[1] 徐波,雷汉伦.探测小天体[M].北京:科学出版社,2018.
[2] Reddy V,Sanchez J,Thirouin A,et al.Challenges in physical characterization of dim space objects:What can we learn from NEOs[C].Advanced Maui Optical and Space Surveillance Technologies Conference. Maui,Hawaii,USA:Maui Economic Development Board,2016.9.
[3] 侯建文.深空探测:小天体探测[M].北京:国防工业出版社,2016.
[4] Mainzer A,Grav T,Masiero J,et al.Characterizing subpopulations within the Near-Earth Objects with NEOWISE:Preliminary Results[J].ApJ,2012,752(2):110-126.
[5] 龚自正,李明,陈川,等.小行星监测预警、安全防御和资源利用的前沿科学问题及关键技术[J].科学通报,2020,65(5):346-372.
[6] Cneos.NEO Groups [EB/OL].https://cneos.jpl.nasa.gov/about/neo_groups.html.2021-2-24.
[7] Veres P,Schmidt N.Methods,means and governance of NEO observation[M].SCHMIDT N.Planetary Defense,Space and Society,Springer,Cham,2019:49-70.
[8] 徐伟彪,赵海斌.小行星深空探测的科学意义和展望[J].地球科学展望,2005,20(11):1183-1190.
[9] 林杨挺.太阳系起源与小天体探测的前沿科学问题[J].空间碎片研究,2019,19(3):14-21.
[10] 胡中为,赵海斌.太阳系考古遗存:小行星[M].北京:科学出版社,2017.
[11] Alvarez L W,Alvarez W,Asaro F,et al. Extraterrestrial cause for the Cretaceous/Tertiary extinction[J]. Science,1980,208(448):1095-1108.
[12] Miller S D,Straka W C,Bachmeier A S,et al. Earth-viewing satellite perspectives on the Chelya-binsk meteor event[J].Proc Natl Acad Sci USA,2013,110:18092-180927.
[13] 胡中为.保卫地球—近地天体的巡视与防御陨击的对策[J].自然杂志,2010,32(3):166-173.
[14] Space Mission Planning Advisory Group.SMPAG 5.5-Planetary Defense Action Plan:DRAFT[R]. October 2018.
[15] Mainzer A,Grav T,Bauer J,et al.NEOWISE observations of near-Earth objects:Preliminary results [J]. ApJ,2011,b(743):156-172.
[16] Grav T,Mainzer A K,Spahr T.Modeling the performance of the LSST in surveying the Near-Earth object population[J].The Astronomical Journal,2016,151(6):1-8.
[17] Tonry J L,Denneau A N,Heinze B,et al.ATLAS:A high-cadence all-sky survey system[J]. Publications of the Astronomical Society of the Pacific,2018,130(988):1-28.
[18] Near-Earth Object Science Definition Team.Update to determine the feasibility of enhancing the search and characterization of NEOs[R].NASA,2017.
[19] Mainzer A,Bauer J,Grav T,et al.Preliminary results from NEOWISE:anenhancement to the wide-field infrared survey explorer for solar system science[J]. ApJ,2011,731(1):53(13pp).
[20] Mainzer A,Grav T,Masiero J,et al.Thermal model calibration for minor planets observed with wide-field infrared survey explorer/NEOWISE[J].ApJ,2011,736(2):100(9pp).
[21] Mainzer A,Grav T,Masiero J,et al.Thermal model calibration for minor planets observed with WISE/NEOWISE:comparison with infrared astronomical satellite[J].ApJ,2011,737(1):L9(6pp).
[22] Mainzer A,Bauer J,Grav T,et al.The population of tiny near-earth objects observed by NEOWISE[J]. ApJ,2014b,784(2):110(7pp).
[23] Mainzer A,Grav T,Bauer J,et al.Survey simulations of a new near-earth asteroid detection system[J]. ApJ,2015,149:172(17pp).
[24] Myhrvold N.Comparing NEO search telescopes[J]. The Astronomical Society of the Pacific,2016,128:045004 (37pp).
[25] Trilling D E,Mueller M,Hora J L,et al. Explore NEOsⅠ:Description and first result from the warm spitzer near-earth object survey[J].AJ,2010,140:770-784.
[26] Mainzer A,Grav T,Masiero J,et al.Neowise studies of spectrophotometrically classified asteroids:preliminary results[J].ApJ,2011,741:90(25pp).
[27] Lebofsky L A,Sykes M V,Tedesco E F,et al.A refined “standard”thermal model for asteroids based on observations of 1Ceres and 2 Pallas[J].Icarus,1986,68(2):239-251.
[28] Lebofsky L A,Spencer J R.Radiometry and thermal modeling of asteroids[A].in Asteroids II[C] ,ed.R.P.Binzel,T.Gehrels,& M.S.Matthews,Tucson,AZ:Univ.Arizona Press,1989:128-147.
[29] Harris A W.A thermal model for near-earth asteroids[J].Icarus,1998,131:291-301.
[30] Mainzer A,Usui F,Trilling D E.Space-Based thermal infrared studies of aseroids[M].Michel P,Demeo F E,Bottke W F.Asteroids IV.Tuscon,AZ:Univ. of Arizona Press,2015.
[31] 姜浩轩,季江徽.小行星热物理及Yarkovsky效应和YORP效应的研究进展[J].天文学进展,2018,36(3):213-231.
