Physics and Astronomy ANNUAL REVIEW 2013–14 UCL DEPARTMENT of PHYSICS and ASTRONOMY
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Javier Peralta Calvillo Generated From: Editor CVN De FECYT Date of Document: 24/01/2021 V 1.4.3 4154B7e2be6a86b67f637261e4ad3d11
Javier Peralta Calvillo Generated from: Editor CVN de FECYT Date of document: 24/01/2021 v 1.4.3 4154b7e2be6a86b67f637261e4ad3d11 This electronic file (PDF) has embedded CVN technology (CVN-XML). The CVN technology of this file allows you to export and import curricular data from and to any compatible data base. List of adapted databases available at: http://cvn.fecyt.es/ 4154b7e2be6a86b67f637261e4ad3d11 General quality indicators of scientific research This section describes briefly the main quality indicators of scientific production (periods of research activity, experience in supervising doctoral theses, total citations, articles in journals of the first quartile, H index...). It also includes other important aspects or peculiarities. My name is Javier Peralta and I was born in Algeciras (1979, Spain). I graduated in Physics at the University of La Laguna (Spain) in 2003, specializing in the fields of Astrophysics and Applied Physics. In 2009, I got an European PhD degree in Physics at the University of the Basque Country (Spain) with the highest qualification ("Cum Laude") . My PhD research, supervised by Professors Agustín Sánchez-Lavega and Ricardo Hueso, focused on the atmospheric dynamics of the planet Venus using data from the space missions Galileo and Venus Express. As a result, 6 articles were published in international peer review journals (4 of them as first author) along with more than 80 citations which allowed to be awarded in 2012 with the “Extraordinary Prize of Doctorate” granted by the University of the Basque Country. After my PhD, I spent the last 10 years (2009-2019) working in different research institutions as postdoctoral researcher: 2 years at IAA/CSIC in Granada (Spain), 3 years at the Astronomical Observatory of Lisbon (CAAUL/OAL, Portugal) and 5 years at the Institute of Space and Astronautical Science of Japan (ISAS/JAXA), funded by JAXA's International Top Young Fellowship (ITYF). -
Laboratory Astrophysics Is the Rosetta Stone That Symposium Enables Astronomers to Understand and Interpret the Distant Cosmos
IAU Symposium IAU IAU Symposium Proceedings of the International Astronomical Union Laboratory astrophysics is the Rosetta Stone that Symposium enables astronomers to understand and interpret the distant cosmos. It provides the tools to interpret and 350 guide astronomical observations and delivers the numbers needed to quantitatively model the processes 350 taking place in space, providing a bridge between 350 Laboratory 14-19 April 2019 observers and modelers. IAU Symposium 350 was 14-19 April 2019 Cambridge, United Kingdom organized by the International Astronomical Union's Cambridge, United Kingdom Laboratory Astrophysics Commission (B5), and was the Interpretation Observations to From Astrophysics: rst topical symposium on laboratory astrophysics Laboratory sponsored by the IAU. Active researchers in observational astronomy, space missions, experimental From Observations Astrophysics: and theoretical laboratory astrophysics, and Laboratory Astrophysics: From Observations astrochemistry discuss the topics and challenges facing astronomy today. Five major topics are covered, to Interpretation to Interpretation spanning from star- and planet-formation through stellar populations to extragalactic chemistry and dark matter. Within each topic, the main themes of laboratory studies, astronomical observations, and theoretical modeling are explored, demonstrating the breadth and the plurality of disciplines engaged in the growing eld of laboratory astrophysics. Edited by Proceedings of the International Astronomical Union Salama and Linnartz Farid Salama Editor in Chief: Professor Maria Teresa Lago This series contains the proceedings of major scienti c Harold Linnartz meetings held by the International Astronomical Union. Each volume contains a series of articles on a topic of current interest in astronomy, giving a timely overview of research in the eld. With contributions by leading scientists, these books are at a level suitable for research astronomers and graduate students. -
RADIAL VELOCITIES in the ZODIACAL DUST CLOUD
