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First Light at Prompt7 (First Light at Prompt7 (Chart32Chart32))ChChilean ilean AAdvanced dvanced RRemote emote TTelescope 32“elescope 32“
operating at Cerro Tololo/Chile (CTIO)operating at Cerro Tololo/Chile (CTIO)
March 04, 2013 Johannes Schedler
ContentContentTeamTeam
Selection of LocationSelection of Location
Project historyProject history
Enclosure/DomeEnclosure/Dome
Telescope SetupTelescope Setup
Control philosophy and software Control philosophy and software
First resultsFirst results
LinksLinks
Our Chart32 TeamOur Chart32 Team Philipp KellerPhilipp Keller UNC (host) UNC (host) http://unc.edu/
http://astrooptik.com Dan Reichart Dan Reichart
Joshua HaislipJoshua Haislip
Aaron LaCluyzeAaron LaCluyze
Justin MooreJustin Moore
Konstantin BuchholdKonstantin Buchhold Johannes Schedler Johannes Schedlerhttp://www.spacephotos.de/ http://panther-observatory.com
Bernd Flach-Wilken Bernd Flach-Wilken http://www.spiegelteam.de/
Volker Wendel Volker Wendel http://www.spiegelteam.de/
Selection of Location at CTIOSelection of Location at CTIOGeographical location > 30° southGeographical location > 30° south
Elevation > high Elevation > high
Sky conditions ++Sky conditions ++
Darkness ++Darkness ++
Humidity > lowHumidity > low
Seeing ++Seeing ++
Clear nights ++Clear nights ++
Infrastructure ++Infrastructure ++
Costs > sharedCosts > shared
Decision for CTIO/UNC ChileDecision for CTIO/UNC ChileReliable infrastructureReliable infrastructure
Optimal sky conditions at 2200 mOptimal sky conditions at 2200 m
Continuous support availableContinuous support available
Dome construction done by UNCDome construction done by UNC
Operating costs taken by UNCOperating costs taken by UNC
Shared use between UNC and usShared use between UNC and us
Dark time for our teamDark time for our teamBright time for UNCBright time for UNC
Override by UNC any time by UNCOverride by UNC any time by UNCin case of special events (GRB)in case of special events (GRB)
Place of Chart32Place of Chart32
4 m Blanco Telescope
Weather conditionsWeather conditionsclear nights at CTIOclear nights at CTIO
Sky conditions at CTIOSky conditions at CTIOtypical mag 21.5-22typical mag 21.5-22
Project HistoryProject History20072007 First contacts in Chile with support of Daniel Verschatse:First contacts in Chile with support of Daniel Verschatse:
Cerro Armazones, then CTIO Cerro Armazones, then CTIO (Cerro Tololo Inter-American Observatory)(Cerro Tololo Inter-American Observatory)
20082008 „ „Go“ from UNC (University of North Carolina) at CTIOGo“ from UNC (University of North Carolina) at CTIO
20092009 Contract signed with UNC in March, fund raisingContract signed with UNC in March, fund raising dome construction plans prepared dome construction plans prepared
20102010 Final drawings ready, start of bid processFinal drawings ready, start of bid process
20112011 Erection of dome building (March-April)Erection of dome building (March-April)
Project HistoryProject History20122012 March: shipment of telescope equipment to ChileMarch: shipment of telescope equipment to Chile
20122012 November: commissioning (Philipp and Konstantin) >first light! November: commissioning (Philipp and Konstantin) >first light!
