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ODT and NGC 2008 Photograph courtesy
GeneralNGCAO wavefront sensor systems Scientific detector systems delivered to LSPScientific detector systems in EuropeSocial Activities
• Cabling
• Support of La Silla Paranal
• Planning
• Ultra-cleaning
• Web pages
• Safety
• Debugging
• Meetings
• …
Photograph courtesy
• Reporting
• Presentations
• Training
• Documentation
• Facilities management
• Hyper-sensitization
• Trouble shooting
• Travel & logistics
• ERP (re-)mastering
• Assembling
• Soldering
• Testing
• Market monitoring
• Procurement
• Order tracking
• Obsolescence hunting
• Stock keeping
• Incoming quality control
• Repairs
• Preventive maintenance
‘The three great essentials to achieve anything worth while are: Hard work, Stick-to-itiveness, and Common sense.’
Thomas A. Edison
The daily essence of successful projects
Stefan Hötzl left on September 30
Mirko Todorovic joined on December 15 as Electronics Technician
ODT and NGC 2008
GeneralNGCAO wavefront sensor systemsScientific detector systems delivered to LSPScientific detector systems in EuropeSocial Activities
• ESO-wide presentation
ü Internal Lessons-Learned meeting
• Improved user documentation
† Maintaining OPT/IR commonalities becoming increasingly difficult
• More effective test procedures
• Clean-up of layouts by contractor
• NGC-owned TWiki with
- production manual
- version tracking
- bug lists
- history files for each board
- test reports
New General detector Controller (NGC)
COM
IF
RxRx
NEXT LINK
IF
STATUS
REG
Tx
Tx
Rx SE
QUENCER
AQ MANAGER
AQ FIFO 1
AQ FIFO
CLOCK and
BIAS
TX COM
DOWNSTREAM
RX LINK
On Board
ADCs
DOWNSTREAM
TX LINK
CONFIG
REGISTER
SYSTEM RESET
MONITOR
TELEMETRY
LINK CONFIG
UPSTREAM
RX LINK
UPSTREAM
TX LINK
COM
IF
Rx
xRxx
NEXT LINK
IFNEXT LINK
IF
STATUS
REG
STATUS
REG
Tx Tx
Tx
Tx
Rx SE
QUENCER
AQ MANAGER
AQ MANAGER
AQ FIFO 1
AQ FIFO
AQ FIFO
CLOCK and
BIAS
TX COM
DOWNSTREAM
RX LINK
On Board
ADCs
DOWNSTREAM
TX LINK
CONFIG
REGISTER
CONFIG
REGISTER
SYSTEM RESET
MONITOR
MONITOR
TELEMETRY
TELEMETRY
LINK CONFIG
UPSTREAM
RX LINK
UPSTREAM
TX LINK
COM
IF
RxRxRxRx
NEXT LINK
IFNEXT LINK
IF
STATUS
REG
STATUS
REG
Tx Tx
Tx
Tx
Rx SE
QUENCER
AQ MANAGER
AQ MANAGER
AQ FIFO 1
AQ FIFO 1
AQ FIFO
AQ FIFO
CLOCK and
BIAS
TX COM
DOWNSTREAM
RX LINK
On Board
ADCs
DOWNSTREAM
TX LINK
CONFIG
REGISTER
CONFIG
REGISTER
SYSTEM RESET
MONITOR
MONITOR
TELEMETRY
TELEMETRY
LINK CONFIG
UPSTREAM
RX LINK
UPSTREAM
TX LINK
Rx
xx
Rx AQ
MANAGER
AQ MANAGER
DOWNSTREAM
RX LINK
On Board
ADCs
MONITOR
MONITOR
TELEMETRY
CLOCK 3, 4
CLOCK 5, 6
CLOCK 7, 8
CLOCK 9, 10CLOCK 13,14
CLOCK 11,12CLOCK 15, 16
CLOCK 1, 2
CLOCK 17,18
BIAS 1..4
BIAS 5..8
BIAS 9..12
BIAS 13..16
BIAS 17..20
PowerMinusVariable
PowerPlusVariable
PowerMinusVariable
PowerPlusVariable
PowerPlusVariable
PowerMinusVariable
PowerPlusHigh PowerPlusHigh
PowerPlusHigh
PowerMinusVariable
PowerPlusVariable PowerPlusHigh
1
2
3
SJ_VAR/GND
PowerMinusHigh Bottom Layer of Board
Top Layer of Board
PowerPlusVariable
PowerMinusVariable
PowerPlusVariable_BP
PowerMinusVariable_BP
1
2
3
SJ2
1
2
3
SJ3
Power RegulatorPositiv
+13V
+8V
Power RegulatorNegativ
-13V
-8V
PowerPlusHigh
PowerMinusHigh
