activity
20052020
most citedThe Sloan Digital Sky Survey Quasar Catalog: Fourteenth Data Release

464 citations · 5.1k across the 58 of their papers we have counts for

collaborators

58 papers

astro-ph.GA2020★ 31 cited

Open Clusters as Tracers on Radial Migration of the Galactic Disk

Y. Q. Chen, G. Zhao

Radial migration is an important process in the Galactic disk. A few open clusters show some evidence on this mechanism but there is no systematic study. In this work, we investiga…

astro-ph.GA2018★ 464 cited

The Sloan Digital Sky Survey Quasar Catalog: Fourteenth Data Release

I. Pâris, P. Petitjean, E. Aubourg +38

We present the Data Release 14 Quasar catalog (DR14Q) from the extended Baryon Oscillation Spectroscopic Survey (eBOSS) of the Sloan Digital Sky Survey IV (SDSS-IV). This catalog i…

astro-ph.CO2017★ 69 cited

Using Voids to Unscreen Modified Gravity

B. Falck, Kazuya Koyama, Gong-bo Zhao +1

The Vainshtein mechanism, present in many models of gravity, is very effective at screening dark matter halos such that the fifth force is negligible and general relativity is reco…

astro-ph.CO2017★ 26 cited

Revealing modified gravity signal in matter and halo hierarchical clustering

Wojciech A. Hellwing, Kazuya Koyama, Benjamin Bose +1

We use a set of N-body simulations employing a modified gravity (MG) model with Vainshtein screening to study matter and halo hierarchical clustering. As test-case scenarios we con…

astro-ph.CO2017★ 97 cited

COLA with scale-dependent growth: applications to screened modified gravity models

Hans A. Winther, Kazuya Koyama, Marc Manera +2

We present a general parallelized and easy-to-use code to perform numerical simulations of structure formation using the COLA (COmoving Lagrangian Acceleration) method for cosmolog…

astro-ph.CO2017★ 34 cited

Theoretical Accuracy in Cosmological Growth Estimation

Benjamin Bose, Kazuya Koyama, Wojciech A. Hellwing +2

We elucidate the importance of the consistent treatment of gravity-model specific non-linearities when estimating the growth of cosmological structures from redshift space distorti…

astro-ph.CO2016★ 59 cited

The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: constraining modified gravity

Eva-Maria Mueller, Will Percival, Eric Linder +4

We use baryon acoustic oscillation and redshift space distortion from the completed Baryon Oscillation Spectroscopic Survey, corresponding to data release 12 of the Sloan Digital S…

astro-ph.CO2016★ 46 cited

Clustering of quasars in the First Year of the SDSS-IV eBOSS survey: Interpretation and halo occupation distribution

Sergio A. Rodríguez-Torres, Johan Comparat, Francisco Prada +10

In current and future surveys, quasars play a key role. The new data will extend our knowledge of the Universe as it will be used to better constrain the cosmological model at reds…

astro-ph.CO2016★ 46 cited

The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: combining correlated Gaussian posterior distributions

Ariel G. Sanchez, Jan Niklas Grieb, Salvador Salazar-Albornoz +17

The cosmological information contained in anisotropic galaxy clustering measurements can often be compressed into a small number of parameters whose posterior distribution is well…

astro-ph.CO2016★ 133 cited

The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Cosmological implications of the Fourier space wedges of the final sample

Jan Niklas Grieb, Ariel G. Sánchez, Salvador Salazar-Albornoz +25

We extract cosmological information from the anisotropic power spectrum measurements from the recently completed Baryon Oscillation Spectroscopic Survey (BOSS), extending the conce…

astro-ph.CO2016★ 14 cited

Redshift Weights for Baryon Acoustic Oscillations : Application to Mock Galaxy Catalogs

