PowerPoint プレゼンテーション

Size: px
Start display at page:

Download "PowerPoint プレゼンテーション"

Transcription

1 HSC-SSP HSC DB

2 2 HSC 2012/8 FL 2014/3 SSP Suprime-Cam HSC : k4k CCDs : k4k CCDs : 185MB/shot 30GB/ 2GB/shot ( 300GB/ ) :

3 1. CCD 2. CCD CCD

4 4 K -IPMU LSST stack (Python, C++) (c.f., IRAF) Python, C++ (SWIG) HSC Add-on MPI, Torque (OpenPBS)

5 HSC-SSP 5

6 6 HSC-SSP Wide (1400 sq.deg) Equator g,r,i,z,y (10-20min) Deep (27 sq.deg) 4 Fields (x 4-5 FOVs) g,r,i,z,y ( hrs) NB387,816,921 ( hrs) UltraDeep (3.5 sq.deg) 2 Fields (x 1FOV) g,r,i,z,y (7-19hrs) NB816,921,1010 ( hrs) Fiducial Pointing Dither Wide Layer Deep/UD Layer

7 7 Tract Coadd 1.7 Tract TAN-WCS Patch Coadd Coadd 4200x4200px, 100px Tract 1 Tract = 9 x 9 Patches 1 Tract 1.7deg Tract Dec=-90 to 90 deg Wide-XMM i RA=0-360deg

8 8 HSC Jargon ccd: CCD STARS FRAME DET -ID visit: 1 HSCA HSCA (112 Frames) visit= mosaic,warp, coadd mosaic: CCD fluxscale warp: coadd: registration

9 9 Procedure CCD CR PSF PS1 PV1.2 (TAN-SIP WCS) PS1 PV1.2 Coadd Coadd (FITS) w/ CORR, WCS+magzero CALEXP SRC, CCD CALSRC per visit Coadd TAN-SIP WCS CCD 2 1 warp Coadd calexp src Coadd (Visit, CCD) (Visit, Patch) (Filter, Patch) (Filter, Patch)

10 Forced Coadd Forced mode g r i z y (ref) y N = band i= 1 2 g i g i = Image sky : χ2 10

11 11 Procedure Coadd forced Coadd Forced _src (Filter, Patch) CCD Forced FORCED CCD Forced SRC (Shot, CCD) Forced HSC-G Coadd Image HSC-R Coadd Image Sky-reSubtracted HSC-I Sky-reSubtracted Coadd HSC-Z HSC-Y Forced HSC-G Corrected Image w/ Corrected WCS+magzero Image HSC-R CCD w/ w/ WCS+magzero HSC-I WCS+magzero HSC-Z HSC-Y

12 12 Coadd ref forced_src mergedet mulitband.py Multi-node 4-8GB >>20GB Coadd Det HSC-G (patch ) HSC-R HSC-I HSC-Z HSC-Y NB0921 meas measmatch ellipse Forced Multi stack.py CORR Coadd calexp HSC-G (patch ) HSC-R HSC-I HSC-Z HSC-Y NB0921

13 13 STARS SSP ID /

14 14 CCD Coadd PSF HDU0: HDU1: HDU2: HDU3: 16bit integer Plane 0 -> BAD Plane 1 -> SAT Plane 2 -> INTRP Plane 3 -> CR Plane 4 -> EDGE Plane 5 -> DETECTED Plane 6 -> DETECTED_NEGATIVE Plane 7 -> CROSSTALK ADU count / Gain

15 15 Crosstalk Saturate CR Detected

16 16 ID Flux Flags

17 17 ID id -- Tract Patch unique ID tract, patch, filter01 ra2000, dec2000 ( ref centroid_{record, sdss}) centroid_sdss_{x, y}, err 3x3 pix shape_sdss_centroid_{x, y}, err

18 18 shape_sdss[] SDSS adaptive moment 2 nd moment shape_hsm_moments[] 2 nd moment by HSM algorithms Kron kron_radius sqrt(a*b) Galaxy Component-Model Fit (CModel) cmodel_{dev, exp}_ellipse[], cmodel_fracdev ¼ exp law 2

19 19 flux_sinc, flux_naive r=12px (~φ2 ) aperture flux_aperture{01,..,09} φ1, 1.5, 2, 3, 4, 5.7, 8.4,..., 23.6 {g,r,i,z,y,nb0921,nb0816}flux_aperture{01,..,09} cgs {g,r,i,z,y,nb0921,nb0816}mag_aperture{01,..,09} PSF flux_psf CModel cmodel_flux, cmodel_{dev, exp}_flux Kron flux_kron

20 20 : detect_is_primary detect_is_tract_inner detect_is_patch_inner Tract Patch Tract Patch (measlist, forcelist) Parent deblend_nchild

