Noether Identities and Gauge-Fixing the Action for Cosmological Perturbations

ArXiv 1311.3828 (2013)

Authors:

Macarena Lagos, Máximo Bañados, Pedro G Ferreira, Sebastián García-Sáenz

Abstract:

We propose and develop a general algorithm for finding the action for cosmological perturbations which rivals the conventional, gauge-invariant approach and can be applied to theories with more than one metric. We then apply it to a particular case of bigravity, focusing on the Eddington- inspired Born-Infeld theory, and show that we can obtain a nearly scale-invariant power spectrum for both scalar and tensor primordial quantum perturbations. Unfortunately, in the case of the minimal Eddington-inspired Born-Infeld theory, we find that the tensor-to-scalar ratio of perturbations is unacceptably large. We discuss the applicability of our general method and the possibility of resurrecting the specific theory we have looked at.

EVOLUTION OF THE SIZES OF GALAXIES OVER 7 < z < 12 REVEALED BY THE 2012 HUBBLE ULTRA DEEP FIELD CAMPAIGN

The Astrophysical Journal American Astronomical Society 777:2 (2013) 155

Authors:

Yoshiaki Ono, Masami Ouchi, Emma Curtis-Lake, Matthew A Schenker, Richard S Ellis, Ross J McLure, James S Dunlop, Brant E Robertson, Anton M Koekemoer, Rebecca AA Bowler, Alexander B Rogers, Evan Schneider, Stephane Charlot, Daniel P Stark, Kazuhiro Shimasaku, Steven R Furlanetto, Michele Cirasuolo

THE 2012 HUBBLE ULTRA DEEP FIELD (UDF12): OBSERVATIONAL OVERVIEW

The Astrophysical Journal Supplement Series American Astronomical Society 209:1 (2013) 3

Authors:

Anton M Koekemoer, Richard S Ellis, Ross J McLure, James S Dunlop, Brant E Robertson, Yoshiaki Ono, Matthew A Schenker, Masami Ouchi, Rebecca AA Bowler, Alexander B Rogers, Emma Curtis-Lake, Evan Schneider, Stephane Charlot, Daniel P Stark, Steven R Furlanetto, Michele Cirasuolo, V Wild, T Targett

Measuring the conceptual understandings of citizen scientists participating in zooniverse projects: A first approach

Astronomy Education Review 12:1 (2013)

Authors:

EE Prather, S Cormier, CS Wallace, C Lintott, M Jordan Raddick, A Smith

Abstract:

The Zooniverse projects turn everyday people into "citizen scientists" who work online with real data to assist scientists in conducting research on a variety of topics related to galaxies, exoplanets, lunar craters, and solar flares, among others. This paper describes our initial study to assess the conceptual knowledge and reasoning abilities of citizen scientists participating in two Zooniverse projects: Galaxy Zoo and Moon Zoo. In order to measure their knowledge and abilities, we developed two new assessment instruments, the Zooniverse Astronomical Concept Survey (ZACS) and the Lunar Cratering Concept Inventory (LCCI). We found that citizen scientists with the highest level of participation in the Galaxy Zoo and Moon Zoo projects also have the highest average correct scores on the items of the ZACS and LCCI. However, the limited nature of the data provided by Zooniverse participants prevents us from being able to evaluate the statistical significance of this finding, and we make no claim about whether there is a causal relationship between one's participation in Galaxy Zoo or Moon Zoo and one's level of conceptual understanding or reasoning ability on the astrophysical topics assessed by the ZACS or the LCCI. Overall, both the ZACS and the LCCI provide Zooniverse's citizen scientists with items that offer a wide range of difficulties. Using the data from the small subset of participants who responded to all items of the ZACS, we found evidence suggesting the ZACS is a reliable instrument (α=0.78), although twenty-one of its forty items appear to have point biserials less than 0.3. The work reported here provides significant insight into the strengths and limitations of various methods for administering assessments to citizen scientists. Researchers who wish to study the knowledge and abilities of citizen scientists in the future should be sure to design their research methods to avoid the pitfalls identified by our initial findings. © 2013 The American Astronomical Society.

Planet Hunters. VI: An Independent Characterization of KOI-351 and Several Long Period Planet Candidates from the Kepler Archival Data

ArXiv 1310.5912 (2013)

Authors:

Joseph R Schmitt, Ji Wang, Debra A Fischer, Kian J Jek, John C Moriarty, Tabetha S Boyajian, Megan E Schwamb, Chris Lintott, Stuart Lynn, Arfon M Smith, Michael Parrish, Kevin Schawinski, Robert Simpson, Daryll LaCourse, Mark R Omohundro, Troy Winarski, Samuel Jon Goodman, Tony Jebson, Hans Martin Schwengeler, David A Paterson, Johann Sejpka, Ivan Terentev, Tom Jacobs, Nawar Alsaadi, Robert C Bailey, Tony Ginman, Pete Granado, Kristoffer Vonstad Guttormsen, Franco Mallia, Alfred L Papillon, Franco Rossi, Miguel Socolovsky

Abstract:

We report the discovery of 14 new transiting planet candidates in the Kepler field from the Planet Hunters citizen science program. None of these candidates overlapped with Kepler Objects of Interest (KOIs) at the time of submission. We report the discovery of one more addition to the six planet candidate system around KOI-351, making it the only seven planet candidate system from Kepler. Additionally, KOI-351 bears some resemblance to our own solar system, with the inner five planets ranging from Earth to mini-Neptune radii and the outer planets being gas giants; however, this system is very compact, with all seven planet candidates orbiting $\lesssim 1$ AU from their host star. A Hill stability test and an orbital integration of the system shows that the system is stable. Furthermore, we significantly add to the population of long period transiting planets; periods range from 124-904 days, eight of them more than one Earth year long. Seven of these 14 candidates reside in their host star's habitable zone.