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ALMA survey of the SCUBA-2 CLS UDS field
We analyse the physical properties of a large, homogeneously selected sample of ALMA-located sub-millimetre galaxies (SMGs). This survey, AS2UDS, identified 707 SMGs across the... -
The UTMOST pulsar timing programme - II
While pulsars possess exceptional rotational stability, large-scale timing studies have revealed at least two distinct types of irregularities in their rotation: red timing... -
X-ray and radio activity of Ly {alpha} emitters
Despite recent progress in understanding Ly {alpha} emitters (LAEs), relatively little is known regarding their typical black hole activity across cosmic time. Here, we study... -
Modelling of wind and supernovae shocks
Cosmic ray (CR) sources leave signatures in the isotopic abundances of CRs. Current models of Galactic CRs that consider supernovae (SNe) shocks as the main sites of particle... -
Discovery and timing of 40 pulsars
We present the results of processing an additional 44 per cent of the High Time Resolution Universe South Low Latitude (HTRU-S LowLat) pulsar survey, the most sensitive blind... -
Very massive radio-loud and radio-quiet AGN
The main objective of this work is to establish and interpret the dominant spectral components and their differences in radio-loud (RL) and radio-quiet (RQ) AGN with very... -
Young radio AGNs study based on SDSS spectroscopy
The gigahertz peaked spectrum (GPS) sources, compact steep spectrum (CSS) radio sources, and high-frequency peaker (HFP) radio sources are thought to be young radio active... -
Classifying Fermi-LAT gamma-ray sources
Machine learning is an automatic technique that is revolutionizing scientific research, with innovative applications and wide use in astrophysics. The aim of this study was to... -
Dust clumps associated with methanol masers
We have constructed the largest sample of dust-associated class II 6.7GHz methanol masers yet obtained. New measurements from the Methanol Multibeam (MMB) survey were combined... -
Unveiling weak radio quasar population at z>=4
We applied image stacking on empty field Faint Images of the Radio Sky at Twenty-Centimeters (FIRST) survey maps centred on optically identified high-redshift quasars at z>=4... -
ALMA polarimetric follow-up of PACO sources
We present Atacama Large Millimetre/submillimiter Array (ALMA) high sensitivity ({sigma}P~0.4mJy) polarimetric observations at 97.5GHz (Band 3) of a complete sample of 32... -
A new sample of southern radio galaxies
In this study we define a new sample of distant powerful radio galaxies in order to study their host galaxy properties and provide targets for future observations of HI... -
Sub-damped Ly{alpha} systems in XQ-100 survey
Sub-damped Lyman {alpha} systems (subDLAs; HI column densities of 19.0<=logN(HI)<20.3) are rarely included in the cosmic HI census performed at redshifts z_abs_>=1.5,... -
Swift obs. of Mrk 421. IV. 5.5yrs obs.
We present the spectral and timing results obtained during the intense observations of Mrk 421 by the Swift-based ultraviolet to X-ray instruments during 2018 April-2023... -
X-ray burst associated to FRB200428 with Insight-HXMT
A double-peak X-ray burst from the Galactic magnetar SGR J1935+2154 was discovered to be associated with the two radio pulses of FRB200428 separated by 28.97+/-0.02ms. Precise... -
Puppis A Fermi-LAT TS and eROSITA images
Supernova remnants (SNRs) interacting with molecular clouds are interesting laboratories to study the acceleration of cosmic rays and their propagation in the dense ambient... -
LOFAR 23MHz sources catalogue
The largely unexplored decametre radio band (10-30MHz) provides a unique window for studying a range of astronomical topics, such as auroral emission from exoplanets,... -
Variability of extragalactic X-ray jets
Unexpectedly strong X-ray emission from extragalactic radio jets on kiloparsec scales has been one of the major discoveries of Chandra, the only X-ray observatory capable of... -
SuperCLASS. I.
The SuperCLuster Assisted Shear Survey (SuperCLASS) is a legacy programme using the e-MERLIN interferometric array. The aim is to observe the sky at L-band (1.4GHz) to a r.m.s.... -
SDSS Stripe 82 VLA 1-2GHz survey
We have used the Karl G. Jansky Very Large Array to image ~100deg^2^ of SDSS Stripe 82 at 1-2GHz. The survey consists of 1026 snapshot observations of 2.5-min duration, using...
