Central Calibration Facilities / CTA Calibration meeting

Slides:



Advertisements
Similar presentations
Institute for Gravitational Research
Advertisements

Weather the state of the atmosphere with respect to wind, temperature, cloudiness, moisture, pressure, etc.
We are called to shine (la la la) Shine (la la la) Shine among them
CW5 Berlin 12/2003 COROT planet field observations at INT La Palma H.J. Deeg 1, M. Deleuil 2, C. Moutou 2 1 IAC, Tenerife; 2 LAM Marseille - Observations.
2009/02/03Meunier et al., Symposium CoRoT EXODAT: Exo-Planet Information System : Evolutions J.-C. Meunier †, M. Deleuil †, C. Moutou †, H. Deeg,
From the first neutrino to CTA A tribute to Astroparticle Physics in South Africa Christian Spiering, DESY Cape Town, April 17, 2012.
Calibration for LHAASO_WFCTA Yong Zhang, LL Ma on behalf of the LHAASO collaboration 32 nd International Cosmic Ray Conference, Beijing 2011.
The Pierre Auger Project By Megan Edwards Bancroft-Rosalie.
OT and the Systematic Automated All-sky Search for Bright Optical Transients Lior Shamir & Robert J. Nemiroff Abstract Real-time detection of bright.
25 YEARS AFTER THE DISCOVERY: SOME CURRENT TOPICS ON LENSED QSOs Santander (Spain), 15th-17th December 2004 Photometric monitoring of SBS : long-term.
New Technology Leads to Better and More Detailed Photos of the Sun Sara Whitbeck Physics 1 Fall 2002.
Emit vs. Reflect.
Organization chart of the functioning of practicums in the Faculty of Education and Psychology.
Planning for a Remote Robotic Observatory in Australia Suketu Bhavsar, Dept. of Physics and Astronomy, University of Kentucky (UK)! Due to the time difference.
My PhD Experience Mireia DosilIFAE-Barcelona29/III/ : B. Sc. Degree in Physics by the Universitat Autònoma de Barcelona (UAB) ● : Diploma.
In-orbit calibration (TOTAL channel) V space -V IBB Raw Earth V (counts) Raw IBB V (counts) =
Chamber with Controlled Atmosphere (AIRFLY) Michal Doubrava – CTU Prague Václav Vacek – CTU Prague Libor Nožka, Miroslav Hrabovský, Petr Schovánek, Miroslav.
Definition Solar energy comes from solar panel.
NICMOS IntraPixel Sensitivity Chun Xu and Bahram Mobasher Space Telescope Science Institute Abstract We present here the new measurements of the NICMOS.
Validation of OMI UV products: results of two ground UV measurement campaigns in Austria P. Weihs 1, M. Blumthaler 2, H. E. Rieder 1,3,*, A. Kreuter 2,
HW 2 Discussion Remember, everything is still an illusion.
Atmospheric Monitoring in the TA experiment
Report of the Working Group Calibration, Monitoring and Site Conveners: Conveners: M. Teshima, B. Khélifi Members: Members: J. Cortina, R.G. Lopez, M.
Wilga 2007 π of the Sky Full π system and simulation Janusz Użycki Faculty of Physics Warsaw University of Technology.
Research and Imaging Program for the SVAS. Current Situation Society supports beginners well –Messier Group –Community Outreach programs Monthly star.
Status Report on Advanced Mesospheric Temperature Mapper Activities at ALOMAR Mike Taylor, P.-Dominique Pautet Utah State University ASAC Meeting - Hamburg,
Two years Night Sky Brightness measurements in The Netherlands | Pamplona
Pachon Sky Camera Christopher Stubbs Chuck Claver Jan 25, 2014.
Atmospheric Aerosol Measurements at the Pierre Auger Observatory The Pierre Auger Observatory operates an array of monitoring devices to record the atmospheric.
H.E.S.S. - MAGIC – CTA meeting Installation of Working Groups Physics & Science Goals MC Simulation & Layout Telescope structures & mirrors Camera designs.
WATER VAPOR RETRIEVAL OVER CLOUD COVER AREA ON LAND Dabin Ji, Jiancheng Shi, Shenglei Zhang Institute for Remote Sensing Applications Chinese Academy of.
Seasonal Change in Titan’s Cloud Activity (A Titan Weather report) Emily Schaller (Caltech) Mike Brown (Caltech), Henry Roe (Lowell Observatory)
Shem Livai Institute for Astronomy Mentor: Colin Aspin Advisor: Bo Reipurth Home Institution: University of Hawaii at Manoa Funding provided through the.
Àlvar Net Dean Facultat de Medicina Universitat Autònoma de Barcelona "Curricular changes relevant to the European Convergency"
OBSERVING THE SUN & PLANETARY TRANSITS Petr HEINZEL Solar Physics Department Astronomical Institute of the Academy of Sciences Czech Republic.
APPLYING OF LANDSCAPE ECOLOGY TO THE PREDICTION OF CLIMATE CHANGES IMPACTS TO AGRICULTURAL CASE STUDY FROM THE CZECH REPUBLIC Ivo MACHAR, Antonín BUČEK,
P.Auger, a major step: Need high statistics large detection area : 2 x3000 km² Uniform sky coverage 2 sites located in each hemisphere Argentina and USA.
PHEMU The Bucharest observational campaign Romanian Astronomical Institute of The Romanian Academy - AIRA ADRIAN SONKA, MARCEL POPESCU, DAN ALIN.
What can we see in the sky?. IN THE SKY WE CAN SEE MUCH MORE!
Optical Astronomy with Cerenkov telescopes E. Oña-Wilhelmi 1,2, O.C. de Jager 1, J. Cortina 3, V. Fonseca 2 1 NWU, Potchefstroom, South Africa. 2 UCM,
Long-term Multispectral Measurements of Skyglow Using Sky Quality Meters Christopher Kyba 1,2, Thomas Ruhtz 1, Jürgen Fischer 1, Franz Hölker 2 1 Freie.
The OmegaCAM photometric systems. OmegaCAM calibration plan (1) Basic OmegaCAM terminology : ● Key bands vs User bands ● Key band -> User band transformation.
Astronomical Projects BEYOND NIGHT SKY. General requirements Weekly Night sky observation. Good knowledge of telescope controlling Imaging. Inviting few.
GERB in-flight calibration Monitoring Instrument Gain.
LSST CCD Chip Calibration Tiarra Stout. LSST Large Synoptic Survey Telescope Camera – 1.6 m by 3 m. 3.2 billion pixels kg (~6173 lbs) 10 square.
Star Map 3D+: Guide to the Night Sky, Planets, Constellations, and Astronomy.
TEM – Lecture 5 Radiative Heat Flow. Radiation Radiation intensity increases with temperature! Every surface above zero K Radiates!
Atmospheric Monitoring for the MAGIC Telescopes Markus Gaug 1,2, Michele Doro 1,2,3, Daniel Garrido 1,2, Christian Fruck 4 for the MAGIC Collaboration.
Grid activities in Czech Republic Jiri Kosina Institute of Physics of the Academy of Sciences of the Czech Republic
Michael Prouza Center for Particle Physics Institute of Physics Academy of Sciences of the Czech Republic Prague Studies of the ultra-high energy cosmic.
Announcements After lecture, we will start with basic image processing using MaxIm DL Dark Sky Night scheduled for tomorrow night (Wednesday). Weather.
Chapter 07 – Rate, Ratio & Variation Q1
Inverse Rendering Shida Beigpour.
NATIONAL INSTITUTE FOR SPACE RESEARCH - INPE
Proper motion accuracy of WFPDB stars
Pointing plans NL (SST-CHEC) David & Remko
OSIRIS flight calibrations so far
I F A E (INSTITUT de FÍSICA d’ALTES ENERGIES) IN FIVE MINUTES
Weather monitoring status and ORM
Atmospheric Aerosol Characterization using
Ultra High Energy Cosmic Ray Spectrum Measured by HiRes Experiment
HEPIX Spring 2012 Meeting Rupert Leitner Charles University, Prague
Chuck F Claver LSST System Scientist & Commissioning Lead
Astronomical Photometry
Tools That Help Us See Celestial Objects
+ = Climate Responses to Biomass Burning Aerosols over South Africa
The Greenhouse Effect Electromagnetic (EM) radiation, radiation processes “Clear Sky” Exercise Earth-Sun System Greenhouse Gases “Cloudy Sky” Exercise.
Star - light, star - bright First star I see to - night.
Ali Evaluation matters and Other Candidate Sites in Ali area?
BUT DIGITAL LIBRARY OPEN ACCESS AT CZECH REPUBLIC
Presentation transcript:

