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The GLORIA demonstrator experimentThe GLORIA demonstrator experiment
Ariel MajcherAriel MajcherNational Centre for Nuclear ResearchNational Centre for Nuclear Research
Warsaw, PolandWarsaw, Poland
XXXII IEEE-SPIE Joint Symposium Wilga 2013, May 29 2013XXXII IEEE-SPIE Joint Symposium Wilga 2013, May 29 2013
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Outline
● GLORIA project● Demonstrator experiments● Pi of the Sky data ● Luiza framework● Results● Conclusions
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GLORIA● FP7 project
http://gloria-project.eu/
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GLORIA● 13 partners, 17 robotic telescopes
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GLORIA● Project goals:
– Create free and open-access network of robotic telescopes for citizen science
– Develop Web 2.0 environment for easy access to telescopes and other network resources
– Design tools for doing „on-line” experiments (observations) and „off-line” experiments (data analysis) new quality: observations possible 24/24
– Develop full framework for doing research with robotic telescopes, allowing also for easy integration with GLORIA network
– Outreach in science and astronomy
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GLORIA structure
RT control interface
On-line experiment
interface
Off-line experiment
interface
Robotic Telescope Controler
Observation Time
Scheduler
Data Access and Analysis
Server
RT data storage
GLORIA data
storage
GLORIA user
database
CPUs
RT and its infrastructure
GLORIA observation database
control
data
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GLORIA experiments● GLORIA should allow users to perform various
on-line and off-line experiments in the network● To present network capabilities and
performance of the developed tools demonstrator experiments are created:
– On-line demonstrators for telescope teleoperation and scheduled sky observations
– Off-line demonstrators for simple (education level) and more advanced (research) image analysis
http://users.gloria-project.eu/
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On-line demonstrator● Sun observations with TAD (Tenerife)
http://users.gloria-project.eu/
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Pi of the Sky project● Leading Polish research units:
– National Centre for Nuclear Research– Center for Theoretical Physics, PAS– Faculty of Physics, University of Warsaw
in cooperation with other institutes● Search for optical signal of GRBs
– wide field sky monitoring with high temporal resolution and automatic detection
● Study other variable objects – supernovae, novae, flare stars,variable stars
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Pi of the Sky projectFirst unit installed in LCO Chile,
moved to San Pedro de Atacama in 2011● 2 CCD cameras 2000×2000 pixels● Canon f = 85mm, d = f/1.2 lenses● Common FoV 20°×20° ● 10 s exposures, ~11m range
13m for 20 coadded frames
Second unit near Huelva, Spain● 4 CCD cameras installed in 2010, 12 to be installed 2013
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Pi of the Sky data● Off-line demonstrator experiment
400 images selected from the telescope in Chile
4 overlapping observation fields considered
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Luiza framework● Analysis tool based on the following approach:
– Data (image) analysis should be divided into small, well defined steps (implemented as so called processors)
– Each step has to have well defined input and output data structure
– By defining universal data structures we make sure that different processors can be connected in a single analysis chain, i.e. exchange data and analysis results
– Processor configuration and their parameters can be set by user at run time in a simple steering file
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Luiza frameworkData structures● GloriaFitsImage - class for storing FITS images
– uses fitsio library for reading and storing images– basic methods for image manipulation
● GloriaFitsTable - class for storing other data– flexible (integers, floats, strings, vectors of int/float)
● GloriaDataContainer – internal storage class– Images and tables stored in “collections”– Each collection has a unique name (string)
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Luiza framework● Steering file
– Allows user to create analysis chain by selecting processors and defining their order
– Allows to define input-output streams and set other processor parameters
● Each Luiza processor gets a pointer to global GloriaDataContainer
– Can create new collection when reading data from file– Can analyse data stored in memory– Can save analysis results to output files
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Data structure
initialization
ControlOf
ProcessingSequence
(image loop)
Luiza frameworkProcessing concept (example)
Luiza Processor manager
Steering file(user input)
Darks
Flats
Raw images
Corrected images
GloriaData
ContainerDark frame
reader
Flat frame reader
Raw image reader
Frame normalizer
Object finder
Astrometry
Image storage
Telescopeparameters
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Luiza framework● General tools
– Input and output of FITS image files (using fitsio)– Input and output of data tables to FITS or text files– Image viewer based on CERN root package
● Image processing tools– Simple geometry operations– Image stacking or averaging– Image normalization dark/bias subtraction and flat correction– Star position & brightness determination– Implementation of astrometry.net– Light curve reconstruction
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Off-line demonstrator● Preprocessing of Pi of the Sky data
– Image stacking, dark subtraction, flat correction– object finding and astrometry– object lists stored to binary FITS tables
● Final analysis - light curve reconstruction– coordinates specified by user– object's brightness normalized to catalogue stars– normalization uncertainty calculated frame by frame– resulting light curve displayed in web interface
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Results● Tests on selected constant stars
Estimated calibration magnitudo distribution uncertainty ∆
Before (dashed) and after (solid) the quality cut ∆ < 0.1
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Results● Light curves of selected variables
W Gem, classical cepheid (delta Cep type) V1388 Ori, eclipsing binary of Algol type (detached)
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Results● Light curves of selected variables
RS Ori, classical Cepheid (delta Cep type) CR Gem, semi-regular variable
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Conclusions● GLORIA network opened for users● Efficient and flexible analysis framework developed ● Pi of the Sky data used for off-line demonstrator● Demonstrator implemented, should be released soon
visit http://users.gloria-project.eu/● Luiza available
– From GLORIA project SVN http://sourceforge.net/projects/gloriaproject/(go to misc → Tools → Analysis)
– From Luiza documentation web page http://hep.fuw.edu.pl/u/zarnecki/gloria/luiza/doc/html/index.html