All Stories

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