scholarly journals NEOPAT: Near-Earth Object PATrol program

2001 ◽  
Vol 183 ◽  
pp. 240-244
Author(s):  
Hong-Kyu Moon ◽  
Moo-Young Chun ◽  
Yong-Ik Byun ◽  
Wonyong Han ◽  
Seung-Lee Kim ◽  
...  
Keyword(s):  
High Efficiency ◽  
Wide Field ◽  
Main Belt ◽  
Earth Object ◽  
Data Pipeline ◽  
Wide Field Of View ◽  
Survey System ◽  
Robotic Telescopes ◽  
Astronomical Research

AbstractIn 2000, Korea Astronomy Observatory launched the Near-Earth Object Patrol (NEOPAT) program. NEOPAT has conducted follow-up observations of NEOCP (NEO Confirmation Page) objects and discovered 52 new main-belt asteroids during the observation runs. We initiated collaboration with the Yonsei Survey Telescopes for Astronomical Research (YSTAR) team for NEO search. Wide-field of view, fast read-out time, and fully autonomous data pipeline will enable us to detect and track NEOs with a high efficiency. Scheduled to begin active operations in mid-2001, our survey system is going to be the first network of robotic telescopes for NEO search with automatic access to both hemispheres.

scholarly journals Small and Robotic Telescopes in the Era of Massive Time-Domain Surveys

2011 ◽  
Vol 7 (S285) ◽  
pp. 235-238
Author(s):  
M. F. Bode ◽  
W. T. Vestrand
Keyword(s):  
Real Time ◽  
Time Domain ◽  
Wide Field ◽  
Small Aperture ◽  
Robotic Telescopes ◽  
On Line ◽  
New Facilities

AbstractWe have entered an era in time-domain astronomy in which the detected rate of explosive transients and important ephemeral states in persistent objects threatens to overwhelm the world's supply of traditional follow-up telescopes. As new, comprehensive time-domain surveys become operational and wide-field multi-messenger observatories come on-line, that problem will become more acute. The goal of this workshop was to foster discussion about how autonomous robotic telescopes and small-aperture conventional telescopes can be employed in the most effective ways to help deal with the coming deluge of scientifically interesting follow-up opportunities. Discussion topics included the role of event brokers, automated event triage, the establishment of cooperative global telescope networks, and real-time coordination of observations at geographically diverse sites. It therefore included brief overviews of the current diverse landscape of telescopes and their interactions, and also considered planned and potential new facilities and operating models.

scholarly journals Recreating the OSIRIS-REx slingshot manoeuvre from a network of ground-based sensors

2020 ◽  
Vol 37 ◽  
Author(s):  
Trent Jansen-Sturgeon ◽  
Benjamin A. D. Hartig ◽  
Gregory J. Madsen ◽  
Philip A. Bland ◽  
Eleanor K. Sansom ◽  
...  
Keyword(s):  
Orbit Determination ◽  
Optical Tracking ◽  
Field Of View ◽  
Line Of Sight ◽  
Wide Field ◽  
Tracking Systems ◽  
Remote Sensors ◽  
Data Pipeline ◽  
Wide Field Of View ◽  
Successful Design

Abstract Optical tracking systems typically trade off between astrometric precision and field of view. In this work, we showcase a networked approach to optical tracking using very wide field-of-view imagers that have relatively low astrometric precision on the scheduled OSIRIS-REx slingshot manoeuvre around Earth on 22 Sep 2017. As part of a trajectory designed to get OSIRIS-REx to NEO 101955 Bennu, this flyby event was viewed from 13 remote sensors spread across Australia and New Zealand to promote triangulatable observations. Each observatory in this portable network was constructed to be as lightweight and portable as possible, with hardware based off the successful design of the Desert Fireball Network. Over a 4-h collection window, we gathered 15 439 images of the night sky in the predicted direction of the OSIRIS-REx spacecraft. Using a specially developed streak detection and orbit determination data pipeline, we detected 2 090 line-of-sight observations. Our fitted orbit was determined to be within about 10 km of orbital telemetry along the observed 109 262 km length of OSIRIS-REx trajectory, and thus demonstrating the impressive capability of a networked approach to Space Surveillance and Tracking.

scholarly journals Tiling strategies for optical follow-up of gravitational-wave triggers by telescopes with a wide field of view

