papers

Publications (17)

cs.CV2025

Using Fixed and Mobile Eye Tracking to Understand How Visitors View Art in a Museum: A Study at the Bowes Museum, County Durham, UK

Claire Warwick, Andrew Beresford, Soazig Casteau +3

The following paper describes a collaborative project involving researchers at Durham University, and professionals at the Bowes Museum, Barnard Castle, County Durham, UK, during w…

cond-mat.mtrl-sci2015

Indium Tin Oxide film characterization using the classical Hall effect

Laurens Willems van Beveren, Evgeniy Panchenko, Nik Anachi +5

We have used the classical Hall effect to electrically characterize Indium Tin Oxide (ITO) films grown by two different techniques on silica substrates. ITO films have the unique p…

astro-ph.GA2018

LoTSS/HETDEX: Optical quasars I. Low-frequency radio properties of optically selected quasars

Gülay Gürkan, Martin Hardcastle, Philip Best +17

The radio-loud/radio-quiet (RL/RQ) dichotomy in quasars is still an open question. Although it is thought that accretion onto supermassive black holes in the centre the host galaxi…

physics.optics2020

A Single Sensor Based Multispectral Imaging Camera using a Narrow Spectral Band Colour Mosaic Integrated on the Monochrome CMOS Image Sensor

Xin He, Yajing Liu, Kumar Ganesan +8

A multispectral image camera captures image data within specific wavelength ranges in narrow wavelength bands across the electromagnetic spectrum. Images from a multispectral camer…

astro-ph.IM2020

Unveiling the rarest morphologies of the LOFAR Two-metre Sky Survey radio source population with self-organised maps

Rafaël I. J. Mostert, Kenneth J. Duncan, Huub J. A. Röttgering +11

The Low Frequency Array (LOFAR) Two-metre Sky Survey (LoTSS) is a low-frequency radio continuum survey of the Northern sky at an unparalleled resolution and sensitivity. In order t…

astro-ph.GA2018

The Causes of the Red Sequence, the Blue Cloud, the Green Valley and the Green Mountain

Stephen Eales, Maarten Baes, Nathan Bourne +23

The galaxies found in optical surveys fall in two distinct regions of a diagram of optical colour versus absolute magnitude: the red sequence and the blue cloud with the green vall…

astro-ph.IM2016

The Detailed Science Case for the Maunakea Spectroscopic Explorer: the Composition and Dynamics of the Faint Universe

Alan McConnachie, Carine Babusiaux, Michael Balogh +173

MSE is an 11.25m aperture observatory with a 1.5 square degree field of view that will be fully dedicated to multi-object spectroscopy. More than 3200 fibres will feed spectrograph…

astro-ph.GA2014

Herschel-ATLAS and ALMA: HATLAS J142935.3-002836, a lensed major merger at redshift 1.027

Hugo Messias, Simon Dye, Neil Nagar +29

[Abridged] Aims: This work focuses on one lensed system, HATLAS J142935.3-002836 (H1429-0028), selected in the Herschel-ATLAS field. Gathering a rich, multi-wavelength dataset, we…

cs.SE2025

Determining Absence of Unreasonable Risk: Approval Guidelines for an Automated Driving System Deployment

Francesca Favaro, Scott Schnelle, Laura Fraade-Blanar +6

This paper provides an overview of how the determination of absence of unreasonable risk can be operationalized. It complements previous theoretical work published by existing deve…

astro-ph.GA2015

H-ATLAS/GAMA: Quantifying the Morphological Evolution of the Galaxy Population Using Cosmic Calorimetry

Stephen Eales, Andrew Fullard, Matthew Allen +28

Using results from the Herschel Astrophysical Terrahertz Large-Area Survey and the Galaxy and Mass Assembly project, we show that, for galaxy masses above approximately 1.0e8 solar…

physics.ins-det2024

New methods of neutrino and anti-neutrino detection from 0.115 to 105 MeV

Nickolas Solomey, Mark Christl, Brian Doty +11

We have developed a neutrino detector with threshold energies from ~0.115 to 105 MeV in a clean detection mode almost completely void of accidental backgrounds. It was initially de…

astro-ph.CO2026

A JWST Paschen-alpha Calibration of the Radio Luminosity-Star Formation Rate Relation at z~1.3

Nick Seymour, Catherine Hale, Imogen Whittam +17

As radio emission from normal galaxies is a dust-free tracer of star formation, tracing the star formation history of the Universe is a key goal of the SKA and ngVLA. In order to i…

cs.RO2020

Waymo's Safety Methodologies and Safety Readiness Determinations

Nick Webb, Dan Smith, Christopher Ludwick +5

Waymo's safety methodologies, which draw on well established engineering processes and address new safety challenges specific to Automated Vehicle technology, provide a firm founda…

astro-ph.CO2011

MAGPHYS: a publicly available tool to interpret observed galaxy SEDs

Elisabete da Cunha, Stephane Charlot, Loretta Dunne +2

We present a simple, physically-motivated model to interpret consistently the emission from galaxies at ultraviolet, optical and infrared wavelengths. We combine this model with a…

astro-ph.IM2019

The Detailed Science Case for the Maunakea Spectroscopic Explorer, 2019 edition

The MSE Science Team, Carine Babusiaux, Maria Bergemann +258

(Abridged) The Maunakea Spectroscopic Explorer (MSE) is an end-to-end science platform for the design, execution and scientific exploitation of spectroscopic surveys. It will unvei…

astro-ph.GA2017

The New Galaxy Evolution Paradigm Revealed by the Herschel Surveys

Stephen Eales, Dan Smith, Nathan Bourne +22

The Herschel Space Observatory has revealed a very different galaxyscape from that shown by optical surveys which presents a challenge for galaxy-evolution models. The Herschel sur…

cs.CY2023

Building a Credible Case for Safety: Waymo's Approach for the Determination of Absence of Unreasonable Risk

Francesca Favaro, Laura Fraade-Blanar, Scott Schnelle +6

This paper presents an overview of Waymo's approach to building a reliable case for safety - a novel and thorough blueprint for use by any company building fully autonomous driving…