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dc.contributor.authorMonnier, JD
dc.contributor.authorBerger, J-P
dc.contributor.authorLe Bouquin, J-B
dc.contributor.authorTuthill, PG
dc.contributor.authorWittkowski, M
dc.contributor.authorGrellmann, R
dc.contributor.authorMüller, A
dc.contributor.authorRenganswany, S
dc.contributor.authorHummel, C
dc.contributor.authorHofmann, K-H
dc.contributor.authorSchertl, D
dc.contributor.authorWeigelt, G
dc.contributor.authorYoung, J
dc.contributor.authorBuscher, D
dc.contributor.authorSanchez-Bermudez, J
dc.contributor.authorAlberdi, A
dc.contributor.authorSchoedel, R
dc.contributor.authorKöhler, R
dc.contributor.authorSoulez, F
dc.contributor.authorThiébaut, É
dc.contributor.authorKluska, J
dc.contributor.authorMalbet, F
dc.contributor.authorDuvert, G
dc.contributor.authorKraus, S
dc.contributor.authorKloppenborg, BK
dc.contributor.authorBaron, F
dc.contributor.authorde Wit, W-J
dc.contributor.authorRivinius, T
dc.contributor.authorMerand, A
dc.date.accessioned2016-06-13T12:09:50Z
dc.date.issued2014-07-24
dc.description.abstractHere we present the results of the 6th biennial optical interferometry imaging beauty contest. Taking advantage of a unique opportunity, the red supergiant VY CMa and the Mira variable R Car were observed in the astronomical H-band with three 4-telescope configurations of the VLTI-AT array using the PIONIER instrument. The community was invited to participate in the subsequent image reconstruction and interpretation phases of the project. Ten groups submitted entries to the beauty contest, and we found reasonable consistency between images obtained from independent workers using quite different algorithms. We also found that significant differences existed between the submitted images, much greater than in past beauty contests that were all based on simulated data. A novel crowd-sourcing" method allowed consensus median images to be constructed, filtering likely artifacts and retaining real features." We definitively detect strong spots on the surfaces of both stars as well as distinct circumstellar shells of emission (likely water/CO) around R Car. In a close contest, Joel Sanchez (IAA-CSIC/Spain) was named the winner of the 2014 interferometric imaging beauty contest. This process has shown that new comers" can use publicly-available imaging software to interpret VLTI/PIONIER imaging data, as long as sufficient observations are taken to have complete uv coverage { a luxury that is often missing. We urge proposers to request adequate observing nights to collect sufficient data for imaging and for time allocation committees to recognise the importance of uv coverage for reliable interpretation of interferometric data. We believe that the result of the proposed broad international project will contribute to inspiring trust in the image reconstruction processes in optical interferometry.en_GB
dc.identifier.citationVol. 9146, article 91461Qen_GB
dc.identifier.doi10.1117/12.2057312
dc.identifier.urihttp://hdl.handle.net/10871/22034
dc.language.isoenen_GB
dc.publisherSociety of Photo-optical Instrumentation Engineers (SPIE) -en_GB
dc.titleThe 2014 interferometric imaging beauty contesten_GB
dc.typeArticleen_GB
dc.date.available2016-06-13T12:09:50Z
dc.descriptionThis is the final version of the article. Available from SPIE via the DOI in this record.en_GB
dc.descriptionFrom Conference Volume 9146: Optical and Infrared Interferometry IV. Jayadev K. Rajagopal; Michelle J. Creech-Eakman; Fabien Malbet. Montréal, Quebec, Canada, June 22, 2014en_GB
dc.identifier.journalProceedings of SPIEen_GB


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