Welcome to the website for the BINGO telescope! This website is currently under construction.
The Baryon acoustic oscillations from Integrated Neutral Gas Observations (BINGO) experiment is a project to build a special purpose radio telescope to map redshifted neutral hydrogen emission between z = 0.13 and 0.48. It is an international project with collaborators in Brazil, Saudi Arabia, Switzerland, United Kingdom and Uruguay. It is the only radio telescope that aims at mapping neutral gas, as traced by the 21cm line, on large angular scales and at redshift z~0.3. We call this method HI intensity mapping.
Using the Baryon Acoustic Oscillations (BAOs) as a standard ruler allows us to measure the expansion of the universe as a function of redshift and so, to constrain the properties of dark energy. The telescope will have no moving parts and consist of a primary mirror of about 40 m diameter and a secondary a bit smaller. It will have around 50 “pixels” (detectors). With this design, the accuracy on the measurement on the acoustic scale will be ~2% for one year of integration time, by performing a drift scan survey of 15 deg x 200 deg. This will be achieved by employing a static 40m dual-dish radio telescope with a resolution of 40 arcmin at 1 GHz.
BINGO is also a pathfinder for using the SKA as an instrument for ultra-deep large-scale IM surveys, particularly for understanding systematic errors and the data analysis challenges for extracting such small cosmological signals.