G. Institute

Thermal states of coldest and hottest neutron stars in soft X-ray transients

crAl, O. Gnedin, K. Levenfish, 2003, astro-ph/0310259.

How is model-related uncertainty quantified and reported in different disciplines?

Statistics, Ole Magnus Theisen, Department of Materials Science, 2022, 2206.12179.

Thermal states of coldest and hottest neutron stars in soft X-ray transients

crAl, O. Gnedin, K. Levenfish, 2003, astro-ph/0310259.

Molecular hydrogen abundance in the dust-free damped Ly-alpha galaxy at z = 3.4

Garching, H Germany, P. Bonifacio, 2000, astro-ph/0011470.