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The 2014 Interferometric Imaging Beauty Contest

机译:2014年干涉成像美容大赛

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Here 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.
机译:在这里,我们展示第六届双年度光学干涉成像选美大赛的结果。利用一个独特的机会,使用PIONIER仪器在VLTI-AT阵列的三个4倍望远镜配置下,在天文H波段观察到了红色超巨型VY CMa和Mira可变R Car。邀请社区参加该项目的后续图像重建和解释阶段。十个小组向选美比赛提交了参赛作品,我们发现使用完全不同的算法从独立工作人员获得的图像之间具有合理的一致性。我们还发现,提交的图像之间存在显着差异,这比以往所有基于模拟数据的选美比赛要大得多。一种新颖的“众包”方法允许构建共识中值图像,过滤可能的伪像并保留“真实特征”。我们确定地检测到了R Car周围的两颗恒星表面以及发射(可能是水/ CO)的不同星际壳(包括水/ CO)上的强斑。在一次激烈的比赛中,乔尔·桑切斯(IAA-CSIC /西班牙)被评为2014年干涉成像选美大赛的获胜者。该过程表明,“新来者”可以使用公开可用的成像软件来解释VLTI / PIONIER成像数据,只要进行足够的观察即可获得完整的uv覆盖率-这种奢侈品经常会丢失。我们敦促提议者要求进行适当的观察之夜,以收集足够的数据进行成像,并要求时间分配委员会认识到uv覆盖对于可靠解释干涉数据的重要性。我们认为,拟议的广泛国际项目的结果将有助于激发人们对光学干涉术中图像重建过程的信任。

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