List of All Tutorials
From CASA Guides
Data Reduction
ALMA Guides Main Page
- (ALMA) The protoplanetary disk source TW Hya at Band 7 (0.87 mm): TWHydraBand7
- CASA 3.4: TW Hya Calibration and Imaging
- CASA 3.3: TW Hya Calibration and Imaging
- (ALMA) The galaxy merger NGC 3256 at Band 3 (3 mm): NGC3256Band3
- CASA 3.4: NGC3256 Calibration and Imaging
- CASA 3.3: NGC3256 Calibration and Imaging
- (ALMA) Mosaic of the galaxy merger NGC 4038/4039 (Antennae) at Band 7 (0.87 mm): AntennaeBand7
- CASA 3.4: Antennae Calibration and Imaging
- CASA 3.3: Antennae Calibration and Imaging
- (ALMA) Mosaic of the protostellar cluster IRAS16293-2422 at Band 9: IRAS16293Band9
- CASA 3.4: IRAS16293 Calibration and Imaging
- CASA 3.3: IRAS16293 Calibration
- (ALMA) Notes on the calibration of Science Verification target BR1202-0725: File:BR1202 SV Band7 Calibration notes.pdf
EVLA Guides Main Page
- (EVLA) Supernova Remnant 3C391 : 6cm Polarimetry and Continuum Imaging, Mosaicking: dataset size 3.1GB
- (EVLA) Carbon Star IRC+10216: high frequency (36GHz), spectral line data reduction: dataset size 1.1GB
- CASA 3.4: IRC+10216 Calibration+Imaging
- CASA 3.3: IRC+10216 Calibration and Imaging
- (EVLA) Supernova G55.7 3.4: Wide-band, wide-field imaging; L-band (1-2 GHz): dataset size 14GB
- CASA 3.4: G55.7 Imaging
- CASA 3.3: G55.7 Imaging
- (EVLA) Supernova SN2010FZ: Wide-band, narrow-field imaging; C-band (5-7 GHz) dataset size: 2.9GB in size
- CASA 3.4: SN2010FZ Imaging
- CASA 3.3: SN2010FZ Imaging
- (EVLA) Calibrating an EVLA OSRO HI data set
- CASA 3.0: HI Calibration and Imaging
CARMA Tutorials Main Page
- (CARMA) Reducing a Spectral-Line mosaic (using CO J=1-0 in M99 (NGC4254) from CARMA STING, Rahman et al. 2010)
- CASA 3.2: Extracting data from MIRIAD and M99 Calibration, Imaging
SMA Tutorials Main Page
- (SMA) Mosaic Observation of an Infrared Dark Cloud in CO(2-1)
- CASA 3.2: IRDC Calibration, Imaging
Simulations
CASA 3.4 Simulations Main Page and CASA 3.3 Simulations Main Page
- Simulation guide for new users: Scale 30 Dor continuum to a greater distance
- Scaling M51 to z=0.1 and z=0.3
- How to simulate a Point Source or other simple model
- CASA 3.4: Component Models
- CASA 3.3: Component Models
- Simulating observations of dust in a nearby Protoplanetary disk
- CASA 3.4: Protoplanetary Disk
- CASA 3.3: Protoplanetary Disk
- Simulation of CO in nearby edge-on galaxy N891
- Simulating the effect of spatial filtering with Einstein's Face
- Simulating observations using the ALMA Compact Array
Guides for Specific Tasks and Applications
Flagging Data
Calibration
Imaging
Analysis
- Masking images for analysis
- How to rotate and slice a cube for pV diagrams
- Stacking Multiple Spectral Lines at Same Position