Probability Distributions.- Linear Models for Regression.- Linear Models for Classification.- Neural Networks.- Kernel Methods.- Sparse Kernel Machines.- Graphical Models.- Mixture Models and EM.- Approximate Inference.- Sampling Methods.- Continuous Latent Variables.- Sequential Data.- Combining Models.

Pattern Recognition and Machine Learning

Context. We present the second Gaia data release, Gaia DR2, consisting of astrometry, photometry, radial velocities, and information on astrophysical parameters and variability, for sources brighter than magnitude 21. In addition epoch astrometry and photometry are provided for a modest sample of minor planets in the solar system. Aims: A summary of the contents of Gaia DR2 is presented, accompanied by a discussion on the differences with respect to Gaia DR1 and an overview of the main limitations which are still present in the survey. Recommendations are made on the responsible use of Gaia DR2 results. Methods: The raw data collected with the Gaia instruments during the first 22 months of the mission have been processed by the Gaia Data Processing and Analysis Consortium (DPAC) and turned into this second data release, which represents a major advance with respect to Gaia DR1 in terms of completeness, performance, and richness of the data products. Results: Gaia DR2 contains celestial positions and the apparent brightness in G for approximately 1.7 billion sources. For 1.3 billion of those sources, parallaxes and proper motions are in addition available. The sample of sources for which variability information is provided is expanded to 0.5 million stars. This data release contains four new elements: broad-band colour information in the form of the apparent brightness in the GBP (330-680 nm) and GRP (630-1050 nm) bands is available for 1.4 billion sources; median radial velocities for some 7 million sources are presented; for between 77 and 161 million sources estimates are provided of the stellar effective temperature, extinction, reddening, and radius and luminosity; and for a pre-selected list of 14 000 minor planets in the solar system epoch astrometry and photometry are presented. Finally, Gaia DR2 also represents a new materialisation of the celestial reference frame in the optical, the Gaia-CRF2, which is the first optical reference frame based solely on extragalactic sources. There are notable changes in the photometric system and the catalogue source list with respect to Gaia DR1, and we stress the need to consider the two data releases as independent. Conclusions: Gaia DR2 represents a major achievement for the Gaia mission, delivering on the long standing promise to provide parallaxes and proper motions for over 1 billion stars, and representing a first step in the availability of complementary radial velocity and source astrophysical information for a sample of stars in the Gaia survey which covers a very substantial fraction of the volume of our galaxy.

/pdf/gaia-data-release-2-summary-of-the-contents-and-survey-539viwt72y.pdf

Gaia Data Release 2. Summary of the contents and survey properties

On 2017 August 17 a binary neutron star coalescence candidate (later designated GW170817) with merger time 12:41:04 UTC was observed through gravitational waves by the Advanced LIGO and Advanced Virgo detectors. The Fermi Gamma-ray Burst Monitor independently detected a gamma-ray burst (GRB 170817A) with a time delay of $\sim$1.7 s with respect to the merger time. From the gravitational-wave signal, the source was initially localized to a sky region of 31 deg$^2$ at a luminosity distance of $40^{+8}_{-8}$ Mpc and with component masses consistent with neutron stars. The component masses were later measured to be in the range 0.86 to 2.26 Msun. An extensive observing campaign was launched across the electromagnetic spectrum leading to the discovery of a bright optical transient (SSS17a, now with the IAU identification of AT 2017gfo) in NGC 4993 (at $\sim$40 Mpc) less than 11 hours after the merger by the One-Meter, Two Hemisphere (1M2H) team using the 1 m Swope Telescope. The optical transient was independently detected by multiple teams within an hour. Subsequent observations targeted the object and its environment. Early ultraviolet observations revealed a blue transient that faded within 48 hours. Optical and infrared observations showed a redward evolution over $\sim$10 days. Following early non-detections, X-ray and radio emission were discovered at the transient's position $\sim$9 and $\sim$16 days, respectively, after the merger. Both the X-ray and radio emission likely arise from a physical process that is distinct from the one that generates the UV/optical/near-infrared emission. No ultra-high-energy gamma-rays and no neutrino candidates consistent with the source were found in follow-up searches. (Abridged)

Multi-messenger Observations of a Binary Neutron Star Merger

This paper describes the ATLAS experiment as installed in i ts experimental cavern at point 1 at CERN. It also presents a brief overview of the expec ted performance of the detector.

http://absimage.aps.org/image/SES08/MWS_SES08-2008-020010.pdf

The ATLAS Experiment at the CERN Large Hadron Collider

基礎講座 電気泳動(Electrophoresis)

Optical sensors, based on the time correlated single photon counting (TCSPC) technique, are found in a range of applications from medical to consumer. This chapter provides an overview of the challenges in TCSPC sensor design for mobile applications. We describe the design of a proof-of-concept TCSPC optical sensor with 10 GS/s conversion rate folded flash time to digital converter (TDC) and on-chip histogram generation, designed to minimize time-domain distortion and have high power efficiency. The proof of concept IC is fabricated in STMicroelectronics 130 nm SPAD foundry process. The system consumes 178.1 pJ per photon at 899 M photon/s, and the TDC achieves state of the art 0.48 pJ/S energy efficiency.

Time of Flight Imaging and Sensing for Mobile Applications

Current 3D Time-of-Flight (ToF) systems typically offer video frame rates. However in safety critical applications, such as automotive LIDAR, faster frame rates, and a reduced latency in 3D perception, would be of considerable benefit. This paper presents initial 3D imaging results from a direct ToF SPAD image sensor, with in-pixel photon processing, that can operate at frame rates exceeding 1kFPS.

1kFPS Time-of-Flight Imaging with a 3D-stacked CMOS SPAD Sensor

We present an achromatic confocal laser scanning system capable of recording spectrally resolved fluorescence lifetime images (sFLIMs) at a rate of >8 frames per second (FPS) for a 128 x 128 image. This frame rate was achieved by optimizing the processing of lifetime calculations from previous results which demonstrated >4 FPS sFLIM imaging. The imaging system is achromatic for a spectral range of 400 - 900 nm, achieved by using reflective optics instead of a transmissive lens system, except for the primary objectives. Two excitation sources have been integrated into the system, 485 nm and 640 nm laser diodes with a pulse width of <70 ps and <90 ps respectively. Imaging is performed via a galvanometric mirror system which scans the laser beam over the sample with the ability to change the Field of View (FOV) on the fly. The collected fluorescence signal is focused into a multimode fiber via a second objective and recollimated onto a transmissive grating for spectral dispersion onto a novel complementary metal–oxide–semiconductor single photon avalanche diode (CMOS SPAD) line array sensor. This sensor can perform lifetime histogram generation on-chip and process over 16.5 Giga events/s enabling fast lifetime data acquisition. High speed sFLIM is demonstrated through imaging of convallaria majalis sections.

High speed spectral fluorescence lifetime imaging for life science applications

Light to frequency converters are used to sense the photocurrents of a buried triplejunction pixel achieving high dynamic range and low dark current colour sensing without the use of colour filters. The pixel is realised in a high voltage 0.35μm CMOS enabling sample manipulation by electrowetting and spectral sensing for a FRET biosensor.

Robert Henderson

Papers

Time of Flight Imaging and Sensing for Mobile Applications

1kFPS Time-of-Flight Imaging with a 3D-stacked CMOS SPAD Sensor

High speed spectral fluorescence lifetime imaging for life science applications

A Buried Triple-Junction Self-Reset Pixel in a 0.35Âµm High Voltage CMOS Process

2007 International Image Sensor Workshop