28 5.3... 34 5.4... 37 5.5... 39 6....

More information

HITACHI HF-2000

HITACHI HF-2000 HITACHI HF-2000 v. 4. 1 1. 2. 3. 4. 5. 6. 7. 8. 9. 10. 11. 12. 13. 14. TV 15. 16. 17. 15 5-1 - 1. 1.1 COLUMN ON 1.2 OBJ. TEMP. MONITOR 20 1.3 POWER HV IP-1 ON ON LOCK (

More information

MultiWriter 5600C 活用マニュアル

MultiWriter 5600C 活用マニュアル 1 *1 2 3 4 5 6 7 8 1 2 3 4 5 6 7 8 9 9 1 2 3 10 11 12 13 14 15 16 17 18 19 20 21 22 23 24 25 1 2 3 a b c 26 27 28 C *1 *2 *2 29 2 2 2 2 2 2 2 2 2 30 *1 *2 ± *1 C C 31 32 33 34 35 36 M C Y K 1 2 3 4 5 6

More information

PowerPoint Presentation

PowerPoint Presentation ガンマ線バースト : ブラックホールの誕生 井岡邦仁 ( 天体核 ) E=mc 2 = = 原子爆弾 太陽 ~10 33 g GRB ~10 52 erg 太陽が一生かけて出すエネルギーを数秒で放出 GRB は宇宙一明るい謎の天体 電磁波 高エネルギー宇宙物理 1967 Vela 衛星が発見核実験の監視衛星ところが γ 線は地球外から! 1973 発表 偶然の発見 高度 12 万 km 周期 5 日

More information

2014.3.10 @stu.hirosaki-u.ac.jp 1 1 1.1 2 3 ( 1) x ( ) 0 1 ( 2)NOT 0 NOT 1 1 NOT 0 ( 3)AND 1 AND 1 3 AND 0 ( 4)OR 0 OR 0 3 OR 1 0 1 x NOT x x AND x x OR x + 1 1 0 x x 1 x 0 x 0 x 1 1.2 n ( ) 1 ( ) n x

More information

untitled

untitled [] 03084 [Pieters et al. 1993] m 21 600-1600 nm 8 nm 8 nm9 km 20 km SN 200 [ MT-300 F5.5 150 cm][ ] [600-1000 nm][1000-1600 nm] CCD [SBIG ST-7E Si-CCD ][SU IncSU320-1.7RT-DInGaAs-CCD ] PC [Phillips co.

More information

pc725v0nszxf_j

pc725v0nszxf_j PC725NSZXF PC725NSZXF PC725NSZXF PC725 DE file PC725 Date Jun. 3. 25 SHARP Corporation PC725NSZXF 2 6 5 2 3 4 Anode Cathode NC Emitter 3 4 5 Collector 6 Base PC725NSZXF PC725YSZXF.6 ±.2.2 ±.3 SHARP "S"

More information

pc817xj0000f_j

pc817xj0000f_j PC87XJF PC87XJF PC87XJF PC87XJF PC87 Date Jun.. 5 SHRP Corporation PC87XJF node Cathode Emitter Collector PC87XJF PC87XIJF node mark. ±..6 ±. Rank mark Factory identification mark Date code PC87.58 ±.5

More information

214 1 11 SU UMa AY Lyr AY ASASSN-14jv CCD ASASSN-14jv SU UMa WZ Sge 28 29 AY Lyr O-C

214 1 11 SU UMa AY Lyr AY ASASSN-14jv CCD ASASSN-14jv SU UMa WZ Sge 28 29 AY Lyr O-C AY Lyr ASASSN-14jv CCD I11G22 214 1 11 SU UMa AY Lyr AY ASASSN-14jv CCD ASASSN-14jv SU UMa WZ Sge 28 29 AY Lyr O-C 1 4 1.1............................. 4 1.2................................ 5 2 7 3 9 4

More information

Outline I. Introduction: II. Pr 2 Ir 2 O 7 Like-charge attraction III.

