论文标题

南希·格雷斯·罗马太空望远镜冠冕仪器观察校准计划

Nancy Grace Roman Space Telescope Coronagraph Instrument Observation Calibration Plan

论文作者

Zellem, Robert T., Nemati, Bijan, Gonzalez, Guillermo, Ygouf, Marie, Bailey, Vanessa P., Cady, Eric J., Colavita, M. Mark, Hildebrandt, Sergi R., Maier, Erin R., Mennesson, Bertrand, Payne, Lindsey, Zimmerman, Neil, Belikov, Ruslan, De Rosa, Robert J., Debes, John, Douglas, Ewan S., Girard, Julien, Groff, Tyler, Kasdin, Jeremy, Lowrance, Patrick J., Macintosh, Bruce, Ryan, Daniel, Weisberg, Carey

论文摘要

NASA的下一个旗舰任务Nancy Grace Roman Space望远镜是一款2.4米的天文台,可在2027年5月之前发射。罗马具有两种乐器:宽场成像器和Coronagraph仪器。罗马的Coronagraph是一项技术演示,将直接成像的当前功能推向较小的对比度($ \ sim $ 10 $^{ - 9} $)和内部工作角度(3〜 $λ$/d)。为了达到这一高度,必须校准罗马冠冕数据,以消除尽可能多的潜在错误来源。在这里,我们介绍了Nancy Grace Roman Space Coronagraph仪器观察校准计划的详细概述,包括识别潜在的误差源以及如何通过天上的校准来减轻它们。

NASA's next flagship mission, the Nancy Grace Roman Space Telescope, is a 2.4-meter observatory set to launch no later than May 2027. Roman features two instruments: the Wide Field Imager and the Coronagraph Instrument. Roman's Coronagraph is a Technology Demonstration that will push the current capabilities of direct imaging to smaller contrast ratios ($\sim$10$^{-9}$) and inner-working angles (3~$λ$/D). In order to achieve this high precision, Roman Coronagraph data must be calibrated to remove as many potential sources of error as possible. Here we present a detailed overview of the Nancy Grace Roman Space Telescope Coronagraph Instrument Observation Calibration Plan including identifying potential sources of error and how they will be mitigated via on-sky calibrations.

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