scholarly journals Corrigendum to ‘Coronavirus disease 2019 in patients with neuroendocrine neoplasms: Preliminary results of the INTENSIVE study’ [European Journal of Cancer 154 (2021) 246-252]

Author(s):  
Nicola Fazio ◽  
Lorenzo Gervaso ◽  
Thorvardur R. Halfdanarson ◽  
Anna La Salvia ◽  
Johannes Hofland ◽  
...  
Author(s):  
Nicola Fazio ◽  
Lorenzo Gervaso ◽  
Thorvadur R. Halfdanarson ◽  
Anna La Salvia ◽  
Johannes Hofland ◽  
...  

Author(s):  
Kazuki Takada ◽  
Shinkichi Takamori ◽  
Naoko Miura ◽  
Yasunori Shikada ◽  
Mototsugu Shimokawa

2019 ◽  
Author(s):  
Krystallenia Alexandraki ◽  
Ioanna Antonopoulou ◽  
Maria Karaflou ◽  
Charikleia Christakou ◽  
Vasiliki Mavroeidi ◽  
...  

2009 ◽  
Vol 9 ◽  
pp. S85 ◽  
Author(s):  
RG Owen ◽  
GJ Morgan ◽  
H Jackson ◽  
FE Davies ◽  
MT Drayson ◽  
...  

1999 ◽  
Vol 173 ◽  
pp. 185-188
Author(s):  
Gy. Szabó ◽  
K. Sárneczky ◽  
L.L. Kiss

AbstractA widely used tool in studying quasi-monoperiodic processes is the O–C diagram. This paper deals with the application of this diagram in minor planet studies. The main difference between our approach and the classical O–C diagram is that we transform the epoch (=time) dependence into the geocentric longitude domain. We outline a rotation modelling using this modified O–C and illustrate the abilities with detailed error analysis. The primary assumption, that the monotonity and the shape of this diagram is (almost) independent of the geometry of the asteroids is discussed and tested. The monotonity enables an unambiguous distinction between the prograde and retrograde rotation, thus the four-fold (or in some cases the two-fold) ambiguities can be avoided. This turned out to be the main advantage of the O–C examination. As an extension to the theoretical work, we present some preliminary results on 1727 Mette based on new CCD observations.


2000 ◽  
Vol 179 ◽  
pp. 163-165
Author(s):  
S. K. Solanki ◽  
M. Fligge ◽  
P. Pulkkinen ◽  
P. Hoyng

AbstractThe records of sunspot number, sunspot areas and sunspot locations gathered over the centuries by various observatories are reanalysed with the aim of finding as yet undiscovered connections between the different parameters of the sunspot cycle and the butterfly diagram. Preliminary results of such interrelationships are presented.


1978 ◽  
Vol 48 ◽  
pp. 31-35
Author(s):  
R. B. Hanson

Several outstanding problems affecting the existing parallaxes should be resolved to form a coherent system for the new General Catalogue proposed by van Altena, as well as to improve luminosity calibrations and other parallax applications. Lutz has reviewed several of these problems, such as: (A) systematic differences between observatories, (B) external error estimates, (C) the absolute zero point, and (D) systematic observational effects (in right ascension, declination, apparent magnitude, etc.). Here we explore the use of cluster and spectroscopic parallaxes, and the distributions of observed parallaxes, to bring new evidence to bear on these classic problems. Several preliminary results have been obtained.


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