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The abundances of carbon and nitrogen in the atmospheres of classical Be stars. [PDF]
Astrophys Space SciPeters GJ +4 more
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Evaluating linear model frameworks for directed predictive influence estimation from hypothalamic calcium imaging. [PDF]
J Neurosci MethodsClementsmith X +3 more
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Localizing individual exciton on a quantum Hall antidot. [PDF]
Nat CommunPu R +7 more
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Real-time visual astronomy using image intensifiers and data modeling
SPIE Proceedings, 2003This paper presents the use of an image intensifier as an astronomical eyepiece for real-time observation of deep sky objects. The optical frequency spectra of observational astronomical objects are reported and compared with the spectral response curve of a Generation 3 intensified optical system.
Holger M Jaenisch +2 more
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Astronomy Education Journal, 2022
There is a critical need for research-based active learning instructional materials for the teaching and learning of STEM in online courses. Every year, hundreds of thousands of undergraduate non-science majors enroll in general education astronomy courses to fulfill their institution’s liberal arts requirements.
Molly Simon +5 more
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There is a critical need for research-based active learning instructional materials for the teaching and learning of STEM in online courses. Every year, hundreds of thousands of undergraduate non-science majors enroll in general education astronomy courses to fulfill their institution’s liberal arts requirements.
Molly Simon +5 more
openaire +1 more source
Data driven model based least squares image reconstruction for radio astronomy
2011 IEEE International Conference on Acoustics, Speech and Signal Processing (ICASSP), 2011Image reconstruction problems in radio astronomy and other fields like biomedical imaging are often ill-posed and some form of regularization is required. This imposes user specified constraints to the reconstruction process that may produce an undesirable bias to the solution.
Stefan J. Wijnholds +1 more
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The ALMA/EVLA project data model: steps toward a common project description for astronomy
SPIE Proceedings, 2008The "Project Data Model" (PDM) is a model of the information that describes an astronomical observing project. In this paper we consider the PDM to cover the Proposal and Observing Preparation phases (also often called Phase 1 and Phase 2), and also the intermediate phase of reviewing and approving the project.
Alan Bridger, Bryan Butler
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Atomic data and modelling in X-ray astronomy
AIP Conference Proceedings, 1998In the next 3 years the study of astronomical X-ray spectra will make a significant advance owing to the launch of several new instruments. These will represent an order of magnitude improvement in both spectral resolving power and sensitivity over current instruments, and will allow use of plasma diagnostics which have not been previously accessible ...
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Quest for supernova R-process: New data in astronomy and nuclear physics, and theoretical modeling
Nuclear Physics A, 2003Abstract We study the r-process nucleosynthesis in Type II supernovae in view of new astronomical data of metal-deficient stars, new nuclear reaction data, and theoretical modeling of neutrino-driven winds. High entropy problem and neutrino interaction problem are discussed in order to resolve them and to look for appropriate physical condition for ...
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A Provenance Data Model for Astronomy
2019In Astronomy as well as in other sciences it is of crucial importance to have information about the origin and history of data, i.e. its provenance information. The IVOA Provenance Data Model shall record this information in a consistent and interoperable way for astronomical data.
Riebe, Kristin +5 more
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