output
19982026
most citedThe Fifth Data Release of the Sloan Digital Sky Survey

744 citations

Showing astro-ph.COShow all

11 papers · 1 filter

astro-ph.CO2024★ 116 cited

The SRG/eROSITA all-sky survey: Cosmology constraints from cluster abundances in the western Galactic hemisphere

V. Ghirardini, E. Bulbul, E. Artis +46

The cluster mass function traces the growth of linear density perturbations and provides valuable insights into the growth of structures, the nature of dark matter, and the cosmolo…

astro-ph.CO2023★ 213 cited

Hyper Suprime-Cam Year 3 Results: Cosmology from Cosmic Shear Power Spectra

Roohi Dalal, Xiangchong Li, Andrina Nicola +35

We measure weak lensing cosmic shear power spectra from the three-year galaxy shear catalog of the Hyper Suprime-Cam (HSC) Subaru Strategic Program imaging survey. The shear catalo…

astro-ph.CO2023★ 85 cited

Hyper Suprime-Cam Year 3 Results: Cosmology from Galaxy Clustering and Weak Lensing with HSC and SDSS using the Minimal Bias Model

Sunao Sugiyama, Hironao Miyatake, Surhud More +27

We present cosmological parameter constraints from a blind joint analysis of three two-point correlation functions measured from the Year 3 Hyper Suprime-Cam (HSC-Y3) imaging data,…

astro-ph.CO2023★ 11 cited

The eROSITA Final Equatorial-Depth Survey (eFEDS) -- Splashback radius of X-ray galaxy clusters using galaxies from HSC survey

Divya Rana, Surhud More, Hironao Miyatake +6

We present the splashback radius measurements around the SRG/eROSITA eFEDS X-ray selected galaxy clusters by cross-correlating them with HSC S19A photometric galaxies. The X-ray se…

astro-ph.CO2022★ 104 cited

EMPRESS. VIII. A New Determination of Primordial He Abundance with Extremely Metal-Poor Galaxies: A Suggestion of the Lepton Asymmetry and Implications for the Hubble Tension

Akinori Matsumoto, Masami Ouchi, Kimihiko Nakajima +42

The primordial He abundance is a powerful probe of cosmology. Currently, is best determined by observations of metal-poor galaxies, while there are on…

astro-ph.CO2016★ 49 cited

Interpreting the strongly lensed supernova iPTF16geu: time delay predictions, microlensing, and lensing rates

Anupreeta More, Sherry H. Suyu, Masamune Oguri +2

We present predictions for time delays between multiple images of the gravitationally lensed supernova, iPTF16geu, which was recently discovered from the intermediate Palomar Trans…

astro-ph.CO2016★ 32 cited

A new quadruple gravitational lens from the Hyper Suprime-Cam Survey: the puzzle of HSC~J115252+004733

Anupreeta More, Chien-Hsiu Lee, Masamune Oguri +16

We report the serendipitous discovery of a quadruply lensed source at , HSC~J115252+004733, from the Hyper Suprime-Cam (HSC) Survey. The source is lensed by an earl…

astro-ph.CO2015★ 26 cited

Passive galaxies as tracers of cluster environments at z~2

V. Strazzullo, E. Daddi, R. Gobat +18

Even 10 billion years ago, the cores of the first galaxy clusters are often found to host a characteristic population of massive galaxies with already suppressed star formation. He…

astro-ph.CO2009★ 115 cited

MOIRCS Deep Survey IV: Evolution of Galaxy Stellar Mass Function Back to z ~ 3

M. Kajisawa, T. Ichikawa, I. Tanaka +11

We use very deep near-infrared (NIR) imaging data obtained in MOIRCS Deep Survey (MODS) to investigate the evolution of the galaxy stellar mass function back to z~3. The MODS data…

astro-ph.CO2009★ 28 cited

MOIRCS Deep Survey III: Active Galactic Nuclei in Massive Galaxies at z=2-4

T. Yamada, M. Kajisawa, M. Akiyama +9

We investigate the X-ray properties of the K-band-selected galaxies at redshift 2 < z < 4 by using our deep near-infrared images obtained in the MOIRCS Deep Survey project and the…

astro-ph.CO2009★ 28 cited

Evidence of a link between the evolution of clusters and their AGN fraction

Caroline van Breukelen, Chris Simpson, Steve Rawlings +9

We discuss the optical properties, X-ray detections, and Active Galactic Nucleus (AGN) populations of four clusters at z ~ 1 in the Subaru-XMM Deep Field (SXDF). The velocity distr…