Acta Photonica Sinica, Volume. 52, Issue 5, 0552206(2023)

Optical Design of a High-efficiency Medium-low Dispersion Spectrograph with Wide-band Based on FOSC Type(Invited)

Hangxin JI1,2、*, Guoxin BA1,2,3, Jun LI1,2, and Haoran YU1,2
Author Affiliations
  • 1National Astronomical Observatories/Nanjing Institute of Astronomical Optics & Technology, Chinese Academy of Sciences, Nanjing 210042, China
  • 2CAS Key Laboratory of Astronomical Optics & Technology, Nanjing Institute of Astronomical Optics & Technology, Nanjing 210042, China
  • 3University of Chinese Academy of Sciences, Beijing 100049, China
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    References(31)

    [1] MARGUTTI R, COWPERTHWAITE P, DOCTOR Z et al. Target of opportunity observations of gravitational wave events with LSST[J]. The Astrophysical Journal, 874, 88(2019).

    [2] VALENTI S, SAND D, YANG Sheng et al. The discovery of the electromagnetic counterpart of GW170817: Kilonova AT 2017gfo/DLT17ck[J]. The Astrophysical Journal Letters, 848, L24(2017).

    [3] NICHOLL M, BERER E, KASEN D et al. The electromagnetic counterpart of the binary neutron star merger LIGO/Virgo GW170817. Ⅲ. optical and UV spectra of a blue kilonova from fast polar ejecta[J]. The Astrophysical Journal Letters, 848, L18(2017).

    [4] PIAN E, D′AVANZO, BENETTI S et al. Spectroscopic identification of r-process nucleosynthesis in a double neutron-star merger[J]. Natural, 551, 67-70(2017).

    [5] JI Hangxin, HU Zhongwen, ZHU Yongtian et al. Wide field multi-object spectrograph for 30m class optical/near infrared telescope[J]. Acta Astronomical Sinica, 60, 69-88(2019).

    [6] STALDER B, REIL K, AGUILAR C et al. Rubin observatory commissioning camera: summit integration[C], 12184, 121840J(2022).

    [7] POBEREZHSKIY I, HEYDORFF K, LUCHIK T et al. Roman coronagraph instrument: engineering overview and status[C], 12180, 121801X(2022).

    [8] ZHAN Hu. The wide-field multiband imaging and slitless spectroscopy survey to be carried out by the survey space telescope of china manned space program[J]. Chinese Science Bulletin, 66, 1290-1298(2021).

    [9] YUAN Xiangyan, LI Zhengyang, LIU Xiaowei et al. Development of the multi-channel photometric survey telescope[C], 11445, 114457M(2020).

    [10] LOVIS C, PEPE F, BOUCHY F et al. The exoplant hunter HARPS: unequalled accuracy and perspectives toward 1 cm s-1 precision[C], 6269, 62690P(2006).

    [11] PEPE F, CRISTIANI S, REBOLO R et al. ESPRESSO at VLT-on-sky performance and first results[J]. Astronomy & Astrophysics, 645, A96(2021).

    [12] HONSCHEID K, FANNING K, BAILEY S et al. The DESI instrument[C], 12184, 121840X(2022).

    [13] TAMURA N, MORITANI Y, YABE K et al. Prime Focus Spectrograph (PFS) for the subaru telescope: its start of the last development phase[C], 12184, 1218410(2022).

    [14] GONZALEZ O, CIRASUOLO M, TAYLOR W et al. MOONS-multi object spectroscopy for the VLT: overview and instrument integration update[C], 12184, 1218412(2022).

    [15] VERNET J, DEKKER H, D'ODORICO S et al. Performances of X-shooter, the new wide band intermediate resolution spectrograph at the VLT[C], 7735, 77351(2010).

    [16] JI Hangxin, CHEN Yi, WANG Lei et al. The current status of the Imaging and Spectrograph (IMSP) for 4m telescope[C], 11447, 114475O(2020).

    [17] CEDILLO J J, BONGIOVANNI A M, EDEROCLITE A et al. The Multi-Object Spectroscopy (MOS) observations automatized production line[C], 10705, 107050X(2018).

    [18] OKE J B, COHEN J G, CARR M et al. The keck low-resolution imaging spectrometer[J]. Publications of the Astronomical Society of the Pacific, 107, 375-385(1995).

    [19] BOFFIN H M, SEDAGHATI E, BLANCHARD G et al. Regaining the FORS: making optical ground-based transmission spectroscopy of exoplanets with VLT+FORS2 possible again[C], 9908, 99082B(2016).

    [20] KASHIKAWA N, INATA M, IYE M et al. FOCAS: faint object camera and spectrograph for the Subaru Telescope[C], 4008, 104-113(2000).

    [21] CEN Xuefen, QIAN Tongling. Faint object spectrograph and camera for 1m telescope[J]. Publications of Yunnan Observatory, 4, 34-42(2003).

    [22] WANG Chuanjun, BAI Jinming, FAN Yufeng et al. Lijiang 2.4-meter Telescope and its instruments[J]. Research in Astronomy and Astrophysics, 19, 149(2019).

    [23] BIANCO A, FRANGIAMORE M, ZANUTTA A et al. VPHGs for astronomy: what we learnt in OPTICON EU and manufacturing perspectives[C], 12188, 1218823(2022).

    [24] TRAUB W A. Constant-dispersion grism spectrometer for channeled spectra[J]. Optical Society of America, 7, 1779-1791(1990).

    [25] HOU Yonghui, TANG Linlin, XU Mingming et al. The LAMOST middle resolution spectrograph[C], 10702, 107021I(2018).

    [26] BALDRY I K, BLAND-HAWTHORN J, ROBERTSON J G. Volume phase holographic gratings: polarization properties and diffraction efficiency[J]. Publications of the Astronomical Society of the Pacific, 116, 403-414(2004).

    [27] JI Hangxin, ZHU Yongtian, HU Zhongwen. Optical system design of high throughput multi-channel spectrograph for very large telescope[J]. Acta Optica Sinica, 39, 0330003(2019).

    [28] PASQUINI L, DELABRE B, ELLIS R et al. New telescope design suitable for massively-multiplexed spectroscopy[C], 9906, 99063C(2012).

    [29] DUMAS D, FENDLER M, BAIER N et al. Curved focal plane detector array for wide field cameras[J]. Applied Optics, 51, 5419-5424(2012).

    [30] JORDEN P, BOURKE D, CASSIDY R et al. Teledyne e2v sensors optimized for ground-based and space applications[C], 10709, 1070903(2018).

    [31] LWERT O. Curved detectors (3D)-status[C](2017).

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    Hangxin JI, Guoxin BA, Jun LI, Haoran YU. Optical Design of a High-efficiency Medium-low Dispersion Spectrograph with Wide-band Based on FOSC Type(Invited)[J]. Acta Photonica Sinica, 2023, 52(5): 0552206

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    Paper Information

    Category: Special Issue for Advanced Science and Technology of Astronomical Optics

    Received: Dec. 27, 2022

    Accepted: Feb. 20, 2023

    Published Online: Jul. 19, 2023

    The Author Email: Hangxin JI (hxji@niaot.ac.cn)

    DOI:10.3788/gzxb20235205.0552206

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