2016 ◽  
Vol 592 ◽  
pp. A82 ◽  
Author(s):  
Shaon Ghosh ◽  
Steven Bloemen ◽  
Gijs Nelemans ◽  
Paul J. Groot ◽  
Larry R. Price
Keyword(s):  
Gravitational Wave ◽  
Field Of View ◽  
Wide Field ◽  
Wide Field Of View

scholarly journals Using machine learning for transient classification in searches for gravitational-wave counterparts

2020 ◽  
Vol 497 (2) ◽  
pp. 1320-1331 ◽  
Author(s):  
Cosmin Stachie ◽  
Michael W Coughlin ◽  
Nelson Christensen ◽  
Daniel Muthukrishna
Keyword(s):  
Gravitational Wave ◽  
Classification Performance ◽  
Light Curves ◽  
Wide Field ◽  
Photometric Observations ◽  
Wide Field Of View ◽  
Astronomical Object ◽  
The Many ◽  
Rule Out

ABSTRACT The large sky localization regions offered by the gravitational-wave interferometers require efficient follow-up of the many counterpart candidates identified by the wide field-of-view telescopes. Given the restricted telescope time, the creation of prioritized lists of the many identified candidates becomes mandatory. Towards this end, we use astrorapid, a multiband photometric light-curve classifier, to differentiate between kilonovae, supernovae, and other possible transients. We demonstrate our method on the photometric observations of real events. In addition, the classification performance is tested on simulated light curves, both ideally and realistically sampled. We show that after only a few days of observations of an astronomical object, it is possible to rule out candidates as supernovae and other known transients.

scholarly journals 280 one-opposition near-Earth asteroids recovered by the EURONEAR with the Isaac Newton Telescope

2018 ◽  
Vol 609 ◽  
pp. A105 ◽  
Author(s):  
O. Vaduvescu ◽  
L. Hudin ◽  
T. Mocnik ◽  
F. Char ◽  
A. Sonka ◽  
...  
Keyword(s):  
Moving Objects ◽  
Wide Field ◽  
Minor Planets ◽  
Main Belt ◽  
Isaac Newton ◽  
Isaac Newton Telescope ◽  
Fast Motion ◽  
The One ◽  
Near Earth Asteroids

Context. One-opposition near-Earth asteroids (NEAs) are growing in number, and they must be recovered to prevent loss and mismatch risk, and to improve their orbits, as they are likely to be too faint for detection in shallow surveys at future apparitions. Aims. We aimed to recover more than half of the one-opposition NEAs recommended for observations by the Minor Planet Center (MPC) using the Isaac Newton Telescope (INT) in soft-override mode and some fractions of available D-nights. During about 130 h in total between 2013 and 2016, we targeted 368 NEAs, among which 56 potentially hazardous asteroids (PHAs), observing 437 INT Wide Field Camera (WFC) fields and recovering 280 NEAs (76% of all targets). Methods. Engaging a core team of about ten students and amateurs, we used the THELI, Astrometrica, and the Find_Orb software to identify all moving objects using the blink and track-and-stack method for the faintest targets and plotting the positional uncertainty ellipse from NEODyS. Results. Most targets and recovered objects had apparent magnitudes centered around V ~ 22.8 mag, with some becoming as faint as V ~ 24 mag. One hundred and three objects (representing 28% of all targets) were recovered by EURONEAR alone by Aug. 2017. Orbital arcs were prolonged typically from a few weeks to a few years; our oldest recoveries reach 16 years. The O−C residuals for our 1854 NEA astrometric positions show that most measurements cluster closely around the origin. In addition to the recovered NEAs, 22 000 positions of about 3500 known minor planets and another 10 000 observations of about 1500 unknown objects (mostly main-belt objects) were promptly reported to the MPC by our team. Four new NEAs were discovered serendipitously in the analyzed fields and were promptly secured with the INT and other telescopes, while two more NEAs were lost due to extremely fast motion and lack of rapid follow-up time. They increase the counting to nine NEAs discovered by the EURONEAR in 2014 and 2015. Conclusions. Targeted projects to recover one-opposition NEAs are efficient in override access, especially using at least two-meter class and preferably larger field telescopes located in good sites, which appear even more efficient than the existing surveys.

