Review of radio frequency interference and potential impacts on the CMB-S4 cosmic microwave background survey
Review of radio frequency interference and potential impacts on the CMB-S4 cosmic microwave background survey
复制标题
射频干扰及其对CMB-S4宇宙微波背景调查的潜在影响回顾
DOI：
10.1117/12.2629651
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发表时间：
2022
期刊：
影响因子：
--
通讯作者：
Whitehorn, Nathan
中科院分区：
文献类型：
--
作者：
Barron, Darcy;Bender, Amy N.;Birdwell, Ian;Carlstrom, John;Delabrouille, Jacques;Guns, Sam T.;Kovac, John M.;Lawrence, Charles R.;Paine, Scott N.;Whitehorn, Nathan
CMB-S4将以前所未有的精度绘制宇宙微波背景，同时测量毫米波时域天空，以促进我们对宇宙学和宇宙的理解。CMB-S4将在南极和智利的阿塔卡马沙漠两个地点进行观测。一个小口径和大口径望远镜与数十万个偏振敏感探测器的组合将在20-300 GHz的几个频段进行观测，以前所未有的灵敏度测量超过50%的天空。CMB-S4试图在灵敏度上取得巨大飞跃，同时在广泛的基本不受保护的频谱范围内进行观测，这些频谱越来越多地用于地面和卫星传输。CMB仪器技术的基本方面使它们容易受到各种频率的射频干扰，包括观测波段以外的频率。地面CMB仪器通过将超导测辐射热计的大焦平面部署到极其干燥的高海拔地点，实现其非凡的灵敏度，具有大的分数带宽，宽视场和多年的积分时间。历史上，合适的观测地点提供了对RFI的重要保护，自然是通过其极其偏远的位置以及对当地排放的限制。由于耦合机制很复杂，不干扰CMB测量的“安全”水平或发射频率并不总是通过简单的计算来确定。我们讨论了与CMB-S4相关的各种类型RFI的干扰模型、缓解策略以及对调查灵敏度的潜在影响。
CMB-S4 will map the cosmic microwave background to unprecedented precision, while simultaneously surveying the millimeter-wave time-domain sky, in order to advance our understanding of cosmology and the universe. CMB-S4 will observe from two sites, the South Pole and the Atacama Desert of Chile. A combination of small- and large-aperture telescopes with hundreds of thousands of polarization-sensitive detectors will observe in several frequency bands from 20–300 GHz, surveying more than 50% of the sky to arcminute resolution with unprecedented sensitivity. CMB-S4 seeks to make a dramatic leap in sensitivity while observing across a broad range of largely unprotected spectrum which is increasingly being utilized for terrestrial and satellite transmissions. Fundamental aspects of CMB instrument technology leave them vulnerable to radio frequency interference (RFI) across a wide range of frequencies, including frequencies outside of their observing bands. Ground-based CMB instruments achieve their extraordinary sensitivities by deploying large focal planes of superconducting bolometers to extremely dry, high-altitude sites, with large fractional bandwidths, wide fields of view, and years of integration time. Suitable observing sites have historically offered significant protection from RFI, both naturally through their extremely remote locations as well as through restrictions on local emissions. Since the coupling mechanisms are complex, “safe” levels or frequencies of emission that would not interfere with CMB measurements cannot always be determined through straightforward calculations. We discuss models of interference for various types of RFI relevant to CMB-S4, mitigation strategies, and the potential impacts on survey sensitivity.