A SURVEY OF RADIAL VELOCITIES in the ZODIACAL DUST CLOUD Brian Harold May Astrophysics Group Department of Physics Imperial College London Thesis submitted for the Degree of Doctor of Philosophy to Imperial College of Science, Technology and Medicine London · 2007 · 2 Abstract This thesis documents the building of a pressure-scanned Fabry-Perot Spectrometer, equipped with a photomultiplier and pulse-counting electronics, and its deployment at the Observatorio del Teide at Izaña in Tenerife, at an altitude of 7,700 feet (2567 m), for the purpose of recording high-resolution spectra of the Zodiacal Light. The aim was to achieve the first systematic mapping of the MgI absorption line in the Night Sky, as a function of position in heliocentric coordinates, covering especially the plane of the ecliptic, for a wide variety of elongations from the Sun. More than 250 scans of both morning and evening Zodiacal Light were obtained, in two observing periods – September-October 1971, and April 1972. The scans, as expected, showed profiles modified by components variously Doppler-shifted with respect to the unshifted shape seen in daylight. Unexpectedly, MgI emission was also discovered. These observations covered for the first time a span of elongations from 25º East, through 180º (the Gegenschein), to 27º West, and recorded average shifts of up to six tenths of an angstrom, corresponding to a maximum radial velocity relative to the Earth of about 40 km/s. The set of spectra obtained is in this thesis compared with predictions made from a number of different models of a dust cloud, assuming various distributions of dust density as a function of position and particle size, and differing assumptions about their speed and direction. -
Panoptes, a Project Building Tool for Citizen Science
Panoptes, a Project Building Tool for Citizen Science Alex Bowyer Chris Lintott Greg Hines Campbell Allen Ed Paget [email protected] [email protected] [email protected] [email protected] [email protected] Zooniverse / Zooniverse / Zooniverse / Zooniverse / Zooniverse / University of Oxford University of Oxford University of Oxford University of Oxford Adler Planetarium Abstract and supporting projects from ecology to planetary science2. An early test project, Snapshot Supernova(Campbell and et. We will demonstrate the newly deployed Panoptes sys- al. 2015), showed that the system was able to cope with large tem for building citizen science projects which involve spikes in traffic, receiving more than a million classifications the public in the crowdsourced analysis of images. Panoptes supports projects built by the Zooniverse, the in under twenty minutes. world’s most successful collection of such projects, and Unlike previous crowdsourcing platforms, Panoptes pro- allows end users - typically scientists and researchers duces more than a list of raw classifications for project sci- with large data sets - to construct advanced classifica- entists. Standard algorithms (e.g (Hines and et. al. 2015)) ag- tion workflows using simple, browser based tools. A gregate individual users’ input into combined results. These particular strength of Panoptes is its ability to support algorithms can be used to implement complex retirement complex retirement and aggregation tools and proce- rules and task assignment, increasing the efficiency of clas- dures, as well as a mechanism for sending notifications sification. As an example of this kind of more advanced task to users as they classify. It thus provides a valuable 3 testbed for those wishing to build their own projects for assignment, we have integrated the SWAPR code devel- the purposes of investigating the behaviour of human- oped by the SpaceWarps ((et. -
Refereed Publications That Name
59 Refereed Publications Since 2011 with Named Co-Authors who are NASA Citizen Scientists Compiled by Marc Kuchner February 2021 Authors in bold are citizen scientists. Aurorasaurus Semeter, J., Hunnekuhl, M., MacDonald, E., Hirsch, M., Zeller, N., Chernenkoff, A., & Wang, J. (2020). The mysterious green streaks below STEVE. AGU Advances, 1, e2020AV000183. https://doi.org/10.1029/2020AV000183 Hunnekuhl, M., & MacDonald, E. (2020). Early ground‐based work by auroral pioneer Carl Størmer on the high‐altitude detached subauroral arcs now known as “STEVE”. Space Weather, 18, e2019SW002384. https://doi.org/10.1029/2019SW002384 S. B. Mende. B. J. Harding, & C. Turner. “Subauroral Green