Zobrazeno 1 - 10
of 31
pro vyhledávání: '"Verkouter, H."'
Autor:
Roshi, D. Anish, Aponte, N., Araya, E., Arce, H., Baker, L. A., Baan, W., Becker, T. M., Breakall, J. K., Brown, R. G., Brum, C. G. M., Busch, M., Campbell, D. B., Cohen, T., Cordova, F., Deneva, J. S., Devogele, M., Dolch, T., Fernandez-Rodriguez, F. O., Ghosh, T., Goldsmith, P. F., Gurvits, L. I., Haynes, M., Heiles, C., Hessel, J. W. T., Hickson, D., Isham, B., Kerr, R. B., Kelly, J., Kiriazes, J. J., Lautenbach, J., Lebron, M., Lewandowska, N., Magnani, L., Manoharan, P. K., Margot, J. L., Marshall, S. E., McGilvray, A. K., Mendez, A., Minchin, R., Negron, V., Nolan, M. C., Olmi, L., Paganelli, F., Palliyaguru, N. T., Pantoja, C. A., Paragi, Z., Parshley, S. C., Peek, J. E. G., Perera, B. B. P., Perillat, P., Pinilla-Alonso, N., Quintero, L., Radovan, H., Raizada, S., Robishaw, T., Route, M., Salter, C. J., Santoni, A., Santos, P., Sau, S., Selvaraj, D., Smith, A. J., Sulzer, M., Vaddi, S., Vargas, F., Venditti, F. C. F., Venkataraman, A., Verkouter, H., Virkki, A. K., Vishwas, A., Weinreb, S., Werthimer, D., Wolszczan, A., Zambrano-Marin, L. F.
The Arecibo Observatory (AO) is a multidisciplinary research and education facility that is recognized worldwide as a leading facility in astronomy, planetary, and atmospheric and space sciences. AO's cornerstone research instrument was the 305-m Wil
Externí odkaz:
http://arxiv.org/abs/2103.01367
The EVN MkIV data processor is being equipped with a high data output capability, called PCInt. In its next phase it will allow very high data output rates, up to 160 Mb/s. This functionality is required for the high spectral resolution that will be
Externí odkaz:
http://arxiv.org/abs/astro-ph/0412292
Autor:
Nutma, T. A., Dabin, C., Valentijn, E. A., Pizzo, R., Deul, E.R., Mol, J-D., de Plaa, J., Verkouter, H.
Publikováno v:
Astronomical Data Analysis Software and Systems XXIX: Proceedings, 527, 477-480
The Euclid common data model is central in, and essential to, the Euclid science ground segment. It defines the format of all data exchanged between the pipelines and stored in the Euclid Archive, and ensures all components can communicate with each
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=narcis______::d35ec0406fbf477003b68b73a66dc6f4
https://research.rug.nl/en/publications/48e447f0-e216-4e86-b0dc-2f87c3dcdb52
https://research.rug.nl/en/publications/48e447f0-e216-4e86-b0dc-2f87c3dcdb52
Autor:
Mulder, W., de Jong, J. T. A., Verdoes Kleijn, G. A., Valentijn, E. A., Williams, O. R., Boxhoorn, D. R., Belikov, A. N., Fabricius, M., Helmich, E. M., Wetzstein, M., Vassallo, T., George, K., Pizzo, R., Deul, E.R., Mol, J-D., de Plaa, J., Verkouter, H.
Publikováno v:
Astronomical Data Analysis Software and Systems XXIX: Proceedings, 615-618
STARTPAGE=615;ENDPAGE=618;TITLE=Astronomical Data Analysis Software and Systems XXIX
STARTPAGE=615;ENDPAGE=618;TITLE=Astronomical Data Analysis Software and Systems XXIX
ESA's Euclid mission will construct a 3D map of the distribution of over a billion galaxies. Multi-band ground-based imaging data will complement the satellite data as it is essential for measuring highly accurate colors required to obtain precise ga
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=narcis______::1156541303f173f5cf2c03aac4a14046
https://research.rug.nl/en/publications/95b3e576-58d1-483a-93c8-2a14fef9d07f
https://research.rug.nl/en/publications/95b3e576-58d1-483a-93c8-2a14fef9d07f
Autor:
Soancatl-Aguilar, V., Williams, O.~R., Ji, C., Valentijn, E.~A., Mathlener, A., Roerdink, J.~B.~T.~M., Pizzo, R., Deul, E.~R., Mol, J.~D., de Plaa, J., Verkouter, H.
Publikováno v:
Astronomical Society of the Pacific Conference Series
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=narcis______::d16e26d6cdd8a0e06d81c8d7b2458033
https://research.rug.nl/en/publications/d4001b8f-2f3c-453a-a1cf-5f79ea79f3f0
https://research.rug.nl/en/publications/d4001b8f-2f3c-453a-a1cf-5f79ea79f3f0
Autor:
Danehkar, A.1 (AUTHOR) danehkar@eurekasci.com
Publikováno v:
Frontiers in Astronomy & Space Sciences. 2024, p1-16. 16p.
Autor:
Schilizzi, R., Aldrich, W., Anderson, B., Bos, A., Campbell, R., Canaris, J., Cappallo, R., Casse, J., Cattani, A., Goodman, J., van Langevelde, H., Maccafferri, A., Millenaar, R., Noble, R., Olnon, F., Parsley, S., Phillips, C., Pogrebenko, S., Smythe, D., Szomoru, A., Verkouter, H., Whitney, A.
Publikováno v:
Experimental Astronomy; August 2001, Vol. 12 Issue: 1 p49-67, 19p
Autor:
Paul, Surajit1,2 (AUTHOR) surajit@physics.unipune.ac.in, Kale, Ruta3 (AUTHOR), Datta, Abhirup4 (AUTHOR), Basu, Aritra5 (AUTHOR), Sur, Sharanya6 (AUTHOR), Parekh, Viral7,8 (AUTHOR), Gupta, Prateek1,6 (AUTHOR), Chatterjee, Swarna4 (AUTHOR), Salunkhe, Sameer1,3 (AUTHOR), Iqbal, Asif9 (AUTHOR), Pandey-Pommier, Mamta10 (AUTHOR), Raja, Ramij4,7 (AUTHOR), Rahaman, Majidul4,11 (AUTHOR), Raychaudhury, Somak12,13 (AUTHOR), Nath, Biman B.2 (AUTHOR), Majumdar, Subhabrata14 (AUTHOR)
Publikováno v:
Journal of Astrophysics & Astronomy. 4/27/2023, Vol. 44 Issue 1, p1-33. 33p.
Autor:
Huib Jan van Langevelde, Olnon, F. M., Verkouter, H., Kramer, B., Garrett, M. A., Szomoru, A., Parsley, S. M., Bos, A.
Publikováno v:
NASA Astrophysics Data System
Traditionally VLBI observations focus on a small patch of sky and image typically a few 100 mas around a bright source, which is often used to self-calibrate the data. High spectral and time resolution is needed to image a larger area, in principle u
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7205965f6a4da90500732564a22cd0eb
https://ui.adsabs.harvard.edu/#abs/2004ASPC..314...50V
https://ui.adsabs.harvard.edu/#abs/2004ASPC..314...50V
Publikováno v:
NASA Astrophysics Data System
The EVN MkIV data processor is being equipped with a high data output capability, called PCInt. In its next phase it will allow very high data output rates, up to 160 Mb/s. This functionality is required for the high spectral resolution that will be
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c4f2a96391f437e3c916fa92214e0f51