ROSSINI achieves integral field spectroscopy without IFUs via rotational slitless imaging combined with tomographic reconstruction, recovering input datacubes to percent-level accuracy in numerical simulations.
Astronomical Journal , year = 1974, month = jun, volume =
11 Pith papers cite this work, alongside 3,843 external citations. Polarity classification is still indexing.
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citation-polarity summary
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astro-ph.IM 3 astro-ph.GA 2 astro-ph.HE 2 astro-ph.SR 1 cond-mat.mtrl-sci 1 eess.IV 1 physics.ao-ph 1roles
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use method 1representative citing papers
Soft X-ray emission from SN 1987A's equatorial ring becomes broader and extends inward after ~2012, while hard X-rays remain compact, indicating growing contribution from reverse-shock-heated interior material.
Defines path-signature descriptors for spectral line profiles and shows they enable unsupervised clustering of MaNGA Hα spaxels into spatially coherent classes whose stacked spectra recover large-scale velocity patterns.
MUSE observations of Tc 1 map structured extinction, Te, and Ne, revealing a low-extinction annulus outside the main fullerene zone that is interpreted as evidence for locally altered dust properties in the core-halo transition.
SPHEREx provides global maps of HeI 10830, OI 8446, and OI 11287 airglow showing temporal and geographic variability linked to solar and seasonal effects.
An integrated UHV MBE-plus-optical-spectroscopy cluster enables in-situ, spatially resolved photoluminescence and Raman measurements on as-grown reactive 2D semiconductors while preserving pristine surfaces.
ALMA CO observations of NGC 4565 reveal a thin non-flaring molecular disk with a central gap, consistent GMC properties to 17 kpc, and a prominent star-forming ring feature.
HazeMatching adapts conditional flow matching with hazy-image guidance to dehaze microscopy images while balancing fidelity and realism on synthetic and real data.
Presents a non-negativity constrained iterative deconvolution method for SKA radio images that is fast and performs well on simulated point and extended sources in noise-free conditions.
Theoretical predictions for local BBH merger rates exceed observations by a factor >10 under conservative SFRD and metallicity assumptions, indicating need for revisions in stellar evolution.
NGC 4264 hosts a fast bar with rotation rate R_cor/a_bar = 0.88 measured via the Tremaine-Weinberg method on MUSE data, indicating internal formation despite ongoing weak interaction.
citing papers explorer
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Integral field spectroscopy with no IFUs: combining wide-field rotational slitless spectroscopy with tomographic reconstruction
ROSSINI achieves integral field spectroscopy without IFUs via rotational slitless imaging combined with tomographic reconstruction, recovering input datacubes to percent-level accuracy in numerical simulations.
-
Chandra X-Ray Imaging and Spatially Resolved Spectroscopy of SN 1987A: Energy-Dependent Morphology of the Equatorial Ring
Soft X-ray emission from SN 1987A's equatorial ring becomes broader and extends inward after ~2012, while hard X-rays remain compact, indicating growing contribution from reverse-shock-heated interior material.
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The Hidden Geometry of Astrophysical Spectra: Path-Signatures of Line Profiles
Defines path-signature descriptors for spectral line profiles and shows they enable unsupervised clustering of MaNGA Hα spaxels into spatially coherent classes whose stacked spectra recover large-scale velocity patterns.
-
MUSE Imaging Spectroscopy of the Fullerene Planetary Nebula Tc 1
MUSE observations of Tc 1 map structured extinction, Te, and Ne, revealing a low-extinction annulus outside the main fullerene zone that is interpreted as evidence for locally altered dust properties in the core-halo transition.
-
Observations of Atmospheric Helium and Oxygen with SPHEREx
SPHEREx provides global maps of HeI 10830, OI 8446, and OI 11287 airglow showing temporal and geographic variability linked to solar and seasonal effects.
-
Ultra-high-vacuum cluster tool for epitaxial synthesis and optical spectroscopy of reactive 2D materials
An integrated UHV MBE-plus-optical-spectroscopy cluster enables in-situ, spatially resolved photoluminescence and Raman measurements on as-grown reactive 2D semiconductors while preserving pristine surfaces.
-
The Radial and Vertical Structure of Molecular Gas in the Edge-On Galaxy NGC 4565
ALMA CO observations of NGC 4565 reveal a thin non-flaring molecular disk with a central gap, consistent GMC properties to 17 kpc, and a prominent star-forming ring feature.
-
HazeMatching: Dehazing Light Microscopy Images with Guided Conditional Flow Matching
HazeMatching adapts conditional flow matching with hazy-image guidance to dehaze microscopy images while balancing fidelity and realism on synthetic and real data.
-
A Non-Negativity Iterative Approach to Image Deconvolution for SKA
Presents a non-negativity constrained iterative deconvolution method for SKA radio images that is fast and performs well on simulated point and extended sources in noise-free conditions.
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Can current models predict the local black hole merger rate?
Theoretical predictions for local BBH merger rates exceed observations by a factor >10 under conservative SFRD and metallicity assumptions, indicating need for revisions in stellar evolution.
-
Evidence of a fast bar in the weakly-interacting galaxy NGC 4264 with MUSE
NGC 4264 hosts a fast bar with rotation rate R_cor/a_bar = 0.88 measured via the Tremaine-Weinberg method on MUSE data, indicating internal formation despite ongoing weak interaction.