M. Coriat - IRAP

M. Coriat
Are you M. Coriat?

Claim your profile, edit publications, add additional information:

Contact Details

M. Coriat

Pubs By Year

External Links

Pub Categories

High Energy Astrophysical Phenomena (32)
Astrophysics of Galaxies (5)
Cosmology and Nongalactic Astrophysics (3)
Instrumentation and Methods for Astrophysics (1)

Publications Authored By M. Coriat

Aims: This work is the first stage of a campaign to search for IMBHs, in low luminosity AGN (LLAGN) and dwarf galaxies. An additional, and equally important, aim of this pilot study is to investigate the consistency between the predictions of several BH scaling relations and the fundamental plane of black hole activity (FP-BH). Methods: We use X-ray and radio luminosity relations in accreting BHs, along with the latest scaling relations between the mass of the central black hole (MBH) and the properties of its host spheroid, to predict MBH in seven LLAGN, that were previously reported to be in the IMBH regime. Read More

X-ray binary observations led to the interpretation that powerful compact jets, produced in the hard state, are quenched when the source transitions to its soft state. The aim of this paper is to discuss the possibility that a powerful dark jet is still present in the soft state. Using the black hole X-ray binaries GX339-4 and H1743-322 as test cases, we feed observed X-ray power density spectra in the soft state of these two sources to an internal shock jet model. Read More

We study in detail the evolution of the 2015 outburst of GS 1354-64 (BW Cir) at optical, UV and X-ray wavelengths using Faulkes Telescope South/LCOGT, SMARTS and Swift. The outburst was found to stay in the hard X-ray state, albeit being anomalously luminous with a peak luminosity of L$_{X} >$ 0.15 L$_{Edd}$, which could be the most luminous hard state observed in a black hole X-ray binary. Read More

We want to test if self-similar magneto-hydrodynamic (MHD) accretion-ejection models can explain the observational results for accretion disk winds in BHBs. In our models, the density at the base of the outflow, from the accretion disk, is not a free parameter, but is determined by solving the full set of dynamical MHD equations without neglecting any physical term. Different MHD solutions were generated for different values of (a) the disk aspect ratio ($\varepsilon$) and (b) the ejection efficiency ($p$). Read More

Black hole X-ray binaries display large outbursts, during which their properties are strongly variable. We develop a systematic spectral analysis of the 3-40 keV RXTE/PCA data in order to study the evolution of these systems and apply it to GX 339-4. Using the low count rate observations, we provide a precise model of the Galactic background at GX 339-4's location and discuss its possible impact on the source spectral parameters. Read More

High resolution X-ray spectra of black hole X-ray binaries (BHBs) show blueshifted absorption lines from disk winds which seem to be equatorial. Winds occur in the Softer (disk-dominated) states of the outburst and are less prominent or absent in the Harder (power-law dominated) states. We use self-similar magneto-hydrodynamic (MHD) accretion-ejection models to explain the disk winds in BHBs. Read More

We report on a multiwavelength observational campaign of the black hole X-ray binary Swift J1753.5-0127 that consists of an ESO/X-shooter spectrum supported by contemporaneous Swift/XRT+UVOT and ATCA data. ISM absorption lines in the X-shooter spectrum allows us to determine E(B-V)=0. Read More

Affiliations: 1SSL/UCB, 2ESO and Harvard, 3Oxford, 4Curtin University, 5Caltech, 6Nagoya University, 7Hiroshima University, 8AIM and Observatoire de Paris, 9IRAP, 10University of Durham, 11University of Southampton, 12Caltech, 13Taiwan Normal University, 14University of Iowa, 15Sabanci University, 16Hiroshima University, 17ESAC, 18University of Michigan, 19Nagoya University and University of Tokyo, 20JPL, 21Nagoya University, 22National Central Univeristy

(abridged) We report on multi-wavelength measurements of Swift J1753.5-0127 in the hard state at L=2.7e36 erg/s (assuming d=3 kpc) in 2014. Read More

