His main research concerns Astrophysics, Galaxy, Galaxy cluster, Redshift and Astronomy. His Dark matter, Redshift survey, Cosmology, Halo and Dark energy investigations are all subjects of Astrophysics research. His research investigates the connection with Dark matter and areas like Cluster which intersect with concerns in Substructure and Gravitational lens.
His work investigates the relationship between Cosmology and topics such as Cosmic microwave background that intersect with problems in Hydrostatic equilibrium. His biological study deals with issues like Surface brightness, which deal with fields such as Observable. His studies deal with areas such as Star formation, Universe, Photometry and Cluster analysis as well as Redshift.
Lauro Moscardini mainly investigates Astrophysics, Galaxy, Redshift, Galaxy cluster and Dark matter. His research on Astrophysics often connects related areas such as Astronomy. His study in Galaxy is interdisciplinary in nature, drawing from both COSMIC cancer database, Cluster analysis and Sky.
His Redshift study combines topics from a wide range of disciplines, such as Dark energy, Luminosity and Cosmic microwave background. His work carried out in the field of Galaxy cluster brings together such families of science as Universe, Structure formation and Gravitational lens. In his study, Scalar field dark matter and Lambda-CDM model is inextricably linked to Dark fluid, which falls within the broad field of Dark matter.
His primary areas of study are Astrophysics, Galaxy, Redshift, Galaxy cluster and Redshift survey. Lauro Moscardini has included themes like Astronomy and Cluster in his Astrophysics study. His Galaxy research includes themes of Telescope, Cosmic microwave background and Sky.
The various areas that Lauro Moscardini examines in his Redshift study include Dark energy, Halo and Stellar mass. His research integrates issues of Amplitude, Range and Density contrast in his study of Galaxy cluster. His Redshift survey research incorporates themes from Cosmic time, Very Large Telescope, Photometry, Function and Sigma.
The scientist’s investigation covers issues in Astrophysics, Galaxy, Redshift, Redshift survey and Astronomy. His research in Astrophysics focuses on subjects like Sigma, which are connected to Distribution. His Galaxy research focuses on Galaxy cluster in particular.
The concepts of his Redshift study are interwoven with issues in Cosmology, Dark energy, Function and Algorithm. Within one scientific family, Lauro Moscardini focuses on topics pertaining to Dark matter under Cosmology, and may sometimes address concerns connected to Correlation function. He studied Redshift survey and Very Large Telescope that intersect with Observatory and Telescope.
This overview was generated by a machine learning system which analysed the scientist’s body of work. If you have any feedback, you can contact us here.
Euclid Definition Study Report
N. Shane;J.~-. Starck;C. Surace;A. Taylor.
arXiv: Cosmology and Nongalactic Astrophysics (2011)
Measuring and modelling the redshift evolution of clustering: the Hubble Deep Field North
S Arnouts;S Arnouts;Stefano Cristiani;Stefano Cristiani;Lauro Moscardini;Sabino Matarrese.
Monthly Notices of the Royal Astronomical Society (1999)
A test of the nature of cosmic acceleration using galaxy redshift distortions
L. Guzzo;M. Pierleoni;B. Meneux;E. Branchini.
Nature (2008)
Comparing the temperatures of galaxy clusters from hydro-N-body simulations to Chandra and XMM-Newton observations
P. Mazzotta;P. Mazzotta;E. Rasia;L. Moscardini;G. Tormen.
arXiv: Astrophysics (2004)
X‐ray properties of galaxy clusters and groups from a cosmological hydrodynamical simulation
Stefano Borgani;G. Murante;V. Springel;A. Diaferio.
Monthly Notices of the Royal Astronomical Society (2004)
The VIMOS Public Extragalactic Redshift Survey (VIPERS). An unprecedented view of galaxies and large-scale structure at 0.5<z<1.2
L. Guzzo;M. Scodeggio;B. Garilli;B. R. Granett.
arXiv: Cosmology and Nongalactic Astrophysics (2013)
Comparing the temperatures of galaxy clusters from hydrodynamical N-body simulations to Chandra and XMM-Newton observations
P. Mazzotta;P. Mazzotta;E. Rasia;Lauro Moscardini;G. Tormen.
Monthly Notices of the Royal Astronomical Society (2004)
Virial Scaling of Massive Dark Matter Halos: Why Clusters Prefer a High Normalization Cosmology
August E. Evrard;August E. Evrard;James Bialek;Michael T. Busha;Martin White.
The Astrophysical Journal (2008)
The VIMOS Public Extragalactic Redshift Survey (VIPERS) - Galaxy clustering and redshift-space distortions at z ≃ 0.8 in the first data release
S. de la Torre;L. Guzzo;L. Guzzo;J. A. Peacock;E. Branchini;E. Branchini.
Astronomy and Astrophysics (2013)
Numerical study of halo concentrations in dark-energy cosmologies
K. Dolag;M. Bartelmann;F. Perrotta;F. Perrotta;C. Baccigalupi;C. Baccigalupi.
Astronomy and Astrophysics (2004)
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