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DOI：
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发表时间：
1985
期刊：
影响因子：
--
作者：
Solly Kimche
通讯作者：
Solly Kimche
用于高精度宇宙微波背景旋光测量的二头肌望远镜的表征
DOI：
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发表时间：
2009
期刊：
影响因子：
--
作者：
Y. Takahashi;P. Ade;D. Barkats;D. Barkats;J. Battle;E. Bierman;J. Bock;J. Bock;H. Chiang;H. Chiang;C. Dowell;L. Duband;E. Hivon;W. Holzapfel;V. Hristov;W. Jones;W. Jones;B. Keating;J. Kovac;C. Kuo;A. Lange;E. Leitch;P. Mason;T. Matsumura;H. Nguyen;N. Ponthieu;C. Pryke;S. Richter;G. Rocha;G. Rocha;K. W. Yoon
通讯作者：
K. W. Yoon
用于毫米/亚毫米望远镜的大面积反射式红外滤光片
DOI：
--
发表时间：
2014
期刊：
影响因子：
--
作者：
Z. Ahmed;J. Grayson;K. Thompson;C. Kuo;G. Brooks;T. Pothoven
通讯作者：
T. Pothoven
DOI：
10.2172/1872087
发表时间：
2022-03
期刊：
--
影响因子：
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作者：
K. Abazajian;Arwa Abdulghafour;G. Addison;Peter Adshead;Z. Ahmed;M. Ajello;D. Akerib;S. Allen;D. Alonso;M. Alvarez;M. Amin;M. Amiri;A. Anderson;B. Ansarinejad;M. Archipley;K. Arnold;M. Ashby;Han Aung;C. Baccigalupi;Carina Baker;Abhishek Bakshi;D. Bard;D. Barkats;D. Barron;P. Barry;J. Bartlett;P. Barton;R. Thakur;N. Battaglia;J. Beall;R. Bean;D. Beck;Sebastian Belkner;K. Benabed;A. Bender;B. Benson;B. Besuner;M. Béthermin;Sanah Bhimani;F. Bianchini;Simon Biquard;Ian Birdwell;C. Bischoff;L. Bleem;Paulina Bocaz;J. Bock;S. Bocquet;K. Boddy;J. Bond;J. Borrill;F. Bouchet;T. Brinckmann;Michael L. Brown;S. Bryan;V. Buza;K. Byrum;E. Calabrese;Victoria Calafut;R. Caldwell;J. Carlstrom;J. Carron;T. Cecil;A. Challinor;V. Chan;C. Chang;S. Chapman;Eric Charles;E. Chauvin;Cheng Cheng-Cheng;G. Chesmore;K. Cheung;Y. Chinone;J. Chluba;Hsiao-mei Cho.;Steve K. Choi;Justin Clancy;S. Clark;A. Cooray;G. Coppi;J. Corlett;W. Coulton;T. Crawford;A. Crites;A. Cukierman;F. Cyr-Racine;Weikai Dai;C. Daley;E. Dart;Gregorg Daues;T. Haan;C. Deaconu;J. Delabrouille;G. Derylo;M. Devlin;E. D. Valentino;M. Dierickx;B. Dober;R. Doriese;S. Duff;D. Dutcher;C. Dvorkin;R. Dunner;T. Eftekhari;J. Eimer;H. E. Bouhargani;T. Elleflot;N. Emerson;J. Errard;T. Essinger-Hileman;G. Fabbian;Valentina Fanfani;A. Fasano;C. Feng;S. Ferraro;J. Filippini;R. Flauger;B. Flaugher;A. Fraisse;J. Frisch;A. Frolov;N. Galitzki;P. Gallardo;Silvia Galli;K. Ganga;M. Gerbino;C. Giannakopoulos;M. Gilchriese;V. Gluscevic;N. Goeckner-wald;D. Goldfinger;Daniel Green;P. Grimes;D. Grin;E. Grohs;R. Gualtieri;Victor