English
Related papers

Related papers: High angular resolution SZ observations with NIKA …

200 papers

We report on the effects of cosmic ray interactions with the Kinetic Inductance Detector (KID) based focal plane array for the Terahertz Intensity Mapper (TIM). TIM is a NASA-funded balloon-borne experiment designed to probe the peak of the…

Kinetic inductance detectors (KID) have great potential in astronomical observation, such as searching for exoplanets, because of their low noise, fast response and photon counting characteristics. In this paper, we present the design…

Instrumentation and Methods for Astrophysics · Physics 2022-09-21 Shiling Yu , Shibo Shu , Ran Duan , Lihui Yang , Di Li

A two-dimensional resonant inelastic x-ray scattering (2D-RIXS) microscopy system has been developed at the beamline BL02U of NanoTerasu. The instrument combines a Wolter type-I mirror for spatial imaging with a varied-line-spacing grating…

Materials Science · Physics 2026-05-07 Kohei Yamamoto , Hakuto Suzuki , Jun Miyawaki

We present near-infrared (H band) surface photometry of 170 galaxies, obtained in 1997 using the Calar Alto 2.2m telescope equipped with the NICMOS3 camera MAGIC. The majority of our targets are selected among bright members of the Virgo…

Astrophysics · Physics 2009-10-31 A. Boselli , G. Gavazzi , P. Franzetti , D. Pierini , M. Scodeggio

Future generation of astronomical imaging spectrometers are targeting the far infrared wavelengths to close the THz astronomy gap. Similar to lens antenna coupled Microwave Kinetic Inductance Detectors (MKIDs), lens absorber coupled MKIDs…

Instrumentation and Methods for Astrophysics · Physics 2023-10-30 Shahab O. Dabironezare , Sven van Berkel , Pierre M. Echternach , Peter K. Day , Charles M. Bradford , Jochem J. A. Baselmans

Precise measurement of neutrino beam direction and intensity was achieved based on a new concept with modularized neutrino detectors. INGRID (Interactive Neutrino GRID) is an on-axis near detector for the T2K long baseline neutrino…

