| Texto completo | |
| Autor(es): |
Crew, G. B.
;
Goddi, C.
;
Matthews, L. D.
;
Rottmann, H.
;
Saez, A.
;
Marti-Vidal, I.
Número total de Autores: 6
|
| Tipo de documento: | Artigo Científico |
| Fonte: | Publications of the Astronomical Society of the Pacific; v. 135, n. 1044, p. 21-pg., 2023-02-01. |
| Resumo | |
The development of the Atacama Large Millimeter/submillimeter Array (ALMA) phasing system (APS) has allowed ALMA to function as an extraordinarily sensitive station for very long baseline interferometry (VLBI) at frequencies of up to 230 GHz (lambda approximate to 1.3 mm). Efforts are now underway to extend the use of the APS to 345 GHz (lambda approximate to 0.87 mm). Here we report a characterization of APS performance at 345 GHz based on a series of tests carried out between 2015 and 2021, including a successful global VLBI test campaign conducted in 2018 October in collaboration with the Event Horizon Telescope. (AU) | |
| Processo FAPESP: | 21/01183-8 - Estudo de jatos astrofísicos em alta resolução por meio de interferometria |
| Beneficiário: | Ciriaco Goddi |
| Modalidade de apoio: | Auxílio à Pesquisa - Jovens Pesquisadores |