High angular resolution SZ observations with NIKA and NIKA2

B. Comis; R. Adam; P. Ade; P. André; M. Arnaud; I. Bartalucci; A. Beelen; A. Benoît; A. Bideaud; N. Billot; O. Bourrion; M. Calvo; A. Catalano; G. Coiffard; F. X. Désert; S. Doyle; J. Goupy; C. Kramer; G. Lagache; S. Leclercq; J. F. Macías-Pérez; P. Mauskopf; F. Mayet; A. Monfardini; F. Pajot; E. Pascale; L. Perotto; E. Pointecouteau; G. Pisano; N. Ponthieu; G. W. Pratt; V. Revéret; A. Ritacco; L. Rodriguez; C. Romero; F. Ruppin; G. Savini; K. Schuster; A. Sievers; S. Triqueneaux; C. Tucker; R. Zylka

High angular resolution SZ observations with NIKA and NIKA2

B. Comis, R. Adam, P. Ade, P. André, M. Arnaud, I. Bartalucci, A. Beelen, A. Benoît, A. Bideaud, N. Billot, O. Bourrion, M. Calvo, A. Catalano, G. Coiffard, F. X. Désert, S. Doyle, J. Goupy, C. Kramer, G. Lagache, S. LeclercqJ. F. Macías-Pérez, P. Mauskopf, F. Mayet, A. Monfardini, F. Pajot, E. Pascale, L. Perotto, E. Pointecouteau, G. Pisano, N. Ponthieu, G. W. Pratt, V. Revéret, A. Ritacco, L. Rodriguez, C. Romero, F. Ruppin, G. Savini, K. Schuster, A. Sievers, S. Triqueneaux, C. Tucker, R. Zylka

Earth and Space Exploration, School of (SESE)

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

Abstract

NIKA2 (New IRAM KID Arrays) is a dual band (150 and 260 GHz) imaging camera based on Kinetic Inductance Detectors (KIDs) and designed to work at the IRAM 30 m telescope (Pico Veleta, Spain). Built on the experience of the NIKA prototype, NIKA2 has been installed at the 30 m focal plane in October 2015 and the commissioning phase is now ongoing. Through the thermal Sunyaev-Zeldovich (tSZ) effect, NIKA2 will image the ionized gas residing in clusters of galaxies with a resolution of 12 and 18 arcsec FWHM (at 150 and 260 GHz, respectively). We report on the recent tSZ measurements with the NIKA camera and discuss the future objectives for the NIKA2 SZ large Program, 300h of observation dedicated to SZ science. With this program we intend to perform a high angular resolution follow-up of a cosmologically-representative sample of clusters belonging to SZ catalogues, with redshift ≥ 0.5. The main output of the program will be the study of the redshift evolution of the cluster pressure profile as well as that of the scaling laws relating the cluster global properties.

Original language	English (US)
Title of host publication	Proceedings of the 51st Rencontres de Moriond on Cosmology 2016
Editors	Etienne Auge, Jacques Dumarchez, Jean Tran Thanh Van
Publisher	ARISF
Pages	289-296
Number of pages	8
ISBN (Electronic)	9791096879014
State	Published - 2016
Event	51st Rencontres de Moriond on Cosmology 2016 - La Thuile, Italy Duration: Mar 19 2016 → Mar 26 2016

Publication series

Name	Proceedings of the 51st Rencontres de Moriond on Cosmology 2016

Conference

Conference	51st Rencontres de Moriond on Cosmology 2016
Country/Territory	Italy
City	La Thuile
Period	3/19/16 → 3/26/16

ASJC Scopus subject areas

Astronomy and Astrophysics

Cite this

Comis, B., Adam, R., Ade, P., André, P., Arnaud, M., Bartalucci, I., Beelen, A., Benoît, A., Bideaud, A., Billot, N., Bourrion, O., Calvo, M., Catalano, A., Coiffard, G., Désert, F. X., Doyle, S., Goupy, J., Kramer, C., Lagache, G., ... Zylka, R. (2016). High angular resolution SZ observations with NIKA and NIKA2. In E. Auge, J. Dumarchez, & J. Tran Thanh Van (Eds.), Proceedings of the 51st Rencontres de Moriond on Cosmology 2016 (pp. 289-296). (Proceedings of the 51st Rencontres de Moriond on Cosmology 2016). ARISF.

High angular resolution SZ observations with NIKA and NIKA2. / Comis, B.; Adam, R.; Ade, P. et al.
Proceedings of the 51st Rencontres de Moriond on Cosmology 2016. ed. / Etienne Auge; Jacques Dumarchez; Jean Tran Thanh Van. ARISF, 2016. p. 289-296 (Proceedings of the 51st Rencontres de Moriond on Cosmology 2016).

