Related papers: Baryon acoustic oscillations signature in the thre…

Detecting Baryon Acoustic Oscillations in Dark Matter from Kinematic Weak Lensing Surveys

We investigate the feasibility of extracting Baryon Acoustic Oscillations (BAO) from cosmic shear tomography. We particularly focus on the BAO scale precision that can be achieved by future spectroscopy-based, kinematic weak lensing (KWL)…

Cosmology and Nongalactic Astrophysics · Physics 2019-05-15 Zhejie Ding , Hee-Jong Seo , Eric Huff , Shun Saito , Douglas Clowe

The Low Redshift survey at Calar Alto (LoRCA)

The Baryon Acoustic Oscillation (BAO) feature in the power spectrum of galaxies provides a standard ruler to measure the accelerated expansion of the Universe. To extract all available information about dark energy, it is necessary to…

Cosmology and Nongalactic Astrophysics · Physics 2016-02-17 J. Comparat , C. -H. Chuang , S. Rodriguez-Torres , M. Pellejero-Ibanez , F. Prada , G. Yepes , H. M. Courtois , G. -B. Zhao , Y. Wang , J. Sanchez , C. Maraston , R. Benton Metcalf , J. Peiro-Perez , F. S. Kitaura , E. Perez , R. M. Gonzalez Delgado

Dark Energy Constraints from Baryon Acoustic Oscillations

Baryon acoustic oscillations (BAO) in the galaxy power spectrum allows us to extract the scale of the comoving sound horizon at recombination, a cosmological standard ruler accurately determined by the cosmic microwave background anisotropy…

Astrophysics · Physics 2008-11-26 Yun Wang

Cosmological constraints from baryon acoustic oscillations and clustering of large-scale structure

We constrain cosmological parameters using combined measurements of the baryon acoustic oscillation (BAO) feature in the correlation function of galaxies and Ly-\alpha absorbers that together cover 0.1 < z < 2.4. The BAO position…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-15 Graeme E. Addison , Gary Hinshaw , Mark Halpern

The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: measurement of the BAO and growth rate of structure of the luminous red galaxy sample from the anisotropic power spectrum between redshifts 0.6 and 1.0

We analyse the clustering of the Sloan Digital Sky Survey IV extended Baryon Oscillation Spectroscopic Survey Data Release 16 luminous red galaxy sample (DR16 eBOSS LRG) in combination with the high redshift tail of the Sloan Digital Sky…

Cosmology and Nongalactic Astrophysics · Physics 2020-12-22 Héctor Gil-Marín , Julián E. Bautista , Romain Paviot , Mariana Vargas-Magaña , Sylvain de la Torre , Sebastien Fromenteau , Shadab Alam , Santiago Ávila , Etienne Burtin , Chia-Hsun Chuang , Kyle S. Dawson , Jiamin Hou , Arnaud de Mattia , Faizan G. Mohammad , Eva-Maria Müller , Seshadri Nadathur , Richard Neveux , Will J. Percival , Anand Raichoor , Mehdi Rezaie , Ashley J. Ross , Graziano Rossi , Vanina Ruhlmann-Kleider , Alex Smith , Amélie Tamone , Jeremy L. Tinker , Rita Tojeiro , Yuting Wang , Gong-Bo Zhao , Cheng Zhao , Jonathan Brinkmann , Joel R. Brownstein , Peter D. Choi , Stephanie Escoffier , Axel de la Macorra , Jeongin Moon , Jeffrey A. Newman , Donald P. Schneider , Hee-Jong Seo , Mariappan Vivek

Probing large-scale structure with large samples of X-ray selected AGN: I Baryonic acoustic oscillations

We investigate the potential of large X-ray-selected AGN samples for detecting baryonic acoustic oscillations (BAO). Though AGN selection in X-ray band is very clean and efficient, it does not provide redshift information, and thus needs to…

