Michael E. Levi

A CMOS delay locked loop and sub-nanosecond time-to-digital converter chip

Many high energy physics and nuclear science applications require sub-nanosecond time resolution measurements over marry thousands of detector channels. Phase-locked loops have been employed in the past to obtain accurate time references for these measurements. An alternative solution, based on a delay-locked loop (DLL) is described. This solution allows for a very high level of integration yet still offers resolution in the sub-nanosecond regime. Two variations on this solution are outlined. A novel phase detector, based on the Muller C element, is used to implement a charge pump where the injected charge approaches zero as the loop approaches lock on the leading edge of an input clock reference. This greatly reduces timing jitter. In the second variation the loop locks to both the leading and trailing clock edges. In this second implementation, software coded layout generators are used to automatically layout a highly integrated, multi-channel, time to digital converter (TDC). Complex clock generation can be achieved by taking symmetric taps off the delay elements. The two circuits, DLL and TDC, were implemented in a CMOS 1.2 /spl mu/m and 0.8 /spl mu/m technology, respectively. Test results show a timing jitter of less than 35 ps for the DLL circuit and better than 135 ps resolution for the TDC circuit.

Quantum efficiency of a back-illuminated CCD imager: an optical approach

We have developed an optical approach for modeling the quantum efficiency (QE) of back-illuminated CCD optical imagers for astronomy. Beyond its simplicity, it has the advantage of providing a complete fringing description for a real system. Standard thin-film calculations are extended by (a) considering the CCD itself as a thin film, and (b) treating the refractive index as complex. The QE is approximated as the fraction of the light neither transmitted nor reflected, which basically says that all absorbed photons produce e-h pairs and each photoproduced e or h is collected. Near-surface effects relevant to blue response must still be treated by standard semiconductor modeling methods. A simple analytic expression describes the QE of a CCD without antireflective (AR) coatings. With AR coatings the system is more easily described by transfer matrix methods. A two-layer AR coating is tuned to give a reasonable description of standard thinned CCDs, while the measured QE of prototype LBNL totally depleted thick CCDs is well described with no adjustable parameters. Application to the new LBNL CCDs indicates that these device swill have QE > 70 percent at (lambda) equals 1000 nm and negligible fringing in optical system faster than approximately f4.0.

A 12 bit analog to digital converter for VLSI applications in nuclear science

A high-density monolithic analog-to-digital converter (ADC) has been designed and tested. The ADC features small silicon area and low power consumption for use in multichannel circuits for massively parallel particle physics detectors. The tested chip contains a linear ramp, precision high-speed comparators, a pipelined counter, and double buffering storage latches fabricated in a 2- mu m, two polysilicon CMOS technology. The prototype integrated circuit successfully combines digital frequencies in excess of 70 MHz with analog signals smaller than 1 mV. Test results show 1/4096 root-mean-square errors at conversion rates above 30 kHz, with less than 4 mW/channel power dissipation.<<ETX>>

Proton radiation damage in high-resistivity n-type silicon CCDs

A new type of p-channel CCD constructed on high-resistivity n-type silicon was exposed to 12 MeV protons at doses up to 1 X 1011 protons/cm2. The charge transfer efficiency was measured as a function of radiation dose and temperature. We previously reported that these CCDs are significantly more tolerant to radiation damage than conventional n-channel devices. In the work reported here, we used pocket pumping techniques and charge transfer efficiency measurements to determine the identity and concentrations of radiation induced traps present in the damaged devices.

Back-illuminated, fully-depleted CCD image sensors for use in optical and near-IR astronomy

Abstract Charge-coupled devices (CCDs) of novel design have been fabricated at Lawrence Berkeley National Laboratory (LBNL), and the first large-format science-grade chips for astronomical imaging are now being characterized at Lick Observatory. They are made on 300-μm thick n-type high-resistivity ( ∼10 000 Ω cm ) silicon wafers, using a technology developed at LBNL to fabricate low-leakage silicon microstrip detectors for high-energy physics. A bias voltage applied via a transparent contact on the back side fully depletes the substrate, making the entire volume photosensitive and ensuring that charge reaches the potential wells with minimal lateral diffusion. The development of a thin, transparent back-side contact compatible with fully depleted operation permits blue response comparable to that obtained with thinned CCDs. Since the entire region is active, high quantum efficiency is maintained to nearly λ=1000 nm , above which the silicon band gap effectively truncates photoproduction. Early characterization results indicate a charge transfer efficiency >0.999995, readout noise 4 es at −132°C, full well capacity >300 000 e s, and quantum efficiency >85% at λ=900 nm .