STEVE Arcs: Evidence for Low- Energy Excitation” Geophysical Research Letters, Volume 46, Issue 24, Pages 14256-14262 (2019) http://doi.org/10.1029/2019GL086145 S. B. Mende. & C. Turner. “Color Ratios of Subauroral (STEVE) Arcs” Journal of Geophysical Research (Space Physics),Volume 124, Issue 7, Pages 5945-5955 (2019) http://doi.org/10.1029/2019JA026851 Y. Nishimura, Y., B, Gallardo-Lacourt, B., Y, Zou, E. Mishin, D.J. Knudsen, E. F. Donovan, V. Angelopoulos, R. Raybell, “Magnetospheric Signatures of STEVE: Implications for the Magnetospheric Energy Source and Interhemispheric Conjugacy” Geophysical Research Letters, Volume 46, Issue 11, Pages 5637-5644 (2019) Elizabeth A. MacDonald, Eric Donovan, Yukitoshi Nishimura, Nathan A. Case, D. Megan Gillies, Bea Gallardo-Lacourt, William E. Archer, Emma L. Spanswick, Notanee Bourassa, Martin Connors, Matthew Heavner, Brian Jackel, Burcu Kosar, David J. Knudsen, Chris Ratzlaff and Ian Schofield, “New science in plain sight: Citizen scientists lead to the discovery of optical structure in the upper atmosphere” Science Advances, vol. -
Future Directions for Citizen Science and Public Policy
FUTURE DIRECTIONS FOR CITIZEN SCIENCE AND PUBLIC POLICY Edited by Katie Cohen and Robert Doubleday Centre for Science and Policy June 2021 FUTURE DIRECTIONS FOR CITIZEN SCIENCE AND PUBLIC POLICY Edited by Katie Cohen and Robert Doubleday Centre for Science and Policy Future directions for citizen science and public policy Open access. Some rights reserved. This work is licensed under the Creative Commons Attribution-Noncommercial 4.0 International (CC BY- NC 4.0) licence. You are free to copy and redistribute the material in any medium or format and remix, transform, and build upon the material, under the following terms: you must give appropriate credit, provide a link to the licence, and indicate if changes were made. You may do so in any reasonable manner, but not in any way that suggests the licensor endorses you or your use. To view the full licence, visit: www.creativecommons.org/licenses/by-nc/4.0/legalcode The Centre for Science and Policy gratefully acknowledges the work of Creative Commons in inspiring our approach to copyright. To find out more go to:www.creativecommons.org The Centre for Science and Policy was set up at the University of Cambridge in 2009 with the mission to improve public policy through the more effective use of evidence and expertise. CSaP does this by creating opportunities for public policy professionals and academics to learn from each other. CSaP has a unique network of over 450 Policy Fellows and 1,750 experts contributing to more dynamic and diverse scientific input to the most pressing public policy challenges. -
FINESSE and ARIEL + CASE: Dedicated Transit Spectroscopy Missions for the Post-TESS Era
FINESSE and ARIEL + CASE: Dedicated Transit Spectroscopy Missions for the Post-TESS Era Fast Infrared Exoplanet FINESSE Spectroscopy Survey Explorer Exploring the Diversity of New Worlds Around Other Stars Origins | Climate | Discovery Jacob Bean (University of Chicago) Presented on behalf of the FINESSE/CASE science team: Mark Swain (PI), Nicholas Cowan, Jonathan Fortney, Caitlin Griffith, Tiffany Kataria, Eliza Kempton, Laura Kreidberg, David Latham, Michael Line, Suvrath Mahadevan, Jorge Melendez, Julianne Moses, Vivien Parmentier, Gael Roudier, Evgenya Shkolnik, Adam Showman, Kevin Stevenson, Yuk Yung, & Robert Zellem Fast Infrared Exoplanet FINESSE Spectroscopy Survey Explorer Exploring the Diversity of New Worlds Around Other Stars **Candidate NASA MIDEX mission for launch in 2023** Objectives FINESSE will test theories of planetary origins and climate, transform comparative planetology, and open up exoplanet discovery space by performing a comprehensive, statistical, and uniform survey of transiting exoplanet atmospheres. Strategy • Transmission spectroscopy of 500 planets: Mp = few – 1,000 MEarth • Phase-resolved emission spectroscopy of a subset of 100 planets: Teq > 700 K • Focus on synergistic science with JWST: homogeneous survey, broader context, population properties, and bright stars Hardware • 75 cm aluminum Cassegrain telescope at L2 • 0.5 – 5.0 μm high-throughput prism spectrometer with R > 80 • Single HgCdTe detector with JWST heritage for science and guiding Origins | Climate | Discovery Advantages of Fast Infrared -
