scholarly journals Reply to comments on “COVID-19 in patients with neuroendocrine neoplasms: Preliminary results of a worldwide survey (The INTENSIVE study)”

2021 ◽  
Author(s):  
Fazio N ◽  
Spada F ◽  
Gervaso L
Keyword(s):  
Neuroendocrine Neoplasms ◽  
Intensive Study ◽  
Preliminary Results

scholarly journals COVID-19 in patients with neuroendocrine neoplasms: Preliminary results of a worldwide survey (The INTENSIVE study)

2021 ◽  
Author(s):  
Nicola Fazio ◽  
Lorenzo Gervaso ◽  
Thorvadur R. Halfdanarson ◽  
Anna La Salvia ◽  
Johannes Hofland ◽  
...  
Keyword(s):  
Neuroendocrine Neoplasms ◽  
Intensive Study ◽  
Preliminary Results

scholarly journals Re: COVID-19 in patients with neuroendocrine neoplasms: Preliminary results of a worldwide survey (The INTENSIVE study)

2021 ◽  
Author(s):  
Kazuki Takada ◽  
Shinkichi Takamori ◽  
Naoko Miura ◽  
Yasunori Shikada ◽  
Mototsugu Shimokawa
Keyword(s):  
Neuroendocrine Neoplasms ◽  
Intensive Study ◽  
Preliminary Results

Immunohistochemical expression of ephrines A2 and A4 receptors in neuroendocrine neoplasms: preliminary results

2019 ◽  
Author(s):  
Krystallenia Alexandraki ◽  
Ioanna Antonopoulou ◽  
Maria Karaflou ◽  
Charikleia Christakou ◽  
Vasiliki Mavroeidi ◽  
...  
Keyword(s):  
Neuroendocrine Neoplasms ◽  
Immunohistochemical Expression ◽  
Preliminary Results

A547 MRC Myeloma IX: Preliminary Results from the Non-Intensive Study

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

The O–C diagrams of minor planets − a new approach to modelling the rotation

1999 ◽  
Vol 173 ◽  
pp. 185-188
Author(s):  
Gy. Szabó ◽  
K. Sárneczky ◽  
L.L. Kiss
Keyword(s):  
Error Analysis ◽  
Time Dependence ◽  
Theoretical Work ◽  
Minor Planet ◽  
Minor Planets ◽  
New Approach ◽  
Preliminary Results ◽  
Ccd Observations

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.

Cyclic Evolution of Sunspots: Gleaning New Results from Old Data

2000 ◽  
Vol 179 ◽  
pp. 163-165
Author(s):  
S. K. Solanki ◽  
M. Fligge ◽  
P. Pulkkinen ◽  
P. Hoyng
Keyword(s):  
Sunspot Number ◽  
Sunspot Cycle ◽  
Preliminary Results ◽  
Butterfly Diagram

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.

Systematic effects in observed parallaxes

1978 ◽  
Vol 48 ◽  
pp. 31-35
Author(s):  
R. B. Hanson
Keyword(s):  
Error Estimates ◽  
Zero Point ◽  
Absolute Zero ◽  
Apparent Magnitude ◽  
Coherent System ◽  
Preliminary Results ◽  
General Catalogue ◽  
Systematic Effects ◽  
New Evidence ◽  
Right Ascension

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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