21 21 Patch-Inner, Tract-Inner, Primary Tract Patch Tract 1 Patch 100px Primary Tract Patch Inner Primary Patch-Inner: 4100 x 4100 px Patch-Outer:

22 22 : flags_pixel_bad (*) defect flags_edge Coadd Coadd flags_offimage FITS flags_cr_{center, any} (*) Cosmic Ray flags_interpolated_{center, any} (**) Interpolate flags_pixel_saturated_{center, any} (**) Overflow flags_suspect_{center, any} (**) 50000ADU flags_bright_object_{center, any} (**) NOMAD (*) coadd (**) center optional

23 23 True centroid_sdss_flags shape_sdss_centroid_flags shape_sdss_flags flux_kron_flags flux_psf_flags cmodel_flux_flags

24 24 PSF classification_extendedness PSF Cmodel(*fac) =0 a_{g,r,i,z,y,nb0921,nb0816} # mag

25 25 multiband merge_peak_{g,r,i,z,y,..} footprint merge_footprint_{g,r,i,z,y,..} forced merge_measurement_{g,r,i,z,y, } S15B i r z y g n921 n816

PowerPoint プレゼンテーション

PowerPoint プレゼンテーション 1 HSC 戦略枠観測 (SSP) データリリースの概要 古澤久徳 ( 国立天文台 ) 2016.6.2 銀河進化研究会 @ 東北大 2 HSC 戦略枠観測 (SSP) すばる主焦点広視野カメラ Hyper Suprime-Cam (HSC) 2012/8FL, 2014/3 共同利用 SSP 開始 宇宙論 (WL) を中心とする戦略的観測 銀河天文学 Transient 現象 太陽系天体などもスコープ

More information

arXiv: v2 [astro-ph.IM] 28 Jul 2017

arXiv: v2  [astro-ph.IM]  28 Jul 2017 Publ. Astron. Soc. Japan (2014) 00(0), 1 28 doi: 10.1093/pasj/xxx000 1 First Data Release of the Hyper Suprime-Cam Subaru Strategic Program arxiv:1702.08449v2 [astro-ph.im] 28 Jul 2017 Hiroaki Aihara 1,

More information

Summary of WISH Filter Set and Sensitivity: Filters suitable for various scientific case Filters cover wavelength range of 1-5µm without any gaps Narr

Summary of WISH Filter Set and Sensitivity: Filters suitable for various scientific case Filters cover wavelength range of 1-5µm without any gaps Narr Summary of WISH Survey Plan Kiyoto Yabe (NAOJ) Summary of WISH Filter Set and Sensitivity: Filters suitable for various scientific case Filters cover wavelength range of 1-5µm without any gaps Narrower

More information

1 239 1 1 1 1 1 50 50 2 2 2 1 J1 G 2 20 50 J L AF 2 Y B 2 1 0 20 25 50 3 20 2 50 1 20 50 2 1 1 5 111 115 5 11 11 1 1 5 5 5 1 5 1 5 211 215 2 2 3 3 2 1 5 50 0 50 5 115 2 2 00 5 2 2 252 0 0 1 1 150 13 0

More information

Ando_JournalClub_160708

Ando_JournalClub_160708 Independent discoveries of a tidally disrupting dwarf galaxy around NGC 253! A Tidally Disrupting Dwarf Galaxy in the Halo of NGC 253 Toloba, E. et al. 2016, ApJL, 816, L5 (hereafter T16, accepted 2015.12.07)

More information

スライド 1

スライド 1 カタログデータベース検索 峯尾聡吾 1 目次 データベースと SQL データベース検索のための汎用の知識 HSC-SSP データベースについて 2 データベースと SQL 多くの テーブル を検索できるようにしたもの = データベース 検索するための言語 = SQL ( テーブルの一例 ) id ra dec mag mag_err failure 1000 150.0 2.0 25.0 1.0 true

More information

subaruUM2010_murayama

subaruUM2010_murayama SuMIRe/PFS 村山斉 (IPMU & Berkeley) Subaru Users Meeting @ 国立天文台 2011.1.19 PFS HSC 5 PFS (FIRST) HSC PFS weak lensing BAO dark energy PFS cf. white paper UM UM PFS exciting SAC HSC UM Eric Prieto (Marseille)

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

Taro13-第6章(まとめ).PDF

Taro13-第6章(まとめ).PDF % % % % % % % % 31 NO 1 52,422 10,431 19.9 10,431 19.9 1,380 2.6 1,039 2.0 33,859 64.6 5,713 10.9 2 8,292 1,591 19.2 1,591 19.2 1,827 22.0 1,782 21.5 1,431 17.3 1,661 20.0 3 1,948 1,541 79.1 1,541 79.1

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

Specview Specview Specview STSCI(Space Telescope SCience Institute) VO Specview Web page htt

