SNAP CCD Development Progress Hakeem Oluseyi January 9, 2003.

Slides:



Advertisements
Similar presentations
Semiconductor detectors
Advertisements

Results of Acceptance Tests of Hyper Suprime-Cam CCDs Yukiko Kamata, Hidehiko Nakaya, Satoshi Miyazaki National Astronomical Observatory of Japan.
The Second Generation of IR detectors for WFC3 Massimo Robberto European Space Agency and Space Telescope Science Institute.
Parameters to choose the CCD The CCD test bench *Temperature range : -55 to +40°C. *Stabilization : < 0.05°C/hour. *5 temperature probes : CCD and electronics.
Armin Karcher, LBNL IEEE/NSS 2001 Proton Radiation Damage in P-Channel CCDs Fabricated on High-Resistivity Silicon. C. Bebek, D. Groom, S. Holland, A.
INTEGRATED CIRCUITS Dr. Esam Yosry Lec. #6.
Vicki Bourget & Vinson Gee April 23, 2014
CHARGE COUPLING TRUE CDS PIXEL PROCESSING True CDS CMOS pixel noise data 2.8 e- CMOS photon transfer.
Ceramic Focal Plane Components For SNAP B. C
Optical image tube with Medipix readout
SuperNova Acceleration Probe Research and Development Efforts
Silicon PIN Diodes: A Promising Technology for UV-Optical Space Astronomy 11 April 2003 Presentation at NHST Workshop Bernard J. Rauscher, Donald F. Figer,
Applied Sensor Technology. Outline Introduction Examples of Sensors Basic readout electronics Semiconductor detectors.
Semiconductor Technology Associates Siliconus Maximus SDW2005 Scientific Detector Workshop June 19 – 25, 2005 Taormina, Italy Richard A Bredthauer Semiconductor.
06/02/2008CCDs1 Charge Coupled Device M.Umar Javed M.Umar Javed.
Mid-IR photon counting array using HgCdTe APDs and the Medipix2 ROIC
Photon Counting Sensors for Future Missions
Barry E. Burke Title Slide.
Photo courtesy NOAO, taken with LBNL fully depleted CCD Optical Characterization of 1.7  m NIR Detectors for SNAP M. Brown (Michigan), J. Balleza (IDTL),
CLIC Collaboration Working Meeting: Work packages November 3, 2011 R&D on Detectors for CLIC Beam Monitoring at LBNL and UCSC/SCIPP Marco Battaglia.
1/23/ Proton Radiation Damage in High- Resistivity n-Type Silicon CCDs C. Bebek, D. Groom, S. Holland, A. Karcher, W. Kolbe, J. Lee, M. Levi, N.
Progress Towards Active Pixel Sensor Detectors for Solar Orbiter Dr Nick Waltham Head of Imaging Systems Division, Space Science & Technology Department,
Bulk Silicon CCDs, Point Spread Functions, and Photon Transfer Curves: CCD Testing Activities at ESO Mark Downing, Dietrich Baade, Sebastian Deiries, (ESO/Instrumentation.
Summary of CMS 3D pixel sensors R&D Enver Alagoz 1 On behalf of CMS 3D collaboration 1 Physics Department, Purdue University, West Lafayette, IN
H.-G. Moser Max-Planck-Institut for Physics, Munich CALOR 06 Chicago June 5-9, 2006 Silicon Photomultiplier, a new device for low light level photon detection.
MPI Halbleiterlabor  Otto-Hahn-Ring 6  München  The Halbleiterlabor is in the unique position to have a highly flexible production.
CCDs in space: the effects of radiation on Hubble’s Advanced Camera for Surveys (ACS) Max Mutchler, David Golimowski (Space Telescope Science Institute),
Juan Estrada July 25, Focal Plane Detectors WBS 1.2 this talk Breakout session L. Buckley-Geer J.E. T.Diehl H. Cease Multi CCD (part of WBS 1.5)
SNAP technical design highlights Supernova Acceleration Probe Development Configuration Launch Physics Discoveries Assembly Technology Physics.
Detector development and physics studies in high energy physics experiments Shashikant Dugad Department of High Energy Physics Review, 3-9 Jan 2008.
SNAP Integration Model V. S14 The SNAP Integration Model Mechanical [ SC4 Breakout ] Robin Lafever LBNL Engineering.
LCFI Collaboration Status Report LCUK Meeting Oxford, 29/1/2004 Joel Goldstein for the LCFI Collaboration Bristol, Lancaster, Liverpool, Oxford, QMUL,
Performances of the COROT CCDs for high accuracy photometry Pernelle Bernardi and the CCD team From Meudon : Tristan Buey, Vincent Lapeyrere, Régis Schmidt,
R&D status of FPCCD VTX and its cooling system Yasuhiro Sugimoto for FPCCD VTX group 1.
