most citedAn ALMA survey of the SCUBA-2 CLS UDS field: Physical properties of 707 Sub-millimetre Galaxies

278 citations

27 papers

astro-ph.CO2020★ 119 cited

The miniJPAS survey: a preview of the Universe in 56 colours

S. Bonoli, A. Marín-Franch, J. Varela +166

The Javalambre-Physics of the Accelerating Universe Astrophysical Survey (J-PAS) will soon start to scan thousands of square degrees of the northern extragalactic sky with a unique…

astro-ph.EP2020★ 20 cited

Near-infrared variability in dusty white dwarfs: tracing the accretion of planetary material

Laura K. Rogers, Siyi Xu, Amy Bonsor +4

The inwards scattering of planetesimals towards white dwarfs is expected to be a stochastic process with variability on human time-scales. The planetesimals tidally disrupt at the…

astro-ph.SR2020★ 6 cited

H--He collision-induced satellite in the Lyman- profile of DBA white dwarf stars

Nicole F. Allard, John F. Kielkopf, Siyi Xu +6

The spectra of helium-dominated white dwarf stars with hydrogen in their atmosphere present a distinctive broad feature centered around 1160~Å\/ in the blue wing of the Lyman- l…

astro-ph.GA2020★ 10 cited

Long-term NIR Variability in the UKIDSS Ultra Deep Survey: a new probe of AGN activity at high redshift

E. Elmer, O. Almaini, M. Merrifield +5

We present the first attempt to select AGN using long-term NIR variability. By analysing the K-band light curves of all the galaxies in the UKIDSS Ultra Deep Survey, the deepest NI…

astro-ph.GA2020★ 38 cited

Detection of vibrational emissions from the helium hydride ion (HeH) in the planetary nebula NGC 7027

David A. Neufeld, Miwa Goto, T. R. Geballe +3

We report the detection of emission in the v=1-0 P(1) (3.51629 micron) and P(2) (3.60776 micron) rovibrational lines of the helium hydride cation (HeH+) from the planetary nebula N…

astro-ph.GA2020★ 20 cited

The MASSIVE Survey XIV -- Stellar Velocity Profiles and Kinematic Misalignments from 200 pc to 20 kpc in Massive Early-type Galaxies

Irina Ene, Chung-Pei Ma, Jonelle L. Walsh +3

We use high spatial resolution stellar velocity maps from the Gemini GMOS integral-field spectrograph (IFS) and wide-field velocity maps from the McDonald Mitchell IFS to study the…