Specview Specview Specview STSCI(Space Telescope SCience Institute) VO Specview Web page   htt Specview Specview Specview STSCI(Space Telescope SCience Institute) VO Specview Web page http://www.stsci.edu/resources/software_hardware/specview http://specview.stsci.edu/javahelp/main.html Specview

More information

<93C18F578B4C8E965F896988E420976D91BC2E6D6364>

<93C18F578B4C8E965F896988E420976D91BC2E6D6364> ɡ ɡ ɡ ɡ ɡ ɡ ɡ ɡ ɡ ɡ ɡ ɡ ɡ ɡ ɡ ɡ (a) Model image + field of view (b) Mosaic image (c) Mosaic + Single-dish image ɡ ɡɡ ɡ ɡɡ ɡ ɡ ɡ ɡ ɡ ɡ ɡ ɡ ɡ ɡ ɡ ɡ ɡ ɡ ɡ ɡ ɡ ɡ ɡɡ ɡ ɡ ɡ ɡ ɡ ɡɡ ɡ ɡ ɡ ɡ ɡ ɡ ɡ ɡ ɡ ɡ ɡ ɡ ɡɡ

More information

No

No No. 1 2 No. 3 4 5 6 7 8 9 10 11 12 No. 13 14 15 16 17 18 19 20 21 22 23 24 25 26 No. 27 28 29 30 31 32 33 34 35 36 37 38 39 40 41 42 43 No. 44 45 46 47 48 49 50 51 52 No. 53 54 55 56 57 58 59 60 61 62

More information

Microsoft PowerPoint - 201409_秀英体の取組み素材(予稿集).ppt

Microsoft PowerPoint - 201409_秀英体の取組み素材(予稿集).ppt 1 2 3 4 5 6 7 8 9 10 11 No Image No Image 12 13 14 15 16 17 18 19 20 21 22 23 No Image No Image No Image No Image 24 No Image No Image No Image No Image 25 No Image No Image No Image No Image 26 27 28

More information

Microsoft Word - ランチョンプレゼンテーション詳細.doc

Microsoft Word - ランチョンプレゼンテーション詳細.doc PS1-1-1 PS1-1-2 PS1-1-3 PS1-1-4 PS1-1-5 PS1-1-6 PS1-1-7 PS1-1-8 PS1-1-9 1 25 12:4514:18 25 12:4513:15 B PS1-1-10 PS1-2-1 PS1-2-2 PS1-2-3 PS1-2-4 PS1-2-5 PS1-2-6 25 13:1513:36 B PS1-2-7 PS1-3-1 PS1-3-2

More information

23_33.indd

23_33.indd 23 2TB 1TB 6TB 3TB 2TB 3TB 3TB 2TB 2TB 1TB 1TB 500GB 4TB 1TB 1TB 500GB 2TB 2TB 1TB 1TB RT RT RT RT RT RT RT MAC 10. 10. 10.6 10.5 MAC 10. 10. 10.6 10.5 MAC 10. 10.6 10.5 MAC 10. 10. 10.6 10.5 MAC 10. 10.6

More information

0.2 Button TextBox: menu tab 2

0.2 Button TextBox: menu tab 2 Specview VO 2012 2012/9/27 Specview Specview STSCI(Space Telescope SCience Institute) VO Specview Web page http://www.stsci.edu/resources/software hardware/specview http://specview.stsci.edu/javahelp/main.html

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

(1)2004年度 日本地理

(1)2004年度 日本地理 1 2 3 4 1 2 3 4 5 6 7 8 9 10 11 12-5.0-5.1-1.4 4.2 8.6 12.4 16.9 19.5 16.6 10.8 3.3-2.0 6.6 16.6 16.6 18.6 21.3 23.8 26.6 28.5 28.2 27.2 24.9 21.7 18.4 22.7 5 1 2 3 4 5 6 7 8 9 10 11 12 2.2 3.5 7.7 11.1

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

nakayama15icm01_l7filter.pptx

nakayama15icm01_l7filter.pptx Layer-7 SDN SDN NFV 50 % 3 MVNO 1 2 ICM @ 2015/01/16 2 1 1 2 2 1 2 2 ICM @ 2015/01/16 3 2 Service Dependent Management (SDM) SDM Simple Management of Access-Restriction Translator Gateway (SMART-GW) ICM

More information

- 1 - - 0.5%5 10 10 5 10 1 5 1

- 1 - - 0.5%5 10 10 5 10 1 5 1 - - - 1 - - 0.5%5 10 10 5 10 1 5 1 - 2 - - - - A B A A A B A B B A - 3 - - 100 100 100 - A) ( ) B) A) A B A B 110 A B 13 - 4 - A) 36 - - - 5 - - 1 - 6-1 - 7 - - 8 - Q.15 0% 10% 20% 30% 40% 50% 60% 70%

More information

ZEMAX Nagata DLL Volume-CAD c Copyright by RIKEN All Rights Reserved : : ( )

ZEMAX Nagata DLL Volume-CAD c Copyright by RIKEN All Rights Reserved : : ( ) ZEMAX Nagata DLL Volume-CAD c Copyright by RIKEN All Rights Reserved : 23 1 26 : ( ) ii 1. Nagata DLL 1 2. Nagata 1 3. VObj 2 3. 1............................................... 2 3. 2.................................................

