Publication data of Clavel, Maica: Link to Inspire

Created with Highcharts 9.0.1CitationsCitationsw/o self-citaionself-citaion2014201620182020202220240250500750100012501500
Created with Highcharts 9.0.1Publicationspublications per yearPublicationsPublications per yearCumulative publications2014201620182020202220240122436486001.534.567.5
Created with Highcharts 9.0.1h-indexh-indexh-indexh-index w/o self-citaion2014201620182020202220240510152025
Created with Highcharts 9.0.1CitationsBreakdown of Most Cited PapersrestThermally-Driven Disc Winds as a Mechanism for X-ray Irradiation Heating in Black Hole X-ray Binaries: The Case Study of GX339-4Thermally-Driven Disc Winds as a Mechanism for X-ray Irradiation Heating in …An X-ray survey of the central molecular zone: Variability of the Fe K$alpha$ emission lineAn X-ray survey of the central molecular zone: Variability of the Fe K$alpha$ …Dark jets in the soft X-ray state of black hole binaries?A unified accretion-ejection paradigm for black hole X-ray binaries. V. Low-frequency quasi-periodic oscillationsA unified accretion-ejection paradigm for black hole X-ray binaries. V. Low-fre…Glimpses of the past activity of Sgr $A^★$ inferred from X-ray echoes in Sgr CThe soft excess of the NLS1 galaxy Mrk 359 studied with an XMM-Newton-NuSTAR monitoring campaignThe soft excess of the NLS1 galaxy Mrk 359 studied with an XMM-Newton-Nu…A unified accretion-ejection paradigm for black hole X-ray binaries - IV. Replication of the 2010–2011 activity cycle of GX 339-4A unified accretion-ejection paradigm for black hole X-ray binaries - IV. Replic…Absorption lines from magnetically-driven winds in X-ray binariesA unified accretion-ejection paradigm for black hole X-ray binaries. II. Observational signatures of jet-emitting disksA unified accretion-ejection paradigm for black hole X-ray binaries. II. Observ…Hard X-ray Morphological and Spectral Studies of The Galactic Center Molecular Cloud Sgr B2: Constraining Past Sgr A* Flaring ActivityHard X-ray Morphological and Spectral Studies of The Galactic Center Molecul…The Intrinsic Two-Dimensional Size of Sagittarius A*A unified accretion-ejection paradigm for black hole X-ray binaries. III. Spectral signatures of hybrid disk configurationsA unified accretion-ejection paradigm for black hole X-ray binaries. III. Spectr…Evolution of the reverberation lag in GX 339–4 at the end of an outburstThe Evolution of GX 339-4 in the Low-hard State as Seen by NuSTAR and SwiftThe Evolution of GX 339-4 in the Low-hard State as Seen by NuSTAR and Swi…An X-ray chimney extending hundreds of parsecs above and below the Galactic CentreAn X-ray chimney extending hundreds of parsecs above and below the Galac…The XMM–Newton view of the central degrees of the Milky WayFifteen years of XMM–Newton and Chandra monitoring of Sgr A$^★$: evidence for a recent increase in the bright flaring rateFifteen years of XMM–Newton and Chandra monitoring of Sgr A$^★$: eviden…Echoes of multiple outbursts of Sagittarius A* revealed by ChandraAlternative explanations for extreme supersolar iron abundances inferred from the energy spectrum of Cygnus X-1Alternative explanations for extreme supersolar iron abundances inferred fro…201420162018202020222024025050075010001250
Created with Highcharts 9.0.1Fraction [%]Breakdown of Most Cited Papers (Fraction)Thermally-Driven Disc Winds as a Mechanism for X-ray Irradiation Heating in Black Hole X-ray Binaries: The Case Study of GX339-4Thermally-Driven Disc Winds as a Mechanism for X-ray Irradiation Heating in …An X-ray survey of the central molecular zone: Variability of the Fe K$alpha$ emission lineAn X-ray survey of the central molecular zone: Variability of the Fe K$alpha$ …Dark jets in the soft X-ray state of black hole binaries?A unified accretion-ejection paradigm for black hole X-ray binaries. V. Low-frequency quasi-periodic oscillationsA unified accretion-ejection paradigm for black hole X-ray binaries. V. Low-fre…Glimpses of the past activity of Sgr $A^★$ inferred from X-ray echoes in Sgr CThe soft excess of the NLS1 galaxy Mrk 359 studied with an XMM-Newton-NuSTAR monitoring campaignThe soft excess of the NLS1 galaxy Mrk 359 studied with an XMM-Newton-Nu…A unified accretion-ejection paradigm for black hole X-ray binaries - IV. Replication of the 2010–2011 activity cycle of GX 339-4A unified accretion-ejection paradigm for black hole X-ray binaries - IV. Replic…Absorption lines from magnetically-driven winds in X-ray binariesA unified accretion-ejection paradigm for black hole X-ray binaries. II. Observational signatures of jet-emitting disksA unified accretion-ejection paradigm for black hole X-ray binaries. II. Observ…Hard X-ray Morphological and Spectral Studies of The Galactic Center Molecular Cloud Sgr B2: Constraining Past Sgr A* Flaring ActivityHard X-ray Morphological and Spectral Studies of The Galactic Center Molecul…The Intrinsic Two-Dimensional Size of Sagittarius A*A unified accretion-ejection paradigm for black hole X-ray binaries. III. Spectral signatures of hybrid disk configurationsA unified accretion-ejection paradigm for black hole X-ray binaries. III. Spectr…Evolution of the reverberation lag in GX 339–4 at the end of an outburstThe Evolution of GX 339-4 in the Low-hard State as Seen by NuSTAR and SwiftThe Evolution of GX 339-4 in the Low-hard State as Seen by NuSTAR and Swi…An X-ray chimney extending hundreds of parsecs above and below the Galactic CentreAn X-ray chimney extending hundreds of parsecs above and below the Galac…The XMM–Newton view of the central degrees of the Milky WayFifteen years of XMM–Newton and Chandra monitoring of Sgr A$^★$: evidence for a recent increase in the bright flaring rateFifteen years of XMM–Newton and Chandra monitoring of Sgr A$^★$: eviden…Echoes of multiple outbursts of Sagittarius A* revealed by ChandraAlternative explanations for extreme supersolar iron abundances inferred from the energy spectrum of Cygnus X-1Alternative explanations for extreme supersolar iron abundances inferred fro…2014201620182020202220240255075100
Created with Highcharts 9.0.1Citations/1 YearCitations/PeriodCitations / 1 YearMoving average201420162018202020222024050100150200250