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(Reference retrieved automatically from Web of Science through information on FAPESP grant and its corresponding number as mentioned in the publication by the authors.)

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

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Author(s):
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Wuensche, Carlos A. [1] ; Abdalla, Elcio [2] ; Abdalla, Filipe [3, 4] ; Barosi, Luciano [5] ; Wang, Bin [6, 7] ; An, Rui [7] ; Barretos, Joao A. M. [2] ; Battye, Richard [8] ; Brito, Francisco A. [5] ; Browne, Ian [8] ; Correia, Daniel [2] ; Costa, Andre A. [6] ; Delabrouille, Jacques [9, 10] ; Dickinson, Clive [8] ; Feng, Chang [11] ; Ferreira, Elisa G. M. [12] ; Fornazier, Karin [2, 3] ; De Gasperis, Giancarlo [13, 14] ; Gutierrez, Priscila [2] ; Harper, Stuart [8] ; Landim, Ricardo G. [15] ; Liccardo, Vincenzo [1, 8] ; Ma, Yin-Zhe [16, 17] ; Machado, Telmo [1] ; Maffei, Bruno [18] ; Marins, Alessandro [2] ; Mendes, Milena M. M. [2] ; Mericia, Eduardo [1] ; Monstein, Christian [19] ; Motta, Pablo [2] ; Novaes, Camila [1] ; Otobone, Carlos H. [2] ; Peel, Michael [20, 21] ; Queiroz, Amilcar R. [5] ; Radcliffe, Christopher [22] ; Remazeilles, Mathieu [8] ; Ribeiro, Rafael M. G. [2] ; Sang, Y. U. [6] ; Santos, Juliana F. R. [2] ; Santos, Larissa [6] ; Santos, V, Marcelo ; Shan, Chenxi [6] ; Silva, Gustavo B. [2] ; Vieira, Frederico [1] ; Vieira, Jordany [2] ; Villela, Thyrso [1, 23] ; Xiao, Linfeng [7] ; Yang, Weiqiang [24] ; Zhang, Jiajun [25] ; Zhang, Xue [6] ; Zhu, Zenghao [26]
Total Authors: 51
Affiliation:
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[1] Inst Nacl Pesquisas Espaciais, Div Astrofis, Av Astronautas 1758, BR-12227010 Sao Jose Dos Campos, SP - Brazil
[2] Univ Sao Paulo, Inst Fis, R Matao 1371, BR-05508090 Sao Paulo, SP - Brazil
[3] Univ Fed Campina Grande, Unidade Acad Fis, BR-58429900 Campina Grande, Paraiba - Brazil
[4] UCL, Gower St, London WC1E 6BT - England
[5] V, Rhodes Univ, Dept Phys & Elect, POB 94, ZA-6140 Grahamstown - South Africa
[6] Yangzhou Univ, Coll Phys Sci & Technol, Ctr Gravitat & Cosmol, Yangzhou 225009, Jiangsu - Peoples R China
[7] Shanghai Jiao Tong Univ, Sch Aeronaut & Astronaut, Shanghai 200240 - Peoples R China
[8] Univ Manchester, Jodrell Bank Ctr Astrophys, Dept Phys & Astron, Oxford Rd, Manchester M13 9PL, Lancs - England
[9] Univ Paris Saclay, CEA, IRFU, F-91191 Gif Sur Yvette - France
[10] Univ Paris Diderot, Lab Astroparticule & Cosmol APC, CNRS, IN2P3, F-75205 Paris 13 - France
[11] Univ Sci & Technol China, Sch Astron & Space Sci, Hefei 230026 - Peoples R China
[12] Max Planck Inst Astrophys, Karl Schwarzschild Str 1, D-85748 Garching - Germany
[13] Univ Roma Tor Vergata, Dipartimento Fis, Via Ric Sci 1, I-00133 Rome - Italy
[14] Ist Nazl Fis Nucl, Sez Roma 2, Via Ric Sci 1, I-00133 Rome - Italy
[15] Tech Universit Munchen, Phys Dept, James Franck Str 1, D-85748 Garching - Germany
[16] Univ KwaZulu Natal, Sch Chem & Phys, Westville Campus, Private Bag X54001, ZA-4000 Durban - South Africa
[17] Univ KwaZulu Natal, NAOC UKZN Computat Astrophys Ctr NUCAC, ZA-4000 Durban - South Africa
[18] Univ Paris Saclay, IAS, F-91405 Orsay - France
[19] Swiss Fed Inst Technol, Inst Particle Phys & Astrophys, HIT J13-2, Wolfgang Pauli Str 27, CH-8093 Zurich - Switzerland
[20] Inst Astrofis Canarias, Tenerife 38200, Canary Islands - Spain
[21] Univ La Laguna ULL, Dept Astrofis, San Cristobal la Laguna 38206 - Spain
[22] Phase2 Microwave Ltd, Unit 1a, Boutton Rd, Stevenage SG1 4QX, Herts - England
[23] Univ Brasilia, ICC Ctr, Inst Fis, Direcao IF, Entrada BT 297 Terreo, BR-70919970 Brasilia, DF - Brazil
[24] Liao Ning Normal Univ, 850 Huanghe Rd Shahekou Dist, Prchina 116029, Liaoning - Peoples R China
[25] CTPU IBS, Theory Bldg, 4th Floor, 55 Expo Ro, Daejeon - South Korea
[26] Shanghai Jiao Tong Univ, Sch Phys & Astron, Shanghai 200240 - Peoples R China
Total Affiliations: 26
Document type: Journal article
Source: Anais da Academia Brasileira de Ciências; v. 93, n. 1 2021.
Web of Science Citations: 0
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 Paraiba, Brazil and consists of two similar to 40m mirrors, a feedhorn array of 50 horns, and no moving parts, working as a drift-scan instrument. It will cover a 15 degrees declination strip centered at similar to delta = -15 degrees, mapping similar to 5400 square degrees in the sky. The BINGO consortium is Led by University of Sao 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. (AU)

FAPESP's process: 14/07885-0 - The BINGO telescope: a new 21 cm window for exploring the dark universe and other astrophysics
Grantee:Elcio Abdalla
Support type: Research Projects - Thematic Grants
FAPESP's process: 15/19936-1 - BINGO: an ultra-sensitive survey of hydrogen and radio continuum emission to measure the dark universe
Grantee:Michael William Peel
Support type: Research Grants - Young Investigators Grants
FAPESP's process: 19/05687-0 - The BINGO telescope 21 cm measurements: Baryon Acoustic Oscillations and Non-gaussianities
Grantee:Carlos Alexandre Wuensche de Souza
Support type: Research Grants - Visiting Researcher Grant - International