More information

B-104

B-104 B-103 B-104 B-105 Fw FW Fw D C rs min E Cr Cor Cr Cor 5 +0.018 +0.010 10 8 0.15 8 2 640 2 190 269 224 27 000 40 000 RNAO- 5108T2 6 +0.018 +0.010 13 8 0.3 9 2 660 2 280 272 233 25 000 37 000 RNAO- 6138T2

More information

スライド 1

スライド 1 2004/12/25 HOP JTPF JASMINE ILOM JAXA) SPICA JELT Yerkes 1m (1897) Palomar 5m (1948) Subaru 8m (1999) 6.5m Large Binocular Telescope(LBT) 8.4m Mt.Graham 18 3m-6m 6.5m 3m Hubble Space Telescope 2.4m (0.115

More information

New version (2.15.1) of Specview is now available Dismiss Windows Specview.bat set spv= Specview set jhome= JAVA (C:\Program Files\Java\jre<version>\

New version (2.15.1) of Specview is now available Dismiss Windows Specview.bat set spv= Specview set jhome= JAVA (C:\Program Files\Java\jre<version>\ Specview VO 2012 2012/3/26 Specview Specview STSCI(Space Telescope SCience Institute) VO Specview Web page http://www.stsci.edu/resources/software hardware/specview http://specview.stsci.edu/javahelp/main.html

More information

http://www.ike-dyn.ritsumei.ac.jp/ hyoo/wave.html 1 1, 5 3 1.1 1..................................... 3 1.2 5.1................................... 4 1.3.......................... 5 1.4 5.2, 5.3....................

More information

LAE で探る z~5 での AGN 環境と 周辺銀河へのフィードバック Based on Kikuta et al. in prep. 初代星 初代銀河研究会, Oct 25th Satoshi KIKUTA (SOKENDAI/NAOJ, M2) Collaborators: Masatoshi

LAE で探る z~5 での AGN 環境と 周辺銀河へのフィードバック Based on Kikuta et al. in prep. 初代星 初代銀河研究会, Oct 25th Satoshi KIKUTA (SOKENDAI/NAOJ, M2) Collaborators: Masatoshi LAE で探る z~5 での AGN 環境と 周辺銀河へのフィードバック Based on Kikuta et al. in prep., Oct 25th Satoshi KIKUTA (SOKENDAI/NAOJ, M2) Collaborators: Masatoshi Imanishi, Kazuhiro Shimasaku, Fumiaki Nakata, Yoshiki Matsuoka

More information

A, B, C. (1) A = A. (2) A = B B = A. (3) A = B, B = C A = C. A = B. (3)., f : A B g : B C. g f : A C, A = C. 7.1, A, B,. A = B, A, A A., A, A

A, B, C. (1) A = A. (2) A = B B = A. (3) A = B, B = C A = C. A = B. (3)., f : A B g : B C. g f : A C, A = C. 7.1, A, B,. A = B, A, A A., A, A 91 7,.,, ( ).,,.,.,. 7.1 A B, A B, A = B. 1), 1,.,. 7.1 A, B, 3. (i) A B. (ii) f : A B. (iii) A B. (i) (ii)., 6.9, (ii) (iii).,,,. 1), Ā = B.. A, Ā, Ā,. 92 7 7.2 A, B, C. (1) A = A. (2) A = B B = A. (3)

More information

untitled

untitled 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 information

03J_sources.key

03J_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 information

J.qxd

J.qxd IQ 2 I/Q IQ IQ IQ IQ 3 IQ 4 5 6 I Q 7 IQ 0 deg 8 IQ I QI I Q Q Q Q { I Q { I I 9 I/QI/QI/Q IQ IQ I/Q Q Σ I IQ I Q 10 I/Q I/Q I/Q IQ IQ 11 π 12 01 00 11 10 13 I/Q I QI I/Q IQ 14 π QI π I/QI Q IQ IQ π 15

More information

広島大学かなた望遠鏡 キャンペーン観測報告

広島大学かなた望遠鏡 キャンペーン観測報告 広島大かなた望遠鏡用 観測装置の現状と今後 広島大学 宇宙科学センター 秋田谷洋 1 Contents 1. 東広島天文台とかなた望遠鏡 東広島天文台 かなた望遠鏡 運用体制 2. 観測装置 HOWPol ( 定常運用中 ) 高速カメラ HONIR ( 開発 試験中 ) 3. まとめ 2 1. 東広島天文台と かなた望遠鏡 3 東広島天文台 東広島市西条地区郊外 ( 大学から車で ~15 分 ) 東経

