All Stories

  1. Halo mass functions in mixed cold and fuzzy dark matter models
  2. Can we extract the intrinsic properties of galaxies from observables?
  3. Sub-millimetre galaxies in hierarchical models: revisiting the need for a top-heavy stellar initial mass function with Bayesian optimization
  4. The PAU Survey: the i -band galaxy luminosity function from the present-day to  z = 2
  5. Outcome of preterm infants (<30 weeks) born to mothers who smoked: propensity score matching study
  6. Using machine learning to classify galaxies
  7. The PAU Survey: measuring intrinsic galaxy alignments in deep wide fields as a function of colour, luminosity, stellar mass, and redshift
  8. How many galaxies should the James Webb Space Telescope see?
  9. Galaxy assembly and evolution in the P-Millennium simulation: Galaxy clustering
  10. Euclid
  11. ANNZ+: an enhanced photometric redshift estimation algorithm with applications on the PAU survey
  12. The PAU survey
  13. The diverse star formation histories of early massive, quenched galaxies in modern galaxy formation simulations
  14. A comparison of pre-existing ΛCDM predictions with the abundance of JWST galaxies at high redshift
  15. How many emission line galaxies will Euclid and Roman see?
  16. The PAU survey: photometric redshift estimation in deep wide fields
  17. The PAU Survey: Galaxy stellar population properties estimates with narrowband data
  18. Galaxy evolution in modified gravity simulations: using galaxy properties to constrain our gravitational model
  19. The Euclid mission: status after launch and early operations
  20. The Uchuu-glam BOSS and eBOSS LRG lightcones: exploring clustering and covariance errors
  21. Understanding the radio luminosity function of star-forming galaxies and its cosmological evolution
  22. A new test of gravity – I. Introduction to the method
  23. The PAU Survey: a new constraint on galaxy formation models using the observed colour redshift relation
  24. Correction to: How limiting is optical follow-up for fast radio burst applications? Forecasts for radio and optical surveys
  25. A new test of gravity – II. Application of marked correlation functions to luminous red galaxy samples
  26. Carbon dioxide monitoring during neonatal stabilisation at delivery (COSTA-Neo)-multi centre observational study
  27. An emulator-based halo model in modified gravity – I. The halo concentration–mass relation and density profile
  28. How limiting is optical follow-up for fast radio burst applications? Forecasts for radio and optical surveys
  29. Galaxy clustering from the bottom up: a streaming model emulator I
  30. The buildup of galaxies and their spheroids: The contributions of mergers, disc instabilities, and star formation
  31. Towards an accurate model of small-scale redshift-space distortions in modified gravity
  32. Fast full N-body simulations of generic modified gravity: conformal coupling models
  33. Fast full N-body simulations of generic modified gravity: derivative coupling models
  34. Halo merger tree comparison: impact on galaxy formation models
  35. Modelling emission lines in star-forming galaxies
  36. Making use of sub-resolution haloes in N-body simulations
  37. Statistics of galaxy mergers: bridging the gap between theory and observation
  38. A machine learning approach to mapping baryons on to dark matter haloes using theeagleandC-EAGLEsimulations
  39. Preliminary clustering properties of the DESI BGS bright targets using DR9 Legacy Imaging Surveys
  40. Efficient exploration and calibration of a semi-analytical model of galaxy formation with deep learning
  41. The assembly bias of emission-line galaxies
  42. Modelling the quenching of star formation activity from the evolution of the colour-magnitude relation in VIPERS
  43. Galaxy formation in the brane world I: overview and first results
  44. Erratum: The host dark matter haloes of [O ii]  emitters at 0.5 < z < 1.5
  45. Building a digital twin of a luminous red galaxy spectroscopic survey: galaxy properties and clustering covariance
  46. Characterizing the target selection pipeline for the Dark Energy Spectroscopic Instrument Bright Galaxy Survey
  47. The PAU Survey: an improved photo-zsample in the COSMOS field
  48. Determining the systemic redshift of Lyman α emitters with neural networks and improving the measured large-scale clustering
