Zobrazeno 1 - 4
of 4
pro vyhledávání: '"Evan J. Arena"'
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 501:4103-4109
Canonically, elliptical galaxies might be expected to have a perfect rotational symmetry, making them ideal targets for flexion studies - however, this assumption hasn't been tested. We have undertaken an analysis of low and high redshift galaxy cata
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6c21ce1dc2db1db96f0bc11cfb7fcfcd
https://doi.org/10.1093/mnras/staa3928
https://doi.org/10.1093/mnras/staa3928
Cosmic flexion, like cosmic shear, is a correlation function whose signal originates from the large-scale structure of the universe. Building on the observational success of cosmic shear, along with the unprecedented quality of large-scale cosmologic
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f56da0aee96959982fa81b263b827fbd
Autor:
David Rapetti, Zeeshan Ahmed, Philip Bull, Kavilan Moodley, Lloyd Knox, Moritz Münchmeyer, Laura Newburgh, Alexander A. Kaurov, Joshua S. Dillon, Erin S. Sheldon, Dionysios Karagiannis, Adrian Liu, Daniel C. Jacobs, Evan J. Arena, Paul O'Connor, J. Richard Shaw, Simon Foreman, Kiyoshi Masui, Neelima Sehgal, Peter T. Timbie, Andrei Nomerotski, Dan Green, Tzu-Ching Chang, Alexander van Engelen, Olivier Perdereau, Adam P. Beardsley, Emanuele Castorina, Albert Stebbins, Aaron Ewall-Wice, Simone Ferraro, David Alonso, Paul Stankus, Chris Sheehy, Emily Kuhn, Benjamin Saliwanchik, Gilbert Holder, Kevin Bandura, Thomas McClintock, Tracy R. Slatyer, Dallas Wulf, Romeel Davé, Eva Silverstein, Yin-Zhe Ma, Francisco Villaescusa-Navarro, Anže Slosar, David Parkinson, William Tyndall, Josef Frisch, Gregory S. Tucker, Hamsa Padmanabhan, Reza Ansari, Andrej Obuljen, R. Shirley, Mustafa A. Amin
The paper outlines research and development needed over the next decade to enable three-dimension mapping of the Universe using the 21 cm line of neutral hydrogen.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::6d354ae952b501ad6e28ba807b0f78ba
https://doi.org/10.2172/1558438
https://doi.org/10.2172/1558438
Autor:
Surjeet Rajendran, Emmanuel Schaan, Albert Stebbins, Thomas McClintock, Andrej Obuljen, Joshua S. Dillon, Simone Ferraro, J. Xavier Prochaska, Moritz Münchmeyer, R. Shirley, J. Richard Shaw, Kavilan Moodley, Marilena LoVerde, Cherry Ng, Francisco Villaescusa Navarro, Tzu-Ching Chang, Laura Newburgh, Nicholas Battaglia, David Rapetti, Anze Slosar, Lloyd Knox, Liam Connor, Jonathan Blazek, Eva Silverstein, Zeeshan Ahmed, Hamsa Padmanabhan, Erin S. Sheldon, Cora Dvorkin, Daniel C. Jacobs, Raphael Flauger, Evan J. Arena, Benjamin Saliwanchik, Gilbert Holder, Philip Bull, David Parkinson, Chris Sheehy, Benjamin Wallisch, Mustafa A. Amin, Dan Green, Tracy R. Slatyer, Josef Frisch, Alexander A. Kaurov, Dionysios Karagiannis, Peter T. Timbie, David Alonso, Emanuele Castorina, Kiyoshi Masui, Romeel Davé, Gregory S. Tucker, William Tyndall, Kevin Bandura, Adrian Liu, Paul O'Connor, Alexander van Engelen, Paul Stankus, Simon Foreman, Andrei Nomerotski, Matthew C. Johnson, Yin-Zhe Ma, Neelima Sehgal, Martin White
PUMA is a proposal for an ultra-wideband, low-resolution and transit interferometric radio telescope operating at $200-1100\,\mathrm{MHz}$. Its design is driven by six science goals which span three science themes: the physics of dark energy (measuri
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::997af86bb57c37128dfee609f44bc4dd
https://doi.org/10.2172/1558437
https://doi.org/10.2172/1558437