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

机译:N带VLTI-MIDI的差分相位延迟观察

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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 micron 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:本研究侧重于VLTI / MIDI仪器中光谱通道之间的差动干涉相位的观察测量。将目标恒星的测量与理论预测进行比较,以便研究分散在潮湿空气中对n条带(约10微米波长)的差分相位测量的影响。在稳定的环境条件下校准后,在校准后实现了1度RMS相位误差的精度,但如果观察之间存在湿度波动,则这种精度会降低。需要稳定和/或监测VLTI管道和隧道中的环境条件,以便使用MIDI实现最佳的差异相位性能。发现测量的差相与基于HITRAN数据库的空气折射率的模型一致。

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