More information

1 2 2 4 4 6 8 20 51 60 61 64 65 65 67 69 69 70 72 12 104,007 13.9 40.7 34.6 2030 16 1 21 1 16 1 1 1979 1979 25 30 12 25 2 60 2 2 3 16 1 1 1/2500 1979 16 9 4 5 16 11 16 12 6 7 3,214 146,390 977 30.4% 39,658

More information

空気の屈折率変調を光学的に検出する超指向性マイクロホン

空気の屈折率変調を光学的に検出する超指向性マイクロホン 23 2 1M36268 2 2 4 5 6 7 8 13 15 2 21 2 23 2 2 3 32 34 38 38 54 57 62 63 1-1 ( 1) ( 2) 1-1 a ( sinθ ) 2J D ( θ ) = 1 (1-1) kaka sinθ ( 3) 1-2 1 Back face hole Amplifier Diaphragm Equiphase wave surface

More information

version 1.0 November 2010 PyRAF Y. Nakajima Computer and Data Management Division Subaru Telescope NAOJ

version 1.0 November 2010 PyRAF Y. Nakajima Computer and Data Management Division Subaru Telescope NAOJ version 1.0 November 2010 PyRAF Y. Nakajima Computer and Data Management Division Subaru Telescope NAOJ Chapter 1 PyRAF 1.1 PyRAF PyRAF IRAF Python STScI 1998 (1) IRAF-CL (2) CL-? (3) IRAF Python wrapper

More information

ADC082S021 2 Channel, 50 ksps to 200 ksps, 8-Bit A/D Converter (jp)

ADC082S021 2 Channel, 50 ksps to 200 ksps, 8-Bit A/D Converter (jp) 2 Channel, 50 ksps to 200 ksps, 8-Bit A/D Converter Literature Number: JAJSAA2 2 200KSPS 8 A/D 2 8 CMOS A/D 50kSPS 200kSPS / IN1 IN2 1 2 SPI QSPI MICROWIRE DSP 2.7V 5.25V 3V 1.6mW 5V 5.8mW 3V 0.12 W 5V

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 - - 24 - - 25 - - 26 - - 27 - - 28 - - 29 - - 30 -

More information

MW鹿児島

MW鹿児島 NGC1068 Dark Matter Halo baryon gas stars SMBH SMBH 1 SMBHs? (AGN) AGN Seyfertization Taniguchi 1987, ApJ, 317, L57 AGN The dead quasar problem (Rees 1990, Science, 247, 817) T AGN ~ 10 8 yrs AGN AGN

More information

icml10yomikai.key

icml10yomikai.key A Fast Augmented Lagrangian Algorithm for Learning Low- Rank Matrices Ryota Tomioka, Taiji Suzuki, Masashi Sugiyama, Hisashi Kashima 2010/8/18 ICML2010 1 Matrix completion [Srebro et al. 05; Abernethy

More information

JA.qxd

JA.qxd Application Note 1432 J rmsj RJ pp J pp t, P σ J rms RJ t (t) 1 ϕ (t) S (t) = P(2π f d t + ϕ (t)) S P f d ϕ (t) J ϕ 1 1 J [s] = ϕ [rad] J [UI] = ϕ [rad] 2π f d 2π Φ(t) 2π f d t ϕ (t) 1 d 1 d ƒ (t) = Φ(t)

More information

B

B 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 information

B

B B07557 0 0 (AGN) AGN AGN X X AGN AGN Geant4 AGN X X X (AGN) AGN AGN X AGN. AGN AGN Seyfert Seyfert Seyfert AGN 94 Carl Seyfert Seyfert Seyfert z < 0. Seyfert I II I 000 km/s 00 km/s II AGN (BLR) (NLR)

More information

X u

X u X u1079037 14 4 1 X X X X X SNR X X ChandraX 0.3-10.0 kev 1 1 X 3 X 1 3 2 X 5 2.1 X... 5 2.1.1 Powerlaw... 5 2.1.2 BlackBody( )... 5 2.1.3 Disk-BlackBody... 6 2.1.4... 8 2.2 X... 9 2.2.1 HMXB:High-Mass

More information

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

X 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 information

meiji_resume_1.PDF

meiji_resume_1.PDF β β β (q 1,q,..., q n ; p 1, p,..., p n ) H(q 1,q,..., q n ; p 1, p,..., p n ) Hψ = εψ ε k = k +1/ ε k = k(k 1) (x, y, z; p x, p y, p z ) (r; p r ), (θ; p θ ), (ϕ; p ϕ ) ε k = 1/ k p i dq i E total = E