20132013 February: CCD camera back from repair, optimization February: CCD camera back from repair, optimization full remote operation and control possible full remote operation and control possible
EnclosureEnclosureDome Diameter 5 mDome Diameter 5 m
Avoid ground seeing:Avoid ground seeing:Telescope height 4.5 m from floorTelescope height 4.5 m from floor
Avoid dome seeing:Avoid dome seeing:Forced ventilation up to 5 m³/secForced ventilation up to 5 m³/sec
OpticsOpticsdesigned by Philipp Kellerdesigned by Philipp Keller
Classical cassegrainClassical cassegrain
Mirror: 0.81m SitallMirror: 0.81m Sitall
Focal length: 5.6 mFocal length: 5.6 m
3-lens Wynne corrector3-lens Wynne corrector
Corrected field: 150 mm (diffraction limited)Corrected field: 150 mm (diffraction limited)
OTAOTA
Open truss designOpen truss design
Robotic dust cover (mirror + baffle)Robotic dust cover (mirror + baffle)
Focusing by secondary mirrorFocusing by secondary mirror
Lasalle mirror supportLasalle mirror support
Remote collimationRemote collimation
MountMount
Equatorial fork mountEquatorial fork mount
Torque motors 200 Nm both axesTorque motors 200 Nm both axes
Encoder resolution 0.01 arc secEncoder resolution 0.01 arc sec
Pointing accuracy <5 arc secPointing accuracy <5 arc sec
Tracking accuracy <0.1 arc sec (5min)Tracking accuracy <0.1 arc sec (5min)
All cables through mountAll cables through mount
CCDCCD
Imager: FLI-16803 ProlineImager: FLI-16803 Proline
4096x4096 at 9 um4096x4096 at 9 um
8-pos FLI 50x50mm Filter wheel8-pos FLI 50x50mm Filter wheel
Resolution: 0.33“/pixelResolution: 0.33“/pixel
Field: 22.3‘ x 22.3‘ Field: 22.3‘ x 22.3‘
Guider: Lodestar at 49mm off axisGuider: Lodestar at 49mm off axis
CTIO
FirewallCTIO
Firewall
DatacenterLe SerenaDatacenterLe Serena
MicrowaveAntenna
MicrowaveAntenna
Internet
MicrowaveAntenna
MicrowaveAntenna
DatacenterCTIO
DatacenterCTIO
FX/TX Converter
FX/TX ConverterFibre Optic Link
Ethernetswitch
Ethernetswitch
IP WebcamIP Webcam
WirelessRouter
WirelessRouter
PC2Backup
PC2Backup
PC1Control
PC1Control
IP Boot ManagerIP Boot
Manager
IP Power switch
IP Power switch
CCD Powerstrip
CCD Powerstrip
TelescopeControllerTelescopeController
Dom
e LightD
ome Light
ScopeDomeController
ScopeDomeController
Dome Rails and ShutterDome Rails and Shutter
110V 60Hz
Ethernet
Scope CoversScope Covers
Dome FansDome Fans
WiFi Antenna
Data & Power Connections in Data & Power Connections in CHART32CHART32
SoftwareSoftware
Sequence Autoslew
Maxim DL
The Skyoptional
CCD
Auxiliaries:ScopedomeWatchdogSMS alert
Pinpoint
Developed by Philipp KellerDeveloped by Philipp Keller
Includes safety, dome and ventilation controlIncludes safety, dome and ventilation control
All sky pointing modelAll sky pointing model
Scheduler for automatedScheduler for automatedimagingimaging
MLPT tracking allows MLPT tracking allows unguided tracking up to unguided tracking up to 20 min20 min
Control via Autoslew/PinpointControl via Autoslew/Pinpoint
Deviation before Deviation before MLPT
All sky pointing model includedAll sky pointing model included
Scheduler for automated imagingScheduler for automated imaging
Control via Autoslew/PinpointControl via Autoslew/Pinpoint
First light image First light image (Nov 2012)(Nov 2012)
NGC253NGC253
10 min L10 min L
3 min RGB3 min RGB
100% crop100% crop
NGC3372 NB 460 min
FutureFuture
• High resolution planetary imaging with moveable pick-up mirrorHigh resolution planetary imaging with moveable pick-up mirror
• Cooperation with professional astronomersCooperation with professional astronomers
• Very long deep exposuresVery long deep exposures
LinksLinks
Chart32 Homepage http://chart32.deChart32 Homepage http://chart32.de
Philipp Keller Homepage http://astrooptik.comPhilipp Keller Homepage http://astrooptik.com
ASA Astrosysteme Austria http://www.astrosysteme.at/ASA Astrosysteme Austria http://www.astrosysteme.at/(Partnership with Philipp Keller)(Partnership with Philipp Keller)
Cerro Tololo Inter-American Observatory (CTIO) http://www.ctio.noao.edu/Cerro Tololo Inter-American Observatory (CTIO) http://www.ctio.noao.edu/
Johannes Schedler Homepage Johannes Schedler Homepage http://panther-observatory.comhttp://panther-observatory.com
Bernd Flach-Wilken/Volker Wendel Homepage Bernd Flach-Wilken/Volker Wendel Homepage http://www.spiegelteam.de/http://www.spiegelteam.de/
Konstantin Buchhold Homepage Konstantin Buchhold Homepage http://www.spacephotos.de/http://www.spacephotos.de/