no code implementations • 21 Jan 2021 • A. J. Rigby, N. Peretto, R. Adam, P. Ade, M. Anderson, P. André, A. Andrianasolo, H. Aussel, A. Bacmann, A. Beelen, A. Benoît, S. Berta, O. Bourrion, A. Bracco, M. Calvo, A. Catalano, M. De Petris, F. -X. Désert, S. Doyle, E. F. C. Driessen, P. García, A. Gomez, J. Goupy, F. Kéruzoré, C. Kramer, B. Ladjelate, G. Lagache, S. Leclercq, J. -F. Lestrade, J. F. Macías-Pérez, P. Mauskopf, F. Mayet, A. Monfardini, L. Perotto, G. Pisano, N. Ponthieu, V. Revéret, I. Ristorcelli, A. Ritacco, C. Romero, H. Roussel, F. Ruppin, K. Schuster, S. Shu, A. Sievers, C. Tucker, E. J. Watkins
Here, we present the first results from the Galactic Star Formation with NIKA2 (GASTON) project, a Large Programme at the IRAM 30-m telescope which is mapping $\approx$2 deg$^2$ of the inner Galactic plane (GP), centred on $\ell$=23. 9$^\circ$, $b$=0. 05$^\circ$, as well as targets in Taurus and Ophiuchus in 1. 15 and 2. 00 mm continuum wavebands.
Astrophysics of Galaxies
no code implementations • 9 Dec 2020 • M. Tapia, P. A. R. Ade, P. S. Barry, T. L. R. Brien, E. Castillo-Domínguez, D. Ferrusca, V. Gómez-Rivera, P. Hargrave, J. L. Hernández Rebollar, A. Hornsby, D. H. Hughes, J. M. Jáuregui-García, P. Mauskopf, D. Murias, A. Papageorgiou, E. Pascale, A. Pérez, S. Rowe, M. W. L. Smith, C. Tucker, M. Velázquez, S. Ventura, S. Doyle
Subsequently, with a re-imaging lens and a black body point source, the beams of every detector are mapped, obtaining a mean FWHM size of $\sim$3. 27 mm, close to the expected 3. 1 mm.
Instrumentation and Methods for Astrophysics
no code implementations • 9 Dec 2020 • T. L. R. Brien, P. A. R. Ade, P. S. Barry, E. Castillo-Domínguez, D. Ferrusca, V. Gómez-Rivera, P. Hargrave, J. L. Hernández Rebollar, A. Hornsby, D. H. Hughes, J. M. Jáuregui-García, P. Mauskopf, D. Murias, A. Papageorgiou, E. Pascale, A. Pérez, S. Rowe, M. W. L. Smith, M. Tapia, C. Tucker, M. Velázquez, S. Ventura, S. Doyle
The Mexico-UK Submillimetre Camera for AsTronomy (MUSCAT) is a 1. 1 mm receiver consisting of 1, 500 lumped-element kinetic inductance detectors (LEKIDs) for the Large Millimeter Telescope (LMT; Volc\'an Sierra Negra in Puebla, M\'exico).
Instrumentation and Methods for Astrophysics
