Everyone Counts? Design Considerations in Online Citizen Science
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Crowd Science: the Organization of Scientific Research in Open ଝ Collaborative Projects
Research Policy 43 (2014) 1–20 Contents lists available at ScienceDirect Research Policy jou rnal homepage: www.elsevier.com/locate/respol Crowd science: The organization of scientific research in open ଝ collaborative projects a,∗ b Chiara Franzoni , Henry Sauermann a Department of Management, Economics and Industrial Engineering (DIG), Politecnico di Milano, P. Leonardo da Vinci 32, Milan 20133, Italy b Georgia Institute of Technology, Scheller College of Business, 800 W. Peachtree St., Atlanta, GA 30308, USA a r t a b i s c l e i n f o t r a c t Article history: A growing amount of scientific research is done in an open collaborative fashion, in projects sometimes Received 15 November 2012 referred to as “crowd science”, “citizen science”, or “networked science”. This paper seeks to gain a more Received in revised form 12 July 2013 systematic understanding of crowd science and to provide scholars with a conceptual framework and Accepted 13 July 2013 an agenda for future research. First, we briefly present three case examples that span different fields Available online 14 August 2013 of science and illustrate the heterogeneity concerning what crowd science projects do and how they are organized. Second, we identify two fundamental elements that characterize crowd science projects Keywords: – open participation and open sharing of intermediate inputs – and distinguish crowd science from Crowd science other knowledge production regimes such as innovation contests or traditional “Mertonian” science. Citizen science Crowdsourcing Third, we explore potential knowledge-related and motivational benefits that crowd science offers over Community-based production alternative organizational modes, and potential challenges it is likely to face. -
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. -
A Citation Study of Citizen Science Projects in Space Science and Astronomy
Odenwald, S. 2018. A Citation Study of Citizen Science Projects in Space Science and Astronomy. Citizen Science: Theory and Practice, 3(2): 5, pp. 1–11. DOI: https://doi.org/10.5334/cstp.152 RESEARCH PAPER A Citation Study of Citizen Science Projects in Space Science and Astronomy Sten Odenwald This paper presents a citation study of 143 publications in refereed journals resulting from 23 citizen science (CS) projects in space science and astronomy. The projects generated a median of two papers during their average of six years of operation. The 143 papers produced 4,515 citations for a median of 10 citations/paper. These papers were compared to a uniform group of papers published in the year 2000 in refereed space science journals. The CS papers have an average annual peak citation rate that is about four times the average of the year-2000 sample. The CS citation history profiles peak within 3 years after paper publication but decline thereafter at a faster pace than the average paper published in 2000. This suggests that CS papers “burn brighter” but remain of interest for only half as long as other papers in space science and astronomy. Nevertheless, CS papers compare well with some of the most highly ranked “Top-1000” research papers of the modern era. The proportion of CS papers surpassing 200 citations is one-in-26, which is 40-fold higher than the proportion for the typical paper published in 2000. The study concludes that CS projects are not only as good as conventional non-CS research projects in generating publishable results, but can actually outperform the citation rates of the typical non-CS papers in space science and astronomy. -
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. -
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. -
Abstracts Connecting to the Boston University Network
20th Cambridge Workshop: Cool Stars, Stellar Systems, and the Sun July 29 - Aug 3, 2018 Boston / Cambridge, USA Abstracts Connecting to the Boston University Network 1. Select network ”BU Guest (unencrypted)” 2. Once connected, open a web browser and try to navigate to a website. You should be redirected to https://safeconnect.bu.edu:9443 for registration. If the page does not automatically redirect, go to bu.edu to be brought to the login page. 3. Enter the login information: Guest Username: CoolStars20 Password: CoolStars20 Click to accept the conditions then log in. ii Foreword Our story starts on January 31, 1980 when a small group of about 50 astronomers came to- gether, organized by Andrea Dupree, to discuss the results from the new high-energy satel- lites IUE and Einstein. Called “Cool Stars, Stellar Systems, and the Sun,” the meeting empha- sized the solar stellar connection and focused discussion on “several topics … in which the similarity is manifest: the structures of chromospheres and coronae, stellar activity, and the phenomena of mass loss,” according to the preface of the resulting, “Special Report of the Smithsonian Astrophysical Observatory.” We could easily have chosen the same topics for this meeting. Over the summer of 1980, the group met again in Bonas, France and then back in Cambridge in 1981. Nearly 40 years on, I am comfortable saying these workshops have evolved to be the premier conference series for cool star research. Cool Stars has been held largely biennially, alternating between North America and Europe. Over that time, the field of stellar astro- physics has been upended several times, first by results from Hubble, then ROSAT, then Keck and other large aperture ground-based adaptive optics telescopes. -