Instrumentation and Detectors · Physics 2015-06-03 K. Abe , N. Abgrall , Y. Ajima , H. Aihara , J. B. Albert , C. Andreopoulos , B. Andrieu , M. D. Anerella , S. Aoki , O. Araoka , J. Argyriades , A. Ariga , T. Ariga , S. Assylbekov , D. Autiero , A. Badertscher , M. Barbi , G. J. Barker , G. Barr , M. Bass , M. Batkiewicz , F. Bay , S. Bentham , V. Berardi , B. E. Berger , I. Bertram , M. Besnier , J. Beucher , D. Beznosko , S. Bhadra , F. d. M. Blaszczyk , J. Blocki , A. Blondel , C. Bojechko , J. Bouchez , S. B. Boyd , A. Bravar , C. Bronner , D. G. Brook-Roberge , N. Buchanan , H. Budd , D. Calvet , S. L. Cartwright , A. Carver , R. Castillo , M. G. Catanesi , A. Cazes , A. Cervera , C. Chavez , S. Choi , G. Christodoulou , J. Coleman , G. Collazuol , W. Coleman , K. Connolly , A. Curioni , A. Dabrowska , I. Danko , R. Das , G. S. Davies , S. Davis , M. Day , G. De Rosa , J. P. A. M. de André , P. de Perio , T. Dealtry , A. Delbart , C. Densham , F. Di Lodovico , S. Di Luise , P. Dinh Tran , J. Dobson , U. Dore , O. Drapier , F. Dufour , J. Dumarchez , S. Dytman , M. Dziewiecki , M. Dziomba , S. Emery , A. Ereditato , J. E. Escallier , L. Escudero , L. S. Esposito , M. Fechner , A. Ferrero , A. J. Finch , E. Frank , Y. Fujii , Y. Fukuda , V. Galymov , G. L. Ganetis , F. C. Gannaway , A. Gaudin , A. Gendotti , M. George , S. Giffin , C. Giganti , K. Gilje , A. K. Ghosh , T. Golan , M. Goldhaber , J. J. Gomez-Cadenas , S. Gomi , M. Gonin , N. Grant , A. Grant , P. Gumplinger , P. Guzowski , A. Haesler , M. D. Haigh , K. Hamano , C. Hansen , D. Hansen , T. Hara , P. F. Harrison , B. Hartfiel , M. Hartz , T. Haruyama , T. Hasegawa , N. C. Hastings , A. Hatzikoutelis , K. Hayashi , Y. Hayato , C. Hearty , R. L. Helmer , R. Henderson , N. Higashi , J. Hignight , A. Hillairet , E. Hirose , J. Holeczek , S. Horikawa , A. Hyndman , A. K. Ichikawa , K. Ieki , M. Ieva , M. Iida , M. Ikeda , J. Ilic , J. Imber , T. Ishida , C. Ishihara , T. Ishii , S. J. Ives , M. Iwasaki , K. Iyogi , A. Izmaylov , B. Jamieson , R. A. Johnson , K. K. Joo , G. V. Jover-Manas , C. K. Jung , H. Kaji , T. Kajita , H. Kakuno , J. Kameda , K. Kaneyuki , D. Karlen , K. Kasami , I. Kato , H. Kawamuko , E. Kearns , M. Khabibullin , F. Khanam , A. Khotjantsev , D. Kielczewska , T. Kikawa , J. Kim , J. Y. Kim , S. B. Kim , N. Kimura , B. Kirby , J. Kisiel , P. Kitching , T. Kobayashi , G. Kogan , S. Koike , A. Konaka , L. L. Kormos , A. Korzenev , K. Koseki , Y. Koshio , Y. Kouzuma , K. Kowalik , V. Kravtsov , I. Kreslo , W. Kropp , H. Kubo , J. Kubota , Y. Kudenko , N. Kulkarni , Y. Kurimoto , R. Kurjata , T. Kutter , J. Lagoda , K. Laihem , M. Laveder , K. P. Lee , P. T. Le , J. M. Levy , C. Licciardi , I. T. Lim , T. Lindner , R. P. Litchfield , M. Litos , A. Longhin , G. D. Lopez , P. F. Loverre , L. Ludovici , T. Lux , M. Macaire , K. Mahn , Y. Makida , M. Malek , S. Manly , A. Marchionni , A. D. Marino , A. J. Marone , J. Marteau , J. F. Martin , T. Maruyama , T. Maryon , J. Marzec , P. Masliah , E. L. Mathie , C. Matsumura , K. Matsuoka , V. Matveev , K. Mavrokoridis , E. Mazzucato , N. McCauley , K. S. McFarland , C. McGrew , T. McLachlan , M. Messina , W. Metcalf , C. Metelko , M. Mezzetto , P. Mijakowski , C. A. Miller , A. Minamino , O. Mineev , S. Mine , A. D. Missert , G. Mituka , M. Miura , K. Mizouchi , L. Monfregola , F. Moreau , B. Morgan , S. Moriyama , A. Muir , A. Murakami , J. F. Muratore , M. Murdoch , S. Murphy , J. Myslik , N. Nagai , T. Nakadaira , M. Nakahata , T. Nakai , K. Nakajima , T. Nakamoto , K. Nakamura , S. Nakayama , T. Nakaya , D. Naples , M. L. Navin , B. Nelson , T. C. Nicholls , C. Nielsen , K. Nishikawa , H. Nishino , K. Nitta , T. Nobuhara , J. A. Nowak , Y. Obayashi , T. Ogitsu , H. Ohhata , T. Okamura , K. Okumura , T. Okusawa , S. M. Oser , M. Otani , R. A. Owen , Y. Oyama , T. Ozaki , M. Y. Pac , V. Palladino , V. Paolone , P. Paul , D. Payne , G. F. Pearce , J. D. Perkin , V. Pettinacci , F. Pierre , E. Poplawska , B. Popov , M. Posiadala , J. -M. Poutissou , R. Poutissou , P. Przewlocki , W. Qian , J. L. Raaf , E. Radicioni , P. N. Ratoff , T. M. Raufer , M. Ravonel , M. Raymond , F. Retiere , A. Robert , P. A. Rodrigues , E. Rondio , J. M. Roney , B. Rossi , S. Roth , A. Rubbia , D. Ruterbories , S. Sabouri , R. Sacco , K. Sakashita , F. Sánchez , A. Sarrat , K. Sasaki , K. Scholberg , J. Schwehr , M. Scott , D. I. Scully , Y. Seiya , T. Sekiguchi , H. Sekiya , M. Shibata , Y. Shimizu , M. Shiozawa , S. Short , M. Siyad , R. J. Smith , M. Smy , J. T. Sobczyk , H. Sobel , M. Sorel , A. Stahl , P. Stamoulis , J. Steinmann , B. Still , J. Stone , M. Stodulski , C. Strabel , R. Sulej , A. Suzuki , K. Suzuki , S. Suzuki , S. Y. Suzuki , Y. Suzuki , Y. Suzuki , J. Swierblewski , T. Szeglowski , M. Szeptycka , R. Tacik , M. Tada , M. Taguchi , S. Takahashi , A. Takeda , Y. Takenaga , Y. Takeuchi , K. Tanaka , H. A. Tanaka , M. Tanaka , M. M. Tanaka , N. Tanimoto , K. Tashiro , I. Taylor , A. Terashima , D. Terhorst , R. Terri , L. F. Thompson , A. Thorley , W. Toki , S. Tobayama , T. Tomaru , Y. Totsuka , C. Touramanis , T. Tsukamoto , M. Tzanov , Y. Uchida , K. Ueno , A. Vacheret , M. Vagins , G. Vasseur , T. Wachala , J. J. Walding , A. V. Waldron , C. W. Walter , P. J. Wanderer , J. Wang , M. A. Ward , G. P. Ward , D. Wark , M. O. Wascko , A. Weber , R. Wendell , N. West , L. H. Whitehead , G. Wikström , R. J. Wilkes , M. J. Wilking , Z. Williamson , J. R. Wilson , R. J. Wilson , T. Wongjirad , S. Yamada , Y. Yamada , A. Yamamoto , K. Yamamoto , Y. Yamanoi , H. Yamaoka , T. Yamauchi , C. Yanagisawa , T. Yano , S. Yen , N. Yershov , M. Yokoyama , T. Yuan , A. Zalewska , J. Zalipska , L. Zambelli , K. Zaremba , M. Ziembicki , E. D. Zimmerman , M. Zito , J. Zmuda

