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- 16:13, 10 May 2024 ALMA Renormalization Correction (hist | edit) [1,885 bytes] Ekeller (talk | contribs) (Created page with "== Applying renormalization corrections to data == ALMA observations of sources with strong line emission are affected by amplitude calibration issues caused by the ALMA normalization strategy, as described in the following Knowledgebase Articles: [https://help.almascience.org/kb/articles/what-are-the-amplitude-calibration-issues-caused-by-alma-s-normalization-strategy] and [https://help.almascience.org/kb/articles/what-errors-could-originate-from-the-correlator-spectral...")
- 12:47, 30 April 2024 VLA Flagging Intro Tutorial (hist | edit) [84,961 bytes] Bsvoboda (talk | contribs) (Copy page from 6.5.4 topical flagging CASA guide)
- 15:34, 21 March 2024 ACA Simulation CASA 6.5.4 (hist | edit) [10,910 bytes] Estarr (talk | contribs) (Created page with "Category: Simulations The commands in this guide have also been verified to work in CASA version 5.6.1. To create a script of the Python code on this page see Extracting scripts from these tutorials. __NOTOC__ == ALMA 12m + ACA + Total Power == We can simulate ALMA observations that use the main array of 12 m antennas augmented by the ACA and Total Power antennas by generating simulated observations for each component separately, and then combining the Measure...")
- 11:42, 1 March 2024 VLA CASA Flagging-CASA6.5.4 (hist | edit) [89,142 bytes] Earzaga (talk | contribs) (Created page with " "This CASA Guide is for Version 6.4.1 of CASA, and was last checked with CASA 6.5.4." * '''This CASA guide is designed for CASA 6.4.1''' * '''This CASA Guide is for the monolithic, not the modular pip-wheel version, version 6.4.1 of CASA that includes the VLA pipeline.''' * Printing Disclaimer: When printing, CASA commands in this guide may be cropped depending on your web browser text size and printer settings. <div style="background-color: #CCFF99;"> Last checked...")
- 14:06, 29 February 2024 MG0414+0534 P-band Spectral Line Tutorial - CASA 6.5.4 (hist | edit) [67,458 bytes] Tcandela (talk | contribs) (Created page with "<!--By Bjorn Emonts--> <b>This CASA Guide is for Version 6.5.4 of CASA.</b> {| class="wikitable" |- | style="background: red; color: white;" | '''DISCLAIMER''' |- | The following guide is for users who are experts in data reduction using CASA. If you are a beginner or novice user, please review other CASA guides found at [https://casaguides.nrao.edu/index.php/Karl_G._Jansky_VLA_Tutorials VLA Tutorials]. |} == Overview == This tutorial describes how to use CASA 6.5....")
- 16:28, 28 February 2024 Imaging Prep CASA 6.1.1 (hist | edit) [22,787 bytes] Tashton (talk | contribs) (Created page with "== Imaging Prep Workflow == Commands for this page can be found in scriptForImagingPrep_template.py available on [https://github.com/aakepley/ALMAImagingScript github]. center|frame|1200px ''Use the Imaging Prep workflow to determine which sections of this guide are applicable to your dataset.'' == Splitting off the calibrated data (Pipeline Calibration) == If your measurement set (ms) is pipeline calibrated, use this step to split off th...")
- 16:10, 28 February 2024 ADMIT Products and Usage CASA 5.4.0 (hist | edit) [15,726 bytes] Tashton (talk | contribs) (Making new version of CASA 5.4 version of ADMIT installation/usage instructions)
- 19:32, 22 February 2024 Protoplanetary Disk Simulation - VLA-CASA6.5.4 (hist | edit) [46,897 bytes] Tseelig (talk | contribs) (Created page with "== Overview == The following tutorial shows how to adopt typical parameters for simulating Karl G. Jansky VLA data. We will use the same image as the [https://casaguides.nrao.edu/index.php?title=Protoplanetary_Disk_Simulation_(CASA_5.4) ALMA tutorial Protoplanetary Disk Simulation]. Follow this link to obtain the [https://casa.nrao.edu/Data/EVLA/simulation/ppdisk672_GHz_50pc.fits protoplanetary disk model image]. Model images are in units of Jy/pixel. Other simulation o...")
- 17:11, 22 February 2024 VLA Data Combination-W49A-CASA6.5.4 (hist | edit) [30,317 bytes] Jkhor (talk | contribs) (Created page with "''This CASA Guide is for Version 6.5.4 of CASA'' == Introduction == A perfect image requires measurement of all spatial scales, which is equivalent to filling in the complete uv plane. Unfortunately, this can never be achieved with an aperture synthesis interferometer, although a large number of baselines, long integration times, and multi-frequency-synthesis are all good approaches to increase the uv-coverage. One method to obtain more baselines is to observe in diffe...")
