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An Introduction to Simdata Scott Schnee (NRAO) AAS Splinter Meeting – Jan 12, 2011
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An Introduction to Simdata

Jan 23, 2016

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An Introduction to Simdata. Scott Schnee (NRAO) AAS Splinter Meeting – Jan 12, 2011. What is Simdata Good For?. Take a model image and find out how it would look if observed with ALMA. Number of antennas Antenna configuration Length of observation Noise *. Thermal Noise Phase Noise. - PowerPoint PPT Presentation
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Page 1: An Introduction to Simdata

An Introduction to Simdata

Scott Schnee (NRAO)

AAS Splinter Meeting – Jan 12, 2011

Page 2: An Introduction to Simdata

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

• Thermal Noise

• Phase Noise

Page 3: An Introduction to Simdata

3

Simdata is a versatile tool within CASA

To learn more:• Go through online simdata guides–http://casaguides.nrao.edu/

• Go to one of our workshops or tutorials–http://science.nrao.edu/alma/

training.php

Page 4: An Introduction to Simdata

30Dor from Spitzer IRAC 8μm from SAGE Resized and now at 230 GHz

Page 5: An Introduction to Simdata

Fourier Transforms of Images

From http://carmilumban-ap186.blogspot.com

Page 6: An Introduction to Simdata

Scales Measured in Early ScienceAntenna Placement uv-coverage synthesized beam

2 hour observation

Point Spread Function

bmaj = 1.0

bmin = 0.9

Page 7: An Introduction to Simdata

Full Science 12m Array - Compact

2 hour observation

Antenna Placement uv-coverage synthesized beam

bmaj = 1.1bmin =

0.96

Note lower sidelobes

Page 8: An Introduction to Simdata

Model: Early Science Configuration

Model Image Convolved Model

“Observed” Image

2 hour observation

Page 9: An Introduction to Simdata

Model: Full Science 12m Array - Compact

Model Image Convolved Model

“Observed” Image

2 hour observation Large scale emission: Observe with ACA and possibly TPA

Page 10: An Introduction to Simdata

Basic Simdata Workflow

• Start CASA • Input image file into Simdata• Predict what ALMA would see using

Simdata• Compare ALMA image with input

image

Page 11: An Introduction to Simdata

Basic Simdata Inputs

• Image / model of target• Observing time• Antenna configuration

Page 12: An Introduction to Simdata

Basic Simdata Inputs

Parameters that can be changed

Current values of parametersExplanation of what the parameters are

Page 13: An Introduction to Simdata

Basic Simdata Inputs

Page 14: An Introduction to Simdata

Model Input FITS FileHeader must include:• Coordinates• Brightness units• Observing frequency• Pixel Scale (angular and spectral)• Polarization (if needed)• OR: Modify FITS image within

Simdata

Page 15: An Introduction to Simdata

predict

• repodir = os.getenv("CASAPATH").split(' ')[0]• antennalist = repodir+"/data/alma/simmos/alma.early.250m.cfg"

Page 16: An Introduction to Simdata

Simdata Output

Page 17: An Introduction to Simdata

Simdata Output - Viewerhttp://casa.nrao.edu/CasaViewerDemo/casaViewerDemo.html

Page 18: An Introduction to Simdata

Your Turn• Download CASA

–http://casa.nrao.edu/• Find/create an image of what you will

observe• Use Simdata to see how it would look

if observed with ALMA• Learn more

–http://casaguides.nrao.edu –http://science.nrao.edu/alma/

training.php