R. Guarino;J. Gudmundsson;I. Gullett;S. Guns;Salman Habib;G. Haller;M. Halpern;N. Halverson;S. Hanany;E. Hand;K. Harrington;M. Hasegawa;M. Hasselfield;M. Hazumi;K. Heitmann;Shawn W. Henderson;B. Hensley;R. Herbst;C. Hervías-Caimapo;J. C. Hill;R. Hills;E. Hivon;R. Hložek;Anna Ho;G. Holder;M. Hollister;W. Holzapfel;J. Hood;Selim C. Hotinli;A. Hryciuk;J. Hubmayr;K. Huffenberger;H. Hui;Roberto Ib'a nez;A. Ibitoye;M. Ikape;Kent Irwin;Cooper Jacobus;O. Jeong;Bradley R. Johnson;D. Johnstone;W. Jones;J. Joseph;B. Jost;Jae Hwan Kang;A. Kaplan;K. Karkare;N. Katayama;R. Keskitalo;Cesiley L. King;T. Kisner;M. Klein;L. Knox;B. Koopman;A. Kosowsky;J. Kovac;E. Kovetz;A. Krolewski;D. Kubik;S. Kuhlmann;C. Kuo;A. Kusaka;A. Lahteenmaki;K-H. Lau;C. Lawrence;Adrian T. Lee;L. Legrand;M. Leitner;C. Leloup;A. Lewis;Dale Li;E. Linder;I. Liodakis;Jia Liu;Kevin Long;T. Louis;M. Loverde;L. Lowry;C. Lu;P. Lubin;Yin-Zhe Ma;T. Maccarone;M. Madhavacheril;Felipe Maldonado;A. Mantz;G. Marques;F. Matsuda;P. Mauskopf;Jared M. May;H. McCarrick;Ken McCracken;J. McMahon;P. Meerburg;J. Melin;F. Menanteau;Joel Meyers;M. Millea;Vivian C. Miranda;D. Mitchell;Joseph Mohr;L. Moncelsi;M. Monzani;Magdy Moshed;T. Mroczkowski;Suvodip Mukherjee;M. Munchmeyer;D. Nagai;C. Nagarajappa;J. Nagy;T. Namikawa;F. Nati;T. Natoli;S. Nerval;L. Newburgh;H. Nguyen;Erikson Nichols;A. Nicola;M. Niemack;B. Nord;Tim Norton;V. Novosad;R. O’Brient;Y. Omori;Giorgio Orlando;B. Osherson;R. Osten;S. Padin;S. Paine;B. Partridge;S. Patil;D. Petravick;M. Petroff;E. Pierpaoli;Mauricio Pilleux;L. Pogosian;K. Prabhu;C. Pryke;G. Puglisi;B. Racine;S. Raghunathan;A. Rahlin;M. Raveri;B. Reese;C. Reichardt;M. Remazeilles;A. Rizzieri;Graça Rocha;N. Roe;K. Rotermund;A. Roy;J. Ruhl;J. Saba;Noah Sailer;M. Salatino;B. Saliwanchik;L. Sapozhnikov;M. S. Rao;L. Saunders;E. Schaan;A. Schillaci;B. Schmitt;D. Scott;N. Sehgal;S. Shandera;B. Sherwin;E. Shirokoff;C. Shiu;S. Simon;B. Singari;A. Slosar;D. Spergel;T. S. Germaine;S. Staggs;A. Stark;G. Starkman;B. Steinbach;R. Stompor;C. Stoughton;A. Suzuki;O. Tajima;C. Tandoi;G. Teply;G. Thayer;K. Thompson;B. Thorne;P. Timbie;M. Tomasi;C. Trendafilova;M. Tristram;C. Tucker;G. Tucker;C. Umilta;A. V. Engelen;J. V. Marrewijk;E. Vavagiakis;C. Vergés;J. Vieira;A. Vieregg;K. Wagoner;B. Wallisch;Gensheng Wang;Guo-Jian Wang;Scott D. Watson;D. Watts;Chris Weaver;L. Wenzl;B. Westbrook;M. White;N. Whitehorn;A. Wiedlea;Paul Williams;R. Wilson;H. Winch;Edward J. Wollack;W. L. K. Wu;Zhilei Xu;V. Yefremenko;Cyndia Yu;D. Zegeye;J. Zivick;A. Zonca
