ALBA Synchrotron
'TheNational Radio Astronomy Observatory, Interferometry, and Synchrotron Radiation Interferometry at ALBA' C. Carilli 'A geometric interpretation of invariant phases in interferometry' N. Thyagarajan
When
Contact info
Laura Torino
Location
Marie S. Curie Room
Where
ALBA Synchrotron
'TheNational Radio Astronomy Observatory, Interferometry, and Synchrotron Radiation Interferometry at ALBA' C. Carilli
Abstract: I will discuss the facilities and science of the US National Radio Astronomy Observatory, with a focus on cosmic synchrotron sources. I will then present the concepts of interferometric imaging, and the application of non-redundant aperture masking and self-calibration using SRI to determine the size and shape of the ALBA synchrotron beam.
'A geometric interpretation of invariant phases in interferometry' N. Thyagarajan
Abstract: Phases in interferometry are a key element to reconstructing the source properties. There are several situations when the phases are poorly constrained due to corrupting effects in the propagation medium and/or the instrument, or not constrained at all. Examples include radio interferometry, X-ray crystallography, seismology, etc. Image reconstruction in these situations have been critically helped by a special class of phases (called closure phases in radio interferometry) that are preserved despite the phase corruptions introduced during the measurement process and therefore encode true morphological information about the object of interest. I will discuss the geometric interpretation of closure phase and its invariance, which until recently had remained unclear.