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Journal Article
Science, ISSN 0036-8075, 02/2017, Volume 355, Issue 6327, pp. 817 - 819
Ultraluminous x-ray sources (ULXs) in nearby galaxies shine brighter than any x-ray source in our Galaxy. ULXs are usually modeled as stellar-mass black holes... 
PHOTON IMAGING CAMERA | MAGNETIZED NEUTRON-STARS | MULTIDISCIPLINARY SCIENCES | XMM-NEWTON | NUSTAR | MASS | Properties | Observations | Wave-motion, Theory of | Pulsars | X-rays | Neutrons | Neutron stars | Magnetism | X rays | Stars & galaxies | X ray sources | Accretion | Galaxies | Luminosity | Mathematical models | Spinning | Physics - High Energy Astrophysical Phenomena
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 02/2019, Volume 622, p. A29
Journal Article
Monthly Notices of the Royal Astronomical Society: Letters, ISSN 1745-3925, 2018, Volume 480, Issue 1, pp. L136 - L140
We report the results of AstroSat and NuSTAR observations of the Be/X-ray binary pulsar SXP 15.3 in the Small Magellanic Cloud during its outburst in late... 
Pulsars: individual: SMC- galaxies: individual: SXP 15.3 | Stars: neutron | Xrays: binaries | LUMINOSITY | galaxies: individual: SXP 15.3 | X-rays: binaries | pulsars: individual: SMC | ASTRONOMY & ASTROPHYSICS | X-RAY | stars: neutron | DISCOVERY | DEPENDENCE | Physics - High Energy Astrophysical Phenomena
Journal Article
Astrophysical Journal, ISSN 0004-637X, 07/2016, Volume 826, Issue 1, pp. 4 - 4
Located in the Small Magellanic Cloud ( SMC), SXP 214 is an X-ray pulsar in a high mass X-ray binary system with a Be-star companion. A recent survey of the... 
X-rays: binaries | stars: neutron | FIELDS | ADVECTION-DOMINATED ACCRETION | ASTRONOMY & ASTROPHYSICS | BINARY-SYSTEMS | NEUTRON-STARS | TIME-SERIES | EMISSION | BLACK-HOLES | Magellanic clouds | Neutron stars | X rays | Pulsars | Mathematical models | XMM (spacecraft) | Companion stars | Accretion disks
Journal Article
Astrophysical Journal, Supplement Series, ISSN 0067-0049, 05/2015, Volume 218, Issue 1, pp. 1 - 19
We have obtained a deep 8 field XMM-Newton mosaic of M33 covering the galaxy out to the D-25 isophote and beyond to a limiting 0.2-4.5 keV unabsorbed flux of 5... 
galaxies: individual (M33) | X-rays: binaries | X-rays: stars | PHOTON IMAGING CAMERA | CHANDRA ACIS SURVEY | BINARY POPULATION | X-RAY SOURCES | GALAXY M33 | VARIABILITY | CHASEM33 | SUPERNOVA-REMNANTS | ASTRONOMY & ASTROPHYSICS | EMISSION | SPECTRA | Galaxies | Pollution sources | Classification | X-ray sources | XMM (spacecraft) | Spiral galaxies | Catalogs | Density
Journal Article
Journal of Chromatography A, ISSN 0021-9673, 07/2015, Volume 1405, pp. 49 - 71
•Rapid direct injection LC/MS-QToF method for total naphthenic acids.•Calculated MDL 0.0004μgmL−1 with linearity down to 0.005μgmL−1 total NAs.•Calibration,... 
Environmental | Merichem | QToF | Isomers | OSPW | Naphthenic | CHEMISTRY, ANALYTICAL | BIOCHEMICAL RESEARCH METHODS | TOXICITY | IDENTIFICATION | SANDS PROCESS WATERS | MIXTURES | PROCESS-AFFECTED WATER | POLAR | SAMPLES | ELECTROSPRAY-IONIZATION
Journal Article
British Journal of Anaesthesia, ISSN 0007-0912, 11/2016, Volume 117, Issue 5, pp. 601 - 609
Journal Article