Rapid GRB Follow-up with the 2-m Robotic Liverpool Telescope

Andreja Gomboc, M. F. Bode, David Carter, Cristiano Guidorzi, Alessandro Monfardini, Carole Mundell, A. M. Newsam, Robert J. Smith, Iain Steele, J. Meaburn

Research output: Chapter in Book/Report/Conference proceedingConference contribution

2 Citations (Scopus)

Abstract

We present the capabilities of the 2‐m robotic Liverpool Telescope (LT), owned and operated by Liverpool John Moores University and situated at Observatorio Roque de Los Muchachos (ORM), La Palma. Robotic control and scheduling of the LT make it especially powerful for observations in time domain astrophysics including: (i) rapid response to Targets of Opportunity: Gamma Ray Bursts, novae, supernovae, comets; (ii) monitoring of variable objects on timescales from seconds to years, and (iii) observations simultaneous or coordinated with other facilities, both ground‐based and from space. Following a GRB alert from the Gamma Ray Observatories HETE‐2, INTEGRAL and Swift we implement a special over‐ride mode which enables observations to commence in about a minute after the alert, including optical and near infrared imaging and spectroscopy. In particular, the combination of aperture, site, instrumentation and rapid response (aided by its rapid slew and fully‐opening enclosure) makes the LT excellently suited to help solving the mystery of the origin of optically dark GRBs, for the investigation of short bursts (which currently do not have any confirmed optical counterparts) and for early optical spectroscopy of the GRB phenomenon in general. We will briefly describe the LT’s key position in the RoboNet‐1.0 network of robotic telescopes.
Original languageEnglish
Title of host publicationInteracting Binaries
Subtitle of host publicationAccretion, Evolution and Outcomes
Pages181-186
DOIs
Publication statusPublished - Oct 2005

Publication series

NameAIP Conference Proceedings
Volume797

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robotics
telescopes
Gamma Ray Observatory
novae
scheduling
enclosure
comets
gamma ray bursts
spectroscopy
supernovae
bursts
astrophysics
apertures

Cite this

Gomboc, A., Bode, M. F., Carter, D., Guidorzi, C., Monfardini, A., Mundell, C., ... Meaburn, J. (2005). Rapid GRB Follow-up with the 2-m Robotic Liverpool Telescope. In Interacting Binaries: Accretion, Evolution and Outcomes (pp. 181-186). (AIP Conference Proceedings; Vol. 797). https://doi.org/10.1063/1.2130231

Rapid GRB Follow-up with the 2-m Robotic Liverpool Telescope. / Gomboc, Andreja; Bode, M. F.; Carter, David; Guidorzi, Cristiano; Monfardini, Alessandro; Mundell, Carole; Newsam, A. M.; Smith, Robert J.; Steele, Iain; Meaburn, J.

Interacting Binaries: Accretion, Evolution and Outcomes. 2005. p. 181-186 (AIP Conference Proceedings; Vol. 797).

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Gomboc, A, Bode, MF, Carter, D, Guidorzi, C, Monfardini, A, Mundell, C, Newsam, AM, Smith, RJ, Steele, I & Meaburn, J 2005, Rapid GRB Follow-up with the 2-m Robotic Liverpool Telescope. in Interacting Binaries: Accretion, Evolution and Outcomes. AIP Conference Proceedings, vol. 797, pp. 181-186. https://doi.org/10.1063/1.2130231
Gomboc A, Bode MF, Carter D, Guidorzi C, Monfardini A, Mundell C et al. Rapid GRB Follow-up with the 2-m Robotic Liverpool Telescope. In Interacting Binaries: Accretion, Evolution and Outcomes. 2005. p. 181-186. (AIP Conference Proceedings). https://doi.org/10.1063/1.2130231
Gomboc, Andreja ; Bode, M. F. ; Carter, David ; Guidorzi, Cristiano ; Monfardini, Alessandro ; Mundell, Carole ; Newsam, A. M. ; Smith, Robert J. ; Steele, Iain ; Meaburn, J. / Rapid GRB Follow-up with the 2-m Robotic Liverpool Telescope. Interacting Binaries: Accretion, Evolution and Outcomes. 2005. pp. 181-186 (AIP Conference Proceedings).
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abstract = "We present the capabilities of the 2‐m robotic Liverpool Telescope (LT), owned and operated by Liverpool John Moores University and situated at Observatorio Roque de Los Muchachos (ORM), La Palma. Robotic control and scheduling of the LT make it especially powerful for observations in time domain astrophysics including: (i) rapid response to Targets of Opportunity: Gamma Ray Bursts, novae, supernovae, comets; (ii) monitoring of variable objects on timescales from seconds to years, and (iii) observations simultaneous or coordinated with other facilities, both ground‐based and from space. Following a GRB alert from the Gamma Ray Observatories HETE‐2, INTEGRAL and Swift we implement a special over‐ride mode which enables observations to commence in about a minute after the alert, including optical and near infrared imaging and spectroscopy. In particular, the combination of aperture, site, instrumentation and rapid response (aided by its rapid slew and fully‐opening enclosure) makes the LT excellently suited to help solving the mystery of the origin of optically dark GRBs, for the investigation of short bursts (which currently do not have any confirmed optical counterparts) and for early optical spectroscopy of the GRB phenomenon in general. We will briefly describe the LT’s key position in the RoboNet‐1.0 network of robotic telescopes.",
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AB - We present the capabilities of the 2‐m robotic Liverpool Telescope (LT), owned and operated by Liverpool John Moores University and situated at Observatorio Roque de Los Muchachos (ORM), La Palma. Robotic control and scheduling of the LT make it especially powerful for observations in time domain astrophysics including: (i) rapid response to Targets of Opportunity: Gamma Ray Bursts, novae, supernovae, comets; (ii) monitoring of variable objects on timescales from seconds to years, and (iii) observations simultaneous or coordinated with other facilities, both ground‐based and from space. Following a GRB alert from the Gamma Ray Observatories HETE‐2, INTEGRAL and Swift we implement a special over‐ride mode which enables observations to commence in about a minute after the alert, including optical and near infrared imaging and spectroscopy. In particular, the combination of aperture, site, instrumentation and rapid response (aided by its rapid slew and fully‐opening enclosure) makes the LT excellently suited to help solving the mystery of the origin of optically dark GRBs, for the investigation of short bursts (which currently do not have any confirmed optical counterparts) and for early optical spectroscopy of the GRB phenomenon in general. We will briefly describe the LT’s key position in the RoboNet‐1.0 network of robotic telescopes.

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