Putting the ‘I’ in Science 1.6 Million Registered Users
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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. -
Planet Hunters, Zooniverse Evaluation Report
Planet Hunters | Evaluation Report 2019 Planet Hunters, Zooniverse Evaluation report Authored by Dr Annaleise Depper Evaluation Officer, Public Engagement with Research Research Services, University of Oxford 1 Planet Hunters | Evaluation Report 2019 Contents 1. Key findings and highlights ..................................................................................... 3 2. Introduction ............................................................................................................ 4 3. Evaluating Planet Hunters ....................................................................................... 5 4. Exploring impacts and outcomes on citizen scientists ............................................. 6 4.1 Increased knowledge and understanding of Astronomy ..................................................................... 7 4.2 An enjoyable and interesting experience ......................................................................................... 12 4.3 Raised aspirations and interests in Astronomy ................................................................................ 13 4.4 Feeling of pride and satisfaction in helping the scientific community ............................................... 17 4.5 Benefits to individual wellbeing ...................................................................................................... 19 5. Learning from the evaluation ................................................................................ 20 5.1 Motivations for taking part in Planet Hunters -
Zooniverse: Observing the World's Largest Citizen Science Platform
Zooniverse: Observing the World’s Largest Citizen Science Platform Robert Simpson Kevin R. Page David De Roure Department of Physics Oxford e-Research Centre Oxford e-Research Centre University of Oxford University of Oxford University of Oxford United Kingdom United Kingdom United Kingdom [email protected] [email protected] [email protected] ABSTRACT data is shown to users in the form of images, video and au- This paper introduces the Zooniverse citizen science project dio via one of the Zooniverse websites. Volunteers are shown and software framework, outlining its structure from an ob- how to perform that required analysis via a simple guide or servatory perspective: both as an observable web-based sys- tutorial such that they can then identify, classify, mark, and tem in itself, and as an example of a platform iteratively label them as researchers would do. developed according to real-world deployment and used at The first Zooniverse project, Galaxy Zoo [4, 3], launched scale. We include details of the technical architecture of Zo- in July 2007 and successfully engaged 165,000 volunteers in oniverse, including the mechanisms for data gathering across the morphological classification of images of galaxies. The the Zooniverse operation, access, and analysis. We consider early success of this first project led the team behind it to the lessons that can be drawn from the experience of design- explore new research domains and types of task and user ing and running Zooniverse, and how this might inform de- interface. velopment of other web observatories. -
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. -
Citizen Scientists Discover Extremely Cold Brown Dwarfs
Citizen Scientists Discover Extremely Cold Brown Dwarfs Aaron Meisner (NSF’s NOIRLab) [email protected] ; (650) 714-8643 Backyard Worlds: Planet 9 Collaboration CatWISE Team NOIRLab/NSF/AURA/P. Marenfeld The time-honored quest to find our Sun’s closest neighbors NASA/Penn State University The time-honored quest to find our Sun’s closest neighbors discovered recently by NASA’s Wide-field Infrared Survey Explorer (WISE) mission NASA/Penn State University DESI imaging processed a quarter petabyte of raw WISE data to create the deepest, most comprehensive all-sky infrared maps the Backyard Worlds: Planet 9 citizen science project • Launched in February 2017 via Zooniverse • More than 7 million user ‘classifications’ • Over 64,000 registered users • Roughly 150,000 unique contributors • Participants from all 50 states, plus Puerto Rico and DC • 167 countries represented today’s news: best ever 3D map of brown dwarfs in the Sun’s cosmic neighborhood Lead author: J. Davy Kirkpatrick (Caltech/IPAC) Video: Jackie Faherty (AMNH)/OpenSpace 3,000 Backyard Worlds brown dwarf discoveries: more than 2 per day! Video: Jonathan Gagné (Rio Tinto Alcan Planetarium) surprise: Sun’s nearest neighbors even weirder than previously thought WISE 0830+2837, prior literature discovered by Backyard Backyard Worlds, Worlds citizen scientist CatWISE Dan Caselden – the WISE 0855, the second coldest known coldest known brown dwarf? brown dwarf, still stands alone! 