  49. Preliminary Target Selection for the DESI Bright Galaxy Survey (BGS)
  50. Are Ly α emitters segregated in protoclusters regions?
  51. Do model emission line galaxies live in filaments at z ∼ 1?
  52. Towards a non-Gaussian model of redshift space distortions
  53. Measuring the baryon acoustic oscillation peak position with different galaxy selections
  54. Constraining structure formation using EDGES
  55. Multiwavelength consensus of large-scale linear bias
  56. AGNs at the cosmic dawn: predictions for future surveys from a ΛCDM cosmological model
  57. Sensitivity analysis of a galaxy formation model
  58. On the Prospect of Using the Maximum Circular Velocity of Halos to Encapsulate Assembly Bias in the Galaxy–Halo Connection
  59. Lyα emitters in a cosmological volume II: the impact of the intergalactic medium
  60. Extensions to the halo occupation distribution model for more accurate clustering predictions
  61. The connection between halo concentrations and assembly histories: a probe of gravity?
  62. Euclid preparation
  63. The evolution of the UV-to-mm extragalactic background light: evidence for a top-heavy initial mass function?
  64. Linear bias forecasts for emission line cosmological surveys
  65. The evolution of SMBH spin and AGN luminosities for z < 6 within a semi-analytic model of galaxy formation
  66. A new approach to finding galaxy groups using Markov Clustering
  67. Lyα emitters in a cosmological volume – I. The impact of radiative transfer
  68. The effect of assembly bias on redshift-space distortions
  69. Large-scale redshift space distortions in modified gravity theories
  70. Correcting for fibre assignment incompleteness in the DESI Bright Galaxy Survey
  71. The evolution of assembly bias
  72. Galaxy formation in the Planck Millennium: the atomic hydrogen content of dark matter haloes
  73. N-body simulations of structure formation in thermal inflation cosmologies
  74. Evolution of galactic magnetic fields
  75. No evidence for modifications of gravity from galaxy motions on cosmological scales
  76. The PAU Survey: spectral features and galaxy clustering using simulated narrow-band photometry
  77. Uncovering substructure with wavelets:proof of concept using Abell 2744
  78. Growing a ‘cosmic beast’: observations and simulations of MACS J0717.5+3745
  79. Nonlinear growth of structure in cosmologies with damped matter fluctuations
  80. The environment of radio galaxies: a signature of AGN feedback at high redshifts
  81. Marked clustering statistics in f(R) gravity cosmologies
  82. A new smooth-k space filter approach to calculate halo abundances
  83. The Impact of Assembly Bias on the Galaxy Content of Dark Matter Halos
  84. Predictions for deep galaxy surveys with JWST from ΛCDM
  85. The effect of thermal velocities on structure formation in N-body simulations of warm dark matter
  86. The host dark matter haloes of [O II] emitters at 0.5 < z < 1.5
  87. A lightcone catalogue from the Millennium-XXL simulation
  88. Understanding the non-linear clustering of high-redshift galaxies
  89. Blending bias impacts the host halo masses derived from a cross-correlation analysis of bright submillimetre galaxies