Central Calibration Facilities / CTA Calibration meeting Universitat Autònoma de Barcelona ( Facultat de Ciències i Biociències, Sala d'Actes ) All-Sky-Camera D. Mandat, M. Pech Institute of Physics of the Academy of Sciences of the Czech Republic & Palacky University Olomouc, Faculty of Science

ASC 08/2015 data updated No new data

LA PALMA Magic All Sky Camera

LA PALMA Seasonal variations

LA PALMA Ratio of clear sky images and total number of images per night 1 – night-long clear sky 0 – night-long covered sky

Clear nights vs. Cloudy nights no. nights Total 439 Fully clear 91 Fully covered 64 LA PALMA Clear nights vs. Cloudy nights

Clear nights vs. Cloudy nights histogram LA PALMA Clear nights vs. Cloudy nights histogram

cf criteria vs night-long clear sky LA PALMA cf criteria vs night-long clear sky

Armazones Seasonal variations

Armazones Ratio of clear sky images and total number of images per night 1 – night-long clear sky 0 – night-long covered sky

Clear nights vs. Cloudy nights Armazones no. nights Total 248 Fully clear 198 Fully covered Clear nights vs. Cloudy nights

Clear nights vs. Cloudy nights histogram Armazones Clear nights vs. Cloudy nights histogram

cf criteria vs night-long clear sky Armazones cf criteria vs night-long clear sky

New Camera installation La Palma & Armazones 2K

New Camera installation La Palma 13 – 16. 10. 2015

FIRST light

944 stars in B filter

1493 stars in V filter

photometry B filter V filter

New Camera installation Armazones 2K 19 – 23. 11. 2015 2m

AtmoHEAD 2016: Atmospheric Monitoring for High Energy AstroParticle Detectors May – June 2016 Olomouc Abstracts Jan – May 2016

backup