Results 81 to 90 of about 1,206 (204)
The Shack–Hartmann wavefront sensor (SHWFS) is widely utilized for ocular aberration measurement. However, large ocular aberrations caused by individual differences can easily make the spot move out of the range of the corresponding sub-aperture in SHWFS,
Haobo Zhang +5 more
doaj +1 more source
A Novel Peak‐Shape Aware Approach for Mass Alignment in Mass Spectrometry
ABSTRACT Rationale In mass spectrometry measurements, mass shifts may be inadvertently introduced due to instrumental drift and calibration inaccuracies, potentially compromising the accuracy of subsequent data analysis. This work presents a novel, label‐free algorithm to improve relative mass alignment between mass spectra.
Thomas Vanhemel +5 more
wiley +1 more source
We investigate extended Ly α emission using integral-field unit (IFU) data from the Hobby–Eberly Telescope Dark Energy Experiment (or HETDEX). We apply the modified Shepard method to image 106,853 Ly α emitters (LAEs) and median-stack them as functions ...
Brianna McKay +10 more
doaj +1 more source
In size, weight, and power (SWaP)-constrained optical systems, such as spaceborne LiDAR, high-precision centroid localization often relies on focal-plane measurements without dedicated wavefront sensors.
Zhonghao Zhao +4 more
doaj +1 more source
Comparing centroiding methods for Shack-Hartmann wavefront sensing with laser guide stars on an ELT
International audienceIn this paper we present the results of a study comparing the performance of various centroiding methods on an extended spot.
Gratadour, Damien +4 more
core +1 more source
Small bodies centroiding via image processing and convolutional neural network [PDF]
LAUREA MAGISTRALECome l’interesse della comunità scientifica per gli small bodies cresce, così il design delle sonde cerca di adattarsi al particolare ambiente che questi impongono.
Pavoni, Marco
core
Background Intensity Estimation for Cassini–ISS Image Using Deep-learning-based Diffusion Model
Accurate background intensity estimation is crucial for precise astrometric measurements in astronomical imaging, particularly in complex scenarios such as those encountered in Cassini Imaging Science Subsystem (ISS) observations of Saturn’s ring system.
Yongxin Chen +3 more
doaj +1 more source
A Robust Geometric Distortion Solution for the Main Survey Camera of CSST
The advancement in sensitivity and field of view of next-generation wide-field survey telescopes requires astrometric measurements with high precision, even in the presence of significant geometric distortions.
Yibo Yan +32 more
doaj +1 more source
The essential optical components of the Swft X-ray Telescope (XRT) are already developed items. They are: the flight spare x-ray mirror from the JET-X/Spectrum-X program and a MOS CCD (CCD22) of the type currently operating in orbit as part of the EPIC ...
core
In the last decade, the importance of high-precise geoid determination at local or national level has been pointed out by Turkish National Geodesy Commission. The Commission has also put objective of modernization of national height system of Turkey to
Uluğ, Raşit +5 more
core