  90. Abell 2744: too much substructure for ΛCDM?
  91. The far infra-red SEDs of main sequence and starburst galaxies
  92. Subhalo Abundance Matching in f(R) Gravity
  93. The evolution of the galaxy content of dark matter haloes
  94. The spatial distribution of neutral hydrogen as traced by low H i mass galaxies
  95. The extraordinary amount of substructure in theHubble Frontier Fieldscluster Abell 2744
  96. Isotropic extragalactic flux from dark matter annihilations: lessons from interacting dark matter scenarios
  97. A unified multiwavelength model of galaxy formation
  98. Measuring galaxy environment with the synergy of future photometric and spectroscopic surveys
  99. The clustering of dark matter haloes: scale-dependent bias on quasi-linear scales
  100. CAN WE DETECT THE COLOR–DENSITY RELATION WITH PHOTOMETRIC REDSHIFTS?
  101. The clustering and halo occupation distribution of Lyman-break galaxies atz ∼ 4
  102. Dark matter–radiation interactions: the structure of Milky Way satellite galaxies
  103. The clustering evolution of dusty star-forming galaxies
  104. Modelling the number density of Hαemitters for future spectroscopic near-IR space missions
  105. Can we distinguish early dark energy from a cosmological constant?
  106. The environments of high-redshift radio galaxies and quasars: probes of protoclusters
  107. The abundance and colours of galaxies in high-redshift clusters in the cold dark matter cosmology
  108. The evolution of the stellar mass versus halo mass relationship
  109. A hybrid multiresolution scheme to efficiently model the structure of reionization on the largest scales
  110. Galaxy cluster lensing masses in modified lensing potentials
  111. The H i mass function as a probe of photoionization feedback on low-mass galaxy formation
  112. Weak lensing by voids in modified lensing potentials
  113. The galaxy–dark matter halo connection: which galaxy properties are correlated with the host halo mass?
  114. A new methodology to test galaxy formation models using the dependence of clustering on stellar mass
  115. Galactic magnetic fields and hierarchical galaxy formation
  116. Dark matter–radiation interactions: the impact on dark matter haloes
  117. The 0.1 <z< 1.65 evolution of the bright end of the [O ii] luminosity function
  118. The origin of the atomic and molecular gas contents of early-type galaxies – II. Misaligned gas accretion
  119. The environments of Ly α blobs – I. Wide-field Ly α imaging of TN J1338−1942, a powerful radio galaxy at z ≃ 4.1 associated with a giant Ly α nebula★
  120. Simulated observations of sub-millimetre galaxies: the impact of single-dish resolution and field variance
  121. Velocity and mass bias in the distribution of dark matter haloes
  122. Galaxy And Mass Assembly (GAMA): the dependence of the galaxy luminosity function on environment, redshift and colour
  123. Nonlinear structure formation in nonlocal gravity
  124. The evolution of the star-forming sequence in hierarchical galaxy formation models
  125. Using the Milky Way satellites to study interactions between cold dark matter and radiation
  126. The observational status of Galileon gravity after Planck
  127. Clustering tomography: measuring cosmological distances through angular clustering in thin redshift shells
  128. Modified gravity with massive neutrinos as a testable alternative cosmological model
  129. The origin of the atomic and molecular gas contents of early-type galaxies – I. A new test of galaxy formation physics
  130. Extending the halo mass resolution of N-body simulations
  131. Herschel-ATLAS/GAMA: How does the far-IR luminosity function depend on galaxy group properties?
  132. PROBABILITY FRIENDS-OF-FRIENDS (PFOF) GROUP FINDER: PERFORMANCE STUDY AND OBSERVATIONAL DATA APPLICATIONS ON PHOTOMETRIC SURVEYS
  133. Halo model and halo properties in Galileon gravity cosmologies
  134. Which galaxies dominate the neutral gas content of the Universe?
  135. How sensitive are predicted galaxy luminosities to the choice of stellar population synthesis model?
  136. Clustering of extremely red objects in Elais-N1 from the UKIDSS DXS with optical photometry from Pan-STARRS 1 and Subaru
  137. Spherical collapse in Galileon gravity: fifth force solutions, halo mass function and halo bias
  138. Simulating the quartic Galileon gravity model on adaptively refined meshes
  139. Nonlinear structure formation in the cubic Galileon gravity model
  140. A dynamical model of supernova feedback: gas outflows from the interstellar medium
  141. The most luminous quasars do not live in the most massive dark matter haloes at any redshift
  142. Constraints on black hole fuelling modes from the clustering of X-ray AGN
  143. How well can we really estimate the stellar masses of galaxies from broad-band photometry?
  144. Parameter space in Galileon gravity models
  145. How robust are predictions of galaxy clustering?
  146. Single-colour diagnostics of the mass-to-light ratio – I. Predictions from galaxy formation models
  147. Luminosity Bias: From Haloes to Galaxies
  148. The ultraviolet colours and dust attenuation of Lyman-break galaxies
  149. Lightcone mock catalogues from semi-analytic models of galaxy formation – I. Construction and application to the BzK colour selection
  150. Linear perturbations in Galileon gravity models
  151. On the role of feedback in shaping the cosmic abundance and clustering of neutral atomic hydrogen in galaxies
  152. The accuracy of the UV continuum as an indicator of the star formation rate in galaxies
  153. The non-linear matter and velocity power spectra in f(R) gravity
  154. Predictions for the CO emission of galaxies from a coupled simulation of galaxy formation and photon-dominated regions
  155. Scaling relations for galaxy clusters in the Millennium-XXL simulation
  156. The clustering of Hα emitters atz=2.23 from HiZELS
  157. The contribution of star-forming galaxies to fluctuations in the cosmic background light
  158. The journey of QSO haloes from z ∼ 6 to the present
  159. Redshift-space distortions in f(R) gravity
  160. CLUSTERING PROPERTIES OF BzK-SELECTED GALAXIES IN GOODS-N: ENVIRONMENTAL QUENCHING AND TRIGGERING OF STAR FORMATION ATz∼ 2