0830+2837 Bardalez Gagliuffi et al. (2020) warmest coolest observing citizen scientist discoveries with premier telescopes Gemini NASA IRTF Blanco Spitzer Keck Hubble crucial distance estimates are based on Spitzer Space Telescope follow-up (Kirkpatrick et al., in press) conclusion • With help from DESI imaging sky maps and citizen scientists, we’ve published the best ever 3D census of nearby brown dwarfs. -
Citizen ASAS-SN: Citizen Science with the All-Sky Automated Survey for Supernovae (ASAS-SN)
Draft version March 4, 2021 Typeset using LATEX default style in AASTeX63 Citizen ASAS-SN: Citizen Science with The All-Sky Automated Survey for SuperNovae (ASAS-SN) C. T. Christy,1 T. Jayasinghe,1 K. Z. Stanek,1 C. S. Kochanek,1 Z. Way,1 J. L. Prieto,2 B. J. Shappee,3 T. W.-S. Holoien,4, ∗ and T. A. Thompson1 1Department of Astronomy, The Ohio State University, 140 West 18th Avenue, Columbus, OH 43210, USA 2N´ucleo de Astronom´ıa,Universidad Diego Portales, Av. Ej´ercito 441, Santiago, Chile 3Institute for Astronomy, University of Hawai'i, 2680 Woodlawn Drive, Honolulu, HI 96822,USA 4The Observatories of the Carnegie Institution for Science, 813 Santa Barbara Street, Pasadena, CA 91101, USA ABSTRACT We present \Citizen ASAS-SN", a citizen science project hosted on the Zooniverse platform which utilizes data from the All-Sky Automated Survey for SuperNovae (ASAS-SN). Volunteers are presented with ASAS-SN g-band light curves of variable star candidates. The classification workflow allows volunteers to classify these sources into major variable groups, while also allowing for the identification of unique variable stars for additional follow-up. Keywords: Variable Stars, Light Curve Classification 1. INTRODUCTION ASAS-SN is a wide-field photometric survey that monitors the entire night sky using 20 telescopes located in both hemispheres (Shappee et al. 2014; Kochanek et al. 2017). The field of view of an ASAS-SN camera is 4.5 deg2, the pixel scale is 800: 0 and the FWHM is ∼2 pixels. ASAS-SN uses image subtraction (Alard & Lupton 1998) for the detection of transients and to generate light curves. -
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. -
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. -
Moedal and the Zooniverse: Harnessing Citizen Science for New Physics Searches
Twitter: @twhyntie MoEDAL and the Zooniverse: Harnessing Citizen Science for new physics searches T. Whyntie a,b a Langton Star Centre, b Queen Mary University of London MoEDAL Software Meeting Wednesday 18th March 2015 Overview • The Zooniverse: - Example: The Milky Way Project. • Panoptes – Zooniverse for all. • Zooniverse and MoEDAL: - Suggested plan for NTD scans; - Using the Worldwide LHC Computing Grid (wLCG). • Questions for the Collaboration. T. Whyntie (Langton Star Centre) #MoEDAL Software Meeting 2 The Zooniverse • World-leading Citizen Science: - https://www.zooniverse.org/ - “Real Science Online” • Led by Prof. Chris Lintott (Uni. Oxford, BBC Sky At Night). • 1,301,214 users as of 13:49 GMT Wednesday 18th March 2015. • Started in astrophysics, now covers many disciplines (including particle CC BY-SA 3.0: Image credit physics – see Higgs Hunters). • Powered by Amazon Web Services. T. Whyntie (Langton Star Centre) #MoEDAL Software Meeting 3 An example: The Milky Way Project • Finding dust bubbles in IR data from the Spitzer Space Telescope: http://www.milkywayproject.org • Draw circles on the images to indicate presence, size and shape of bubbles. • Also look for green EGOs. • And anything else that’s odd – the real power of Citizen Science! • Images classified multiple times by many users. T. Whyntie (Langton Star Centre) #MoEDAL Software Meeting 4 T. Whyntie (Langton Star Centre) #MoEDAL Software Meeting 5 Panoptes – Zooniverse for All • The Zooniverse team are developing a tool to allow anyone to assemble their own Citizen Science projects: Panoptes - Panoptes (API): https://github.com/zooniverse/Panoptes - Front End: https://github.com/zooniverse/Panoptes-Front-End/ • Requirements for setting up a project: - Subject sets – images to be classified by the Zooniverse Users (ZUs); - Workflow – series of questions and tasks to be performed by ZUs resulting in a “classification” for each subject; - Science case and background material to provide context.