no code implementations • 21 Dec 2020 • J. Kammerer, M. Kasper, M. J. Ireland, R. Köhler, R. Laugier, F. Martinache, R. Siebenmorgen, M. E. van den Ancker, R. van Boekel, T. M. Herbst, E. Pantin, H. -U. Käufl, D. J. M. Petit dit de la Roche, V. D. Ivanov
We aim to measure the brightness of all three components of the T Tauri system (T Tau N, T Tau Sa, T Tau Sb) in the mid-infrared in order to obtain photometry around the $\sim 9. 7~\mu m$ silicate feature.
Solar and Stellar Astrophysics
no code implementations • 5 Oct 2020 • E. R. Garro, D. Minniti, M. Gómez, J. Alonso-García, R. H. Barbá, B. Barbuy, J. J. Clariá, A. N. Chené, B. Dias, M. Hempel, V. D. Ivanov, P. W. Lucas, D. Majaess, F. Mauro, C. Moni Bidin, T. Palma, J. B. Pullen, R. K. Saito, L. Smith, F. Surot, S. Ramírez Alegría, M. Rejkuba, V. Ripepi
Milky Way globular clusters (MW GCs) are difficult to identify at low Galactic latitudes because of high differential extinction and heavy star crowding.
Astrophysics of Galaxies Solar and Stellar Astrophysics
