Search Results - "Reis, R. C."
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Black hole accretion discs in the canonical low-hard state
Published in Monthly notices of the Royal Astronomical Society (21-02-2010)“…Stellar mass black holes in the low-hard state may hold clues to jet formation and basic accretion disc physics, but the nature of the accretion flow remains…”
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Broad line emission from iron K- and L-shell transitions in the active galaxy 1H 0707-495
Published in Nature (28-05-2009)“…Since the 1995 discovery of the broad iron K-line emission from the Seyfert galaxy MCG-6-30-15 (ref. 1), broad iron K lines have been found in emission from…”
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On the determination of the spin of the black hole in Cyg X-1 from X-ray reflection spectra
Published in Monthly notices of the Royal Astronomical Society (01-07-2012)“…The spin of Cygnus X-1 is measured by fitting reflection models to Suzaku data covering the energy band 0.9-400 keV. The inner radius of the accretion disc is…”
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4
A 200-Second Quasi-Periodicity After the Tidal Disruption of a Star by a Dormant Black Hole
Published in Science (American Association for the Advancement of Science) (24-08-2012)“…Supermassive black holes (SMBHs; mass is greater than or approximately 10 5 times that of the Sun) are known to exist at the center of most galaxies with…”
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A reflection origin for the soft and hard X-ray excess of Ark 120
Published in Monthly notices of the Royal Astronomical Society (01-01-2011)“…Over the last few years, several models have been proposed to interpret the widespread soft excess observed in the X-ray spectra of type 1 active galactic…”
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X-ray luminosities of optically selected cataclysmic variables and application to the Galactic ridge X-ray emission
Published in Monthly notices of the Royal Astronomical Society (11-04-2013)“…By studying Swift X-ray spectra of an optically selected, non-magnetic sample of nearby cataclysmic variables (CVs), we show that there is a population with…”
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Long XMM observation of the narrow-line Seyfert 1 galaxy IRAS 13224−3809: rapid variability, high spin and a soft lag
Published in Monthly notices of the Royal Astronomical Society (11-03-2013)“…The narrow-line Seyfert 1 galaxy IRAS 13224−3809 has been observed with XMM-Newton for 500 ks. The source is rapidly variable on time-scales down to a few 100…”
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Reflection from the strong gravity regime in a lensed quasar at redshift z = 0.658
Published in Nature (London) (13-03-2014)“…Observations of a gravitationally lensed quasar at redshift 0.658 imply a high spin parameter, which indicates that this supermassive black hole grew by…”
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Determining the spin of two stellar-mass black holes from disc reflection signatures
Published in Monthly notices of the Royal Astronomical Society (21-05-2009)“…We present measurements of the dimensionless spin parameters and inner-disc inclination of two stellar-mass black holes. The spin parameter of SWIFT…”
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Measuring the Spin of GRS 1915+105 with Relativistic Disk Reflection
Published in The Astrophysical journal (20-11-2009)“…GRS 1915+105 harbors one of the most massive known stellar black holes in the Galaxy. In 2007 May, we observed GRS 1915+105 for ~117 ks in the low/hard state…”
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Explaining the hard excesses in active galactic nuclei
Published in Monthly notices of the Royal Astronomical Society (11-10-2010)“…A common model invoked to describe the X-ray spectra of active galaxies includes a relativistically blurred reflection component, which in some cases can be…”
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A systematic look at the very high and low/hard state of GX 339−4: constraining the black hole spin with a new reflection model
Published in Monthly notices of the Royal Astronomical Society (11-07-2008)“…We present a systematic study of GX 339−4 in both its very high and low hard states from simultaneous observations made with XMM–Newton and RXTE in 2002 and…”
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Multistate observations of the Galactic black hole XTE J1752−223: evidence for an intermediate black hole spin
Published in Monthly notices of the Royal Astronomical Society (01-02-2011)“…The Galactic black hole candidate XTE J1752−223 was observed during the decay of its 2009 outburst with the Suzaku and XMM-Newton observatories. The observed…”
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SUZAKU OBSERVATION OF THE BLACK HOLE CANDIDATE MAXI J1836-194 IN A HARD/INTERMEDIATE SPECTRAL STATE
Published in The Astrophysical journal (20-05-2012)“…We report on a Suzaku observation of the newly discovered X-ray binary MAXI J1836-194. The source is found to be in the hard/intermediate spectral state and…”
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15
On Neutral Absorption and Spectral Evolution in X-Ray Binaries
Published in The Astrophysical journal (10-12-2009)“…Current X-ray observatories make it possible to follow the evolution of transient and variable X-ray binaries across a broad range in luminosity and source…”
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16
Artificial intelligence for skin cancer detection and classification for clinical environment: a systematic review
Published in Frontiers in medicine (08-01-2024)“…Skin cancer is one of the most common forms worldwide, with a significant increase in incidence over the last few decades. Early and accurate detection of this…”
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Spatial Model of Optimization Applied in the Distributed Generation Photovoltaic to Adjust Voltage Levels
Published in Energies (Basel) (01-11-2021)“…The main objective of this work is to develop a methodology for analyzing the quality of the voltage level in the distribution power grid to identify and…”
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Incidence of cardiovascular risk factors in female patients with systemic lupus erythematosus: a 3-year follow-up cohort
Published in Lupus (01-10-2018)“…Objectives To evaluate the incidence and variability of traditional coronary artery disease (CAD) risk factors in a cohort of lupus patients and to investigate…”
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Thermal emission from the stellar-mass black hole binary XTE J1118+480 in the low/hard state
Published in Monthly notices of the Royal Astronomical Society. Letters (01-05-2009)“…We report on the detection of a thermal disc component from the stellar-mass black hole binary XTE J1118+480 in the canonical low/hard state. The presence of a…”
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MULTI-WAVELENGTH COVERAGE OF STATE TRANSITIONS IN THE NEW BLACK HOLE X-RAY BINARY SWIFT J1910.2-0546
Published in The Astrophysical journal (01-04-2014)“…Understanding how black holes accrete and supply feedback to their environment is one of the outstanding challenges of modern astrophysics. Swift J1910.2-0546…”
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