NewEvery arXiv paper, its researchers & institutions — mapped.
papers

Publications (15)

astro-ph.CO2009

On the dependence between UV luminosity and Lyman-alpha equivalent width in high redshift galaxies

Kim K. Nilsson, Ole Moeller-Nilsson, Palle Moeller +2

astro-ph.CO2011

X-ray Constraints on the Lyman-Alpha Escape Fraction

Zhen-Ya Zheng, Sangeeta Malhotra, Jun-Xian Wang +7

astro-ph.CO2010

Stellar properties of z ~ 1 Lyman-break galaxies from ACS slitless grism spectra

Kim K. Nilsson, Ole Möller-Nilsson, Piero Rosati +5

astro-ph.IM2010

Future management needs of a "software-driven" science community

Kim K. Nilsson, Ole Moeller-Nilsson

astro-ph2006

An on-going multi-wavelength survey of Ly-alpha emitters at redshifts z = 2 - 8

Kim K. Nilsson, Johan P. U. Fynbo, Palle Moller +1

astro-ph.CO2011

Lyman-alpha emitters as tracers of the transitioning Universe

Kim K. Nilsson, Palle Møller

astro-ph.CO2011

The nature of z ~ 2.3 Lyman-alpha emitters

Kim K. Nilsson, Göran Östlin, Palle Møller +4

astro-ph.CO2009

Understanding Lyman-alpha emitters

Kim K. Nilsson, Klaus Meisenheimer, Nicholas Bond +5

astro-ph2007

A multi-wavelength study of z = 3.15 Lyman-alpha emitters in the GOODS South Field

Kim K. Nilsson, P. Moeller, O. Moeller +7

astro-ph.CO2009

Ly-alpha emitters: blue dwarfs or supermassive ULIRGs? Evidence for a transition with redshift

Kim K. Nilsson, Palle Moeller

astro-ph2007

Narrow-band surveys for very high redshift Lyman-alpha emitters

Kim K. Nilsson, Alvaro Orsi, Cedric G. Lacey +2

astro-ph.GA2011

A Link to the Past: Using Markov Chain Monte Carlo Fitting to Constrain Fundamental Parameters of High-Redshift Galaxies

N. Pirzkal, B. Rothberg, Kim K. Nilsson +4

astro-ph.CO2011

A Lyα blob and zabs {\approx} zem damped Lyα absorber in the dark matter halo of the binary quasar Q 0151+048

Tayyaba Zafar, Palle Møller, Cédric Ledoux +7

astro-ph2007

The Lyman-alpha Emission Line as a Cosmological Tool

Kim K. Nilsson

astro-ph2009

Evolution in the properties of Lyman-alpha emitters from redshifts z ~ 3 to z ~ 2

Kim K. Nilsson, Christian Tapken, Palle Moeller +5