PowerPlusHigh_BP
PowerMinusHigh_BP
Power RegulatorPositiv 28V
Power RegulatorNegativ
-12V
-5V
1
2
3
SJ4
1
2
3
SJ1
PowerPlusVariable
1
2
3
SJ5
Obj100
NGC performance
PMC Interface
PCI BUS Interface
Link Processing
and Video Data
Extraction
VIDEO FIFO
DMA
Header #01
PCI REGISTERS
MASTER IF
Rx
Tx
Rx
Tx
Downstream Link
Upstream Link
One Header
Stripped in each
Direction
• RON < 3 e- @ 50 kpix/s demonstrated with e2v CCD types 44-82 and 231
ü MUSE requirements are met
ü Ditto for KMOS, SPHERE IR T/T WFS, and ZIMPOL
ü NGC much more immune to pick-up noise than FIERA is
ü Successfully installed at ODT test benches
• Start-up time of software < 2.5 s
• Standard ADCs run at 1 MHz; on-going developments:
- 3 MHz version of 32AQ board
- 40 MHz high-speed board
• Improved over-voltage protection
• New PMC I/F board for VLTI applications not using SPARTA
† With1310-nm fiber link, could place LLCUs in central computer room.
General change request not supported by LSP Re-consider for every new instrument
NGC deliveries and production in 2008/2009
Systems are due for:○ MUSE (prototype +)○ KMOS○ SPHERE○ ZIMPOL○ Lab usage
• Two successful revisions of Basic and Transition Board
• 32AQ Board unaltered
• Produced 7 power supply units
• Developed new 2-board housing
with fan (for laboratory use only)
Stock ~sufficient for deliveries in 2009 to:• KMOS• MUSE• SPHERE• ZIMPOL
All accomplished
NGC-AOPlan: • Develop standard WFS module for all forthcoming VLT AO systems
• Test controller from Marseille / OHP / Grenoble: OCam
• Combine NGC digital and OCam analog electronics
• General sFPDP I/F to SPARTA at LLCU level
Status:
• Bias and clock-driver boards received from OCam
• NGC sequencer board derived from NGC basic board
(Xilinx Virtex-5 instead of II-Pro)
• Firmware prototyped
ü First ‘laboratory light’ achieved in November
† Waiting for ESO-Ocam
• sFPDP development starting
ODT and NGC 2008
GeneralNGCAO Wavefront sensor systemsScientific detector systems delivered to LSPScientific detector systems in EuropeSocial Activities
(EM-)CCD220 for wavefront sensing @ VLT(or: management at a distance)
StoreArea
Image Area
240x12024□µm
StoreArea
Image Area
240x12024□µm
OP 1
OP 2 GainRegisters
OP 3
OP 4 GainRegisters
OP 8GainRegisters
OP 7
OP 6GainRegisters
OP 5
StoreAreaStoreArea
Image Area
240x12024□µm
StoreArea
Image Area
240x12024□µm
OP 1OP 1
OP 2 GainRegisters
OP 2 GainRegisters
OP 3OP 3
OP 4 GainRegisters
OP 4 GainRegisters
OP 8GainRegisters
OP 8GainRegisters
OP 7OP 7
OP 6GainRegisters
OP 6GainRegisters
OP 5OP 5
• Standard WFS chip for GALACSI/GRAAL/SPHERE
• OCam test controller needed for CCD220 testing by e2v
• Delivery by Marseille delayed
† Two deliveries to e2v failed; 3rd attempt in 2009 January
Nov 2007 ELT AO WFS Possible Developments
Joint tests of pnCCDs with MPE-HLL
• 264x264 51-μm pixels• 450 μm thick • Split frame-transfer device• 528 amplifiers + CAMEX (ASIC)• 1000 fps• RON < 3e
1111
300 400 500 600 700 800 900 1000 110020
30
40
50
60
70
80
90
100
QE pnCCD First Test Run
Wavelength [nm]
QE %
• Plausible back-up for CCD220• Device too small for LGS and SH@E-ELT• But OK for XAO with pyramid WFS?• XAO needs 3 kfps – AApnCCDs?