  161. The evolution of massive galaxies in semi-analytical models of galaxy formation
  162. Clustering of EROs from UKIDSS DXS and Pan-STARRS PS1
  163. Can galactic outflows explain the properties of Ly α emitters?
  164. Predictions for the intrinsic UV continuum properties of star-forming galaxies and the implications for inferring dust extinction
  165. The nature and descendants of Lyman-break galaxies in the Λ cold dark matter cosmology
  166. Testing dark energy using pairs of galaxies in redshift space
  167. The evolution of active galactic nuclei across cosmic time: what is downsizing?
  168. Cosmic evolution of the atomic and molecular gas contents of galaxies
  169. Statistical analysis of galaxy surveys - IV. An objective way to quantify the impact of superstructures on galaxy clustering statistics
  170. Modelling the dusty universe - II. The clustering of submillimetre-selected galaxies
  171. Massive, red galaxies in a hierarchical universe - II. Clustering of Extremely Red Objects
  172. On the impact of empirical and theoretical star formation laws on galaxy formation
  173. The spatial distribution of cold gas in hierarchical galaxy formation models
  174. Are the superstructures in the two-degree field galaxy redshift survey a problem for hierarchical models?
  175. Which haloes host Herschel-ATLAS galaxies in the local Universe?
  176. The role of submillimetre galaxies in hierarchical galaxy formation
  177. The evolution of Lyman-break galaxies in the cold dark matter model
  178. TESTING GRAVITY USING THE GROWTH OF LARGE-SCALE STRUCTURE IN THE UNIVERSE
  179. Modelling the spectral energy distribution of galaxies: introducing the artificial neural network
  180. Grand unification of AGN activity in the ΛCDM cosmology
  181. Effects of cosmological model assumptions on galaxy redshift survey measurements
  182. Modelling redshift space distortions in hierarchical cosmologies
  183. Designing a space-based galaxy redshift survey to probe dark energy
  184. The parameter space of galaxy formation
  185. The redshift evolution of the mass function of cold gas in hierarchical galaxy formation models
  186. Probing dark energy with future redshift surveys: a comparison of emission line and broad-band selection in the near-infrared
  187. Predictions forHerschelfrom Λ-cold dark matter: unveiling the cosmic star formation history
  188. Empirical Hα emitter count predictions for dark energy surveys
  189. Simulations of quintessential cold dark matter: beyond the cosmological constant
  190. How BAO measurements can fail to detect quintessence
  191. Extremely Red Objects in a Hierarchical Universe
  192. Modelling the dusty universe - I. Introducing the artificial neural network and first applications to luminosity and colour distributions
  193. Cosmological parameter constraints from SDSS luminous red galaxies: a new treatment of large-scale clustering
  194. Modelling galaxy clustering: is new physics needed in galaxy formation models?
  195. The fate of substructures in cold dark matter haloes
  196. Evolution of supermassive black hole spins in the ΛCDM cosmology
  197. Massive, red galaxies in a hierarchical universe - I. Counts of extremely red objects and basic properties
  198. Testing model predictions of the cold dark matter cosmology for the sizes, colours, morphologies and luminosities of galaxies with the SDSS
