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Differential phase delay observations with VLTI/MIDI at N-band

机译:在N波段使用VLTI / MIDI进行差分相位延迟观察

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This investigation focuses on observational measurements of the differential interferometric phase between spectral channels in the VLTI/MIDI instrument. Measurements of target stars are compared with theoretical predictions in order to investigate the effects of dispersion in humid air on differential phase measurements at N band (~ 10 μm wavelength). An accuracy of 1 degree RMS phase error is achieved after calibration during stable environmental conditions, but this accuracy is degraded if there are fluctuations in humidity between observations. Stabilisation and/or monitoring of the environmental conditions in the VLTI ducts and tunnels will be required in order to achieve the best differential phase performance with MIDI. The measured differential phases are found to be consistent with a model for the refractive index of air based on the HITRAN database.
机译:这项研究的重点是在VLTI / MIDI仪器中频谱通道之间的差分干涉相位的观测测量。将目标恒星的测量值与理论预测值进行比较,以研究潮湿空气中的色散对N波段(〜10μm波长)处的相位差测量的影响。在稳定的环境条件下进行校准后,可以达到1度RMS相位误差的精度,但是如果观测之间的湿度存在波动,则该精度会降低。为了使MIDI达到最佳差分相位性能,将需要稳定和/或监视VLTI管道和隧道中的环境条件。发现基于HITRAN数据库,测得的微分相位与空气折射率模型一致。

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