Supporting Observatories

Mount Wilson

The success of the Astronomy Research Seminar is only possible due to the participation and support of the astronomical observatories that commit their resources and personnel to our mission. We are grateful for their past and current efforts to bring published astronomical research to an increasing number of students teams.

The very first Astronomy Research Seminar (2001) utilized a robotic telescope at the fully automated Fairborn Observatory, located on Mt. Hopkins in southern Arizona. The Fairborn Observatory’s fully automatic telescopes began operation in 1983 and have been in continuous operation since then. The pioneering Fairborn Observatory developments in automation and remote access has inspired many other collections and networks of robotic telescopes.

The majority of seminar student team observations are now made with remote, robotic telescopes, including those at the Great Basin Observatory, Las Cumbres Observatory, Sierra Remote Observatories, iTelescope, and Orion Observatory. Student teams have also made observations at large, manually-operated telescopes at Mt. Wilson Observatory (60-and 100-inch telescopes), Kitt Peak National Observatory (2.1-meter telescope), and Pine Mountain Observatory (24-inch telescope). All these observatories have been vital to the development of the Astronomy Research Seminar.

College of the Desert Mary Reagan Observatory

The Mary Reagan Observatory is located at College of the Desert’s Mecca/Thermal Campus. It features a 1.0-meter PlaneWave CDK1000 telescope inside a 16-foot AstroHaven dome. The telescope is fully robotic and serves astronomy lectures and labs as well as the Astronomy Research Seminar.

Groups of students are using the 1-meter telescope to observe double stars and Cepheid variable stars. In addition, the telescope will be used for photometry and spectroscopy to observe stars, galaxies, asteroids and comets. With its remotely accessed robotic telescope, the Mary Reagan Observatory welcomes collaboration with student researchers both locally and internationally.

Astronomy Research Seminar student teams and astronomy club members gather around the PlaneWave Instruments 1.0 meter fully robotic telescope at the College of the Desert’s Mary Reagan Observatory. Located at 138 feet below sea level, this is the lowest research observatory in the world.
The PlaneWave Instruments 1.0-meter telescope is housed in an AstroHaven dome. The observatory, which is totally robotic, is only visited by humans on rare occasions. The observatory installation by Observatory Systems was completed in a matter of days.
The 1-meter telescope, shown in the factory with engineers and supporters, is the third in a line of direct-drive telescopes. First was the Cal Poly 18-inch aperture telescope built by students at California Polytechnic State University, San Luis Obispo. Second was the 0.7-meter PlaneWave Instruments CDK-700 telescope of which 50 are conducting research every night at observatories around the world.

Las Cumbres Observatory

lco.global

Las Cumbres Observatory (LCO) is a global network of identical 0.4-, 1.0-, and 2.0-meter robotic telescopes installed in totally automated observatories. With uniform matching telescopes and instruments, continuous observations can be made seamlessly as observations are passed from one telescope to another as the Earth rotates.

A number of student seminar teams in Hawaii have made use of the 2.0-meter Faulks Telescope North. Other student teams have made observations with 0.4-meter telescope under the auspices of an LCO educational outreach program that grants observational time based on proposals.

LCO’s Faulks Telescope North<br />
LCO’s Faulks Telescope North on the summit of Haleakala on the island of Maui.  This telescope has been used by a number of seminar student teams in Hawaii with published results.<br />
LCO’s global network<br />
Two of the many 0.4=meter telescopes in LCO’s global network.  These are located on the island of Tenerife, one of the Canary Islands.  These and other LCO telescope are being used by student seminar teams to observe exoplanet transits and obtain light curves on long-period tumbling asteroids.<br />

iTelescope

www.itelescope.net

The totally robotic telescopes in the iTelescope network are located at various locations around the planet. Dozens of Astronomy Research Seminar papers have been based on iTelescope robotic observations. These papers were, for the most part, written by student teams in the greater San Diego area.

Initial use of iTelescope in research seminars was launched by Pat and Grady Boyce (Boyce Research Initiatives and Educational Foundation, BRIEF) www.boyce-astro.org at the Army and Navy Academy, and then spread by BRIEF to high schools and community colleges in the San Diego area, including Grossmont College, Miramar College, and Mesa College.

iTelescope Telescopes in Australia<br />
Although located worldwide, the largest assembly of iTelescope telescopes is in a large roll-off enclosure in Australia.  The largest of the telescope, sitting like a king in the middle of the enclosure, is a PlaneWave Instruments CDK-700 telescope, one of 50 such research telescopes spread around the world.<br />

Sierra Remote Observatories

sierra-remote.com

Sierra Remote Observatories is a collection of a number of co-located robotic observatories in the Sierra Nevada mountains of east-central California.

A number of Astronomy Research teams have used a PlaneWave Instruments CDK-17 (17-inch aperture) telescope located in the large roll-off roof enclosure at SRO.

Fairborn Observatory

schwab.tsuniv.edu

The Fairborn Observatory was founded by Russ Genet in 1979. Louis Boyd joined Russ as Co-Director in 1981. First fully automatic telescope operation was achieved in October 1983 and the pioneering Fairborn Observatory automated telescopes have been in continuous operation since then, growing in number from one 10-inch telescope to 14 fully robotic telescopes.

The Fairborn Observatory’s 2-meter telescope was the first robotic spectroscopic telescope. The Fairborn Observatory was moved from Russ’ back yard in the town of Fairborn, Ohio, to Mt. Hopkins in southern Arizona in 1985, and was then relocated south of Patagonia, Arizona ten years later. The Fairborn Observatory is credited with the first remote access in 1987.

Russell Genet Jr. (1979) centers a star at the Fairborn Observatory’s first telescope (left).  The UBV photometer, DC amplifier, high voltage power supply, and strip chart recorder are visible.  A Radio Shack TRS-80 microcomputer (right) was used for data reduction.  Also shown are a thermal printer, modem, and (upper left) a floppy drive.
Russ Genet’s Fairborn 10 robotic telescope (left) was the first to be installed at the Automatic Photoelectric Telescope (APT) Service on Mt. Hopkins in 1985.  Lou Boyd’s Phoenix 10 was the second telescope on Mt. Hopkins, while the Vanderbilt 16 (shown with Doug Hall, right) was funded by the National Science Foundation.
The three original robotic telescopes at the rear of the Fairborn Observatory are almost obscured by the four 0.8-meter telescopes that were subsequently added—completely filling up the available space.  These seven robotic telescopes observed together harmoniously every clear night on Mt. Hopkins for many years.

President

Dr. Rachel Freed

Phone

707-326-8310

InStAR

Links

Privacy

TOS

 

Links

Home
Contact Us

Newsletter

Copyright 2026 - InStaR