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![Page 1: CANGAROO の現況 Status of CANGAROO project Masaki Mori ICRR, University of Tokyo 「 CANGAROO 望遠鏡によるガンマ線天文学の新展開」 Dec.11-12, 2003 京都大 学](https://reader036.fdocuments.net/reader036/viewer/2022062519/56649f065503460f94c1b29a/html5/thumbnails/1.jpg)
CANGAROOCANGAROO の現況の現況Status of CANGAROO Status of CANGAROO
projectprojectMasaki MoriMasaki Mori
ICRR, University of TokyoICRR, University of Tokyo
「 CANGAROO 望遠鏡によるガンマ線天文学の新展開」 Dec.11-12, 2003 京都大学Workshop “New developments in Gamma-ray Astronomy with the CANGAROO telescope”, Dec.11-12, Kyoto U.
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Brief history of Brief history of CANGAROOCANGAROO
1987: SN1987A explosion 1990: 3.8m telescope moved 1990: ICRR-Adelaide Physics agreement 1992: Start obs. of 3.8m tel. 1995: PSR 1706-44 result published 1998: SNR1006 result published 1999: 7m telescope completed 2000: Upgrade to 10m telescope 2001: U.Tokyo-U.Adelaide agreement 2002: Second and third 10m tel. 2003: Fourth 10m tel.
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JANZOSJANZOS experiment in New experiment in New ZealandZealand
Japan Australia New Zealand Observation of Supernova 1987A
Air shower detector array
+
3 Fixed 2m Cherenkov telescopes
1987-1989, Black Birch, South Island
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Why Woomera?Why Woomera?
New Zealand is wet New Zealand is wet and not many clear and not many clear nights…nights…
Woomera: Woomera: Outskirt of desertOutskirt of desert Former rocket launch Former rocket launch
site, prohibited area: site, prohibited area: existing infrastructure existing infrastructure and support centerand support center
BIGRAT telescope was BIGRAT telescope was operated by Adelaide operated by Adelaide groupgroup
ELDO rocket Launch site in ’60s
BIGRAT
(BIcentinnial Gamma RAy Telescope)
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3.8m3.8m telescope telescope (ex. Lunar-ranging (ex. Lunar-ranging
telescope)telescope)
Tadashi Kifune & John Patterson
224ch imaging camera at prime focus
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CANGAROO 7mCANGAROO 7m telescopetelescope Completed in March Completed in March
19991999 60 x 80cm CFRP-based 60 x 80cm CFRP-based
spherical mirror spherical mirror segments segments (first plastic-(first plastic-base mirror in the base mirror in the world!)world!)
Focal length 8mFocal length 8m Alt-azimuth mountAlt-azimuth mount 552ch552ch imaging cameraimaging camera Timing and time-over-Timing and time-over-
threshold measurementthreshold measurement(March 1999)
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CANGAROO 10mCANGAROO 10m telescopetelescope
Upgraded in March Upgraded in March 20002000
114 x 80cm CFRP-114 x 80cm CFRP-basedbased spherical spherical mirror segmentsmirror segments
552ch imaging 552ch imaging cameracamera
Charge measurement Charge measurement (ADC)(ADC) addedadded
” ”CANGAROO-III T1”CANGAROO-III T1” (March 2000)
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CANGAROO-III T1 target CANGAROO-III T1 target listlist
SNR/Pulsar CrabSNR/Pulsar Crab SNR RX J1713.7-3946SNR RX J1713.7-3946
(Nature2002)(Nature2002) AGN Mrk421AGN Mrk421 (ApJL2002)(ApJL2002) Starburst galaxy NGC253Starburst galaxy NGC253 (AAL02,AA03)(AAL02,AA03) SN1987ASN1987A (ApJL2003)(ApJL2003) Pulsar PSR 1706-44Pulsar PSR 1706-44 (PhD 2003)(PhD 2003) SNR SN1006SNR SN1006 (PhD 2002)(PhD 2002) PSR 1259-63/SS2833PSR 1259-63/SS2833 (( 投稿中投稿中 )) AGN PKS2155-304, PKS2005-489AGN PKS2155-304, PKS2005-489 SNR RX J0852-4622SNR RX J0852-4622 SNR RCW86SNR RCW86 Galactic Center/Sgr A*Galactic Center/Sgr A* Galactic jet object SS433Galactic jet object SS433 EGRET unID 3EG J1234-1318EGRET unID 3EG J1234-1318 Galaxy Small Magellanic CloudGalaxy Small Magellanic Cloud Vela pulsarVela pulsar
Signal Publish
Signal: detected, upper limit, under analysis
Publish: published, in preparation
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Crab nebulaCrab nebula
“Standard candle” is observed as it should be – Our telescope is working properly!
C. Itoh, Ph.D. thesis 2003
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SNR RX J1713.7-3946SNR RX J1713.7-3946 SNR detected by X-ray SNR detected by X-ray
satellitesatellite Non-thermal emissionNon-thermal emission
Energy spectrum
Enomoto et al. Nature 2002Significance map
Gamma-ray signal = (ON) – (OFF)
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SNR RX J1713.7-3946: SNR RX J1713.7-3946: emission from protons?emission from protons?
Hard to explain by emission from electrons (Brems, IC)
Emission from protons (0)?
