SIMBOL-X. Peter Lechner MPI-HLL Project Review Schloss Ringberg, science background. mission. telescope.

Similar documents
The Simbol-X. Low Energy Detector. Peter Lechner PNSensor & MPI-HLL. on behalf of the LED consortium. Paris, Simbol-X Symposium. P.

The Simbol-X focal plane

The focal plane of the Simbol X space mission

The Wide Field Imager

STATE-OF-THE-ART SILICON DETECTORS FOR X-RAY SPECTROSCOPY

MPE's views on SDDs as focal plane detectors for SFA

Active Pixel Matrix for X-ray Satellite Missions

The Wide Field Imager for the Athena X-ray Observatory

erosita mirror calibration:

Wide Field Imager for Athena

The Digital Data Processing Unit for the HTRS on board IXO

Detectors for AXIS. Eric D. Miller Catherine Grant (MIT)

The superconducting microcalorimeters array for the X IFU instrument on board of Athena Luciano Gottardi

Gas Pixel Detectors. Ronaldo Bellazzini INFN - Pisa. 8th International Workshop on Radiation Imaging Detectors (IWORID-8) Pisa 2-6/july 2

MPI Halbleiterlabor. MPI Semiconductor Laboratory. MPI mf

The Wide Field Imager Instrument for Athena

Highly Miniaturised Radiation Monitor (HMRM) Status Report. Yulia Bogdanova, Nicola Guerrini, Ben Marsh, Simon Woodward, Rain Irshad

DepFET detectors in astrophysics and particle physics instrumentation (and photon science)

Norbert Meyners, DESY. LCTW 09 Orsay, Nov. 2009

Detectors that cover a dynamic range of more than 1 million in several dimensions

Pixel hybrid photon detectors

Caliste 64, an innovative CdTe hard X-ray micro-camera

The Hot and Energetic Universe

The Asteroid Finder Focal Plane

Development and Performance of. Kyoto s X-ray Astronomical SOI pixel sensor Sensor

ITk silicon strips detector test beam at DESY

MONS Field Monitor. System Definition Phase. Design Report

DELIVERABLE!D60.4! 1k!x!1k!pnCCD!Conceptual!Design! WP60!Advanced!Instrumentation!Development! 1 ST Reporting Period.

OPAL Optical Profiling of the Atmospheric Limb

Multi-Element Si Sensor with Readout ASIC for EXAFS Spectroscopy 1

THE OFFICINE GALILEO DIGITAL SUN SENSOR

Wide field imager instrument for the Advanced Telescope for High Energy Astrophysics

A LATERAL SENSOR FOR THE ALIGNMENT OF TWO FORMATION-FLYING SATELLITES

AIDA-2020 Advanced European Infrastructures for Detectors at Accelerators. Deliverable Report. CERN pixel beam telescope for the PS

Chromatic X-Ray imaging with a fine pitch CdTe sensor coupled to a large area photon counting pixel ASIC

Single Photon Counting in the Visible

Strip Detectors. Principal: Silicon strip detector. Ingrid--MariaGregor,SemiconductorsasParticleDetectors. metallization (Al) p +--strips

Selecting an image sensor for the EJSM VIS/NIR camera systems

Spectroscopic Performance of DEPFET active Pixel Sensor Prototypes suitable for the high count rate Athena WFI Detector

PNCCD for photon detection from near infrared to X-rays

CaSSIS. Colour and Stereo Surface Imaging System. L. Gambicorti & CaSSIS team

DATA COMPRESSION & PROCESSING

Inverted-COR: Inverted-Occultation Coronagraph for Solar Orbiter

LISA and SMART2 Optical Work in Europe

Muon detection in security applications and monolithic active pixel sensors

Wide X-ray Field of View

STA1600LN x Element Image Area CCD Image Sensor

CCD1600A Full Frame CCD Image Sensor x Element Image Area

Light gathering Power: Magnification with eyepiece:

EUDET Pixel Telescope Copies

PLATO Preliminary Requirements Review Technical Report

The Wide-Field Imager for IXO: Status and future activities

MAORY E-ELT MCAO module project overview

X-ray Evolving-Universe Spectroscopy

MIRI The Mid-Infrared Instrument for the JWST. ESO, Garching 13 th April 2010 Alistair Glasse (MIRI Instrument Scientist)

