activity
19992021
most citedAn optical supernova associated with the X-ray flash XRF 060218

544 citations · 1.9k across the 31 of their papers we have counts for

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Showing 2018Show all

9 papers · 1 filter

astro-ph.GA2018

Cold gas in the early Universe. Survey for neutral atomic-carbon in GRB host galaxies at 1 < z < 6 from optical afterglow spectroscopy

K. E. Heintz, C. Ledoux, J. P. U. Fynbo +14

We present a survey for neutral atomic-carbon (CI) along gamma-ray burst (GRB) sightlines, which probes the shielded neutral gas-phase in the interstellar medium (ISM) of GRB host…

astro-ph.GA2018

Metals, depletion and dimming: decrypting dust

Tayyaba Zafar, Palle Møller

Dust plays a pivotal role in the chemical enrichment of the interstellar medium. In the era of mid/high resolution spectra and multi-band spectral energy distributions, testing ext…

astro-ph.GA2018

A Lyman limit system associated with galactic winds

Hadi Rahmani, Celine Peroux, Ilane Schroetter +9

Projected quasar galaxy pairs provide powerful means to study the circumgalactic medium (CGM) that maintains the relics of galactic feedback and the accreted gas from the intergala…

astro-ph.GA2018

Stellar masses, metallicity gradients and suppressed star formation revealed in a new sample of absorption selected galaxies

N. H. P. Rhodin, L. Christensen, P. Møller +2

Context. Absorbing galaxies are selected via the detection of characteristic absorption lines which their gas-rich media imprint in the spectra of distant light-beacons. The proxim…

astro-ph.GA2018

ALMA observations of a metal-rich damped Lyα absorber at z = 2.5832: evidence for strong galactic winds in a galaxy group

J. P. U. Fynbo, K. E. Heintz, M. Neeleman +7

We report on the results of a search for CO(3-2) emission from the galaxy counterpart of a high-metallicity Damped Ly-alpha Absorber (DLA) at z=2.5832 towards the quasar Q0918+1636…

astro-ph.GA2018

Characterising the Circum-Galactic Medium of Damped Lyman- Absorbing Galaxies

Ramona Augustin, Celine Peroux, Palle Moller +8

Gas flows in and out of galaxies through their circumgalactic medium (CGM) are poorly constrained and direct observations of this faint, diffuse medium remain challenging. We use a…