Anais da Academia Brasileira de Ciências (May 2021)

Baryon Acoustic Oscillations from Integrated Neutral Gas Observations: an instrument to observe the 21cm hydrogen line in the redshift range 0.13 < z < 0.45 – status update

  • CARLOS A. WUENSCHE,
  • ELCIO ABDALLA,
  • FILIPE ABDALLA,
  • LUCIANO BAROSI,
  • BIN WANG,
  • RUI AN,
  • JOÃO A. M. BARRETOS,
  • RICHARD BATTYE,
  • FRANCISCO A. BRITO,
  • IAN BROWNE,
  • DANIEL CORREIA,
  • ANDRÉ A. COSTA,
  • JACQUES DELABROUILLE,
  • CLIVE DICKINSON,
  • CHANG FENG,
  • ELISA G. M. FERREIRA,
  • KARIN FORNAZIER,
  • GIANCARLO DE GASPERIS,
  • PRISCILA GUTIERREZ,
  • STUART HARPER,
  • RICARDO G. LANDIM,
  • VINCENZO LICCARDO,
  • YIN-ZHE MA,
  • TELMO MACHADO,
  • BRUNO MAFFEI,
  • ALESSANDRO MARINS,
  • MILENA M. M. MENDES,
  • EDUARDO MERICIA,
  • CHRISTIAN MONSTEIN,
  • PABLO MOTTA,
  • CAMILA NOVAES,
  • CARLOS H. OTOBONE,
  • MICHAEL PEEL,
  • AMILCAR R. QUEIROZ,
  • CHRISTOPHER RADCLIFFE,
  • MATHIEU REMAZEILLES,
  • RAFAEL M. G. RIBEIRO,
  • YU SANG,
  • JULIANA F. R. SANTOS,
  • LARISSA SANTOS,
  • MARCELO. V. SANTOS,
  • CHENXI SHAN,
  • GUSTAVO B. SILVA,
  • FREDERICO VIEIRA,
  • JORDANY VIEIRA,
  • THYRSO VILLELA,
  • LINFENG XIAO,
  • WEIQIANG YANG,
  • JIAJUN ZHANG,
  • XUE ZHANG,
  • ZENGHAO ZHU

DOI
https://doi.org/10.1590/0001-3765202120201096
Journal volume & issue
Vol. 93, no. suppl 1

Abstract

Read online

Abstract BINGO (BAO from Integrated Neutral Gas Observations) is a unique radio telescope designed to map the intensity of neutral hydrogen distribution at cosmological distances, making the first detection of Baryon Acoustic Oscillations (BAO) in the frequency band 980 MHz - 1260 MHz, corresponding to a redshift range 0.127 < z < 0.449. BAO is one of the most powerful probes of cosmological parameters and BINGO was designed to detect the BAO signal to a level that makes it possible to put new constraints on the equation of state of dark energy. The telescope will be built in Paraíba, Brazil and consists of two \thicksim 40m mirrors, a feedhorn array of 50 horns, and no moving parts, working as a drift-scan instrument. It will cover a 15 ^{\circ} ∘ declination strip centered at \sim \delta ∼ δ =-15 ^{\circ} ∘, mapping \sim ∼ 5400 square degrees in the sky. The BINGO consortium is led by University of São Paulo with co-leadership at National Institute for Space Research and Campina Grande Federal University (Brazil). Telescope subsystems have already been fabricated and tested, and the dish and structure fabrication are expected to start in late 2020, as well as the road and terrain preparation.

Keywords