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Search indexed NASA NTRS and DOE OSTI research on propulsion, heat transfer, battery materials and energy systems. Follow report and document links to the original sources.
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Examples of Machine Learning with TBFM Data SWIM Industry/FAA Team (SWIFT) Briefing
This briefing discusses how machine learning could be applied to large aviation data problems, using TBFM SWIM data elements and data analytics lessons learned from ATD-2.
Swift Spectra of AT2018cow: A White Dwarf Tidal Disruption Event?
The bright transient AT2018cow has been unlike any other known type of transient. Its high brightness, rapid rise and decay, and initially nearly featureless spectrum are unprecedented and difficult to explain using models for similar burst sources. We present evidence for faint γ -ray emission continuing for at least 8 d, and featureless spectra in the ultraviolet bands – both unusual for eruptive sources. The X-ray variability of the source has a burst-like character. The UV-optical spectrum does not show any CNO line but is well described by a blackbody. We demonstrate that a model invoking the tidal disruption of a 0.1–0.4Msun helium white dwarf (WD) by a 105–106Msun black hole located in the outskirts of galaxy Z 137-068 could provide an explanation for most of the characteristics shown in the multiwavelength observations. A blackbody-like emission is emitted from an opaque photosphere, formed by the debris of the WD disruption. Broad features showing up in the optical/infrared spectra in the early stage are probably velocity broadened lines produced in a transient high-velocity outward moving cocoon. The asymmetric optical/infrared lines that appeared at a later stage are emission from an atmospheric layer when it detached from thermal equilibrium with the photosphere, which undergoes more rapid cooling. The photosphere shrinks when its temperature drops, and the subsequent in fall of the atmosphere produced asymmetric line profiles. Additionally, a non-thermal jet might be present, emitting X-rays in the 10–150 kcV band.
Simultaneous Radio and X Ray Observations of Swift J 1818.0 1607
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Advanced Concepts Swift Study
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Application of PSP on the SWiFT Model in the National Transonic Facility
This report details the results from a Pressure Sensitive Paint test on a blended/hybrid wing body model conducted at the National Transonic Facility. This test investigated potential instabilities that can occur at high Reynolds number and low Mach number testing conditions. The upper surface of the model was coated with pressure sensitive paint, and data was collected at various Mach numbers and angles of attack. For this test, typical pitch-pause testing was completed as well as a novel continuous sweep functionality that provided much greater angle of attack resolution. Results from this test will be presented, including indications of potential instability points in the testing envelope.
A Hard Look at Relativistic Reverberation in MCG-5-23-16 and SWIFT J2127.4+5654: Testing the Lamppost Model
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Implications for accretion flow dynamics from a spectral study of Swift J1357.2–0933
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BASS. XXXV. The M BH –σ* Relation of 105 Month Swift-BAT Type 1 AGNs
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Swift Multiwavelength Follow-up of LVC S200224ca and the Implications for Binary Black Hole Mergers
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Swift Follow-up of Reported Radio Pulsars at Fermi 4FGL Unassociated Sources
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Long-term monitoring of Ark 120 with Swift
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Swift-XRT Follow-up of Gravitational-wave Triggers in the Second Advanced LIGO/Virgo Observing Run
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Characterizing X-ray, UV, and optical variability in NGC 6814 using high-cadence Swift observations from a 2022 monitoring campaign
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Alive but Barely Kicking: News from 3+ yr of Swift and XMM-Newton X-Ray Monitoring of Quasiperiodic Eruptions from eRO-QPE1
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First characterization of a new high-mass X-ray binary in LMC eRASSU J050810.4−660653 with SRG /ART-XC, NuSTAR , and Swift
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A Swift Response to Newly Discovered, Nearby Transients
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Gamma-ray-emitting narrow-line Seyfert 1 galaxies: the Swift view
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