Brian May Plays “God Save the Queen” from the Roof of Buckingham Palace to Commemorate Queen Elizabeth II’S Golden Jubilee on June 3, 2002
Exclusive interview Brian May plays “God Save the Queen” from the roof of Buckingham Palace to commemorate Queen Elizabeth II’s Golden Jubilee on June 3, 2002. © 2002 Arthur Edwards 26 Astronomy • September 2012 As a teenager, Brian Harold May was shy, uncer- tain, insecure. “I used to think, ‘My God, I don’t know what to do, I don’t know what to wear, I don’t know who I am,’ ” he says. For a kid who didn’t know who he was or what he wanted, he had quite a future in store. Deep, abiding interests and worldwide success A life in would come on several levels, from both science and music. Like all teenagers beset by angst, it was just a matter of sorting it all out. Skiffle, stars, and 3-D A postwar baby, Brian May was born July 19, 1947. In his boyhood home on Walsham Road in Feltham on the western side of Lon- science don, England, he was an only child, the offspring of Harold, an electronics engineer and senior draftsman at the Ministry of Avia- tion, and Ruth. (Harold had served as a radio operator during World War II.) The seeds for all of May’s enduring interests came early: At age 6, Brian learned a few chords on the ukulele from his father, who was a music enthusiast. A year later, he awoke one morning to find a “Spanish guitar hanging off the end of my bed.” and At age 7, he commenced piano lessons and began playing guitar with enthusiasm, and his father’s engineering genius came in handy to fix up and repair equipment, as the family had what some called a modest income. -
Arxiv:2010.15996V1 [Astro-Ph.IM] 29 Oct 2020 Keywords: ARIEL, Exoplanets, Transit Photometry, Light Curves, Stellar Spots, Machine Learning
Draft version November 2, 2020 Typeset using LATEX default style in AASTeX63 Lessons Learned from the 1st ARIEL Machine Learning Challenge: Correcting Transiting Exoplanet Light Curves for Stellar Spots Nikolaos Nikolaou ,1 Ingo P. Waldmann ,1 Angelos Tsiaras ,1 Mario Morvan ,1 Billy Edwards ,1 Kai Hou Yip ,1 Giovanna Tinetti ,1 Subhajit Sarkar,2 James M. Dawson,2 Vadim Borisov,3 Gjergji Kasneci,3 Matej Petkovic,´ 4 Tomaˇz Stepiˇsnik,4 Tarek Al-Ubaidi,5, 6 Rachel Louise Bailey ,6 Michael Granitzer ,7 Sahib Julka ,7 Roman Kern,8 Patrick Ofner ,8 Stefan Wagner,9 Lukas Heppe ,10 Mirko Bunse ,10 and Katharina Morik 10 1Department of Physics and Astronomy, University College London, Gower Street, London, WC1E 6BT, UK 2School of Physics and Astronomy, Cardiff University, The Parade, Cardiff, CF24 3AA, UK 3Department of Computer Science, University of Tuebingen, Tuebingen, Germany 4Joˇzef Stefan Institute, Ljubljana, Slovenia 5DCCS, Austria 6Space Research Institute, Austrian Academy of Sciences, Austria 7Chair of Data Science, University of Passau, Germany 8Know-Center GmbH - Research Center for Data-Driven Business & Big Data Analytics, Austria 9Commission for Astronomy, Austrian Academy of Sciences, Graz, Austria 10Artificial Intelligence Group, TU Dortmund University, Germany Submitted to ApJ ABSTRACT The last decade has witnessed a rapid growth of the field of exoplanet discovery and characterisation. However, several big challenges remain, many of which could be addressed using machine learning methodology. For instance, the most prolific method for detecting exoplanets and inferring several of their characteristics, transit photometry, is very sensitive to the presence of stellar spots. The current practice in the literature is to identify the effects of spots visually and correct for them manually or discard the affected data. -
ADSUG Charter, Membership, Terms
ADS Users Group Welcome Kathy Flanagan STScI ADS Users Group Meeting - 11/2/2017 Membership ● Kathy Flanagan (chair) ● Carrie Anderson (NASA/GSFC Astrochemistry Lab) ● Roc Cutri (IPAC, Caltech) ● Ruth Kneale (NSO) / Line Nybakk Akerholt (U. Oslo) ● Chris Lintott (U. Oxford / Zooniverse) ● Sandy Payette / Erick Peirson (Cornell U. Library, arXiv) ● Josh Peek (STScI) ● Matthew Turk (iSchool at UIUC) ● Jake VanderPlas (U. Washington eScience Institute) ● Michael Wise (Netherlands Institute for Radio Astronomy) New Members Line Nybakk Akerholt, head Librarian, Science Library, U. Oslo. Line holds a MS in Library and Information Science from U. Oslo, where she is responsible for the library's collections in astronomy and astrophysics, and the Science library's collection in library and information