Design and Characterization of 64K Pixels Chips Working in Single Photon Processing Mode

Progress in CMOS technology and in fine pitch bump bonding has made possible the development of high granularity single photon counting detectors for X-ray imaging. This thesis studies the design and characterization of three pulse processing chips with 65536 square pixels of 55 µm x 55 µm designed in a commercial 0.25 µm 6-metal CMOS technology. The 3 chips share the same architecture and dimensions and are named Medipix2, Mpix2MXR20 and Timepix. The Medipix2 chip is a pixel detector readout chip consisting of 256 x 256 identical elements, each working in single photon counting mode for positive or negative input charge signals. The preamplifier feedback provides compensation for detector leakage current on a pixel by pixel basis. Two identical pulse height discriminators are used to define an energy window. Every event falling inside the energy window is counted with a 13 bit pseudo-random counter. The counter logic, based in a shift register, also behaves as the input/output register for the pixel. Each cell also has an 8-bit configuration register which allows masking, test-enabling and 3-bit individual threshold adjust for each discriminator. The chip can be configured in serial mode and readout either serially or in parallel. Measurements show an electronic noise ~160 e- rms with a gain of ~9 mV/ke-. The threshold spread after equalization of ~120 e- rms brings the full chip minimum detectable charge to ~1100 e-. The analog static power consumption is ~8 µW per pixel with Vdda=2.2 V. The Mpix2MXR20 is an upgraded version of the Medipix2. The main changes in the pixel consist of: an improved tolerance to radiation, improved pixel to pixel threshold uniformity, and a 14-bit counter with overflow control. The chip periphery includes new threshold DACs with smaller step size, improved linearity, and better temperature dependence. Timepix is an evolution of the Mpix2MXR20 which provides independently in each pixel information of arrival time, time-over-threshold or event counting. Timepix uses as a time reference an external clock (Ref_Clk) up to 100 MHz which is distributed all over the pixel matrix during acquisition mode. The preamplifier is improved and there is a single discriminator with 4-bit threshold adjustment in order to reduce the minimum detectable charge limit. Measurements show an electrical noise ~100 e- rms and a gain of ~16.5 mV/ke-. The threshold spread after equalization of ~35 e- rms brings the full chip minimum detectable charge either to ~650 e- with a naked chip (i.e. gas detectors) or ~750 e- when bump-bonded to a detector. The pixel static power consumption is ~13.5 µW per pixel with Vdda=2.2 V and Ref_Clk=80 MHz. This family of chips have been used for a wide variety of applications. During these studies a number of limitations have come to light. Among those are limited energy resolution and surface area. Future developments, such as Medipix3, will aim to address those limitations by carefully exploiting developments in microelectronics

A study of the interacting binary V 393 Scorpii

We present high resolution J-band spectroscopy of V 393 Sco obtained with the CRIRES at the ESO Paranal Observatory along with a discussion of archival IUE spectra and published broad band magnitudes. The best fit to the spectral energy distribution outside eclipse gives $T_{1}$= 19000 $\pm$ 500 $K$ for the gainer, $T_{2}$= 7250 $\pm$ 300 $K$ for the donor, $E(B-V)$= 0.13 $\pm$ 0.02 mag. and a distance of $d$= 523 $\pm$ 60 pc, although circumstellar material was not considered in the fit. We argue that V 393 Sco is not a member of the open cluster M7. The shape of the He I 1083 nm line shows orbital modulations that can be interpreted in terms of an optically thick pseudo-photosphere mimicking a hot B-type star and relatively large equatorial mass loss through the Lagrangian L3 point during long cycle minimum. IUE spectra show several (usually asymmetric) absorption lines from highly ionized metals and a narrow L$\alpha$ emission core on a broad absorption profile. The overall behavior of these lines suggests the existence of a wind at intermediate latitudes. From the analysis of the radial velocities we find $M_{2}/M_{1}$= 0.24 $\pm$ 0.02 and a mass function of $f$= 4.76 $\pm$ 0.24 M$\odot$. Our observations favor equatorial mass loss rather than high latitude outflows as the cause for the long variability.Comment: 13 pages, 14 figures, 7 tables. Accepted for publication in MNRAS, main journa

DESIGN OF LOW-POWER LOW-VOLTAGE SUCCESSIVE-APPROXIMATION ANALOG-TO-DIGITAL CONVERTERS

Ph.DDOCTOR OF PHILOSOPH

Optimal Area Allocation for Yield Enhancement of DAC

Práce seznamuje s metodami návrhu pro zvýšení výtěžnosti a omezení chyb ve shodných strukturách. Systematické a náhodné chyby jsou shledány zdrojem neshod mezi strukturami. Je představen model náhodných chyb za využití log-normálové hustoty pravděpodobnosti. Pomocí nové metodologie založené na celočíselném pogramování (celočíselné optimalizaci) je navržena optimalizace parametrické výtěžnosti integrovaných obvodů. Je představen algoritmus generování optimální topologie. Topologie je demonstrována na R-2R D/A převodníku a výsledky jsou porovnány s jivým řešením.Recent research in yield enhancement techniques and mitigation of device mismatch is presented. Systematic and random mismatch is studied and identified as the cause of device mismatch. Model based on log-normal PDF is introduced. Optimization of IC parameter yield is suggested and conducted with help of a new methodology based on mathematical programming. An algorithm for the impact based area allocation of critical matched devices is shown as well as algorithms for common centroid layout of different sized devices. Newly developed algorithms are presented on binary weighted R-2R DAC as it is a common IC and comparison to other solutions is given

Noise-Shaping SAR ADCs.

This work investigates hybrid analog-to-digital converters (ADCs) that combine the phenomenal energy efficiency of successive-approximation (SAR) ADCs with the resolution enhancement strategies used by noise-shaping converters. Because charge-redistribution SAR ADCs contain few active components and rely on highly digital controllers, SAR ADCs demonstrate the best energy efficiencies of all low bandwidth, moderate resolution converters (~10 bits). SAR ADCs achieve remarkable power efficiency at low resolution, but as the resolution of the SAR ADC increases, the specifications for input-referred comparator noise become more stringent and total DAC capacitance becomes too large, which degrades both power efficiency and bandwidth. For these reasons, lower resolution, lower bandwidth applications tend to favor traditional SAR ADC architectures, while higher bandwidth, higher resolution applications tend to favor pipeline-SARs. Although the use of amplifiers in pipeline-assisted SARs relaxes the comparator noise requirements and improves bandwidth, amplifier design becomes more of a challenge in highly scaled processes with reduced supply voltages. In this work, we explore the use of feedback and noise-shaping to enhance the resolution of SAR ADCs. Unlike pipeline-SARs, which require high-gain, linear amplifiers, noise-shaping SARs can be constructed using passive FIR filter structures. Furthermore, the use of feedback and noise-shaping reduces the impact of thermal kT/C noise and comparator noise. This work details and explores a new class of noise-shaping SARs.PhDElectrical EngineeringUniversity of Michigan, Horace H. Rackham School of Graduate Studieshttps://deepblue.lib.umich.edu/bitstream/2027.42/113647/1/fredenbu_1.pd