Search Results - "Kaaret, P."
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Enhanced X-ray emission from Lyman break analogues and a possible LX-SFR-metallicity plane
Published in Monthly notices of the Royal Astronomical Society (01-04-2016)“…The source of energetic photons that heated and reionized the early Universe remains uncertain. Early galaxies had low metallicity and recent population…”
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X-ray binary formation in low-metallicity blue compact dwarf galaxies
Published in Monthly notices of the Royal Astronomical Society (01-07-2014)“…X-rays from binaries in small, metal-deficient galaxies may have contributed significantly to the heating and reionization of the early Universe. We…”
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Observations of Magnetospheric Solar Wind Charge Exchange
Published in The Astrophysical journal (01-10-2023)“…Abstract The study of solar wind charge exchange (SWCX) emission is vital to both the X-ray astrophysics and heliophysics communities. SWCX emission…”
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Effects of metallicity on high-mass X-ray binary formation
Published in Monthly notices of the Royal Astronomical Society (01-01-2020)“…ABSTRACT The heating of the intergalactic medium in the early, metal-poor Universe may have been partly due to radiation from high-mass X-ray binaries (HMXBs)…”
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Enhanced X-ray emission from candidate Lyman continuum emitting galaxies
Published in Monthly notices of the Royal Astronomical Society (11-08-2019)“…ABSTRACT X-ray binaries may have helped reionize the early Universe by enabling Lyman continuum escape. We analysed a set of eight local galaxies that are…”
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A Disc-Dominated and Clumpy Circumgalactic Medium of the Milky Way Seen in X-Ray Emission
Published in Nature astronomy (19-10-2020)“…The Milky Way galaxy is surrounded by a circumgalactic medium (CGM) that may play a key role in galaxy evolution as the source of gas for star formation and a…”
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Revisiting the radio/X-ray flux correlation in the black hole V404 Cyg: from outburst to quiescence
Published in Monthly notices of the Royal Astronomical Society (01-10-2008)“…We report results of Chandra X-ray and Very Large Array (VLA) radio observations of the Galactic accreting black hole V404 Cyg (GS 2023+338) in its quiescent…”
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Rapid turn-on of a luminous X-ray source in the candidate Lyman continuum emitting galaxy Tol 0440-381
Published in Monthly notices of the Royal Astronomical Society. Letters (01-03-2022)“…ABSTRACT Chandra observations of the nearby candidate Lyman continuum (LyC) emitting galaxy Tol 0440-381 show brightening of an X-ray source by at least a…”
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THE 2015 DECAY OF THE BLACK HOLE X-RAY BINARY V404 CYGNI: ROBUST DISK-JET COUPLING AND A SHARP TRANSITION INTO QUIESCENCE
Published in The Astrophysical journal (10-01-2017)“…ABSTRACT We present simultaneous X-ray and radio observations of the black hole X-ray binary V404 Cygni at the end of its 2015 outburst. From 2015 July…”
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Observations of the Disk/Jet Coupling of MAXI J1820+070 during Its Descent to Quiescence
Published in The Astrophysical journal (01-01-2021)“…Black hole X-ray binaries in the quiescent state (Eddington ratios typically 10−5) display softer X-ray spectra (photon indices Γ ∼ 2) compared to…”
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A Search for the 3.5 keV Line from the Milky Way’s Dark Matter Halo with HaloSat
Published in The Astrophysical journal (01-07-2021)“…Previous detections of an X-ray emission line near 3.5 keV in galaxy clusters and other dark-matter-dominated objects have been interpreted as observational…”
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OPTICAL EMISSION OF THE ULTRALUMINOUS X-RAY SOURCE NGC 5408 X-1: DONOR STAR OR IRRADIATED ACCRETION DISK?
Published in The Astrophysical journal (01-02-2012)“…We obtained three epochs of simultaneous Hubble Space Telescope (HST)/Wide Field Camera 3 and Chandra observations of the ultraluminous X-ray source (ULX) NGC…”
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VERITAS Observations of the Galactic Center Region at Multi-TeV Gamma-Ray Energies
Published in The Astrophysical journal (01-06-2021)“…Abstract The Galactic Center (GC) region hosts a variety of powerful astronomical sources and rare astrophysical processes that emit a large flux of nonthermal…”
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The black hole candidate XTE J1752−223 towards and in quiescence: optical and simultaneous X-ray-radio observations
Published in Monthly notices of the Royal Astronomical Society (01-07-2012)“…We present optical, X-ray and radio observations of the black hole transient (BHT) XTE J1752−223 towards and in quiescence. Optical photometry shows that the…”
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A multi-wavelength view of distinct accretion regimes in the pulsating ultraluminous X-ray source NGC 1313 X-2
Published in Monthly notices of the Royal Astronomical Society (07-03-2022)“…ABSTRACT NGC 1313 X-2 is one of the few known pulsating ultraluminous X-ray sources (PULXs), and so is thought to contain a neutron star that accretes at…”
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Transition of an X-ray binary to the hard ultraluminous state in the blue compact dwarf galaxy VII Zw 403
Published in Monthly notices of the Royal Astronomical Society (21-04-2015)“…We examine the X-ray spectra of VII Zw 403, a nearby low-metallicity blue compact dwarf (BCD) galaxy. The galaxy has been observed to contain an X-ray source,…”
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HaloSat Observations of Heliospheric Solar Wind Charge Exchange
Published in The Astrophysical journal (06-09-2021)“…X-ray emission from solar wind charge exchange (SWCX) produced in interplanetary space contaminates every astrophysical observation, regardless of the…”
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A long-term X-ray monitoring of the ultraluminous X-ray source NGC 5408 X-1 with Swift reveals the presence of dips but no orbital period
Published in Monthly notices of the Royal Astronomical Society (01-08-2013)“…NGC 5408 X-1 is a well-studied ultraluminous X-ray source (ULX) that has been seen to emit in X-rays persistently above the Eddington limit of a stellar mass…”
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Measurement of the Extragalactic Background Light Spectral Energy Distribution with VERITAS
Published in The Astrophysical journal (10-11-2019)“…The extragalactic background light (EBL), a diffuse photon field in the optical and infrared range, is a record of radiative processes over the universe's…”
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Gamma-ray Observations of Tycho's Supernova Remnant with VERITAS and Fermi
Published in The Astrophysical journal (10-02-2017)“…High-energy gamma-ray emission from supernova remnants (SNRs) has provided a unique perspective for studies of Galactic cosmic-ray acceleration. Tycho's SNR is…”
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