activity
20182020
most citedFirst star-forming structures in fuzzy cosmic filaments

161 citations · 226 across the 4 of their papers we have counts for

collaborators

22 papers

astro-ph.GA202060 cited

The galaxy-halo connection of emission-line galaxies in IllustrisTNG

Boryana Hadzhiyska, Sandro Tacchella, Sownak Bose +1

We employ the hydrodynamical simulation IllustrisTNG-300-1 to explore the halo occupation distribution (HOD) and environmental dependence of luminous star-forming emission-line gal…

astro-ph.CO2020

Evidence for galaxy assembly bias in BOSS CMASS redshift-space galaxy correlation function

Sihan Yuan, Boryana Hadzhiyska, Sownak Bose +2

Building accurate and flexible galaxy-halo connection models is crucial in modeling galaxy clustering on non-linear scales. Recent studies have found that halo concentration by its…

astro-ph.CO2020

Extensions to models of the galaxy-halo connection

Boryana Hadzhiyska, Sownak Bose, Daniel Eisenstein +1

We explore two widely used empirical models for the galaxy-halo connection, subhalo abundance matching (SHAM) and the halo occupation distribution (HOD) and compare their predictio…

astro-ph.GA2020

The BUFFALO HST Survey

Charles L. Steinhardt, Mathilde Jauzac, Ana Acebron +91

The Beyond Ultra-deep Frontier Fields and Legacy Observations (BUFFALO) is a 101 orbit + 101 parallel Cycle 25 Hubble Space Telescope Treasury program taking data from 2018-2020. B…

astro-ph.CO2019

Galaxy Formation with BECDM -- II. Cosmic Filaments and First Galaxies

Philip Mocz, Anastasia Fialkov, Mark Vogelsberger +11

Bose-Einstein Condensate Dark Matter (BECDM; also known as Fuzzy Dark Matter) is motivated by fundamental physics and has recently received significant attention as a serious alter…

astro-ph.CO2019

Universal structure of dark matter haloes over a mass range of 20 orders of magnitude

Jie Wang, Sownak Bose, Carlos S. Frenk +4

Cosmological models in which dark matter consists of cold elementary particles predict that the dark halo population should extend to masses many orders of magnitude below those at…