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Published byWarren Richard Modified over 9 years ago
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An Introduction to Simdata Scott Schnee (NRAO) Victoria Workshop – Jan 18, 2011
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What is Simdata Good For? Number of antennas Antenna configuration Length of observation Noise Take a model image and find out how it would look if observed with ALMA
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Model Image 30Dor Spitzer IRAC 8um image from SAGE
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Model Image Resized and now at 230 GHz
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Fourier Transforms of Images From http://carmilumban-ap186.blogspot.com
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Scales Measured by ES Configuration Antenna Placement uv-coverage synthesized beam 2 hour observation
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Scales Measured by FS Compact Antenna Placement uv-coverage synthesized beam 2 hour observation
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Scales Measured by FS Extended Antenna Placement uv-coverage synthesized beam 2 hour observation
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Model Image in ES Configuration Model ImageConvolved Model“Observed” Image 2 hour observation
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Model Image in FS Compact Model ImageConvolved Model“Observed” Image 2 hour observation
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Model Image in FS Extended Model ImageConvolved Model“Observed” Image 2 hour observation
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Basic Simdata Inputs Image / model of target Observing time Antenna configuration
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Basic Simdata Inputs
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FITS Image Basics Coordinates Brightness Observing Frequency Resolution (angular and spectral) Polarization (if needed)
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modifymodel modifymodel = True skymodel = “30dor.fits” inbright = ”0.1mJy/pixel” indirection = "J2000 10:00:00 -40:00:00” incell = "0.25arcsec” incenter = "230GHz” inwidth = '2GHz'
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setpointings integration = '600s’ mapsize = "” pointingspacing = ""
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predict repodir = os.getenv("CASAPATH").split(' ')[0] antennalist = repodir+"/data/alma/simmos/alma.early.250m.cfg"
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Simdata Output analyze = True showarray = True showconvolved = True showdifference = False showfidelity = False
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Simdata Output
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Simdata Output - Viewer
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Other Simdata Options Thermal Noise thermalnoise = ‘tsys-atm’ image = True vis=‘$project.noisy.ms’
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Other Simdata Options Thermal Noise Convolved ModelThermal NoiseNo Thermal Noise
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Other Simdata Options Phase Noise Convolved ModelNo Phase NoisePhase Noise
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Other Simdata Options Phase Noise Create measurement set with simdata Use the “toolkit” to add phase noise – http://casa.nrao.edu/docs/CasaRef/CasaRef.html http://casa.nrao.edu/docs/CasaRef/CasaRef.html – http://casaguides.nrao.edu/index.php?title=Corrupt http://casaguides.nrao.edu/index.php?title=Corrupt – sm.openfromms("simPN.ms") – sm.settrop(mode='screen',pwv=1.0,deltapwv=0.15) – sm.corrupt() – sm.done() Use clean (in CASA) to make the image
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Your Turn Find a fits file of an object you want to image Use simdata to see how it would look if observed with ALMA – Rescale image if necessary – Try different antenna configurations – Add noise if interested Don’t be afraid to ask for help!
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