More information

NL-22/NL-32取扱説明書_操作編

NL-22/NL-32取扱説明書_操作編 MIC / Preamp ATT NL-32 A C ATT AMP 1 AMP 2 AMP 3 FLAT FLAT CAL.SIG. OVER LOAD DET. AMP 4 AMP 5 A/D D/A CONV. AMP 6 AMP 7 A/D CONV. Vref. AMP 8 AMP 10 DC OUT AMP 9 FILTER OUT AC DC OUT AC OUT KEY SW Start

More information

1) 1-1 1 1) 14 2) (1) 2.2 3) (1)(2) 2 3 1-2 1214 4) 4 2. 2.1 2-1 5 2-2 2-1 6 7 2.2 2-2 8 3. 3.1 3.2 1) 1 14 2003 9 3.2.1 3-1 (1) 2 2 2 ASTER DN 0255 DN 2 2 2 DN (2) 10 GSLR DN 3-1 3.2.2 DN (1) DN DN DN

More information

Jasmine

Jasmine Jasmine Jasmine Jasmine 1.... 3 1.1.... 3 1.2.... 5 1.3.... 6 1.4.... 8 1.5....11 1.6.... 13-2 - Jasmine 1. 1.1. - 3 - Jasmine - 4 - Jasmine 1.2. 1 20-5 - Jasmine 1.3. - 6 - Jasmine [ERR0001] [ERR0001]

More information

"Moir6 Patterns on Video Pictures Taken by Solid State Image Sensors" by Okio Yoshida and Akito Iwamoto (Toshiba Research and Development Center, Tosh

Moir6 Patterns on Video Pictures Taken by Solid State Image Sensors by Okio Yoshida and Akito Iwamoto (Toshiba Research and Development Center, Tosh "Moir6 Patterns on Video Pictures Taken by Solid State Image Sensors" by Okio Yoshida and Akito Iwamoto (Toshiba Research and Development Center, Toshiba Corporation, Kawasaki) Reproduced resolution chart

More information

2

2 2 3 4 5 6 7 0 10 20 30 40 50 60 70 9 10 11 12 13 14 15 86.0% 14.0% 79.5% 20.5% 60 111 16 .. 17 ** p

More information

Jasmine 1.... 3 1.1.... 3 1.2.... 5 1.3.... 7 1.4.... 9 1.5....11 1.6.... 13 1.7.... 14-2 -

Jasmine 1.... 3 1.1.... 3 1.2.... 5 1.3.... 7 1.4.... 9 1.5....11 1.6.... 13 1.7.... 14-2 - Jasmine Jasmine Jasmine 1.... 3 1.1.... 3 1.2.... 5 1.3.... 7 1.4.... 9 1.5....11 1.6.... 13 1.7.... 14-2 - Jasmine 1. 1.1. - 3 - Jasmine [ERR0001] [ERR0001] [ERR0001] [ERR0034] [ERR0032] [ERR0034] - 4

More information

untitled

untitled ( ) (mm) (GHz)=300( ) 30 300GHz=1 10mm ( 2GHz2Mbps) Gbps= Mbps ( m),? S G=P/Pi30dB=1000 Gm=4πS/λ 2, S= 80λ 2 Gm=30dB η=g/gm, S= 80λ 2,G=27dB η=50% (GHz) 80 70 60 50 40 30 20 10 16 19 22 25 28 31 34 37

More information

1 1 H Li Be Na M g B A l C S i N P O S F He N Cl A e K Ca S c T i V C Mn Fe Co Ni Cu Zn Ga Ge As Se B K Rb S Y Z Nb Mo Tc Ru Rh Pd Ag Cd In Sn Sb T e

1 1 H Li Be Na M g B A l C S i N P O S F He N Cl A e K Ca S c T i V C Mn Fe Co Ni Cu Zn Ga Ge As Se B K Rb S Y Z Nb Mo Tc Ru Rh Pd Ag Cd In Sn Sb T e No. 1 1 1 H Li Be Na M g B A l C S i N P O S F He N Cl A e K Ca S c T i V C Mn Fe Co Ni Cu Zn Ga Ge As Se B K Rb S Y Z Nb Mo Tc Ru Rh Pd Ag Cd In Sn Sb T e I X e Cs Ba F Ra Hf Ta W Re Os I Rf Db Sg Bh

More information

1. Introduction 2 1. Opacity / PWV The opacity in these bands can vary rapidly and markedly as a function of precipitable water vapour (PWV), particul

1. Introduction 2 1. Opacity / PWV The opacity in these bands can vary rapidly and markedly as a function of precipitable water vapour (PWV), particul SCUBA-2: on-sky calibration using submillimetre standard sources Dempsey et al. 2013, MN, 430, 2534 Reported by Y. Tamura (IoA, UTokyo) 2-Oct-2014 1 1. Introduction 2 1. Opacity / PWV The opacity in these

More information

ELECTRONIC 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 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 information