通讯作者：
K. Abazajian;Arwa Abdulghafour;G. Addison;Peter Adshead;Z. Ahmed;M. Ajello;D. Akerib;S. Allen;D. Alonso;M. Alvarez;M. Amin;M. Amiri;A. Anderson;B. Ansarinejad;M. Archipley;K. Arnold;M. Ashby;Han Aung;C. Baccigalupi;Carina Baker;Abhishek Bakshi;D. Bard;D. Barkats;D. Barron;P. Barry;J. Bartlett;P. Barton;R. Thakur;N. Battaglia;J. Beall;R. Bean;D. Beck;Sebastian Belkner;K. Benabed;A. Bender;B. Benson;B. Besuner;M. Béthermin;Sanah Bhimani;F. Bianchini;Simon Biquard;Ian Birdwell;C. Bischoff;L. Bleem;Paulina Bocaz;J. Bock;S. Bocquet;K. Boddy;J. Bond;J. Borrill;F. Bouchet;T. Brinckmann;Michael L. Brown;S. Bryan;V. Buza;K. Byrum;E. Calabrese;Victoria Calafut;R. Caldwell;J. Carlstrom;J. Carron;T. Cecil;A. Challinor;V. Chan;C. Chang;S. Chapman;Eric Charles;E. Chauvin;Cheng Cheng-Cheng;G. Chesmore;K. Cheung;Y. Chinone;J. Chluba;Hsiao-mei Cho.;Steve K. Choi;Justin Clancy;S. Clark;A. Cooray;G. Coppi;J. Corlett;W. Coulton;T. Crawford;A. Crites;A. Cukierman;F. Cyr-Racine;Weikai Dai;C. Daley;E. Dart;Gregorg Daues;T. Haan;C. Deaconu;J. Delabrouille;G. Derylo;M. Devlin;E. D. Valentino;M. Dierickx;B. Dober;R. Doriese;S. Duff;D. Dutcher;C. Dvorkin;R. Dunner;T. Eftekhari;J. Eimer;H. E. Bouhargani;T. Elleflot;N. Emerson;J. Errard;T. Essinger-Hileman;G. Fabbian;Valentina Fanfani;A. Fasano;C. Feng;S. Ferraro;J. Filippini;R. Flauger;B. Flaugher;A. Fraisse;J. Frisch;A. Frolov;N. Galitzki;P. Gallardo;Silvia Galli;K. Ganga;M. Gerbino;C. Giannakopoulos;M. Gilchriese;V. Gluscevic;N. Goeckner-wald;D. Goldfinger;Daniel Green;P. Grimes;D. Grin;E. Grohs;R. Gualtieri;Victor R. Guarino;J. Gudmundsson;I. Gullett;S. Guns;Salman Habib;G. Haller;M. Halpern;N. Halverson;S. Hanany;E. Hand;K. Harrington;M. Hasegawa;M. Hasselfield;M. Hazumi;K. Heitmann;Shawn W. Henderson;B. Hensley;R. Herbst;C. Hervías-Caimapo;J. C. Hill;R. Hills;E. Hivon;R. Hložek;Anna Ho;G. Holder;M. Hollister;W. Holzapfel;J. Hood;Selim C. Hotinli;A. Hryciuk;J. Hubmayr;K. Huffenberger;H. Hui;Roberto Ib'a nez;A. Ibitoye;M. Ikape;Kent Irwin;Cooper Jacobus;O. Jeong;Bradley R. Johnson;D. Johnstone;W. Jones;J. Joseph;B. Jost;Jae Hwan Kang;A. Kaplan;K. Karkare;N. Katayama;R. Keskitalo;Cesiley L. King;T. Kisner;M. Klein;L. Knox;B. Koopman;A. Kosowsky;J. Kovac;E. Kovetz;A. Krolewski;D. Kubik;S. Kuhlmann;C. Kuo;A. Kusaka;A. Lahteenmaki;K-H. Lau;C. Lawrence;Adrian T. Lee;L. Legrand;M. Leitner;C. Leloup;A. Lewis;Dale