EVLA Wide-Band Wide-Field Imaging: G55.7 3.4: Difference between revisions

Latest revision as of 17:57, 12 November 2015

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+#REDIRECT [[EVLA Wide-Band Wide-Field Imaging: G55.7 3.4-CASA4.4]]
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-== BEFORE YOU START==
-Make sure you have done the steps described at [[Initial_instructions_for_2010| the initial instructions for the 2010 Synthesis Workshop Tutorials]].
--->
-== Overview ==
-This CASA Guide describes the flagging, calibration, and imaging of the supernova remnant [http://simbad.u-strasbg.fr/simbad/sim-id?Ident=G55.7+3.4&NbIdent=1&Radius=2&Radius.unit=arcmin&submit=submit+id G55.7+3.4.].  The data were taken on August 23, 2010, in the first D-configuration for which the new wide-band capabilities of the WIDAR correlator were available.  The 8-hour-long observation includes all available 1 GHz of bandwidth in L-band, from 1-2 GHz in frequency.
-The measurement set which provides a starting point for this Guide has been imported from the SDM file set and time-averaged to 10 seconds.  Both of these options are available from the NRAO data archive, and since this operation can be relatively time-consuming,  The original data set