[{"date_updated":"2024-04-08T06:58:50Z","volume":11444,"status":"public","month":"12","extern":"1","arxiv":1,"language":[{"iso":"eng"}],"publication":"Space Telescopes and Instrumentation 2020: Ultraviolet to Gamma Ray","oa_version":"Preprint","scopus_import":"1","year":"2020","conference":{"start_date":"2020-12-14","name":"Astronomical Telescopes + Instrumentation","end_date":"2020-12-18","location":"Virtual"},"day":"13","publication_identifier":{"eissn":["1996-756X"],"isbn":["978-151063675-0"]},"title":"A small satellite version of a soft x-ray polarimeter","author":[{"first_name":"Herman L.","last_name":"Marshall","full_name":"Marshall, Herman L."},{"first_name":"Sarah","last_name":"Heine","full_name":"Heine, Sarah"},{"first_name":"Alan","last_name":"Garner","full_name":"Garner, Alan"},{"full_name":"Gullikson, Eric","first_name":"Eric","last_name":"Gullikson"},{"full_name":"Guenther, Moritz","first_name":"Moritz","last_name":"Guenther"},{"first_name":"Christopher","last_name":"Leitz","full_name":"Leitz, Christopher"},{"full_name":"Masterson, Rebecca","last_name":"Masterson","first_name":"Rebecca"},{"last_name":"Miller","first_name":"Eric","full_name":"Miller, Eric"},{"full_name":"Zhang, William","last_name":"Zhang","first_name":"William"},{"first_name":"Rozenn","last_name":"Boissay Malaquin","full_name":"Boissay Malaquin, Rozenn"},{"full_name":"Caiazzo, Ilaria","id":"8ae5b6e7-2a03-11ee-914d-b58ed7a3b47d","orcid":"0000-0002-4770-5388","first_name":"Ilaria","last_name":"Caiazzo"},{"first_name":"Deepto","last_name":"Chakrabarty","full_name":"Chakrabarty, Deepto"},{"first_name":"Rosemary","last_name":"Davidson","full_name":"Davidson, Rosemary"},{"last_name":"Gallo","first_name":"Luigi","full_name":"Gallo, Luigi"},{"first_name":"Ralf K.","last_name":"Heilmann","full_name":"Heilmann, Ralf K."},{"last_name":"Heyl","first_name":"Jeremy","full_name":"Heyl, Jeremy"},{"full_name":"Kara, Erin","last_name":"Kara","first_name":"Erin"},{"full_name":"Marscher, Alan","first_name":"Alan","last_name":"Marscher"},{"last_name":"Schulz","first_name":"Norbert","full_name":"Schulz, Norbert"}],"user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","date_created":"2024-03-26T10:36:20Z","article_number":"114442Y","external_id":{"arxiv":["2012.02829"]},"intvolume":"     11444","quality_controlled":"1","oa":1,"publisher":"SPIE","doi":"10.1117/12.2562811","main_file_link":[{"url":"https://doi.org/10.48550/arXiv.2012.02829","open_access":"1"}],"type":"conference","publication_status":"published","_id":"15228","abstract":[{"text":"We describe a new implementation of a broad-band soft X-ray polarimeter, substantially based on a previous design. This implementation, the Pioneer Soft X-ray Polarimeter (PiSoX) is a SmallSat, designed for NASA’s call for Astrophysics Pioneers, small missions that could be CubeSats, balloon experiments, or SmallSats. As in REDSoX, the grating arrangement is designed optimally for the purpose of polarimetry with broad-band focussing optics by matching the dispersion of the spectrometer channels to laterally graded multilayers (LGMLs). The system can achieve polarization modulation factors over 90%. For PiSoX, the optics are lightweight Si mirrors in a one-bounce