RoboTAP: Target priorities for robotic microlensing observations
文献类型:期刊论文
作者 | Hundertmark, M.2; Street, R. A.3; Tsapras, Y.2; Bachelet, E.3; Dominik, M.4; Horne, K.4; Bozza, V.5,6; Bramich, D. M.19; Cassan, A.7,8; D'Ago, G.9 |
刊名 | ASTRONOMY & ASTROPHYSICS |
出版日期 | 2018-01-05 |
卷号 | 609页码:13 |
ISSN号 | 1432-0746 |
关键词 | gravitational lensing: micro methods: observational methods: statistical |
DOI | 10.1051/0004-6361/201730692 |
英文摘要 | Context. The ability to automatically select scientifically-important transient events from an alert stream of many such events, and to conduct follow-up observations in response, will become increasingly important in astronomy. With wide-angle time domain surveys pushing to fainter limiting magnitudes, the capability to follow-up on transient alerts far exceeds our follow-up telescope resources, and effective target prioritization becomes essential. The RoboNet-II microlensing program is a pathfinder project, which has developed an automated target selection process (RoboTAP) for gravitational microlensing events, which are observed in real time using the Las Cumbres Observatory telescope network. Aims. Follow-up telescopes typically have a much smaller field of view compared to surveys, therefore the most promising microlensing events must be automatically selected at any given time from an annual sample exceeding 2000 events. The main challenge is to select between events with a high planet detection sensitivity, with the aim of detecting many planets and characterizing planetary anomalies. Methods. Our target selection algorithm is a hybrid system based on estimates of the planet detection zones around a microlens. It follows automatic anomaly alerts and respects the expected survey coverage of specific events. Results. We introduce the RoboTAP algorithm, whose purpose is to select and prioritize microlensing events with high sensitivity to planetary companions. In this work, we determine the planet sensitivity of the RoboNet follow-up program and provide a working example of how a broker can be designed for a real-life transient science program conducting follow-up observations in response to alerts; we explore the issues that will confront similar programs being developed for the Large Synoptic Survey Telescope (LSST) and other time domain surveys. |
WOS关键词 | GRAVITATIONAL LENSING EXPERIMENT ; EARTH-MASS PLANETS ; OGLE-III ; TELESCOPE NETWORK ; GALACTIC PLANETS ; BLACK-HOLE ; SNOW LINE ; EVENT ; SYSTEM ; STAR |
资助项目 | NPRP from the Qatar National Research Fund (a member of Qatar Foundation)[X-019-1-006] ; Chinese Academy of Sciences[XDB09000000] ; National Natural Science Foundation of China (NSFC)[11333003] ; National Natural Science Foundation of China (NSFC)[11390372] ; NASA ; STFC[ST/M001296/1] ; National Aeronautics and Space Administration |
WOS研究方向 | Astronomy & Astrophysics |
语种 | 英语 |
出版者 | EDP SCIENCES S A |
WOS记录号 | WOS:000419994600002 |
资助机构 | NPRP from the Qatar National Research Fund (a member of Qatar Foundation) ; NPRP from the Qatar National Research Fund (a member of Qatar Foundation) ; Chinese Academy of Sciences ; Chinese Academy of Sciences ; National Natural Science Foundation of China (NSFC) ; National Natural Science Foundation of China (NSFC) ; NASA ; NASA ; STFC ; STFC ; National Aeronautics and Space Administration ; National Aeronautics and Space Administration ; NPRP from the Qatar National Research Fund (a member of Qatar Foundation) ; NPRP from the Qatar National Research Fund (a member of Qatar Foundation) ; Chinese Academy of Sciences ; Chinese Academy of Sciences ; National Natural Science Foundation of China (NSFC) ; National Natural Science Foundation of China (NSFC) ; NASA ; NASA ; STFC ; STFC ; National Aeronautics and Space Administration ; National Aeronautics and Space Administration ; NPRP from the Qatar National Research Fund (a member of Qatar Foundation) ; NPRP from the Qatar National Research Fund (a member of Qatar Foundation) ; Chinese Academy of Sciences ; Chinese Academy of Sciences ; National Natural Science Foundation of China (NSFC) ; National Natural Science Foundation of China (NSFC) ; NASA ; NASA ; STFC ; STFC ; National Aeronautics and Space Administration ; National Aeronautics and Space Administration ; NPRP from the Qatar National Research Fund (a member of Qatar Foundation) ; NPRP from the Qatar National Research Fund (a member of Qatar Foundation) ; Chinese Academy of Sciences ; Chinese Academy of Sciences ; National Natural Science Foundation of China (NSFC) ; National Natural Science Foundation of China (NSFC) ; NASA ; NASA ; STFC ; STFC ; National Aeronautics and Space Administration ; National Aeronautics and Space Administration |
源URL | [http://ir.bao.ac.cn/handle/114a11/37377] |
专题 | 中国科学院国家天文台 |
通讯作者 | Hundertmark, M. |
作者单位 | 1.Liverpool John Moores Univ, Astrophys Res Inst, Liverpool CH41 1LD, Merseyside, England 2.Univ Heidelberg ZAH, Astron Rech Inst, Zentrum Astron, D-69120 Heidelberg, Germany 3.Las Cumbres Observ Global Telescope Network, 6740 Cortona Dr,Suite 102, Goleta, CA 93117 USA 4.Univ St Andrews, Sch Phys & Astron, SUPA, St Andrews KY16 9SS, Fife, Scotland 5.Univ Salerno, Dipartimento Fis ER Caianiello, Via Giovanni Paolo II 132, I-84084 Fisciano, SA, Italy 6.Ist Nazl Fis Nucl, Sez Napoli, Via Cintia, I-80126 Naples, Italy 7.UPMC Univ Paris 6, Sorbonne Univ, 98 Bis Bd Arago, F-75014 Paris, France 8.Inst Astrophys Paris, CNRS, UMR 7095, 98 Bis Bd Arago, F-75014 Paris, France 9.INAF Observ Capodimonte, Salita Moiariello 16, I-80131 Naples, Italy 10.European Southern Observ, Karl Schwarzschild Str 2, D-85748 Munich, Germany |
推荐引用方式 GB/T 7714 | Hundertmark, M.,Street, R. A.,Tsapras, Y.,et al. RoboTAP: Target priorities for robotic microlensing observations[J]. ASTRONOMY & ASTROPHYSICS,2018,609:13. |
APA | Hundertmark, M..,Street, R. A..,Tsapras, Y..,Bachelet, E..,Dominik, M..,...&Shvartzvald, Y..(2018).RoboTAP: Target priorities for robotic microlensing observations.ASTRONOMY & ASTROPHYSICS,609,13. |
MLA | Hundertmark, M.,et al."RoboTAP: Target priorities for robotic microlensing observations".ASTRONOMY & ASTROPHYSICS 609(2018):13. |
入库方式: OAI收割
来源:国家天文台
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