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1by Manolis Plionis“... model of Basilakos et al., we manage to break the σ₈–Ωₘ degeneracy. The resulting cosmological...”
Published 2010
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2by Manolis Plionis“... of σ₈, we find stringent simultaneous constraints in the (Ωₘ, w) plane, with Ωₘ= 0.26 ± 0.05, w =−0.93⁺⁰˙¹¹₋₀․₁₉....”
Published 2009
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3by Manolis Plionis“... halo mass is ∼ 10¹³ h⁻¹ Mꙩ and ≿5 × 10¹³ h⁻¹ Mꙩ, respectively....”
Published 2008
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4by Manolis Plionis“... of Mₕ ≃ 2.7 (±0.6) × 10¹² h⁻¹MꙨ, while the corresponding value for optical galaxies is Mₕ≃ 6.3 (±2.1...”
Published 2012
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5by Manolis Plionis“...We use group-sized haloes, with masses in the range 1013 < M < 2 × 1014 h−1Mʘ, identified with a...”
Published 2007
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7by Manolis Plionis“... band sources (at a median ¯z ≃ 1), which translates into a host dark matter halo mass of ∼ 10¹³ h⁻¹Mꙩ...”
Published 2012
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9by Manolis Plionis, ROBERTO GIOVANNI TERLEVICH AFONSO, Elena Kirilovsky Terlevich, RICARDO CHAVEZ MURILLO“... relation of the Constitution SNIa set provide Ωₘ =0.31±0.01 and ω=−1.06 ± 0.05.We also find that the joint...”
Published 2011
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11by Manolis Plionis“...We estimate the two-point correlation function of dark matter haloes, with masses ≥ 1013 h−1 M...”
Published 2007
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12by Manolis Plionis“...We use dark matter haloes identified in the M🇦🇷🇪N🇴🇸🇹🇷🇺🇲 U🇳🇮🇻🇪🇷🇸🇪🇽 and galaxy...”
Published 2010
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15by Manolis Plionis“...¹³ h⁻¹M⨀. The Xray AGN bias and the corresponding dark-matter host halo mass, are significantly higher...”
Published 2013
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16by Manolis Plionis“...¹³h⁻¹Mꙩ. The Xray AGN bias and the corresponding dark-matter host halo mass, are significantly higher...”
Published 2012
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