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dc.contributor.authorHundertmark, M.
dc.contributor.authorStreet, R. A.
dc.contributor.authorTsapras, Y.
dc.contributor.authorBachelet, E.
dc.contributor.authorDominik, M.
dc.contributor.authorHorne, K.
dc.contributor.authorBozza, V.
dc.contributor.authorBramich, D. M.
dc.contributor.authorCassan, A.
dc.contributor.authorD'Ago, G.
dc.contributor.authorJaimes, R. Figuera
dc.contributor.authorKains, N.
dc.contributor.authorRanc, C.
dc.contributor.authorSchmidt, R. W.
dc.contributor.authorSnodgrass, C.
dc.contributor.authorWambsganss, J.
dc.contributor.authorSteele, I. A.
dc.contributor.authorMao, S.
dc.contributor.authorMent, K.
dc.contributor.authorMenzies, J.
dc.contributor.authorLi, Z.
dc.contributor.authorCross, S.
dc.contributor.authorMaoz, D.
dc.contributor.authorShvartzvald, Y.
dc.date.accessioned2017-10-20T14:30:15Z
dc.date.available2017-10-20T14:30:15Z
dc.date.issued2018-01-05
dc.identifier.citationHundertmark , M , Street , R A , Tsapras , Y , Bachelet , E , Dominik , M , Horne , K , Bozza , V , Bramich , D M , Cassan , A , D'Ago , G , Jaimes , R F , Kains , N , Ranc , C , Schmidt , R W , Snodgrass , C , Wambsganss , J , Steele , I A , Mao , S , Ment , K , Menzies , J , Li , Z , Cross , S , Maoz , D & Shvartzvald , Y 2018 , ' RoboTAP : target priorities for robotic microlensing observations ' , Astronomy & Astrophysics , vol. 609 , A55 . https://doi.org/10.1051/0004-6361/201730692en
dc.identifier.issn0004-6361
dc.identifier.otherPURE: 251290448
dc.identifier.otherPURE UUID: de045188-5b80-4e61-ad82-d9bf70eda57e
dc.identifier.otherArXiv: http://arxiv.org/abs/1710.00523v1
dc.identifier.otherScopus: 85040311060
dc.identifier.otherWOS: 000419994600002
dc.identifier.otherORCID: /0000-0002-3202-0343/work/75996770
dc.identifier.urihttps://hdl.handle.net/10023/11892
dc.descriptionK.H. acknowledges support from STFC grant ST/M001296/1.en
dc.description.abstractContext. 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 microlens- ing 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, aiming at the detection of 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, exploring the issues that will confront similar programs being developed for the Large Synoptic Survey Telescope (LSST) and other time domain surveys.
dc.format.extent13
dc.language.isoeng
dc.relation.ispartofAstronomy & Astrophysicsen
dc.rights© 2017, ESO. This work has been made available online in accordance with the publisher’s policies. This is the author created, accepted version manuscript following peer review and may differ slightly from the final published version. The final published version of this work is available at 10.1051/0004-6361/201730692en
dc.subjectGravitational lensing: microen
dc.subjectMethods: observationalen
dc.subjectMethods: statisticalen
dc.subjectQB Astronomyen
dc.subjectQC Physicsen
dc.subjectNDASen
dc.subject.lccQBen
dc.subject.lccQCen
dc.titleRoboTAP : target priorities for robotic microlensing observationsen
dc.typeJournal articleen
dc.contributor.sponsorScience & Technology Facilities Councilen
dc.description.versionPostprinten
dc.contributor.institutionUniversity of St Andrews. School of Physics and Astronomyen
dc.contributor.institutionUniversity of St Andrews. St Andrews Centre for Exoplanet Scienceen
dc.identifier.doihttps://doi.org/10.1051/0004-6361/201730692
dc.description.statusPeer revieweden
dc.identifier.grantnumberST/M001296/1en


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