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

Comis, B, Adam, R, Ade, P, André, P, Arnaud, M, Bartalucci, I, Beelen, A, Benoît, A, Bideaud, A, Billot, N, Bourrion, O, Calvo, M, Catalano, A, Coiffard, G, Désert, FX, Doyle, S, Goupy, J, Kramer, C, Lagache, G, Leclercq, S, Macías-Pérez, JF, Mauskopf, P, Mayet, F, Monfardini, A, Pajot, F, Pascale, E, Perotto, L, Pointecouteau, E, Pisano, G, Ponthieu, N, Pratt, GW, Revéret, V, Ritacco, A, Rodriguez, L, Romero, C, Ruppin, F, Savini, G, Schuster, K, Sievers, A, Triqueneaux, S, Tucker, C & Zylka, R 2016, High angular resolution SZ observations with NIKA and NIKA2. in E Auge, J Dumarchez & J Tran Thanh Van (eds), Proceedings of the 51st Rencontres de Moriond on Cosmology 2016. Proceedings of the 51st Rencontres de Moriond on Cosmology 2016, ARISF, pp. 289-296, 51st Rencontres de Moriond on Cosmology 2016, La Thuile, Italy, 3/19/16.

@inproceedings{e97ed7f693fd479fbacf245271bd3177,

title = "High angular resolution SZ observations with NIKA and NIKA2",

abstract = "NIKA2 (New IRAM KID Arrays) is a dual band (150 and 260 GHz) imaging camera based on Kinetic Inductance Detectors (KIDs) and designed to work at the IRAM 30 m telescope (Pico Veleta, Spain). Built on the experience of the NIKA prototype, NIKA2 has been installed at the 30 m focal plane in October 2015 and the commissioning phase is now ongoing. Through the thermal Sunyaev-Zeldovich (tSZ) effect, NIKA2 will image the ionized gas residing in clusters of galaxies with a resolution of 12 and 18 arcsec FWHM (at 150 and 260 GHz, respectively). We report on the recent tSZ measurements with the NIKA camera and discuss the future objectives for the NIKA2 SZ large Program, 300h of observation dedicated to SZ science. With this program we intend to perform a high angular resolution follow-up of a cosmologically-representative sample of clusters belonging to SZ catalogues, with redshift ≥ 0.5. The main output of the program will be the study of the redshift evolution of the cluster pressure profile as well as that of the scaling laws relating the cluster global properties.",

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

note = "Funding Information: We would like to thank the IRAM staff for their support during the campaigns. The NIKA dilution cryostat has been designed and built at the Institut N{\'e}el. In particular, we acknowledge the crucial contribution of the Cryogenics Group, and in particular Gregory Garde, Henri Rodenas, Jean Paul Leggeri, Philippe Camus. This work has been partially funded by the Foundation Nanoscience Grenoble, the LabEx FOCUS ANR-11-LABX-0013 and the ANR under the contracts ”MKIDS”, ”NIKA” and ANR-15-CE31-0017. This work has benefited from the support of the European Research Council Advanced Grant ORISTARS under the European Union{\textquoteright}s Seventh Framework Programme (Grant Agreement no. 291294). We acknowledge fundings from the ENIGMASS French LabEx (R. A., F. R. and B. C.), the CNES post-doctoral fellowship program (R. A.), the CNES doctoral fellowship program (A. R.) and the FOCUS French LabEx doctoral fellowship program (A. R.). Publisher Copyright: {\textcopyright} 2016 Published by ARISF. All rights reserved.; 51st Rencontres de Moriond on Cosmology 2016 ; Conference date: 19-03-2016 Through 26-03-2016",

year = "2016",

language = "English (US)",

series = "Proceedings of the 51st Rencontres de Moriond on Cosmology 2016",

publisher = "ARISF",

pages = "289--296",

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

booktitle = "Proceedings of the 51st Rencontres de Moriond on Cosmology 2016",

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TY - GEN

T1 - High angular resolution SZ observations with NIKA and NIKA2

AU - Comis, B.

AU - Adam, R.

AU - Ade, P.

AU - André, P.

AU - Arnaud, M.

AU - Bartalucci, I.

AU - Beelen, A.

AU - Benoît, A.

AU - Bideaud, A.

AU - Billot, N.

AU - Bourrion, O.

AU - Calvo, M.

AU - Catalano, A.

AU - Coiffard, G.

AU - Désert, F. X.

AU - Doyle, S.

AU - Goupy, J.

AU - Kramer, C.

AU - Lagache, G.

