Generalized quantum Zernike Hamiltonians admit a polynomial Higgs-type algebra yielding a deformed oscillator whose structure function factors, allowing algebraic energy spectra for N=1 to 5 with conjectures for all N.
Physica , year = 1934, month = may, volume =
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Bulgeless galaxies trace the upper envelope of the mass-R1 relation with scatter driven by central stellar density and the spatial configuration of mergers rather than their number.
Edge discontinuities in coadds cause significant shear biases only in extreme cases such as two-input-image stacks or 25% PSF size jumps, and these cases can be flagged and removed with a simple PSF variation statistic.
A method to generate realistic virtual mirror maps from measured data enables systematic evaluation of surface specifications for the Einstein Telescope's optical performance.
citing papers explorer
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Generalized quantum Zernike Hamiltonians: Polynomial Higgs-type algebras and algebraic derivation of the spectrum
Generalized quantum Zernike Hamiltonians admit a polynomial Higgs-type algebra yielding a deformed oscillator whose structure function factors, allowing algebraic energy spectra for N=1 to 5 with conjectures for all N.
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Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies
Bulgeless galaxies trace the upper envelope of the mass-R1 relation with scatter driven by central stellar density and the spatial configuration of mergers rather than their number.
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Edges In Coadded Images
Edge discontinuities in coadds cause significant shear biases only in extreme cases such as two-input-image stacks or 25% PSF size jumps, and these cases can be flagged and removed with a simple PSF variation statistic.
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Mirror Surface Evaluation for the Einstein Telescope Using Virtual Mirror Maps
A method to generate realistic virtual mirror maps from measured data enables systematic evaluation of surface specifications for the Einstein Telescope's optical performance.