Cosmology and Nongalactic Astrophysics · Physics 2018-05-07 Gert Hütsi , Marat Gilfanov , Alexander Kolodzig , Rashid Sunyaev

Baryon Acoustic Oscillation Theory and Modelling Systematics for the DESI 2024 results

This paper provides a comprehensive overview of how fitting of Baryon Acoustic Oscillations (BAO) is carried out within the upcoming Dark Energy Spectroscopic Instrument's (DESI) 2024 results using its DR1 dataset, and the associated…

Cosmology and Nongalactic Astrophysics · Physics 2025-04-14 Shi-Fan Chen , Cullan Howlett , Martin White , Patrick McDonald , Ashley J. Ross , Hee-Jong Seo , Nikhil Padmanabhan , J. Aguilar , S. Ahlen , S. Alam , O. Alves , U. Andrade , R. Blum , D. Brooks , X. Chen , S. Cole , T. M. Davis , K. Dawson , A. de la Macorra , Arjun Dey , Z. Ding , P. Doel , S. Ferraro , A. Font-Ribera , D. Forero-Sánchez , J. E. Forero-Romero , C. Garcia-Quintero , E. Gaztañaga , S. Gontcho A Gontcho , M. M. S Hanif , K. Honscheid , T. Kisner , A. Kremin , A. Lambert , M. Landriau , M. E. Levi , M. Manera , A. Meisner , J. Mena-Fernández , R. Miquel , A. Muñoz-Gutiérrez , E. Paillas , N. Palanque-Delabrouille , W. J. Percival , F. Prada , A. Pérez-Fernández , M. Rashkovetskyi , M. Rezaie , A. Rosado-Marin , G. Rossi , R. Ruggeri , E. Sanchez , D. Schlegel , J. Silber , G. Tarlé , M. Vargas-Magaña , B. A. Weaver , J. Yu , S. Yuan , R. Zhou , Z. Zhou

Euclid preparation. BAO analysis of photometric galaxy clustering in configuration space

With about 1.5 billion galaxies expected to be observed, the very large number of objects in the Euclid photometric survey will allow for precise studies of galaxy clustering from a single survey, over a large range of redshifts $0.2 < z <…

