The close circumstellar environment of the semi-regular S-type star pi1

Details The close circumstellar environment of the semi-regular S-type star pi1 The close circumstellar environment of the semi-regular S-type star pi1

Feb 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008ycat..34820561s&link_type=abstract

VizieR On-line Data Catalog: J/A+A/482/561. Originally published in: 2008A&A...482..561S

Physics

Interferometry, Stars: Variable

Scientific paper

All the data products are stored in the FITS-based, optical interferometry data exchange format (OI-FITS), described in Pauls et al. (2005PASP..117.1255P). The OI Exchange Format is a standard for exchanging calibrated data from optical (visible/infrared) stellar interferometers. The standard is based on the Flexible Image Transport System (FITS), and supports storage of the optical interferometric observables including visibilities and differential phases. Several routines to read and write this format in various languages can be found in: Webpage http://www.mrao.cam.ac.uk/research/OAS/oi_data/oifits.html
(2 data files).

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