output
19922026
most citedObservation of a New Narrow Charmonium State in Exclusive B+-->K+ pi+pi- J/psi Decays

2k citations

Showing 2022 · astro-ph.COShow all

12 papers · 2 filters

astro-ph.CO2022★ 19 cited

Flashlights: An Off-Caustic Lensed Star at Redshift = 1.26 in Abell 370

Ashish Kumar Meena, Wenlei Chen, Adi Zitrin +10

We report the discovery of a transient seen in a strongly lensed arc at redshift in \emph{Hubble Space Telescope} imaging of the Abell 370 galaxy cluster. The tr…

astro-ph.CO2022★ 11 cited

Constraining Cosmological Parameters using the Cluster Mass-Richness Relation

Mohamed H. Abdullah, Gillian Wilson, Anatoly Klypin +1

The cluster mass-richness relation (MRR) is an observationally efficient and potentially powerful cosmological tool for constraining the mean matter density of the universe and the…

astro-ph.CO2022★ 34 cited

A close quasar pair in a disk-disk galaxy merger at z = 2.17

Yu-Ching Chen, Xin Liu, Adi Foord +7

Galaxy mergers produce pairs of supermassive black holes (SMBHs), which may be witnessed as dual quasars if both SMBHs are rapidly accreting. The kiloparsec (kpc)-scale separation…

astro-ph.CO2022★ 7 cited

Galaxy clusters at z~1 imaged by ALMA with the Sunyaev-Zel'dovich effect

T. Kitayama, S. Ueda, N. Okabe +15

We present high angular-resolution measurements of the thermal Sunyaev-Zel'dovich effect (SZE) toward two galaxy clusters, RCS J2319+0038 at z=0.9 and HSC J0947-0119 at z=1.1, by t…

astro-ph.CO2022★ 7 cited

Perturbation Theory Remixed: Improved Nonlinearity Modeling beyond Standard Perturbation Theory

Zhenyuan Wang, Donghui Jeong, Atsushi Taruya +2

We present a novel EPT (th-order Eulerian Perturbation Theory) scheme to model the nonlinear density field by the summation up to th-order density fields in perturbation t…

astro-ph.CO2022★ 23 cited

Revealing Dark Matter Dress of Primordial Black Holes by Cosmological Lensing

Masamune Oguri, Volodymyr Takhistov, Kazunori Kohri

Stellar-mass primordial black holes (PBHs) from the early Universe can directly contribute to the gravitational wave (GW) events observed by LIGO, but can only comprise a subdomina…