Publication | Open Access
SearchCal: a virtual observatory tool for searching calibrators in optical long baseline interferometry
155
Citations
25
References
2006
Year
Long baseline interferometry requires fringe contrast calibration to derive true visibility and astrophysical parameters, and selecting suitable calibration stars is essential for achieving the precision of instruments such as the VLTI. The authors developed SearchCal, a software that builds an evolving catalog of calibrator stars within user‑defined angular distance and magnitude limits around a target, with a first version for bright objects (V ≤ 10, K ≤ 5). SearchCal queries CDS star catalogs via web requests, supplies necessary data for calibrator selection, computes missing photometry to 0.1 mag accuracy and angular diameters to better than 10 % precision, and calculates each star’s squared visibility based on observation wavelength and maximum baseline, integrating.
In long baseline interferometry, the raw fringe contrast must be calibrated to obtain the true visibility and then those observables that can be interpreted in terms of astrophysical parameters. The selection of suitable calibration stars is crucial for obtaining the ultimate precision of interferometric instruments like the VLTI. We have developed software SearchCal that builds an evolutive catalog of stars suitable as calibrators within any given user-defined angular distance and magnitude around the scientific target. We present the first version of SearchCal dedicated to the bright-object case V<=10; K<=5). Star catalogs available at the CDS are consulted via web requests. They provide all the useful information for selecting of calibrators. Missing photometries are computed with an accuracy of 0.1 mag and the missing angular diameters are calculated with a precision better than 10%. For each star the squared visibility is computed by taking the wavelength and the maximum baseline of the foreseen observation into account.} SearchCal is integrated into ASPRO, the interferometric observing preparation software developed by the JMMC, available at the address: http://mariotti.fr.
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