Spectropolarimeter's optical design for the Arago space mission project by Eduard Muslimov et al. on Monday 21 November

Arago is a concept of space mission submitted to the European Space Agency's

M7 science program. It will target a number of science cases in stellar physics

including the characterisation of star-planet interactions. The concept is

based on a 1-m class Ritchey-Chretien F/13 telescope mounted on an Ariel-type

platform. The scientific payload includes a common polarimetric unit and 2

spectrographs connected via a dichroic splitter. The polarimetric unit consists

of 6 MgF2 plates in pairs connected by optical contact and a Wollaston

analyzer. Each of the spectral channels represents an echelle spectrograph. The

first one will operate in the UV range 119-320 nm with the spectral resolving

power of R>25 000. It consists of an off-axis parabolic collimator, an echelle

grating in a quasi-Littrow mounting, a cross-disperser concave grating, and a

CMOS camera. The cross-disperser grating works also as a camera mirror and

represents a holographic grating recorded with aberrated wavefronts and on a

spherical substrate. The spectral image is projected onto a d-doped CMOS

detector. The second spectral channel operates in the visible range 350-888 nm

with R>35 000 and uses an immersed grating. The image is focused with a 4-lens

objective onto a CMOS detector. In addition, the optical design includes two

stages of fine-guiding system. The first stage represents a projecting system

tracking the image around the entrance pinhole and communicating with the

platform actuators. The second one is fed by the 0-th diffraction order of the

visible channel echelle. It is communicating with a tip-tilt mirror in front of

the dichroic. The first stage should improve the platform pointing accuracy

from 8" to 200 mas precision to guarantee that the star images passes through

the instrument's entrance pinhole. The second stage should correct the pointing

accuracy further as well as some thermo-elastic deformations.

arXiv: http://arxiv.org/abs/http://arxiv.org/abs/2211.09931v1