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Report of the Working Group Calibration, Monitoring and Site Conveners: M. Teshima, B. Khélifi Members: J. Cortina, R.G. Lopez, M. Gaug, E. Giraud, R. Mirzoyan, P. Mayumdar, M. Mori, V. Mitev, M. Panter, A. Sillampaä, S. Swordy, J.P. Tavernet, G. Vasileiadis, S. Wagner Activity: 5 phone-conferences, email exchanges Draft for the Letter of Intend Calibration and atmospheric monitoring What to calibrate and to monitor? • Atmospheric monitoring: Extinction coefficient • Optical components: Mirrors, funnels, photocathods Conversion factor: # ADC per Cherenkov photons B. Khélifi • Camera electronics: Gain, flat fielding, usable pixels, … WG Calibration/Monitoring/Site Paris, 02/03/2007 Camera performances • Functioning parameters of the cameras not treated here, Just the camera characteristics used for the data analysis • Channel noise – From electronics – From Night Sky Background No need of specific instrumentation • Conversion factor: #ADC per photoelectron – Components: efficiency of the integration window, electronic gains, Photodetector internal gain LED flashers B. Khélifi WG Calibration/Monitoring/Site Paris, 02/03/2007 Camera performances (2) • Flat fielding – Different detection efficiency between channels Funnels, photocathods LED flashers • Usable channels − Malfunctioning reasons depend on camera technology − Big efforts should be done to their identifications No need of specific instrumentation B. Khélifi WG Calibration/Monitoring/Site Paris, 02/03/2007 Optical components • Involved components: Mean Photocathod efficiency, mean funnel and mirrors efficiency • This global efficiency allows an absolute calibration Use of muon rings B. Khélifi WG Calibration/Monitoring/Site Paris, 02/03/2007 Atmospheric monitoring • Standard weather conditions Meteo station • Water vapor and cloud monitoring Infrared radiometers B. Khélifi WG Calibration/Monitoring/Site Paris, 02/03/2007 Atmospheric monitoring (2) • Estimation of the optical depth above telescopes: LIDAR Transmissometer (transmissivity at the ground layers) Results of LIDAR simulations V. Mitev • Photometric telescope Cirrus cloud – Continuous monitoring TRmodel = 0.5836 – Cross-check with TRmeas LIDAR = 0.5830 TRmodel = 0.9498 TRmeas = 0.9508 (9-10.4 km) (3-5 km) • Atmosphere profile Troposphere/Desert Dust – Radiosondes: seasonal variations 60° B. Khélifi Dust layer WG Calibration/Monitoring/Site Paris, 02/03/2007 Conclusions • Draft of the WG has been submitted (8 pages) • For the Design Study (Working Package 12): – Big efforts on the LIDAR technique to routinely correct for atmosphere variations Closer work with atmospheric physicists – Efforts to measure and to use the seasonal atmospheric profile measured by radiosondes – Apply and test these atmospheric corrections to the data analysis B. Khélifi WG Calibration/Monitoring/Site Paris, 02/03/2007 Candidates for CTA sites Criteria of selection • • • • • • • Altitude above 1.5 km Small cloud coverage: good nights > 60% Atmosphere transparent and dry Latitude around +30° N and -30° S Facility of site access Political stability … B. Khélifi WG Calibration/Monitoring/Site Paris, 02/03/2007 CTA North Sites - Parameters Location (long itud e) Location (Lattitud e) Heig ht R ig id ity cutoff Land owner Av aliab le flat area Typ e of g round Access from nearb y City (hrs) Access from EU (hrs) Nearest international airp ort 17.86 W 28.75 N 2200 m IAC 300x300m2 soil, rocks 1 5 La Palma Clear nig hts (sp ectroscop ic nig ht)/yr Photometric nig hts/yr Days with g round fog /yr Lig ht p ollution 75% Av summer d ay /nig ht temp Av winter d ay / nig ht temp # of d ays with wind v el (>10m/s) # of Cyclones and Tornad es / 10yr Annual p recip itation(mm) Av summer humid ity Av winter humid ity Av snow d ep th M aximum snow d ep th last 10yr 17 2 13 % Electric p ower line W ater Hand y/M ob il serv ice Distance to hig h b and wid th internet Sites - Parameters B. Khélifi 2400 m 112.5 W 37.5 N 1800-3000 M una K ea 78.96E 32.78N 4300m State Ind ia G ov t v ast 2x2km2 10x10 km2 soil, rocks soil,rocks 6-7 hrs 2 1 21-22 19 5 Delhi S.L.C. Tenerife 260 190 low low low v ery low 20/10-15C -5/-15C 19% nil 2mm 15-45% 10-40% 10-40% 40-60% Yes Yes Yes 0 No Yes No 0 0 0 90 260K m 260K m 75K m Nearest hotels or lod g e (mins) Nearest restaurants (mins) Nearest hosp itals (mins) Dang