Vladimir Vassiliev UCLA

Simulation of High Resistivity (CMOS) Pixels

Resolution studies on silicon strip sensors with fine pitch

Gas scintillation Glass GEM detector for high-resolution X-ray imaging and CT

Nuclear Instruments and Methods in Physics Research A

NIRCam Optical Analysis

Design and Performance of a Pinned Photodiode CMOS Image Sensor Using Reverse Substrate Bias

Test Beam Measurements for the Upgrade of the CMS Phase I Pixel Detector

CCDs for Earth Observation James Endicott 1 st September th UK China Workshop on Space Science and Technology, Milton Keynes, UK

Fast Solar Polarimeter

A Prototype Amplifier-Discriminator Chip for the GLAST Silicon-Strip Tracker

Electron-Bombarded CMOS

A 1m Resolution Camera For Small Satellites


X-Ray Spectroscopy with a CCD Detector. Application Note

Earth Emitted Longwave Energy. 240 W/m 2. Top of the Atmosphere (TOA)

Design of a Free Space Optical Communication Module for Small Satellites

Towards a 10 μs, thin high resolution pixelated CMOS sensor system for future vertex detectors

Mission requirements and satellite overview

Arrays of digital Silicon Photomultipliers Intrinsic performance and Application to Scintillator Readout

Pixel sensors with different pitch layouts for ATLAS Phase-II upgrade

An integral eld spectrograph for the 4-m European Solar Telescope

A new Infra-Red Camera for COAST. Richard Neill - PhD student Supervisor: Dr John Young

e2v Launches New Onyx 1.3M for Premium Performance in Low Light Conditions

High SEE Tolerance in a Radiation Hardened CMOS Image Sensor Designed for the Meteosat Third Generation FCI-VisDA Instrument

SLICING THE UNIVERSE CCDs for MUSE

TAOS II: Three 88-Megapixel astronomy arrays of large area, backthinned, and low-noise CMOS sensors

LCLS project update. John Arthur. LCLS Photon Systems Manager

Non-adaptive Wavefront Control

Virgo status and commissioning results

RP220 Trigger update & issues after the new baseline

CFHT and Subaru Wide Field Camera

Interplanetary CubeSats mission for space weather evaluations and technology demonstration

BMC s heritage deformable mirror technology that uses hysteresis free electrostatic

Low Cost Earth Sensor based on Oxygen Airglow

CMS Tracker Upgrades. R&D Plans, Present Status and Perspectives. Benedikt Vormwald Hamburg University on behalf of the CMS collaboration

PAPER NUMBER: PAPER TITLE: Multi-band CMOS Sensor simplify FPA design. SPIE, Remote sensing 2015, Toulouse, France.

MERIS US Workshop. Instrument Overview. Steven Delwart

CMOS sensor for TAOS 2

CCD Procurement Specification EUV Imaging Spectrometer

SOAR Integral Field Spectrograph (SIFS): Call for Science Verification Proposals

CMOS pixel sensors developments in Strasbourg

LISA AIV/T. N. Dinu Jaeger ARTEMIS. [joint work with APC and CNES]

PandaX-III High Pressure Gas TPC and its Prototype

Silicon Drift Detector. with On- Chip Ele ctronics for X-Ray Spectroscopy. KETEK GmbH Am Isarbach 30 D O berschleißheim GERMANY

Transcription:

SIMBOL-X Peter Lechner MPI-HLL Project Review Schloss Ringberg, 24.04.07 science background mission telescope detector payload low energy detector

science background science targets black holes astrophysics - matter in the vicinity of a BH - history of supermassive BH formation particle acceleration in the universe - mechanism, efficiency, maximum energy requirements cover the sensitivity gap SIMBOL-X = INTEGRAL : coded mask optics hard energy X-ray range covered by INTEGRAL + energy range sensitivity focal length field of view angular resolution spectral resolution timing accuracy 0.5 80 kev ( 100 kev) 0.1 10 µcrab 18 20 m 12 arcmin @ 30 kev 20 arcsec HEW @ 30 kev 150 ev @ 6 kev (Fe line) 1.3 kev @ 68 kev (Ti line) ~ 100 µsec > 15 kev : mcrab 12 arcmin 30 degrees + angular resolution of XMM XMM : focusing optics < 10 kev : µcrab 15 arcsec 30 arcmin

mission mission scenario detector and mirror spacecraft 4 days orbit (20.000 / 180.000 km) > 70 % observation time time budget 0.5 y 2.5 y 2 y commissioning nominal operational phase extension provision net science time: > 100 Msec no. of pointings: ~ 1000 (+ 500) on-board data storage telemetry 1x / orbit status French Italian German consortium phase A (F, D Jun07, I Nov07) phase B likely to come in 2008 launch end 2013 (Soyuz/Kourou) formation flight probably 1st science mission autonomous operation alignment by radio antennas and laser system positioning accuracy: 1 x 1 x 3 cm³ positioning knowledge: 0.5 x 0.5 cm²

