Institution
Institute of Cosmology and Gravitation, University of Portsmouth
About: Institute of Cosmology and Gravitation, University of Portsmouth is a based out in . It is known for research contribution in the topics: Galaxy & Redshift. The organization has 297 authors who have published 1207 publications receiving 76919 citations.
Topics: Galaxy, Redshift, Dark energy, Dark matter, Cosmic microwave background
Papers published on a yearly basis
Papers
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TL;DR: In this paper, the authors present an analysis of the main systematic effects that could impact the measurement of CMB polarization with the proposed CORE space mission, and employ timeline-to-map simulations to verify that the CORE instrumental set-up and scanning strategy allow us to measure sky polarization to a level of accuracy adequate to the mission science goals.
Abstract: We present an analysis of the main systematic effects that could impact the measurement of CMB polarization with the proposed CORE space mission. We employ timeline-to-map simulations to verify that the CORE instrumental set-up and scanning strategy allow us to measure sky polarization to a level of accuracy adequate to the mission science goals. We also show how the CORE observations can be processed to mitigate the level of contamination by potentially worrying systematics, including intensity-to-polarization leakage due to bandpass mismatch, asymmetric main beams, pointing errors and correlated noise. We use analysis techniques that are well validated on data from current missions such as Planck to demonstrate how the residual contamination of the measurements by these effects can be brought to a level low enough not to hamper the scientific capability of the mission, nor significantly increase the overall error budget. We also present a prototype of the CORE photometric calibration pipeline, based on that used for Planck, and discuss its robustness to systematics, showing how CORE can achieve its calibration requirements. While a fine-grained assessment of the impact of systematics requires a level of knowledge of the system that can only be achieved in a future study phase, the analysis presented here strongly suggests that the main areas of concern for the CORE mission can be addressed using existing knowledge, techniques and algorithms.
28 citations
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University of Michigan1, Carleton College2, University of Pennsylvania3, Lawrence Berkeley National Laboratory4, University of California, Berkeley5, University of Chicago6, University College London7, Rhodes University8, Fermilab9, Institut d'Astrophysique de Paris10, SLAC National Accelerator Laboratory11, Stanford University12, Institute of Cosmology and Gravitation, University of Portsmouth13, National Center for Supercomputing Applications14, University of Illinois at Urbana–Champaign15, Autonomous University of Barcelona16, Institut de Ciències de l'Espai17, Texas A&M University18, Ludwig Maximilian University of Munich19, California Institute of Technology20, Max Planck Society21, Ohio State University22, Australian Astronomical Observatory23, Catalan Institution for Research and Advanced Studies24, University of Sussex25, Universidade Federal do Rio Grande do Sul26
TL;DR: In this paper, the authors reported the discovery of the eighth and ninth known Trojans in stable orbits around Neptune's leading Lagrange point, L4, in data obtained during the 2013-14 and 2014-15 observing seasons by the Dark Energy Survey, using the DECam on the 4-meter Blanco telescope at Cerro Tololo Inter-American Observatory.
Abstract: We report the discovery of the eighth and ninth known Trojans in stable orbits around Neptune's leading Lagrange point, L4. The objects 2014 QO 441 and 2014 QP 441 were detected in data obtained during the 2013-14 and 2014-15 observing seasons by the Dark Energy Survey, using the Dark Energy Camera (DECam) on the 4-meter Blanco telescope at Cerro Tololo Inter-American Observatory. Both are in high-inclination orbits (18.8 ∘ and 19.4 ∘ respectively). With an eccentricity of 0.104, 2014 QO 441 has the most eccentric orbit of the eleven known stable Neptune Trojans. Here we describe the search procedure and investigate the objects' long-term dynamical stability and physical properties.
28 citations
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Leibniz Institute for Neurobiology1, Autonomous University of Madrid2, Spanish National Research Council3, University of California, Berkeley4, Lawrence Berkeley National Laboratory5, University of Paris6, Institute of Cosmology and Gravitation, University of Portsmouth7, Pierre-and-Marie-Curie University8, University of Portsmouth9, University of Utah10, Yale University11, Harvard University12, Shanghai Astronomical Observatory13, Carnegie Mellon University14, Johns Hopkins University15, University of Cambridge16, Sejong University17, Max Planck Society18, Pennsylvania State University19, Ohio University20, New York University21, University of St Andrews22, National Autonomous University of Mexico23
TL;DR: In this article, Ata et al. presented a Bayesian phase-space reconstruction of the cosmic large-scale matter density and velocity fields from the Sloan Digital Sky Survey-III Baryon Oscillations Spectroscopic Survey Data Release 12 CMASS galaxy clustering catalogue.
