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1 to 10 of 24 Results
May 29, 2024
Daniel Stern, 2024, "NuSTAR Observations of Candidate Subparsec Binary Supermassive Black Holes", https://doi.org/10.48577/jpl.NQJCVA, Astrophysical Journal, JPL Open Repository
We present analysis of NuSTAR X-ray observations of three AGN that were identified as candidate subparsec binary supermassive black hole (SMBH) systems in the Catalina Real-Time Transient Survey based on apparent periodicity in their optical light curves. Simulations predict that...
Dec 6, 2023
Daniel Stern, 2023, "The High Energy X-ray Probe (HEX-P): resolving the nature of Sgr A* flares, compact object binaries, ultra-relativistic cosmic-rays and particle accelerators in the Galactic Center", https://doi.org/10.48577/jpl.BCST9N, Frontiers in Astronomy and Space Sciences, JPL Open Repository
HEX-P is a probe-class mission concept that will combine high spatial resolution X-ray imaging (< 10′′ FWHM) and broad spectral coverage (0.2–80 keV) with a sensitivity far superior to current facilities (including XMM-Newton and NuSTAR). These capabilities will enable revolution...
Nov 22, 2023
Daniel Stern, 2023, "The High Energy X-ray Probe (HEX-P): Probing Accretion onto Stellar Mass Black Holes", https://doi.org/10.48577/jpl.BJHZU1, Frontiers in Astronomy and Space Sciences, JPL Open Repository
Accretion is a universal astrophysical process that plays a key role in cosmic history, from the epoch of reionization to galaxy and stellar formation and evolution. Accreting stellar-mass black holes in X-ray binaries are one of the best laboratories to study the accretion proce...
Oct 30, 2023
Daniel Stern, 2023, "The High Energy X-ray Probe: Resolved X-ray Populations in Extragalactic Environments", https://doi.org/10.48577/jpl.ASQKCD, Frontiers in Astronomy and Space Sciences, JPL Open Repository
The High Energy X-ray Probe (HEX-P) is a probe-class mission concept that will combine high spatial resolution X-ray imaging (<20 arcsec FWHM) and broad spectral coverage (0.2–80 keV) with a sensitivity superior to current facilities (including XMM-Newton and NuSTAR). HEX-P will...
Oct 30, 2023
Daniel Stern, 2023, "The High Energy X-ray Probe (HEX-P): Studying Extreme Accretion with Ultraluminous X-ray Sources", https://doi.org/10.48577/jpl.3AYAGF, Frontiers in Astronomy and Space Sciences, JPL Open Repository
Ultraluminous X-ray sources (ULXs) represent an extreme class of accreting compact objects: from the identification of some of the accretors as neutron stars to the detection of powerful winds travelling at 0.1-0.2 c, the increasing evidence points towards ULXs harbouring stellar...
Oct 1, 2020
Daniel Stern, 2020, "SN 1987A: CONSTRAINING THE HARD X-RAY CONTINUUM AND ITS EVOLUTION WITH NUSTAR", https://doi.org/10.48577/jpl.LQN1YG, Astrophysical Journal, JPL Open Repository
NuSTAR observed SN1987A multiple times from July 2012 to August 2014 with a total exposure of 2.7 Ms. These observations allowed the determination of the hard X-ray emission from the remnant up to ∼ 25 keV. The continuum spectrum between 3 and 25 keV can be equally well described...
Sep 16, 2020
Daniel Stern, 2020, "Chandra Observations of Candidate Sub-Parsec Binary Supermassive Black Holes", https://doi.org/10.48577/jpl.II0DEP, Astrophysical Journal, JPL Open Repository
We present analysis of Chandra X-ray observations of seven quasars that were identified as candi- date sub-parsec binary supermassive black hole (SMBH) systems in the Catalina Real-Time Transient Survey (CRTS) based on apparent periodicity in their optical light curves. Simulatio...
Sep 15, 2020
Daniel Stern, 2020, "BAT AGN Spectroscopic Survey – XIII. The nature of the most luminous obscured AGN in the low-redshift universe", https://doi.org/10.48577/jpl.GKY0JM, Monthly Notices of the Royal Astronomical Society, JPL Open Repository
We present a multi wavelength analysis of the 28 most luminous low-redshift narrow-line,ultra-hard X-ray selected active galactic nuclei (AGN) within the 70 month Swift/BAT all-skysurvey, with bolometric luminosities of log¹Lbolerg s􀀀1º > 45:25. The broad goal of our studyis to...
Sep 15, 2020
Daniel Stern, 2020, "SAGITTARIUS A⋆ HIGH ENERGY X-RAY FLARE PROPERTIES DURING NuSTAR MONITORING OF THE GALACTIC CENTER FROM 2012 TO 2015", https://doi.org/10.48577/jpl.TRBTIW, Astrophysical Journal, JPL Open Repository
Understanding the origin of the aring activity from the Galactic center supermassive black hole, Sagittarius A?, is a major scientic goal of the NuSTAR Galactic plane survey campaign. We report on the data obtained between July 2012 and April 2015, including 28 observations with...
Sep 15, 2020
Daniel Stern, 2020, "An Iwasawa-Taniguchi Effect for Compton-thick Active Galactic Nuclei", https://doi.org/10.48577/jpl.9VMAHO, Monthly Notices of the Royal Astronomical Society, JPL Open Repository
Here we present the first study of an Iwasawa-Taniguchi/‘X-ray Baldwin’ e↵ect forCompton-thick active galactic nuclei (AGN). We report a statistically significant anticorrelationbetween the rest-frame equivalent width (EW) of the narrow core of theneutral FeK↵ fluorescence emissi...
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