Marshall, Herman L.Herman L.MarshallGünther, H. MoritzH. MoritzGüntherHeilmann, Ralf K.Ralf K.HeilmannSchulz, Norbert S.Norbert S.SchulzEgan, MarkMarkEganHellickson, TimTimHellicksonHeine, Sarah N. T.Sarah N. T.HeineWindt, David L.David L.WindtGullikson, Eric M.Eric M.GulliksonRamsey, BrianBrianRamseyTAGLIAFERRI, GianpieroGianpieroTAGLIAFERRIPARESCHI, GiovanniGiovanniPARESCHI2021-02-252021-02-2520182329-4124http://hdl.handle.net/20.500.12386/30614We describe an optical design and possible implementation of a broadband soft x-ray polarimeter. Our arrangement of gratings is designed optimally for the purpose of polarimetry with broadband focusing optics by matching the dispersion of the spectrometer channels to laterally graded multilayers (LGMLs). The system can achieve polarization modulation factors over 90%. We implement this design using a single optical system by dividing the entrance aperture into six sectors; high efficiency, blazed gratings from opposite sectors are oriented to disperse to a common LGML forming three channels covering the wavelength range from 35 to 75 Å (165 to 350 eV). The grating dispersions and LGML position angles for each channel are 120 deg to each other. CCD detectors then measure the intensities of the dispersed spectra after reflection and polarizing by the LGMLs, giving the three Stokes parameters needed to determine a source's linear polarization fraction and orientation. The design can be extended to higher energies as LGMLs are developed further. We describe examples of the potential scientific return from instruments based on this design.ELETTRONICOenArticle10.1117/1.JATIS.4.1.0110052-s2.0-85044737288000429569000005https://www.spiedigitallibrary.org/journals/Journal-of-Astronomical-Telescopes-Instruments-and-Systems/volume-4/issue-01/011005/Design-of-a-broadband-soft-x-ray-polarimeter/10.1117/1.JATIS.4.1.011005.full?SSO=12018JATIS...4a1005MFIS/05 - ASTRONOMIA E ASTROFISICA