activity
20242026
most citedHYACINTH: HYdrogen And Carbon chemistry in the INTerstellar medium in Hydro simulations

8 citations · 15 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.GA2026

Same galaxy, different CGM: how the metal loading of galactic winds regulates the baryon cycle in Milky Way-mass galaxies

Prachi Khatri, Freeke van de Voort, Rebekka Bieri +5

The circumgalactic medium (CGM) is both the reservoir of gas that fuels star formation and galaxy growth, and the repository for the mass, energy, and metals expelled through stell…

astro-ph.CO2025

Probing the warm dark matter mass with [C II] intensity mapping

Elena Marcuzzo, Cristiano Porciani, Emilio Romano-Díaz +3

The nature of dark matter (DM) is still debated. While cold DM (CDM) is the standard paradigm, warm DM (WDM) may ease some small-scale tensions in the CDM framework. Line-intens…

astro-ph.CO2025★ 1 cited

Constraining the [CII] luminosity function from the power spectrum of line-intensity maps at redshift 3.6

Elena Marcuzzo, Cristiano Porciani, Emilio Romano-Díaz +1

Forthcoming measurements of the line-intensity mapping (LIM) power spectrum (PS) are expected to provide valuable constraints on astrophysical and cosmological quantities. We focus…

astro-ph.GA2024★ 6 cited

The [C II] line emission as an interstellar medium probe in the MARIGOLD galaxies

Prachi Khatri, Emilio Romano-Díaz, Cristiano Porciani

The [C II] fine-structure line at 157.74 m is one of the brightest far-infrared emission lines and an important probe of galaxy properties like the star formation rate (SFR) and…

astro-ph.GA2024★ 8 cited

HYACINTH: HYdrogen And Carbon chemistry in the INTerstellar medium in Hydro simulations

Prachi Khatri, Cristiano Porciani, Emilio Romano-Díaz +2

Aims. We present a new sub-grid model, HYACINTH -- HYdrogen And Carbon chemistry in the INTerstellar medium in Hydro simulations -- for computing the non-equilibrium abundances of…