Journal: Monthly Notices of the Royal Astronomical Society
Publication
Estimating the bispectrum of the Very Small Array data
We estimate the bispectrum of the Very Small Array data from the compact and extended configuration observations released in 2002 December, and compare our...
Estimating the impact of recombination uncertainties on the cosmological parameter constraints from cosmic microwave background experiments
We use our most recent training set for the RICO code to estimate the impact of recombination uncertainties on the posterior probability distributions which...
Estimations of the magnetic field strength in the torus of IC 5063 using near-infrared polarimetry
An optically and geometrically thick torus obscures the central engine of active galactic nuclei (AGN) from some lines of sight. From a magnetohydrodynamical...
ETHOS 1: a high-latitude planetary nebula with jets forged by a post-common-envelope binary central star
We report on the discovery of ETHOS 1 (PN G068.1+11.0), the first spectroscopically confirmed planetary nebula (PN) from a survey of the SuperCOSMOS Science...
Euclid preparation - XXIII. Derivation of galaxy physical properties with deep machine learning using mock fluxes and H-band images
Next-generation telescopes, like Euclid, Rubin/LSST, and Roman, will open new windows on the Universe, allowing us to infer physical properties for tens of...
Euclid: the potential of slitless infrared spectroscopy: a z = 5.4 quasar and new ultracool dwarfs
We demonstrate the potential of Euclid 's slitless spectroscopy to discover high-redshift ( $z>5$) quasars and their main photometric contaminant, ultracool...
Evaluating cosmological biases using photometric redshifts for Type Ia Supernova cosmology with the Dark Energy Survey Supernova Program
Cosmological analyses with Type Ia Supernovae (SNe Ia) have traditionally been reliant on spectroscopy for both classifying the type of supernova and obtaining...
Evaluating hydrodynamical simulations with green valley galaxies
We test cosmological hydrodynamical simulations of galaxy formation regarding the properties of the blue cloud (BC), green valley (GV), and red sequence (RS)...
Evaluating quenching in cosmological simulations of galaxy formation with spectral covariance in the optical window
Cosmological hydrodynamical simulations provide valuable insights on galaxy evolution when coupled with observational data. Comparisons with real galaxies are...