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.
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8 Pith papers cite this work, alongside 95 external citations. Polarity classification is still indexing.
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Multi-epoch stellar occultations reveal Quaoar is an oblate spheroid with density 1.760±0.109 g/cm³, consistent with Maclaurin hydrostatic equilibrium and dwarf planet status.
X-ray timing and spectral analysis of ASKAP J174508.9-505149 detects matching periodicity and features consistent with an accreting magnetic CV.
High-speed imaging of four lunar impact flashes reveals lower variance in initial intensity than total energy and no correlation between them, suggesting decoupled vapor and ejecta phases.
The asteroid 2022 OB5 rotates every 1.542 minutes, making surface operations impractical despite its favorable orbit.
The paper reports the design, commissioning on two runs, and measured performance of proto-Lightspeed, a seeing-limited high-speed imager delivering sub-electron read noise on the Magellan Clay Telescope.
Optical imaging and BAGPIPES SED fitting of eight FXTs yields candidate hosts consistent with WD-IMBH TDEs or BNS mergers for most events, with one reclassified as a Galactic flare and evidence for diverse origins.
Discovery of an eclipsing neutron star LMXB with clocked bursts, orbital period 6.483 hr, companion mass 0.6-0.8 Msun, and helium burst indications from energy ratio 120-130.
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.
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Size, shape, density, and atmospheric limit of (50000) Quaoar revealed from 14 years of stellar occultation
Multi-epoch stellar occultations reveal Quaoar is an oblate spheroid with density 1.760±0.109 g/cm³, consistent with Maclaurin hydrostatic equilibrium and dwarf planet status.
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The X-ray emission of the long-period transient and accreting cataclysmic variable ASKAP J174508.9-505149
X-ray timing and spectral analysis of ASKAP J174508.9-505149 detects matching periodicity and features consistent with an accreting magnetic CV.
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High-Speed Observations of Lunar Impact Flashes
High-speed imaging of four lunar impact flashes reveals lower variance in initial intensity than total energy and no correlation between them, suggesting decoupled vapor and ejecta phases.
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Accessible does not mean exploitable: HiPERCAM reveals the ultra-fast rotation of 2022 OB$_5$
The asteroid 2022 OB5 rotates every 1.542 minutes, making surface operations impractical despite its favorable orbit.
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proto-Lightspeed: a high-speed, ultra-low read noise imager on the Magellan Clay Telescope
The paper reports the design, commissioning on two runs, and measured performance of proto-Lightspeed, a seeing-limited high-speed imager delivering sub-electron read noise on the Magellan Clay Telescope.
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Optical observations of candidate host galaxies of eight fast X-ray transients
Optical imaging and BAGPIPES SED fitting of eight FXTs yields candidate hosts consistent with WD-IMBH TDEs or BNS mergers for most events, with one reclassified as a Galactic flare and evidence for diverse origins.
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Einstein Probe discovery of EP J171159.4-333253: an eclipsing neutron star low-mass X-ray binary with clocked bursts
Discovery of an eclipsing neutron star LMXB with clocked bursts, orbital period 6.483 hr, companion mass 0.6-0.8 Msun, and helium burst indications from energy ratio 120-130.