Thanks to the large collecting area (3 x ~1500 cm$^2$ at 1.5 keV) and wide field of view (30' across in full field mode) of the X-ray cameras on board the European Space Agency X-ray observatory XMM-Newton, each individual pointing can result in the detection of hundreds of X-ray sources, most of which are newly discovered. Recently, many improvements in the XMM-Newton data reduction algorithms have been made. Read More

Affiliations: 1ICRAR/Curtin University, 2ICRAR/Curtin University, 3ICRAR/Curtin University, 4ICRAR/Curtin University, 5U Southampton, 6AIM/CEA-Saclay, 7U Cape Town, 8NYU Abu Dhabi, 9NYU Abu Dhabi, 10U Alberta, 11ICRAR/Curtin University, 12INAF, 13Oxford University, 14U Wisconsin-Madison, 15SRON, 16NASA/GSFC, 17Radboud U, 18Wheaton College, 19U Amsterdam, 20Cambridge, 21U Barcelona, 22MIT, 23NRC, 24U Virginia, 25U Alberta, 26SRON, 27ISS, 28CSIRO

MAXI J1836-194 is a Galactic black hole candidate X-ray binary that was discovered in 2011 when it went into outburst. In this paper, we present the full radio monitoring of this system during its `failed' outburst, in which the source did not complete a full set of state changes, only transitioning as far as the hard intermediate state. Observations with the Karl G. Read More

This is a White Paper in support of the mission concept of the Large Observatory for X-ray Timing (LOFT), proposed as a medium-sized ESA mission. We discuss the potential of LOFT for the study of the physics of accretion and ejection around compact objects. For a summary, we refer to the paper. Read More

Affiliations: 1University of Cape Town, 2Joint Institute for VLBI in Europe, 3University of Oxford, 4University of Cape Town, 5Square Kilometre Array South Africa, 6FÖMI Satellite Geodetic Observatory, 7CSIRO Astronomy and Space Science, 8Max-Planck-Institut für Radioastronomie

Galaxies and supermassive black holes (SMBHs) are believed to evolve through a process of hierarchical merging and accretion. Through this paradigm, multiple SMBH systems are expected to be relatively common in the Universe. However, to date there are poor observational constraints on multiple SMBHs systems with separations comparable to a SMBH gravitational sphere of influence (<< 1 kpc). Read More

We present follow-up radio observations of ESO 243-49 HLX-1 from 2012 using the Australia Telescope Compact Array (ATCA) and the Karl G. Jansky Very Large Array (VLA). We report the detection of radio emission at the location of HLX-1 during its hard X-ray state using the ATCA. Read More

We characterized the broad-band X-ray spectra of Swift J1745-26 during the decay of the 2013 outburst using INTEGRAL ISGRI, JEM-X and Swift XRT. The X-ray evolution is compared to the evolution in optical and radio. We fit the X- ray spectra with phenomenological and Comptonization models. Read More

Affiliations: 1University of Cape Town, 2Joint Institute for VLBI in Europe, 3University of Oxford, 4University of Cape Town, 5Square Kilometre Array South Africa, 6University of Oxford, 7Satellite Geodetic Observatory, Institute of Geodesy, Cartography and Remote Sensing, 8CSIRO Astronomy and Space Science, 9Max-Planck-Institut für Radioastronomie, 10The University of Manchester, 11University of Cambridge

Galaxies are believed to evolve through merging, which should lead to multiple supermassive black holes in some. There are four known triple black hole systems, with the closest pair being 2.4 kiloparsecs apart (the third component is more distant at 3 kiloparsecs), which is far from the gravitational sphere of influence of a black hole with mass $\sim$10$^9$ M$_\odot$ (about 100 parsecs). Read More

