A catalogue of galaxies in the HDF-South: Photometry and structural parameters
A European Southern Observatory Very Large Telescope Survey of Near-Infrared (Z <= 25) Selected Galaxies at Redshifts 4.5 < z < 6: Constraining the Cosmic Star Formation Rate near the Reionization Epoch
A K-band-Selected Photometric Redshift Catalog in the Hubble Deep Field South: Sampling the Rest-Frame V Band to z =3
A method to search for strong galaxy-galaxy lenses in optical imaging surveys
A Morphological Study of Gamma-Ray Burst Host Galaxies
A Multivariate Analysis of Galaxies in the Hubble Deep Field-North
Anglo-Australian Telescope Imaging and Microslit Spectroscopy in the Southern Hubble Deep Field
A NICMOS Search for High-Redshift Elliptical Galaxy Candidates
Assessing the galaxy population out to z ~ 2 using the Hubble Deep Field South
A Substantial Population of Red Galaxies at z > 2: Modeling of the Spectral Energy Distributions of an Extended Sample
A Survey for Ha emitting galaxies AT z ~= 2.2
A survey of unresolved objects in the Hubble Deep Field South
A VLT/FORS2 spectroscopic survey in the HDF-S
Bias in the estimation of global luminosity functions
Candidate high-redshift and primeval galaxies in Hubble Deep Field South
Cloning Dropouts: Implications for Galaxy Evolution at High Redshift
Clustering of galaxies at faint magnitudes
Constraints on the Cosmic Near-Infrared Background Excess from NICMOS Deep Field Observations
Constraints on z~10 Galaxies from the Deepest Hubble Space Telescope NICMOS Fields
Counts and Sizes of Galaxies in the Hubble Deep Field South: Implications for the Next Generation Space Telescope
Deep galaxy counts, extragalactic background light and the stellar baryon budget
Deep MUSE observations in the HDFS. Morpho-kinematics of distant star-forming galaxies down to 108M
Detectable signatures of cosmic radiative feedback
Detection of Evolved High-Redshift Galaxies in Deep NICMOS/VLT Impages
Evidence for a New Elliptical-Galaxy Paradigm: Sersic and Core Galaxies
Evidence for evolving spheroidals in the Hubble Deep Fields North and South
Evolution in the Colors of Lyman Break Galaxies from z~4 to z~3
Extended Lyman a haloes around individual high-redshift galaxies revealed by MUSE
Faint Blue Objects in the Hubble Deep Field-South Revealed: White Dwarfs, Subdwarfs, and Quasars
Faint Blue Objects on the Hubble Deep Field North and South as Possible Nearby Old Halo White Dwarfs
First gas-phase metallicity gradients of 0.1 z 0.8 galaxies with MUSE
FORS spectroscopy of galaxies in the Hubble Deep Field-South
Galaxy number counts - VI. An H-band survey of the Herschel Deep Field
High-Redshift Candidates and the Nature of Small Galaxies in the Hubble Deep Field
High-z massive galaxies in the Hubble Deep Field South
Ha emitting galaxies and the cosmic star formation rate at z =~ 2.2
Identification of absorbing galaxies towards the QSO J2233-606 in the Hubble Deep Field South
IMAGES. II. A surprisingly low fraction of undisturbed rotating spiral disks at z ~ 0.6 The morpho-kinematical relation 6 Gyr ago
IMAGES. III. The evolution of the near-infrared Tully-Fisher relation over the last 6 Gyr
Image simulation with shapelets
Infrared spectroscopy of faint 15 mu m sources in the Hubble Deep Field South: First hints at the properties of the sources of the IR background
Interpreting the optical data of the Hubble Deep Field South: colors, morphological number counts and photometric redshifts
Investigating the Metal Line Systems at Z=1.9 toward J2233-606 in the Hubble Deep Field South
Large Disklike Galaxies at High Redshift
Mass-dependent Color Evolution of Field Galaxies back to z~3 over the Wide Range of Stellar Mass
Measuring the redshift evolution of clustering: the Hubble Deep Field South
Multicolor Observations of the Hubble Deep Field South
MUSE deep-fields: the Ly a luminosity function in the Hubble Deep Field-South at 2.91 < z < 6.64
Near-Infrared Camera and Multi-Object Spectrometer Observations of the Hubble Deep Field: Observations, Data Reduction, and Galaxy Photometry
