High resolution SZ observations at the IRAM 30-m telescope with NIKA

R. Adam; A. Adane; P. Ade; P. André; A. Beelen; B. Belier; A. Benoît; A. Bideaud; N. Billot; N. Boudou; O. Bourrion; M. Calvo; A. Catalano; G. Coiffard; B. Comis; A. D'Addabbo; F. X. Désert; S. Doyle; J. Goupy; C. Kramer; S. Leclercq; J. F. Macías-Pérez; J. Martino; P. Mauskopf; F. Mayet; A. Monfardini; F. Pajot; E. Pascale; L. Perotto; E. Pointecouteau; N. Ponthieu; V. Revéret; L. Rodriguez; F. Ruppin; G. Savini; K. Schuster; A. Sievers; C. Tucker; R. Zylka

High resolution SZ observations at the IRAM 30-m telescope with NIKA

R. Adam, A. Adane, P. Ade, P. André, A. Beelen, B. Belier, A. Benoît, A. Bideaud, N. Billot, N. Boudou, O. Bourrion, M. Calvo, A. Catalano, G. Coiffard, B. Comis, A. D'Addabbo, F. X. Désert, S. Doyle, J. Goupy, C. KramerS. Leclercq, J. F. Macías-Pérez, J. Martino, P. Mauskopf, F. Mayet, A. Monfardini, F. Pajot, E. Pascale, L. Perotto, E. Pointecouteau, N. Ponthieu, V. Revéret, L. Rodriguez, F. Ruppin, G. Savini, K. Schuster, A. Sievers, C. Tucker, R. Zylka

Earth and Space Exploration, School of (SESE)

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

Abstract

High resolution observations of the thermal Sunyaev-Zel'dovich (tSZ) effect are necessary to allow the use of clusters of galaxies as a probe for large scale structures at high redshifts. With its high resolution and dual-band capability at millimeter wavelengths, the NIKA camera can play a significant role in this context. NIKA is based on newly developed Kinetic Inductance Detectors (KIDs) and operates at the IRAM 30m telescope, Pico Veleta, Spain. In this paper, we give the status of the NIKA camera, focussing on the KID technology. We then present observations of three galaxy clusters: RX J1347.5-1145 as a demonstrator of the NIKA capabilities and the recent observations of CL J1226.9+3332 (z = 0.89) and MACS J0717.5+3745 (z = 0.55). We also discuss prospects for the final NIKA2 camera, which will have a 6.5 arcminute field of view with about 5000 detectors in two bands at 150 and 260 GHz.

Original language	English (US)
Title of host publication	Proceedings of the 49th Rencontres de Moriond on Cosmology 2014
Editors	Etienne Auge, Jacques Dumarchez, Jean Tran Thanh Van
Publisher	ARISF
Pages	73-76
Number of pages	4
ISBN (Electronic)	9782954640051
State	Published - 2014
Event	49th Rencontres de Moriond on Cosmology 2014 - La Thuile, Italy Duration: Mar 22 2014 → Mar 29 2014

Publication series

Name	Proceedings of the 49th Rencontres de Moriond on Cosmology 2014

Conference

Conference	49th Rencontres de Moriond on Cosmology 2014
Country/Territory	Italy
City	La Thuile
Period	3/22/14 → 3/29/14

ASJC Scopus subject areas

Astronomy and Astrophysics

Cite this

Adam, R., Adane, A., Ade, P., André, P., Beelen, A., Belier, B., Benoît, A., Bideaud, A., Billot, N., Boudou, N., Bourrion, O., Calvo, M., Catalano, A., Coiffard, G., Comis, B., D'Addabbo, A., Désert, F. X., Doyle, S., Goupy, J., ... Zylka, R. (2014). High resolution SZ observations at the IRAM 30-m telescope with NIKA. In E. Auge, J. Dumarchez, & J. Tran Thanh Van (Eds.), Proceedings of the 49th Rencontres de Moriond on Cosmology 2014 (pp. 73-76). (Proceedings of the 49th Rencontres de Moriond on Cosmology 2014). ARISF.

