Results 71 to 80 of about 577 (218)
ABSTRACT Cervical cancer is the fourth most common cancer among women worldwide, with higher prevalence in low‐resource countries due to limited access to screening and HPV vaccination. Nucleic acid amplification tests (NAATs) such as Xpert HPV (Cepheid), enable rapid detection of high‐risk HPV (HR‐HPV) genotypes.
Valentin Lemoine +10 more
wiley +1 more source
The evolution of the Galactic nuclear bulge traced by Cepheid variable stars [PDF]
The Galactic nuclear bulge hosts significant populations of young stars, within a few hundred parsecs around the Galactic Centre, unlike the more extended bulge. Recently, we discovered classical Cepheid variable stars (hereinafter Cepheids) in the Galactic nuclear bulge.
openaire +1 more source
The Draco Dwarf spheroidal (dSph) galaxy is one of the nearest and the most dark-matter-dominated satellites of the Milky Way. We obtained multiepoch near-infrared (NIR, JHK _s ) observations of the central region of Draco dSph covering a sky area of ∼21′
Anupam Bhardwaj +6 more
doaj +1 more source
ABSTRACT Nearly all cervical cancer cases are caused by high‐risk human papillomavirus (hrHPV) infections. The World Health Organization recommends screening for hrHPV using nucleic acid amplification tests (NAATs) that detect hrHPV DNA or mRNA. Lack of access to affordable, point‐of‐care screening tests in resource‐limited settings leads to women ...
Emilie Newsham Novak +9 more
wiley +1 more source
Investigating Fourier Coefficient Relationships of Cepheid Variable Stars
Cepheid stars are valuable due to their usefulness in determining distances within our galaxy, and to other galaxies. Cepheid stars’ light variation can be parameterized using a Fourier series with coefficients Ai and i . Fourier coefficients have been
Morgan, Siobahn, Cronin, Forrest
core
Using Cepheid Variable Pulsation Properties to Trace Galaxy Age and Metallicity [PDF]
Cepheid variable stars have long been used as distance indicators due to their strong period-luminosity relation. However, the period of a Cepheid is affected by its metallicity so any difference in metal-content between calibration Cepheids and Cepheids
Short, L
core +1 more source
Self-consistent Nonlinear Classical Cepheid Pulsations during Stellar Evolution with MESA
We extend the time-dependent convection (TDC) treatment in MESA by introducing eddy-viscous dissipation. This software change brings MESA-TDC into closer alignment with the radial stellar pulsation (RSP) framework of the MESA-RSP module.
Ebraheem Farag +7 more
doaj +1 more source
Non-particle dark matter from Hubble parameter
The measurements of the Hubble parameter using the cosmic microwave background radiation appear to be inconsistent with the measurements of this parameter using Cepheid variable stars.
Nikodem J. Popławski
doaj +1 more source
CCD Photometry of Cepheid Variable
The main purpose of this project is to become familiar with the techniques and methods of observational astronomy and CCD photometry. I will observe the brightness of stars and deduce some properties of these stars from these observations.
Demarais, Benjamin T.
core
Using an updated and significantly augmented sample of Cepheid and tip of the red giant branch (TRGB) distances to 28 nearby spiral and irregular galaxies, covering a wide range of metallicities, we have searched for evidence of a correlation of the zero-
Barry F. Madore, Wendy L. Freedman
doaj +1 more source