10:30 12:00 P.G. vs vs vs 2

10:30 12:00 P.G. vs vs vs 2 1 10:30 12:00 P.G. vs vs vs 2 LOGIT PROBIT TOBIT mean median mode CV 3 4 5 0.5 1000 6 45 7 P(A B) = P(A) + P(B) - P(A B) P(B A)=P(A B)/P(A) P(A B)=P(B A) P(A) P(A B) P(A) P(B A) P(B) P(A B) P(A) P(B) P(B

More information

- 2 -

- 2 - - 1 - - 2 - - 3 - - 4 - - 5 - - 6 - - 7 - - 8 - - 9 - A) B) C) D) E) F) - 10 - G) H) I) J) P - 11 - 001 1,416,0003/4 1,062,000 002 100,000 50,00023 1,150,000 2,100,000 200,000+ 100,0000.9 1,600,000 JA

More information

IIC Proposal of Range Extension Control System by Drive and Regeneration Distribution Based on Efficiency Characteristic of Motors for Electric

IIC Proposal of Range Extension Control System by Drive and Regeneration Distribution Based on Efficiency Characteristic of Motors for Electric IIC-1-19 Proposal of Range Extension Control System by Drive and Regeneration Distribution Based on Efficiency Characteristic of Motors for Electric Vehicle Toru Suzuki, Hiroshi Fujimoto (Yokohama National

More information

459

459 459 40 5 200606-1,940 7 - - - 480.2 3.6+0.8 40 4,00010 0.791 50 5 200608-2,740 5 - - - 600.2 4.1+0.8 51 4,00010 1.122 65 5 200610-3,500 5 - - - 760.3 4.1+0.8 67 4,00010 1.445 75 5 200611-5,360 3 - - -

More information

35

35 D: 0.BUN 7 8 4 B5 6 36 6....................................... 36 6.................................... 37 6.3................................... 38 6.3....................................... 38 6.4..........................................

More information

23_33.indd

23_33.indd 23 16 26 25 24 2 30 2 19 20 1 21 1 22 9 11 15 14 23 2 3 5 1 6 12 14 29 P.26 P.26 P.26 P.26 P.2 P.26 P.2 P.2 P.2 P.2 P.2 P.2 P.24 P.24 P.24 P.24 P.24 MAC 10. 10.6 10.5 1TB 2TB XP XP MAC 10. 10. 10.6 10.5

More information

http://aucfan.com 200913 - - TEL03-5423-7815 E-mail : ad@aucfan.com 150-0012 1-3-14 ASAX9F http://ad.aucfan.com/aucfan_mediasheet.pdf TOP 140 Yahoo! 20089 PV 4,500PV UU 140UU URL aucfan.com http://aucfan.com

More information

noted by Kazuma MATSUDA (force) (mechanics) (statics) (dynamics) O F OA O (point of application) (line of action) (vector) F F F

noted by Kazuma MATSUDA (force) (mechanics) (statics) (dynamics) O F OA O (point of application) (line of action) (vector) F F F noted by Kazuma MATSUDA 2016 5 29 1. (force) (mechancs) (statcs) (dynamcs) 1.1 1 1 O F OA O (pont of applcaton) (lne of acton) (vector) F F F F 1.2 ( ) 1 (kg-wt) (Internatonal System of Unt, SI) kg SI

More information

Microsoft Word - RMD_75.doc

Microsoft Word - RMD_75.doc Review Multi Dimensional Data Multi Dimensional Acquire *.nd MetaMorph.nd Muliti Dimensional Acquisition Stack Tiff Multi Dimensional Acquisition Z nd nd 1 Review Multi Dimensional Data nd Review Multi

More information

Contents 1. Ia cosmology 2. Ia / rate 3.

Contents 1. Ia cosmology 2. Ia / rate 3. WISH ( ) Contents 1. Ia cosmology 2. Ia / rate 3. supernova (CC SN) Ia (SN Ia) supernova classification supernova Ia (SN Ia) - : redshift z~1.5 - progenitor system: Single Degenerate? Double Degenerate?

More information

2017 (413812)

2017 (413812) 2017 (413812) Deep Learning ( NN) 2012 Google ASIC(Application Specific Integrated Circuit: IC) 10 ASIC Deep Learning TPU(Tensor Processing Unit) NN 12 20 30 Abstract Multi-layered neural network(nn) has

More information

研究室ガイダンス(H28)福山研.pdf

研究室ガイダンス(H28)福山研.pdf 1 2 3 4 5 4 He M. Roger et al., JLTP 112, 45 (1998) A.F. Andreev and I.M. Lifshitz, Sov. Phys. JETP 29, 1107 (1969) Born in 2004 (hcp 4 He) E. Kim and M.H.W. Chan, Nature 427, 225 (2004); Science 305,

More information

7. y fx, z gy z gfx dz dx dz dy dy dx. g f a g bf a b fa 7., chain ule Ω, D R n, R m a Ω, f : Ω R m, g : D R l, fω D, b fa, f a g b g f a g f a g bf a