The Zwicky transient facility observing system

The Zwicky Transient Facility (ZTF) is a synoptic optical survey for high-cadence time-domain astronomy. Building upon the experience and infrastructure of the highly successful Palomar Transient Factory (PTF) team, ZTF will survey more than an order of magnitude faster than PTF in sky area and volume in order to identify rare, rapidly varying optical sources. These sources will include a trove of supernovae, exotic explosive transients, unusual stellar variables, compact binaries, active galactic nuclei, and asteroids. The single-visit depth of 20.4 mag is well matched to spectroscopic follow-up observations, while the co-added images will provide wide sky coverage 1.5 – 2 mag deeper than SDSS. The ZTF survey will cover the entire Northern Sky and revisit fields on timescales of a few hours, providing hundreds of visits per field each year, an unprecedented cadence, as required to detect fast transients and variability. This high-cadence survey is enabled by an observing system based on a new camera having 47 deg2 field of view – a factor of 6.5 greater than the existing PTF camera - equipped with fast readout electronics, a large, fast exposure shutter, faster telescope and dome drives, and various measures to optimize delivered image quality. Our project has already received an initial procurement of e2v wafer-scale CCDs and we are currently fabricating the camera cryostat. International partners and the NSF committed funds in June 2014 so construction can proceed as planned to commence engineering commissioning in 2016 and begin operations in 2017. Public release will allow broad utilization of these data by the US astronomical community. ZTF will also promote the development of transient and variable science methods in preparation for the seminal first light of LSST.

Point-spread function in depleted and partially depleted CCDs

The point spread function obtainable in an astronomical instrument using CCD readout is limited by a number of factors, among them the lateral diffusion of charge before it is collected in the potential wells. They study this problem both theoretically and experimentally, with emphasis on the thick CCDs on high-resistivity n-type substrates being developed at Lawrence Berkeley National Laboratory.

Signal processing in the front-end electronics of BaBar vertex detector

Abstract The microstrip vertex detector in BaBar experiment will be read out by a purposely designed front-end chip. The chip performs amplification and analog-to-digital conversion to retain the information of the charge induced on the readout strips. It stores the digital data during the trigger latency time and associates the incoming trigger with the relevant hit data. Data are buffered and sent off in sparsified form when a readout command is received. The present paper discusses the signal processing performed by the chip.

Precision measurements of the SLC beam energy

A method of precisely determining the beam energy in high-energy linear colliders has been developed using dipole spectrometers and synchrotron radiation detectors. The method of measurement indirectly observes the deflection of charged beams via the narrow beams of synchrotron radiation they emit. Beam lines implementing this method have been installed on the Stanford Linear Collider (SLC). An absolute energy measurement with an accuracy of better than delta E/E=5*10/sup -4/ can be achieved on a pulse-to-pulse basis. The operation of this system is described.<<ETX>>

SNAP focal plane

The proposed SuperNova/Acceleration Probe (SNAP) mission will have a two-meter class telescope delivering diffraction-limited images to an instrumented 0.7 square-degree field sensitive in the visible and near-infrared wavelength regime. We describe the requirements for the instrument suite and the evolution of the focal plane design to the present concept in which all the instrumentation -- visible and near-infrared imagers, spectrograph, and star guiders -- share one common focal plane.The proposed SuperNova/Acceleration Probe (SNAP) mission will have a two-meter class telescope delivering diffraction-limited images to an instrumented 0.7 square-degree field sensitive in the visible and near-infrared wavelength regime. We describe the requirements for the instrument suite and the evolution of the focal plane design to the present concept in which all the instrumentation -- visible and near-infrared imagers, spectrograph, and star guiders -- share one common focal plane.