Nearly all the sky is covered by Lyman-a emission around high-redshift galaxies
NICMOS Imaging of DRGs in the HDF-S: A Relation between Star Formation and Size at z ~ 2.5
On the characteristics of tidal structures of interacting galaxies
Photometric Redshifts and Selection of High-Redshift Galaxies in the NTT and Hubble Deep Fields
Photometric redshifts in the Hubble Deep Fields: evolution of extinction and the star formation rate
Photometric redshifts with the Multilayer Perceptron Neural Network: Application to the HDF-S and SDSS
Pitch angles of distant spiral galaxies
Predictions for the Counts of Faint, High-Redshift Galaxies in the Mid-Infrared
Quantitative morphological analysis of the Hubble Deep Field North and Hubble Deep Field South - I. Early- and late-type luminosity-size relations of galaxies out to z~ 1
Radio Observations of the Hubble Deep Field-South Region. II. The 1.4 GHz Catalog and Source Counts
Radio Observations of the Hubble Deep Field-South Region. I. Survey Description and Initial Results
Radio Observations of the Hubble Deep Field-South Region. Iv. Optical Properties of the Faint Radio Population
Spectroscopy and stellar populations of star-forming galaxies at z ~ 3 in the Hubble Deep Field - South
Star Formation History in the NICMOS Northern Hubble Deep Field
Star Formation in the NICMOS HDF
Statistics of galaxy warps in the HDF North and South
Statistics of interacting galaxies at z ~ 0.7
Structure of visible and dark matter components in spiral galaxies at redshifts z = 0.5{-0.9}
Surface photometry and structure of high redshift disk galaxies in the HDF-S NICMOS field
The Assembly of Massive Galaxies from Near-Infrared Observations of the Hubble Deep Field-South
The B-Band Luminosity Function of Red and Blue Galaxies up to z = 3.5
The contribution of faint Lyman-a emitters to extended Lyman-a halos constrained by MUSE clustering measurements
The Evolution of the Galaxy Luminosity Function in the Rest-Frame Blue Band up to z=3.5
The Evolution of the Stellar Mass Function of Galaxies from z = 4.0 and the First Comprehensive Analysis of its Uncertainties: Evidence for Mass-Dependent Evolution
The faint radio sky: radio astronomy becomes mainstream
The first VLT FORS1 spectra of Lyman-break candidates in the HDF-S and AXAF Deep Field
The Hubble Deep Fields
The Hubble Deep Field South: Formulation of the Observing Campaign
The Hubble Deep Field South: STIS Imaging
The Large Binocular Camera Image Simulator
The Luminosity, Stellar Mass, and Number Density Evolution of Field Galaxies of Known Morphology from z = 0.5 to 3
The morphology of extremely red objects
The MUSE 3D view of the Hubble Deep Field South
The MUSE Hubble Ultra Deep Field Survey. XI. Constraining the low-mass end of the stellar mass - star formation rate relation at z < 1
The Relative Star Formation Histories of Spiral Bulges and Elliptical Galaxies in the Hubble Deep Fields
The Rest-Frame Optical Luminosity Density, Color, and Stellar Mass Density of the Universe from z = 0 to z = 3
The Size Evolution of Galaxies since z~3: Combining SDSS, GEMS, and FIRES
The Star Formation Rate Intensity Distribution Function: Implications for the Cosmic Star Formation Rate History of the Universe
Ultradeep Near-Infrared ISAAC Observations of the Hubble Deep Field South: Observations, Reduction, Multicolor Catalog, and Photometric Redshifts
Updating reionization scenarios after recent data
VLT and HST observations of a candidate high redshift elliptical galaxy in the Hubble Deep Field South
VLT narrow-band photometry in the Lyman continuum of two galaxies at z ~3. Limits to the escape of ionizing flux
WFPC2 Observations of the Hubble Deep Field South
What Do We Learn from IRAC Observations of Galaxies at 2 < z < 3.5?
Launched in 1990, the NASA/ESA Hubble Space Telescope remains the premier UV and visible light telescope in orbit. With well over 1.6 million observations from 10 different scientific instruments, the ESA Hubble Science Archive is a treasure trove of astronomical data to be exploited.
