Performance of the polarization leakage correction in the PILOT data
Performance of the polarization leakage correction in the PILOT data
复制标题
PILOT 数据中偏振泄漏校正的性能
DOI：
10.1007/s10686-022-09882-5
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发表时间：
2023
影响因子：
3
通讯作者：
Bernard J
中科院分区：
文献类型：
--
作者：
Bernard J
用于长波长观测稀薄星际介质的偏振仪器(Pilot)是一项气球载实验，旨在测量240微米(1.2太赫兹)波长的热尘埃的偏振发射。PILOT实验于2015年和2019年从加拿大安大略省蒂明斯起飞，2017年4月从澳大利亚爱丽丝斯普林斯起飞。该仪器在第二次飞行期间的飞行性能在中进行了描述。在这篇文章中，我们介绍了没有给出的数据处理步骤，以及我们最近实施的数据处理步骤，以校正几个剩余的仪器效应。额外的数据处理涉及与探测器串扰和读出电路记忆效应相关的校正，以及从总强度到极化的泄漏。我们使用PILOT第三次飞行期间获得的数据说明了上述影响和我们的校正性能，但用于评估这些影响对最终科学就绪数据的影响的方法和我们的校正策略将适用于所有PILOT数据。我们表明，上述修正，特别是对于用PILOT进行精确偏振测量最关键的偏振泄漏强度的修正，其准确度在3号飞行期间在木星上测量到的精度优于0.4%。
The Polarized Instrument for Long-wavelength Observation of the Tenuous interstellar medium (PILOT) is a balloon-borne experiment that aims to measure the polarized emission of thermal dust at a wavelength of 240µm (1.2 THz). ThePILOTexperiment flew from Timmins, Ontario, Canada in 2015 and 2019 and from Alice Springs, Australia in April 2017. The in-flight performance of the instrument during the second flight was described in . In this paper, we present data processing steps that were not presented in and that we have recently implemented to correct for several remaining instrumental effects. The additional data processing concerns corrections related to detector cross-talk and readout circuit memory effects, and leakage from total intensity to polarization. We illustrate the above effects and the performance of our corrections using data obtained during the third flight ofPILOT, but the methods used to assess the impact of these effects on the final science-ready data, and our strategies for correcting them will be applied to allPILOTdata. We show that the above corrections, and in particular that for the intensity to polarization leakage, which is most critical for accurate polarization measurements withPILOT, are accurate to better than 0.4% as measured on Jupiter during flight#3.
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影响因子：
6.5
作者：
A. Mangilli;J. Aumont;J. Bernard;A. Buzzelli;G. Gasperis;J. Durrive;K. Ferrière;G. Foënard;A. Hughes;A. Lacourt;R. Misawa;L. Montier;B. Mot;I. Ristorcelli;H. Roussel;P. Ade;D. Alina;P. Bernardis;E. Pino;Jean-Pierre Dubois;C. Engel;V. Guillet;P. Hargrave;R. Laureijs;Y. Longval;B. Maffei;A. M. Magalhes;C. Marty;S. Masi;J. Montel;F. Pajot;E. Perot;L. Rodriguez;M. Salatino;M. Saccoccio;G. Savini;S. Stever;J. Tauber;C. Tibbs;C. Tucker
通讯作者：
A. Mangilli;J. Aumont;J. Bernard;A. Buzzelli;G. Gasperis;J. Durrive;K. Ferrière;G. Foënard;A. Hughes;A. Lacourt;R. Misawa;L. Montier;B. Mot;I. Ristorcelli;H. Roussel;P. Ade;D. Alina;P. Bernardis;E. Pino;Jean-Pierre Dubois;C. Engel;V. Guillet;P. Hargrave;R. Laureijs;Y. Longval;B. Maffei;A. M. Magalhes;C. Marty;S. Masi;J. Montel;F. Pajot;E. Perot;L. Rodriguez;M. Salatino;M. Saccoccio;G. Savini;S. Stever;J. Tauber;C. Tibbs;C. Tucker
