most citedA SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): JWST Reveals a Filamentary Structure around a z=6.61 Quasar

91 citations · 236 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.GA2024★ 2 cited

Introducing the BRAHMA simulation suite: Signatures of low mass black hole seeding models in cosmological simulations

Aklant K. Bhowmick, Laura Blecha, Paul Torrey +6

The first "seeds" of supermassive black holes (BH) can range from . However, the lowest mass seeds () are inaccessible to most cosm…

astro-ph.GA2023★ 2 cited

Building Semi-Analytic Black Hole Seeding Models Using IllustrisTNG Host Galaxies

Analis Eolyn Evans, Laura Blecha, Aklant Kumar Bhowmick

Because early black holes (BHs) grew to in less than 1 Gyr of cosmic time, BH seeding models face stringent constraints. To efficiently constrain the paramete…

astro-ph.GA2023★ 91 cited

A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): JWST Reveals a Filamentary Structure around a z=6.61 Quasar

Feige Wang, Jinyi Yang, Joseph F. Hennawi +56

We present the first results from the JWST ASPIRE program (A SPectroscopic survey of biased halos In the Reionization Era). This program represents an imaging and spectroscopic sur…

astro-ph.GA2023★ 77 cited

A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): A First Look at the Rest-frame Optical Spectra of Quasars Using JWST

Jinyi Yang, Feige Wang, Xiaohui Fan +53

Studies of rest-frame optical emission in quasars at have historically been limited by the wavelengths accessible by ground-based telescopes. The James Webb Space Telescope (…

astro-ph.EP2023★ 64 cited

Rotation Periods, Inclinations, and Obliquities of Cool Stars Hosting Directly Imaged Substellar Companions: Spin-Orbit Misalignments are Common

Brendan P. Bowler, Quang H. Tran, Zhoujian Zhang +10

The orientation between a star's spin axis and a planet's orbital plane provides valuable information about the system's formation and dynamical history. For non-transiting planets…