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  • Lotz et al. 2004; Abraham et al. 2007; Wang et al. 2012; Lee et al. 2013), and they are well suited to analyse large samples of galaxies of mixed morphologies....
  • G., 2006, ApJ, 640, L111 Tweed D., Devriendt J., Blaizot J., Colombi S., Slyz A., 2009, A&A, 506, 647 Vogelsberger M., Genel S., Sijacki D., Torrey P., Springel V., Hernquist L., 2013, MNRAS, 436, 3031 Wang T. et al., 2012, ApJ, 752, 134 Welker C., Devriendt J., Dubois Y., Pichon C., Peirani S., 2014, in press Whitaker K....
  • F., 1982, Nature, 300, 407 Zhang Y., Yang X., Faltenbacher A., Springel V., Lin W., Wang H., 2009, ApJ, 706, 747 Zhang Y., Yang X., Wang H., Wang L., Mo H....
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Measuring the primordial power spectrum: principal component analysis of the cosmic microwave background

Leach, Samuel

In: Monthly Notices of the Royal Astronomical Society, 2006, vol. 372, no. 2, p. 646-654

  • Many such power spectrum parametrizations exist and these include bandpowers (Wang, Spergel & Strauss 1999; Bridle et al. 2003; Hannestad 2004), band-colours (Bridle et al. 2003), wavelet bandpowers (Mukherjee & Wang 2003a,c), orthogonal wavelets (Mukherjee & Wang 2003b)....
  • E. et al., 2006, ApJ, 647, 813 Mukherjee P., Wang Y., 2003a, ApJ, 593, 38 Mukherjee P., Wang Y., 2003b, ApJ, 598, 779 Mukherjee P., Wang Y., 2003c, ApJ, 599, 1 Mukherjee P., Wang Y., 2005, JCAP, 0512, 007 ´ O Ruanaidh J....
  • D, 66, 103508 Tegmark M., Taylor A., Heavens A., 1997, ApJ, 480, 22 Tochini-Valentini D., Douspis M., Silk J., 2005, MNRAS, 359, 31 Verde L. et al., 2003, ApJS, 148, 195 Wang Y., Spergel D., Strauss M....
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The signature of dark energy on the local Hubble flow

Macciò, Andrea V. ; Governato, Fabio ; Horellou, Cathy

In: Monthly Notices of the Royal Astronomical Society, 2005, vol. 359, no. 3, p. 941-948

  • Wang & Steinhardt (1998) have provided an approximation to α in quintessence models, which showed that the differences between the linear peculiar velocities in models with different w are negligible, as the growth factor depends mainly on 0 and dark energy dominates only at late times....
  • It has been argued from linear perturbation theory that dark energy has little effect on the local dynamics (Lahav et al. 1991; Wang & Steinhardt 1998)....
  • J., 1992, ApJS, 80, 479 van den Bergh S., 1999, A&AR, 9, 273 Verde L. et al., 2003, ApJS, 148, 195 Wang L., Steinhardt P....
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Optimized detection of shear peaks in weak lensing maps

Marian, Laura ; Smith, Robert E. ; Hilbert, Stefan ; Schneider, Peter

In: Monthly Notices of the Royal Astronomical Society, 2012, vol. 423, no. 2, p. 1711-1725

  • Wang et al. (2004) presented a forecast for LSST in which besides WL counts Figure 6....
  • A., Wang S., Haiman Z., May M., Huffenberger K., 2011, ArXiv e-prints Kuijken K., 2010, in Block D....
  • M., Wang S., Lim E....
  • Wang et al....
  • Wang et al....
  • Wang et al....
  • This anisotropy mainly owes to a preferred direction of satellite accretion along large-scale filaments (Tormen 1997; Vitvitska et al. 2002; Aubert, Pichon & Colombi 2004; Knebe et al. 2004; Wang et al. 2005; Zentner et al. 2005b)....
  • Dubinski 1992; Warren et al. 1992; Porciani, Dekel & Hoffman 2002a; Bailin & Steinmetz 2005; Faltenbacher et al. 2005; Wang et al. 2005)....
  • S., 2002, ApJ, 581, 799 Wang H....
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Properties of dark matter haloes in clusters, filaments, sheets and voids

Hahn, Oliver ; Porciani, Cristiano ; Carollo, C. Marcella ; Dekel, Avishai

In: Monthly Notices of the Royal Astronomical Society, 2007, vol. 375, no. 2, p. 489-499

  • Wang et al. (2006) suggest that the survival of these fossil haloes may be related to the ‘temperature’ of the surrounding flow....
  • Wang et al. 2006, for a possible explanation)....
  • G., 2006, ApJ, 640, L111 Wang H....
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Structure formation with suppressed small-scale perturbations

Schneider, Aurel

In: Monthly Notices of the Royal Astronomical Society, 2015, vol. 451, no. 3, p. 3117-3130

  • Other possibilities with similar effects on small scales are decaying DM (Kaplinghat 2005; Wang et al. 2014), later forming DM (Agarwal et al. 2014), or ultralight axion DM (Marsh & Silk 2014)....
  • D, 88, 3502 Wang J., White S....
  • M., 2007, MNRAS, 380, 93 Wang M....
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Tidal effects and the environment dependence of halo assembly

Hahn, Oliver ; Porciani, Cristiano ; Dekel, Avishai ; Carollo, C. Marcella

In: Monthly Notices of the Royal Astronomical Society, 2009, vol. 398, no. 4, p. 1742-1756

  • Wang, Mo & Jing (2007) found that small old haloes tend to reside next to very massive haloes....
  • Particles that enter the Hill sphere might not be accretable if they have too high velocities to be captured by the halo (see also Wang et al. 2007)....
  • C., 2002, MNRAS, 331, 98 Wang H....
  • (3) z Here σR and σR are, respectively, the real- and redshift-space standard deviations and f (z) denotes the growth rate of structure, which in the framework of general relativity is well approximated as 0.55 f (z) m (z) (Wang & Steinhardt 1998)....
  • M., Tormen G., Kauffmann G., 2001, MNRAS, 328, 726 Springel V. et al., 2005, Nat, 435, 629 Wang L., Steinhardt P....