Outline I. Introduction: II. Pr 2 Ir 2 O 7 Like-charge attraction III. Masafumi Udagawa Dept. of Physics, Gakushuin University Mar. 8, 16 @ in Gakushuin University Reference M. U., L. D. C. Jaubert, C. Castelnovo and R. Moessner, arxiv:1603.02872 Outline I. Introduction:

More information

2 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

2 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 information

NJW4124 IC ( ) NJW4124 AC-DC 1cell/2cell IC / 1 NJW4124M / Bi-CMOS NJW4124M : DMP20 P-CHG 1 20 Q-CHG NFB 2 19 CS1 TX-SW 3 18 CS2 GND 4 17 VS PC 5 16 V

NJW4124 IC ( ) NJW4124 AC-DC 1cell/2cell IC / 1 NJW4124M / Bi-CMOS NJW4124M : DMP20 P-CHG 1 20 Q-CHG NFB 2 19 CS1 TX-SW 3 18 CS2 GND 4 17 VS PC 5 16 V IC ( ) AC-DC 1cell/2cell IC / 1 M / Bi-CMOS M : DMP20 P-CHG 1 20 Q-CHG NFB 2 19 CS1 TX-SW 3 18 CS2 GND 4 17 VS PC 5 16 VREF ADP 6 15 V + 7 14 TDET 8 13 TH C1 9 12 TL C2 10 11 CHG-SW M - 1 - (Ta=25 C) V

More information

JMP V4 による生存時間分析

JMP V4 による生存時間分析 V4 1 SAS 2000.11.18 4 ( ) (Survival Time) 1 (Event) Start of Study Start of Observation Died Died Died Lost End Time Censor Died Died Censor Died Time Start of Study End Start of Observation Censor

More information

calibT1.dvi

calibT1.dvi 1 2 flux( ) flux 2.1 flux Flux( flux ) Flux [erg/sec/cm 2 ] erg/sec/cm 2 /Å erg/sec/cm 2 /Hz 1 Flux -2.5 Vega Vega ( Vega +0.03 ) AB cgs F ν [erg/cm 2 /s/hz] m(ab) = 2.5 logf ν 48.6 V-band 2.2 Flux Suprime-Cam

More information

untitled

untitled 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

hν 688 358 979 309 308.123 Hz α α α α α α No.37 に示す Ti Sa レーザーで実現 術移転も成功し 図 9 に示すよ うに 2 時間は連続測定が可能な システムを実現した Advanced S o l i d S t a t e L a s e r s 2016, JTu2A.26 1-3. 今後は光周波 数比計測装置としてさらに改良 を加えていくとともに

More information

無印良品 2012 自転車 カタログ

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 information

(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.

(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. CTA - 2f - 2015 ( 27 ) 14NM160L (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 198 56 m 58.4

More information

™…{,

™…{, 16:30-17:40 1-36 1-37 1-38 1-39 1-40 1-41 1-42 33 10:00-11:10 1-43 1-44 1-45 1-46 1-47 1-48 1-49 12:00-12:50 LS4 34 16:30-17:40 1-50 1-51 1-52 1-53 1-54 1-55 1-56 35 16:30-17:40 1-57 1-58 1-59 1-60 1-61

More information

PSG共通フォーマットv110

PSG共通フォーマットv110 PSG PSG (Vers.1.00) Ver.1.10 (1) Code=125 20(EXT) (2) (3) Ver.1.00 3-1 (1) ASCII Little Endian(X86) Big Endian(UNIX ) (2) PSG (3) (4) (5) 4byte channel 2byte (6) PSG Ver.1.10 2001 5 1 page.2 3-2 32bytes

More information

CdTe γ 02cb059e :

CdTe γ 02cb059e : CdTe γ 02cb059e : 2006 5 2 i 1 1 1.1............................................ 1 1.2............................................. 2 1.3............................................. 2 2 3 2.1....................................

More information

BIT -2-

BIT -2- 2004.3.31 10 11 12-1- BIT -2- -3-256 258 932 524 585 -4- -5- A B A B AB A B A B C AB A B AB AB AB AB -6- -7- A B -8- -9- -10- mm -11- fax -12- -13- -14- -15- s58.10.1 1255 4.2 30.10-16- -17- -18- -19-6.12.10

More information

PowerPoint Presentation

PowerPoint Presentation Sgr A* の赤外線観測 西山正吾 ( 京都大学 ) NIR obserbvations of the Galactic center 2/46 NIR obserbvations of the Galactic center 3/46 NIR obserbvations of the Galactic center 4/46 Dereddened flux density [mjy] 40 20

More information

155 13 2 15 B97176 1 1.1. 4 1.2. 5 1.2.1. 1.2.2. 1.3. 7 2. 2.1. 9 2.2. 1 2.3. 13 2.4. 16 3. 3.1. 3.1.1. 18 3.1.2. 26 3.1.3. 33 3.2. 3.2.1. 34 3.2.2. 5 4. 4.1. 52 4.2. 53 54 55 2 1 1.1 1.2 1.3 3 4 Fig.

