22:
201:, the microlensing programme is carried on as RoboNet-II. Starting in 2008, RoboNet-II has been using the expert system for microlensing anomaly detection that is being provided by the
141:. For the technological aims of integrating a global network to act effectively as a single instrument, and maximizing the scientific return by applying the newest developments in
357:
198:
202:
171:
Apart from their science use, the telescopes forming the RoboNet-1.0 have also been made available for two educational programmes, the
187:
105:
156:, RoboNet-1.0 had two major science goals that critically depend on these requirements: the determination of origin and nature of
138:
43:
176:
385:
86:
58:
165:
172:
183:
65:
39:
134:
130:
32:
72:
153:
327:
261:
250:
54:
230:
218:
161:
126:
241:
236:
225:
194:
278:- RoboNet-II: Follow-up observations of microlensing events with a robotic network of telescopes
256:
122:
193:
With the official end of RoboNet-1.0 in
October 2007, and the earlier acquisition of the two
157:
152:
With the flexible scheduling and short response time of robotic telescopes being ideal for
371:
Burst
Observer and Optical Transient Exploring System (BOOTES) Robotic Telescope Network
379:
146:
79:
282:
274:
300:
145:, RoboNet adopted the intelligent-agent architecture devised and maintained by the
244:
and OGLE-2006-BLG-109Lc (a pair similar to
Jupiter and Saturn in the Solar system)
21:
137:
in
Australia, managed by a consortium of ten UK universities under the lead of
206:
142:
205:(ARTEMiS). RoboNet-II aims at obtaining a first census of cool terrestrial
347:
365:
286:- A Metric and Optimisation Scheme for Microlens Planet Searches
342:
15:
337:
203:
Automated
Robotic Terrestrial Exoplanet Microlensing Search
332:
217:
RoboNet data have contributed to the detection of several
233:(the most Earth-like planet at the time of its discovery)
125:, the largest of their kind in the world, comprising the
370:
353:
Las
Cumbres Observatory Global Telescope Network (LCOGT)
121:-1.0 was a prototype global network of UK-built 2-metre
352:
46:. Unsourced material may be challenged and removed.
221:(in the order of announcement of their discovery)
199:Las Cumbres Observatory Global Telescope Network
182:The RoboNet microlensing programme, led by the
247:OGLE-2007-BLG-368Lb a cold Neptune-Mass planet
8:
366:Microlensing Observations in Astrophysics
106:Learn how and when to remove this message
348:University of St Andrews Astronomy Group
186:, engages in a common campaign with the
292:
7:
343:LJMU Astrophysics Research Institute
253:a massive planet orbiting an M dwarf
44:adding citations to reliable sources
129:on La Palma (Canary Islands), the
14:
361:episode on RoboNet (August 2007)
139:Liverpool John Moores University
20:
31:needs additional citations for
1:
264:a cold, ~10 Earth Mass planet
177:National Schools‘ Observatory
284:MNRAS, 396, 2087–2102 (2009)
160:, and the detection of cool
402:
190:collaboration since 2005.
166:gravitational microlensing
133:on Maui (Hawaii), and the
173:Faulkes Telescope Project
184:University of St Andrews
135:Faulkes Telescope South
131:Faulkes Telescope North
276:AN , 330, 1, 4 (2009)
154:time-domain astronomy
40:improve this article
242:OGLE-2006-BLG-109Lb
237:OGLE-2005-BLG-169Lb
231:OGLE-2005-BLG-390Lb
226:OGLE-2005-BLG-071Lb
219:extra-solar planets
213:Research highlights
162:extra-solar planets
127:Liverpool Telescope
386:Robotic telescopes
262:MOA-2009-BLG-266Lb
257:MOA-2009-BLG-387Lb
251:MOA-2009-BLG-319Lb
195:Faulkes Telescopes
123:robotic telescopes
116:
115:
108:
90:
393:
359:The Sky at Night
338:ARTEMiS homepage
328:RoboNet homepage
315:
314:
312:
311:
297:
158:gamma-ray bursts
111:
104:
100:
97:
91:
89:
48:
24:
16:
401:
400:
396:
395:
394:
392:
391:
390:
376:
375:
324:
319:
318:
309:
307:
301:"NASA: Artemis"
299:
298:
294:
271:
215:
112:
101:
95:
92:
49:
47:
37:
25:
12:
11:
5:
399:
397:
389:
388:
378:
377:
374:
373:
368:
363:
355:
350:
345:
340:
335:
333:eSTAR homepage
330:
323:
322:External links
320:
317:
316:
291:
290:
289:
288:
280:
270:
267:
266:
265:
259:
254:
248:
245:
239:
234:
228:
214:
211:
114:
113:
28:
26:
19:
13:
10:
9:
6:
4:
3:
2:
398:
387:
384:
383:
381:
372:
369:
367:
364:
362:
360:
356:
354:
351:
349:
346:
344:
341:
339:
336:
334:
331:
329:
326:
325:
321:
306:
302:
296:
293:
287:
285:
281:
279:
277:
273:
272:
268:
263:
260:
258:
255:
252:
249:
246:
243:
240:
238:
235:
232:
229:
227:
224:
223:
222:
220:
212:
210:
208:
204:
200:
196:
191:
189:
185:
180:
178:
174:
169:
167:
163:
159:
155:
150:
148:
147:eSTAR project
144:
140:
136:
132:
128:
124:
120:
110:
107:
99:
88:
85:
81:
78:
74:
71:
67:
64:
60:
57: –
56:
52:
51:Find sources:
45:
41:
35:
34:
29:This article
27:
23:
18:
17:
358:
308:. Retrieved
304:
295:
283:
275:
216:
192:
181:
170:
164:by means of
151:
118:
117:
102:
93:
83:
76:
69:
62:
50:
38:Please help
33:verification
30:
310:2022-07-20
269:References
207:exoplanets
66:newspapers
143:e-Science
96:July 2022
55:"RoboNet"
380:Category
175:and the
119:RoboNet
80:scholar
188:PLANET
82:
75:
68:
61:
53:
87:JSTOR
73:books
305:NASA
59:news
197:by
42:by
382::
303:.
209:.
179:.
168:.
149:.
313:.
109:)
103:(
98:)
94:(
84:·
77:·
70:·
63:·
36:.
Text is available under the Creative Commons Attribution-ShareAlike License. Additional terms may apply.