telescope leadership Osservatorio Astronomico di Brera, Italy industry contract: Alenia principle nested mirrors, Wolter-I geometry technique Ni electroforming replication Pt/C multi-layer coating by sputtering 2 spider support structures effective area (on axis) > 1000 cm2 @ 2 kev > 600 cm2 @ 8 kev > 100 cm2 @ 70 kev parameters no. of shells ~ 100 focal length diameter shell tickness 20 m ~ 70 cm 1/3 of XMM

detector payload leadership Service d Astrophysique CEA Saclay, France industry contracts: Alcatel, Astrium ANTENNAS COLLIMATOR : DPCA HONEYCOMB STRUCTURE DPDPA1 DPDPA2 DPHEDEA DPLEDEA DPACDEA RADIATOR : DPTCA DPFPA FPA SUPPORT STABLE PLATFORM SP PLATFORM

detector payload low energy detector (LED) energy range 0.5 20 kev high energy detector (HED) energy range 5 kev CdTe / CdZnTe (both under test) pixel size 625 x 625 µm focal plane format 128 x 128 sub-units of 16 x 16 3D integration of fe-electronics status: working 8 x 8 module active anti-coincidence shield plastic scintillator PMT readout fibre coupling status: material selection "Calliste64" HED subunit Calliste256 1 cm² 4 side buttable 4 r/o ASICs self-triggered 64 x in FP

LED requirements science drivers cosmic X-ray background estimation source confusion limit source identification, overlap with HED Fe line spectroscopy anticoincidence pulsar timing studies hard X-ray mission specifications field of view 12 arcmin > 7 cm Ø angular resolution 20 arcsec point spread function <1.9 mm energy range 0.5 20 kev energy resolution 150 kev @ 6 kev min. frametime time resolution 100 µsec "transparent" s/c constraints LED parameters format 8 x 8 cm² 128 x 128 pixels pixel size 625 µm thin entrance window thickness 450 µm low electronic noise 10 el. ENC r/o time / row 4 µsec window mode 32 pixels monolithic device high temperature -40 C

LED layout collaboration HLL/MPE: detector, thermal and mechanical interfaces IAAT: daq system Macro Pixel Detector SDD & DEPFET pixel size 625 µm focal plane format 128 x 128 sensitive area 8 x 8 cm² largely redundant quadrants, individual r/o & control readout modes full frame CCD-like, bi-directional window mode selectable window size, no additional hardware

LED dummy SIMBOL-X LED dummy design according to the current state of knowledge and technology 128 x 128 pixels (625 µm) organised in 4 independent quadrants processing of dummy wafers finished front- and backside metallisation for demonstration structural & thermal model (phase B)

LED readout and control Active Pixel Sensor XEUS prototype 2 x SWITCHER-II control ASIC 64 channel control chip 2 ports / channel supply of switched voltages high voltage CMOS process > 20 V p-p 50 MHz clock CAMEX 64 readout chip (baseline) 64 channel amplifier source follower 8-fold CDS filter 64/1 analog multiplexer readout time / row ~ 6 µsec VELA readout chip (option) collaboration with PoliMi 4 channel prototype tested 64 channel version in design drain current readout current integration / deintegration filter readout time / row < 3 µsec

LED performance experience from XEUS WFI 64 x 64 prototypes DEPFET pixels readout time / row FWHM @ 6 kev 75 x 75 µm² ~ 20 µsec 133 ev Macro Pixel Detector 4 x 4 prototype pixel size integration time FWHM @ 6 kev 1 x 1 mm² 1 µsec 122 ev extrapolated SX energy resolution assumptions RT leakage current r/o time / row serial noise 0.1 1 na/cm² 4 µsec 5 el. r.m.s. radiation damage by solar protons real results soon to come

LED demonstrator quadrant prototype science verification module phase B, operation with HED 500 µm pixels format 64 x 64 sensitive area 32 x 32 mm² status 2 chips on PXD5 production difference in DEPFET clear structure 1st Al layer, to be patterned this week available in Jul07

summary & outlook Low Energy Detector Simbol-X representative detector in summer Simbol-X mission good chance to get into phase B in 2008 if that occurs flight hardware processing in 2008