More information

ガイドライン(案) 実践資料編.doc

ガイドライン(案) 実践資料編.doc (1) 15 (2) (3) 1.... 1 1.1... 1 1.2... 1 2.... 3 2.1... 3 2.2... 3 2.2.1... 3 2.3... 5 2.4... 5 2.4.1... 5 2.4.2... 6 3.... 7 4....12 4.1... 12 4.2... 14 5....20 5.1... 20 5.1.2... 22 5.1.3... 23 5.2...

More information

CMOS GPS GPS HARP CCD CMOS CMOS CMOS CMOS CCD i

CMOS GPS GPS HARP CCD CMOS CMOS CMOS CMOS CCD i 23 CMOS A Study of Capturing Star by Conventional CMOS Camera with Small Lens 1120224 2012 3 1 CMOS GPS GPS HARP CCD CMOS CMOS CMOS CMOS CCD i Abstract A Study of Capturing Star by Conventional CMOS Camera

More information

12-7 12-7 12-7 12-7 12-8 12-10 12-10 12-10 12-11 12-12 12-12 12-14 12-15 12-17 12-18 10 12-19 12-20 12-20 12-21 12-22 12-22 12-23 12-25 12-26 12-26 12-29 12-30 12-30 12-31 12-33 12-34 12-3 12-35 12-36

More information

ISLE 2010/08/17

ISLE 2010/08/17 ISLE 2010/08/17 Talk plan 1. ISLE 2. 3. 4. 2011A 2010/8/17 OAOUM 2010 ISLE 2010/8/17 OAOUM 2010 ISLE OASIS HAWAII (HgCdTe 1024 1024) 4.2 4.2 arcmin 2, 0.25 arcsec/pix (13 Filters) 2006B FWHM = 0.75 arcsec

More information

56cm 1 15 1960 2 8 2 2 1 2008 1992 2 1992 2 3562mm 3773mm 2 1980 1991 2008 2007 2003 5 2 3 2003 2005 2008 2010 2005 2008 2012 2010 2012 4 7 4 5 2 1975 1994 8 2008 NPO 2 2010 3 2013 2016 3 2008 2009 14

More information

2

2 III 0713011005 2009 3 23 2 i (Gamma-Ray Burst : GRB) 10 msec 100 sec GRB 10 52 erg 10 48 erg GRB GRB GRB GRB 2007 Ikaros (Interplanetary Kite craft Accelerated by Radiation Of the Sun) (GAmma-ray burst

More information

Δ Δ Δ 250

Δ Δ Δ 250 高エネルギー粒子用 Si検出器 第 10 章 1 特性 1-1 1-2 1-3 有感エリア 暗電流 接合容量 応答速度 2 シンチレータ式Si検出器 3 ダイレクト式Si検出器 3-1 3-2 3-3 3-4 3-5 空乏層の厚さ チャネリング効果 出力波高のばらつき ノイズとエネルギー分解能 位置検出用Si検出器 章 4 新たな取り組み 10 高エネルギー粒子用 5 応用例 粒子衝突実験 FGST

More information

main.dvi

main.dvi WIDGET CCD 03PR029 2 15 ( ) WIDGET WIDGET CCD PC Swift Swift CCD Canon EF35mm 3 Canon EF50mm 4 WIDGET 64 64 0.94 arcmin Swift Swift Swift 1 4 1.1................................. 4 1.2.......................

More information

(2/12) AV OA

(2/12) AV OA June 2016 Mn-Zn UU (2/12) AV OA (3/12) RoHS UU PE22 UU 79 129 31 PE22 UU 79 115 31 PC40 0 129 30 PE90 0 150 20 1 151 25 120 160 20 80 30N 30N 25N C C 30 to +5 30 to +85 RoHS https://product.tdk.com/info/ja/environment/rohs/index.html

More information

Microsoft Word - 章末問題

Microsoft Word - 章末問題 1906 R n m 1 = =1 1 R R= 8h ICP s p s HeNeArXe 1 ns 1 1 1 1 1 17 NaCl 1.3 nm 10nm 3s CuAuAg NaCl CaF - - HeNeAr 1.7(b) 2 2 2d = a + a = 2a d = 2a 2 1 1 N = 8 + 6 = 4 8 2 4 4 2a 3 4 π N πr 3 3 4 ρ = = =

More information

1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 21 22 23 5 2 5 24 () () () () () 1 1 150 50 50 1 1 ( 15,000 ) 150 ( 15,000 ) 100 50 50 1 1 ( 6,000 ) 150 ( 6,000 ) 100 50 50 1 1 150 1 1 150 100 0.25

More information

2

2 Rb Rb Rb :10256010 2 3 1 5 1.1....................................... 5 1.2............................................. 5 1.3........................................ 6 2 7 2.1.........................................

