Capturing Event Metadata in the Sky: a Java-Based Application for Receiving Astronomical Internet Feeds
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The Messenger
Czech Republic joins ESO The Messenger Progress on ALMA CRIRES Science Verification Gender balance among ESO staff No. 128 – JuneNo. 2007 The Organisation The Czech Republic Joins ESO Catherine Cesarsky The XXVIth IAU General Assembly, held This Agreement was formally confirmed (ESO Director General) in Prague in 2006, clearly provided a by the ESO Council at its meeting on boost for the Czech efforts to join ESO, 6 December and a few days thereafter by not the least in securing the necessary the Czech government, enabling a sign- I am delighted to welcome the Czech public and political support. Thus our ing ceremony in Prague on 22 December Republic as our 13th member state. From Czech colleagues used the opportunity (see photograph below). This was impor- its size, the Czech Republic may not be- to publish a fine and very interesting pop- tant because the Agreement foresaw long to the ‘big’ member states, but the ular book about Czech astronomy and accession by 1 January 2007. With the accession nonetheless marks an impor- ESO, which, together with the General signatures in place, the agreement could tant point in ESO’s history and, I believe, Assembly, created considerable media be submitted to the Czech Parliament in the history of Czech astronomy as well. interest. for ratification within an agreed ‘grace pe- The Czech Republic is the first of the riod’. This formal procedure was con- Central and East European countries to On 20 September 2006, at a meeting at cluded on 30 April 2007, when I was noti- join ESO. The membership underlines ESO Headquarters, the negotiating teams fied of the deposition of the instrument of ESO’s continuing evolution as the prime from ESO and the Czech Republic arrived ratification at the French Ministry of European organisation for astronomy, at an agreement in principle, which was Foreign Affairs. -
Optimal Observing of Astronomical Time Series Using Autonomous Agents
Optimal Observing of Astronomical Time Series using Autonomous Agents Eric S. Saunders Submitted by Eric Sanjay Saunders to the University of Exeter as a thesis for the degree of Doctor of Philosophy in Physics, September, 2007. This thesis is available for Library use on the understanding that it is copyright material and that no quotation from the thesis may be published without proper acknowledgement. I certify that all material in this thesis which is not my own work has been identified and that no material has previously been submitted and approved for the award of a degree by this or any other University. Signed: ........................... Eric S. Saunders Date: ................ Abstract This thesis demonstrates a practical solution to the problem of effective observation of time- varying phenomena using a network of robotic telescopes. The best way to place a limited number of observations to cover the dynamic range of frequencies required by an observer is addressed. An observation distribution geometrically spaced in time is found to minimise aliasing effects arising from sparse sampling, substantially improving signal detection quality. Further, such an optimal distribution may be reordered, as long as the distribution of spacings is preserved, with almost no loss of signal quality. This implies that optimal observing strategies can retain significant flexibil- ity in the face of scheduling constraints, by providing scope for on-the-fly adaptation. An adaptive algorithm is presented that implements such an optimal sampling in an uncertain observing en- vironment. This is incorporated into an autonomous software agent that responds dynamically to changing conditions on a robotic telescope network, without explicit user control. -
Gaia Science Alerts Workshop 2010 Abstract Book Dr Giuseppe Altavilla
Gaia Science Alerts Workshop 2010 Abstract Book Abstracts of talks and posters at the Gaia Science Alerts Workshop, held at the Institute of As- tronomy, Cambridge, June 23-25 2010. Dr Giuseppe Altavilla, Bologna, Italy Gaia & The Discovery of Supernovae - poster This poster gives an overview of the discovery rate of supernovae (SNe) with time. Data about all SNe detected so far and about the expected Gaia SN detections are shown, focussing on type Ia SNe. The expected Gaia contribution to the discovery of new SNe is also compared with the expected performances of other surveys such as LSST, Pan-STARRS, SkyMapper and other projects. Finally, a few examples show how these SN detections, if coupled with a proper spectro-photometric follow- up, can contribute to the understanding of SNe. Dr Martin Altmann, Heidelberg, Germany Ground Based Optical Tracking of Gaia The Ground based optical tracking (GBOT) project, required to ensure the precision of Gaia's orbit is another observing campaign to be conducted during the complete operational phase of Gaia. Precise knowledge of the satellite's orbit (both position and velocity vector) is mandatory in order to reach the scientific goals of the mission. One part of this effort is GBOT, which has the task to deliver astrometric measurements of Gaia on a daily basis, using a network of imagers on small (1-2 m) telescopes. The very nature of this undertaking implies similarities but also differences to the Science Alert program. In my contribution I will present GBOT and its status and also comment on its conceptual relation to the science alert follow up. -
An Anomaly Detector with Immediate Feedback to Hunt for Planets of Earth
Mon. Not. R. Astron. Soc. 000, 000–000 (0000) Printed 30 October 2018 (MN LATEX style file v2.2) An anomaly detector with immediate feedback to hunt for planets of Earth mass and below by microlensing M. Dominik,1⋆† N. J. Rattenbury,2 A. Allan,3 S. Mao,2 D. M. Bramich,4 M. J. Burgdorf,5 E. Kerins,2 Y. Tsapras,5 and Ł. Wyrzykowski6,7 1SUPA, University of St Andrews, School of Physics & Astronomy, North Haugh, St Andrews, KY16 9SS, United Kingdom 2Jodrell Bank Observatory, Macclesfield, Cheshire, SK11 9DL, United Kingdom 3School of Physics, University of Exeter, Stocker Road, Exeter EX4 4QL, United Kingdom 4Isaac Newton Group of Telescopes, Apartado de Correos 321, 38700 Santa Cruz de La Palma, Canary Islands, Spain 5Astrophysics Research Institute, Liverpool John Moores University, Twelve Quays House, Egerton Wharf, Birkenhead, CH41 1LD, United Kingdom 6Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, United Kingdom 7Warsaw University Astronomical Observatory, Al. Ujazdowskie 4, 00-478 Warszawa, Poland 30 October 2018 ABSTRACT The discovery of OGLE 2005-BLG-390Lb, the first cool rocky/icy exoplanet, impressively demonstrated the sensitivity of the microlensing technique to extra-solar planets below 10 M⊕. A planet of 1 M⊕ instead of the expected 5 M⊕ for OGLE 2005-BLG-390Lb (with an uncertainty factor of two) in the same spot would have provided a detectable deviation with an amplitude of ∼ 3 per cent and a duration of ∼ 12 h. While a standard sampling interval of 1.5 to 2.5 hours for microlensing follow-up observations appears to be insuffi- cient for characterizing such light curve anomalies and thereby claiming the discovery of the planets that caused these, an early detection of a deviation could trigger higher-cadence sam- pling which would have allowed the discovery of an Earth-mass planet in this case.