Cosmology and Nongalactic Astrophysics · Physics 2025-03-18 Euclid Collaboration , V. Duret , S. Escoffier , W. Gillard , I. Tutusaus , S. Camera , N. Tessore , F. J. Castander , N. Aghanim , A. Amara , L. Amendola , S. Andreon , N. Auricchio , C. Baccigalupi , M. Baldi , S. Bardelli , P. Battaglia , A. Biviano , D. Bonino , E. Branchini , M. Brescia , J. Brinchmann , A. Caillat , G. Cañas-Herrera , V. Capobianco , C. Carbone , V. F. Cardone , J. Carretero , S. Casas , M. Castellano , G. Castignani , S. Cavuoti , K. C. Chambers , A. Cimatti , C. Colodro-Conde , G. Congedo , C. J. Conselice , L. Conversi , Y. Copin , F. Courbin , H. M. Courtois , M. Cropper , A. Da Silva , H. Degaudenzi , S. de la Torre , G. De Lucia , A. M. Di Giorgio , H. Dole , F. Dubath , X. Dupac , S. Dusini , A. Ealet , M. Farina , R. Farinelli , S. Farrens , F. Faustini , S. Ferriol , F. Finelli , S. Fotopoulou , N. Fourmanoit , M. Frailis , E. Franceschi , M. Fumana , S. Galeotta , B. Gillis , C. Giocoli , J. Gracia-Carpio , A. Grazian , F. Grupp , S. V. H. Haugan , W. Holmes , F. Hormuth , A. Hornstrup , P. Hudelot , K. Jahnke , M. Jhabvala , B. Joachimi , E. Keihänen , S. Kermiche , A. Kiessling , M. Kilbinger , B. Kubik , M. Kunz , H. Kurki-Suonio , O. Lahav , A. M. C. Le Brun , S. Ligori , P. B. Lilje , V. Lindholm , I. Lloro , G. Mainetti , D. Maino , E. Maiorano , O. Mansutti , S. Marcin , O. Marggraf , K. Markovic , M. Martinelli , N. Martinet , F. Marulli , R. Massey , S. Maurogordato , E. Medinaceli , S. Mei , M. Melchior , Y. Mellier , M. Meneghetti , E. Merlin , G. Meylan , A. Mora , M. Moresco , B. Morin , L. Moscardini , E. Munari , R. Nakajima , C. Neissner , R. C. Nichol , S. -M. Niemi , C. Padilla , S. Paltani , F. Pasian , K. Pedersen , W. J. Percival , V. Pettorino , S. Pires , G. Polenta , M. Poncet , L. A. Popa , L. Pozzetti , F. Raison , R. Rebolo , J. Rhodes , G. Riccio , E. Romelli , M. Roncarelli , R. Saglia , Z. Sakr , D. Sapone , B. Sartoris , J. A. Schewtschenko , P. Schneider , T. Schrabback , A. Secroun , E. Sefusatti , G. Seidel , S. Serrano , P. Simon , C. Sirignano , G. Sirri , A. Spurio Mancini , L. Stanco , J. -L. Starck , J. Steinwagner , P. Tallada-Crespí , D. Tavagnacco , A. N. Taylor , I. Tereno , S. Toft , R. Toledo-Moreo , F. Torradeflot , J. Valiviita , T. Vassallo , G. Verdoes Kleijn , A. Veropalumbo , Y. Wang , J. Weller , G. Zamorani , F. M. Zerbi , E. Zucca , M. Bolzonella , C. Burigana , M. Calabrese , D. Di Ferdinando , J. A. Escartin Vigo , L. Gabarra , S. Matthew , N. Mauri , A. Pezzotta , M. Pöntinen , C. Porciani , V. Scottez , M. Tenti , M. Viel , M. Wiesmann , Y. Akrami , V. Allevato , I. T. Andika , M. Archidiacono , F. Atrio-Barandela , A. Balaguera-Antolinez , M. Ballardini , D. Bertacca , M. Bethermin , A. Blanchard , L. Blot , H. Böhringer , S. Borgani , M. L. Brown , S. Bruton , R. Cabanac , A. Calabro , B. Camacho Quevedo , A. Cappi , F. Caro , C. S. Carvalho , T. Castro , F. Cogato , S. Contarini , T. Contini , A. R. Cooray , S. Davini , F. De Paolis , G. Desprez , A. Díaz-Sánchez , S. Di Domizio , J. M. Diego , A. G. Ferrari , P. G. Ferreira , A. Finoguenov , K. Ganga , J. García-Bellido , T. Gasparetto , E. Gaztanaga , F. Giacomini , F. Gianotti , G. Gozaliasl , A. Gregorio , M. Guidi , C. M. Gutierrez , A. Hall , S. Hemmati , H. Hildebrandt , J. Hjorth , J. J. E. Kajava , Y. Kang , V. Kansal , D. Karagiannis , C. C. Kirkpatrick , S. Kruk , M. Lattanzi , M. Lembo , G. Leroy , J. Lesgourgues , T. I. Liaudat , S. J. Liu , A. Loureiro , G. Maggio , M. Magliocchetti , F. Mannucci , R. Maoli , J. Martín-Fleitas , C. J. A. P. Martins , L. Maurin , R. B. Metcalf , M. Miluzio , P. Monaco , C. Moretti , C. Murray , S. Nadathur , K. Naidoo , A. Navarro-Alsina , S. Nesseris , K. Paterson , A. Pisani , D. Potter , I. Risso , P. -F. Rocci , M. Sahlén , E. Sarpa , A. Schneider , D. Sciotti , E. Sellentin , M. Sereno , A. Silvestri , L. C. Smith , K. Tanidis , C. Tao , G. Testera , R. Teyssier , S. Tosi , A. Troja , M. Tucci , C. Valieri , A. Venhola , D. Vergani , F. Vernizzi , G. Verza , P. Vielzeuf , N. A. Walton

DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations

We present cosmological results from the measurement of baryon acoustic oscillations (BAO) in galaxy, quasar and Lyman-$\alpha$ forest tracers from the first year of observations from the Dark Energy Spectroscopic Instrument (DESI), to be…

Cosmology and Nongalactic Astrophysics · Physics 2025-04-14 DESI Collaboration , A. G. Adame , J. Aguilar , S. Ahlen , S. Alam , D. M. Alexander , M. Alvarez , O. Alves , A. Anand , U. Andrade , E. Armengaud , S. Avila , A. Aviles , H. Awan , B. Bahr-Kalus , S. Bailey , C. Baltay , A. Bault , J. Behera , S. BenZvi , A. Bera , F. Beutler , D. Bianchi , C. Blake , R. Blum , S. Brieden , A. Brodzeller , D. Brooks , E. Buckley-Geer , E. Burtin , R. Calderon , R. Canning , A. Carnero Rosell , R. Cereskaite , J. L. Cervantes-Cota , S. Chabanier , E. Chaussidon , J. Chaves-Montero , S. Chen , X. Chen , T. Claybaugh , S. Cole , A. Cuceu , T. M. Davis , K. Dawson , A. de la Macorra , A. de Mattia , N. Deiosso , A. Dey , B. Dey , Z. Ding , P. Doel , J. Edelstein , S. Eftekharzadeh , D. J. Eisenstein , A. Elliott , P. Fagrelius , K. Fanning , S. Ferraro , J. Ereza , N. Findlay , B. Flaugher , A. Font-Ribera , D. Forero-Sánchez , J. E. Forero-Romero , C. S. Frenk , C. Garcia-Quintero , E. Gaztañaga , H. Gil-Marín , S. Gontcho A Gontcho , A. X. Gonzalez-Morales , V. Gonzalez-Perez , C. Gordon , D. Green , D. Gruen , R. Gsponer , G. Gutierrez , J. Guy , B. Hadzhiyska , C. Hahn , M. M. S Hanif , H. K. Herrera-Alcantar , K. Honscheid , C. Howlett , D. Huterer , V. Iršič , M. Ishak , S. Juneau , N. G. Karaçaylı , R. Kehoe , S. Kent , D. Kirkby , A. Kremin , A. Krolewski , Y. Lai , T. -W. Lan , M. Landriau , D. Lang , J. Lasker , J. M. Le Goff , L. Le Guillou , A. Leauthaud , M. E. Levi , T. S. Li , E. Linder , K. Lodha , C. Magneville , M. Manera , D. Margala , P. Martini , M. Maus , P. McDonald , L. Medina-Varela , A. Meisner , J. Mena-Fernández , R. Miquel , J. Moon , S. Moore , J. Moustakas , N. Mudur , E. Mueller , A. Muñoz-Gutiérrez , A. D. Myers , S. Nadathur , L. Napolitano , R. Neveux , J. A. Newman , N. M. Nguyen , J. Nie , G. Niz , H. E. Noriega , N. Padmanabhan , E. Paillas , N. Palanque-Delabrouille , J. Pan , S. Penmetsa , W. J. Percival , M. M. Pieri , M. Pinon , C. Poppett , A. Porredon , F. Prada , A. Pérez-Fernández , I. Pérez-Ràfols , D. Rabinowitz , A. Raichoor , C. Ramírez-Pérez , S. Ramirez-Solano , C. Ravoux , M. Rashkovetskyi , M. Rezaie , J. Rich , A. Rocher , C. Rockosi , N. A. Roe , A. Rosado-Marin , A. J. Ross , G. Rossi , R. Ruggeri , V. Ruhlmann-Kleider , L. Samushia , E. Sanchez , C. Saulder , E. F. Schlafly , D. Schlegel , M. Schubnell , H. Seo , A. Shafieloo , R. Sharples , J. Silber , A. Slosar , A. Smith , D. Sprayberry , T. Tan , G. Tarlé , P. Taylor , S. Trusov , L. A. Ureña-López , R. Vaisakh , D. Valcin , F. Valdes , M. Vargas-Magaña , L. Verde , M. Walther , B. Wang , M. S. Wang , B. A. Weaver , N. Weaverdyck , R. H. Wechsler , D. H. Weinberg , M. White , J. Yu , Y. Yu , S. Yuan , C. Yèche , E. A. Zaborowski , P. Zarrouk , H. Zhang , C. Zhao , R. Zhao , R. Zhou , T. Zhuang , H. Zou

