Search Results - Debackere, Stijn N B

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  1. 1
    The impact of the observed baryon distribution in haloes on the total matter power spectrum

    The impact of the observed baryon distribution in haloes on the total matter power spectrum by Debackere, Stijn N B, Schaye, Joop, Hoekstra, Henk

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  2. 2
    How baryons can significantly bias cluster count cosmology

    How baryons can significantly bias cluster count cosmology by Debackere, Stijn N B, Schaye, Joop, Hoekstra, Henk

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  3. 3
    Galaxy cluster aperture masses are more robust to baryonic effects than 3D halo masses

    Galaxy cluster aperture masses are more robust to baryonic effects than 3D halo masses by Debackere, Stijn N B, Hoekstra, Henk, Schaye, Joop

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  4. 4
    Why are we still using 3D masses for cluster cosmology?

    Why are we still using 3D masses for cluster cosmology? by Debackere, Stijn N B, Hoekstra, Henk, Schaye, Joop, Heitmann, Katrin, Habib, Salman

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  5. 5
    How baryons can significantly bias cluster count cosmology

    How baryons can significantly bias cluster count cosmology by Debackere, Stijn N B, Schaye, Joop, Hoekstra, Henk

    Published in arXiv.org
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  6. 6
    Galaxy cluster aperture masses are more robust to baryonic effects than 3D halo masses

    Galaxy cluster aperture masses are more robust to baryonic effects than 3D halo masses by Debackere, Stijn N B, Hoekstra, Henk, Schaye, Joop

    Published in arXiv.org
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  7. 7
    Why are we still using 3D masses for cluster cosmology?

    Why are we still using 3D masses for cluster cosmology? by Debackere, Stijn N B, Hoekstra, Henk, Schaye, Joop, Heitmann, Katrin, Habib, Salman

    Published in arXiv.org
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  8. 8
    The impact of the observed baryon distribution in haloes on the total matter power spectrum

    The impact of the observed baryon distribution in haloes on the total matter power spectrum by Debackere, Stijn N B, Schaye, Joop, Hoekstra, Henk

    Published in arXiv.org
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