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Line-Intensity Mapping: 2017 Status Report
Ely D. Kovetz,Marco P. Viero,Adam Lidz,Laura Newburgh,Mubdi Rahman,Eric R. Switzer,Marc Kamionkowski,J. E. Aguirre,Marcelo A. Alvarez,James J. Bock,J. Richard Bond,Goeffry Bower,C. Matt Bradford,Patrick C. Breysse,Philip Bull,Tzu-Ching Chang,Yun-Ting Cheng,Dongwoo Chung,Kieran Cleary,Asantha Corray,A. T. Crites,Rupert A. C. Croft,O. Doré,Michael Eastwood,Andrea Ferrara,José Fonseca,Daniel C. Jacobs,Garrett K. Keating,Guilaine Lagache,Gunjan Lakhlani,Adrian Liu,Kavilan Moodley,Norm Murray,Aurélie Pénin,Gergö Popping,Anthony R. Pullen,Dominik Reichers,Shun Saito,Ben Saliwanchik,Mario G. Santos,Rachel S. Somerville,G. Stacey,George Stein,Francesco Villaescusa-Navarro,Eli Visbal,Amanda Weltman,Laura Wolz,Micheal Zemcov +47 more
TLDR
In this paper, the authors report on the recent advances in theory, instrumentation and observation that were presented in these workshops and some of the opportunities and challenges that were identified looking forward.Abstract:
Following the first two annual intensity mapping workshops at Stanford in March 2016 and Johns Hopkins in June 2017, we report on the recent advances in theory, instrumentation and observation that were presented in these meetings and some of the opportunities and challenges that were identified looking forward. With preliminary detections of CO, [CII], Lya and low-redshift 21cm, and a host of experiments set to go online in the next few years, the field is rapidly progressing on all fronts, with great anticipation for a flood of new exciting results. This current snapshot provides an efficient reference for experts in related fields and a useful resource for nonspecialists. We begin by introducing the concept of line-intensity mapping and then discuss the broad array of science goals that will be enabled, ranging from the history of star formation, reionization and galaxy evolution to measuring baryon acoustic oscillations at high redshift and constraining theories of dark matter, modified gravity and dark energy. After reviewing the first detections reported to date, we survey the experimental landscape, presenting the parameters and capabilities of relevant instruments such as COMAP, mmIMe, AIM-CO, CCAT-p, TIME, CONCERTO, CHIME, HIRAX, HERA, STARFIRE, MeerKAT/SKA and SPHEREx. Finally, we describe recent theoretical advances: different approaches to modeling line luminosity functions, several techniques to separate the desired signal from foregrounds, statistical methods to analyze the data, and frameworks to generate realistic intensity map simulations.read more
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Semi-analytic forecasts for JWST - II. Physical properties and scaling relations for galaxies at z = 4-10
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Galaxy formation in the Planck Millennium : the atomic hydrogen content of dark matter haloes.
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User’s guide to extracting cosmological information from line-intensity maps
TL;DR: In this paper, a comprehensive framework for modeling the line-intensity mapping power spectrum, including redshift space distortions and the Alcock-Paczynski effect, is presented. But the power spectrum is not robust to cosmology and astrophysics at the same time.
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TL;DR: The third generation of the Sloan Digital Sky Survey (SDSS-III) took data from 2008 to 2014 using the original SDSS wide-field imager, the original and an upgraded multi-object fiber-fed optical spectrograph, a new near-infrared high-resolution spectrogram, and a novel optical interferometer.
Journal ArticleDOI
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Shadab Alam,Metin Ata,Stephen Bailey,Florian Beutler,Dmitry Bizyaev,Dmitry Bizyaev,Jonathan Blazek,Adam S. Bolton,Joel R. Brownstein,Angela Burden,Chia-Hsun Chuang,Chia-Hsun Chuang,Johan Comparat,Antonio J. Cuesta,Kyle S. Dawson,Daniel J. Eisenstein,Stephanie Escoffier,Héctor Gil-Marín,Héctor Gil-Marín,Jan Niklas Grieb,Nick Hand,Shirley Ho,Karen Kinemuchi,D. Kirkby,Francisco S. Kitaura,Francisco S. Kitaura,Francisco S. 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,Marcos Pellejero-Ibanez,Will J. Percival,Patrick Petitjean,Francisco Prada,Francisco Prada,Adrian M. Price-Whelan,Beth Reid,Beth Reid,Sergio Rodríguez-Torres,Sergio Rodríguez-Torres,Natalie A. Roe,Ashley J. Ross,Ashley J. Ross,Nicholas P. Ross,Graziano Rossi,Jose Alberto Rubino-Martin,Jose Alberto Rubino-Martin,Shun Saito,Salvador Salazar-Albornoz,Lado Samushia,Ariel G. Sánchez,Siddharth Satpathy,David J. Schlegel,Donald P. Schneider,Claudia G. Scóccola,Claudia G. Scóccola,Claudia G. Scóccola,Hee-Jong Seo,Erin Sheldon,Audrey Simmons,Anže Slosar,Michael A. Strauss,Molly E. C. Swanson,Daniel Thomas,Jeremy L. Tinker,Rita Tojeiro,Mariana Vargas Magaña,Mariana Vargas Magaña,Jose Alberto Vazquez,Licia Verde,David A. Wake,David A. Wake,Yuting Wang,Yuting Wang,David H. Weinberg,Martin White,Martin White,W. Michael Wood-Vasey,Christophe Yèche,Idit Zehavi,Zhongxu Zhai,Gong-Bo Zhao,Gong-Bo Zhao +90 more
TL;DR: In this article, the authors present cosmological results from the final galaxy clustering data set of the Baryon Oscillation Spectroscopic Survey, part of the Sloan Digital Sky Survey III.
Journal ArticleDOI
The Average Star Formation Histories of Galaxies in Dark Matter Halos from z = 0-8
TL;DR: In this article, a robust method to constrain average galaxy star formation rates, star formation histories (SFHs), and the intracluster light (ICL) as a function of halo mass is presented.
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