Astronomy

An overview of Andor's solutions for Astronomy

Astronomy

Two interacting galaxies, M51 (Whirlpool Galaxy) and NGC 5195. Courtesy of Prof. Andrzej Pigulski, Wroclaw University, Poland

The high sensitivity, ultra-low noise performance of Andor Technology's vacuum Thermoelectric (TE) cooled CCD and Electron Multiplying CCD (EMCCD) cameras is well suited to a diversity of demanding astronomy applications.

The industry-leading TE vacuum cooling of the large area iKon CCD range, enable extensive field of view observation, coupled with long exposure times for deep space imaging. EMCCD technology (in the form of Andor's award-winning iXon3 EMCCD Camera range) has proven highly effective for Single Photon Counting, Lucky Astronomy and also Adaptive Optics.

Now, Andor have brought EMCCD single photon sensitivity to the mainstream astronomy community with the new low-cost Luca EMCCD cameras.

26 Sep 2006 Andor Cameras Help Astronomers Find Planets Around Distant Stars

The choice whether or not to opt for EMCCD for astronomy depends very much on your ability to employ longer exposure times to collect enough signal.

The rule of thumb is that if long exposures and slower pixel readout speeds can routinely be employed, such that enough photons can be collected to significantly overcome the read noise floor, then a low-noise, deep-cooled, back illuminated iKon slow-scan camera platform is recommended.

Finally, it should be remembered that EMCCDs can essentially be made single photon sensitive and can even be used to count individual photons!

Multimedia Library
Application Images (7)
Application Movies (2)
Publications Database
S. BukvicExperimental Stark widths in the Pb IV and Pb V spectra2011
T. SagunerA spectroscopic survey of faint, high-Galactic-latitude red clump stars2011
Fang ZhangOn the fluorescence of C60 at room temperature2010
T. Kotani, S. Laco...Pupil remapping for high contrast astronomy: results from an optical testbed2009
B. S. Lanchester, ...Simultaneous imaging of aurora on small scale in OI (777.4 nm) and N21P to estimate energy and flux of precipitation2009
R. Baranowski?, R....V440 Per: the longest period overtone Cepheid2009
G. A. Swartzlander...Astronomical demonstration of an optical vortex coronagraph2008
A. H. WillitsfordRESONANCE RAMAN SPECTROSCOPY IN THE ULTRAVIOLET USING A TUNABLE LASER2008
J. M. Sullivan, M....An optical study of multiple NEIAL events driven by low energy electron precipitation2008
H. Dahlgren, N. Iv...Morphology and dynamics of aurora at fine scale: first results from the ASK instrument2008
A. N. WenzFew-Body Physics in a Three-Component Fermi Gas2008
M.W. Noble, D. M. ...Observing the Solar Corona with a Tunable Fabry-Perot Filter2008
M. Noble, D. Rust,...Observing the Solar Corona with a Tunable Fabry-Perot Filter2008
K. Ahn, J. Chae, H...CAPABILITY OF THE FAST IMAGING SOLAR SPECTROGRAPH ON NST/BBSO FOR OBSERVING FILAMENTS/PROMINENCES AT THE SPECTRAL LINES H, Ca II 8542, AND Ca II K2008
W. FongExtrasolar Planet Transit Photometry at Wallace Astrophysical Observatory2008
E. M. Griffin, A. ...Upper thermospheric neutral wind and temperature measurements from an extended spatial field2008
D. J. Pinfield, M....Mining the Next Generation of Surveys for Cool Star Science2008
C. Grec, C. Aime, ...Contrast inversion in the 557:6 nm line detected with diferential speckle interferometry2007
T. F. Blake, S. C....Enhancing the resolution of spectral images from the Advanced Electro-Optical System Spectral Imaging Sensor2007
A. A. S. Gulbis, J...Charon’s radius and atmospheric constraints from observations of a stellar occultation2006
A.A.S. Gulbis, J.L...Electron-Multiplying CCD Imaging: Effectiveness for Stellar Occultations by Faint Objects2006
V. J. ChambersDesign of a Steerable Two-beam System for Simultaneous On- and Off-axis Imaging with the NUI Galway L3-CCD Camera2006
S. P. Souza, B. A....POETS: Portable Occultation, Eclipse, and Transit System2006
V. Shimansky, N. A...The new pre-cataclysmic binary PG 2200+0852006
K. K. Ghosh, V. Su...RBS 1032: a dwarf-nucleated spheroidal galaxy with an intermediate-mass black hole hosted in a globular cluster2006
M. BurmeisterEvidence for bipolar jets from the optical spectra of the prototypical symbiotic star Z Andromedae2006
A. Blazit, E. Thi´...CPNG-Algol: photon-counting cameras for visible interferometry2005
A. M. Cherepashchu...INTEGRAL observations of SS433: Results of a coordinated campaign2005
C. K. Hoegemann, J...Hybrid Instrument for Turbulence Detection: Wavefront Sensing and Scintillation Detection in a Fully Automatic Device2004
R. Wilson, J. Bate...Development of a Portable SLODAR Turbulence Profiler2004
L. M. R. Gartside,...Calibration of an intensified CCD camera at low light levels
A.A.S. Gulbis, J.L...Recent Stellar Occultation Observations Using High-Speed, Portable Camera Systems
I. DicaireKinematics of the SINGS Nearby Galaxies Survey – II