Search Publications

OGLE-2017-BLG-1186: first application of asteroseismology and Gaussian processes to microlensing
DOI: 10.1093/mnras/stz1873 Bibcode: 2019MNRAS.488.3308L

Kim, S. -L.; Lee, C. -U.; Bennett, D. P. +102 more

We present the analysis of the event OGLE-2017-BLG-1186 from the 2017 Spitzer microlensing campaign. This is a remarkable microlensing event because its source is photometrically bright and variable, which makes it possible to perform an asteroseismic analysis using ground-based data. We find that the source star is an oscillating red giant with a…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 15
Initial phases of high-mass star formation: a multiwavelength study towards the extended green object G12.42+0.50
DOI: 10.1093/mnras/stz466 Bibcode: 2019MNRAS.485.1775I

Tej, Anandmayee; Liu, Tie; Ishwara Chandra, C. H. +4 more

We present a multiwavelength study of the extended green object, G12.42+0.50, in this paper. The associated ionized, dust, and molecular components of this source are studied in detail employing various observations at near-, mid- and far-infrared, submillimetre, and radio wavelengths. Radio continuum emission mapped at 610 and 1390 MHz, using the…

2019 Monthly Notices of the Royal Astronomical Society
Herschel 15
The nature of the soft excess and spectral variability in the Seyfert 1 galaxy Zw 229.015
DOI: 10.1093/mnras/stz1988 Bibcode: 2019MNRAS.488.4831T

Welsh, W. F.; Gallo, L. C.; Waddell, S. G. H. +2 more

We have carried out a systematic analysis of the nearby (z = 0.0279) active galaxy Zw 229.015 using multi-epoch, multi-instrument, and deep pointed observations with XMM-Newton, Suzaku, Swift,and NuSTAR. Spectral and temporal variability are examined in detail on both the long (weeks-to-years) and short (hours) time-scales. A deep Suzaku observati…

2019 Monthly Notices of the Royal Astronomical Society
Suzaku XMM-Newton 15
Simulating cosmological substructure in the solar neighbourhood
DOI: 10.1093/mnrasl/slz142 Bibcode: 2019MNRAS.490L..32S

Grand, Robert J. J.; Gómez, Facundo A.; Marinacci, Federico +8 more

We explore the predictive power of cosmological, hydrodynamical simulations for stellar phase-space substructure and velocity correlations with the AURIGA simulations and AURIGAIA mock Gaia catalogues. We show that at the solar circle the AURIGA simulations commonly host phase-space structures in the stellar component that have constant orbital en…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 15
TT Arietis: 40 yr of photometry
DOI: 10.1093/mnras/stz2381 Bibcode: 2019MNRAS.489.2961B

Bruch, Albert

In an effort to characterize variations on the time-scale of hours and smaller during the high and low states of the nova-like variable TT Ari, light curves taken over the course of more than 40 yr are analysed. It is found that the well-known negative superhump observed during the high state persists until the present day at an average period of …

2019 Monthly Notices of the Royal Astronomical Society
Gaia 15
Evidence for a clumpy disc-wind in the star-forming Seyfert 2 galaxy MCG-03-58-007
DOI: 10.1093/mnras/sty3327 Bibcode: 2019MNRAS.483.2836M

Campana, S.; Schartel, N.; Santos-Lleó, M. +9 more

We report the results of a detailed analysis of a deep simultaneous 130 ksXMM-Newton and NuSTAR observation of the nearby (z = 0.0315) and bright (L_bol∼ 3× 10^{45} erg s^{-1}) starburst-active galactic nucleus (AGN) Seyfert 2 system: MCG-03-58-007. From the broad-band fitting we show that most of the obscuration needs to be modelled with a toroid…

2019 Monthly Notices of the Royal Astronomical Society
XMM-Newton 15
Molecular envelope around the HII region RCW 120
DOI: 10.1093/mnras/stz2048 Bibcode: 2019MNRAS.488.5641K

Wiebe, D. S.; Anderson, L. D.; Kirsanova, M. S. +5 more

The H II region RCW 120 is a well-known object, which is often considered as a target to verify theoretical models of gas and dust dynamics in the interstellar medium. However, the exact geometry of RCW 120 is still a matter of debate. In this work, we analyse observational data on molecular emission in RCW 120 and show that 13CO(2-1) a…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 15
Using deep Residual Networks to search for galaxy-Ly α emitter lens candidates based on spectroscopic selection
DOI: 10.1093/mnras/sty2708 Bibcode: 2019MNRAS.482..313L

Wang, Jiancheng; Shu, Yiping; Li, Rui +4 more

More than 100 galaxy-scale strong gravitational lens systems have been found by searching for the emission lines coming from galaxies with redshifts higher than the lens galaxies. Based on this spectroscopic-selection method, we introduce the deep Residual Networks (ResNet; a kind of deep Convolutional Neural Networks) to search for the galaxy-Ly …

2019 Monthly Notices of the Royal Astronomical Society
eHST 15
SOFIA/FORCAST resolves 30-40 µm extended dust emission in nearby active galactic nuclei
DOI: 10.1093/mnras/sty3338 Bibcode: 2019MNRAS.483.3404F

Togi, Aditya; Alonso-Herrero, Almudena; Fuller, Lindsay +7 more

We present arcsecond-scale observations of the active galactic nuclei (AGNs) of seven nearby Seyfert galaxies observed from the Stratospheric Observatory For Infrared Astronomy (SOFIA) using the 31.5 and 37.1 µm filters of the Faint Object infraRed CAmera for the SOFIA Telescope (FORCAST). We isolate unresolved emission from the torus and fi…

2019 Monthly Notices of the Royal Astronomical Society
eHST 14
Multiwavelength observations of the EUV variable metal-rich white dwarf GD 394
DOI: 10.1093/mnras/sty3218 Bibcode: 2019MNRAS.483.2941W

Redfield, Seth; Casewell, Sarah L.; Burleigh, Matthew R. +13 more

We present new Hubble Space Telescope (HST) ultraviolet and ground-based optical observations of the hot, metal-rich white dwarf GD 394. Extreme-ultraviolet (EUV) observations in 1992-1996 revealed a 1.15 d periodicity with a 25 per cent amplitude, hypothesized to be due to metals in a surface accretion spot. We obtained phase resolved HST/Space T…

2019 Monthly Notices of the Royal Astronomical Society
Gaia eHST 14