papers

Publications (115)

astro-ph.GA2025

Exploring quasar evolution with proximate molecular absorbers: Insights from the kinematics of highly ionized nitrogen

R. Cuellar, P. Noterdaeme, S. Balashev +3

We investigate the presence and kinematics of NV absorption proximate to high redshift quasars selected upon the presence of strong and HI absorption at the quasar redshift…

astro-ph.CO2013

The Galaxy Counterparts of the two high-metallicity DLAs at z=2.412 and z=2.583 towards Q0918+1636

J. P. U. Fynbo, S. Geier, L. Christensen +9

The quasar Q0918+1636 (z=3.07) has two intervening high-metallicity Damped Lyman-alpha Absorbers (DLAs) along the line of sight, at redshifts of z=2.412 and 2.583. The z=2.583 DLA…

astro-ph.CO2012

Deuterium at high-redshift: Primordial abundance in the zabs = 2.621 damped Ly-alpha system towards CTQ247

P. Noterdaeme, S. López, V. Dumont +3

The detection of neutral deuterium in the low-metallicity damped Lyman-α system at zabs = 2.621 towards the quasar CTQ247 is reported. Using a high signal-to-noise and high spectr…

astro-ph.IM2022

CUBES: a UV spectrograph for the future

S. Covino, S. Cristiani, J. M. Alcala' +86

In spite of the advent of extremely large telescopes in the UV/optical/NIR range, the current generation of 8-10m facilities is likely to remain competitive at ground-UV wavelength…

astro-ph.CO2010

A translucent interstellar cloud at z=2.69: CO, H2 and HD in the line-of-sight to SDSS J123714.60+064759.5

P. Noterdaeme, P. Petitjean, C. Ledoux +3

We present the analysis of a sub-DLA system (log N(H^0)=20.0+/-0.15, z_abs=2.69) toward SDSS J123714+064759 (z_em=2.78). Using the VLT/UVES and X-shooter spectrographs, we detect H…

astro-ph.GA2021

CII*/CII ratio in high-redshift DLAs: ISM phase separation drives the observed bimodality of [CII] cooling rates

S. A. Balashev, K. N. Telikova, P. Noterdaeme

We discuss observations of CII*/CII ratios and cooling rates due to [CII]158m emission in high-redshift intervening damped Lyman- systems towards quasars. We show that…