Authors: R. P. J. Tilanus, T. P. Krichbaum, J. A. Zensus, A. Baudry, M. Bremer, H. Falcke, G. Giovannini, R. Laing, H. J. van Langevelde, W. Vlemmings, Z. Abraham, J. Afonso, I. Agudo, A. Alberdi, J. Alcolea, D. Altamirano, S. Asadi, K. Assaf, P. Augusto, A-K. Baczko, M. Boeck, T. Boller, M. Bondi, F. Boone, G. Bourda, R. Brajsa, J. Brand, S. Britzen, V. Bujarrabal, S. Cales, C. Casadio, V. Casasola, P. Castangia, J. Cernicharo, P. Charlot, L. Chemin, Y. Clenet, F. Colomer, F. Combes, J. Cordes, M. Coriat, N. Cross, F. D'Ammando, D. Dallacasa, J-F. Desmurs, R. Eatough, A. Eckart, D. Eisenacher, S. Etoka, M. Felix, R. Fender, M. Ferreira, E. Freeland, S. Frey, C. Fromm, L. Fuhrmann, K. Gabanyi, R. Galvan-Madrid, M. Giroletti, C. Goddi, J. Gomez, E. Gourgoulhon, M. Gray, I. di Gregorio, R. Greimel, N. Grosso, J. Guirado, K. Hada, A. Hanslmeier, C. Henkel, F. Herpin, P. Hess, J. Hodgson, D. Horns, E. Humphreys, B. Hutawarakorn Kramer, V. Ilyushin, V. Impellizzeri, V. Ivanov, M. Julião, M. Kadler, E. Kerins, P. Klaassen, K. van 't Klooster, E. Kording, M. Kozlov, M. Kramer, A. Kreikenbohm, O. Kurtanidze, J. Lazio, A. Leite, M. Leitzinger, J. Lepine, S. Levshakov, R. Lico, M. Lindqvist, E. Liuzzo, A. Lobanov, P. Lucas, K. Mannheim, J. Marcaide, S. Markoff, I. Martí-Vidal, C. Martins, N. Masetti, M. Massardi, K. Menten, H. Messias, S. Migliari, A. Mignano, J. Miller-Jones, D. Minniti, P. Molaro, S. Molina, A. Monteiro, L. Moscadelli, C. Mueller, A. Müller, S. Muller, F. Niederhofer, P. Odert, H. Olofsson, M. Orienti, R. Paladino, F. Panessa, Z. Paragi, T. Paumard, P. Pedrosa, M. Pérez-Torres, G. Perrin, M. Perucho, D. Porquet, I. Prandoni, S. Ransom, D. Reimers, M. Rejkuba, L. Rezzolla, A. Richards, E. Ros, A. Roy, A. Rushton, T. Savolainen, R. Schulz, M. Silva, G. Sivakoff, R. Soria-Ruiz, R. Soria, M. Spaans, R. Spencer, B. Stappers, G. Surcis, A. Tarchi, M. Temmer, M. Thompson, J. Torrelles, J. Truestedt, V. Tudose, T. Venturi, J. Verbiest, J. Vieira, P. Vielzeuf, F. Vincent, N. Wex, K. Wiik, T. Wiklind, J. Wilms, E. Zackrisson, H. Zechlin

Very long baseline interferometry at millimetre/submillimetre wavelengths (mmVLBI) offers the highest achievable spatial resolution at any wavelength in astronomy. The anticipated inclusion of ALMA as a phased array into a global VLBI network will bring unprecedented sensitivity and a transformational leap in capabilities for mmVLBI. Building on years of pioneering efforts in the US and Europe the ongoing ALMA Phasing Project (APP), a US-led international collaboration with MPIfR-led European contributions, is expected to deliver a beamformer and VLBI capability to ALMA by the end of 2014 (APP: Fish et al. Read More

As a complement to our optical and near-infrared study of the continuum properties of GX 339-4 in the two hard and one soft state observations made by the ESO/VLT FORS2 and ISAAC in early 2010, we report here on the results of our spectral line analysis for the same observations. In the soft state, the presence of strong Balmer, Paschen and Brackett emission lines points to the optical and near-infrared spectra stemming from the irradiated chromosphere of the optically thick and geometrically thin accretion disc. Most of these HI features are still detected in emission in both hard states but are veiled by the compact jets continuum. Read More

