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The HPOL Spectropolarimeter at Ritter Observatory

机译:里特天文台的HPOL分光仪

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The HPOL spectropolarimeter, previously operated by the University of Wisconsin at Pine Bluff Observatory (PBO), has been restored and relocated to the University of Toledo's Ritter Observatory. We achieved first light with HPOL at Ritter Observatory on 2012 March 11. We present a detailed instrument description of HPOL in its current configuration at Ritter Observatory, and a description of the standard observing procedure. We performed frequent observations of unpolarized standard stars to calibrate the instrumental polarization. We present polarimetric calibration results for observations spanning 2012 March 11 to 2013 May 2. Our calibration work shows that the systematic uncertainties of observations obtained with HPOL at Ritter Observatory are comparable to, and sometimes outperform, the systematic uncertainties obtained at PBO. We have successfully recommissioned the HPOL spectropolarimeter at Ritter Observatory, making it once again available for ongoing science observations.
机译:以前由威斯康星大学派恩布拉夫天文台(PBO)运营的HPOL分光旋光仪已经恢复并搬迁到托莱多大学里特天文台。我们于2012年3月11日在Ritter天文台用HPOL取得了第一眼光。我们对非极化标准星进行了频繁观察,以校准仪器极化。我们将提供2012年3月11日至2013年5月2日之间观测值的极化校准结果。我们的校准工作表明,在Ritter天文台使用HPOL获得的观测结果的系统不确定性与在PBO获得的系统不确定性相当,有时甚至优于。我们已经成功地在Ritter天文台重新启用了HPOL分光仪,使其可以再次用于正在进行的科学观测。

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