Slide repeated from last year
• Joint usage of ODT test bench continued• Could help MPE-HLL to make good progress
Standard VLT AO WFS system
(GALACSI, GRAAL, SPHERE)
ü Prepared very comprehensive FDR documentation† Waiting for ESO-OCam, NGC-AO, and more detectors• Baseline detector is CCD 220 from e2v • Need to build 15 systems in 2009-2011 (AOD want them earlier)
1 2 3 4 5 6 7 8
A
B
C
D
87654321
D
C
B
A
Title
Number RevisionSize
A2
Date: 18-Oct-2008 Sheet of File: H:\Projects\AO Facility\Documents\Designs\PDR\Protel\WFSCameraSystem.ddbDrawn By:
AC IN
Thermal Controller
3U 19" Rack
AC IN
Instrument
Pow
er In
& P
eltier
Driv
e
Ther
mal M
onito
ring
Sync
h. IN
Sync
h. O
UT
Fibr
e LLC
UFi
bre R
TC
Digital Control
Pow
er In
& P
eltier
Driv
e
Ther
mal M
onito
ring
Sync
h. IN
Sync
h. O
UT
Fibr
e LLC
UFi
bre R
TC
Head Power
AC IN
Over Temperature
WFS Camera HeadPower Supply
Head Power
AC IN
Over Temperature
Head Power
Coolant From SCPWater
InWaterOut
AC Mains
AC In
Gbit Eth.
(19" 5U Rack)LLCU
AC In
Gbit Eth.
Fiber InFiber Out
NGC PCI I/FFiber InFiber Out AC Mains
LAN to Instrument
JUMO-LLCU Serial Fiber
Camera Head
Serial Link
Serial Comm.Serial Link
WorkstationOUT
RxTx
FibreConverter
OUTRxTx
Thermal Cabinet
Head Electronics IN3
COM 2 RS422
Alarm Relay OUT 5
CCD220 IN1Logic IN 1
Peltier Backside IN2
Peltier Control OUT1
JUMO
Head Electronics IN3
COM 2 RS422
Alarm Relay OUT 5
CCD220 IN1Logic IN 1
Peltier Backside IN2
Peltier Control OUT1
TxINRx
RS232-422/Fibre ConverterTxINRx
To Alarm Handling Unit
Thermal Alarm
Over Temperature Alarm
AC Mains
Camera Head - LLCU
Alarm
Serial
WFS Camera Head
To Other Camera HeadsSynchronization
To RTC SPARTACamera Head -RTC
Fiber Link
Fibre Link
3U 19" Rack
Control IN
Peltier Drive
Kniel CUI 15.3
Power Supply
Control IN
Peltier Drive
Thermal Monitoring
W1
W2
W3
W4 W5
W11
W6
W8
W9
W10
Peltier Drive
AC MainsAC Mains
W12
15V 3A
Peltier Control
To Alarm Handling Unit
Thermal Cabinet
Thermal Cabinet
Back Connector Panel
1 - cooling fluid in2 - cooling fluid return3 - fiber feedthrough4 - electrical connector 15 - electrical connector 26 - flushing valves
Nov 2007 ELT AO WFS Possible Developments 1313
Detectors for E-ELT AO WFS
• Feasibility-study phase with 4 contractors successfully completed
• Issued new CfT for Technology (Pixel) Demonstrator
• Awarded 3 fixed-price contracts (all CMOS-based)
• Last one is supposed to enter Design Review in January, 2009
• First one has already reached shuttle-run phase
† Contractors are struggling with combination of speed and read noise
(some find it difficult to just read the requirements)
• Continually refined requirements (models, contractors’ responses, etc.)
