The duration of this training session will be about one hour. This will allow users to produce products of higher quality than the ones publicly available at the ALMA Science archive, as well as to tailor them to the specific requirements of their science projects. Throughout the tutorial participants will be guided on how to tweak different parameters of the pipeline tasks to e.g., improve the quality of the continuum baseline fit, to change channel widths, flag antennas, etc. In this training session participants will learn how to run the ALMA Science Pipeline to re-process SD data to fit their own scientific purposes. ALMA Interferometric data refers to observations obtained with either the ALMA 12-m Array or 7-m Array, while SD data refers to observations obtained with the 12-m dishes of the ALMA Total Power Array. The ALMA Science Pipeline is used for the automated calibration and imaging of ALMA interferometric and single-dish (SD) data. I-TRAIN #18: The ALMA Single-Dish Pipeline With interferometric data. The duration of each training session is about one hour, including a live demo and interactive Q&A.Ĭontact us by submitting a ticket to the ALMA HelpDesk (Department "General Queries") if you wish to provide your feedback on I-TRAIN.Īccess or subscribe to the calendar of sessions at Training session The sessions cover a wide range of topics of interest to the ALMA user community with the aim to help users gain expertise in working The European ARC Network organizes I-TRAIN, a regular series of Interactive Training in Reduction and Analysis of INterferometric data.
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