More information

untitled

untitled I RITE A B C D E F A B C LSI D LSI E/ F / G H I J K/ L / M A B 1 Intelligent Thermal Technology 2 17 18 19 LSI / LSI / / / 3 A IT 105-130 180 IT 4 off 5 6 B IT A RECO-View 630BF 100 7 100 100 RD919 A 8

More information

JA2008

JA2008 A1 1 10 vs 3 2 1 3 2 0 3 2 10 2 0 0 2 1 0 3 A2 3 11 vs 0 4 4 0 0 0 0 0 3 6 0 1 4 x 11 A3 5 4 vs 5 6 5 1 0 0 3 0 4 6 0 0 1 0 4 5 A4 7 11 vs 2 8 8 2 0 0 0 0 2 7 2 7 0 2 x 11 A5 9 5 vs 3 10 9 4 0 1 0 0 5

More information

NJW4108 IC ( ) NJW4108 1cell/2cell IC NJW4108V / Bi-CMOS NJW4108V : SSOP20 P-CHG 1 20 Q-CHG NFB 2 19 CS1 CNT 3 18 CS2 GND 4 17 VS NC 5 16 VREF F-CHG 6

NJW4108 IC ( ) NJW4108 1cell/2cell IC NJW4108V / Bi-CMOS NJW4108V : SSOP20 P-CHG 1 20 Q-CHG NFB 2 19 CS1 CNT 3 18 CS2 GND 4 17 VS NC 5 16 VREF F-CHG 6 IC ( ) 1cell/2cell IC V / Bi-CMOS V : SSOP20 P-CHG 1 20 Q-CHG NFB 2 19 CS1 CNT 3 18 CS2 GND 4 17 VS NC 5 16 VREF F-CHG 6 15 V + 7 14 TDET 8 13 TH C1 9 12 TL C2 10 11 V - 1 - (Ta=25 C) V + +15 V C1 V C1

More information

LTC 自己給電絶縁型コンパレータ

LTC 自己給電絶縁型コンパレータ AC 120V TECCOR 4008L4 OR EUIVALENT NEUTRAL 2N2222 HEATER 25Ω 150Ω 1k 1N4004 2.5k 5W 5.6V R1 680k 390Ω 100µF LE 47k C1 0.01µF ZC ZC COMPARISON > R = R O e B (1/T 1/T O ) B = 3807 1µF THERM 30k YSI 44008

More information

温度計技術資料1.PDF

温度計技術資料1.PDF 2 TM01010 TM02010 TM03010 TM04010 TM05010 TM05020 TM05030 TM05040 TM05050 TM05060 TM05070 TM05080 TM05090 TM05100 TM05210 TM05220 TM05230 TM05240 TM05250 TM05260 TM05270 TM05280 TM05290 TM05300 TM05310

More information

PE-CVD X PTO Sawyer-tower 3.1 PTO Sawyer-tower Sawyer-tower a c 25

PE-CVD X PTO Sawyer-tower 3.1 PTO Sawyer-tower Sawyer-tower a c 25 PbTiO3(PTO) 14 2 5 1.1 1 1.2 2 2.1 PE-CVD 3 2.2 X 7 2.3 9 2.4 10 2.5 12 2.6 13 PTO Sawyer-tower 3.1 PTO 14 3.2 Sawyer-tower 16 3.2.1 3.2.2 Sawyer-tower 3.3 20 4.1 a c 25 4.2 26 4.3 27 4.4 27 5.1 34 1.1

More information

2

2 2007 8 12 1 Q&A Q1 A 2007 6 29 2008 1 1 14 1 12 1 2 3 1 1 13 1 2 15 1 1 2 Q2 A 627 1 20 1 1 3 15 2003 18 2 3 4 5 3 406 44 2 1997 7 16 5 1 1 15 4 52 1 31 268 17 5 60 55 50 1999 3 9 1999 3 39 40 44 100 1

More information

AD8212: 高電圧の電流シャント・モニタ

AD8212: 高電圧の電流シャント・モニタ 7 V typ 7 0 V MSOP : 40 V+ V SENSE DC/DC BIAS CIRCUIT CURRENT COMPENSATION I OUT COM BIAS ALPHA 094-00 V PNP 0 7 V typ PNP PNP REV. A REVISION 007 Analog Devices, Inc. All rights reserved. 0-9 -- 0 40

More information

Fermi ( )

