The DFM Telescope was manufactured by DFM Engineering, Inc. in 1999. The main telescope is equipped with a five-port instrument box. The main port is called the “on-axis” port, where the optical path goes straight through the instrument box. The instrument box contains a rotating mirror that can direct the optical path out of any of the other four ports (aligned to the cardinal directions). One of these four ports (the North port) is dedicated as an off-axis auto-guiding port. The other three ports are reserved for other instrumentation and detector design.
The instrument box also contains two filter wheels (separate from the camera filter wheels described below). The primary filter wheel has six slots and is aligned with the on-axis port. The secondary filter wheel has eight slots and is aligned with the south port. More than twenty filters are available that cover wide and narrow bands from the infrared (IR) to the ultraviolet (UV).
Alongside the DFM Telescope is the Finderscope. By design, its plate scale is 180.9″/mm. However, we use a 0.5x focal reducer to bring the plate scale to 361.0″/mm and attach a ZWO Deep-Sky CMOS. This setup gives us a 2.36° x 1.58° FoV which is useful for wide-field frames and calibrating the system.
The original imaging system attained first light on August 16, 2000, and the wide-field imaging system (now retired) attained “second light” on September 23, 2004 and ran through 2020. The present configuration, described above, brought us to a “third light” in the late summer of 2022.
Site Specifications
- 39° 15′ 16.32″ N
- 76° 42′ 34.2″ W
- Elevation: 95 meters
- True north is 18° counterclockwise, with respect to the axis of the building.
Main DFM Telescope Specifications
- Ritchey–Chrétien Cassegrain, equatorial fork-mount
- Made by DFM Engineering, Inc.
- Aperture Measurement: f/8, 32″ (812 mm)
- Focal Length: 256″ (6500 mm)
- Plate Scale: 31.7″/mm
Finder Scope Specifications
- Meade 127ED f/9 APO Refractor
- Aperture Measurement: f/9, 5″ (127mm)
- Focal Length: 45″ (1140 mm)
- Plate Scale: 180.9″/mm
Capabilities
Average of 3″ seeing at zenith
14 mag limiting magnitude for point source at zenith
The Research Team is constantly working to better estimate these and other values. See the Research Tab for more information.
Computers
Control Computer
- CPU: Intel Pentium(R) 4
- GPU: Nvidia GeForce 6200
- MBo: iEi IMBA-8650GN-R22
- RAM: 2x1GB
- PSU: Standard ATX 450w
- Case: Proprietary DFM chassis/Desk
- Storage: 500GB HDD
- Other: Proprietary DFM Motor Driver ISA Card
Data Computer
- CPU: Intel i7-12700
- GPU: Nvidia RTX 3060 (Dell OEM)
- MBo: Asus TUF GAMING Z690-PLUS WIFI (DDR5 Variant)
- RAM: 2x8GB DDR5-4800Mhz
- PSU: Corsair RM 750w
- Case: Lian Li 205 Mesh RGB
- Storage: 500Gb SSD, 1TB HDD
- Other: 10Gb Ethernet Expansion Card, USB2.0-to-RS232 Expansion Card
Cameras
Currently in Use
- ZWO ASI178MM – frequently used monochrome CMOS on-axis
- ZWO ASI294MM Pro – active cooled monochrome CMOS on-axis
- ZWO ASI2600MM Pro – active cooled monochrome CMOS on spotter scope
- ZWO ASI482MC – color camera used for fun 🙂
- ZWO ASI432MM – large field of view good for solar in lunar imaging
Filter Wheels
- ZWO EFWmini – 5 x 1.25” light filters
- U – Ultraviolet
- V – Visible
- B – Blue
- R – Red
- I – Infrared