High resolution SZ observations at the IRAM 30-m telescope with NIKA. / Adam, R.; Adane, A.; Ade, P. et al.
Proceedings of the 49th Rencontres de Moriond on Cosmology 2014. ed. / Etienne Auge; Jacques Dumarchez; Jean Tran Thanh Van. ARISF, 2014. p. 73-76 (Proceedings of the 49th Rencontres de Moriond on Cosmology 2014).

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

Adam, R, Adane, A, Ade, P, André, P, Beelen, A, Belier, B, Benoît, A, Bideaud, A, Billot, N, Boudou, N, Bourrion, O, Calvo, M, Catalano, A, Coiffard, G, Comis, B, D'Addabbo, A, Désert, FX, Doyle, S, Goupy, J, Kramer, C, Leclercq, S, Macías-Pérez, JF, Martino, J, Mauskopf, P, Mayet, F, Monfardini, A, Pajot, F, Pascale, E, Perotto, L, Pointecouteau, E, Ponthieu, N, Revéret, V, Rodriguez, L, Ruppin, F, Savini, G, Schuster, K, Sievers, A, Tucker, C & Zylka, R 2014, High resolution SZ observations at the IRAM 30-m telescope with NIKA. in E Auge, J Dumarchez & J Tran Thanh Van (eds), Proceedings of the 49th Rencontres de Moriond on Cosmology 2014. Proceedings of the 49th Rencontres de Moriond on Cosmology 2014, ARISF, pp. 73-76, 49th Rencontres de Moriond on Cosmology 2014, La Thuile, Italy, 3/22/14.

@inproceedings{1b9807f1a7b34a4d9643f7bf1f25963b,

title = "High resolution SZ observations at the IRAM 30-m telescope with NIKA",

abstract = "High resolution observations of the thermal Sunyaev-Zel'dovich (tSZ) effect are necessary to allow the use of clusters of galaxies as a probe for large scale structures at high redshifts. With its high resolution and dual-band capability at millimeter wavelengths, the NIKA camera can play a significant role in this context. NIKA is based on newly developed Kinetic Inductance Detectors (KIDs) and operates at the IRAM 30m telescope, Pico Veleta, Spain. In this paper, we give the status of the NIKA camera, focussing on the KID technology. We then present observations of three galaxy clusters: RX J1347.5-1145 as a demonstrator of the NIKA capabilities and the recent observations of CL J1226.9+3332 (z = 0.89) and MACS J0717.5+3745 (z = 0.55). We also discuss prospects for the final NIKA2 camera, which will have a 6.5 arcminute field of view with about 5000 detectors in two bands at 150 and 260 GHz.",

author = "R. Adam and A. Adane and P. Ade and P. Andr{\'e} and A. Beelen and B. Belier and A. Beno{\^i}t and A. Bideaud and N. Billot and N. Boudou and O. Bourrion and M. Calvo and A. Catalano and G. Coiffard and B. Comis and A. D'Addabbo and D{\'e}sert, {F. X.} and S. Doyle and J. Goupy and C. Kramer and S. Leclercq and Mac{\'i}as-P{\'e}rez, {J. F.} and J. Martino and P. Mauskopf and F. Mayet and A. Monfardini and F. Pajot and E. Pascale and L. Perotto and E. Pointecouteau and N. Ponthieu and V. Rev{\'e}ret and L. Rodriguez and F. Ruppin and G. Savini and K. Schuster and A. Sievers and C. Tucker and R. Zylka",

note = "Publisher Copyright: {\textcopyright} 2014 Proceedings of the 49th Rencontres de Moriond on Cosmology 2014. All rights reserved.; 49th Rencontres de Moriond on Cosmology 2014 ; Conference date: 22-03-2014 Through 29-03-2014",

year = "2014",

language = "English (US)",

series = "Proceedings of the 49th Rencontres de Moriond on Cosmology 2014",

publisher = "ARISF",

pages = "73--76",

editor = "Etienne Auge and Jacques Dumarchez and {Tran Thanh Van}, Jean",

booktitle = "Proceedings of the 49th Rencontres de Moriond on Cosmology 2014",

}

TY - GEN

T1 - High resolution SZ observations at the IRAM 30-m telescope with NIKA

AU - Adam, R.

