Cosmological Search for Ultra-Light Axions

Proceedings of the 11th Patras Workshop on Axions, WIMPs and WISPs, PATRAS 2015 (2015) 3-10

Authors:

D Grin, R Hlozek, DJE Marsh, PG Ferreira

Abstract:

Ultralight axions (ULAs) with masses in the range 10-33 eV ma 10-18 eV (motivated by string theory) might contribute to the dark-matter or dark-energy density of the Universe. ULAs would suppress the growth of structure on small scales and change the shape of the cosmic microwave background (CMB) anisotropy power spectra. In this work, we compute cosmological observables over the full ULA mass range and then use them to search for evidence of ULAs using CMB temperature data from the Planck satellite, large-scale CMB polarization data from Wilkinson Microwave Anisotropy Probe (WMAP), smallerscale CMB experiments, as well as the WiggleZ galaxy-redshift survey. In the mass range 10-32 eV ma 10-25.5 eV, the ULA relic-density must obey the constraint ah2 0.006 at 95%-confidence. For ma & 10-24 eV, ULAs are indistinguishable from standard cold dark matter on the length scales probed while for ma . 10-32 eV, ULAs are allowed to compose a significant fraction of the dark energy. If primordial gravitational waves are detected, limits to the primordial isocurvature fraction will put severe constraints on ULA dark matter. In the future, weak-lensing measurements of the CMB will yield even more powerful probes of the ULA hypothesis.

Defining and Measuring Success in Online Citizen Science: A Case Study of Zooniverse Projects

Computing in Science and Engineering IEEE 17:4 (2015) 28-41

Authors:

J Cox, EY Oh, Brooke Simmons, C Lintott, K Masters, A Greenhill, G Graham, K Holmes

Abstract:

Although current literature highlights a wide variety of potential citizen science project outcomes, no prior studies have systematically assessed performance against a comprehensive set of criteria. The study reported here is the first to propose a novel framework for assessing citizen science projects against multiple dimensions of success. The authors apply this framework to a sample of projects that form part of the online Zooniverse platform and position these projects against a success matrix that measures both contribution to science and public engagement levels relative to other projects in the sample. Their results indicate that better-performing projects tend to be those that are more established, as well as those in the area of astronomy. Implications for citizen science practitioners include the need to consider the impact of core competencies on project performance, as well as the importance of relationships between the central organization and science teams.

From clicks to publications: How the public is changing the way we do research

Proceedings of Science 18-20-October-2015 (2015)

Authors:

L Trouille, C Lintott, L Fortson

Abstract:

Processing our increasingly large datasets (e.g., image, audio, video, multidimensional data, etc. poses a bottleneck for producing real scientific outcomes. Citizen science-engaging the publi in research-provides a solution, particularly when coupled with machine learning algorithm and sophisticated task allocation and retirement rules. Zooniverse is the most widely used an successful citizen science platform, with almost 1.5 million volunteers worldwide and havin supported over 50 projects across the disciplines (including ecology, archaeology, climate science oncology, physics, astronomy, and the humanities). To date, Zooniverse projects have produce over 100 peer-reviewed publications. Faced with a rapidly growing demand for citizen scienc projects, Zooniverse has launched a new 'Project Builder' interface which allows anyone to buil and maintain their own citizen science project using a set of browser-based tools.

Validation of a priori CME arrival predictions made using real‐time heliospheric imager observations

Space Weather American Geophysical Union (AGU) 13:1 (2015) 35-48

Authors:

Kimberley Tucker‐Hood, Chris Scott, Mathew Owens, David Jackson, Luke Barnard, Jackie A Davies, Steve Crothers, Chris Lintott, Robert Simpson, Neel P Savani, J Wilkinson, B Harder, GM Eriksson, EML Baeten, Lily Lau Wan Wah

RELATIVELY SUCCESSFUL

NEW SCIENTIST 228:3042 (2015) 29-33