144 citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- Saint Mary's UniversityCA4 papers
- California Institute of TechnologyUS3 papers
- Center for Astrophysics Harvard & SmithsonianUS3 papers
- Centre National de la Recherche ScientifiqueFR3 papers
- University of CambridgeGB3 papers
- University of MichiganUS3 papers
- Astronomy and SpaceAU2 papers
- Heidelberg UniversityDE2 papers
- Jet Propulsion LaboratoryUS2 papers
- Leiden UniversityNL2 papers
- Max Planck Institute for Radio AstronomyDE2 papers
- National Institute for AstrophysicsIT2 papers
9 papers
XMM-Newton multi-year campaign on NGC 55 ULX-1: Resolving the wind and its variability with RGS
C. Pinto, S. Caserta, F. Barra +12
Winds are an important ingredient in the evolution of X-ray binary (XRB) systems, particularly those at high accretion rates such as ultra-luminous X-ray sources (ULXs), because th…
XRISM/Resolve Spectroscopy of the Central Engine in the Seyfert-1 AGN Mrk 279
Jon M. Miller, Xin Xiang, Doyee Byun +9
High-resolution X-ray spectroscopy with XRISM gives an unprecedented view of the ``central engine'' in active galactic nuclei, providing unique insights into black hole accretion a…
Impact of stochastic star-formation histories and dust on selecting quiescent galaxies with JWST photometry
K. Lisiecki, D. Donevski, A. W. S. Man +16
While the James Webb Space Telescope (JWST) now allows identifying quiescent galaxies (QGs) out to early epochs, the photometric selection of quiescent galaxy candidates (QGCs) and…
Structural evolution of quiescent galaxies at intermediate redshifts at UV and red rest-frame wavelengths
Michele Pizzardo, Ivana Damjanov, Jubee Sohn +1
We model the wavelength dependence of structural parameters for a mass-limited sample () of quiescent galaxies with using $griz…
XRISM Reveals a Remnant Torus in the Low-Luminosity AGN M81*
Jon M. Miller, Ehud Behar, Hisamitsu Awaki +10
Up to 40% of galaxies in the local universe host a low-luminosity active galactic nucleus (LLAGN), making it vital to understand this mode of black hole accretion. However, the pre…
Intracluster light in the core of z~2 galaxy proto-clusters
S. V. Werner, N. A. Hatch, J. Matharu +5
Intracluster light is thought to originate from stars that were ripped away from their parent galaxies by gravitational tides and galaxy interactions during the build up of the clu…
Modelling the Extreme X-ray Spectrum of IRAS 13224-3809
Chia-Ying Chiang, D. J. Walton, A. C. Fabian +2
The extreme NLS1 galaxy IRAS 13224-3809 shows significant variability, frequency depended time lags, and strong Fe K line and Fe L features in the long 2011 XMM-Newton observation.…
The NuSTAR spectrum of Mrk 335: Extreme relativistic effects within 2 gravitational radii of the event horizon?
M. L. Parker, D. R. Wilkins, A. C. Fabian +18
We present 3-50 keV NuSTAR observations of the AGN Mrk 335 in a very low flux state. The spectrum is dominated by very strong features at the energies of the iron line at 5-7 keV a…
Structure of 55Ti from relativistic one-neutron knockout
P. Maierbeck, R. Gernhäuser, R. Krücken +62
Results are presented from a one-neutron knockout reaction at relativistic energies on 56Ti using the GSI FRS as a two-stage magnetic spectrometer and the Miniball array for gamma-…