Understanding the dynamics behind black hole state transitions and the changes they reflect in outbursts has become long-standing problem. The X-ray reflection spectrum describes the interaction between the hard X-ray source (the power-law continuum) and the cool accretion disc it illuminates, and thus permits an indirect view of how the two evolve. We present a systematic analysis of the reflection spectrum throughout three outbursts (500+ observations) of the black hole binary GX 339-4, representing the largest study applying a self-consistent treatment of reflection to date. Read More

Recently, Diaz Trigo et al. reported an XMM-Newton detection of relativistically Doppler-shifted emission lines associated with steep-spectrum radio emission in the stellar-mass black hole candidate 4U 1630-47 during its 2012 outburst. They interpreted these lines as indicative of a baryonic jet launched by the accretion disk. Read More

Affiliations: 1Curtin/ICRAR, 2U Cape Town, 3Curtin/ICRAR, 4U Cape Town, 5CSIRO/CASS, 6U Alberta, 7U Cape Town, 8U Amsterdam, 9INAF/OAB, 10AIM/CEA-Saclay, 11U Southampton, 12Radboud U, 13USRA, 14U Amsterdam, 15U Barcelona, 16IAC, 17CSIRO/CASS, 18CSIRO/CASS

Swift J1745-26 is an X-ray binary towards the Galactic Centre that was detected when it went into outburst in September 2012. This source is thought to be one of a growing number of sources that display "failed outbursts", in which the self-absorbed radio jets of the transient source are never fully quenched and the thermal emission from the geometrically-thin inner accretion disk never fully dominates the X-ray flux. We present multifrequency data from the Very Large Array, Australia Telescope Compact Array and Karoo Array Telescope (KAT- 7) radio arrays, spanning the entire period of the outburst. Read More

The nature of accretion onto stellar mass black holes in the low/hard state remains unresolved, with some evidence suggesting that the inner accretion disc is truncated and replaced by a hot flow. However, the detection of relativistic broadened Fe emission lines, even at relatively low luminosities, seems to require an accretion disc extending fully to its innermost stable circular orbit. Modelling such features is however highly susceptible to degeneracies, which could easily bias any interpretation. Read More

Circinus X-1 is a bright and highly variable X-ray binary which displays strong and rapid evolution in all wavebands. Radio flaring, associated with the production of a relativistic jet, occurs periodically on a ~17-day timescale. A longer-term envelope modulates the peak radio fluxes in flares, ranging from peaks in excess of a Jansky in the 1970s to an historic low of milliJanskys during the years 1994 to 2007. Read More

Affiliations: 1University of Southampton, 2University of Southampton, 3University of Southampton, 4Max Planck Institute fur Extraterrestriche Physik, 5University of Southampton

We have systematically studied the effect of the orbital inclination in the outburst evolution of black hole transients. We have included all the systems observed by the Rossi X-ray timing explorer in which the thermal, accretion disc component becomes strongly dominant at some point of the outburst. Inclination is found to modify the shape of the tracks that these systems display in the colour/luminosity diagrams traditionally used for their study. Read More

Galactic black hole binaries produce powerful outflows with emit over almost the entire electromagnetic spectrum. Here, we report the first detection with the Herschel observatory of a variable far-infrared source associated with the compact jets of the black hole transient GX 339-4 during the decay of its recent 2010-2011 outburst, after the transition to the hard state. We also outline the results of very sensitive radio observations conducted with the Australia Telescope Compact Array, along with a series of near-infrared, optical (OIR) and X-ray observations, allowing for the first time the re-ignition of the compact jets to be observed over a wide range of wavelengths. Read More