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

kubostat2017e p.1 I 2017 (e) GLM logistic regression : : :02 1 N y count data or

kubostat2017e p.1 I 2017 (e) GLM logistic regression : : :02 1 N y count data or kubostat207e p. I 207 (e) GLM kubo@ees.hokudai.ac.jp https://goo.gl/z9ycjy 207 4 207 6:02 N y 2 binomial distribution logit link function 3 4! offset kubostat207e (https://goo.gl/z9ycjy) 207 (e) 207 4

More information

3-2 PET ( : CYRIC ) ( 0 ) (3-1 ) PET PET [min] 11 C 13 N 15 O 18 F 68 Ga [MeV] [mm] [MeV]

3-2 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 information

ホームページ原稿H22年会プログラム(座長あり)_清修正

ホームページ原稿H22年会プログラム(座長あり)_清修正 49 22 9 15 17 3-1-1 9 16 4-5 9 17 4 9 17 1 3 5 7 2 4 6 8 (9 15-17 ) 1) 10 5 2) PC PC Windows PCWindows XPPower Point 2003 USB 3) 30 15 PC USB 4) PC USB 5) USB 9 16 10:0011309 15 1400 9 17 1000 ) 90cm 160cm

More information

) km 200 m ) ) ) ) ) ) ) kg kg ) 017 x y x 2 y 5x 5 y )

) km 200 m ) ) ) ) ) ) ) kg kg ) 017 x y x 2 y 5x 5 y ) 001 ) g 20 g 5 300 g 7 002 720 g 2 ) g 003 0.8 m 2 ) cm 2 004 12 15 1 3 1 ) 005 5 0.8 0.4 ) 6 006 5 2 3 66 ) 007 1 700 12 ) 008 0.315 ) 009 500 g ) kg 0.2 t 189 kg 17.1 kg 010 5 1 2 cm 3 cm )km 2-1 - 011

More information

23 1 Section ( ) ( ) ( 46 ) , 238( 235,238 U) 232( 232 Th) 40( 40 K, % ) (Rn) (Ra). 7( 7 Be) 14( 14 C) 22( 22 Na) (1 ) (2 ) 1 µ 2 4

23 1 Section ( ) ( ) ( 46 ) , 238( 235,238 U) 232( 232 Th) 40( 40 K, % ) (Rn) (Ra). 7( 7 Be) 14( 14 C) 22( 22 Na) (1 ) (2 ) 1 µ 2 4 23 1 Section 1.1 1 ( ) ( ) ( 46 ) 2 3 235, 238( 235,238 U) 232( 232 Th) 40( 40 K, 0.0118% ) (Rn) (Ra). 7( 7 Be) 14( 14 C) 22( 22 Na) (1 ) (2 ) 1 µ 2 4 2 ( )2 4( 4 He) 12 3 16 12 56( 56 Fe) 4 56( 56 Ni)

More information

kubostat2015e p.2 how to specify Poisson regression model, a GLM GLM how to specify model, a GLM GLM logistic probability distribution Poisson distrib

kubostat2015e p.2 how to specify Poisson regression model, a GLM GLM how to specify model, a GLM GLM logistic probability distribution Poisson distrib kubostat2015e p.1 I 2015 (e) GLM kubo@ees.hokudai.ac.jp http://goo.gl/76c4i 2015 07 22 2015 07 21 16:26 kubostat2015e (http://goo.gl/76c4i) 2015 (e) 2015 07 22 1 / 42 1 N k 2 binomial distribution logit

More information

株主通信:第18期 中間

株主通信:第18期 中間 19 01 02 03 04 290,826 342,459 1,250,678 276,387 601,695 2,128,760 31,096 114,946 193,064 45,455 18,478 10,590 199,810 22,785 2,494 3,400,763 284,979 319,372 1,197,774 422,502 513,081 2,133,357 25,023

More information

untitled

untitled 1 2 3 4 5 6 7 Point 60,000 50,000 40,000 30,000 20,000 10,000 0 29,979 41,972 31,726 45,468 35,837 37,251 24,000 20,000 16,000 12,000 8,000 4,000 0 16,795 22,071 20,378 14 13 12 11 10 0 12.19 12.43 12.40

More information

株主通信 第16 期 報告書

株主通信 第16 期 報告書 10 15 01 02 1 2 3 03 04 4 05 06 5 153,476 232,822 6,962 19,799 133,362 276,221 344,360 440,112 412,477 846,445 164,935 422,265 1,433,645 26,694 336,206 935,497 352,675 451,321 1,739,493 30,593 48,894 153,612

More information