HAWC ，SOFIA 远红外相机和旋光仪
影响因子：
1.3
作者：
D. Harper;M. Runyan;C. Dowell;C. Wirth;M. Amato;T. Ames;M. Amiri;S. Banks;A. Bartels;D. Benford;M. Berthoud;E. Buchanan;S. Casey;N. Chapman;D. Chuss;B. Cook;R. Derro;J. Dotson;R. Evans;D. Fixsen;I. Gatley;J. A. Guerra;M. Halpern;R. Hamilton;L. Hamlin;C. Hansen;S. Heimsath;Alfonso Hermida;G. Hilton;R. Hirsch;M. Hollister;Carl F. Hostetter;K. Irwin;C. Jhabvala;M. Jhabvala;J. Kastner;A. Kovács;Sean Lin;R. Loewenstein;L. Looney;E. Lopez;S. Maher;J. Michail;T. Miller;S. Moseley;G. Novak;R. Pernic;T. Rennick;H. Rhody;E. Sandberg;Dale Sandford;F. Santos;R. Shafer;E. Sharp;P. Shirron;J. Siah;R. Silverberg;L. Sparr;Robert Spotz;J. Staguhn;Armen S. Toorian;Shannon Towey;J. Tuttle;J. Vaillancourt;G. Voellmer;C. Volpert;Shu I. Wang;Edward J. Wollack
通讯作者：
Edward J. Wollack
DOI：
--
发表时间：
2014
期刊：
影响因子：
--
作者：
P. Ade;N. Aghanim;D. Alina;G. Aniano;C. Armitage;M. Arnaud;M. Ashdown;F. Atrio;J. Aumont;C. Baccigalupi;A. Banday;R. B. Barreiro;E. Battaner;C. Beichman;K. Benabed;S. Colombi;L. Colombo;C. Combet;F. Couchot;A. Coulais;B. Crill;A. Curto;F. Cuttaia;L. Danese;R. Davies;R. Davis;P. Bernardis;A. Rosa;G. Zotti;J. Delabrouille;C. Dickinson;J. Diego;S. Donzelli;M. Douspis;J. Dunkley;X. Dupac;H. Eriksen;E. Falgarone;L. Fanciullo;F. Finelli;O. Forni;M. Frailis;A. Fraisse;E. Franceschi;S. Galeotta;K. Ganga;T. Ghosh;M. Giard;J. Gonz;A. Gregorio;A. Gruppuso;V. Guillet;F. Hansen;D. Harrison;G. Helou;C. Hern;S. Hildebrandt;E. Hivon;M. Hobson;W. Holmes;A. Hornstrup;W. Jones;M. Juvela;R. Keskitalo;T. Kisner;R. Kneissl;J. Knoche;M. Kunz;H. Kurki;G. Lagache;A. Lasenby;R. Leonardi;F. Levrier;M. Liguori;P. Lilje;M. Linden;A. Magalh;D. Maino;N. Mandolesi;M. Maris;D. Marshall;P. Martin;S. Masi;S. Matarrese;P. Mazzotta;A. Melchiorri;L. Mendes;A. Mennella;M. Migliaccio;A. Moneti;L. Montier;G. Morgante;D. Mortlock;D. Munshi;J. Murphy;P. Naselsky;F. Nati;P. Natoli;C. Netterfield;F. Noviello;D. Novikov;I. Novikov;C. A. Oxborrow;L. Pagano;F. Pajot;R. Paladini;D. Paoletti;F. Pasian;O. Perdereau;L. Perotto;F. Perrotta;F. Piacentini;M. Piat;D. Pietrobon;S. Plaszczynski;F. Poidevin;E. Pointecouteau;G. Polenta;L. Popa;G. Pratt;S. Prunet;L. Puget;R. Rebolo;M. Reinecke;M. Remazeilles;C. Renault;S. Ricciardi;T. Riller;I. Ristorcelli;G. Rocha;C. Rosset;G. Roudier;B. Rusholme;M. Sandri;G. Savini;L. Spencer;V. Stolyarov;R. Stompor;R. Sudiwala;D. Sutton;J. Tauber;L. Terenzi;M. Tomasi;M. Tristram;M. Tucci;G. Umana;L. Valenziano;Jussi Väliviita;B. Tent;P. Vielva;F. Villa;L. Wade;B. Wandelt;A. Zonca
通讯作者：
A. Zonca
1800 颗恒星的偏振观测
DOI：
--
发表时间：
1971
期刊：
影响因子：
--
作者：
D. Mathewson;V. Ford
通讯作者：
V. Ford
Herschel-SPIRE 上飞行模型机载校准源的性能
DOI：
--
发表时间：
2006
期刊：
SPIE Astronomical Telescopes + Instrumentation
影响因子：
--
作者：
P. Hargrave;T. Waskett;T. Lim;B. Swinyard
通讯作者：
B. Swinyard