Publication data of Cruz, Marcos: Link to Inspire

Created with Highcharts 9.0.1CitationsCitationsw/o self-citaionself-citaion1995200020052010201520202025025050075010001250
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Created with Highcharts 9.0.1CitationsBreakdown of Most Cited PapersrestOstrogradsky–Hamilton approach to geodetic brane gravityClassical relativistic spinning particle with anomalous magnetic moment: The Precession of spinClassical relativistic spinning particle with anomalous magnetic moment: The…Unexplained correlation between the Cosmic Microwave Background temperature and the local matter density distributionUnexplained correlation between the Cosmic Microwave Background temper…Effective Field Equations of Brane-Induced ElectromagnetismUsing CMB polarization to constrain the anomalous nature of the Cold Spot with an incomplete sky-coverageUsing CMB polarization to constrain the anomalous nature of the Cold Spot w…Phantom cosmology with a decaying cosmological parameter Lambda(t) induced from five-dimensional (5D) geometrical vacuumPhantom cosmology with a decaying cosmological parameter Lambda(t) ind…Near-infrared K-band imaging of a sample of ultra-steep-spectrum radio sources selected at 74 MHzNear-infrared K-band imaging of a sample of ultra-steep-spectrum radio sourc…WMAP anomalous signal in the ecliptic planeBianchi VII_h models and the cold spot textureCMB polarization as a probe of the anomalous nature of the Cold SpotThe 6C** sample of steep-spectrum radio sources. 2. Redshift distribution and the space density of high-redshift radio galaxiesThe 6C** sample of steep-spectrum radio sources. 2. Redshift distribution an…The 6C** sample of steep-spectrum radio sources. 1. Radio data, near-infrared imaging and optical spectroscopyThe 6C** sample of steep-spectrum radio sources. 1. Radio data, near-infrare…The WMAP cold spotAnomalous variance in the WMAP data and Galactic Foreground residualsThe CMB cold spot: texture, cluster or void?A Cosmic Microwave Background feature consistent with a cosmic textureThe non-gaussian cold spot in wmap: significance, morphology and foreground contributionThe non-gaussian cold spot in wmap: significance, morphology and foregrou…The non-gaussian cold spot in the 3-year wmap dataDetection of a non-gaussian spot in wmap1995200020052010201520202025025050075010001250
Created with Highcharts 9.0.1Fraction [%]Breakdown of Most Cited Papers (Fraction)Ostrogradsky–Hamilton approach to geodetic brane gravityClassical relativistic spinning particle with anomalous magnetic moment: The Precession of spinClassical relativistic spinning particle with anomalous magnetic moment: The…Unexplained correlation between the Cosmic Microwave Background temperature and the local matter density distributionUnexplained correlation between the Cosmic Microwave Background temper…Effective Field Equations of Brane-Induced ElectromagnetismUsing CMB polarization to constrain the anomalous nature of the Cold Spot with an incomplete sky-coverageUsing CMB polarization to constrain the anomalous nature of the Cold Spot w…Phantom cosmology with a decaying cosmological parameter Lambda(t) induced from five-dimensional (5D) geometrical vacuumPhantom cosmology with a decaying cosmological parameter Lambda(t) ind…Near-infrared K-band imaging of a sample of ultra-steep-spectrum radio sources selected at 74 MHzNear-infrared K-band imaging of a sample of ultra-steep-spectrum radio sourc…WMAP anomalous signal in the ecliptic planeBianchi VII_h models and the cold spot textureCMB polarization as a probe of the anomalous nature of the Cold SpotThe 6C** sample of steep-spectrum radio sources. 2. Redshift distribution and the space density of high-redshift radio galaxiesThe 6C** sample of steep-spectrum radio sources. 2. Redshift distribution an…The 6C** sample of steep-spectrum radio sources. 1. Radio data, near-infrared imaging and optical spectroscopyThe 6C** sample of steep-spectrum radio sources. 1. Radio data, near-infrare…The WMAP cold spotAnomalous variance in the WMAP data and Galactic Foreground residualsThe CMB cold spot: texture, cluster or void?A Cosmic Microwave Background feature consistent with a cosmic textureThe non-gaussian cold spot in wmap: significance, morphology and foreground contributionThe non-gaussian cold spot in wmap: significance, morphology and foregrou…The non-gaussian cold spot in the 3-year wmap dataDetection of a non-gaussian spot in wmap19952000200520102015202020250255075100
Created with Highcharts 9.0.1Citations/1 YearCitations/PeriodCitations / 1 YearMoving average19952000200520102015202020250255075100125150175