[32] Bowell E,Hapke B,Domingue D,et al. Application of photometric models to asteroids[A].in Asteroids II[C].Proceedings of the Conference,Tucson,AZ:University of Arizona Press,1989:524-556.
[33] Mainzer A,Masiero J,Grav T,et al.Neowise studies of asteroids with sloan photometry:preliminary results[J].ApJ,2012,745:7(9pp).
[34] Grav T,Mainzer A K,Bauer J,et al.WISE/NEOWISE observations of the JOVIANTROJANS:preliminary results[J].APJ,2011,742:40(10pp).
[35] Grav T,Mainzer A K,Bauer J,et al.WISE/NEOWISE observations of the HILDA population:preliminary results [J].ApJ,2012,744(2):197(15pp).
[36] Masiero J R,Mainzer A K,Bauer J M et al. Asteroid family identification using the hierarchical clustering methodand wise/neowise physical properties[J]. ApJ,2013,770:7(22pp).
[37] Carruba V,Domingos R C,Nesvorny D,et al.A multi-domain approach to asteroid families identification[J].MNRAS,2013,433(3):2075-2096.
[38] Walsh K J,Delbo M,Bottke W F,et al. Introducing the Eulalia and new Polana asteroid families:Re-assessingprimitive asteroid families in the inner Main Belt[J].Icarus,2013,225(1):283-297.
[39] Milani A,Cellino A,Knezevic Z,et al.Asteroid families classification:Exploiting very large datasets[J]. Icarus,2014,239:46-73.
[40] 李春来,刘建军,严韦,等.小行星探测科学目标进展与展望[J].深空探测学报,2019,6(5):424-436.
[41] Interagency Working Group.Report on near-earth object impact threat emergency protocols[R].Near-Earth Object Impact Threat Emergency Protocols Subcommittee On Space Weather,Security,And Hazards Committee On Homeland And National Security Of The National Science & Technology Council,January 2021.
[42] Bely P Y.The design and construction of large optical telescope[M] ,Berlin:Spring-er-Verlag,2010.
[43] 孙海彬,孙胜利.近地小行星观测技术分析[J].深空探测学报,2020,7(2):197-205.
[44] Wright E L.WISE-the wide-field infrared survey explorer[J].Proc.of SPIE,2009,7419:741902.
[45] 常锐.小行星的巡天观测[J].国际太空,2017,463:34-37.
[46] Koch D G,Borucki W,Dunham E,et al.Overview and status of the Kepler Mission[J].Proc.of SPIE,2004,5487:1491-1500.
[47] 王新涛,郑建华,李明涛.地球公转轨道危地小行星天基光学监测仿真研究[J].光学精密工程,2020,28(11):2564-2571.
[48] Tedesco E F,Muinonen K,Price S D.Space-based infared near-Earth asteroid survey simulation[J]. P&SS,2000,48(9):801-816.
[49] Wright E L.Angular power spectra of the COBE DIRBE maps[J].ApJ,1998,496:1-8.
[50] Gorjian V,Wright E L,Chary R R.Tentative detection of the cosmic infrared background at 2.2 and 3.5 microns using ground-based and space-based observations[J].ApJ,2000,536(2):550-560.
[51] Leinert C,Bowyer S,Haikala L K,et al.The 1997 reference of diffuse night sky brightness.Astron[J]. Astrophys.Supplement,1998,127:1-99.
[52] Greenstreet S,Ngo H,Gladman B.The orbital distribution of Near-Earth Objects inside Earth’s orbit[J]. Icarus,2012,217(1),355-366.
[53] Grav T,Jedicke R,Denneau L,et al.The Pan-STARRS synthetic solar system model:a tool for testing and efficiency determination of the moving object processing system[J].PASP,2011,123,423-447.
[54] Tom C,Loose M,Gulbransen D J,et al.Astronomy FPA advancements at rockwell scientific[J].Proc. of SPIE,2006,6265:62652K.
[55] Dorn M,Mcmurtry C,Pipher J,et al.A monolithic 2k×2k LWIR HgCdTe detector array for passively cooled space missions[J].Proc.SPIE,2018,107 09:1070907.
[56] Mcmurtry C W,Dorn M,Cabrera M S,et al. Candidate 10 micron HgCdTe Arrays for the NEOCam space mission[J].Proc.of SPIE,2016,9915:99150D.
[57] Loose M,Lewyn L,Durmus H,et al.SIDECAR low-power control ASIC for focal plane arrays including AD conversion and bias generation[J].Proc. of SPIE,2003,4841:782-794.
[58] Storrie-lombaridi L J,Dodd S R.Spitzer warm mission:maximizing the science return in the extended mission phase[J].Proc.Of SPIE,2012,8448:84481E.
[59] Kroes G,Kragt J,Navarro R,et al.Opto-mechanical design for transmission optics in cryogenic IR instrumentation[J].Proc.of SPIE,2008,7018:70182D.
[60] Heys S,Swinyard B,Ferleta M,et al.Thermal and con-tamination control of the Mid-Infrared Instrument for JWST[J].Proc.of SPIE,2004,5497:39-50.
[61] Stewart E M.The James Webb Space Telescope:contamination control and materials[J].Proc.of SPIE,2018,10748:107480H.
