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Bagla J. S.
Bagla J.S.
Bagla Jasjeet S.
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J.S.
J. S.
Jasjeet S.
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http://hub.abes.fr/oup/periodical/mnras/1998/volume_299/issue_2/101046j13658711199801788x/authorship/1
http://hub.abes.fr/oup/periodical/mnras/2000/volume_314/issue_3/101046j13658711200003314x/authorship/2
http://hub.abes.fr/oup/periodical/mnras/2010/volume_405/issue_3/101111j13652966201016612x/authorship/2
http://hub.abes.fr/oup/periodical/mnras/2010/volume_407/issue_1/101111j13652966201016933x/authorship/1
http://hub.abes.fr/oup/periodical/mnras/2005/volume_360/issue_1/101111j13652966200509028x/authorship/1
http://hub.abes.fr/oup/periodical/mnras/2005/volume_360/issue_2/101111j13652966200509084x/authorship/2
http://hub.abes.fr/oup/periodical/mnras/2009/volume_395/issue_2/101111j13652966200914592x/authorship/1
http://hub.abes.fr/oup/periodical/mnras/1998/volume_297/issue_1/101046j13658711199801492x/authorship/1
http://hub.abes.fr/oup/periodical/mnras/2009/volume_396/issue_4/101111j13652966200914880x/authorship/1
http://hub.abes.fr/oup/periodical/mnras/1998/volume_294/issue_1/101046j13658711199801328x/authorship/3
http://hub.abes.fr/oup/periodical/mnras/1997/volume_286/issue_4/101093mnras28641023/authorship/1
http://hub.abes.fr/oup/periodical/mnras/2010/volume_405/issue_4/101111j13652966201016647x/authorship/2
http://hub.abes.fr/oup/periodical/mnras/2005/volume_358/issue_3/101111j13652966200508858x/authorship/1
http://hub.abes.fr/oup/periodical/mnras/2008/volume_390/issue_2/101111j13652966200813793x/authorship/1
http://hub.abes.fr/oup/periodical/mnrasl/2005/volume_356/issue_1/101111j17453933200508577x/authorship/2
http://hub.abes.fr/oup/periodical/mnras/2009/volume_393/issue_2/101111j13652966200814224x/authorship/1
http://hub.abes.fr/oup/periodical/mnras/2009/volume_397/issue_2/101111j13652966200915012x/authorship/1
http://hub.abes.fr/oup/periodical/mnras/1997/volume_289/issue_3/101093mnras2893671/authorship/1
http://hub.abes.fr/oup/periodical/mnras/2001/volume_325/issue_3/101046j13658711200104509x/authorship/2
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WMAP constraints on low redshift evolution of dark energy
Transfer of power in non-linear gravitational clustering
Clustering of galaxies at high redshifts
Gamma-ray bursts from stellar remnants: probing the Universe at high redshift
Evolution of galaxy clustering
Effects of the size of cosmological N-body simulations on physical quantities - III. Skewness
Comments on the size of the simulation box in cosmological N-body simulations
Gravitational collapse in an expanding background and the role of substructure - II. Excess power at small scales and its effect on collapse of structures at larger scales
H i as a probe of the large-scale structure in the post-reionization universe
Fractal dimensions of a weakly clustered distribution and the scale of homogeneity
Fractal dimension as a measure of the scale of homogeneity
The observed evolution of galaxy clustering versus epoch-dependent biasing models
Metal enrichment and reionization constraints on early star formation
Understanding the origin of CMB constraints on dark energy
Gravitational collapse in an expanding universe: scaling relations for two-dimensional collapse revisited
The Adaptive TreePM: an adaptive resolution code for cosmological N-body simulations
Neutral hydrogen at high redshifts as a probe of structure formation - III. Radio maps from TV-body simulations
A comparison of simulated and analytic major merger counts
Gravitational collapse in an expanding background and the role of substructure - I. Planar collapse
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