The oscillating behavior of the pair correlation function in galaxies

The pair correlation function (PCF) for galaxies presents typical oscillations in the range 20-200 Mpc/h which are named baryon acoustic oscillation (BAO). We first review and test the oscillations of the PCF when the 2D/3D vertexes of the…

Cosmology and Nongalactic Astrophysics · Physics 2014-01-29 L. Zaninetti

Coherent Combination of Baryon Acoustic Oscillation Statistics and Peculiar Velocity Measurements from Redshift Survey

New statistical method is proposed to coherently combine Baryon Acoustic Oscillation statistics (BAO) and peculiar velocity measurements exploiting decomposed density-density and velocity-velocity spectra in real space from the observed…

Cosmology and Nongalactic Astrophysics · Physics 2011-06-07 Yong-Seon Song

The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample

We present cosmological results from the final galaxy clustering data set of the Baryon Oscillation Spectroscopic Survey, part of the Sloan Digital Sky Survey III. Our combined galaxy sample comprises 1.2 million massive galaxies over an…

Cosmology and Nongalactic Astrophysics · Physics 2017-07-26 Shadab Alam , Metin Ata , Stephen Bailey , Florian Beutler , Dmitry Bizyaev , Jonathan A. Blazek , Adam S. Bolton , Joel R. Brownstein , Angela Burden , Chia-Hsun Chuang , Johan Comparat , Antonio J. Cuesta , Kyle S. Dawson , Daniel J. Eisenstein , Stephanie Escoffier , Héctor Gil-Marín , Jan Niklas Grieb , Nick Hand , Shirley Ho , Karen Kinemuchi , David Kirkby , Francisco Kitaura , Elena Malanushenko , Viktor Malanushenko , Claudia Maraston , Cameron K. McBride , Robert C. Nichol , Matthew D. Olmstead , Daniel Oravetz , Nikhil Padmanabhan , Nathalie Palanque-Delabrouille , Kaike Pan , Marcos Pellejero-Ibanez , Will J. Percival , Patrick Petitjean , Francisco Prada , Adrian M. Price-Whelan , Beth A. Reid , Sergio A. Rodríguez-Torres , Natalie A. Roe , Ashley J. Ross , Nicholas P. Ross , Graziano Rossi , Jose Alberto Rubiño-Martín , Ariel G. Sánchez , Shun Saito , Salvador Salazar-Albornoz , Lado Samushia , Siddharth Satpathy , Claudia G. Scóccola , David J. Schlegel , Donald P. Schneider , Hee-Jong Seo , Audrey Simmons , Anže Slosar , Michael A. Strauss , Molly E. C. Swanson , Daniel Thomas , Jeremy L. Tinker , Rita Tojeiro , Mariana Vargas Magaña , Jose Alberto Vazquez , Licia Verde , David A. Wake , Yuting Wang , David H. Weinberg , Martin White , W. Michael Wood-Vasey , Christophe Yèche , Idit Zehavi , Zhongxu Zhai , Gong-Bo Zhao

