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EPJ Web of Conferences 257, 00017 (2022) mm Universe @ NIKA2 4 Conclusions

We have demonstrated the capability of instantaneously mapping large areas of the sky (onedegree diameter FoV) in spectroscopic mode by exploiting FTS coupled to KIDs.

KISS has played a fundamental role as the test bed for dedicated spectral mapper large-telescope, CONCERTO, which has currently passed its technical commissioning phase, as reported in [16]. Despite its pioneering and challenging nature, it has paved the way for the technological advancement of the mm observations ground-based at multi-wavelength large FoV.

In this paper, we have reported the integrated Venus brightness temperature and the uncalibrated spectral maps of Jupiter.

Acknowledgements. The KID arrays described in this paper have been produced at the PTA Grenoble microfabrication facility. This work has been partially supported by the LabEx FOCUS ANR-11-LABX-0013, the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation program (project CONCERTO, grant agreement No 788212), and the Excellence Initiative of Aix-Marseille University-A*Midex, a French “Investissements d’Avenir” program. This work has been partially funded by the Spanish Ministry of Science under the project AYA2017-84185-P. Based on observations made with the first QUIJOTE telescope (QT-1), operated on the island of Tenerife in the Spanish Observatorio del Teide of the Instituto de Astrofisica de Canarias.

References

[1] K. Basu, M. Remazeilles, J. B. Melin et al., Experimental Astronomy, (2021)

[2] D. H. Martin and E. Puplett, Infrared Physics 10, 105-109 (1970)

[3] A. Fasano, M. Aguiar, A. Benoit et al., JLTP 199, 529-536 (2020)

[4] A. Catalano, A. Bideaud, O. Bourrion et al., A&A 641, A179 (2020)

[5] S. Masi, P. de Bernardis, A. Paiella et al., JCAP 7, 3 (2003)

[6] Concerto Collaboration, P. Ade, M. Aravena et al., A&A 642, 13 (2020)

[7] J. Zmuidzinas, Annual Review of Condensed Matter Physics 3, 169 (2012)

[8] M. De Petris, S. De Gregori, M. Decina et al., MNRAS 429, 849–858 (2013)

[9] A. Ritacco, N. Ponthieu, A. Catalano et al., A&A 599, A34 (2017)

[10] R. Adam, A. Adane, P. Ade et al., A&A 609, A115 (2018)

[11] L. D. Spencer, Dissertation, Spectral characterization of the HERSCHEL SPIRE photometer, (University of Lethbridge, Canada, 2005), ADS bibcode 2005MsT..........1S

[12] A. Fasano, J. F. Macías-Pérez, A. Benoit, A. et al., A&A accepted, eprint arXiv:2109.03145

[13] A. Fasano, M. Aguiar, A. Benoit et al., EPJ Web of Conferences 228, (2020)

[14] A. Bellotti, Dissertation, Jupiter: a study of atmospheric composition, structure, and dynamics using microwave techniques, (Georgia Institute of Technology, 2018), http://hdl.handle.net/1853/61122

[15] Planck Collaboration, Y. Akrami, M. Ashdown et al., A&A 607, A122 (2017)

[16] A. Monfardini, A. Beelen, A. Benoit et al., JLTP submitted, eprint arXiv:2106.14028 Rh