Quantifying Interstellar Extinction at High Galactic Latitudes

Kavli Affiliate: Kaisey Mandel | Summary:A detailed map of the distribution of dust at high Galactic latitudes is essential for future cosmic microwave background (CMB) polarization experiments because the dust, while diffuse, remains a significant foreground in these regions. We develop a Bayesian model to identify a region of the Hertzsprung-Russell (HR) diagram suited to […]


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Waveform Modelling for the Laser Interferometer Space Antenna

Kavli Affiliate: Ulrich Sperhake | Summary:LISA, the Laser Interferometer Space Antenna, will usher in a new era in gravitational-wave astronomy. As the first anticipated space-based gravitational-wave detector, it will expand our view to the millihertz gravitational-wave sky, where a spectacular variety of interesting new sources abound: from millions of ultra-compact binaries in our Galaxy, to […]


Continue.. Waveform Modelling for the Laser Interferometer Space Antenna

Waveform Modelling for the Laser Interferometer Space Antenna

Kavli Affiliate: Ulrich Sperhake | Summary:LISA, the Laser Interferometer Space Antenna, will usher in a new era in gravitational-wave astronomy. As the first anticipated space-based gravitational-wave detector, it will expand our view to the millihertz gravitational-wave sky, where a spectacular variety of interesting new sources abound: from millions of ultra-compact binaries in our Galaxy, to […]


Continue.. Waveform Modelling for the Laser Interferometer Space Antenna

Improved Planck constraints on axion-like early dark energy as a resolution of the Hubble tension

Kavli Affiliate: George Efstathiou | Summary:Axion-like early dark energy (EDE) as an extension to $Λ$CDM has been proposed as a possible solution to the ‘Hubble tension’. We revisit this model using a new cosmic microwave background (CMB) temperature and polarization likelihood constructed from the it Planck NPIPE data release. In a Bayesian analysis, we find […]


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FlexKnot and Gaussian Process for 21 cm global signal analysis and foreground separation

Kavli Affiliate: George Efstathiou | First 5 Authors: Stefan Heimersheim, Leiv Rønneberg, Henry Linton, Filippo Pagani, Anastasia Fialkov | Summary: The cosmological 21 cm signal is one of the most promising avenues to study the Epoch of Reionization. One class of experiments aiming to detect this signal is global signal experiments measuring the sky-averaged 21 […]


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Boson stars in massless and massive scalar-tensor gravity

Kavli Affiliate: Ulrich Sperhake | Summary:We study phenomenological features and stability of boson stars in massless and massive scalar-tensor theory of gravity with Damour-Esposito-Farese coupling. This coupling between the tensor and scalar sectors of the theory leads to a phenomenon called spontaneous scalarization, the onset of which we investigate by numerically computing families of boson-star […]


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Manifestly covariant variational principle for gauge theories of gravity

Kavli Affiliate: Anthony Lasenby | Summary:A variational principle for gauge theories of gravity is presented, which maintains manifest covariance under the symmetries to which the action is invariant, throughout the calculation of the equations of motion and conservation laws. This is performed by deriving explicit manifestly covariant expressions for the Euler–Lagrange variational derivatives and Noether’s […]


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Progress in the Design of the Atacama Large Aperture Submillimeter Telescope

Kavli Affiliate: Richard Hills | Summary:The Atacama Large Aperture Submillimeter Telescope (AtLAST) aims to be the premier next generation large diameter (50 meter) single dish observatory capable of observations across the millimeter/submillimeter spectrum, from 30~GHz to 1~THz. AtLAST will be sited in Chile at approximately 5100 meters above sea level, high in the Atacama Desert […]


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QUIJOTE scientific results — XIII. Intensity and polarization study of supernova remnants in the QUIJOTE-MFI wide survey: CTB 80, Cygnus Loop, HB 21, CTA 1, Tycho and HB 9

Kavli Affiliate: Anthony Lasenby | Summary:We use the new QUIJOTE-MFI wide survey (11, 13, 17 and 19 GHz) to produce spectral energy distributions (SEDs), on an angular scale of 1 deg, of the supernova remnants (SNRs) CTB 80, Cygnus Loop, HB 21, CTA 1, Tycho and HB 9. We provide new measurements of the polarized […]


Continue.. QUIJOTE scientific results — XIII. Intensity and polarization study of supernova remnants in the QUIJOTE-MFI wide survey: CTB 80, Cygnus Loop, HB 21, CTA 1, Tycho and HB 9

Flat-sky Angular Power Spectra Revisited

Kavli Affiliate: Anthony Challinor | Summary:We revisit the flat-sky approximation for evaluating the angular power spectra of projected random fields by retaining information about the correlations along the line of sight. With broad, overlapping radial window functions, these line-of-sight correlations are suppressed and are ignored in the Limber approximation. However, retaining the correlations is important […]


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