A Bolometer Array Instrument for Millimeter Wavelength Philippe Camus, CNRS-CRTBT (Grenoble) Milano, July 6th, 2001.

Slides:

Advertisements

Similar presentations

Observing the SZ Effect with the IRAM 30-meter and the Plateau de Bure Interferometer (on behalf of Francois-Xavier Desert)

Advertisements

Bolometric astronomical imaging at mm wavelengths

Observational techniques meeting #7. Detectors CMOS (active pixel arrays) Arrays of pixels, each composed on a photodetector (photodiode), amplifier,

PACS IIDR 01/02 Mar 2001 Instrument Overview1 PACS Instrument Design Description and System Performance A. Poglitsch.

Detection Methods Coherent ↔ Incoherent Photon Detection ↔ Bolometric Photon Counting ↔ Integrating.

Requirements for a bolometer prototype at the 30m telescope S.Leclercq 23/04/2009.

Device Fabrication Facilities NFFJeol JBX6300FS Direct write on wafers, high throughput, mask writing, for nanoelectronics –25, 50, 100 kV accelerating.

CCD-style imaging for the JCMT. SCUBA-2 technology  the ability to construct large format detector arrays  signal readouts that can be multiplexed To.

Ultimate Cold-Electron Bolometer with Strong Electrothermal Feedback Leonid Kuzmin Chalmers University of Technology Bolometer Group Björkliden

TES Bolometer Array with SQUID readout for Apex

RUN HISTORY Preparation: 17/10Cryostat, pumps and electronics mounted in the cabin (total time 2h) 18/10Cooling down to 80mK. Resonances OK (SRON array)

PALM Project Jan COO All-Hands Mtg. Project 1640 is an infrared, coronographic integral-field spectrograph for high-contrast companion.

Презентація за розділом “Гумористичні твори”

Характеристика ІНДІЇ.

Процюк Н.В. вчитель початкових класів Боярської ЗОШ І – ІІІ ст №4

Á L V A R O S Á N C H E Z M O N G E B A R C E L O N A - N O V E M B E R 23, 2006 Centimeter and Millimeter Emission from Selected High-Mass Star-Forming.

SLAC, May 12th, 2004J.L. Puget PLANCK J.L. Puget Institut d'Astrophysique Spatiale Orsay.

CCD Detectors in High- Resolution Biology Jian Guan

Cardiff University Astronomy Instrumentation Group IRAM Camera meeting October 13-14, Cardiff University Astronomical Instrumentation Peter Ade.

A. Monfardini, IAP 26/06/ Kinetic Inductance Detectors for CoRE-like applications Potentially involving (from the technical point-of-view): - Grenoble.

LEKIDs effort in Italy Martino Calvo B-Pol workshop, IAP Paris, July.

1 Néel people involved in NIKA Researchers:Engineers/Technicians: Alain BenoitGregory Garde (mechanics) Aurelien BideaudJulien Minet (FPGA) Philippe Camus.

STATUS REPORT OF FPC SPICA Task Force Meeting March 29, 2010 MATSUMOTO, Toshio (SNU)

ConX – XEUS meeting Panu Helistö, Mikko Kiviranta Utrecht,

A. Monfardini, IAP 30/07/ NIKA (Néel IRAM KID Array) First light at the 30-m IRAM dish NIKA collaboration: - Institut Néel - Grenoble - AIG - Cardiff.

AMICA Antarctic Multiband Infrared CAmera Favio Bortoletto INAF – Osservatorio Astronomico di Padova on behalf of the AMICA collaboration Telescope and.

Silicon  -Calorimeters at Saclay Main Architecture: All-Si STANDARD Technologies including collective approach for large (1024 pixels) buttable X-rays.

Planar Antenna-Coupled Hot-electron Microbolometer Shafinaz Ali 1, Dan Mccammon 1, Lance D. Cooley 2, Kari.L.Nelms 1, John Peck 3, Daniel Prober 4, Dan.

Our Mission Visible detectors fully matching the requirements of Adaptive Optics wavefront sensors for 10m class telescopes do not yet exist: current detectors.

One of the activities of the spatial team of the CNRS/CRTBT Samuel Leclercq, CNRS/CRTBT (Grenoble, France) European Network on Applied Cryodetectors Munich,

Bolometer Camera Plans at MPIfR, Bonn E. Kreysa, Kaustuv moni Basu, H.-P. Gemünd, G. Siringo, A. Kovacs, F. Schuller, A. Weiß, K. Menten Max-Planck-Institute.

GMTNIRS (Giant Magellan Telescope Near-IR Spectrograph) Survey Science Group Workshop 3 조 김상혁 김재영 최나현

Neel IRAM KIDs Array - Cryostat - Filters - Cold electronics - Measurement methods and assumptions for Sensitivity calculation - Antenna-coupled 42 pixels.

Electrical characterization of a superconducting hot spot microbolometer S.Cibella, R. Leoni, G. Torrioli, M. G. Castellano, A. Coppa, F. Mattioli IFN-CNR,

Detection Methods Coherent ↔ Incoherent Photon Detection ↔ Bolometric Photon Counting ↔ Integrating.