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. -
Citizen Science As a Tool for Scientific Research and Societal Benefit at NASA
https://ntrs.nasa.gov/search.jsp?R=20180001255 2019-08-30T12:26:13+00:00Z Citizen Science as a Tool for Scientific Research and Societal Benefit at NASA Dr. Amy Kaminski NASA Headquarters, USA Australian Citizen Science Association Conference February 7, 2018 • NASA’s strategic goals include advancing knowledge and opportunity in space and improving life on Earth. • We support these goals through extensive programs in space and Earth science research accomplished via space-based missions and research funding. • NASA’s “system” is configured to conduct science using (1) in-house personnel and (2) grants, contracts, and agreements with external entities (academia, industry, international space agencies). NASA’s Citizen Science Universe + NASA-funded Disk Detective JunoCam ^ Uses NASA data/assets Planet 9: Backyard Worlds * Completed/defunct +Planet Hunters # Challenge/prize competition ^Galaxy Zoo ^Radio Galaxy Zoo +Target Asteroids ^Exoplanet Explorers +Asteroid Mappers *#Asteroid Data Hunter Challenge Citizen science Asteroid Data, Education, and Tools (CADET) projects +Stardust@home *#Cassini Rings Challenge Aurorasaurus Meteor Counter +Moon Mappers ^Student Spaceflight ^Moon Zoo Experiments Program +Mercury Mappers *#Open NASA Earth Exchange Challenges NASA S’COOL NASA/USGS Adopt-a-Pixel GLOBE/GLOBE Observer +Mars Mappers Ecological forecasting using crowdsourcing (multiple projects) *Clickworkers *#Climate Resilience Data Challenge ^Planet Four *General Aviation Study of Harmful Algal Blooms ^Planet Four: Terrains Citizen Science for Earth Systems Programs (multiple projects) Planet Four: Ridges *Astrobiology Citizen Science # * Mars Balance Mass Challenge *MAPPER Extending Astrophysics Research Capabilities: Disk Detective • WISE telescope data analysis • 28,000+ volunteers with no professional training; depth of knowledge replaced by volume of participation • Speeds completion of research – 2.5 million images reviewed since 2014 • “Super users” become Finding planetary systems part of research team – with help from 28,000 named on published new colleagues. -
Zooniverse Planet Hunters: Your Feedback
Zooniverse Planet Hunters: your feedback Page 1: The Planet Hunters team needs your feedback! We are evaluating the Planet Hunters platform to understand its impact; gain a better understanding of who takes part and why volunteers engage; and explore the possible benefits and barriers to volunteers. We want to hear your feedback so we can learn how to improve Planet Hunters TESS and other projects on Zooniverse. Please complete this short survey and let us know your thoughts. This survey should take around 5-10 minutes to complete. How will my data be used? We will use your data for the purposes of understanding who is engaging with Zooniverse Planet Hunters, and exploring your experiences of the project. This feedback will inform the overall learning and evaluation of Planet Hunters. The results will be published in a case study that will be publicly available on our Planet Hunters blog page and the University of Oxford webpages. Please note, your responses will be anonymised and no names will be published. If you have a concern about any aspect of the evaluation, please email [email protected]. For Zooniverse's User Agreement and Privacy Policy, please visit www.zooniverse.org/privacy. For for further details about how your data will be used in this survey, see Privacy Notice. Who is conducting this evaluation and why? Annaleise Depper (Public Engagement with Research Evaluation Officer, University of Oxford). I work with researchers at Oxford who are engaging the public through their research and support 1 / 24 researchers to explore and evidence the impact of their engagement activities. -
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. -
Peter Pan Disks: Long-Lived Accretion Disks Around Young M Stars
Draft version January 16, 2020 Typeset using LATEX twocolumn style in AASTeX62 Peter Pan Disks: Long-lived Accretion Disks Around Young M Stars Steven M. Silverberg,1, ∗ John P. Wisniewski,2 Marc J. Kuchner,3 Kellen D. Lawson,2 Alissa S. Bans,4 John H. Debes,5 Joseph R. Biggs,6 Milton K.D. Bosch,6 Katharina Doll,6 Hugo A. Durantini Luca,6, 7 Alexandru Enachioaie,6 Joshua Hamilton,6 Jonathan Holden,6 and Michiharu Hyogo6, 8 The Disk Detective Collaboration 1MIT Kavli Institute for Astrophysics and Space Research, 77 Massachusetts Avenue, Cambridge, MA, 02139, USA 2Homer L. Dodge Department of Physics and Astronomy, University of Oklahoma, 440 W. Brooks Street, Norman, OK 73019, USA 3NASA Goddard Space Flight Center, Exoplanets and Stellar Astrophysics Laboratory, Code 667, Greenbelt, MD 20771 4Department of Physics, Emory University, 201 Dowman Drive, Atlanta, GA 30322, USA 5Space Telescope Science Institute, 3700 San Martin Dr., Baltimore, MD 21218, USA 6Disk Detective Citizen Scientist 7IATE-OAC, Universidad Nacional de C´ordoba-CONICET. Laprida 854, X5000 BGR, C´ordoba, Argentina 8Meisei University, 2-1-1 Hodokubo, Hino, Tokyo 191-0042, Japan Submitted to ApJ ABSTRACT WISEA J080822.18-644357.3, an M star in the Carina association, exhibits extreme infrared excess and accretion activity at an age greater than the expected accretion disk lifetime. We consider J0808 as the prototypical example of a class of M star accretion disks at ages & 20 Myr, which we call \Peter Pan" disks, since they apparently refuse to grow up. We present four new Peter Pan disk candidates identified via the Disk Detective citizen science project, coupled with Gaia astrometry.