ALMA SIS14: Difference between revisions
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= Overview = | |||
= Data Description = | |||
== | = Individual Lessons = | ||
=== Getting Oriented in CASA === | |||
We'll begin by getting you oriented in CASA. | |||
* Your first task and script | * Your first task and script | ||
* Orienting yourself with a new data set | * Orienting yourself with a new data set | ||
* Basic phase and amplitude calibration | === Calibrating Data === | ||
* | |||
* | Next we'll look at how we calibrate data. | ||
* Flux calibration | |||
* | * The three columns and basic calibration flow | ||
* [[ALMA_SIS14_apcal|Basic phase and amplitude calibration]] | |||
* [[ALMA_SIS14_applycal|Applying calibrations]] | |||
* [[ALMA_SIS14_fluxcalqso|Flux calibration using a quasar]] | |||
* [[ALMA_SIS14_fluxcalplanet|Flux calibration using a solar system body]] | |||
* [[ALMA_SIS14_bandpass|Bandpass calibration]] | |||
=== Flagging Data === | |||
A large part of the human input to data reduction comes from identifying problematic data, which is usally removed from the data set in a process called "flagging." | |||
* Basic flagging | * Basic flagging | ||
* Basic data inspection | * Basic data inspection | ||
== More | === Manipulating Data === | ||
* Splitting and averaging data | |||
* Manipulating the three columns | |||
* Combining several data sets | |||
=== Imaging === | |||
* Demonstrating the effect of calibration - your first imaging example | |||
* Basic continuum imaging | |||
* Basic line imaging | |||
* UV continuum subtraction | |||
=== Self-Calibration === | |||
* Basic self-calibration | |||
* Averaging in self-calibration | |||
* Self-calibration tips and tricks | |||
=== Analysis === | |||
* Derive image statistics | |||
* Make moment maps | |||
* Fit a gaussian | |||
* Inspection using the CASA viewer | |||
= More Resources = | |||
Latest revision as of 19:37, 26 February 2014
Overview
Data Description
Individual Lessons
Getting Oriented in CASA
We'll begin by getting you oriented in CASA.
- Your first task and script
- Orienting yourself with a new data set
Calibrating Data
Next we'll look at how we calibrate data.
- The three columns and basic calibration flow
- Basic phase and amplitude calibration
- Applying calibrations
- Flux calibration using a quasar
- Flux calibration using a solar system body
- Bandpass calibration
Flagging Data
A large part of the human input to data reduction comes from identifying problematic data, which is usally removed from the data set in a process called "flagging."
- Basic flagging
- Basic data inspection
Manipulating Data
- Splitting and averaging data
- Manipulating the three columns
- Combining several data sets
Imaging
- Demonstrating the effect of calibration - your first imaging example
- Basic continuum imaging
- Basic line imaging
- UV continuum subtraction
Self-Calibration
- Basic self-calibration
- Averaging in self-calibration
- Self-calibration tips and tricks
Analysis
- Derive image statistics
- Make moment maps
- Fit a gaussian
- Inspection using the CASA viewer
