no code implementations • 23 Feb 2021 • F. Ambrosino, A. Miraval Zanon, A. Papitto, F. Coti Zelati, S. Campana, P. D'Avanzo, L. Stella, T. Di Salvo, L. Burderi, P. Casella, A. Sanna, D. de Martino, M. Cadelano, A. Ghedina, F. Leone, F. Meddi, P. Cretaro, M. C. Baglio, E. Poretti, R. P. Mignani, D. F. Torres, G. L. Israel, M. Cecconi, D. M. Russell, M. D. Gonzalez Gomez, A. L. Riverol Rodriguez, H. Perez Ventura, M. Hernandez Diaz, J. J. San Juan, D. M. Bramich, F. Lewis
Millisecond spinning, low magnetic field neutron stars are believed to attain their fast rotation in a 0. 1-1 Gyr-long phase during which they accrete matter endowed with angular momentum from a low-mass companion star.
High Energy Astrophysical Phenomena
1 code implementation • 11 Feb 2008 • D. M. Bramich
In the context of difference image analysis (DIA), we present a new method for determining the convolution kernel matching a pair of images of the same field.