Optical Design Options For Pollux: UV Spectropolarimeter Project For The Habitable Worlds Observatory
Pollux is a project of UV spectropolarimeter proposed as a European contribution for the planned NASA-led Habitable Worlds Observatory.
In the present study we consider design options for four spectral channels. The two main channels operate in the range of 118-472 nm. We consider a few design options depending on the hosting telescope size and the approach to correct the aberrations in the camera part and show that the resolving power of R > 90 000 is reachable.
In addition, we study 2 other channels: a visible and near infrared spectropolarimeter, which could reach up to 1050 nm or 1800 nm depending on the detector choice, and a far UV channel operating in the range of 100-120 nm. We also provide two design options with different resolution and main disperser type for these channels.
Eduard Muslimov, Coralie Neiner, Jean-Claude Bouret
Comments: 23 pages, 13 figures, 6 tables
Subjects: Instrumentation and Methods for Astrophysics (astro-ph.IM)
Cite as: arXiv:2410.01491 [astro-ph.IM] (or arXiv:2410.01491v1 [astro-ph.IM] for this version)
https://doi.org/10.48550/arXiv.2410.01491
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Journal reference: Proc. SPIE 13093, 130933D (2024)
Related DOI:
https://doi.org/10.1117/12.3020175
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Submission history
From: Eduard Muslimov
[v1] Wed, 2 Oct 2024 12:43:56 UTC (4,572 KB)
https://arxiv.org/abs/2410.01491
Astrobiology, Astronomy,