Zobrazeno 1 - 10
of 10
pro vyhledávání: '"L. M. Newton"'
Publikováno v:
Analytical and quantitative cytology and histology. 20(2)
To investigate the accuracy with which the nuclei of cells in overlapped and thick clusters in cervical/ vaginal smears can be classified independent of the segmentation algorithm used and to determine the influence of three-dimensional (3-D) process
Publikováno v:
Analytical and quantitative cytology and histology. 20(2)
To use three-dimensional (3-D) imaging and localized adaptive image analysis to enable automated cervical smear screening systems to efficiently and effectively process thick and overlapped cell clusters currently left unprocessed.Instrumentation was
Publikováno v:
Allergy. 18:131-147
Publikováno v:
Nature. 313:374-376
The braking index, n, of a pulsar, which describes the dependence of the braking torque on rotation frequency, is a fundamental parameter of pulsar electrodynamics. Simple theoretical arguments, based on the assumption of a constant dipolar magnetic
Publikováno v:
Arizona medicine. 37(11)
Autor:
L. M. Newton
Publikováno v:
Publications of the Astronomical Society of Australia. 7:105-106
Autor:
L. M. Newton
Publikováno v:
Publications of the Astronomical Society of Australia. 4:492-493
Autor:
N. W. Broten, R. X. McGee, L. M. Newton, Takeshi Oka, J. M. MacLeod, L. W. Avery, J. W. Brooks
Publikováno v:
The Astrophysical Journal. 209:L143
The J=1..-->..0 and J=8..-->..7 rotational transitions of interstellar cyanodiacetylene have been observed in Sgr B2. These observations confirm the earlier detection of this heavy molecule, and provide further information on its excitation. The J=8.
Publikováno v:
The Astrophysical Journal. 236:L25
The paper reports on timing variations, which over a 2 year interval have shown large variations in the period of PSR 0820+02. It is shown that these variations are consistent with the pulsar being a member of a binary system with an orbital period o
Autor:
R. N. Manchester, D. J. Cooke, J. H. Taylor, L. M. Newton, M. Damashek, P. R. Backus, J. J. Condon
Publikováno v:
The Astrophysical Journal. 268:832