Results 21 to 30 of about 2,005,952 (304)

An Optimal Integral Controller for Adaptive Optics Systems

open access: yesSensors, 2023
Integral controllers are commonly employed in astronomical adaptive optics. This work presents a novel tuning procedure for integral controllers in adaptive optics systems which relies on information about the measured disturbances. This tuning procedure
Pedro Escárate   +3 more
doaj   +1 more source

Spectral Templates Optimal for Selecting Galaxies at z > 8 with the JWST

open access: yesThe Astrophysical Journal, 2023
The selection of high-redshift galaxies often involves spectral energy distribution (SED) fitting to photometric data, an expectation for contamination levels, and measurement of sample completeness—all vetted through comparison to spectroscopic redshift
Rebecca L. Larson   +11 more
doaj   +1 more source

Photometric Accuracy of Deconvolved Simulated Astronomical Images

open access: yesThe Astrophysical Journal, 2005
A study of the photometric accuracy of deconvolved astronomical images was undertaken by processing two simulated images with several well-known algorithms. The simulations consisted of an image of a simple star field and an image of an active galactic nucleus (AGN).
Stephen R. McNeil, J. Ward Moody
openaire   +1 more source

VLBI Network SIMulator: An Integrated Simulation Tool for Radio Astronomers

open access: yes, 2018
In this paper we introduce a software package, the Very Long Baseline Interferometry Network SIMulator (VNSIM), which provides an integrated platform assisting radio astronomers to design the Very Long Baseline Interferometry (VLBI) experiments and evaluate the network performance with a user-friendly interface. Though VNSIM is motivated to be designed
Zhao, Zhen, An, Tao, Lao, Baoqiang
openaire   +2 more sources

Query driven visualization of astronomical catalogs [PDF]

open access: yes, 2011
Interactive visualization of astronomical catalogs requires novel techniques due to the huge volumes and complex structure of the data produced by existing and upcoming astronomical surveys.
Hugo Buddelmeijer   +6 more
core   +2 more sources

Self-consistent Atmosphere Representation and Interaction in Photon Monte Carlo Simulations

open access: yesThe Astrophysical Journal
We present a self-consistent representation of the atmosphere and implement the interactions of light with the atmosphere using a photon Monte Carlo approach.
J. R. Peterson   +3 more
doaj   +1 more source

DeepSurveySim: Simulation Software and Benchmark Challenges for Astronomical Observation Scheduling

open access: yesDeepSurveySim: Simulation Software and Benchmark Challenges for Astronomical Observation Scheduling, 2023
Modern astronomical surveys have multiple competing scientific goals. Optimizing the observation schedule for these goals presents significant computational and theoretical challenges, and state-of-the-art methods rely on expensive human inspection of simulated telescope schedules.
Voetberg, Maggie, Nord, Brian
openaire   +2 more sources

A Lightweight Procedural Layer for Hybrid Experimental–Computational Workflows in Materials Science

open access: yesAdvanced Engineering Materials, EarlyView.
We unveil a prototype hybrid‐workflow framework that fuses automatedcomputation with hands‐on experiments. Built atop pyiron, a lightweight, parameterized layer translates procedure descriptions into executable manual steps, syncing instrument settings, human interventions, and data capture in real‐time today.
Steffen Brinckmann   +8 more
wiley   +1 more source

Constructing a Galaxy Cluster Catalog in IllustrisTNG300 Using the Mulguisin Algorithm

open access: yesThe Astrophysical Journal
We present a new simulated galaxy cluster catalog based on the IllustrisTNG simulation. We use the Mulguisin (MGS) algorithm to identify galaxy overdensities.
Lael Shin   +4 more
doaj   +1 more source

Kinematic Evidence of an Embedded Protoplanet in HD 142666 Identified by Machine Learning

open access: yesThe Astrophysical Journal, 2023
Observations of protoplanetary disks have shown that forming exoplanets leave characteristic imprints on the gas and dust of the disk. In the gas, these forming exoplanets cause deviations from Keplerian motion, which can be detected through molecular ...
J. P. Terry   +3 more
doaj   +1 more source

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