Overview of the Advanced X-ray Imaging Satellite (AXIS)
arXiv:2311.00780 · doi:10.1117/12.2677468
Abstract
The Advanced X-ray Imaging Satellite (AXIS) is a Probe-class concept that will build on the legacy of the Chandra X-ray Observatory by providing low-background, arcsecond-resolution imaging in the 0.3-10 keV band across a 450 arcminute field of view, with an order of magnitude improvement in sensitivity. AXIS utilizes breakthroughs in the construction of lightweight segmented X-ray optics using single-crystal silicon, and developments in the fabrication of large-format, small-pixel, high readout rate CCD detectors with good spectral resolution, allowing a robust and cost-effective design. Further, AXIS will be responsive to target-of-opportunity alerts and, with onboard transient detection, will be a powerful facility for studying the time-varying X-ray universe, following on from the legacy of the Neil Gehrels (Swift) X-ray observatory that revolutionized studies of the transient X-ray Universe. In this paper, we present an overview of AXIS, highlighting the prime science objectives driving the AXIS concept and how the observatory design will achieve these objectives.
arXiv commentPublished in Proceedings of SPIE Optics & Photonics 2023, San Diego
References in corpus (35)
- Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
- GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
- A Fundamental Relation Between Supermassive Black Holes and Their Host Galaxies
- The Demography of Massive Dark Objects in Galaxy Centres
- The M-sigma and M-L Relations in Galactic Bulges and Determinations of their Intrinsic Scatter
- Revisiting the Scaling Relations of Black Hole Masses and Host Galaxy Properties
- Black Holes, Galaxy Formation, and the M_BH-sigma Relation
- The obscured growth of massive black holes
- Chandra imaging of the complex X-ray core of the Perseus cluster
- The Chandra Deep Field-South Survey: 7 Ms Source Catalogs
- Planetary evaporation by UV & X-ray radiation: basic hydrodynamics
- Estimation of the XUV radiation onto close planets and their evaporation
- The stellar rotation--activity relationship in fully convective M dwarfs
- Identification and properties of intense star-forming galaxies at redshifts z>10
- The active lives of stars: a complete description of rotation and XUV evolution of F, G, K, and M dwarfs
- The coronal X-ray - age relation and its implications for the evaporation of exoplanets
- Understanding Dual AGN Activation in the Nearby Universe
- Frequent flaring in the TRAPPIST-1 system - unsuited for life?
- The Observational Signatures of Supermassive Black Hole Seeds
- Strong XUV irradiation of the Earth-sized exoplanets orbiting the ultracool dwarf TRAPPIST-1
- XUV-driven mass loss from extrasolar giant planets orbiting active stars
- The Hard X-Ray Luminosity Function of High-Redshift () Active Galactic Nuclei
- COS-Burst: Observations of the Impact of Starburst-Driven Winds on the Properties of the Circum-Galactic Medium
- Extreme hydrodynamic losses of Earth-like atmospheres in the habitable zones of very active stars
- Supermassive black holes in cosmological simulations II: the AGN population and predictions for upcoming X-ray missions
- Varstrometry for Off-nucleus and Dual sub-Kpc AGN (VODKA): Hubble Space Telescope Discovers Double Quasars
- Deep Chandra Observations of ESO 428-G014: III. High Resolution Spectral Imaging of the Ionization Cone and Radio Jet Region
- The XUV environments of exoplanets from Jupiter-size to super-Earth
- CHEERS Results from NGC 3393, III: Chandra X-ray Spectroscopy of the Narrow Line Region
- A Bayesian Analysis of SDSS J0914+0853, a Low-Mass Dual AGN Candidate
- AGN Triality of Triple Mergers: Detection of Faint X-ray Point Sources
- Two decades of optical timing of the shortest-period binary star system HM Cancri
- Deep Chandra Observations of NGC 5728: Morphology and Spectral Properties of the Extended X-ray Emission
- XUV emission of the young planet-hosting star V1298\,Tau from coordinated observations with XMM-Newton and HST
- The strongly irradiated planets in Praesepe
Cited by in corpus (22)
- The NewAthena mission concept in the context of the next decade of X-ray astronomy
- Mildly Super-Eddington Accretion Onto Slowly-Spinning Black Holes Explains the X-Ray Weakness of the Little Red Dots
- Exploring the AGN Fraction of a Sample of JWST's Little Red Dots at : Overmassive Black Holes Are Strongly Favored
- The Dual Nature of GHZ9: Coexisting Active Galactic Nuclei and Star Formation Activity in a Remote X-ray Source at z = 10.145
- A unified accretion disc model for supermassive black holes in galaxy formation simulations: method and implementation
- SRG/eROSITA No. 5: Discovery of quasi-periodic eruptions every ~3.7 days from a galaxy at z>0.1
- Surveying the onset and evolution of supermassive black holes at high-z with AXIS
- Modeling Multiple X-Ray Reflection in Super-Eddington Winds
- X-ray Redshifts for Obscured Active Galactic Nuclei with AXIS Deep and Intermediate Surveys
- Demonstrating repetitive non-destructive readout (RNDR) with SiSeRO devices
- Electron-Ion Equilibration in the Merging Galaxy Cluster A665
- Colloquium: Multimessenger astronomy with continuous gravitational waves and future detectors
- Detection of molecular clouds in the PeVatron candidate source LHAASO J03415258 by the Nobeyama 45-m radio telescope
- Advancing Precision Particle Background Estimation for Future X-ray Missions: Correlated Variability between AMS and Chandra/XMM-Newton
- Morphology of Relativistically Broadened Line Emission from Axisymmetric Equatorial Accretion Disks
- BASS XLV: Quantifying AGN Selection Effects in the Chandra COSMOS-Legacy Survey with BASS
- Searching for Axion-Like Particles with X-ray Observations of Alpha Centauri
- Probing the Diversity of Type Ia Supernova Remnants in 3-D Hydrodynamic Simulations with X-ray Spectral Synthesis
- Direct observation of the X-ray counterpart of the Hα filaments and of the sloshing spiral in the Perseus galaxy cluster
- New Hard X-Ray and Multiwavelength Study of the PeVatron Candidate PWN G0.9+0.1 in the Galactic Center Region
- The Drivers of the Decline in Supermassive Black Hole Growth at
- Simulation-calibrated Bayesian inference for progenitor properties of the microquasar SS 433