Browsing UMBC Center for Space Sciences and Technology (CSST) / Center for Research and Exploration in Space Sciences & Technology II (CRSST II) by Title
Now showing items 689-708 of 784
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T CrB: Radio Observations during the 2016–2017 "Super-active" State
(The American Astronomical Society, 2019-10-07)We obtained radio observations of the symbiotic binary and known recurrent nova T Coronae Borealis following a period of increased activity in the optical and X-ray bands. A comparison of our observations with those made ... -
TANAMI - Multiwavelength and Multimessenger Observations of Active Galaxies
(2015-07-08)Extragalactic jets launched from the immediate vicinity of supermassive black holes in radio-loud active galactic nuclei (AGN) are key objects in modern astronomy and astroparticle physics. AGN jets carry a fraction of the ... -
TANAMI - Tracking Active Galactic Nuclei with Austral Milliarcsecond Interferometry
(2010-01-18)We present a summary of the observation strategy of TANAMI (Tracking Active Galactic Nuclei with Austral Milliarcsecond Interferometry), a monitoring program to study the parsec-scale structure and dynamics of relativistic ... -
TANAMI and RadioAstron observations of AGN
(2014-08-07) -
TANAMI blazars in the IceCube PeV-neutrino fields
(EDP sciences, 2014-06-24)The IceCube Collaboration has announced the discovery of a neutrino flux in excess of the atmospheric background. Owing to the steeply falling atmospheric background spectrum, events at PeV energies most likely have an ... -
TANAMI counterparts to IceCube high-energy neutrino events
(arXiv, 2015-02-10)Since the discovery of a neutrino flux in excess of the atmospheric background by the IceCube Collaboration, searches for the astrophysical sources have been ongoing. Due to the steeply falling background towards higher ... -
TANAMI monitoring of Centaurus A: The complex dynamics in the inner parsec of an extragalactic jet
(EDP sciences, 2014-10-01)Context. Centaurus A (Cen A) is the closest radio-loud active galactic nucleus. Very Long Baseline Interferometry (VLBI) enables us to study the spectral and kinematic behavior of the radio jet-counterjet system on ... -
The TANAMI Multiwavelength Program: Dynamic spectral energy distributions of southern blazars
(EDP sciences, 2018-03-03)Context. Simultaneous broadband spectral and temporal studies of blazars are an important tool for investigating active galactic nuclei (AGN) jet physics. Aims. We study the spectral evolution between quiescent and ... -
The TANAMI Program
(AIP Publishing, 2010-07-22)TANAMI (Tracking Active Galactic Nuclei with Austral Milliarcsecond Interferometry) is a monitoring program to study the parsec-scale structures and dynamics of relativistic jets in active galactic nuclei (AGN) of the ... -
The TANAMI Program: Southern-Hemisphere AGN on (Sub-)parsec Scales
(Proceedings of Science, 2012-10-09)The Southern Hemisphere VLBI monitoring program TANAMI provides dual-frequency (8 GHz and 22 GHz), milliarcsecond monitoring of extragalactic jets south of −30◦ declination. The TANAMI sample consists of a combined radio ... -
TANAMI: Milliarcsecond Resolution Observations of Extragalactic Gamma-ray Sources
(arXiv, 2009-12-31)The TANAMI (Tracking AGN with Austral Milliarcsecond Interferometry) and associated programs provide comprehensive radio monitoring of extragalactic gamma-ray sources south of declination -30 degrees. Joint quasi-simultaneous ... -
TANAMI: tracking active galactic nuclei with austral milliarcsecond interferometry
(EDP sciences, 2010-09-10)Context. A number of theoretical models vie to explain the γ-ray emission from active galactic nuclei (AGN). This was a key discovery of EGRET. With its broader energy coverage, higher resolution, wider field of view and ... -
TANAMI: Tracking Active Galactic Nuclei with Austral Milliarcsecond Interferometry⋆
(EDP sciences, 2018-02-07)Context. TANAMI is a multiwavelength program monitoring active galactic nuclei (AGN) south of − 30° declination including high-resolution very long baseline interferometry (VLBI) imaging, radio, optical/UV, X-ray, and γ-ray ... -
Temperature calibration of the E and B Experiment
(World Scientific, 2017)The E and B Experiment (EBEX) is a balloon-borne polarimeter designed to measure the polarization of the cosmic microwave background radiation and to characterize the polarization of galactic dust. EBEX was launched December ... -
TES pixel optimization for the ATHENA X-IFU instrument
(2019-07-22)ATHENA is a European led x-ray observatory due for launch in the early 2030s. The X-ray Integral Field Unit (X-IFU) instrument on ATHENA will have an array of 3168 TES microcalorimeters, 2.5 eV resolution (at 7 keV), 5 arc ... -
A test platform for the detection and readout chain for the Athena X-IFU
(2021-07-07)We present a test platform for the Athena X-IFU detection chain, which will serve as the first demonstration of the representative end-to-end detection and readout chain for the X-IFU, using prototypes of the future ... -
Tests of General Relativity and Fundamental Physics with Space-based Gravitational Wave Detectors
(2019-03-07)Low-frequency gravitational-wave astronomy can perform precision tests of general relativity and probe fundamental physics in a regime previously inaccessible. A space-based detector will be a formidable tool to explore ... -
Thermal Crosstalk Measurements and Simulations for an X-ray Microcalorimeter Array
(Springer, 2020-01-18)Arrays of high-density microcalorimeters require careful heat sinking in order to minimize the thermal crosstalk between nearby pixels. For the array of microcalorimeters developed for the Athena X-ray Integral Field Unit ... -
Thermal fluctuation noise in Mo/Au superconducting transition-edge sensor microcalorimeters
(AIP, 2019-04-23)In many superconducting transition-edge sensor (TES) microcalorimeters, the measured electrical noise exceeds theoretical estimates based on a thermal model of a single body thermally connected to a heat bath. Here, we ... -
Thermal Impact of Cosmic Ray Interaction with an X-Ray Microcalorimeter Array
(Springer Nature Switzerland AG., 2020-02-13)The X-ray Integral Field Unit (X-IFU) instrument on the Athena mission will be positioned at the Lagrangian point L2 and be subject to cosmic rays generated by astrophysics sources, primarily relativistic protons. Previous ...