2014
DOI: 10.1093/mnras/stt2431
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The properties of warm dark matter haloes

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Cited by 479 publications
(676 citation statements)
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References 68 publications
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“…• We present a method to estimate the number of substructures in a host halo, and show that it agrees very well with warm DM simulations from Lovell et al (2014). Based on this, we provide approximative constraints on mixed DM models by comparing the expected number of substructures to the observed number of Milky-Way satellites.…”
Section: Discussionmentioning
confidence: 59%
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“…• We present a method to estimate the number of substructures in a host halo, and show that it agrees very well with warm DM simulations from Lovell et al (2014). Based on this, we provide approximative constraints on mixed DM models by comparing the expected number of substructures to the observed number of Milky-Way satellites.…”
Section: Discussionmentioning
confidence: 59%
“…Number of predicted Milky-Way satellites with mass above 10 8 h −1 M from the model (Eq. 17) and from simulations by Lovell et al (2014). For the case of CDM the perfect agreement is by construction, since the model is calibrated to this number.…”
Section: Estimating the Number Of Dwarf Satellitesmentioning
confidence: 87%
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“…Historically, cosmological WDM simulations, and hence semi-analytic galaxy formation models built on them, have suffered from uncertainties introduced by spurious selfbound DM clumps arising from numerical discreetness effects (Wang & White 2007). These spurious haloes have been carefully removed from the halo catalogue on which our GALFORM model is based by applying the procedure of Lovell et al (2014), which improves the reliability of comparisons between our results and observations. We note that hydrodynamical simulations by Gao & Theuns (2007) and Gao et al (2015) have demonstrated a novel star formation mechanism in WDM, which occurs in filaments rather than in collapsed dark matter haloes.…”
Section: Introductionmentioning
confidence: 98%