Abstract: Author(s): Ata, M; Kitaura, FS; Chuang, CH; Rodriguez-Torres, S; Angulo, RE; Ferraro, S; Gil-Marin, H; McDonald, P; Monteagudo, CH; Muller, V; Yepes, G; Autefage, M; Baumgarten, F; Beutler, F; Brownstein, JR; Burden, A; Eisenstein, DJ; Guo, H; Ho, S; McBride, C; Neyrinck, M; Olmstead, MD; Padmanabhan, N; Percival, WJ; Prada, F; Rossi, G; Sanchez, AG; Schlegel, D; Schneider, DP; Seo, HJ; Streblyanska, A; Tinker, J; Tojeiro, R; Vargas-Magana, M | Abstract: We present a Bayesian phase-space reconstruction of the cosmic large-scale matter density and velocity fields from the Sloan Digital Sky Survey-III Baryon Oscillations Spectroscopic Survey Data Release 12 CMASS galaxy clustering catalogue. We rely on a given ∧ cold dark matter cosmology, a mesh resolution in the range of 6-10 h-1 Mpc, and a lognormal-Poisson model with a redshift-dependent non-linear bias. The bias parameters are derived from the data and a general renormalized perturbation theory approach. We use combined Gibbs and Hamiltonian sampling, implemented in the ARGO code, to iteratively reconstruct the darkmatter density field and the coherent peculiar velocities of individual galaxies, correcting hereby for coherent redshift space distortions. Our tests relying on accurate N-body-based mock galaxy catalogues show unbiased real space power spectra of the non-linear density field up to k ~ 0.2 h Mpc-1, and vanishing quadrupoles down to r ~ 20 h-1 Mpc. We also demonstrate that the non-linear cosmic web can be obtained from the tidal field tensor based on the Gaussian component of the reconstructed density field. We find that the reconstructed velocities have a statistical correlation coefficient compared to the true velocities of each individual lightcone mock galaxy of r ~ 0.68 including about 10 per cent of satellite galaxies with virial motions (about r = 0.75 without satellites). The power spectra of the velocity divergence agree well with theoretical predictions up to k ~ 0.2 h Mpc-1. This work will be especially useful to improve, for example, baryon acoustic oscillation reconstructions, kinematic Sunyaev- Zeldovich, integrated Sachs-Wolfe measurements or environmental studies.
28 citations
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TL;DR: In this article, a method for measuring the evolution of the growth of structure using redshift-space distortions (RSDs) is presented, which removes the need to make measurements in redshift shells.
Abstract: The low-statistical errors on cosmological parameters promised by future galaxy surveys will only be realized with the development of new, fast, analysis methods that reduce potential systematic problems to low levels. We present an efficient method for measuring the evolution of the growth of structure using redshift-space distortions (RSDs), that removes the need to make measurements in redshift shells. We provide sets of galaxy-weights that cover a wide range in redshift, but are optimized to provide differential information about cosmological evolution. These are derived to optimally measure the coefficients of a parametrization of the redshift-dependent matter density, which provides a framework to measure deviations from the concordance ΛCDM cosmology, allowing for deviations in both geometric and/or growth. We test the robustness of the weights by comparing with alternative schemes and investigate the impact of galaxy bias. We extend the results to measure the combined anisotropic baryon acoustic oscillation and RSD signals.
28 citations
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TL;DR: In this article, the authors identify and characterize a compact star cluster, which they term NGC 3628-UCD1, embedded in a stellar stream around the spiral galaxy NGC3628, and demonstrate that at least some of the massive star cluster population may be created through tidal stripping.
Abstract: Using Subaru/Suprime-Cam wide-field imaging and both Keck/ESI and LBT/MODS spectroscopy, we identify and characterize a compact star cluster, which we term NGC 3628-UCD1, embedded in a stellar stream around the spiral galaxy NGC 3628. The size and luminosity of UCD1 are similar to $\omega$ Cen, the most luminous Milky Way globular cluster, which has long been suspected to be the stripped remnant of an accreted dwarf galaxy. The object has a magnitude of $i=19.3$ mag (${\rm L}_{\rm i}=1.4\times10^{6}~{\rm L}_{\odot}$). UCD1 is marginally resolved in our ground-based imaging, with a half-light radius of $\sim10$ pc. We measure an integrated brightness for the stellar stream of $i=13.1$ mag, with $(g-i)=1.0$. This would correspond to an accreted dwarf galaxy with an approximate luminosity of ${\rm L}_i\sim4.1\times10^{8}~{\rm L}_{\odot}$. Spectral analysis reveals that UCD1 has an age of $6.6$ Gyr , $[\rm{Z}/\rm{H}]=-0.75$, an $[{\alpha}/\rm{Fe}]=-0.10$. We propose that UCD1 is an example of an $\omega$ Cen-like star cluster possibly forming from the nucleus of an infalling dwarf galaxy, demonstrating that at least some of the massive star cluster population may be created through tidal stripping.
28 citations
Authors
Showing all 297 results
Name | H-index | Papers | Citations |
---|---|---|---|
Robert C. Nichol | 187 | 851 | 162994 |
Daniel Thomas | 134 | 846 | 84224 |
Will J. Percival | 129 | 473 | 87752 |
Tommaso Treu | 126 | 715 | 49090 |
Claudia Maraston | 103 | 362 | 59178 |
Marco Cavaglia | 93 | 372 | 60157 |
Ashley J. Ross | 90 | 248 | 46395 |
David A. Wake | 89 | 214 | 46124 |
László Á. Gergely | 89 | 426 | 60674 |
L. K. Nuttall | 89 | 253 | 54834 |
Rita Tojeiro | 87 | 229 | 43140 |
Roy Maartens | 86 | 432 | 23747 |
David Keitel | 85 | 253 | 56849 |
Davide Pietrobon | 83 | 152 | 62010 |
Gong-Bo Zhao | 81 | 287 | 35540 |