10/26/20151 Observational Astrophysics I Astronomical detectors Kitchin pp
1 An introduction to radiation hard Monolithic Active Pixel Sensors Or: A tool to measure Secondary Vertices Dennis Doering*, Goethe University Frankfurt.
Tranfer of CCD technology to industry CCD technology transfer to industry is underway (cont’)
MIT Lincoln Laboratory NU Status-1 JAB 11/20/2015 Advanced Photodiode Development 7 April, 2000 James A. Burns ll.mit.edu.
Development of CCDs for the SXI We have developed 2 different types of CCDs for the SXI in parallel.. *Advantage =>They are successfully employed for current.
Lawrence Berkeley National Laboratory MicroSystems Laboratory U.S. Department of Energy Detector R&D Review July 8 th, 2009 S. Holland.
Effects of Surrounding Materials on Proton-Induced Energy Deposition in Large Silicon Diode Arrays Christina L. Howe 1, Robert A. Weller 1, Robert A. Reed.
FPCCD option Yasuhiro Sugimoto 2012/5/24 ILD 1.
FPCCD Vertex detector 22 Dec Y. Sugimoto KEK.
3/16/04mwb, sek, MIT/CSR MIT XIS Status 16 March 2004 Overview: TCE board rebuild status Back-illuminated CCD performance & status (Slightly) improved.
1 Wojciech Dulinski Pixel 2000, Genova, Italy Pixel Sensors for Single Photon Detection Contents - Idea and basic architecture.
Fig. 1: Cross section of a circular DEPMOS- FET pixel cell. Charges collected in the “in- ternal gate’ modulate the transistor current. DEPMOSFET team,
The Second Generation of IR detectors for WFC3 Massimo Robberto European Space Agency and Space Telescope Science Institute.
FPCCD VTX Overview Yasuhiro Sugimoto KEK Tokubetsu-Suisin annual meeting 11.
SPIE Astronomical Instrumentation June 26, 2008 Physics of reverse annealing in high- resistivity ACIS Chandra CCDs Catherine E. Grant (MIT) Bev LaMarr,
in collaboration with Jamie Holder & Vladimir Vassiliev
Report to LCFI Oversight Committee, January 2007 ■ Introduction – towards the ILC ■ Some international VXD developments ■ Progress with LCFI sensor development.
General detectors. CCDs Charge Coupled Devices invented in the 1970s Sensitive to light from optical to X-rays In practice, best use in optical and X-rays.
February 21, 2002TIPS meeting1 "Data contained herein is exempt from ITAR regulations under CFR 125.4(13) -- data approved for public disclosure." TIPS.
Brenna Flaugher for the DES Collaboration BIRP Meeting August 12, 2004 Tucson Fermilab, U Illinois, U Chicago, LBNL, CTIO/NOAO 1 DES Instrument Project.
Scientific DetectorWorkshop, 2005 Taormina Characterization of 1.7um cutoff detectors for SNAP Roger Smith Caltech.
Federico Faccio CERN/PH-MIC
1 Performance of a CCD tracker at room temperature T. Tsukamoto (Saga Univ.) T. Kuniya, H. Watanabe (Saga Univ.); A. Miyamoto, Y. Sugimoto (KEK); S. Takahashi,
Vertex detector R&D Work Plan in /3/11 Y. Sugimoto for KEK-Tohoku-TohokuGakuin-Niigata- ToyamaCMT Collaboration.
MAXI - Monitor of All-sky X-ray Image Performance of the engineering model of the MAXI/SSC Katayama H. a, Tomida H. a, Matsuoka M. a, Tsunemi H. a,b, Miyata.
HST Cal Conf -- Oct 27, Calibration Status and Results for Wide Field Camera 3 – R. Kimble/GSFC, Calibration Status and Results.
LSST Sensor Requirements and Characterization of prototype LSST CCDs V. Radeka, J. Frank, J.C. Geary, D.K. Gilmore, I. Kotov, P. O’Connor, P. Takacs, J.A.
FP-CCD GLD VERTEX GROUP Presenting by Tadashi Nagamine Tohoku University ILC VTX Ringberg Castle, May 2006.
RD42 Status Report W. Trischuk for the RD42 Collaboration LHCC Meeting – June 12, 2013 Development of CVD Diamond Tracking Detectors for Experiments at.
X-ray CCD with low noise charge injection.
Infrared Detectors Grown on Silicon Substrates
Detector Basics The purpose of any detector is to record the light collected by the telescope. All detectors transform the incident radiation into a some.
LSST Camera Detector Status
SCIENTIFIC CMOS PIXELS
Yasuhiro Sugimoto KEK 17 R&D status of FPCCD VTX Yasuhiro Sugimoto KEK 17
Status of CCD Vertex Detector R&D for GLC
Presentation transcript:

SNAP CCD Development Progress Hakeem Oluseyi January 9, 2003

H. M. Oluseyi 2 Development Team LBNL Physics/Astrophysics C. Bebek, M. Levi, H. Oluseyi, S. Perlmutter, V. Prasad LBNL Engineering J. Bercovitz, A. Karcher, W. Kolbe LBNL Microsystems Laboratory S. Holland, N. Palaio, G. Wang Student Interns H. Bertsch, S. Farid, M. Wagner

H. M. Oluseyi 3 Outline Motivation and Technology Commercialization of CCD Technology Precision 4-Side Buttable Packaging Characterization Results Summary

H. M. Oluseyi 4 SNAP r in =6.0 mrad; r out =13.0 mrad r in = mm; r out = mm Guider HgCdTe Spectrograph CCDs Spectrograph port SNAP CCD Design Drivers Wavelength Response Plate Scale/PSF Radiation Tolerance HgCdTe Area Match

H. M. Oluseyi 5 LBNL CCD Technology

H. M. Oluseyi 6 Outline Motivation and Technology Commercialization of CCD Technology Precision 4-Side Buttable Packaging Characterization Results Summary

H. M. Oluseyi 7 LBNL MicroSystems Laboratory CCD’s fabricated at LBNL Microsystems Laboratory Commercialization efforts at CCD foundry in progress Thermco furnaces at LBNL Microsystems Laboratory 150 mm Lithography tool at LBNL Microsystems Laboratory

H. M. Oluseyi 8 Commercially fabricated 150 mm wafer Front-illuminated 2k x 4k (15  m pixel) Back-illumination technology development in progress Fabrication at Dalsa Semiconductor (formerly Mitel) 150 mm DALSA-fabbed wafer. Large rectangular devices are 2k x 4k, 15  m; large square devices are 2.8k x 2.8k, 10.5  m with 4-corner readout.

H. M. Oluseyi 9 SNAP Prototype

H. M. Oluseyi 10 Outline Motivation and Technology Commercialization of CCD Technology Precision 4-Side Buttable Packaging Characterization Results Summary

H. M. Oluseyi 11 Packaged 2k  2k CCD

H. M. Oluseyi 12 CCD Assembly and Test Established a factory to reliably package devices: With reliable connectivity (wire-bonding) Without damage to optically active surface Without ESD damage Without excessive mechanical stress on CCD Packaging status: Used LBNL speckle interferometer to study detector distortion due to differential CTE of CCD, substrate, and moly mount. About a dozen configurations have been studied. Thick AlN looks acceptable for now. Future: CCD mounted to a “thick” silicon substrate is the preferred solution to minimize stress in CCD. We will explore the elimination of wire-bonds and support of the CCD over its entire area. Speckle interferograph – excursions within 6  m.

H. M. Oluseyi 13 Outline Motivation and Technology Commercialization of CCD Technology Precision 4-Side Buttable Packaging Characterization Results Summary

H. M. Oluseyi 14 LBNL CCD Performance Pixel size Well depth Linearity Dark current Sensitivity Persistence Read noise Quantum efficiency Charge transfer efficiency CTE radiation degradation Diffusion Intrapixel response Radiation − Proton when irradiated cold − 60 Co when cold − Heavy ion study Fabrication Packaging  10.5  m devices work, need more experience.  130 ke – for 10.5  m pixel.  Better than 1%.  2 e – /hr/pixel.  3.5  V/e –  Erase mechanism is effective.  2 e –.  Extended red performance realized.  CTI ~ pre-irradiation.  1.5x g/MeV-cm 2  On-going study.   More robust than existing space devices when damaged warm.  No surprises.  An activity during the next 6 months.  Partially commercialized.  Underway R&D areas.

H. M. Oluseyi 15 QE & Noise Performance 2 layer anti-reflection coating: ~ 600A ITO, ~1000A SiO 2

H. M. Oluseyi 16 Radiation Tolerance CTE is measured using the 55 Fe X-ray method at 128 K. The readout speed is 30 kHz, the X-ray density is 0.015/pixel. Degradation is about 1  g/MeV. [1]L.Cawley, C.Hanley, “WFC3 Detector Characterization Report #1: CCD44 Radiation Test Results,” Space Telescope Science Institute Instrument Science Report WFC , Oct.2000 [2] T. Hardy, R. Murowinski, M.J. Deen, “Charge transfer efficiency in proton damaged CCDs,” IEEE Trans. Nucl. Sci., 45(2), pp , April 1998

H. M. Oluseyi 17 Spatial resolution limited by diffusion of photogenerated carriers during drift from generation point to CCD potential wells Key issue for SNAP: Desire for small pixel sizes requires spatial resolution consistent with pixel size Major ramifications on technology development and device design PSF Results V SUB = 20V V SUB = 60V 1100 x 800 back-illuminated CCD, 15  m pixels

H. M. Oluseyi 18 Summary Fully depleted, back-illuminated CCD technology —Device physics —Fabrication at LBNL and commercially —Spatial resolution Use at telescopes On-going efforts —Deployment of more CCD’s at telescopes —Completing 4-side buttable packaging —CCD Development for SNAP Moving towards “Volume” manufacturing Proton damage studies (June 2002 IEEE Trans. Nucl. Sci., Jan ‘02 SPIE) Good spatial resolution and small pixel size –10.5  m pixels with PSF ~ 4  m  –Higher voltages/thinner wafers