  199. Statistical analysis of galaxy surveys - I. Robust error estimation for two-point clustering statistics
  200. Mock galaxy redshift catalogues from simulations: implications for Pan-STARRS1
  201. The clustering of Lyα emitters in a ΛCDM Universe
  202. The properties of submm galaxies in hierarchical models
  203. Science with ASKAP
  204. What is the best way to measure baryonic acoustic oscillations?
  205. Creating synthetic universes in a computer
  206. The colours of satellite galaxies in groups and clusters
  207. Offspring of SPACE: the spectrograph channel of the ESA Dark Energy Mission EUCLID
  208. The 2dF-SDSS LRG and QSO Survey: evolution of the clustering of luminous red galaxies since z = 0.6
  209. Luminous red galaxies in hierarchical cosmologies
  210. The assembly bias of dark matter haloes to higher orders
  211. SPACE: the spectroscopic all-sky cosmic explorer
  212. Galaxy evolution in the infrared: comparison of a hierarchical galaxy formation model with Spitzer data
  213. Black hole growth in hierarchical galaxy formation
  214. The detectability of baryonic acoustic oscillations in future galaxy surveys
  215. Narrow-band surveys for very high redshift Lyman-$\mathsf{\alpha}$ emitters
  216. Statistical analysis of galaxy surveys - III. The non-linear clustering of red and blue galaxies in the 2dFGRS
  217. The structural and photometric properties of early-type galaxies in hierarchical models
  218. Science with the Australian Square Kilometre Array Pathfinder
  219. A primer on hierarchical galaxy formation: the semi-analytical approach
  220. Breaking the hierarchy of galaxy formation
  221. Galaxy groups in the 2dF Galaxy Redshift Survey: the number density of groups
  222. Cosmic cookery: growing galaxies in a computer
  223. Cosmological parameters from cosmic microwave background measurements and the final 2dF Galaxy Redshift Survey power spectrum