scholarly journals The UTMOST survey for magnetars, intermittent pulsars, RRATs, and FRBs – I. System description and overview

2020 ◽  
Vol 492 (4) ◽  
pp. 4752-4767 ◽  
Author(s):  
V Venkatraman Krishnan ◽  
C Flynn ◽  
W Farah ◽  
A Jameson ◽  
M Bailes ◽  
...  
Keyword(s):  
Galactic Plane ◽  
Single Pulse ◽  
Wide Field ◽  
Flux Limit ◽  
Wide Field Of View ◽  
Survey Results ◽  
Average Flux ◽  
Early Survey ◽  
Radio Transients

ABSTRACT We describe the ongoing ‘survey for magnetars, intermittent pulsars, rotating radio transients, and fast radio bursts’ (SMIRF), performed using the newly refurbished UTMOST telescope. SMIRF repeatedly sweeps the southern Galactic plane performing real-time periodicity and single pulse searches, and is the first survey of its kind carried out with an interferometer. SMIRF is facilitated by a robotic scheduler which is capable of fully autonomous commensal operations. We report on the SMIRF observational parameters, the data analysis methods, the survey’s sensitivity to pulsars, techniques to mitigate radio frequency interference, and present some early survey results. UTMOST’s wide field of view permits a full sweep of the Galactic plane to be performed every fortnight, two orders of magnitude faster than previous surveys. In six months of operations from 2018 January to June, we have performed ∼10 sweeps of the Galactic plane with SMIRF. Notable blind redetections include the magnetar PSR J1622−4950, the RRAT PSR J0941−3942 and the eclipsing pulsar PSR J1748−2446A. We also report the discovery of a new pulsar, PSR J1659−54. Our follow-up of this pulsar at an average flux limit of ≤20 mJy, categorizes this as an intermittent pulsar with a high nulling fraction of <0.002.

Brief summary of Kleť photographic search programme for minor planets

1999 ◽  
Vol 173 ◽  
pp. 189-192
Author(s):  
J. Tichá ◽  
M. Tichý ◽  
Z. Moravec
Keyword(s):  
Ccd Camera ◽  
Minor Planet ◽  
Minor Planets ◽  
Main Belt

AbstractA long-term photographic search programme for minor planets was begun at the Kleť Observatory at the end of seventies using a 0.63-m Maksutov telescope, but with insufficient respect for long-arc follow-up astrometry. More than two thousand provisional designations were given to new Kleť discoveries. Since 1993 targeted follow-up astrometry of Kleť candidates has been performed with a 0.57-m reflector equipped with a CCD camera, and reliable orbits for many previous Kleť discoveries have been determined. The photographic programme results in more than 350 numbered minor planets credited to Kleť, one of the world's most prolific discovery sites. Nearly 50 per cent of them were numbered as a consequence of CCD follow-up observations since 1994.This brief summary describes the results of this Kleť photographic minor planet survey between 1977 and 1996. The majority of the Kleť photographic discoveries are main belt asteroids, but two Amor type asteroids and one Trojan have been found.

STM studies of crystal growth

1991 ◽  
Vol 49 ◽  
pp. 374-375
Author(s):  
M. G. Lagally
Keyword(s):  
Crystal Growth ◽  
Molecular Beam ◽  
Chemical Vapor ◽  
Sputter Deposition ◽  
Field Of View ◽  
Scanning Tunneling ◽  
Wide Field ◽  
Tunneling Microscopy ◽  
Wide Field Of View ◽  
The One

It has been recognized since the earliest days of crystal growth that kinetic processes of all Kinds control the nature of the growth. As the technology of crystal growth has become ever more refined, with the advent of such atomistic processes as molecular beam epitaxy, chemical vapor deposition, sputter deposition, and plasma enhanced techniques for the creation of “crystals” as little as one or a few atomic layers thick, multilayer structures, and novel materials combinations, the need to understand the mechanisms controlling the growth process is becoming more critical. Unfortunately, available techniques have not lent themselves well to obtaining a truly microscopic picture of such processes. Because of its atomic resolution on the one hand, and the achievable wide field of view on the other (of the order of micrometers) scanning tunneling microscopy (STM) gives us this opportunity. In this talk, we briefly review the types of growth kinetics measurements that can be made using STM. The use of STM for studies of kinetics is one of the more recent applications of what is itself still a very young field.

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