@Article{WuenscheAABWABBBBCCDDFFFGGHLLMMMMMMMMNOPQRRRSSSSSSVVTXYZZZ:2021:InOb21,
author = "Wuensche, Carlos Alexandre and Abdalla, Elcio and Abdalla, Filipe
and Barosi, Luciano and Wang, Bin and An, Rui and Barretos,
Jo{\~a}o A. M. and Battye, Richard and Brito, Francisco A. and
Browne, Ian and Correia, Daniel and Costa, Andr{\'e} A. and
Delabrouille, Jacques and Dickinson, Clive and Feng, Chang and
Ferreira, Elisa G. M. and Fornazier, Karin and Gasperis, Giancarlo
de and Gutierrez, Priscila and Harper, Stuart and Landim, Ricardo
G. and Liccardo, Vincenzo and Ma, Yin-Zhe and Machado, Telmo and
Maffei, Bruno and Marins, Alessandro and Mendes, Milena M. M. and
Mericia, Eduardo Jubini and Monstein, Christian and Motta, Pablo
and Novaes, Camila Paiva and Otobone, Carlos H. and Peel, Michael
and Queiroz, Amilcar R. and Radcliffe, Christopher and Remazeille,
Mathieu and Ribeiro, Rafael M. G. and Sang, Yu and Santos, Juliana
F. R. and Santos, Larissa and Santos, Marcelo V. and Shan, Chenxi
and Silva, Gustavo B. and Vieira, Frederico Augusto Silva and
Vieira, Jordany and Thyrso, Villela and Xiao, Linfeng and Yang,
Weiqiang and Zhang, Jiajun and Zhang, Xue and Zhu, Zenghao",
affiliation = "{Instituto Nacional de Pesquisas Espaciais (INPE)} and
{Universidade de S{\~a}o Paulo (USP)} and {Universidade Federal
de Campina Grande (UFGC)} and {Rhodes University} and {Yangzhou
University} and {Shanghai Jiao Tong UniversitY} and {Universidade
de S{\~a}o Paulo (USP)} and {The University of Manchester} and
{Rhodes University} and {The University of Manchester} and
{Universidade de S{\~a}o Paulo (USP)} and {Yangzhou University}
and {Universit{\'e} Paris Diderot} and {The University of
Manchester} and {University of Science and Technology of China}
and {Max-Planck-Institut fr Astrophysik} and {Universidade de
S{\~a}o Paulo (USP)} and {Universit{\`a} degli Studi di Roma Tor
Vergata} and {Universidade de S{\~a}o Paulo (USP)} and {The
University of Manchester} and {Technische Universit{\"a}t
M{\"u}nchen} and {Instituto Nacional de Pesquisas Espaciais
(INPE)} and {University of KwaZulu-Natal} and {Instituto Nacional
de Pesquisas Espaciais (INPE)} and {Universit{\'e} Paris-Saclay}
and {Universidade de S{\~a}o Paulo (USP)} and {Universidade de
S{\~a}o Paulo (USP)} and {Instituto Nacional de Pesquisas
Espaciais (INPE)} and {ETH Z{\"u}rich} and {Universidade de
S{\~a}o Paulo (USP)} and {Instituto Nacional de Pesquisas
Espaciais (INPE)} and {Universidade de S{\~a}o Paulo (USP)} and
{Phase2 Microwave Ltd} and {Rhodes University} and {Phase2
Microwave Ltd} and {The University of Manchester} and
{Universidade de S{\~a}o Paulo (USP)} and {Yangzhou University}
and {Universidade de S{\~a}o Paulo (USP)} and {Yangzhou
University} and {Rhodes University} and {Yangzhou University} and
{Universidade de S{\~a}o Paulo (USP)} and {Instituto Nacional de
Pesquisas Espaciais (INPE)} and {Universidade de S{\~a}o Paulo
(USP)} and {Instituto Nacional de Pesquisas Espaciais (INPE)} and
{Shanghai Jiao Tong University} and {Liao Ning Normal University}
and CTPU-IBS and {Yangzhou University} and {Shanghai Jiao Tong
University}",
title = "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",
journal = "Anais da Academia Brasileira de Ci{\^e}ncias",
year = "2021",
volume = "93",
number = "Suppl. 1",
pages = "19",
keywords = "21cm cosmology, radio astronomy, baryon acoustic oscillations,
BAO.",
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
Para{\'{\i}}ba, Brazil and consists of two \∼ 40m
mirrors, a feedhorn array of 50 horns, and no moving parts,
working as a drift-scan instrument. It will cover a 15\◦
declination strip centered at \∼ \δ = 15\◦,
mapping \∼ 5400 square degrees in the sky. The BINGO
consortium is led by University of S{\~a}o 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.",
doi = "10.1590/0001-3765202120201096",
url = "http://dx.doi.org/10.1590/0001-3765202120201096",
issn = "0001-3765",
label = "self-archiving-INPE-MCTIC-GOV-BR",
language = "en",
targetfile = "j8MgcCW6YxhjPjBrCKVcRhx.pdf",
urlaccessdate = "08 maio 2024"
}