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In phase retrieval, the goal is to recover a signal $\boldsymbol{x}\in\mathbb{C}^N$ from the magnitudes of linear measurements $\boldsymbol{Ax}\in\mathbb{C}^M$. While recent theory has established that $M\approx 4N$ intensity measurements are necessary and sufficient to recover generic $\boldsymbol{x}$, there is great interest in reducing the number of measurements through the exploitation of sparse $\boldsymbol{x}$, which is known as compressive phase retrieval. In this work, we detail a novel, probabilistic approach to compressive phase retrieval based on the generalized approximate message passing (GAMP) algorithm. We then present a numerical study of the proposed PR-GAMP algorithm, demonstrating its excellent phase-transition behavior, robustness to noise, and runtime. For example, to successfully recover $K$-sparse signals, approximately $M\geq 2K\log_2(N/K)$ intensity measurements suffice when $K\ll N$ and $\boldsymbol{A}$ has i.i.d Gaussian entries. When recovering a 6k-sparse 65k-pixel grayscale image from 32k randomly masked and blurred Fourier intensity measurements, PR-GAMP achieved 99\% success rate with a median runtime of only 12.6 seconds. Compared to the recently proposed CPRL, sparse-Fienup, and GESPAR algorithms, experiments show that PR-GAMP has a superior phase transition and orders-of-magnitude faster runtimes as the problem dimensions increase.
We demonstrate a wavefront sensor based on the compressive sensing, single-pixel camera. Using a high-resolution spatial light modulator (SLM) as a variable waveplate, we weakly couple an optical field's transverse-position and polarization degrees of freedom. By placing random, binary patterns on the SLM, polarization serves as a meter for directly measuring random projections of the real and imaginary components of the wavefront. Compressive sensing techniques can then recover the wavefront. We acquire high quality, 256x256 pixel images of the wavefront from only 10,000 projections. Photon-counting detectors give sub-picowatt sensitivity.

This tutorial paper provides an exposition of a flexible geometric framework for high dimensional estimation problems with constraints. The paper develops geometric intuition about high dimensional sets, justifies it with some results of asymptotic convex geometry, and demonstrates connections between geometric results and estimation problems. The theory is illustrated with applications to sparse recovery, matrix completion, quantization, linear and logistic regression and generalized linear models.
In order to measure an event in time, you must use a shorter one. But then, to measure the shorter event, you must use an even shorter one. And so on. So, now, how do you measure the shortest event ever created?
We demonstrate experimentally algorithmic super-resolution for diagnostics of short pulses (amplitude and phase). Our approach is based on using the measured data for finding a mathematical basis in which the pulse is represented compactly.
Recurring misinterpretations due to the infamous coherent artifact imply that pulse-measurement methods operate best using single shot. Fortunately, such methods have recently been extended to pulses about 1 ns long—filling a gaping technological hole that has existed for almost 50 years.
Recently, the long-overdue study of the coherent artifact in FROG and SPIDER technique occurred, and the results were shocking for many. Simulations (see Fig. 2) involved one stable train of short pulses and two unstable trains of longer pulses, the latter comprising the stable train's short pulse plus longer random components.3,4 It was found that neither method retrieves a typical pulse in the unstable trains, but FROG's pulse lengths are at least reasonable.
Dear Igor,.....I thought you may be interested in our two new demos which can be seen in the movies below.They both won first place for the best ICASSP 2014 demo.The first is a sub-Nyquist cognitive radio system which samples signals with 6Ghz Nyquist rate at 380Mhz and recovers them in real time. The second is a sub-Nyquist radar system that samples and processes radar signals with 30Mhz Nyquist rate at 1Mhz. Clutter filtering and denoising are performed at the low rate as well.If you have any questions, I'd be happy to answer them.Best,Yonina
Hey Igor,While being in a creative mood recently I made a comics describing the principles of CS in MRI. It's linked from my CS page.Thought you might be interested.
The problem of recovering a low-rank matrix from a set of observations corrupted with gross sparse error is known as the robust principal component analysis (RPCA) and has many applications in computer vision, image processing and web data ranking. It has been shown that under certain conditions, the solution to the NP-hard RPCA problem can be obtained by solving a convex optimization problem, namely the robust principal component pursuit (RPCP). Moreover, if the observed data matrix has also been corrupted by a dense noise matrix in addition to gross sparse error, then the stable principal component pursuit (SPCP) problem is solved to recover the low-rank matrix. In this paper, we develop efficient algorithms with provable iteration complexity bounds for solving RPCP and SPCP. Numerical results on problems with millions of variables and constraints such as foreground extraction from surveillance video, shadow and specularity removal from face images and video denoising from heavily corrupted data show that our algorithms are competitive to current state-of-the-art solvers for RPCP and SPCP in terms of accuracy and speed.