Combining galaxy and 21cm surveys

Acoustic waves traveling through the early Universe imprint a characteristic scale in the clustering of galaxies, QSOs and inter-galactic gas. This scale can be used as a standard ruler to map the expansion history of the Universe, a…

Cosmology and Nongalactic Astrophysics · Physics 2016-02-17 J. D. Cohn , Martin White , Tzu-Ching Chang , Gil Holder , Nikhil Padmanabhan , Olivier Doré

Signatures of the Primordial Universe from Its Emptiness: Measurement of Baryon Acoustic Oscillations from Minima of the Density Field

Sound waves from the primordial fluctuations of the Universe imprinted in the large-scale structure, called baryon acoustic oscillations (BAOs), can be used as standard rulers to measure the scale of the Universe. These oscillations have…

Cosmology and Nongalactic Astrophysics · Physics 2016-05-04 Francisco-Shu Kitaura , Chia-Hsun Chuang , Yu Liang , Cheng Zhao , Charling Tao , Sergio Rodriguez-Torres , Daniel J. Eisenstein , Hector Gil-Marin , Jean-Paul Kneib , Cameron McBride , Will Percival , Ashley J. Ross , Ariel G. Sanchez , Jeremy Tinker , Rita Tojeiro , Mariana Vargas-Magana , Gong-Bo Zhao

Theoretical Systematics of Future Baryon Acoustic Oscillation Surveys

Future Baryon Acoustic Oscillation surveys aim at observing galaxy clustering over a wide range of redshift and galaxy populations at great precision, reaching tenths of a percent, in order to detect any deviation of dark energy from the…

Cosmology and Nongalactic Astrophysics · Physics 2018-05-31 Zhejie Ding , Hee-Jong Seo , Zvonimir Vlah , Yu Feng , Marcel Schmittfull , Florian Beutler

The Acoustic Peak in the Lyman Alpha Forest

We present the first simulation of the signature of baryonic acoustic oscillations (BAO) in Lyman alpha forest data containing 180,000 mock quasar sight-lines. We use eight large dark-matter only simulations onto which we paint the Lyman…

Cosmology and Nongalactic Astrophysics · Physics 2009-11-09 Anže Slosar , Shirley Ho , Martin White , Thibaut Louis

Phenomenology of BAO evolution from Lagrangian to Eulerian Space

The baryon acoustic oscillation (BAO) feature provides an important distance scale for the measurement of the expansion history of the Universe. Theoretical models of the BAO in the distribution of biased tracers of the large scale…

Cosmology and Nongalactic Astrophysics · Physics 2017-03-01 Tobias Baldauf , Vincent Desjacques

Optimising Baryon Acoustic Oscillation Surveys - I: Testing the concordance LCDM cosmology

We optimize the design of future spectroscopic redshift surveys for constraining the dark energy via precision measurements of the baryon acoustic oscillations (BAO), with particular emphasis on the design of the Wide-Field Multi-Object…

Astrophysics · Physics 2008-11-26 David Parkinson , Chris Blake , Martin Kunz , Bruce A. Bassett , Robert C. Nichol , Karl Glazebrook

The BAO scale -- how standard is the standard ruler?

Analyses of baryon acoustic oscillations (BAO) commonly employ template-based methods to extract compressed parameters from the clustering of dark-matter tracers, which are then interpreted in terms of ratios of the sound-horizon scale and…

Cosmology and Nongalactic Astrophysics · Physics 2026-03-20 Francisco Asensio-Rivera , Nils Schöneberg , Héctor Gil-Marín , Licia Verde

The Ups and Downs of Baryon Oscillations

Baryon acoustic oscillations, measured through the patterned distribution of galaxies or other baryon tracing objects on very large (100 Mpc) scales, offer a possible geometric probe of cosmological distances. Pluses and minuses in this…

Astrophysics · Physics 2007-05-23 Eric V. Linder