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A 300-parsec-long jet-inflated bubble around a powerful microquasar in the galaxy NGC 7793
Online Contents | 2010|Contributors: Soria, Roberto -
A CENSUS OF X-RAY NUCLEAR ACTIVITY IN NEARBY GALAXIES
Online Contents | 2009|Contributors: Soria, Roberto -
A CENSUS OF X-RAY NUCLEAR ACTIVITY IN NEARBY GALAXIES
Online Contents | 2009|Contributors: Soria, Roberto -
A COMPLETE SAMPLE OF ULTRALUMINOUS X-RAY SOURCE HOST GALAXIES
Online Contents | 2011|Contributors: Soria, Roberto -
A COMPLETE SAMPLE OF ULTRALUMINOUS X-RAY SOURCE HOST GALAXIES 49
Online Contents | 2011|Contributors: Soria, Roberto -
A DEEP CHANDRA ACIS SURVEY OF M83Based on observations made with NASA's Chandra X-Ray Observatory. NASA's Chandra Observatory is operated by Smithsonian Astrophysical Observatory under contract NAS83060 and the data were obtained through program GO1-12115.
Online Contents | 2014|Contributors: Soria, Roberto -
AN EXPANDED HST/WFC3 SURVEY OF M83: PROJECT OVERVIEW AND TARGETED SUPERNOVA REMNANT SEARCHBased on observations with the NASA/ESA Hubble Space Telescope, obtained at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS5-26555.
Online Contents | 2014|Contributors: Soria, Roberto -
AN X-RAY VIEW OF STAR FORMATION IN THE CENTRAL 3 kpc OF NGC 2403
Online Contents | 2010|Contributors: Soria, Roberto -
A study of the new X-ray transient RXTE J2123-058 during its post-outburst state
Online Contents | 1999| -
Constraints on active galactic nucleus accretion disc viscosity derived from continuum variability
Online Contents | 2004|Contributors: Soria, Roberto -
Discovery of an optical counterpart to the hyperluminous X-ray source in ESO 243-49
Online Contents | 2010| -
Discovery of a Transient X-Ray Source in the Compact Stellar Nucleus of NGC 2403
Online Contents | 2007|Contributors: Soria, Roberto -
DISCOVERY OF A TRANSIENT X-RAY SOURCE IN THE COMPACT STELLAR NUCLEUS OF NGC 2403
Online Contents | 2007|Contributors: Soria, Roberto -
Do Ultraluminous X-Ray Sources Exist in Dwarf Galaxies?
Online Contents | 2008|Contributors: Soria, Roberto -
DO ULTRALUMINOUS X-RAY SOURCES EXIST IN DWARF GALAXIES?
Online Contents | 2008|Contributors: Soria, Roberto -
Erratum: Probable intermediate-mass black holes in NGC 4559: XMM-Newton spectral and timing constraints
Online Contents | 2004|Contributors: Soria, Roberto -
HOT DIFFUSE EMISSION IN THE NUCLEAR STARBURST REGION OF NGC 2903
Online Contents | 2012|Contributors: Soria, Roberto -
How rapidly do neutron stars spin at birth? Constraints from archival X-ray observations of extragalactic supernovae
Online Contents | 2008|Contributors: Soria, Roberto -
Irradiation models for ULXs and fits to optical data
Online Contents | 2007|Contributors: Soria, Roberto -
Optical and infrared signatures of ultra-luminous X-ray sources
Online Contents | 2005|Contributors: Soria, Roberto -
Optical and X-ray luminosities of expanding nebulae around ultraluminous X-ray sources
Online Contents|Contributors: Soria, Roberto -
Optical spectroscopy of GX 339-4 during the high-soft and low-hard states - I
Online Contents | 1999| -
Optical spectroscopy of GX 339-4 during the high-soft and low-hard states - II. Line ionization and emission region
Online Contents | 2001|Contributors: Soria, Roberto -
Outbursts of the intermediate-mass black hole HLX-1: a wind instability scenario
Online Contents | 2017| -
Probable intermediate-mass black holes in NGC 4559: XMM-Newton spectral and timing constraints
Online Contents | 2004|Contributors: Soria, Roberto -
Probable intermediate-mass black holes in NGC 4559: XMM-Newton spectral and timing constraints
Online Contents | 2004|Contributors: Soria, Roberto -
RECOVERY OF THE HISTORICAL SN1957D IN X-RAYS WITH CHANDRA Based on observations made with NASA's Chandra X-ray Observatory, the NASA/ESA Hubble Space Telescope (HST), the 6.5 m Magellan Telescopes located at Las Campanas Observatory, and the Gemini Observatory. NASA's Chandra Observatory is operated by Smithsonian Astrophysical Observatory under contract NAS83060 and the data were obtained through program GO1-12115. The HST observations were obtained at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc. (AURA), under NASA contract NAS 5-26555. The new HST observations were obtained through programs GO-12513 and GO-12683. Data in the HST archive from program GO-11360 were also used. The ground-based observations were obtained through NOAO, which is operated by Association of Universities for Research in Astronomy, Inc., for the National Science Foundation.
Online Contents | 2012|Contributors: Soria, Roberto -
Revisiting the ultraluminous supersoft source in M 101: an optically thick outflow model
Online Contents | 2016|Contributors: Soria, Roberto -
Spectra of black hole accretion models of ultraluminous X-ray sources
Online Contents|Contributors: Soria, Roberto -
THE BIRTH OF AN ULTRALUMINOUS X-RAY SOURCE IN M83Based on observations made with NASA's Chandra X-Ray Observatory, the NASA/ESA Hubble Space Telescope (HST), Swift, the 6.5 m Magellan Telescopes located at Las Campanas Observatory, and the Gemini Observatory. NASA's Chandra Observatory is operated by Smithsonian Astrophysical Observatory under contract NAS83060, and the data were obtained through program GO1-12115. The HST observations were obtained at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy (AURA), Inc., under NASA contract NAS 5-26555. The new HST observations were obtained through programs GO-12513 and GO-12683. Data in the HST archive from program GO-11360 were also used. The ground-based observations were obtained from the Magellan I Telescope at the Las Campanas Observatory and from the Gemini South Telescope of the Gemini Observatory, both awarded through NOAO, which is operated by Association of Universities for Research i
Online Contents | 2012| -
THE FADING OF TWO TRANSIENT ULTRALUMINOUS X-RAY SOURCES TO BELOW THE STELLAR MASS EDDINGTON LIMIT
Online Contents | 2013|Contributors: Soria, Roberto -
The nature of the companion star in Circinus X-1
Online Contents | 2015|Contributors: Soria, Roberto -
The star-forming environment of an ultraluminous X-ray source in NGC4559: an optical study
Online Contents | 2005| -
ULTRALUMINOUS X-RAY SOURCE CORRELATIONS WITH STAR-FORMING REGIONS
Online Contents | 2009|Contributors: Soria, Roberto -
ULTRALUMINOUS X-RAY SOURCE CORRELATIONS WITH STAR-FORMING REGIONS
Online Contents | 2009|Contributors: Soria, Roberto
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