RefleX provides a flexible Monte Carlo code for X-ray reprocessing in quasi-arbitrary geometries around AGN, validated against pexrav/MYTorus/BNTorus, with released RXTorus torus model showing bound-electron effects on NGC 424 fits.
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6 Pith papers cite this work. Polarity classification is still indexing.
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XRISM data on NGC 1068 indicates neutral Fe K fluorescence originates in optically thin gas and ionized lines trace a fast outflow, implying complex geometry in this Compton-thick AGN.
Reddening maps of the LMC and SMC are produced via SED fitting of RGB stars from SMASH and VMC photometry, yielding mean E(B-V) of 0.076 mag and 0.058 mag with relative spatial structure stable across three stellar atmosphere models but absolute values differing by up to 0.03 mag.
Veiling-corrected lithium abundances in eight young clusters peak at 3.3-3.8 dex with upper age limits of ~5 Myr, alongside slightly sub-solar iron and barium overabundances up to 0.75 dex.
Simulations show that iterative source removal and maximum likelihood decoding can recover point-source positions and fluxes from 1.5D coded-aperture data with 5-arcmin resolution in one axis and 5-degree resolution in the other.
A catalog of 251 soft X-ray counterparts for 250 unassociated Swift-BAT hard X-ray sources classifies 94 as AGN and 58 as galaxies with supporting redshift and limited optical data.
citing papers explorer
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RefleX: X-ray absorption and reflection in active galactic nuclei for arbitrary geometries
RefleX provides a flexible Monte Carlo code for X-ray reprocessing in quasi-arbitrary geometries around AGN, validated against pexrav/MYTorus/BNTorus, with released RXTorus torus model showing bound-electron effects on NGC 424 fits.
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A XRISM view of the iron line complex in NGC 1068: Rethinking the prototypical Compton-thick AGN
XRISM data on NGC 1068 indicates neutral Fe K fluorescence originates in optically thin gas and ionized lines trace a fast outflow, implying complex geometry in this Compton-thick AGN.
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Reddening maps of the Magellanic Clouds using spectral energy distribution fitting of red giants
Reddening maps of the LMC and SMC are produced via SED fitting of RGB stars from SMASH and VMC photometry, yielding mean E(B-V) of 0.076 mag and 0.058 mag with relative spatial structure stable across three stellar atmosphere models but absolute values differing by up to 0.03 mag.
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PENELLOPE: IX. Lithium, iron and barium elemental abundances in eight nearby young clusters
Veiling-corrected lithium abundances in eight young clusters peak at 3.3-3.8 dex with upper age limits of ~5 Myr, alongside slightly sub-solar iron and barium overabundances up to 0.75 dex.
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Simulations of a 2 x 1.5D coded aperture camera for X-ray astronomy
Simulations show that iterative source removal and maximum likelihood decoding can recover point-source positions and fluxes from 1.5D coded-aperture data with 5-arcmin resolution in one axis and 5-degree resolution in the other.
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Source identification for the Swift-BAT 150-month hard X-ray catalog using soft X-ray observations
A catalog of 251 soft X-ray counterparts for 250 unassociated Swift-BAT hard X-ray sources classifies 94 as AGN and 58 as galaxies with supporting redshift and limited optical data.