Cosmic ray origin?
Enomoto et al. Nature 2002
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SNR RX J1713.7-3946: SNR RX J1713.7-3946: counter argumentscounter arguments
Reimer & Pohl, A&A 390 (2002) L43
Butt et al., Nature 418 (2002) 489
0.8
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Markarian 421Markarian 421 The first TeV blazar in The first TeV blazar in
the northern skythe northern sky z=0.031 (~130Mpc)z=0.031 (~130Mpc) Flare in 2001Flare in 2001 Large zenith angle Large zenith angle
observation from observation from Woomera: higher Woomera: higher energyenergy
Intergalactic Intergalactic absorption by IR:absorption by IR:No 10TeV photons?No 10TeV photons?
Optical imageOkumura et al. ApJL 2002
Gamma-ray signal = (ON) – (OFF)
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Mrk 421: hint for Mrk 421: hint for cosmology?cosmology?
Emission above 10 TeV detected
Fewer IR photons?
Okumura et al. ApJL 2002
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Starburst galaxy NGC253Starburst galaxy NGC253
Nearby spiral Nearby spiral galaxy (2.4Mpc)galaxy (2.4Mpc)
Starburst Starburst activityactivityfrequent SNefrequent SNe
Optical
image
Gamma-ray signal = (ON) – (OFF)
Itoh et al.
A&AL 2002
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CANGAROO-I sources CANGAROO-I sources revisitedrevisited
PSR 1706-44PSR 1706-44 SN1006 NE rimSN1006 NE rim
S. Hara, Ph.D. thesis 2002J. Kushida, Ph.D. thesis 2003
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SN1987ASN1987AEnomoto, Ksenofontov, Katagiri, Tsuchiya et al., ApJ, 591(2003)L25-28
Order improved ULs
In 2003-6, the shock front willCollides with these rings!Interesting to continue observations
CII-10h
CIII
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PSR1259-63/SS2883PSR1259-63/SS2883 48ms pulsar/Be star binary
Eccentricity 0.87, Torb=1236.72days
X-ray emission around periastron
Synchrotron emission from
nonthermal electrons
TeV inverse Compton emission?
Dec’00Mar’01
Upper limits from obs. By 10m telescope
Limits on a model
parameterKawachi et al., submitted
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Galactic CenterGalactic Center CANGAROO 10m resultCANGAROO 10m result
Gamma-ray signal(ON-OFF)
( 7.5σ )Sgr A* and Sgr A East
VLA radio continuum image (6cm)
Radio image (90cm)
CANGAROO-II
AlphaTsuchiya, Ph.D. thesis in prep.
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RX J0852.0-4622RX J0852.0-4622
ROSAT X-ray image
8o
Vela SNR
Maximum X-ray emission
2o
Gamma-ray signal(ON-OFF)
8.0
Katagiri, Ph.D. thesis in prep.
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CANGAROO sensitivityCANGAROO sensitivity
H. Kubo, 2003
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CANGAROO-IIICANGAROO-III projectproject An array of four 10m telescopesAn array of four 10m telescopes
T1
T4 (2003)
T3 (2002)
T2
(2002)T2 (2002)
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Second 10m telescopeSecond 10m telescope Completed in 2002, Completed in 2002,
operaring since Dec. operaring since Dec. 20022002
Refined FRP-based Refined FRP-based mirror segmentsmirror segments
427ch427ch imaging imaging cameracamera
Fast ADCs and TDCsFast ADCs and TDCs
“ “CANGAROO-III T2”CANGAROO-III T2”
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T2 imaging cameraT2 imaging camera
Light guide
R3479+Preamp
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T2 electronicsT2 electronics
All VME-basedAll VME-based 16bit q-ADC16bit q-ADC VME frontendVME frontend TDCTDC Pattern triggerPattern trigger Linux OSLinux OS
Kubo et al., ICRC2001
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Event samples of T2Event samples of T2
TDC ADC
Scaler Star
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T1 TDC
T2 TDC
T1 ADC
T2 ADC
Samples of stereo eventsSamples of stereo events
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Stereo reconstructionStereo reconstruction
T1
T2overlay
Gamma-ray direction
(This is just an illustrative example.)
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Present statusPresent status
T3 T2 T1 T4Dec. 2002 startedJul. 2003 started Since 2000 Jul. 2003
completed
427ch Imaging camera for T2, T3, T4
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Systematic survey of Systematic survey of SNRsSNRs
Crab nebula
(” Standard candle” )
Vela ( CANGAROO )
RX J1713.7-3946 ( CANGAROO )
Cas A ( HEGRA )
RCW86 ( CANGAROO under analysis )
RX J0852-46 ( CANGAROO under analysis )
Chandra
・ optical
Chandra
ASCA
Chandra
ROSAT
ROSAT
SN1006 ( CANGAROO )
ASCA
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Galactic plane surveyGalactic plane survey
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International International coordinationcoordination Continuous observation of time Continuous observation of time
variable objectsvariable objects(ex. Blazars)(ex. Blazars)
Multiwavelength campaignMultiwavelength campaign
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““Evolution” of the TeV Evolution” of the TeV gamma-ray skygamma-ray sky
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““Evolution” in number of Evolution” in number of objectsobjects
“Kifune plot” ©Rene Ong
2002
Log scale