Asorey et al., 2020 - Google Patents
HIR4: cosmology from a simulated neutral hydrogen full sky using Horizon Run 4Asorey et al., 2020
View PDF- Document ID
- 9659896809749965786
- Author
- Asorey J
- Parkinson D
- Shi F
- Song Y
- Ahn K
- Kim J
- Yao J
- Zhang L
- Zuo S
- Publication year
- Publication venue
- Monthly Notices of the Royal Astronomical Society
External Links
Snippet
The distribution of cosmological neutral hydrogen will provide a new window into the large- scale structure of the Universe with the next generation of radio telescopes and surveys. The observation of this material, through 21 cm line emission, will be confused by foreground …
- 229910052739 hydrogen 0 title abstract description 83
Classifications
-
- G—PHYSICS
- G01—MEASURING; TESTING
- G01S—RADIO DIRECTION-FINDING; RADIO NAVIGATION; DETERMINING DISTANCE OR VELOCITY BY USE OF RADIO WAVES; LOCATING OR PRESENCE-DETECTING BY USE OF THE REFLECTION OR RERADIATION OF RADIO WAVES; ANALOGOUS ARRANGEMENTS USING OTHER WAVES
- G01S13/00—Systems using the reflection or reradiation of radio waves, e.g. radar systems; Analogous systems using reflection or reradiation of waves whose nature or wavelength is irrelevant or unspecified
- G01S13/88—Radar or analogous systems specially adapted for specific applications
- G01S13/89—Radar or analogous systems specially adapted for specific applications for mapping or imaging
- G01S13/90—Radar or analogous systems specially adapted for specific applications for mapping or imaging using synthetic aperture techniques, e.g. correcting range migration errors
- G01S13/9035—Particular SAR processing techniques not provided for elsewhere, e.g. squint mode, doppler beam-sharpening mode, spotlight mode, bistatic SAR, inverse SAR
-
- G—PHYSICS
- G01—MEASURING; TESTING
- G01J—MEASUREMENT OF INTENSITY, VELOCITY, SPECTRAL CONTENT, POLARISATION, PHASE OR PULSE CHARACTERISTICS OF INFRA-RED, VISIBLE OR ULTRA-VIOLET LIGHT; COLORIMETRY; RADIATION PYROMETRY
- G01J3/00—Spectrometry; Spectrophotometry; Monochromators; Measuring colour
- G01J3/28—Investigating the spectrum
Similar Documents
| Publication | Publication Date | Title |
|---|---|---|
| Padmanabh et al. | The MPIfR–MeerKAT galactic plane survey–i. system set-up and early results | |
| Jelić et al. | Realistic simulations of the Galactic polarized foreground: consequences for 21-cm reionization detection experiments | |
| Remazeilles et al. | Sensitivity and foreground modelling for large-scale cosmic microwave background B-mode polarization satellite missions | |
| De Gasperin et al. | The effect of the ionosphere on ultra-low-frequency radio-interferometric observations | |
| Pober et al. | The importance of wide-field foreground removal for 21 cm cosmology: a demonstration with early MWA epoch of reionization observations | |
| Dowell et al. | The LWA1 low frequency sky survey | |
| Keisler et al. | Measurements of sub-degree B-mode polarization in the cosmic microwave background from 100 square degrees of SPTpol data | |
| Zaroubi et al. | Imaging neutral hydrogen on large scales during the Epoch of Reionization with LOFAR | |
| Pen et al. | The GMRT EoR experiment: limits on polarized sky brightness at 150 MHz | |
| Dye et al. | Modelling high-resolution ALMA observations of strongly lensed highly star-forming galaxies detected by Herschel | |
| Asorey et al. | HIR4: cosmology from a simulated neutral hydrogen full sky using Horizon Run 4 | |
| Van Eck et al. | Diffuse polarized emission in the LOFAR Two-meter Sky Survey | |
| Gary et al. | Magnetography of solar flaring loops with microwave imaging spectropolarimetry | |
| Luken et al. | Radio observations of supernova remnant G1. 9+ 0.3 | |
| Blake | Power spectrum modelling of galaxy and radio intensity maps including observational effects | |
| Schnitzeler et al. | S-PASS/ATCA: a window on the magnetic universe in the Southern hemisphere | |
| Akahori et al. | Exploring the intergalactic magnetic field by means of Faraday tomography | |
| Burgay et al. | The Perseus Arm Pulsar Survey | |
| Bate et al. | Major substructure in the M31 outer halo: the South-West Cloud | |
| Geil et al. | Polarized foreground removal at low radio frequencies using rotation measure synthesis: uncovering the signature of hydrogen reionization | |
| McKinley et al. | Measuring the global 21-cm signal with the MWA-I: improved measurements of the Galactic synchrotron background using lunar occultation | |
| Wang et al. | ASKAP observations of multiple rapid scintillators reveal a degrees-long plasma filament | |
| Kubota et al. | Expected constraints on models of the epoch of reionization with the variance and skewness in redshifted 21 cm-line fluctuations | |
| Vaughan et al. | Behind the mask: can HARMONI@ ELT detect biosignatures in the reflected light of Proxima b? | |
| Jensen et al. | Uncovering fossils of the distant Milky Way with UNIONS: NGC 5466 and its stellar stream |