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The effects of cold ischaemia on tumour morphology and DNA quality for whole genome sequencing: A systematic comparative study of a series of renal tumours in a single institution

Autor: Browning, L, Cabes, M, Roberts, ISD, Rendek, A, Collantes, E, McCole, M, Colling, RT, Pell, R, Henderson, S, Schuh, A, Verrill, C

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=od______1064::c8451849cfbe6162edf8dcc9be579a70
https://ora.ox.ac.uk/objects/uuid:fef07316-a3e7-4b0b-84cc-5e7805858342

Euclid preparation III. Galaxy cluster detection in the wide photometric survey, performance and algorithm selection

Autor: Euclid Collaboration, Adam, R., Vannier, M., Maurogordato, S., Biviano, A., Adami, C., Ascaso, B., Bellagamba, F., Benoist, C., Cappi, A., D��az-S��nchez, A., Durret, F., Farrens, S., Gonzalez, A. H., Iovino, A., Licitra, R., Maturi, M., Mei, S., Merson, A., Munari, E., Pell��, R., Ricci, M., Rocci, P. F., Roncarelli, M., Sarron, F., Amoura, Y., Andreon, S., Apostolakos, N., Arnaud, M., Bardelli, S., Bartlett, J., Baugh, C. M., Borgani, S., Brodwin, M., Castander, F., Castignani, G., Cucciati, O., De Lucia, G., Dubath, P., Fosalba, P., Giocoli, C., Hoekstra, H., Mamon, G. A., Melin, J. B., Moscardini, L., Paltani, S., Radovich, M., Sartoris, B., Schultheis, M., Sereno, M., Weller, J., Burigana, C., Carvalho, C. S., Corcione, L., Kurki-Suonio, H., Lilje, P. B., Sirri, G., Toledo-Moreo, R., Zamorani, G.

Publikováno v: Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2019, 627, pp.A23. ⟨10.1051/0004-6361/201935088⟩
Euclid Collaboration 2019, ' Euclid preparation III. Galaxy cluster detection in the wide photometric survey, performance and algorithm selection ', Astronomy & Astrophysics, vol. 627, A23 . https://doi.org/10.1051/0004-6361/201935088
Astronomy & astrophysics, 2019, Vol.627, pp.A23 [Peer Reviewed Journal]
Astronomy and Astrophysics (0004-6361), 627, A23

Galaxy cluster counts in bins of mass and redshift have been shown to be a competitive probe to test cosmological models. This method requires an efficient blind detection of clusters from surveys with a well-known selection function and robust mass

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7b358dad699b89d8fa331c0239d5d613

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