INSTITUTO DE ESTRUCTURA DE LA MATERIA

Slides:



Advertisements
Similar presentations
Basics of mm interferometry Turku Summer School – June 2009 Sébastien Muller Nordic ARC Onsala Space Observatory, Sweden.
Advertisements

64th OSU International Symposium on Molecular Spectroscopy June 22-26, 2009 José Luis Doménech Instituto de Estructura de la Materia 1 MEASUREMENT OF ROTATIONAL.
Calibration Ron Maddalena NRAO – Green Bank November 2012.
IFCA Activities in R&D for ILC Instituto de Física de Cantabria [CSIC-UC] Spain.
The SMA CO(6-5) & 690 GHz Continuum Observations of Arp 220 Satoki Matsushita (ASIAA) D. Iono (CfA), C.-Y. Chou (ASIAA), M. Gurwell (CfA), P.-Y. Hsieh.
CHARACTERIZATION of the SiC 3 H - anion N. Inostroza 1, M. L. Senent 1 1 Instituto de Estructura de la Materia, C.S.I.C, Departamento de Astrofísica Molecular.
Radio Aeronomy at Onsala Space Observatory Peter Forkman
FIR Optics Meeting – January Calibration issues related to the optical performances David Teyssier.
Tunable Bandpass Filter. Specifications Tuning range:1.5 GHz to 2.5 GHz Low insertion loss 50  terminations Stable magnitude response over the full tuning.
Performance Evaluation of SiPM Arrays under Strong Magnetic Fields
The concept Provide a small (2 K) difference signal to allow continuous receiver gain measurement to 1% Alternate between three loads: 300K, 400K, sky.
Antenna Gain and Source calibration Jim Gibson and Jack Welch.
Thermally Deformable Mirrors: a new Adaptive Optics scheme for Advanced Gravitational Wave Interferometers Marie Kasprzack Laboratoire de l’Accélérateur.
Calibration Ron Maddalena NRAO – Green Bank July 2009.
Calibration and Data reduction Strategies Cormac Purcell & Ned Ladd Mopra Training Weekend May 2005.
Recoil Polarimetry in Meson Photoproduction at MAMI Mark Sikora, Derek Glazier, Dan Watts School of Physics, University of Edinburgh, UK Introduction The.
Spectral Line Calibration Techniques with Single Dish Telescopes K. O’Neil NRAO - GB.
Polarization at IRAM Status and Plans S.Guilloteau Laboratoire d’Astrophysique de Bordeaux.
AIC Colour 05 1 Reflectance changes in white reflectance standards measured in different instruments with 0/d geometry Joaquín Campos, Alicia Pons and.
The ALMA TelCal subsystem Dominique Broguière, Institut de RadioAstronomie Millimétrique (IRAM) TelCal Phasing meeting – Grenoble -10/12/2012.
O. YAZIDI, A. BEN HOURIA AND Z. BEN LAKHDAR, LSAMA, Universitè de Tunis El Manar, Tunis, TUNISIA M. L. SENENT, Departamento de Astrofísica Molecular e.
Making MOPRA go! Lucyna Kedziora-Chudczer Friend of the telescope (UNSW)
1 EVLA System Commissioning Results EVLA Advisory Committee Meeting, March 19-20, 2009 Rick Perley EVLA Project Scientist.
AST 443: Submm & Radio Astronomy November 18, 2003.
J. Cernicharo. “The interpreation H 2 O Observations” Water Vapour in Astrophysics Models and Observations FROM ISO, SWAS and ODIN TO HERSCHEL José Cernicharo.
The Robert C Byrd Green Bank Telescope Frank Ghigo, National Radio Astronomy Observatory US VLBI Meeting, Socorro, Nov 2011 VLBI usage: About 15% of GBT.
Extragalactic Absorption Lines Observed from Arecibo Chris Salter (National Astronomy & Ionosphere Center, Arecibo Observatory, Puerto Rico)
65th OSU International Symposium on Molecular Spectroscopy June 21-25, 2010 José Luis Doménech Instituto de Estructura de la Materia 1 TIME-RESOLVED ROTATIONAL.
EFFECT OF TEMPERATURE ON POLYETHYLENE TERAPHTHALATE COATED ECCS PLATES IN ACETIC-ACETATE MEDIUM. E.Zumelzu(1), F. Rull(2), C. Ortega(3), C. Cabezas(4)
ALMA Science WorkshopMay 14, 2004 Present and Future Thomas W. Folkers Arizona Radio Observatory.
Molecular Clouds in in the LMC at High Resolution: The Importance of Short ALMA Baselines T. Wong 1,2,4, J. B. Whiteoak 1, M. Hunt 2, J. Ott 1, Y.-N. Chin.