1 Engineering issues for FPCCD VTX Detector Y. Sugimoto KEK July 24, 2007.

N I K A Grenoble (Néel, IRAM, LPSC, LAOG) Cardiff SRON Roma-Trento Néel IRAM KIDs Array Grenoble (Néel, IRAM, LPSC, LAOG) Cardiff SRON Roma-Trento.

HEP-Aachen/16-24 July 2003 L.Chabert IPNL Latest results ot the EDELWEISS experiment : L.Chabert Institut de Physique Nucléaire de Lyon ● CEA-Saclay DAPNIA/DRECAM.

Superconducting Cold-Electron Bolometer with SIS´ and Josephson Tunnel Junctions and JFET Readout Leonid Kuzmin Chalmers University of Technology, MC2.

Optimisation of the PACS Chopper Markus Nielbock Ulrich Klaas Jeroen Bouwman Helmut Dannerbauer Jürgen Schreiber Ulrich Grözinger.

Clusters of Galaxies in the Microwaves

Welcome to the technical meeting on the future bolometer instrument for the IRAM 30m telescope Monday morning: presentations: context and site, 10 arcmin.

Véronique SANGLARD Université de Lyon, UCBL1 CNRS/IN2P3/IPNLyon Status of EDELWEISS-II.

Single photon counting detector for THz radioastronomy. D.Morozov 1,2, M.Tarkhov 1, P.Mauskopf 2, N.Kaurova 1, O.Minaeva 1, V.Seleznev 1, B.Voronov 1 and.

Page 1 Science Payload and Advanced Concepts Office STJs as Photon Detectors.

B-Pol L. Piccirillo Jodrell Bank Centre for Astrophysics (University of Manchester) A European mission to get a CMB polarization measurement limited only.

Status DETECTORS: -Baseline for 2mm: -Baseline for 2mm: NICA 5a (144 pixels, IRAM, 30nm sputtering); average sensitivity: 6mK/Hz 0.5 (1Hz) corresponding.

Demonstration of a Far-IR Detector for Space Imaging Principal Investigators: C. Darren Dowell (326), Jonas Zmuidzinas (Caltech) Co-Investigators: Peter.

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.

MPI Semiconductor Laboratory, The XEUS Instrument Working Group, PNSensor The X-ray Evolving-Universe Spectroscopy (XEUS) mission is under study by the.

The Field Camera Unit Results from technical meeting S. Scuderi INAF – Catania.

Electrical properties of background-limited membrane- isolation TESs for far-IR/subMM spectroscopy M. Kenyon, P. K. Day, C. M Bradford, J. J. Bock, & H.

13,14 July 2005 Feasibility/Concept Study Mid Term Status Review CCAT Instrumentation Gordon Stacey and the Instrumentation Subgroup.

1 CCAT Instrumentation G.J. Stacey Cornell University.

Some considerations about design and technology AE IS DT Science-Techno Tea meeting Diego Perini

From Edelweiss I to Edelweiss II

Leonid Kuzmin and Ian Agulo

Photon counting CCDs as wavefront sensors for LBT A.O. systems

Measure the width of date and D on a dime

Проф. д-р Васил Цанов, Институт за икономически изследвания при БАН

Електронни услуги на НАП

Сътрудничество между полицията и другите специалисти в България

Съобщение Ръководството на НУ “Христо Ботев“ – гр. Елин Пелин

НАЦИОНАЛНА АГЕНЦИЯ ЗА ПРИХОДИТЕ

Съвременни софтуерни решения

от проучване на общественото мнение,

Васил Големански Ноември, 2006

Програма за развитие на селските райони

Моето наследствено призвание

Безопасност на движението

Presentation transcript:

A Bolometer Array Instrument for Millimeter Wavelength Philippe Camus, CNRS-CRTBT (Grenoble) Milano, July 6th, 2001

Bolometric Millimeter Camera Sunyaev-Zel’dovich effect High-Z objects and star formation regions imaging at 1mm => wavelength 1.2mm /2.1mm Which detector at 2.1mm? IRAM 30m Field 5X5 arcmin

Today and future Instruments MAMBO (IRAM 30m) 37 bolometer array on Si3N4 membrane (MPfir)

Optical Layout Cryostat Dilution mK Adaptation to ‘any’ detector Arrays

NbSi Bolometer (CSNSM/ Service d’Aéronomie) Bolometer on thin Si 3 N 4 Memebrane 5X5mm e=100nm Thin film geometry optimisation (typ. 100X400  e=100nm) NEP = W/Hz or W/Hz

Small Array Development (6X6 detectors) NbSi layer co-evaporation & Lithography Objective 8X8 bolometers

Electronic Read-Out Multiplexing is required to reduce the number of output amplifiers (JFET) Low dissipation/low temperature operation (HEMTor MOSFET?) Objective of 8 detector/amplifier