Data mining of near-Earth asteroids in the Subaru Suprime-Cam archive

被引:5
|
作者
Vaduvescu, O. [1 ,2 ]
Conovici, M. [3 ]
Popescu, M. [2 ,4 ,5 ]
Sonka, A. [5 ,6 ]
Paraschiv, A. [7 ,8 ]
Lacatus, D. [7 ,8 ]
Tudorica, A. [9 ,10 ]
Hudin, L. [11 ]
Curelaru, L. [12 ]
Inceu, V. [13 ]
Zavoianu, D. [5 ,12 ]
Cornea, R. [12 ,13 ]
Toma, R. [12 ,14 ]
Asher, D. J. [14 ]
Hadnett, J. [15 ,17 ]
Cheallaigh, L. O. [16 ,17 ]
机构
[1] Isaac Newton Grp Telescopes, Apartado Correos 321, E-38700 Santa Cruz De La Palma, Canary Islands, Spain
[2] Observ Paris, IMCCE, Paris, France
[3] Ostrov Observ, Amateur Astronomer, Constanta, Romania
[4] Romanian Acad, Astron Inst, Bucharest, Romania
[5] Bucharest Astroclub, B Dul Lascar Catargiu 21, Bucharest, Romania
[6] Admiral Vasile Urseanu Observ, Bucharest, Romania
[7] Inst Geodynam Sabba S Stefanescu, Bucharest, Romania
[8] Univ Bucharest, Res Ctr Atom Phys & Astrophys, Fac Phys, Magurele Ilfov, Romania
[9] Bonn Cologne Grad Sch Phys & Astron, Cologne, Germany
[10] Rhein Friedrich Wilhelms Univ Bonn, Argelander Inst Astron, Bonn, Germany
[11] ROASTERR 1 Observ, Amateur Astronomer, Cluj Napoca, Romania
[12] Romanian Soc Meteors & Astron SARM, Targoviste, Romania
[13] Univ Babes Bolyai, Fac Phys & Informat, Cluj Napoca, Romania
[14] Armagh Observ & Planetarium, Armagh, North Ireland
[15] Royal Sch, Armagh, North Ireland
[16] St Pauls High Sch, Newry, North Ireland
[17] Armagh Observ, Armagh, North Ireland
关键词
minor planets; asteroids - solar system: general - astrometry - methods: data analysis - astronomical databases: miscellaneous; MAIN-BELT ASTEROIDS; DISTRIBUTIONS; GALAXIES; SIZE; INT;
D O I
10.1002/asna.201713296
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
As part of the EURONEAR project, almost 70,000 mosaic Suprime-Cam images taken between 1999 and 2013 were data-mined for about 9,800 near-Earth asteroids (NEAs) known by 2013 May. Using our PRECOVERY server and the new Find Subaru CCD tool, we scrutinized 4,186 candidate CCD images possibly holding 518 NEAs. We found 113 NEAs as faint as V<25 magnitude, their positions being measured in 589 images using Astrometrica, and then reported to the Minor Planet Center. Among them, 18 objects represent encounters of previously single opposition NEAs, their orbital arcs being extended by up to 10years. In the second part of this work, we searched for unknown NEAs in 78 sequences (780 CCD fields) of 4-5 mosaic images selected from the same Suprime-Cam archive and totaling 16.6 deg(2), with the aim to assess the faint NEA distribution observable with an 8-m class survey. A total of 2,018 moving objects were measured, from which we identified 18 better NEA candidates. Using the Rcfilter in good weather conditions, mostly dark time and sky directions slightly biased towards the ecliptic, at least one NEA could be discovered in every 1 deg(2) surveyed.
引用
收藏
页码:527 / 535
页数:9
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