Li;E. Linder;I. Liodakis;Jia Liu;Kevin Long;T. Louis;M. Loverde;L. Lowry;C. Lu;P. Lubin;Yin-Zhe Ma;T. Maccarone;M. Madhavacheril;Felipe Maldonado;A. Mantz;G. Marques;F. Matsuda;P. Mauskopf;Jared M. May;H. McCarrick;Ken McCracken;J. McMahon;P. Meerburg;J. Melin;F. Menanteau;Joel Meyers;M. Millea;Vivian C. Miranda;D. Mitchell;Joseph Mohr;L. Moncelsi;M. Monzani;Magdy Moshed;T. Mroczkowski;Suvodip Mukherjee;M. Munchmeyer;D. Nagai;C. Nagarajappa;J. Nagy;T. Namikawa;F. Nati;T. Natoli;S. Nerval;L. Newburgh;H. Nguyen;Erikson Nichols;A. Nicola;M. Niemack;B. Nord;Tim Norton;V. Novosad;R. O’Brient;Y. Omori;Giorgio Orlando;B. Osherson;R. Osten;S. Padin;S. Paine;B. Partridge;S. Patil;D. Petravick;M. Petroff;E. Pierpaoli;Mauricio Pilleux;L. Pogosian;K. Prabhu;C. Pryke;G. Puglisi;B. Racine;S. Raghunathan;A. Rahlin;M. Raveri;B. Reese;C. Reichardt;M. Remazeilles;A. Rizzieri;Graça Rocha;N. Roe;K. Rotermund;A. Roy;J. Ruhl;J. Saba;Noah Sailer;M. Salatino;B. Saliwanchik;L. Sapozhnikov;M. S. Rao;L. Saunders;E. Schaan;A. Schillaci;B. Schmitt;D. Scott;N. Sehgal;S. Shandera;B. Sherwin;E. Shirokoff;C. Shiu;S. Simon;B. Singari;A. Slosar;D. Spergel;T. S. Germaine;S. Staggs;A. Stark;G. Starkman;B. Steinbach;R. Stompor;C. Stoughton;A. Suzuki;O. Tajima;C. Tandoi;G. Teply;G. Thayer;K. Thompson;B. Thorne;P. Timbie;M. Tomasi;C. Trendafilova;M. Tristram;C. Tucker;G. Tucker;C. Umilta;A. V. Engelen;J. V. Marrewijk;E. Vavagiakis;C. Vergés;J. Vieira;A. Vieregg;K. Wagoner;B. Wallisch;Gensheng Wang;Guo-Jian Wang;Scott D. Watson;D. Watts;Chris Weaver;L. Wenzl;B. Westbrook;M. White;N. Whitehorn;A. Wiedlea;Paul Williams;R. Wilson;H. Winch;Edward J. Wollack;W. L. K. Wu;Zhilei Xu;V. Yefremenko;Cyndia Yu;D. Zegeye;J. Zivick;A. Zonca
第二季安静观测：95 GHz 宇宙微波背景偏振功率谱的测量
DOI：
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发表时间：
2012
期刊：
影响因子：
--
作者：
Q. C. D. Araujo;C. Bischoff;A. Brizius;I. Buder;Y. Chinone;K. Cleary;R. N. Dumoulin;A. Kusaka;R. Monsalve;S. Naess;L. Newburgh;R. Reeves;I. Wehus;J. Zwart;L. Bronfman;R. Bustos;S. Church;C. Dickinson;H. Eriksen;T. Gaier;J. Gundersen;M. Hasegawa;M. Hazumi;K. Huffenberger;K. Ishidoshiro;M. Jones;P. Kangaslahti;D. Kapner;D. Kubik;C. Lawrence;M. Limon;J. McMahon;A. Miller;M. Nagai;H. Nguyen;G. Nixon;T. Pearson;L. Piccirillo;Simon J. E. Radford;A. Readhead;J. Richards;D. Samtleben;M. Seiffert;M. Shepherd;K. Smith;S. Staggs;O. Tajima;K. Thompson;K. Vanderlinde;R. Williamson
通讯作者：
R. Williamson