Rubin-LSST

Abstract:

We present morphological classifications based on Galaxy Zoo analysis of 71,052 galaxies with imaging from the United Kingdom Infrared Telescope Infrared Deep Sky Survey (UKIDSS). Galaxies were selected out of the Galaxy Zoo 2 (GZ2) sample, so also have gri imaging from the Sloan Digital Sky Survey. An identical classification tree, and vote weighting/aggregation was applied to both UKIDSS and GZ2 classifications enabling direct comparisons. With this Research Note we provide a public release of the GZ:UKIDSS morphologies and discuss some initial comparisons with GZ2.

Abstract:

A search for leptoquark pair production decaying into te-t¯e+ or tμ-t¯μ+ in final states with multiple leptons is presented. The search is based on a dataset of pp collisions at s=13TeV recorded with the ATLAS detector during Run 2 of the Large Hadron Collider, corresponding to an integrated luminosity of 139 fb-1. Four signal regions, with the requirement of at least three light leptons (electron or muon) and at least two jets out of which at least one jet is identified as coming from a b-hadron, are considered based on the number of leptons of a given flavour. The main background processes are estimated using dedicated control regions in a simultaneous fit with the signal regions to data. No excess above the Standard Model background prediction is observed and 95% confidence level limits on the production cross section times branching ratio are derived as a function of the leptoquark mass. Under the assumption of exclusive decays into te- (tμ-), the corresponding lower limit on the scalar mixed-generation leptoquark mass mLQmixd is at 1.58 (1.59) TeV and on the vector leptoquark mass mU~1 at 1.67 (1.67) TeV in the minimal coupling scenario and at 1.95 (1.95) TeV in the Yang–Mills scenario.

Abstract:

<jats:title>Abstract</jats:title><jats:p>We present a cosmological analysis of the combination of the DES-Y3, KiDS-1000 and HSC-DR1 weak lensing samples under a joint harmonic-space pipeline making use of angular scales down to ℓ<jats:sub>max</jats:sub>=4500, corresponding to significantly smaller scales (δθ ~ 2.4') than those commonly used in cosmological weak lensing studies. We are able to do so by accurately modelling non-linearities and the impact of baryonic effects using<jats:monospace>Baccoemu</jats:monospace>. We find<jats:italic>S</jats:italic><jats:sub>8</jats:sub>≡<jats:italic>σ</jats:italic><jats:sub>8</jats:sub>√(Ω<jats:sub>m</jats:sub>/0.3) = 0.795<jats:sup>+0.015</jats:sup><jats:sub>-0.017</jats:sub>, in relatively good agreement with CMB constraints from<jats:italic>Planck</jats:italic>(less than ~1.8<jats:italic>σ</jats:italic>tension), although we obtain a low value of Ω<jats:sub>m</jats:sub>=0.212<jats:sup>+0.017</jats:sup><jats:sub>-0.032</jats:sub>, in tension with<jats:italic>Planck</jats:italic>at the ~3σ level. We show that this can be recast as an H<jats:sub>0</jats:sub>tension if one parametrises the amplitude of fluctuations and matter abundance in terms of variables without hidden dependence on H<jats:sub>0</jats:sub>. Furthermore, we find that this tension reduces significantly after including a prior on the distance-redshift relationship from BAO data, without worsening the fit. In terms of baryonic effects, we show that failing to model and marginalise over them on scales<jats:italic>ℓ</jats:italic>≲ 2000 does not significantly affect the posterior constraints for DES-Y3 and KiDS-1000, but has a mild effect on deeper samples, such as HSC-DR1. This is in agreement with our ability to only mildly constrain the parameters of the Baryon Correction Model with these data.</jats:p>