A new compact hierarchical triple main-sequence star system G1010 was discovered through combined low- and high-SNR spectroscopy, Gaia DR3 data, and TESS light curve analysis, showing an inner eclipsing binary rather than a compact object companion.
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2 Pith papers cite this work. Polarity classification is still indexing.
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New calibration data from white dwarf standards show no significant sensitivity offset between ACS/WFC chips in F606W and F814W, contradicting a prior 0.05 mag global difference.
citing papers explorer
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Discovery of a compact hierarchical triple main-sequence star system while searching for binary stars with compact objects
A new compact hierarchical triple main-sequence star system G1010 was discovered through combined low- and high-SNR spectroscopy, Gaia DR3 data, and TESS light curve analysis, showing an inner eclipsing binary rather than a compact object companion.
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Investigating ACS/WFC Amp-to-Amp Sensitivities
New calibration data from white dwarf standards show no significant sensitivity offset between ACS/WFC chips in F606W and F814W, contradicting a prior 0.05 mag global difference.