C. Chandler, Synthesis Imaging Summer School, 24 June Mm-Wave Interferometry Claire Chandler Why a special lecture on mm interferometry? –everything.
Observing Strategies at cm wavelengths Making good decisions Jessica Chapman Synthesis Workshop May 2003.
ROTATIONAL SPECTROSCOPY OF CO SOLVATED WITH PARA-H 2 MOLECULES Paul Raston and Wolfgang Jäger Department of Chemistry, University of Alberta, Edmonton,
1 Problems and Challenges in the mm/submm. 2 Effect of atmosphere on data: Tsys Mean Refraction Phase fluctuations Correction techniques Other facility.
Beam Instrumentation for the HIE-ISOLDE linac Francesca Zocca ISOLDE Workshop and Users Meeting December CERN Instituto de Estructura de la.
Starring Kim Arvidsson Matthew Povich Jamie Riggs Directed by B. Murray Lewis Limits on OH 5 GHz Maser Emission from an OH/IR Star and a Proto-Planetary.
1 Synthesis Imaging Workshop Sept 24-28, 2001, ATCA Narrabri Calibration & Flagging Mark Wieringa  Theory of calibration  Practice - RFI & malfunctions.
Science IPT A. Wootten Lead NRAO is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc.
Jan URSI1 Fast Switching Phase Compensation for ALMA Mark Holdaway NRAO/Tucson Other Fast Switching Contributors: Frazer Owen Michael Rupen Chris.
Atmospheric phase correction at the Plateau de Bure interferometer IRAM interferometry school 2006 Aris Karastergiou.
Fourth IRAM Millimeter Interferometry School 2004: Atmospheric phase correction 1 Atmospheric phase correction Jan Martin Winters IRAM, Grenoble.
Charles L Wrench RCRU Determining Cloud Liquid Water Path from Radiometer measurements at Chilbolton.
NAT crystals exposed to HCl: a systematic RAIR investigation Rafael Escribano, Víctor J. Herrero, Belén Maté, Miguel Angel Moreno and Ismael K. Ortega.
A Time Efficient Experimental Approach to Catalogues for Astrophysics Frank C. De Lucia Ivan Medvedev Department of Physics Ohio State University Workshop.
Rick PerleyEVLA Feeds CDR 17 February Performance of the L-Band Feed Rick Perley.
Atmospheric extinction Suppose that Earth’s atmosphere has mass absorption coefficient  at wavelength. If f 0 is flux of incoming beam above atmosphere,
José Luis Doménech, RD08 70th International Symposium on Molecular Spectroscopy Urbana Champaign, June 22-26,2015 NEW ACCURATE WAVENUMBERS OF H 35 Cl +
An Experimental Approach to the Prediction of Complete Millimeter and Submillimeter Spectra at Astrophysical Temperatures Ivan Medvedev and Frank C. De.
Astrochemistry with the Upgraded Combined Array for Research in Millimeter-wave Astronomy D. N. Friedel Department of Astronomy University of Illinois.
Objectives  Distinguish between Accuracy and Precision.  Determine the Precision of Measured quantities.
HiRadMat Primary Beam Overview C. Hessler, B. Goddard, M. Meddahi On behalf of the HiRadMat Primary beam line working group HiRadMat Project Review
M. De Petris – Sept. 21st, in collaboration with G. Amico 1, A. Baù 2, D. Buzi 1, S. De Gregori 1, M. Gervasi 2, L. Lamagna 1, S. Masieri.
IRAM Observing School 2007 Clemens Thum IRAM, Grenoble, France Lecture 2 : Fundamentals continued calibration efficiencies beam shape observing modes (single.
A brief introduction to QiTai radio Telescope (QTT)
The HCl/H2O Solid System: Infrared Spectra of HCl Tri-and Hexahydrate
International Symposium on Molecular Spectroscopy
The microwave spectrum of lactaldehyde, the simplest chiral sugar.
ALMA water vapour radiometer project
JINR: J. Budagov, M. Lyablin., G. Shirkov.
Observing Strategies for the Compact Array
Calibration of the ACA System
Polarization Calibration
Two Kinds of Polarized Light
LABORATORY AND ASTRONOMICAL DISCOVERY OF HYDROMAGNESIUM ISOCYANIDE
ALMA Calibration Introduction
Formic Acid or 18OH Absorption?
Feed & Front End PDR—Sys. Reqts
大气折射与天线指向.
Research progress of 7mm receiver amplitude calibration
Presentation transcript:

INSTITUTO DE ESTRUCTURA DE LA MATERIA DPTO FÍSICA MOLECULAR TEST OF THE SEMITRANSPARENT VANE CALIBRATION SCHEME J. Martín-Pintado Design and construction of the device: S. Navarro, M. Carter (IRAM) Implementation : W. Brunswig and A. Sievers (IRAM) Tests: J. Martín-Pintado, J. Cernicharo, J.R. Pardo, A. Rodríguez (IEM-CSIC) 12/5/2018

INSTITUTO DE ESTRUCTURA DE LA MATERIA DPTO FÍSICA MOLECULAR Device Rotary actuator (switch time 1 s) 90 and 230 GHz observations Standard calibration system Position 1 * 1.5 m from the receiver * Orthogonal linear polarizations Position 2 * 10-15 cm from the receiver * No polarization 1 2 12/5/2018

INSTITUTO DE ESTRUCTURA DE LA MATERIA DPTO FÍSICA MOLECULAR Vane material (B.Lazareff and F.Mattiocco, IRAM, June 2001) Polymer foams 1 cm thickness Transmission 0.9 at 100 GHz 12/5/2018

INSTITUTO DE ESTRUCTURA DE LA MATERIA DPTO FÍSICA MOLECULAR Testing the main hypothesis (Position 1) Tvane = f´ * Tamb+(1-f)*TN2 f’=f Measurement of the transmission (1-f) of the S/T vane Continuum sources using beam switching with vane-on and off 0.5% accuracy in 30 s for a 6 Jy source at 100GHz Polarization effects (0.3% ?) Measurement of Tvane Calibrated with N2 and ambient loads Accuracy: <3%: 1.5% saturation of 10% on the ambient load 1.2% for 1 K in the N2 load 1.8% for 0.5% in the transmission coefficient 12/5/2018

INSTITUTO DE ESTRUCTURA DE LA MATERIA DPTO FÍSICA MOLECULAR Effects of standing waves (Position 2) Tilt the semitransparent vane: Measurements of the stable ambient load (bandpass) calibrated with the semitransparent vane-N2 load Accuracy: <3% IF THE MAIN ASUMPTION OF THE S/T VANE CALIBRATION SCHEME IS FULFILL TO BETTER THAN 3%? Comparison of the accuracy of the S/T vane calibration relative to the dual-load and chopper wheel calibration systems 12/5/2018

INSTITUTO DE ESTRUCTURA DE LA MATERIA DPTO FÍSICA MOLECULAR Comparison of calibration schemes (Position 2) Measurements of the intensity of astronomical sources at different elevations calibrated with: Dual-load with atmospheric opacity from ATM+sky emission Semitransparent vane with 2nd order correction ATM+water Chopper wheel with 2nd order correction ATM+water Check the relative accuracy of the three schemes to correct for elevation effects 12/5/2018