With the recent discovery of a dozen dusty star-forming galaxies and around 30 quasars at z > 5 that are hyper-luminous in the infrared (μ L IR > 1013 L⊙, where...
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PublicationProbing the high-redshift universe with SPICA: Toward the epoch of reionisation and beyond
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PublicationProcessing GOTO data with the Rubin Observatory LSST Science Pipelines I: Production of coadded frames
The past few decades have seen the burgeoning of wide-field, high-cadence surveys, the most formidable of which will be the Legacy Survey of Space and Time...
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PublicationProcessing GOTO survey data with the Rubin Observatory LSST Science Pipelines II: Forced Photometry and lightcurves
We have adapted the Vera C. Rubin Observatory Legacy Survey of Space and Time (LSST) Science Pipelines to process data from the Gravitational-wave Optical...
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PublicationSolar Space Density of the Red Clump Stars and the Scale-Length of the Thin Disc
We estimated the scale-length of the thin disc with the J and W1 magnitudes of the most probable red clump stars in the Galactic plane, - 0°.5 ⩽ b ⩽ +0°.5, in...
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PublicationSPICA and the Chemical Evolution of Galaxies: The Rise of Metals and Dust
The physical processes driving the chemical evolution of galaxies in the last 11Gyr cannot be understood without directly probing the dust-obscured phase of...
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PublicationThe bivariate gas-stellar mass distributions and the mass functions of early- and late-type galaxies at z {∼} 0
We report the bivariate $HI$ - and $H 2$ -stellar mass distributions of local galaxies in addition of an inventory of galaxy mass functions, MFs, for $HI$ , $H...
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PublicationThe Dawes Review 10: The impact of deep learning for the analysis of galaxy surveys
The amount and complexity of data delivered by modern galaxy surveys has been steadily increasing over the past years. New facilities will soon provide imaging...
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PublicationThe GLEAMing of the first supermassive black holes: II. A new sample of high-redshift radio galaxy candidates
While unobscured and radio-quiet active galactic nuclei are regularly being found at redshifts $z > 6$ , their obscured and radio-loud counterparts remain...
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PublicationThe Magellanic Clouds as a Template for the Study of Stellar Populations and Galaxy Interactions
The Magellanic System represents one of the best places to study the formation and evolution of galaxies. Photometric surveys of various depths, areas and...