Zobrazeno 1 - 10
of 29
pro vyhledávání: '"Einar H. Gudmundsson"'
Publikováno v:
Journal of Psychoeducational Assessment. 37:263-279
The study examined the psychometric properties of the Children’s Emotional Adjustment Scale–Preschool Version (CEAS-P), a new behavioral rating scale completed by parents. The scale measures preschoolers’ emotional functioning across three comp
Autor:
P. M. Vreeswijk, Robert Chapman, Pall Jakobsson, C. Ledoux, Alain Smette, J. P. U. Fynbo, Gunnlaugur Björnsson, A. De Cia, Tayyaba Zafar, D. Malesani, T. R. Marsh, V. S. Dhillon, Steve Schulze, Einar H. Gudmundsson, S. P. Littlefair
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 412:2229-2240
We present high time resolution (1.09 s) photometry of GRB 080210 obtained with ULTRASPEC mounted on the ESO/3.6-m telescope, starting 68.22 min after the burst and lasting for 26.45 min. The light curve is smooth on both short (down to 2.18 s) and l
Autor:
Einar H. Gudmundsson
Publikováno v:
Nordic Psychology. 61:29-45
Translated but unstandardised psychological instruments are widely used in non-English speaking countries. For many of these instruments meagre information is available on the method of translation, extent of adaptations, reliability, validity and ot
Publikováno v:
Nordic Psychology. 61:14-25
To compare developmental ratings of mothers and fathers, 58 couples, parents of four year olds, mothers and fathers rated separately their children’s development on a 190-item eightsubtest inventor...
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 376:1375-1384
We explore galaxy properties in general and properties of host galaxies of gamma-ray bursts (GRBs) in particular, using N-body/Eulerian hydrodynamic simulations and the stellar population synthesis model, Starburst99, to infer observable properties.
Publikováno v:
The Astrophysical Journal. 647:1238-1249
We extend the standard fireball model, widely used to interpret gamma-ray burst (GRB) afterglow light curves, to include energy injections, and apply the model to the afterglow light curves of GRB 990510, GRB 000301C and GRB 010222. We show that disc
Publikováno v:
The Astrophysical Journal. 640:L5-L8
In gamma-ray burst research it is quite common to fit the afterglow light curves with a broken power law to interpret the data. We apply this method to a computer simulated population of afterglows and find systematic differences between the known mo
Autor:
Einar H. Gudmundsson, Jens Hjorth, B. Thomsen, J. P. U. Fynbo, G. Östlin, Gunnlaugur Björnsson, J. Gorosabel, Palle Møller, Gudlaugur Johannesson, Dan M. Watson, P. Jakobsson, B. L. Jensen
Publikováno v:
Jakobsson, P, Björnsson, G, Fynbo, J P U, Jóhannesson, G, Hjorth, J, Thomsen, B, Møller, P, Watson, D, Jensen, B L, Östlin, G, Gorosabel, J & Gudmundsson, E H 2005, ' Ly+ and ultraviolet emission from high-redshift gamma-ray burst hosts: to what extent do gamma-ray bursts trace star formation ? ', Royal Astronomical Society. Monthly Notices, vol. 362, pp. 245-251 .
We report the result of a search for Ly-alpha emission from the host galaxies of the gamma-ray bursts (GRBs) 030226 (z = 1.986), 021004 (z = 2.335) and 020124 (z = 3.198). We find that the host galaxy of GRB 021004 is an extended (around 8 kpc) stron
Autor:
Andy Taylor, V. S. Sigmundsson, Einar H. Gudmundsson, O. E. Rognvaldsson, E. van Kampen, J. Hjorth, Thomas R. Greve, P. Jakobsson, Simon Dye
Publikováno v:
Astronomy & Astrophysics. 386:12-30
[ABRIDGED] We estimate the total mass distribution of the galaxy cluster CL0024+1654 from the measured source depletion due to lens magnification in the R band. Within a radius of 0.54Mpc/h, a total projected mass of (8.1+/-3.2)*10^14 M_sol/h (EdS) i
Autor:
E. van Kampen, Thomas R. Greve, Andreas O. Jaunsen, Jens Hjorth, Andy Taylor, Lars Lindberg Christensen, O. E. Rognvaldsson, Pall Jakobsson, V. S. Sigmundsson, Einar H. Gudmundsson
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 322:131-140
We have obtained U and R band observations of the depletion of background galaxies due to the gravitational lensing of the galaxy cluster CL0024+1654 (z=0.39). The radial depletion curves show a significant depletion in both bands within a radius of