science. Erick Peirson, lead system architect, arXiv-NG. Erick holds a PhD from Arizona State University (ASU) where he was a founding member of the Digital Innovation Group that explores the intersections of science and society in the digital age. 2015 SR Recommendation “The panel recommends that ADS sets up a user group, comprised of a representative user community including a member of the NASA archive community that provides guidance to ADS on: 1. Annual operations/development plans 2. Prioritization of new tools and infrastructure improvements 3. Applicability to science 4. Access to data” Charter The ADS Users Group (ADSUG) advises the ADS on the operations of the project, and recommends changes and improvements to both its services and procedures in order to maximize the scientific productivity of the community it serves. The ADSUG will advocate for the user community and provide suggestions regarding content curation, technical infrastructure, management, and priority setting. -
Annual Review 2011/12
UCL DEPARTMENT OF PHYSICS AND ASTRONOMY PHYSICS AND ASTRONOMY 2011–12 ANNUAL REVIEW PHYSICS AND ASTRONOMY ANNUAL REVIEW 2011–12 Contents Welcome It is an honour to write this WELCOME 1 introduction standing, to misquote Newton, on the shoulders of giants. COMMUNITY FOCUS 3 Jonathan Tennyson finished his Teaching Lowdown 4 tenure as Head of Department in September 2011 and so the majority Student Accolades 4 of the material contained in this Outstanding PhD Theses Published 5 Review records achievements under his leadership. In addition, Tony Career Profiles 6 Harker is currently acting as Head of Science in Action 8 Department in many matters and will continue to do so until October 2012. Alumni Matters 9 This is due to my on-going commitments with the ATLAS experiment on the ACADEMIC SHOWCASE 11 Large Hadron Collider (LHC) at CERN. Staff Accolades 12 I currently spend a large amount of my time in Geneva and I am very grateful Academic Appointments 14 to both Tony and Jonathan, as well as to other members of staff for helping Doctor of Philosophy (PhD) 15 to make this transition a success. In Portrait of Dr Phil Jones 16 particular I would also like to thank Hilary Wigmore as Departmental Manager and Raman Prinja as the new Director of RESEARCH SPOTLIGHT 17 Teaching for their continued support. Atomic, Molecular, Optical and Position Physics (AMOPP) 19 High Energy Physics (HEP) 21 “Success in such long- Condensed Matter and term, high-impact projects Materials Physics (CMMP) 25 requires sustained vision Astrophysics (Astro) 29 and dedicated work by Biological Physics (BioP) 33 excellent scientists over Research Statistics 35 many years.” Staff Snapshot 38 Underpinning this success is the outstanding quality of scientific research and education within the Department. -
The Practical Use of Cosmic Shear As a Probe of Gravity
The Practical use of Cosmic Shear as a Probe of Gravity Donnacha Kirk Thesis submitted for the Degree of Doctor of Philosophy of the University College London Department of Physics & Astronomy UNIVERSITY COLLEGE LONDON April 2011 I, Donnacha Kirk, confirm that the work presented in this thesis is my own. Where information has been derived from other sources, I confirm that this has been indicated in the thesis. Specifically: • The work on luminosity functions and red galaxy fractions in section 2.7 was done by Dr. Michael Schneider (then at Durham) as part of our collaboration on the paper Kirk et al. (2010). • The work in chapters 3 & 4 is my contribution to, and will form the substantial part of, papers in preparation with collaborators Prof. Rachel Bean and Istvan Lazslo at Cornell University. The MG effect on the linear growth function was computed by Istvan Lazslo. • The Great08 section of chapter 6 draws on my contributions to the Great08 Handbook (Bridle et al. 2009), Great08 Results Paper (Bridle et al. 2010a) and Great10 Handbook (Kitching et al. 2010). To Mum and Dad, for everything. Boyle. ... an’ it blowed, an’ blowed – blew is the right word, Joxer, but blowed is what the sailors use... Joxer. Aw, it’s a darlin’ word, a daarlin’ word. Boyle. An’, as it blowed an’ blowed, I often looked up at the sky an’ assed meself the question – what is the stars, what is the stars? Voice of Coal Vendor. Any blocks, coal-blocks; blocks, coal-blocks! Joxer. Ah, that’s the question, that’s the question – what is the stars? Boyle.