parabolic configuration. High efficiency, blazed gratings from opposite sectors are oriented to disperse to a LGML forming a channel covering the wavelength range from 35 Å to 75 Å (165 - 350 eV). Upon satellite rotation, the intensities of the dispersed spectra, after reflection and polarizing by the LGMLs, give 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.","lang":"eng"}],"citation":{"apa":"Marshall, H. L., Heine, S., Garner, A., Gullikson, E., Guenther, M., Leitz, C., … Schulz, N. (2020). A small satellite version of a soft x-ray polarimeter. In <i>Space Telescopes and Instrumentation 2020: Ultraviolet to Gamma Ray</i> (Vol. 11444). Virtual: SPIE. <a href=\"https://doi.org/10.1117/12.2562811\">https://doi.org/10.1117/12.2562811</a>","chicago":"Marshall, Herman L., Sarah Heine, Alan Garner, Eric Gullikson, Moritz Guenther, Christopher Leitz, Rebecca Masterson, et al. “A Small Satellite Version of a Soft X-Ray Polarimeter.” In <i>Space Telescopes and Instrumentation 2020: Ultraviolet to Gamma Ray</i>, Vol. 11444. SPIE, 2020. <a href=\"https://doi.org/10.1117/12.2562811\">https://doi.org/10.1117/12.2562811</a>.","short":"H.L. Marshall, S. Heine, A. Garner, E. Gullikson, M. Guenther, C. Leitz, R. Masterson, E. Miller, W. Zhang, R. Boissay Malaquin, I. Caiazzo, D. Chakrabarty, R. Davidson, L. Gallo, R.K. Heilmann, J. Heyl, E. Kara, A. Marscher, N. Schulz, in:, Space Telescopes and Instrumentation 2020: Ultraviolet to Gamma Ray, SPIE, 2020.","ista":"Marshall HL, Heine S, Garner A, Gullikson E, Guenther M, Leitz C, Masterson R, Miller E, Zhang W, Boissay Malaquin R, Caiazzo I, Chakrabarty D, Davidson R, Gallo L, Heilmann RK, Heyl J, Kara E, Marscher A, Schulz N. 2020. A small satellite version of a soft x-ray polarimeter. Space Telescopes and Instrumentation 2020: Ultraviolet to Gamma Ray. Astronomical Telescopes + Instrumentation vol. 11444, 114442Y.","ama":"Marshall HL, Heine S, Garner A, et al. A small satellite version of a soft x-ray polarimeter. In: <i>Space Telescopes and Instrumentation 2020: Ultraviolet to Gamma Ray</i>. Vol 11444. SPIE; 2020. doi:<a href=\"https://doi.org/10.1117/12.2562811\">10.1117/12.2562811</a>","mla":"Marshall, Herman L., et al. “A Small Satellite Version of a Soft X-Ray Polarimeter.” <i>Space Telescopes and Instrumentation 2020: Ultraviolet to Gamma Ray</i>, vol. 11444, 114442Y, SPIE, 2020, doi:<a href=\"https://doi.org/10.1117/12.2562811\">10.1117/12.2562811</a>.","ieee":"H. L. Marshall <i>et al.</i>, “A small satellite version of a soft x-ray polarimeter,” in <i>Space Telescopes and Instrumentation 2020: Ultraviolet to Gamma Ray</i>, Virtual, 2020, vol. 11444."},"article_processing_charge":"No","date_published":"2020-12-13T00:00:00Z"},{"publication_identifier":{"isbn":["978-151063675-0"],"eissn":["1996-756X"]},"article_processing_charge":"No","date_published":"2020-12-13T00:00:00Z","day":"13","citation":{"ieee":"J. Heyl, I. Caiazzo, S. Gallagher, K. Hoffman, and S. Safi-Harb, “The Colibrì high-resolution x-ray telescope,” in <i>Space Telescopes and Instrumentation 2020: Ultraviolet to Gamma Ray</i>, Virtual, 2020, vol. 11444.","mla":"Heyl, Jeremy, et al. “The Colibrì High-Resolution x-Ray Telescope.” <i>Space Telescopes