7. y fx, z gy z gfx dz dx dz dy dy dx. g f a g bf a b fa 7., chain ule Ω, D R n, R m a Ω, f : Ω R m, g : D R l, fω D, b fa, f a g b g f a g f a g bf a 9 203 6 7 WWW http://www.math.meiji.ac.jp/~mk/lectue/tahensuu-203/ 2 8 8 7. 7 7. y fx, z gy z gfx dz dx dz dy dy dx. g f a g bf a b fa 7., chain ule Ω, D R n, R m a Ω, f : Ω R m, g : D R l, fω D, b fa,

More information

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

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 , (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 information

HIDES (T.B.D.) HIDES-F (T.B.D.)

HIDES (T.B.D.) HIDES-F (T.B.D.) HIDES-F 2017.8.8 version 0.9.9.1 1 2 2 3 2.1 HIDES (T.B.D.)................................. 3 2.2 HIDES-F (T.B.D.)................................ 3 2.3..................................... 3 2.3.1 GUI...................

More information

iZotope RXユーザーガイド

iZotope RXユーザーガイド 2 izotope RX Table of Contents................................. 4 izotope RX. 4 izotope RX Advanced. 5. 5 izotope RX................. 6. 6 /. 7. 7. 7. 7. 8. 8. 8. 9. 9. 10. 11. 11. 11. 11. 12. 13 izotope

More information

磁性物理学 - 遷移金属化合物磁性のスピンゆらぎ理論

磁性物理学 - 遷移金属化合物磁性のスピンゆらぎ理論 email: takahash@sci.u-hyogo.ac.jp May 14, 2009 Outline 1. 2. 3. 4. 5. 6. 2 / 262 Today s Lecture: Mode-mode Coupling Theory 100 / 262 Part I Effects of Non-linear Mode-Mode Coupling Effects of Non-linear

More information

untitled

untitled 50cm 2500mm 300mm 15 CCD 15 100 1 2 3 4 23 SORA Kwak SeungJo 1 1.1 1995 20 2015 6 18 1931 1 2 3 2 ˆ 300mm 2500mm ˆ 2 1.2 WASP 1: 15 2048 2048 CCD 200mm 70 13 WASP 8 1.3 50cm 1 1: CCD 2: 1.4 MOST MOST 15

More information

第 1 回ディープラーニング分散学習ハッカソン <ChainerMN 紹介 + スパコンでの実 法 > チューター福 圭祐 (PFN) 鈴 脩司 (PFN)

第 1 回ディープラーニング分散学習ハッカソン <ChainerMN 紹介 + スパコンでの実 法 > チューター福 圭祐 (PFN) 鈴 脩司 (PFN) 第 1 回ディープラーニング分散学習ハッカソン チューター福 圭祐 (PFN) 鈴 脩司 (PFN) https://chainer.org/ 2 Chainer: A Flexible Deep Learning Framework Define-and-Run Define-by-Run Define Define by Run Model

More information

MCS-8M

MCS-8M 4-296-435-02 (1) Volume I MCS-8M 2011 Sony Corporation m a b c I-2 ...I-6...I-7...I-8...I-8...I-9 1...I-10...I-11 1 2 3 4 5 1 2 3 4 5 2...I-17...I-19...I-21...I-23...I-26 3...I-28...I-31...I-35...I-36...I-37...I-39...I-40...I-41...I-42...I-42...I-46...I-47

More information

a b GE(General Erectrics) 9 4 irr (JAPLA 2009/12) Example1 120 P = C r + C 2 (1 + r) C t 1 (1 + r) t 1 + C t + F (1 + r) t 10

a b GE(General Erectrics) 9 4 irr (JAPLA 2009/12) Example1 120 P = C r + C 2 (1 + r) C t 1 (1 + r) t 1 + C t + F (1 + r) t 10 1 SHIMURA Masato 2010 9 27 1 1 2 CF 6 3 10 *1 irr irr irr(inner rate of return)function is able to written only few lines,and it is very powerful and useful for simulate unprofitable business model. 1

More information

BRC-X1000

BRC-X1000 C-455-100-02(1) BRC-X1000/H800 2016 Sony Corporation 2 3 4 5 6 4 D E 5 6 7 A B C F G 7 8 9 0 qa qs SYSTEM SELECT IN IR SELECT VISCA RS - 422 OUT OSD OFF CAMERA SETUP 1 qd 2 3 4 5 6 7 8 LAN 12V qf HDMI

More information

Microsoft Word - Meta70_Preferences.doc

Microsoft Word - Meta70_Preferences.doc Image Windows Preferences Edit, Preferences MetaMorph, MetaVue Image Windows Preferences Edit, Preferences Image Windows Preferences 1. Windows Image Placement: Acquire Overlay at Top Left Corner: 1 Acquire

More information