activity
20162022
most citedProbing the structure of the gas in the Milky Way through X-ray high resolution spectroscopy

37 citations · 99 across the 8 of their papers we have counts for

collaborators
Showing 2018Show all

6 papers · 1 filter

astro-ph.HE2018

The Soft-Excess in Mrk 509: Warm Corona or Relativistic Reflection?

Javier A. Garcia, Erin Kara, Dominic Walton +15

We present the analysis of the first NuSTAR observations ( ks), simultaneous with the last SUZAKU observations ( ks), of the active galactic nucleus of the brigh…

astro-ph.HE2018

On the discrepancy between the X-ray and UV absorption measurements of OVI in the local ISM

Efraín Gatuzz, Javier A. García, Timothy R. Kallman

The total amount of OVI present in the interstellar medium (ISM) obtained via absorption measurements in UV and X-ray spectra is currently in disagreement, with the latter being si…

astro-ph.HE2018

Chandra high-resolution spectra of 4U~1630-47: the disappearance of the wind

E. Gatuzz, M. Diaz Trigo, J. C. A. Miller-Jones +1

We present the analysis of six {\it Chandra} X-ray high-resolution observations of the black hole low-mass X-ray binary 4U~1630-47 taken during its 2012-2013 outburst. {\rm Fe}~{\s…

astro-ph.HE2018

3D mapping of the neutral X-ray absorption in the local interstellar medium: The Gaia and XMM-Newton synergy

Efraín Gatuzz, S. Rezaei Kh., Timothy R. Kallman +4

We present a three-dimensional map of the hydrogen density distribution in the Galactic interstellar medium. The hydrogen equivalent column densities were obtained from the Explori…

astro-ph.HE2018

What we learn from the X-ray grating spectra of Nova SMC 2016

M. Orio, J. -U. Ness, A. Dobrotka +17

Nova SMC 2016 has been the most luminous nova known in the direction of the Magellanic Clouds. It turned into a very luminous supersoft X-ray source between day 16 and 28 after the…

astro-ph.HE2018

Carbon X-ray absorption in the local ISM: fingerprints in X-ray Novae spectra

E. Gatuzz, J. -U. Ness, T. W. Gorczyca +3

We present a study of the C K-edge using high-resolution LETGS Chandra spectra of four novae during their super-soft-source (SSS) phase. We identified absorption lines due to C~ii…