Fangzhou Zhu, Nikhil Padmanabhan, Martin White +2

Large redshift surveys capable of measuring the Baryon Acoustic Oscillation (BAO) signal have proven to be an effective way of measuring the distance-redshift relation in cosmology…

astro-ph.CO2016★ 30 cited

Simulation tests of galaxy cluster constraints on chameleon gravity

Harry Wilcox, Robert C. Nichol, Gong-bo Zhao +3

We use two new hydrodynamical simulations of CDM and gravity to test the methodology used by Wilcox et al. 2015 (W15) in constraining the effects of a fifth force on the…

gr-qc2016★ 87 cited

Screening fifth forces in generalized Proca theories

Antonio De Felice, Lavinia Heisenberg, Ryotaro Kase +3

For a massive vector field with derivative self-interactions, the breaking of the gauge invariance allows the propagation of a longitudinal mode in addition to the two transverse m…

astro-ph.CO2015★ 33 cited

Searching for scalar gravitational interactions in current and future cosmological data

Alireza Hojjati, Aaron Plahn, Alex Zucca +4

Modified gravity theories often contain a scalar field of gravitational strength which interacts with matter. We examine constraints on the range and the coupling strength of a sca…

astro-ph.CO2015★ 43 cited

Consistent Modified Gravity Analysis of Anisotropic Galaxy Clustering Using BOSS DR11

Yong-Seon Song, Atsushi Taruya, Eric Linder +6

We analyse the clustering of cosmic large scale structure using a consistent modified gravity perturbation theory, accounting for anisotropic effects along and transverse to the li…

astro-ph.CO2015★ 148 cited

Modified Gravity N-body Code Comparison Project

Hans A. Winther, Fabian Schmidt, Alexandre Barreira +12

Self-consistent -body simulations of modified gravity models are a key ingredient to obtain rigorous constraints on deviations from General Relativity using large-scale st…

astro-ph.CO2015★ 40 cited

Reconstruction of the dark matter-vacuum energy interaction

Yuting Wang, Gong-Bo Zhao, David Wands +2

An interaction between the vacuum energy and dark matter is an intriguing possibility which may offer a way of solving the cosmological constant problem. Adopting a general prescri…

gr-qc2015★ 22 cited

f(R) gravity on non-linear scales: The post-Friedmann expansion and the vector potential

Daniel B Thomas, Marco Bruni, Kazuya Koyama +2

Many modified gravity theories are under consideration in cosmology as the source of the accelerated expansion of the universe and linear perturbation theory, valid on the largest…

astro-ph.CO2015★ 7 cited

Model-independent constraints on dark energy and modified gravity with the SKA

Gong-Bo Zhao, David Bacon, Roy Maartens +2

Employing a nonparametric approach of the principal component analysis (PCA), we forecast the future constraint on the equation of state of dark energy, and on the effective…

astro-ph.CO2015★ 11 cited

Cosmology from HI galaxy surveys with the SKA

Filipe B. Abdalla, Philip Bull, Stefano Camera +8

The Square Kilometer Array (SKA) has the potential to produce galaxy redshift surveys which will be competitive with other state of the art cosmological experiments in the next dec…

astro-ph.CO2015★ 5 cited

Synergy between the Large Synoptic Survey Telescope and the Square Kilometre Array

David Bacon, Sarah Bridle, Filipe B. Abdalla +18

We provide an overview of the science benefits of combining information from the Square Kilometre Array (SKA) and the Large Synoptic Survey Telescope (LSST). We first summarise the…

astro-ph.CO2015★ 10 cited

Measuring redshift-space distortions with future SKA surveys

Alvise Raccanelli, Philip Bull, Stefano Camera +8

The peculiar motion of galaxies can be a particularly sensitive probe of gravitational collapse. As such, it can be used to measure the dynamics of dark matter and dark energy as w…

astro-ph.CO2014★ 63 cited

The Vainshtein Mechanism in the Cosmic Web

Bridget Falck, Kazuya Koyama, Gong-bo Zhao +1

We investigate the dependence of the Vainshtein screening mechanism on the cosmic web morphology of both dark matter particles and halos as determined by ORIGAMI. Unlike chameleon…

astro-ph.CO2014★ 21 cited

Observable physical modes of modified gravity

Alireza Hojjati, Levon Pogosian, Alessandra Silvestri +1

At linear order in cosmological perturbations, departures from the growth in the cosmological standard model can be quantified in terms of two functions of redshift and Fourier…