activity
20082024
most citedNitrogen K-shell photoabsorption

49 citations · 298 across the 17 of their papers we have counts for

collaborators

17 papers

astro-ph.IM2024★ 1 cited

The first cut is the cheapest: optimizing Athena/X-IFU-like TES detectors resolution by filter truncation

M. Teresa Ceballos, Nicolás Cardiel, Beatriz Cobo +4

The X-ray Integral Field Unit (X-IFU) instrument on the future ESA mission Athena X-ray Observatory is a cryogenic micro-calorimeter array of Transition Edge Sensor (TES) detectors…

astro-ph.IM2022★ 1 cited

XSLIDE (X-Ray Spectral Line IDentifier and Explorer): a quick-look tool for XRISM

Efrem Braun, Chris Baluta, Trisha F. Doyle +7

We present XSLIDE (X-Ray Spectral Line IDentifier and Explorer), a graphical user interface that has been designed as a quick-look tool for the upcoming X-Ray Imaging and Spectrosc…

astro-ph.IM2020

The XSTAR Atomic Database

Claudio Mendoza, Manuel A. Bautista, Jérôme Deprince +7

We describe the atomic database of the XSTAR spectral modeling code, summarizing the systematic upgrades carried out in the past twenty years to enable the modeling of K lines from…

astro-ph.IM2019★ 12 cited

Towards 100,000-pixel microcalorimeter arrays using multi-absorber transition-edge sensors

S. J. Smith, J. S. Adams, S. R. Bandler +15

We report on the development of multi-absorber transition edge sensors (TESs), referred to as hydras. A hydra consists of multiple x-ray absorbers each with a different thermal con…

physics.atom-ph2018★ 6 cited

K-shell photoabsorption and photoionization of trace elements. III. Isoelectronic sequences with electron number

C. Mendoza, M. A. Bautista, P. Palmeri +3

This is the final report of a three-paper series on the K-shell photoabsorption and photoionization of trace elements, namely F, Na, P, Cl, K, Sc, Ti, V, Cr, Mn, Co, Cu and Zn. K l…

astro-ph.IM2017★ 6 cited

K-shell photoabsorption and photoionization of trace elements. II. Isoelectronic sequences with electron number

C. Mendoza, M. A. Bautista, P. Palmeri +3

We are concerned with improving the diagnostic potential of the K lines and edges of elements with low cosmic abundances that are observed in the X-ray spectra of supernova remnant…