Telescope

The 7DT array

An array of twenty commercial 50-cm telescopes, operated as a single instrument. Off-the-shelf optics kept it inexpensive and quick to bring on line; the filter set is what makes it unusual.

20Telescopes16 online
50.8cmPrimary diameter
f/3.0Focal ratio
1.34 × 0.90°FoV per unit
Overview

One instrument in twenty parts

7DT is an array of twenty 50-cm commercial off-the-shelf telescopes. Each unit is a PlaneWave DeltaRho 500 optical tube assembly on an L-500 direct-drive mount operated in equatorial configuration, paired with a Moravian Instruments C3-61000 PRO CMOS camera — every unit identical but for the filters it carries. Sixteen of the twenty are deployed and operational as of June 2026, and the four remaining units complete the array. All operational units share a common configuration and show consistent optical performance in routine use.

Across the sixteen operational units the point-spread function measured at field center on good nights ranges from 1.4 to 2.2 arcseconds FWHM, with an array median of 2.0 arcseconds closely tracking the median site seeing. Unit-to-unit scatter in delivered FWHM is 0.2 arcseconds, and the PSF grows by 0.3 arcseconds from field center to corner while ellipticity stays below 0.1 over the central 80 percent of the field. The array behaves as a coherent set of instruments rather than sixteen independent telescopes. Median delivered FWHM has held stable to within 0.3 arcseconds since routine survey operations began in July 2024.

The 7-Dimensional Telescope array seen from the front
DeltaRho 500 Each unit is a 508 mm corrected Cassegrain on an L-500 direct-drive mount, with its own camera and filter wheel.
Performance

As measured on sky

1.4–2.2PSF FWHM at center
2.0Array median FWHM
0.2Unit-to-unit scatter
< 0.1PSF ellipticity
15–25mmagZero-point uncertainty

For the canonical 100-second exposure the 5-sigma point-source depth reaches 19.06 mag in the bluest medium band (m400) and 16.60 mag at the longest wavelength (m875), peaking at 19.61 mag in m475 near maximum system throughput. The Sloan broad bands reach 20.59, 20.25 and 19.17 mag in g, r and i. These are nominal-condition figures: seeing better than 2.0 arcseconds, airmass below 1.5, and non-bright nights.

5σ point-source depth, single 100 s exposure, nominal conditions
m400 (bluest medium band)19.06 mag
m475 (peak throughput)19.61 mag
m875 (reddest medium band)16.60 mag
Sloan g20.59 mag
Sloan r20.25 mag
Sloan i19.17 mag
Specifications

System summary

7DT system specifications — June 2026
Array
Telescopes in the array20
Currently operational16 (as of June 2026)
Field of view per pointing≈ 1.25 deg²
Spectral resolutionR = 30–70
Unit telescope
OTAPlaneWave DeltaRho 500
Optical designCorrected Cassegrain
Primary diameter50.8 cm
Focal length1537 mm
Focal ratiof/3.0
Image circle70 mm (≈ 2.6°)
MountPlaneWave L-500, direct drive
Mount slew rate20 deg s⁻¹
Camera & filters
CameraMoravian C3-61000 PRO
SensorSONY IMX455 back-illuminated CMOS
Sensor size36 × 24 mm
Sensor dimension9576 × 6388 pixels
Pixel size3.76 µm
Pixel scale0.5 arcsec
Field of view per unit1.34° × 0.90°
Filter wheel9 slots per unit
Broad bandsSloan u, g, r, i, z
Medium-band filters (design)40
Medium-band filters installed35 (as of June 2026)
Wavelength coverage375–875 nm
Medium-band FWHM14–41 nm (typ. 25–30)
Site
ObservatoryEl Sauce, Río Hurtado Valley, Chile
Coordinates30°28′16″ S, 70°45′47″ W
Altitude1600 m
Median seeing≈ 1.5 arcsec
Clear nights> 300 per year
Zenith sky brightness21.97 mag arcsec⁻²
Computing & storage
Processing serverProton — 2 × AMD EPYC 7513
CPU / memory128 cores @ 2.6 GHz / 512 GB
GPU2 × NVIDIA A100, 82 GB (NVLink)
StorageLyman 2 × 1.2 PB, Balmer 1.2 PB
Total capacity≈ 3.6 PB
Data linkKREONET, GridFTP ≈ 80 MB s⁻¹