Detection of Light

Detection of Light - Spring Semester 2017

Location & Time

The lectures take place in room HL 414 in the Huygens building, on Thursdays from 13:45 - 15:30 hr (unless otherwise noted - see schedule below).


The lecturer of 'Part A' is Prof. Dr. Bernhard Brandl, office: #535 (Oort building), phone (071) 527-5830, email.

'Part B' will be taught by a number of expert guest lecturers (see below).

The teaching assistant is Michael Wilby, office: #570, email.

Course level is 500. The course language is English.

Course concept and content

Detectors are the crucial link between the astronomical target and the observer. As astronomers are aiming at fainter and fainter objects the quality and calibration of the detector systems have become increasingly important. The main goal of this course is to provide an overview of the various physical principles and techniques to detect electromagnetic radiation, from the UV to the sub-millimeter.

The course is split in two parts:

'Part A' (3 ECTS) is aimed at the observational astronomer and provides an overview of common  detector technologies and their operation.  Course topics are intrinsic and extrinsic photo-conductors, photodiodes and other junction-based detectors, detector arrays, bolometers, coherent receivers, and submillimeter- and millimeterwave heterodyne receivers. The course will not only provide the physical background of the various detector technologies but also cover practical aspects, which are of general interest to the observer, such as cosmetic quality and detector artifacts, linearity and dynamical range, spectral response and bandwidth, quantum efficiency and noise.

 'Part B' (3 ECTS) can be followed by all astronomy MSc students, but is mainly aimed at students of 'Astronomy & Instrumentation' or physics.  It consists of talks on specific topics, given by renowned guest lecturers. 

Students may follow 'Part A' only, but students who want to get credits for 'Part B' must have followed 'Part A' before.

Credits and grading

'Part A' and 'Part B' count each 3 ECTS (3+3).

The grade for 'Part A' is based to 80% on the written exam and 20% on the mandatory homeworks. The exam is on 13 April, 14:00 - 17:00 hr. It is a written, "closed book" exam. Pocket calculators are required at the exam.

The credits for 'Part B' require the attendance of (most of) the lectures of 'Part B', as well as a written report based on a literature study.  The topic of the latter is closely related to one of the guest lectures.  The report has to be written within 6 weeks.  The reports will not receive a numerical grade but follow the O/V/G scheme for simplicity.


The course will be heavily based on the book Detection of Light - from the Ultraviolet to the Submillimeter, by George Rieke, 2nd Edition, 2003, Cambridge University Press, ISBN 0-521-01710-6. It is recommended that students get their own copy of this book.

Recommended for further reading are:

Schedule 'Part A'


Friday, 3-Feb-17, 09:00 - 10:45

Organization & Refresher of Solid State Physics

General: grading, exercises, book, nature of light, EM spectrum, technology, photographic plate, overview of detectors principles and types; solid state physics: atomic energy levels, crystal: bands, conductors and semi-condd., k-vector, Fermi energy

Intrinsic Photoconductors & Noise

general principle, box diagram, conductivity, mobility, tau, gain, quantum efficiency and responsivity; intro noise: poisson & Gaussian & 1/f noise; detector noise: Johnson, kTC, 1/f, BLIP

Extrinsic Photoconductors

energy bands, doping, wavelength ranges, limitations, drawbacks and comparisons; BIB detectors, photodiodes, avalanche diodes

IR Arrays & CCDs

IR arrays: principle, construction, readout electronics; CCDs: principle, back/front illuminated, thinned, readout, CTE, CT architectures, variants

IR Arrays & CCDs


Operations and Artifacts

Readout schemes: SUR, Fowler, linearity & dynamic range, data rates; cryogenics


Basic operation, time constants, superconducting, edged; comparison: responsivity, noise, NEP

Heterodyne Detectors

general principle, IF, mixing, sidebands, bandwidth, components (HEB, SIS); performance: throughput, S/N, noise and antenna temperature, comparison coherent-incoherent detectors

  13-Apr-17 14:00 - 17:00hr EXAM in room HL414  


Program 'Part B' - TBD

Date Speaker Affiliation Topic
20-04-17 Akira Endo TU Delft  
04-05-17 Michel Antolovic TU Delft  
11-05-17 Marco Beijersbergen cosine, U Leiden  
18-05-17 Alessandra Menicucci TU Delft  
01-06-17 Derek Ives - cancelled ESO  
08-06-17  Jochem Baselmans SRON/TU Delft  
15-06-17 Jian-Rong Gao SRON  








Literature/Research Projects - TBD

Lecturer Project title Student Due date
Akira Endo Astronomical Instruments and the Uncertainty Principle Dilovan Serindag 6-June-17
Akira Endo Are Photons invisible? Eimear O'Reilly 6-June-17
Michel Antolovic Photon counting Imaging Systems for Space Applications Riccardo Baldo 28-July-17
Michel Antolovic Electron multiplication in CCDs Niloofar Khorshid 10-July-17
Marco Beijersbergen Detecting X-ray Photons with a DEPFET Andrew Barr 27-June-17
Marco Beijersbergen Detecting Gamma-ray Photons Dirk van Dam 28-July-17
Alessandra Menicucci SPENVIS radiation environment and its effect on detectors: L2 Orbit John Hefele 17-July-17
Alessandra Menicucci SPENVIS radiation environment and its effect on detectors: Highly Elliptical Orbit Irene Haasnoot 17-July-17
Jochem Baselmans MKIDs and LEKIDs Max Wijsman 21-July-17
Jochem Baselmans Designing an on-chip spectrometer Louis Martin 21-July-17
J.R. Gao Should LiteBird use TES or KID detectors? Dominique Petit 28-July-17
J.R. Gao Can you use KIDs for X-ray astronomy? Hasan Albanna 28-July-17