  224. Cosmic cookery: making a stereoscopic 3D animated movie
  225. The properties of Ly  emitting galaxies in hierarchical galaxy formation models
  226. The metal enrichment of galaxies and galaxy clusters in the cold dark matter universe
  227. Statistical analysis of galaxy surveys — II. The three-point galaxy correlation function measured from the 2dFGRS
  228. Theoretical Models of the Halo Occupation Distribution: Separating Central and Satellite Galaxies
  229. The 2dF Galaxy Redshift Survey: correlation with the ROSAT-ESO flux-limited X-ray galaxy cluster survey
  230. The SCUBA Half-Degree Extragalactic Survey -- I. Survey motivation, design and data processing
  231. The metal enrichment of elliptical galaxies in hierarchical galaxy formation models
  232. The 2dF Galaxy Redshift Survey: power-spectrum analysis of the final data set and cosmological implications
  233. Constraints on the dark energy equation of state from the imprint of baryons on the power spectrum of clusters
  234. Where are the stars?
  235. The metal enrichment of the intracluster medium in hierarchical galaxy formation models
  236. The abundance of Lyα emitters in hierarchical models
  237. The 2dF Galaxy Redshift Survey: the nature of the relative bias between galaxies of different spectral type
  238. Can the faint submillimetre galaxies be explained in the Λ cold dark matter model?
  239. The 2dF Galaxy Redshift Survey: luminosity functions by density environment and galaxy type
  240. The 2dF Galaxy Redshift Survey: stochastic relative biasing between galaxy populations
  241. Galaxy groups in the Two-degree Field Galaxy Redshift Survey: the luminous content of the groups
  242. The 2dF Galaxy Redshift Survey: the local E+A galaxy population
  243. Galaxy evolution, cosmology and dark energy with the Square Kilometer Array
  244. Predictions for the SKA from hierarchical galaxy formation models
  245. The 2dF Galaxy Redshift Survey: spherical harmonics analysis of fluctuations in the final catalogue
  246. The 2dF Galaxy Redshift Survey: Wiener reconstruction of the cosmic web
  247. The 2dF Galaxy Redshift Survey: voids and hierarchical scaling models
  248. Substructure analysis of selected low-richness 2dFGRS clusters of galaxies
  249. The 2dF Galaxy Redshift Survey: higher-order galaxy correlation functions
  250. The 2dF Galaxy Redshift Survey: the clustering of galaxy groups
  251. Heating of galactic discs by infalling satellites
  252. The 2dF Galaxy Redshift Survey: hierarchical galaxy clustering
  253. The 2dF Galaxy Redshift Survey: the blue galaxy fraction and implications for the Butcher-Oemler effect
  254. Chemical enrichment of ICM in a hierarchical galaxy formation model including SNe Ia
  255. Galaxy groups in the 2dFGRS: the group-finding algorithm and the 2PIGG catalogue
  256. Galaxy ecology: groups and low-density environments in the SDSS and 2dFGRS
  257. What Shapes the Luminosity Function of Galaxies?
  258. The 2dF Galaxy Redshift Survey: correlation functions, peculiar velocities and the matter density of the Universe
  259. The 2dF Galaxy Redshift Survey: galaxy clustering per spectral type
  260. The power spectrum of galaxy clustering in the APM Survey
  261. The Halo Occupation Distribution and the Physics of Galaxy Formation
  262. The effects of photoionization on galaxy formation — III. Environmental dependence in the luminosity function
  263. The properties of spiral galaxies: confronting hierarchical galaxy formation models with observations
  264. The 2dF Galaxy Redshift Survey: the luminosity function of cluster galaxies
  265. Universal building blocks
  266. A comparison of gas dynamics in smooth particle hydrodynamics and semi-analytic models of galaxy formation
  267. Galaxy formation using halo merger histories taken from N-body simulations
  268. Parameter constraints for flat cosmologies from cosmic microwave background and 2dFGRS power spectra
  269. The 2dF Galaxy Redshift Survey: the bJ-band galaxy luminosity function and survey selection function
  270. The 2dF Galaxy Redshift Survey: the bias of galaxies and the density of the Universe
  271. The 2dF Galaxy Redshift Survey: the environmental dependence of galaxy star formation rates near clusters
  272. New Upper Limit on the Total Neutrino Mass from the 2 Degree Field Galaxy Redshift Survey
  273. The 2dF Galaxy Redshift Survey: the amplitudes of fluctuations in the 2dFGRS and the CMB, and implications for galaxy biasing
  274. The 2dF Galaxy Redshift Survey: galaxy luminosity functions per spectral type
  275. The 2dF Galaxy Redshift Survey: the dependence of galaxy clustering on luminosity and spectral type
  276. On the formation of globular cluster systems in a hierarchical Universe
  277. The effects of photoionization on galaxy formation - I. Model and results atz=0
  278. The effects of photoionization on galaxy formation - II. Satellite galaxies in the Local Group
  279. The 2dF Galaxy Redshift Survey: Constraints on Cosmic Star Formation History from the Cosmic Spectrum
  280. Hierarchical galaxy formation
  281. Evidence for a non-zero and a low matter density from a combined analysis of the 2dF Galaxy Redshift Survey and cosmic microwave background anisotropies
  282. A Million Element Integral Field Unit (MEIFU)
  283. The 2dF Galaxy Redshift Survey: a targeted study of catalogued clusters of galaxies
  284. Cluster correlations in redshift space
  285. The 2dF Galaxy Redshift Survey: the power spectrum and the matter content of the Universe
  286. The clustering evolution of the galaxy distribution
  287. The 2dF Galaxy Redshift Survey: luminosity dependence of galaxy clustering
  288. The 2dF galaxy redshift survey: near-infrared galaxy luminosity functions
  289. The impact of galaxy formation on the X-ray evolution of clusters
  290. The 2dF Galaxy Redshift Survey: the number and luminosity density of galaxies
  291. A measurement of the cosmological mass density from clustering in the 2dF Galaxy Redshift Survey
  292. A comparison of semi-analytic and smoothed particle hydrodynamics galaxy formation
  293. The Infrared Side of Galaxy Formation. I. The Local Universe in the Semianalytical Framework
  294. Higher order clustering in the Durham/UKST and Stromlo-APM Galaxy Redshift Surveys
  295. The dependence of velocity and clustering statistics on galaxy properties
  296. The evolution of disc galaxies
  297. The nature of galaxy bias and clustering
  298. The Durham/UKST Galaxy Redshift Survey -- VI. Power spectrum analysis of clustering
  299. Properties of galaxy clusters: mass and correlation functions
  300. Modelling the evolution of galaxy clustering
  301. The K-band Hubble diagram for the brightest cluster galaxies: a test of hierarchical galaxy formation models
  302. The Epoch of Galaxy Formation
  303. The seeds of rich galaxy clusters in the Universe
  304. Testing deprojection algorithms on mock angular catalogues: evidence for a break in the power spectrum
  305. Testing deprojection algorithms on mock angular catalogues: evidence for a break in the power spectrum
  306. Evolution of the Hubble sequence in hierarchical models for galaxy formation
  307. A wide-field K-band survey -- II. Galaxy clustering
  308. Large-scale fluctuations in the distribution of galaxies
  309. Faint galaxy counts as a function of morphological type in a hierarchical merger model
  310. Testing Ansatze for quasi-non-linear clustering: the linear APM power spectrum
  311. The real-space correlation function measured from the APM Galaxy Survey
  312. A comparison of the evolution of density fields in perturbation theory and numerical simulations - II. Counts-in-cells analysis
  313. Hierarchical correlations in models of galaxy clustering
  314. A comparison of the evolution of density fields in perturbation theory and numerical simulations - I. Non-linear evolution of the power spectrum
  315. The three-dimensional power spectrum measured from the APM Galaxy Survey - II. Use of the two-dimensional power spectrum
  316. The three-dimensional power spectrum measured from the APM Galaxy Survey - I. Use of the angular correlation function
  317. Self-avoiding random walks as a probe of large-scale structure in the Universe
  318. A New Numerical Inversion of Limber's Equation
  319. Correlation Function and Power Spectra in Cosmology
  320. Bringing light to a dark Universe
  321. Fare luce su un universo oscuro
  322. Universe: Simulations of Structure and Galaxy Formation
  323. Forming Globular Cluster Systems in a Semi-Analytic Scheme
  324. A Million Element Integral Field Unit (MEIFU)
  325. Measuring Large-Scale Structure with the 2dF Galaxy Redshift Survey
  326. The Evolution of Galaxy Mass in Hierarchical Models