AU - Adane, A.

AU - Ade, P.

AU - André, P.

AU - Beelen, A.

AU - Belier, B.

AU - Benoît, A.

AU - Bideaud, A.

AU - Billot, N.

AU - Boudou, N.

AU - Bourrion, O.

AU - Calvo, M.

AU - Catalano, A.

AU - Coiffard, G.

AU - Comis, B.

AU - D'Addabbo, A.

AU - Désert, F. X.

AU - Doyle, S.

AU - Goupy, J.

AU - Kramer, C.

AU - Leclercq, S.

AU - Macías-Pérez, J. F.

AU - Martino, J.

AU - Mauskopf, P.

AU - Mayet, F.

AU - Monfardini, A.

AU - Pajot, F.

AU - Pascale, E.

AU - Perotto, L.

AU - Pointecouteau, E.

AU - Ponthieu, N.

AU - Revéret, V.

AU - Rodriguez, L.

AU - Ruppin, F.

AU - Savini, G.

AU - Schuster, K.

AU - Sievers, A.

AU - Tucker, C.

AU - Zylka, R.

PY - 2014

Y1 - 2014

N2 - High resolution observations of the thermal Sunyaev-Zel'dovich (tSZ) effect are necessary to allow the use of clusters of galaxies as a probe for large scale structures at high redshifts. With its high resolution and dual-band capability at millimeter wavelengths, the NIKA camera can play a significant role in this context. NIKA is based on newly developed Kinetic Inductance Detectors (KIDs) and operates at the IRAM 30m telescope, Pico Veleta, Spain. In this paper, we give the status of the NIKA camera, focussing on the KID technology. We then present observations of three galaxy clusters: RX J1347.5-1145 as a demonstrator of the NIKA capabilities and the recent observations of CL J1226.9+3332 (z = 0.89) and MACS J0717.5+3745 (z = 0.55). We also discuss prospects for the final NIKA2 camera, which will have a 6.5 arcminute field of view with about 5000 detectors in two bands at 150 and 260 GHz.

AB - High resolution observations of the thermal Sunyaev-Zel'dovich (tSZ) effect are necessary to allow the use of clusters of galaxies as a probe for large scale structures at high redshifts. With its high resolution and dual-band capability at millimeter wavelengths, the NIKA camera can play a significant role in this context. NIKA is based on newly developed Kinetic Inductance Detectors (KIDs) and operates at the IRAM 30m telescope, Pico Veleta, Spain. In this paper, we give the status of the NIKA camera, focussing on the KID technology. We then present observations of three galaxy clusters: RX J1347.5-1145 as a demonstrator of the NIKA capabilities and the recent observations of CL J1226.9+3332 (z = 0.89) and MACS J0717.5+3745 (z = 0.55). We also discuss prospects for the final NIKA2 camera, which will have a 6.5 arcminute field of view with about 5000 detectors in two bands at 150 and 260 GHz.

UR - http://www.scopus.com/inward/record.url?scp=85090645948&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=85090645948&partnerID=8YFLogxK

M3 - Conference contribution

AN - SCOPUS:85090645948

T3 - Proceedings of the 49th Rencontres de Moriond on Cosmology 2014

SP - 73

EP - 76

BT - Proceedings of the 49th Rencontres de Moriond on Cosmology 2014

A2 - Auge, Etienne

A2 - Dumarchez, Jacques

A2 - Tran Thanh Van, Jean

PB - ARISF

T2 - 49th Rencontres de Moriond on Cosmology 2014

Y2 - 22 March 2014 through 29 March 2014

ER -

High resolution SZ observations at the IRAM 30-m telescope with NIKA

Abstract

Publication series

Conference

ASJC Scopus subject areas

Other files and links

Fingerprint

Cite this