X 20, 1 1 HETE-2 Swift CCD GRB CCD CCD CCD
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- しらん あいきょう
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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
![7 GRB050709 ( )...................... 12 1.8 TAROT( 25cm) GRB050904 ( ) GRB(z=6.3)[14]................ 13 1.9 GRB050904 (I-band ) X (0.](/docs-images/45/20569480/images/page_5.jpg "5-10ev ) light curve prompt emission afterglow [14].......................... 13 1.10 ROTSE-III( 45cm) 19 VLT( 8m) 2.6 15.5......................... 14 1.")
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
![2.4 MEADE LX90-30 CCD SBIG ST-9XE PC CCD GRB CCD PC WIDGET [mm] [mm] 304.](/docs-images/40/20569480/images/22-0.png "8 3048 f/10 0.38 4.5 /sec 2.2: MEADE LX90-30 2.7: CCD ST-9XE 2.")
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
![4.1: 4.2: CCD CC- DOPS [ ] [ ] [ ] 9 8.96 9.37 81 84 11 10.62 11.03 90 97 12 11.](/docs-images/40/20569480/images/30-0.png "87 11.03 94 97 4.1: 35 90 100 90 90 35 100 32 CCD 22.24 11 10 4.1 11 90 4.1.2 CCD CCD 28")
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
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