The existing radio and X-ray flux correlation for Galactic black holes in the hard and quiescent states relies on a sample which is mostly dominated by two sources (GX 339-4 and V404 Cyg) observed in a single outburst. In this paper, we report on a series of radio and X-ray observations of the recurrent black hole GX 339-4 with the Australia Telescope Compact Array, the Rossi X-ray Timing Explorer and the Swift satellites. With our new long term campaign, we now have a total of 88 quasi-simultaneous radio and X-ray observations of GX 339-4 during its hard state, covering a total of seven outbursts over a 15--year period. Read More

We revisit a core prediction of the disc instability model (DIM) applied to X-ray binaries. The model predicts the existence of a critical mass transfer rate, which depends on disc size, separating transient and persistent systems. We therefore selected a sample of 52 persistent and transient neutron star and black hole X-ray binaries and verified if observed persistent (transient) systems do lie in the appropriate stable (unstable) region of parameter space predicted by the model. Read More

The microquasar GX 339-4, known to exhibit powerful compact jets that dominate its radio to near-infrared emission, entered an outburst in 2010 for the fifth time in about fifteen years. An extensive radio to X-ray multi-wavelength campaign was immediately triggered, and we report here on ESO/FORS2+ISAAC optical and near-infrared spectroscopic observations, supported by ATCA radio and RXTE/Swift X-ray quasi-simultaneous data. GX 339-4 was observed at three different epochs, once in the soft state and twice in the hard state. Read More

High resolution spectra of Galactic Black Holes (GBH) reveal the presence of highly ionised absorbers. In one GBH, accreting close to the Eddington limit for more than a decade, a powerful accretion disc wind is observed to be present in softer X-ray states and it has been suggested that it can carry away enough mass and energy to quench the radio jet. Here we report that these winds, which may have mass outflow rates of the order of the inner accretion rate or higher, are an ubiquitous component of the jet-free soft states of all GBH. Read More

Affiliations: 1ICRAR - Curtin, 2U. Alberta, 3U. Amsterdam, 4U. Southampton, 5U. Paris Diderot, 6NRAO, 7NASA/GSFC, 8MIT, 9NRAO, 10IAC, 11U. Southampton, 12U. Wisconsin-Madison, 13U. Nijmegen, 14U. Michigan, 15U. Amsterdam, 16U. Barcelona, 17U. Virginia, 18ASTRON

We present an intensive radio and X-ray monitoring campaign on the 2009 outburst of the Galactic black hole candidate X-ray binary H1743-322. With the high angular resolution of the Very Long Baseline Array, we resolve the jet ejection event and measure the proper motions of the jet ejecta relative to the position of the compact core jets detected at the beginning of the outburst. This allows us to accurately couple the moment when the jet ejection event occurred with X-ray spectral and timing signatures. Read More

In recent years, much effort has been devoted to unraveling the connection between the accretion flow and the jets in accreting compact objects. In the present work, we report new constraints on these issues, through the long term study of the radio and X-ray behaviour of the black hole candidate H1743-322. This source is known to be one of the `outliers' of the universal radio/X-ray correlation, i. Read More

We present the results of deep radio observations with the Australia Telescope Compact Array (ATCA) of the globular cluster NGC 6388. We show that there is no radio source detected (with a r.m. Read More

GX 339-4 has been one of the key sources for unravelling the accretion ejection coupling in accreting stellar mass black holes. After a long period of quiescence between 1999 and 2002, GX 339-4 underwent a series of 4 outbursts that have been intensively observed by many ground based observatories [radio, infrared(IR), optical] and satellites (X-rays). Here, we present results of these broad-band observational campaigns, focusing on the optical-IR (OIR)/X-ray flux correlations over the four outbursts. Read More

We investigate the early phase of the first state change during the 2008 September-November outburst of H1743-322, first detected by the INTEGRAL satellite. We analyse INTEGRAL, RXTE, Swift, and XMM/Newton observations, which provide coverage of the quiescence to outburst evolution in the 3-200 keV range every few days. The energy spectra are well fitted by a phenomenological model consisting of an exponentially cut-off power law plus a disc component. Read More