If the gas in filaments and halos shares the same velocity field than the luminous matter, it will generate measurable temperature anisotropies due to the Kinematic Sunyaev-Zeldovich effect. We compute the distribution function of the KSZ…

Astrophysics · Physics 2009-11-13 F. Atrio-Barandela , J. P. Muecket , R. Genova-Santos

In the coming years, Sunyaev-Zel'dovich (SZ) measurements can dramatically improve our understanding of the Intergalactic Medium (IGM) and the role of feedback processes on galaxy formation, allowing us to calibrate important astrophysical…

We propose a new method to use the kinematic Sunyaev-Zeldovich for measuring the baryon fraction in cluster of galaxies. In this proposal we need a configuration in which a supernova Type Ia resides in a brightest cluster galaxy of…

Cosmology and Nongalactic Astrophysics · Physics 2019-02-12 Shant Baghram

We detect the kinematic Sunyaev-Zel'dovich (kSZ) effect with a statistical significance of $4.2 \sigma$ by combining a cluster catalogue derived from the first year data of the Dark Energy Survey (DES) with CMB temperature maps from the…

The KPNO International Spectroscopic Survey (KISS) is an objective-prism survey for extragalactic emission-line objects. It combines many of the features of previous slitless spectroscopic surveys with the advantages of modern CCD…

The intergalactic medium (IGM) plays an important role in the formation and evolution of galaxies. Recent developments in upcoming radio telescopes are starting to open up the possibility of making a first direct detection of the 21 cm…

Cosmology and Nongalactic Astrophysics · Physics 2019-10-09 Robin Kooistra , Marta B. Silva , Saleem Zaroubi , Marc A. W. Verheijen , Elmo Tempel , Kelley M. Hess

The Sunyaev-Zeldovich (SZ) effect is a promising tool for detecting the presence of hot gas out to the galaxy cluster peripheries. We developed a spectral imaging algorithm dedicated to the SZ observations of nearby galaxy clusters with…

Cosmology and Nongalactic Astrophysics · Physics 2016-01-26 H. Bourdin , P. Mazzotta , E. Rasia

We construct a pipeline for simulating weak lensing cosmology surveys with the Square Kilometre Array (SKA), taking as inputs telescope sensitivity curves; correlated source flux, size and redshift distributions; a simple ionospheric model;…

Cosmology and Nongalactic Astrophysics · Physics 2016-10-26 Anna Bonaldi , Ian Harrison , Stefano Camera , Michael L. Brown

The Cosmology Large Angular Scale Surveyor (CLASS) is a polarization-sensitive telescope array located at an altitude of 5,200 m in the Chilean Atacama Desert and designed to measure the polarized Cosmic Microwave Background (CMB) over…

We report on the development of scalable prototype microwave kinetic inductance detector (MKID) arrays tailored for future multi-kilo-pixel experiments that are designed to simultaneously characterize the polarization properties of both the…

We present a stacked lensing analysis of 96 galaxy clusters selected by the thermal Sunyaev-Zel'dovich (SZ) effect in maps of the cosmic microwave background (CMB). We select foreground galaxy clusters with a $5\sigma$-level SZ threshold in…

Dusty starless cores play an important role in regulating the initial phases of the formation of stars and planets. In their interiors, dust grains coagulate and ice mantles form, thereby changing the millimeter emissivities and hence the…

CONCERTO is a millimeter-wave imaging instrument that operated on the Atacama Pathfinder Experiment (APEX) telescope from April 2021 to May 2023. Its primary scientific objectives include the study of galaxy clusters through the…

Signal Processing · Electrical Eng. & Systems 2026-04-29 Mounir Abdkrimi , Olivier Rossetto , O. Bourrion , Christophe Vescovi , C. Hoarau