AU - Leclercq, S.

AU - Macías-Pérez, J. F.

AU - Mauskopf, P.

AU - Mayet, F.

AU - Monfardini, A.

AU - Pajot, F.

AU - Pascale, E.

AU - Perotto, L.

AU - Pointecouteau, E.

AU - Pisano, G.

AU - Ponthieu, N.

AU - Pratt, G. W.

AU - Revéret, V.

AU - Ritacco, A.

AU - Rodriguez, L.

AU - Romero, C.

AU - Ruppin, F.

AU - Savini, G.

AU - Schuster, K.

AU - Sievers, A.

AU - Triqueneaux, S.

AU - Tucker, C.

AU - Zylka, R.

N1 - Funding Information: We would like to thank the IRAM staff for their support during the campaigns. The NIKA dilution cryostat has been designed and built at the Institut Néel. In particular, we acknowledge the crucial contribution of the Cryogenics Group, and in particular Gregory Garde, Henri Rodenas, Jean Paul Leggeri, Philippe Camus. This work has been partially funded by the Foundation Nanoscience Grenoble, the LabEx FOCUS ANR-11-LABX-0013 and the ANR under the contracts ”MKIDS”, ”NIKA” and ANR-15-CE31-0017. This work has benefited from the support of the European Research Council Advanced Grant ORISTARS under the European Union’s Seventh Framework Programme (Grant Agreement no. 291294). We acknowledge fundings from the ENIGMASS French LabEx (R. A., F. R. and B. C.), the CNES post-doctoral fellowship program (R. A.), the CNES doctoral fellowship program (A. R.) and the FOCUS French LabEx doctoral fellowship program (A. R.). Publisher Copyright: © 2016 Published by ARISF. All rights reserved.

PY - 2016

Y1 - 2016

N2 - NIKA2 (New IRAM KID Arrays) is a dual band (150 and 260 GHz) imaging camera based on Kinetic Inductance Detectors (KIDs) and designed to work at the IRAM 30 m telescope (Pico Veleta, Spain). Built on the experience of the NIKA prototype, NIKA2 has been installed at the 30 m focal plane in October 2015 and the commissioning phase is now ongoing. Through the thermal Sunyaev-Zeldovich (tSZ) effect, NIKA2 will image the ionized gas residing in clusters of galaxies with a resolution of 12 and 18 arcsec FWHM (at 150 and 260 GHz, respectively). We report on the recent tSZ measurements with the NIKA camera and discuss the future objectives for the NIKA2 SZ large Program, 300h of observation dedicated to SZ science. With this program we intend to perform a high angular resolution follow-up of a cosmologically-representative sample of clusters belonging to SZ catalogues, with redshift ≥ 0.5. The main output of the program will be the study of the redshift evolution of the cluster pressure profile as well as that of the scaling laws relating the cluster global properties.

AB - NIKA2 (New IRAM KID Arrays) is a dual band (150 and 260 GHz) imaging camera based on Kinetic Inductance Detectors (KIDs) and designed to work at the IRAM 30 m telescope (Pico Veleta, Spain). Built on the experience of the NIKA prototype, NIKA2 has been installed at the 30 m focal plane in October 2015 and the commissioning phase is now ongoing. Through the thermal Sunyaev-Zeldovich (tSZ) effect, NIKA2 will image the ionized gas residing in clusters of galaxies with a resolution of 12 and 18 arcsec FWHM (at 150 and 260 GHz, respectively). We report on the recent tSZ measurements with the NIKA camera and discuss the future objectives for the NIKA2 SZ large Program, 300h of observation dedicated to SZ science. With this program we intend to perform a high angular resolution follow-up of a cosmologically-representative sample of clusters belonging to SZ catalogues, with redshift ≥ 0.5. The main output of the program will be the study of the redshift evolution of the cluster pressure profile as well as that of the scaling laws relating the cluster global properties.

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UR - http://www.scopus.com/inward/citedby.url?scp=85088926346&partnerID=8YFLogxK

M3 - Conference contribution

AN - SCOPUS:85088926346

T3 - Proceedings of the 51st Rencontres de Moriond on Cosmology 2016

SP - 289

EP - 296

BT - Proceedings of the 51st Rencontres de Moriond on Cosmology 2016

A2 - Auge, Etienne

A2 - Dumarchez, Jacques

A2 - Tran Thanh Van, Jean

PB - ARISF

T2 - 51st Rencontres de Moriond on Cosmology 2016

Y2 - 19 March 2016 through 26 March 2016

ER -

High angular resolution SZ observations with NIKA and NIKA2

Abstract

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ASJC Scopus subject areas

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