• About mid-2009 issue CfT for Scaled-down Demonstrator
ODT and NGC 2008
GeneralNGCAO wavefront sensor systemsScientific detector systems delivered to LSPScientific detector systems in EuropeSocial Activities
X-shooter
• FIERA software defines 2 nearly fully independent virtual cameras on one common front-end electronics
• VIS system (with MIT/LL CCID-20)• UVB system (with e2v CCD44-82)ü Requirements-compliant systems delivered to Paranal
Giraffe upgrade
• First deep-depletion device with dual-layer coating (e2v)• Successfully commissioned in 2008 May• Prototype for VIMOS red upgradeüThicker silicon offers decisive advantages - but also suffers more particle hits
Major improvement in red sensitivityMuch reduced fringing
10,000 s
2005 Assembly Hall
Garching
OmegaCAM: from Lagerhalle to Bodega
2006 Storage Hall
Garching
2008 Bodega Paranal
OmegaCAM: between the bodegas
• Shipped to Paranal• Re-assembledü Fully successfully testedü I/F instrument / detector system verifiedü Packed and safely stored• Awaiting VST
† Filters from Barr Ass. broken (again …)
OmegaCAM: one CCD failed
Typically asked questions:
How bad is it?
It’s very bad
Is damage due to transport?
No, it isn’t
When will CCD be un-kaputted?
CCD can’t be repaired
Can it be replaced?
Yes. At cost and risk
Will it be replaced?
It depends
31 CCDs functioning as before!
Here it is
(Identical CCD died years ago under similar circumstances)
ODT and NGC 2008
GeneralNGCAO wavefront sensor systemsScientific detector systems delivered to LSPScientific detector systems in EuropeSocial Activities
Multi-unit Spectroscopic Explorer (MUSE)
(Multi = 24 = MANY)
Tee Pee
• 4k x 4k engineering-grade CCD 231 from e2v extensively tested• Helped to debug 2nd ODT test bench and NGCü Requirements are met• Final detector head just manufactured – will install science-grade CCDü Prototype system to be delivered in March• Agreement reached with AI Potsdam for support of serial production† ESO has become part of MUSE Consortium: extra bureaucracy• TeePee serial production initiated
ZIMPOL (SPHERE)
Originally, ZIMPOL was supposed to provide a VLT-compliant detector system
Now, the ODT may more nearly be supplying a ZIMPOL-compliant detector system
• Comprehensive FDR documentation submitted• NGC system produced
UVES red upgrade• EMMI red released for cannibalism• Installation in 2009 July
VIMOS red upgrade• Contract with e2v signed in 2008 (?)• 5 deep-depletion CCDs due before 2009 August • Installation in P84
FIERA• 2009 releases of VLTSW (incl. enhancements)
Pulpo1• Multiple clean-ups after upgrade attempts on LSP
MIT/LL Phase 4• Have given up on receiving any devices
Miscellaneous
ESPRESSO Phase A• Broad survey of detector options
Ultra-stable Cryostat• Procurement of parts
ODT and NGC 2008
GeneralNGCAO wavefront sensor systemsScientific detector systems delivered to LSPScientific detector systems in EuropeSocial Activities
Team building efforts
INS SADness
ODT Isar Party
Thank you, Sebastian!
Happy holidays!
NGC 2264 (WFI@ESO/MPG 2.2-m)[WFI celebrating 10th anniversary!]