DFM Engineering can accommodate your specific requirements.
Inquire about custom sizes, specialized instrumentations or custom optical systems.
Without a mount capable of high speed and great precision utilizing absolute position encoders, with a high natural resonant frequency, continuous accurate tracking of many satellites is not possible.
The definitive Space Domain Awareness (SDA) telescope / camera with 26-inch aperture F/1.7 4.4-degree FOV providing optical surveillance rivaling the world's finest and most relied upon systems.
Specifically designed to detect asteroids and provide warning of an impact with the Earth. Offering F/2 and 7.5-degree FOV with a modified 110 Megapixel CCD Schmidt Camera.
Allows telescopes to perform wide field astronomy such as multi object photometry, super nova patrol, variable stars, planetary transits, occultations, orbital debris searches, asteroid searches, etc.
(Alt-Alt) Eliminates both the blind-spot at the zenith and the need to flip the telescope when it crosses the meridian. This mount offers fast tracking of debris targets in any direction across the sky.
6144 X 6144 X 10 µm detector offers up to 46fps, 95% Quantum Efficiency, full well capacity above 110ke-, 12 and 16-bit modes, for asteroid searching and Space Situational Awareness (SSA) applications.
Provides excellent pointing and tracking accuracy previously only available on larger telescopes. A 20 kg instrument load provides generous growth potential.
Our typical 0.5 & 0.6M telescopes offer a F/3 primary mirror with an effective ratio of F/8. Providing stiffness for smooth tracking and excellent accuracy.
Our 1.3M "Big-Iron" mount supports a 200kg instrument load of up to 100cm in length providing nearly unlimited instrumentation potential.
Since 1979, DFM has worked closely with leading professional astronomers to customize telescopes for specific requirements and dedicated research.
Every Optical System is custom created to meet customer specifications. Our in-house optical facility manufactures and tests all mirrors 26" and larger.
Our custom-designed optical systems may take the form of a siderostat, or a Coude' telescope of Alt-Az, Alt-Alt, or equatorial configuration.
Our seeing monitor performs sky brightness, atmospheric transmission, and extinction coefficients measurements. Performs autoguiding and star centering functions. Offers full robotic operation.
A gimbal is a gimbal is a gimble? NO it's NOT! Tracking speed and payload have a huge impact on the motors, the mount, and controls. DFM offers all 3 configurations in many sizes for various applications.
DFM has provided numerous heliostats. We have developed a special polar alignment technique using a two mirror system to fold the light downward.
Our elevation-over-azimuth scanner design are used for remote sensing, including pollution monitoring and enforcement, fugitive dust detection, clear air turbulence, and meteorological research.
These have been used for the JPL / Keck telescope testbed interferometer as well as on larger systems and provide extremely low jitter in the axis motion and in the mirror piston.
Allows handicapped access to the eyepiece by using a series of relay lenses and folding mirrors to reposition the focal plane for ADA compliance of public facilities.
Provides the option to rotate through (8) 50mm filters in one imaging session without having to switch between filters. Offers full robotic operation.
These modules provide autoguiding and star centering functions increasing your pointing accuracy by placing celestial objects in the center of the field.
Using a single channel classical photo multiplier tube (PMT) of various types, in a housing connecting an aperture wheel, filter wheel, fabry lens and/or GAM.
Allows up to 5 instruments to be mounted: N, S, E, W, and straight through. Holds the DFM filter changer. Comes with a networkable control system.
Allows selection between two different cameras, or camera and eyepiece. Allows direct imaging or fields viewing to verify and center an object.
DFM's shutter's flawless performance over ten million operational cycles and counting is useful wherever a large shutter is required: CCD cameras, spectrographs, or giant telescopes with large beam sizes.
Allowing for full robotic operation, the Smart Auto Guider™ can simultaneously support direct imaging and support a spectrograph.
A remotely controlled optical system offering classical dispersion utilizing a decker, bilateral adjustable slit, collimator, filter wheel, gratings, and detector.
Computer controlled research grade filter selection. Filter Changer unit with an 8-position filter cassette holding 125-mm X 125-mm X 9-mm thick filters.
A X-Y stage is typically needed to allow off axis guiding for long integrations (or exposures) when performing direct imaging. Custom designs available.
Provides a user-friendly interface to the telescope. Utilizing a PC, you have continual position display, status reporting, and an easy-to-use, menu-driven command set.
A 10' tall 16.5' diameter observatory, specifically created to house our LEO ScopeTM, delivers superior Delivered Image Quality (DIQ) and enhanced "dome seeing"
A 40' tall 24.5' diameter observatory features low thermal mass with a short time constant to provide for optimal observing. Integrated mirror handling equipment provides safe and easy servicing of telescope optics.
Our 20' tall 24.5' diameter observatory offers the best "dome seeing" from a modern observatory to ensure customers have the highest Delivered Image Quality (DIQ) possible for their site.