CMOS camera


As part of a collaboration with the European Space Agency (ESA), the Schmidt telescope, located at the Centro Astronómico Hispánico en Andalucía – Calar Alto Observatory (CAHA), is equipped with a large-scale camera C5S-150 + GPS. This camera allows astronomers to observe a larger portion of the sky in a single image, thus improving the chances of detecting a missing near-Earth object. It features a novel CMOS sensor with new telescope and camera control computers.

The official list of findings with the Schmidt telescope is maintained here by the Minor Planet Center.

In a nutshell

fotoDRL

Instrument name  CMOS C5S-150
Observing technique  Direct imaging camera
Sensor  CMOS Sony IMX411ALR
Physical size

 53.42 x 40.07 mm

Resolution  14208 × 10656  pixels
Pixels size  3.76 × 3.76 μm
Scale  0.324”/px 
Field of view  76.75’ x 57.56’
 

 

Conversion factor  0.76 e-/ADU
Full well capacity  50,000 e- at gain = 0
Read-out-noise  3.52 e- at gain = 0
Shutter  Rolling Shutter (no mechanical)
 

 

 

 

 

Space Safety Programme Near Earth Objects pillars

Space Safety Programme Near Earth Objects pillars
The Schmidt telescope at Calar Alto is set to receive a key upgrade to its detector thanks to the support of the European Space Agency (ESA) within the framework of the “Work Package 2: Observations with Opportunity Telescope”.

CMOS IMX411 sensor: This state-of-the-art Sony detector features 3.76 μm pixels, high quantum efficiency (> 85 % in the visible), and high-speed readout (> 20 fps at full resolution). It will allow very wide fields to be captured without sacrificing depth or temporal resolution.

Scientific advantages:

  • Rapid imaging of large areas of the sky, ideal for Near-Earth Object (NEO) surveys and stellar variability studies.
  • Very low read noise (< 2 e⁻ RMS), benefiting observations of faint objects and low-surface-brightness targets.
  • Integration and control: ESA is funding both the hardware and the development of the remote-control electronics, integrating the camera into the observatory’s Python-based instrumentation. Additionally, WP2 includes automated reduction pipelines and real-time transient alert systems.

This upgrade places the Schmidt among the few historic Schmidt telescopes equipped with modern CMOS technology, extending its operational life and enhancing its discovery capabilities within ESA’s surveillance strategy.

 

History:

The Calar Alto Schmidt telescope has a legacy spanning more than seven decades:

Origin (1954–1980)

  • Designed by Bernhard Schmidt & Otto Heckmann and installed at the Hamburg Observatory in 1954 for wide-field photographic surveys and stellar cartography.
  • 24 × 24 cm photographic plates captured a 5.5° × 5.5° field at f/3 with two objective prisms for low-resolution spectroscopy.

Relocation and installation at Calar Alto (1980–1999)

  • In 1980, the Max-Planck-Institut für Astronomie moved it to the Sierra de los Filabres (2 168 m).
  • It was refurbished after decades of intensive use in Hamburg, adapting it for remote observing and darker skies.

Modernization and current use (2000– ...)

  • In the early 2000s it fell into disuse and was retrofitted for automated operations.
  • Since 2017, under contract with the ESA, it has been dedicated to near-Earth object (NEO) detection campaigns, providing critical data for planetary defense. The first cameras used were based on small CCD sensors: an SBIG ST-10XME (from 2015 to 2019) then an FLI ProLine PL230-42 (from 2020 until late 2025). Despite their limited field of view and efficiency, thousands of successful observations were performed. Erwin Schwab's website compiles some nice findings done with these CCD cameras.

The Schmidt telescope has received multiple mechanical and electronic upgrades at Calar Alto, culminating now with the WP2 project and the IMX411 sensor, which completely renews its focal system.

With this new camera, the Schmidt will continue to be a pillar of wide-field astronomy and a key instrument for asteroid and transient tracking, carrying on more than 70 years of observing history.

 

Technical Specifications

  
Telescope name Calar Alto Schmidt Telescope (formerly “Großer-Hamburger-Schmidtspiegel”)
Corrector plate material & diameter UBK 7, Ø 0.8 m
Primary mirror material & diameter ZK 7, Ø 1.2 m
Radius of curvature 5 m
Focal length / f-ratio 2.4 m / f/3
Construction year 1954
Manufacturer Carl Zeiss Jena, Germany
Shipped to Calar Alto & mounting 1975; installed on new Grubb-Parsons mount
SBIG ST-10XME camera (2015-12 to 2019-12)    Field of view 21.3′ × 14.3′
FLI ProLine PL230-42 camera (2020-01 to 2025-10)      Field of view 44.0′ × 44.4′; pixel size 1.29″ × 1.29″
Historical references Jochen Schramm, Sterne über Hamburg (German); Birkle, Belleman & Elsässer (1994)

 

Press Releases

 

Gallery

First light with the new camera, November 2025 by G. Bergond

M33 300s 1 500

M33 300s

Orionsatel 500

Horse Nebula 100s

NGC188 300s 500

NGC188 200s

 

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