ism3d

0.3.dev1

User Guide

Installation
Usage
Credits
History

Technical Specification/Notes

Parameter File Format
Keywords

Development

Maintance
Background
Design Goals
Acknowledgement
See also
Reference
ISM3D Dictionary
ISM3D call graph

Tutorials: Direct API Usage

ism3d.uvhelper: visibility imaging
ism3d.arts: model artificial sources in different shapes
ism3d.arts.lens: model artificial sources with gravitational lensing effects
ism3d.xyhelper.maskmoment: derive moment0/moment1 maps from spectral cubes

Benchmarking

Invert
Test the performance of the Image-to-MS-related modules

Tutorials: Modeling

Example BX610: perform model fitting using method=‘amoeba’ for the Band 4 Cycle 2 DataSet
Example BX610: perform model fitting using method=‘amoeba’ for the Band 4 Cycle 5 DataSet
Example BX610: perform model fitting using method=‘amoeba’ for the Band 6 Cycle 3 DataSet
Invert Visibility + Plot 1D spectra (may take a while)
Example BX610: perform model fitting using method=‘emcee’
Example HXMM01: test the MS-simulation modules

Tutorials: misc

Tutorials & Examples

Tutorials: Data Preparation

Example: GN20 (z~4 SMF) : Data Prep
Example: BX610 (High-z SFG) : Data Prep
Example: HXMM01 (High-z Merger)
Example GN20: perform imaging of CO 2-1 dataset
Example: BX610 (High-z SFG) : Data Imaging
Tutorials & Examples

API Reference

ism3d

ism3d

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ism3d.maths.stats »
ism3d.maths.stats.rng_seeded

ism3d.maths.stats.rng_seeded¶

ism3d.maths.stats.rng_seeded(seed=None)[source]¶: return a seeded RNG plus is_mkl mkl_random is preferrred over numpy.random

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