- 2003
- Published
Very high column density and small reddening towards GRB 020124 at z=3.20
Hjorth, Jens, Møller, P., Gorosabel, J., Fynbo, Johan Peter Uldall, Toft, Sune, Jaunsen, A. O., Kaas, A. A., Pursimo, T., Torii, K., Kato, T., Yamaoka, H., Yoshida, A., Thomsen, B., Andersen, M. I., Burud, I., Kasper, L., Palazzi, E., Pian, E. & Van den Heuvel, E. P. J., 2003, In: Astrophysical Journal. 597, 2, p. 699-705Research output: Contribution to journal › Journal article › Research › peer-review
- Published
X-ray, Lya and Ha emission from simulated disk galaxies
Sommer-Larsen, J., Toft, Sune, Rasmussen, J., Pedersen, K., Götz, M. & Portinari, L., 2003, In: Astrophysics and Space Science. 284, p. 693-696Research output: Contribution to journal › Journal article › Research › peer-review
- Published
The galaxy population of the z= 1 cluster of galaxies MG2016+112
Toft, Sune, Soucail, G. & Hjorth, Jens, 1 Sep 2003, In: Monthly Notices of the Royal Astronomical Society. 344, p. 337-346 10 p.Research output: Contribution to journal › Journal article › Research › peer-review
- Published
Discovery of an overdensity of faint red galaxies in the vicinity of the z=1.786 radio galaxy 3C294*
Toft, Sune, Pedersen, K., Ebeling, H. & Hjorth, Jens, 2003, In: Monthly Notices of the Royal Astronomical Society. 341, p. 55-58Research output: Contribution to journal › Journal article › Research › peer-review
- Published
GRB 130603B: VLT/X-shooter redshift confirmation.
Xu, D., de Ugarte Postigo, A., Malesani, Daniele Bjørn, Schulze, S., Fynbo, Johan Peter Uldall, Watson, Darach Jafar, D'Elia, V., Goldoni, P. & Vestergaard, Marianne, 2003, In: GRB Coordinates Network, Circular Service, No. 14757. 4757, p. 1Research output: Contribution to journal › Journal article › Research › peer-review
- 2004
- Published
Magnetic field generation in collisionless shocks: pattern growth and transport
Frederiksen, J. T., Hededal, C. B., Haugbølle, Troels & Nordlund, Åke, 13 Mar 2004, In: Astrophysical Journal. 608, 1, p. L13-L16 3 p.Research output: Contribution to journal › Journal article › Research › peer-review
- Published
Non-fermi power-law acceleration in astrophysical plasma shocks
Hededal, C. B., Haugbølle, Troels, Frederiksen, J. T. & Nordlund, Åke, 22 Nov 2004, In: Astrophysical Journal. 617, 2, p. L107-L110 3 p.Research output: Contribution to journal › Journal article › Research › peer-review
- Published
Deep near-infrared imaging of RDCS J1252.9-2927 at z = 1.237. The colour-magnitude diagram
Lidman, C., Rosati, P., Demarco, R., Nonino, M., Mainieri, V., Stanford, S. ~. & Toft, Sune, 1 Mar 2004, In: Astronomy & Astrophysics. 416, p. 829-837 9 p.Research output: Contribution to journal › Journal article › Research › peer-review
- Published
Detection of Lyman-α emission from a DLA galaxy: Possible implications for a luminosity-metallicity relation at z = 2-3
Møller, P., Fynbo, Johan Peter Uldall & Fall, S. M., 1 Aug 2004, In: Astronomy and Astrophysics. 422, 2, p. L33-L37Research output: Contribution to journal › Journal article › Research › peer-review
- Published
The supernova 2003lw associated with X-ray flash 031203
Thomsen, B., Hjorth, Jens, Watson, Darach Jafar, Gorosabel, J., Fynbo, Johan Peter Uldall, Jensen, B. L., Andersen, Michael Ingemann, Dall, T. H., Rasmussen, J. R., Bruntt, H., Laurikainen, E., Augusteijn, T., Pursimo, T., Germany, L., Jakobsson, P. & Pedersen, K., 1 May 2004, In: Astronomy and Astrophysics. 419, 2, p. L21-L25Research output: Contribution to journal › Journal article › Research › peer-review
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Divergent reflections around the photon sphere of a black hole
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176
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Challenges and Techniques for Simulating Line Emission
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168
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Spitzer Matching Survey of the UltraVISTA Ultra-deep Stripes (SMUVS): Full-mission IRAC Mosaics and Catalogs
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Impact of Helium ii Resonant Absorption on the Ultraviolet Background Modeled in Three Dimensions
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A Steep Decline in the Galaxy Space Density beyond Redshift 9 in the CANUCS UV Luminosity Function
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The Heavy Metal Survey: Star Formation Constraints and Dynamical Masses of 21 Massive Quiescent Galaxies at z = 1.3–2.3
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