ATNF instruments have been used to generate numerous catalogues and databases. A selection of the major ones appears below.

The ATNF Pulsar Catalogue is a comprehensive database of all published pulsars.

The Rapid ASKAP Continuum Survey (RACS) is an observatory led project to survey the sky in the ASKAP low, mid, and high bands. The first RACS-low epoch covered the whole southern sky and up to a declination of +41 degrees with a median field RMS of ~0.25 mJy/beam.

The ATCA Calibrator Database is kept up to date with multi-frequency ATCA flux density measurements of several hundred radio sources, providing information on their usefulness as phase calibrators for ATCA observations.

The HI Parkes All Sky Survey (HIPASS) used the 13-beam 21cm multibeam receiver, which provided a 64 MHz bandwidth, centred on 1394.5 MHz, and divided into 1024 channels, providing a velocity range of -1280 < cz < 12700 km/s with a channel width of approx. 13.2 km/s. The entire HIPASS survey detected over 5300 galaxies identified purely by their HI content.

The Parkes Galactic All Sky Survey (GASS) is a survey of the atomic hydrogen (HI) emission in the Milky Way for the entire sky south of a declination of +1°. GASS covered all Milky Way velocities between LSR -400 km/s and 500 km/s. The first data release of GASS provides spectra and velocity integrated maps with a 16 arcmin angular resolution, 0.82 km/s spectral resolution and an rms sensitivity of 57 mK.

The Australia Telescope 20 GHz (AT20G) Survey is a blind 20 GHz survey of the entire southern sky with |b|>1.5 degrees. Observations were made with the ATCA, with the final AT20G catalogue consisting of 5890 sources above a 20 GHz flux density limit of 40 mJy.

The Parkes-MIT-NRAO (PMN) Surveys were conducted in June and November 1990 and used a seven-beam receiver to survey the sky between declinations of -87° and +10° at a frequency of 4850 MHz.

ATPMN is a source catalogue of 9040 radio sources resulting from high-resolution observations of 8385 Parkes-MIT-NRAO (PMN) sources with the ATCA. The catalogue lists flux density and structural measurements at 4.8 and 8.6 GHz, derived from observations of all PMN sources in the declination range between -87° and -38.5 (with |b| > 2°) with 4.8 GHz flux densities typically greater than 70 mJy.

The LBA Calibrator Survey (LCS) provided accurate positions and correlated flux densities for 1100 compact extragalactic radio sources at declinations < -30° from VLBI observations with the Long Baseline Array at 8.3 GHz.

The Millimetre Astronomy Legacy Team 90 GHz (MALT90) survey mapped 16 emission lines simultaneously at frequencies near 90 GHz with the Mopra telescope. The target clumps were selected from the 870 micron APEX Telescope Large Area Survey of the Galaxy (ATLASGAL) to host the early stages of high-mass star formation and include pre-stellar clumps, protostellar clumps, and H II regions.

The Mopra Central Molecular Zone Survey was a multi-molecular line mapping survey of the Central Molecular Zone (CMZ) of the Galaxy. The CMZ extends approximately 3 degrees along the Galactic plane (l ~ 359° to +2°) and 0.3 degrees out of the plane. The CMZ was mapped across a broad range of frequencies in the 3 and 7-mm bands.

The Mopra Southern Galactic Plane CO Survey mapped the distribution and dynamics of the carbon monoxide molecule (CO) along a 35 degree sector of the Galactic Plane, from l=300—345°.

The H2O Southern Galactic Plane Survey (HOPS) mapped 100 square degrees of the Galactic plane from l = 290° through to l = 30° and b ± 0.5°, for water masers and thermal molecular line emission using the 22-m Mopra telescope.