Faulkes Telescope North

Faulkes Telescope North
Name	Faulkes Telescope North
Organization	Las Cumbres Observatory
Location	Haleakala Observatory, Maui, Hawaii
Altitude	3055 m
Established	2006
Telescope type	2.0 m Ritchey–Chrétien reflector
Owner	Las Cumbres Observatory, Faulkes Telescope Project

Faulkes Telescope North Faulkes Telescope North is a 2.0 metre Ritchey–Chrétien research and educational telescope located at Haleakala Observatory on Maui, Hawaii. The instrument is operated by Las Cumbres Observatory and was developed with funding from the Dill Faulkes Educational Trust to support research linked to institutions such as the University of Oxford, the University of Cardiff, the Open University, and a networked array including Faulkes Telescope South. It serves both professional programs tied to observatories and citizen science initiatives coordinated with schools, universities, and public outreach partners.

Overview

The telescope provides a high-resolution optical platform for photometry, spectroscopy, and time-domain astronomy that interfaces with facilities like the Keck Observatory, Subaru Telescope, Gemini Observatory, and the Very Large Telescope for complementary multi-wavelength campaigns. It supports cooperative projects involving institutions such as the Space Telescope Science Institute, the California Institute of Technology, the Massachusetts Institute of Technology, and the Harvard–Smithsonian Center for Astrophysics, while enabling follow-up observations for missions including the Transiting Exoplanet Survey Satellite, the Zwicky Transient Facility, and the Neil Gehrels Swift Observatory. Faulkes Telescope North integrates with networks like the Global Relay of Observatories Watching Transients Happen, the Astronomical Ring for Access to Spectroscopy, and schools partnered through the Faulkes Telescope Project and Las Cumbres Observatory Global Telescope Network.

History and Development

Development began after philanthropic support by Dill Faulkes enabled collaboration with institutions including the University of London, the University of Exeter, the Royal Astronomical Society, and the Institute of Astronomy at Cambridge. The project drew technical input from companies and institutions such as ASTELCO, the Isaac Newton Group of Telescopes, the United Kingdom Astronomy Technology Centre, and the European Southern Observatory. Commissioning activities involved partnerships with NASA, the National Science Foundation, the United Kingdom Science and Technology Facilities Council, and collaborations with researchers at the University of California, Berkeley, and the University of Oxford. Upgrades and maintenance have been coordinated with organizations like the American Astronomical Society, the International Astronomical Union, the Association of Universities for Research in Astronomy, and the SETI Institute.

Location and Facility

Situated on Haleakala, the site neighbors facilities at Haleakala Observatory and shares the summit region with projects tied to the University of Hawaii and the Institute for Astronomy, and is sited in proximity to instruments such as the Pan-STARRS telescopes and the Air Force Maui Optical and Supercomputing observatory. The facility infrastructure interfaces with Maui County authorities, the State of Hawaii environmental oversight bodies, and collaborates with cultural stakeholders including the Office of Hawaiian Affairs and local Native Hawaiian organizations for site stewardship. Operations coordinate with airport authorities and emergency services on Maui and maintain data links with international data centers such as the Centre de Données astronomiques de Strasbourg, the NASA/IPAC Infrared Science Archive, and the Mikulski Archive for Space Telescopes.

Design and Instrumentation

The telescope is a 2.0 m Ritchey–Chrétien reflector built with components from specialized suppliers and integrated with control systems used by organizations like the Las Cumbres Observatory, the Faulkes Telescope Project, and collaborating university labs at the University of Southampton and Cardiff University. Instrumentation includes imaging cameras with CCDs and EMCCDs developed with input from institutions such as the European Space Agency, instrumentation groups at Caltech, and detector manufacturers used by Gemini Observatory and the Subaru Telescope. Spectrographs, filter wheels, and autoguiders allow programs in exoplanet transit photometry, supernova follow-up, and near-Earth object astrometry compatible with pipelines used by the Pan-STARRS team, the Catalina Sky Survey, and the Minor Planet Center. Control software integrates protocols common to the Global Relay of Observatories Watching Transients Happen and robotic scheduling systems developed with partners like the University of Oxford and Las Cumbres Observatory.

Operations and Educational Programs

Operations are managed by Las Cumbres Observatory and the Faulkes Telescope Project in partnership with educational bodies including the Open University, the University of Leicester, and the Royal Museums Greenwich for curriculum development and teacher training. The telescope supports outreach programs tied to Science Foundation institutions, citizen science platforms such as Zooniverse, and international collaborations with the European Southern Observatory outreach arm, the Australian Astronomical Observatory education programs, and the National Schools’ Observatory. Professional access is coordinated with research groups at institutions including the University of Cambridge, the University of Sydney, the University of Edinburgh, and the Max Planck Institute for Astronomy, while amateur groups such as the Royal Astronomical Society of Canada and the Astronomical Society of the Pacific leverage the facility for public engagement.

Notable Observations and Discoveries

Faulkes Telescope North has contributed to time-domain astronomy with follow-up observations of transients discovered by facilities including the Swift Observatory, the Zwicky Transient Facility, and the Pan-STARRS project, and has supported exoplanet transit confirmations for targets from the Kepler mission, the K2 mission, and the Transiting Exoplanet Survey Satellite in coordination with research groups at the Harvard–Smithsonian Center for Astrophysics and the Massachusetts Institute of Technology. The telescope has aided characterization of supernovae observed by the Palomar Transient Factory and the All-Sky Automated Survey for SuperNovae, and has produced astrometry for near-Earth objects that was reported to the Minor Planet Center and used by teams at Jet Propulsion Laboratory and the International Astronomical Union Minor Planet Center. Collaborations have involved contributors from the University of Oxford supernova groups, the University of California, Santa Cruz transient teams, and spectroscopic follow-up with instruments at observatories such as Gemini and Keck.

Category:Telescopes Category:Observatories in Hawaii Category:Las Cumbres Observatory