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ASCL Code Record

[ascl:2301.006] Self-cal: Optical/IR long-baseline interferometry

Self-cal produces radio-interferometric images of an astrophysical object. The code is an adaptation of the self-calibration algorithm to optical/infrared long-baseline interferometry, especially to make use of differential phases and differential visibilities. It works together with the Mira image reconstruction software and has been used mainly on VLTI data. Self-cal, written in Yorick, is also available as part of fitsOmatic (ascl:2301.005).

Code site:
https://forge.oca.eu/trac/fitOmatic/wiki/self-cal
Used in:
https://ui.adsabs.harvard.edu/abs/2015A%2526A...577A..51M https://ui.adsabs.harvard.edu/abs/2011A%2526A...529A.163O
Described in:
https://ui.adsabs.harvard.edu/abs/2011A%2526A...526A.107M
Bibcode:
2023ascl.soft01006M

Views: 973

ascl:2301.006
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