and Instrumentation 2020: Ultraviolet to Gamma Ray</i>, vol. 11444, 114442A, SPIE, 2020, doi:<a href=\"https://doi.org/10.1117/12.2562625\">10.1117/12.2562625</a>.","ama":"Heyl J, Caiazzo I, Gallagher S, Hoffman K, Safi-Harb S. The Colibrì high-resolution x-ray telescope. In: <i>Space Telescopes and Instrumentation 2020: Ultraviolet to Gamma Ray</i>. Vol 11444. SPIE; 2020. doi:<a href=\"https://doi.org/10.1117/12.2562625\">10.1117/12.2562625</a>","ista":"Heyl J, Caiazzo I, Gallagher S, Hoffman K, Safi-Harb S. 2020. The Colibrì high-resolution x-ray telescope. Space Telescopes and Instrumentation 2020: Ultraviolet to Gamma Ray. Astronomical Telescopes + Instrumentation vol. 11444, 114442A.","short":"J. Heyl, I. Caiazzo, S. Gallagher, K. Hoffman, S. Safi-Harb, in:, Space Telescopes and Instrumentation 2020: Ultraviolet to Gamma Ray, SPIE, 2020.","apa":"Heyl, J., Caiazzo, I., Gallagher, S., Hoffman, K., &#38; Safi-Harb, S. (2020). The Colibrì high-resolution x-ray telescope. In <i>Space Telescopes and Instrumentation 2020: Ultraviolet to Gamma Ray</i> (Vol. 11444). Virtual: SPIE. <a href=\"https://doi.org/10.1117/12.2562625\">https://doi.org/10.1117/12.2562625</a>","chicago":"Heyl, Jeremy, Ilaria Caiazzo, Sarah Gallagher, Kelsey Hoffman, and Samar Safi-Harb. “The Colibrì High-Resolution x-Ray Telescope.” In <i>Space Telescopes and Instrumentation 2020: Ultraviolet to Gamma Ray</i>, Vol. 11444. SPIE, 2020. <a href=\"https://doi.org/10.1117/12.2562625\">https://doi.org/10.1117/12.2562625</a>."},"abstract":[{"text":"We propose a high-time-resolution, high-spectral-resolution X-ray telescope that uses transition-edge sensors (TES) as detectors and collector optics to direct the X-rays onto the focal plane, providing a large effective area in a small satellite. The key science driver of the instrument is to study neutron stars and accreting black holes. The proposed instrument is built upon two technologies that are already at high TRL: TES X-ray detectors and collector optics.","lang":"eng"}],"_id":"15229","conference":{"location":"Virtual","name":"Astronomical Telescopes + Instrumentation","start_date":"2020-12-14","end_date":"2020-12-18"},"year":"2020","oa_version":"None","publication":"Space Telescopes and Instrumentation 2020: Ultraviolet to Gamma Ray","type":"conference","publication_status":"published","scopus_import":"1","quality_controlled":"1","language":[{"iso":"eng"}],"publisher":"SPIE","doi":"10.1117/12.2562625","article_number":"114442A","intvolume":"     11444","status":"public","extern":"1","month":"12","author":[{"first_name":"Jeremy","last_name":"Heyl","full_name":"Heyl, Jeremy"},{"id":"8ae5b6e7-2a03-11ee-914d-b58ed7a3b47d","full_name":"Caiazzo, Ilaria","first_name":"Ilaria","last_name":"Caiazzo","orcid":"0000-0002-4770-5388"},{"first_name":"Sarah","last_name":"Gallagher","full_name":"Gallagher, Sarah"},{"full_name":"Hoffman, Kelsey","last_name":"Hoffman","first_name":"Kelsey"},{"full_name":"Safi-Harb, Samar","first_name":"Samar","last_name":"Safi-Harb"}],"date_created":"2024-03-26T10:36:40Z","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","date_updated":"2024-04-08T06:59:43Z","volume":11444,"title":"The Colibrì high-resolution x-ray telescope"}]