M. Romano

collaborators

2 papers

astro-ph.GA2026

Higher resolution optical spectra of $M_{*} < 1 0^{10} M_{⊙}$ galaxies reveal outflow signatures unresolved by the SDSS

B. Hagedorn, C. Cicone, C. Vignali +5

Galactic outflows are predicted to be ubiquitous in low-mass galaxies, but observational evidence is lacking. Both a low signal-to-noise and a low spectral resolution can severely…

astro-ph.GA2024

The ALPINE-ALMA [CII] Survey: Modelling ALMA and JWST lines to constrain the interstellar medium of $z \sim 5$ galaxies

E. Veraldi, L. Vallini, F. Pozzi +13

In this work, we devise a model for estimating UV and optical line emission (i.e., CIII] $1909$ A, H $I^^{2}$ , [OIII] $5007$ A, H $I^\pm$ , [NII] $6583$ A) tracing HII regions in the interstell…

Higher resolution optical spectra of M∗​<1010 M⊙​ galaxies reveal outflow signatures unresolved by the SDSS

The ALPINE-ALMA [CII] Survey: Modelling ALMA and JWST lines to constrain the interstellar medium of z∼5 galaxies

Higher resolution optical spectra of $M_{*} < 1 0^{10} M_{⊙}$ galaxies reveal outflow signatures unresolved by the SDSS

The ALPINE-ALMA [CII] Survey: Modelling ALMA and JWST lines to constrain the interstellar medium of $z \sim 5$ galaxies