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Spectra from surveys hosted by Data Central. Most spectra were taken with the multi-object spectroscopy facilities 2dF (Anglo-Australian Telescope) and 6dF (UK Schmidt Telescope).

High frequency water maser and HI spectra are available through this web service. The water maser phenomena are found in active galactic nuclei (AGN) and have been surveyed with...

CANDELS is designed to document the first third of galactic evolution from z = 8 to 1.5 via deep imaging of more than 250,000 galaxies with WFC3/IR and ACS. It will also find...

By observing 25 massive galaxy clusters with HST's new panchromatic imaging capabilities (Wide-field Camera 3, WFC3, and the Advanced Camera for Surveys, ACS), CLASH will...

Hubble Infrared Pure Parallel Imaging Extragalactic Survey (HIPPIES) utilizes long-duration pure parallel visits (~> 3 orbits) of HST at high Galactic latitude...

The results of the analysis of 205 brightest sources (S>15mJy), which were found in the sky survey at the declination of the pulsar in the Crab Nebula, are presented. The...

The Spitzer Survey of Stellar Structure in Galaxies (S4G) together with its Early Type Galaxy (ETG) extension stands as the mostextensive dataset of deep, uniform mid-infrared...

The Calar Alto Void Integral-field Treasury surveY (CAVITY) is a legacy project aimed at characterising the population of galaxies inhabiting voids, which are the most...

We present cosmological parameter constraints from a tomographic weak gravitational lensing analysis of ~450deg^2^ of imaging data from the Kilo Degree Survey (KiDS). For a flat...

We present the final data release of the Kilo-Degree Survey (KiDS-DR5), a public European Southern Observatory (ESO) wide-field imaging survey optimised for weak gravitational...

The increasingly neutral intergalactic gas at z>6 impacts the Lyman-{alpha} (Ly{alpha}) flux observed from galaxies. One luminous galaxy, COLA1, stands out because of its...

We quantify the stellar rotation of galaxies by computing the {lambda}R parameter, a proxy for the stellar angular momentum in a sample of 106 intermediate-redshift galaxies...

We present the First Cosmic Gamma-ray Horizon (1CGH) catalogue, featuring gamma-ray detections above 10GeV based on 16 years of observations with the Fermi Large Area Telescope...

The identification of AGN and SB regions in galaxies is crucial for understanding the role of various physical processes in galaxy evolution. Molecular line ratios, such as the...

This paper presents a search for high redshift galaxies from the Euclid Early Release Observations program `Magnifying Lens.' The 1.5deg2 area covered by the twin Abell lensing...

The Euclid Early Release Observations (ERO) programme targeted the Perseus cluster of galaxies, gathering deep data in the central region of the cluster over 0.7deg^2^,...

The second data release of the LOFAR Two-Metre Sky Survey (LoTSS) covers 27% of the northern sky, with a total area of ~5700deg^2^. The high angular resolution of LOFAR with...

Galaxy properties are known to correlate most tightly with the galaxy effective stellar velocity dispersion {sigma}e. Here, we look for additional trends at fixed {sigma}e using...

Bars inhabit the majority of local-Universe disc galaxies and may be important drivers of galaxy evolution through the redistribution of gas and angular momentum within discs....