output
20022025
most citedThe density-matrix renormalization group in the age of matrix product states

4.2k citations

Showing astro-ph.GAShow all

86 papers · 1 filter

astro-ph.GA202372 cited

A Tale of Two Disks: Mapping the Milky Way with the Final Data Release of APOGEE

Julie Imig, Cathryn Price, Jon A. Holtzman +24

We present new maps of the Milky Way disk showing the distribution of metallicity ([Fe/H]), -element abundances ([Mg/Fe]), and stellar age, using a sample of 66,496 red giant st…

astro-ph.GA20236 cited

Infrared spectroscopic confirmation of z~2 photometrically-selected obscured quasars

Yuzo Ishikawa, Ben Wang, Nadia L. Zakamska +3

The census of obscured quasar populations is incomplete, and remains a major unsolved problem, especially at higher redshifts, where we expect a greater density of galaxy formation…

astro-ph.GA202314 cited

Wide binary stars formed in the turbulent interstellar medium

Siyao Xu, Hsiang-Chih Hwang, Chris Hamilton +1

The ubiquitous interstellar turbulence regulates star formation and the scaling relations between the initial velocity differences and the initial separations of stars. We propose…

astro-ph.GA20236 cited

Detections of [C II] 158 m and [O III] 88 m in a Local Lyman Continuum Emitter, Mrk 54, and its Implications to High-redshift ALMA Studies

Ryota Ura, Takuya Hashimoto, Akio K. Inoue +17

We present integral field, far-infrared (FIR) spectroscopy of Mrk 54, a local Lyman Continuum Emitter (LCE), obtained with FIFI-LS on the Stratospheric Observatory for Infrared Ast…

astro-ph.GA202348 cited

The AGNIFS survey: spatially resolved observations of hot molecular and ionised outflows in nearby active galaxies

R. A. Riffel, T. Storchi-Bergmann, R. Riffel +17

We present the hot molecular and warm ionised gas kinematics for 33 nearby () X-ray selected active galaxies using the Hm and Br emiss…

astro-ph.GA202321 cited

Detecting isolated stellar-mass black holes by the Roman telescope

Sedighe Sajadian, Kailash C. Sahu

Isolated Stellar-Mass BlackHoles (ISMBHs) are potentially discernible through microlensing observations. In this work, we study detecting and characterizing ISMBHs with the Roman o…