Search Publications

A comprehensive search for the radio counterpart of GW190814 with the Australian Square Kilometre Array Pathfinder
DOI: 10.1093/mnras/stab3628 Bibcode: 2022MNRAS.510.3794D

Gromadzki, M.; Wang, Z.; Buckley, D. A. H. +13 more

We present results from a search for the radio counterpart to the possible neutron star-black hole merger GW190814 with the Australian Square Kilometre Array Pathfinder. We have carried out 10 epochs of observation spanning 2-655 d post-merger at a frequency of 944 MHz. Each observation covered 30 deg2, corresponding to 87 per cent of t…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 21
Minute-cadence observations of the LAMOST fields with the TMTS: I. Methodology of detecting short-period variables and results from the first-year survey
DOI: 10.1093/mnras/stab2812 Bibcode: 2022MNRAS.509.2362L

Shi, Jianrong; Zhang, Xiaobin; Wang, Xiaofeng +18 more

Tsinghua University-Ma Huateng Telescopes for Survey (TMTS), located at Xinglong Station of NAOC, has a field of view up to 18 deg2. The TMTS has started to monitor the LAMOST sky areas since 2020, with the uninterrupted observations lasting for about 6 h on average for each sky area and a cadence of about 1 min. Here, we introduce the …

2022 Monthly Notices of the Royal Astronomical Society
Gaia 21
Hidden in the haystack: low-luminosity globular clusters towards the Milky Way bulge
DOI: 10.1093/mnras/stab2463 Bibcode: 2022MNRAS.509.4962G

Rejkuba, M.; Zoccali, M.; Rojas-Arriagada, A. +8 more

Recent wide-area surveys have enabled us to study the Milky Way with unprecedented detail. Its inner regions, hidden behind dust and gas, have been partially unveiled with the arrival of near-infrared (IR) photometric and spectroscopic data sets. Among recent discoveries, there is a population of low-mass globular clusters, known to be missing, es…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 21
The white dwarf binary pathways survey - VI. Two close post-common envelope binaries with TESS light curves
DOI: 10.1093/mnras/stac604 Bibcode: 2022MNRAS.512.1843H

Gänsicke, B. T.; Rebassa-Mansergas, A.; Raddi, R. +9 more

Establishing a large sample of post-common-envelope binaries (PCEBs) that consist of a white dwarf plus an intermediate mass companion star of spectral type AFGK, offers the potential to provide new constraints on theoretical models of white dwarf binary formation and evolution. Here, we present a detailed analysis of two new systems, TYC 110-755-…

2022 Monthly Notices of the Royal Astronomical Society
Gaia eHST 21
Asteroseismology of RR Lyrae stars with non-radial modes
DOI: 10.1093/mnras/stac1793 Bibcode: 2022MNRAS.515.3439N

Smolec, Radosław; Netzel, Henryka

The additional signals observed in the frequency spectra of the first-overtone RR Lyrae stars, which form a period ratio around 0.61 with the period of the first overtone, are a common phenomenon for RRc and RRd stars, as well as for first-overtone classical Cepheids. The recently proposed model explains these signals as harmonics of non-radial mo…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 20
The Mantis Network II: examining the 3D high-resolution observable properties of the UHJs WASP-121b and WASP-189b through GCM modelling
DOI: 10.1093/mnras/stac2246 Bibcode: 2022MNRAS.517..240L

Lee, Elspeth K. H.; Heng, Kevin; Tsai, Shang-Min +4 more

The atmospheres of ultra hot Jupiters (UHJs) are prime targets for the detection of molecules and atoms at both low and high spectral resolution. We study the atmospheres of the UHJs WASP-121b and WASP-189b by performing 3D general circulation models (GCMs) of these planets using high temperature correlated-k opacity schemes with ultra-violet (UV)…

2022 Monthly Notices of the Royal Astronomical Society
eHST 20
A new method for finding nearby white dwarfs exoplanets and detecting biosignatures
DOI: 10.1093/mnras/stac2823 Bibcode: 2022MNRAS.517.2622L

Vanderburg, Andrew; Lustig-Yaeger, Jacob; Stevenson, Kevin B. +5 more

We demonstrate that the James Webb Space Telescope (JWST) can detect infrared (IR) excess from the blended light spectral energy distribution of spatially unresolved terrestrial exoplanets orbiting nearby white dwarfs. We find that JWST is capable of detecting warm (habitable-zone; Teq = 287 K) Earths or super-Earths and hot (400-1000 K…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 20
The impact of a massive Sagittarius dSph on GD-1-like streams
DOI: 10.1093/mnras/stac2311 Bibcode: 2022MNRAS.516.1685D

Price-Whelan, Adrian M.; Belokurov, Vasily; Evans, N. Wyn +1 more

We investigate the effects of a massive ($\gtrsim 4\times 10^{10}\, \mathrm{M}_\odot$) Sagittarius dwarf spheroidal galaxy (Sgr) on stellar streams using test particle simulations in a realistic Milky Way potential. We find that Sgr can easily disrupt streams formed more than ~3 Gyr ago, while stars stripped more recently are generally unaffected.…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 20
The RapidXMM upper limit server: X-ray aperture photometry of the XMM-Newton archival observations
DOI: 10.1093/mnras/stac272 Bibcode: 2022MNRAS.511.4265R

Georgakakis, A.; Georgantopoulos, I.; Kretschmar, P. +4 more

This paper presents the construction of the RapidXMM database that is available through the XMM-Newton Science Archive and offers access to upper limits and aperture photometry across the field of view of the XMM-Newton Pointed and Slew Survey observations. The feature of RapidXMM is speed. It enables the fast retrieval of X-ray upper limits and p…

2022 Monthly Notices of the Royal Astronomical Society
XMM-Newton 20
21 new long-term variables in the GX 339-4 field: two years of MeerKAT monitoring
DOI: 10.1093/mnras/stac756 Bibcode: 2022MNRAS.512.5037D

Heywood, I.; Wijers, R. A. M. J.; Woudt, P. A. +14 more

We present 21 new long-term variable radio sources found commensally in 2 yr of weekly MeerKAT monitoring of the low-mass X-ray binary GX 339-4. The new sources are vary on time-scales of weeks to months and have a variety of light-curve shapes and spectral index properties. Three of the new variable sources are coincident with multiwavelength cou…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 20