erous animals End emic d isease Scientific facilities Political stub ility CTA-North Hanle So. Utah Teid e La Palma no no ENO Stab le La Palma no no IAO yes no no ENO Stab le Teid e So. Utah Hanle WG Calibration/Monitoring/Site M una K ea Paris, 02/03/2007 CTA South Sites - Parameters Location (long itud e) Location (Lattitud e) Heig ht R ig id ity cutoff Land owner Av aliab le flat area Typ e of g round Access from nearb y City (hrs) Access from EU (hrs) Nearest international airp ort Clear nig hts (sp ectroscop ic nig ht)/yr Photometric nig hts/yr Days with g round fog /yr Lig ht p ollution Av summer d ay /nig ht temp Av winter d ay / nig ht temp # of d ays with wind v el (>10m/s) # of Cyclones and Tornad es / 10yr Annual p recip itation(mm) Av summer humid ity Av winter humid ity Av snow d ep th M aximum snow d ep th last 10yr W oomera Alma 16.5 E 23.26 S 1800 m 136.786 E 31.099 S 160 m 67.75W 23.00 S 4600-5100m 70.41 W 24.66 S 2635 m 70.73 W 29.25 S 2200-2400m 68.46 W 24.32 S 4300m 69.05 W 24.25 S 3100m g v mnt 500kx300k Soil 5 25 Ad elaid e State Vast Soil, rocks 2 16+3 Calama Chile Nearb y summits Soil, rocks 2 16+3 Antofag asta Chile Low slop es Soil, rocks 2 16+2 La Serena ? Larg e ? Too small 4? 16+3 Antofag asta 3? 16+3 Antofag asta 72 % <80 % >63 % Some None 90 % 75-80 % 82 % 62 % Some Very low 0.9xParanal? 0.9xParanal? Paranal? Paranal? 5/0C -5/-15C D:freq uent N:rare Days>25m/s each year 14C 11C 25 % 0 <10 mm 10-25 % <10 % 5 mm 2-3 9.5 63 % 54 % None 19 11 10 % 188 mm B. Khélifi 30-50 % 10-30 % Yes Yes Yes 10km Nearest hotels or lod g e (mins) Nearest restaurants (mins) Nearest hosp itals (mins) Sites - Parameters 27 11 25-50 % Electric p ower line W ater Hand y/M ob il serv ice Distance to hig h b and wid th internet Dang erous animals End emic d isease Scientific facilities Political stub ility CTA-South Paranal-La M ontura (ch) La Silla-Viscachas (ch) El Huesco (ch) HESS 15 15 15 HESS no no CANG AR OO HESS W oomera 40km 40km 200km,1500km Alma None 15 % 0 Site D (ch) None 6C -8C 1-9km/s ? <15mm 30-50 % 5-15 % ? 14C 5C 0-9km/s ? <10mm 25-30% 10-15% ? No Yes ? ? ? ? 200km 200km ~ 200km, ~ 1500km ESO or 200km ESO or 200km ~ 200km, ~ 700km 250km 250km 250, 1500km 220km 220km 220, 1500km No No ESO Stab le No Chag as? ESO Stab le No No No Stab le No Stab le VLT La Silla El Huesco Site D WG Calibration/Monitoring/Site Paris, 02/03/2007 Known Cherenkov sites • Thomas Highlands, Namibia • Tenerife Teide, La Palma • Himalaya Hanle (India) • Woomera (Australia) Good quality possible sites Useful for comparisons B. Khélifi WG Calibration/Monitoring/Site Paris, 02/03/2007 Sites for optical astronomy La Silla • Chilean sites – – – – La Silla - Atacama desert Paranal – 12 km from coast (VLT) La Montura … High quality atmospheric conditions Between 2.000 and 3.000 m a.s.l. Caution: available area B. Khélifi WG Calibration/Monitoring/Site Paris, 02/03/2007 Exploration of new sites • Based on satellite survey Erasmus Eramus Staden, 2001 – Cloud cover, water vapor – Data over 5 years Good fraction of clear nights Altitude above 3.500 m a.s.l. Very large area Can be isolated B. Khélifi clear nights • 5-10 candidates in Northern Argentina Chajnantor WG Calibration/Monitoring/Site Archibarca Catamarca 1st half Paris, 02/03/2007 Exploration of new sites (2) • On site explorations (12-2006) • On site measurements − Telescope: Newton with CCD cam. − U, V, B POCITOS Pocitos 74% N 67% 60% La Silla ALMA clear nights – E. Giraud, G. Vasileiadis, M. Gaczarzyk, T. Schweizer, A. Rovero, E. Colombo – 4 sites visited Erasmus S 24° 32.118’ 3722 m a.s.l. Plateau below ALMA site Chajnantor Sus7052 Antonio Pocitos Archibarca Tolar G. W 67° 4.363’ Catamarca Tolar Grande B. Khélifi WG Calibration/Monitoring/Site 1st half Paris, 02/03/2007 Conclusions • Big activity of the WG members to identify candidates literacy, reports on web, personal contacts, visits, measurements,… • Draft of the WG has been submitted (23 pages) • Good starting point for the Design Study Even if Northern sites are so few and other possibilities have not yet investigated (e.g. South Utah) • For the Design Study (Working Package 4): – Use long-term data from satellites and in-situ measurements – Identify site facilities (for the access and the building phase) B. Khélifi WG Calibration/Monitoring/Site Paris, 02/03/2007 Thank you to all for your contributions