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SPHEREx: an all-sky NIR spectral survey

机译:SPHEREx:全方位的近红外光谱调查

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SPHEREx, a mission in NASA's Medium Explorer (MIDEX) program recently selected for Phase-A implementation, is an all-sky survey satellite that will produce a near-infrared spectrum for every 6 arcsecond pixel on the sky. SPHEREx has a simple, high-heritage design with large optical throughput to maximize spectral mapping speed. While the legacy data products will provide a rich archive of spectra for the entire astronomical community to mine, the instrument is optimized for three specific scientific goals: to probe inflation through the imprint primordial non-Gaussianity left on today's large-scale cosmological structure; to survey the Galactic plane for water and other biogenic ices through absorption line studies; and to constrain the history of galaxy formation through power spectra of background fluctuations as measured in deep regions near the ecliptic poles. The aluminum telescope consists of a heavily baffled, wide-field off-axis reflective triplet design. The focal plane is imaged simultaneously by two mosaics of H2R.G detector arrays separated by a dichroic beamsplitter. SPHEREx assembles spectra through the use of mass and volume efficient linear variable filters (LVFs) included in the focal plane assemblies, eliminating the need for any dispersive or moving elements. Instead, spectra are constructed through a series of small steps in the spacecraft attitude across the sky, modulating the location of an object within the FOV and varying the observation wavelength in each exposure. The spectra will cover the wavelength range between 0.75 and 5.0 μm at spectral resolutions ranging between R=35 and R=130. The entire telescope is cooled passively by a series of three V-groove radiators below 80K. An additional stage of radiative cooling is included to reduce the long wavelength focal plane temperature below 60K, controlling the dark current. As a whole, SPHEREx requires no new technologies and carries large technical and resource margins on every aspect of the design.
机译:SPHEREx是NASA的中型探索者(MIDEX)计划的一项任务,该计划最近被选定用于A期实施,它是一颗全天候的勘测卫星,它将为天空中每6弧秒像素产生近红外光谱。 SPHEREx具有简单的高继承性设计,并具有较大的光通量,可最大程度地提高光谱映射速度。虽然传统数据产品将为整个天文学界提供丰富的光谱档案,但该仪器针对三个特定的科学目标进行了优化:通过当今大规模宇宙学结构上留下的原始非高斯性烙印来探测通货膨胀;通过吸收线研究调查银河系中的水和其他生物冰;并通过背景波动的功率谱来限制星系形成的历史,该功率谱是在黄道极附近的深处测得的。铝制望远镜由一个非常折光的宽视场偏轴反射三重态设计组成。焦平面同时由两个由二向色分束器隔开的H2R.G检测器阵列镶嵌而成。 SPHEREx通过使用焦平面组件中包含的质量和体积有效的线性可变滤波器(LVF)来组装光谱,从而无需任何色散或移动元素。取而代之的是,光谱是通过航天器在天空中的姿态中的一系列小步骤构造的,从而调制了物体在FOV内的位置并在每次曝光中改变了观察波长。光谱将覆盖在0.75至5.0μm之间的波长范围,光谱分辨率介于R = 35和R = 130之间。整个望远镜由一系列低于80K的三个V型槽散热器被动冷却。包括辐射冷却的附加阶段,以将长波长焦平面温度降低到60K以下,从而控制暗电流。总体而言,SPHEREx不需要任何新技术,并且在设计的各个方面都具有很大的技术和资源裕度。

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