How Variable Is the Mayo Score Between Observers and Might This Affect Trial Recruitment or Outcome?

Autor: Walsh, AJ, Brain, O, Keshav, S, Buchel, OC, Merrin, B, Rolinski, M, Thomas, S, White, L, Altman, DG, Travis, S

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::71563e034bc6babf18682cee7bfe5f41
https://ora.ox.ac.uk/objects/uuid:a1680f74-f12d-4f19-97f9-2f73b4f30401

Which Activity Index for Ulcerative Colitis (UC)? Evaluation of Inter-Observer Variation in Clinical, Endoscopic and Composite Indices

Autor: Walsh, AJ, Brain, O, Keshav, S, Buchel, OC, Merrin, B, Rolinski, M, Thomas, S, White, L, von Herbay, A, Warren, BF, Altman, DG, Travis, S

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::4fa2c617c3a8d0c49190daa339f7596b
https://ora.ox.ac.uk/objects/uuid:0f682594-ba03-4d15-abca-b22213b18643

Survey overview and data release 1⋆⋆⋆

Autor: Beuther, H, Bihr, S, Rugel, M, Johnston, K, Wang, Y, Walter, F, Brunthaler, A, Walsh, AJ, Ott, J, Stil, J, Henning, T, Schierhuber, T, Kainulainen, J, Heyer, M, Goldsmith, PF, Anderson, LD, Longmore, SN, Klessen, RS, Glover, SCO, Urquhart, JS, Plume, R, Ragan, SE, Schneider, N, McClure-Griffiths, NM, Menten, KM, Smith, R, Roy, N, Shanahan, R, Nguyen-Luong, Q, Bigiel, F

Publikováno v: Astronomy & Astrophysics
Beuther, H, Bihr, S, Rugel, M, Johnston, K, Wang, Y, Walter, F, Brunthaler, A, Walsh, A J, Ott, J, Still, J, Henning, T, Schierhube, T, Kainulainen, K, Heyer, M, Goldsmith, P, Anderson, L D, Longmore, S N, Klessen, R S, Glover, S C O, Urquhart, J S, Plume, R, Ragan, S E, Schneider, N, McClure-Griffiths, N M, Menten, K M, Smith et al, R, Roy, N, Shanahan, R, Nguyen-Luong, Q & Bigiel, F 2016, ' The HI/OH/Recombination line survey of the inner Milky Way (THOR) ', Astronomy & Astrophysics, vol. 595 . https://doi.org/10.1051/0004-6361/201629143

Context: The past decade has witnessed a large number of Galactic plane surveys at angular resolutions below 20". However, no comparable high-resolution survey exists at long radio wavelengths around 21cm in line and continuum emission. Methods: Empl

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3e649c457b6caa0ff8ab68d149732008

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