Search Publications

To TDE or not to TDE: the luminous transient ASASSN-18jd with TDE-like and AGN-like qualities
DOI: 10.1093/mnras/staa859 Bibcode: 2020MNRAS.494.2538N

Gromadzki, M.; Kochanek, C. S.; Foley, R. J. +26 more

We present the discovery of ASASSN-18jd (AT 2018bcb), a luminous optical/ultraviolet(UV)/X-ray transient located in the nucleus of the galaxy 2MASX J22434289-1659083 at z = 0.1192. Over the year after discovery, Swift UltraViolet and Optical Telescope (UVOT) photometry shows the UV spectral energy distribution of the transient to be well modelled …

2020 Monthly Notices of the Royal Astronomical Society
XMM-Newton eHST 56
Hic sunt dracones: Cartography of the Milky Way spiral arms and bar resonances with Gaia Data Release 2
DOI: 10.1051/0004-6361/201936645 Bibcode: 2020A&A...634L...8K

Katz, D.; Haywood, M.; Gerhard, O. +5 more

In this paper we introduce a new method for analysing Milky Way phase-space which allows us to reveal the imprint left by the Milky Way bar and spiral arms on the stars with full phase-space data in Gaia Data Release 2. The unprecedented quality and extended spatial coverage of these data allowed us to discover six prominent stellar density struct…

2020 Astronomy and Astrophysics
Gaia 56
The Gaia reference frame for bright sources examined using VLBI observations of radio stars
DOI: 10.1051/0004-6361/201936161 Bibcode: 2020A&A...633A...1L

Lindegren, Lennart

Context. Positions and proper motions of Gaia sources are expressed in a reference frame that ideally should be non-rotating relative to distant extragalactic objects, coincident with the International Celestial Reference System (ICRS), and consistent across all magnitudes. For sources fainter than 16th magnitude, this is achieved through Gaia's d…

2020 Astronomy and Astrophysics
Gaia Hipparcos 56
Fundamental parameters for 45 open clusters with Gaia DR2, an improved extinction correction and a metallicity gradient prior
DOI: 10.1093/mnras/staa2983 Bibcode: 2020MNRAS.499.1874M

Cantat-Gaudin, T.; Moitinho, A.; Paunzen, E. +4 more

Reliable fundamental parameters of open clusters (OCs) such as distance, age, and extinction are key to our understanding of Galactic structure and stellar evolution. In this work, we use Gaia Data Release 2 (DR2) to investigate 45 OCs listed in the New catalogue of optically visible open clusters and candidates (DAML) but with no previous astrome…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 56
Nondetection of Helium in the Upper Atmospheres of Three Sub-Neptune Exoplanets
DOI: 10.3847/1538-3881/abbee6 Bibcode: 2020AJ....160..258K

Désert, Jean-Michel; Mansfield, Megan; Kasper, David +5 more

We present a search for helium in the upper atmospheres of three sub-Neptune-sized planets to investigate the origins of these ubiquitous objects. The detection of helium for a low-density planet would be strong evidence for the presence of a primary atmosphere accreted from the protoplanetary nebula because large amounts of helium are not expecte…

2020 The Astronomical Journal
Gaia 56
Are inner disc misalignments common? ALMA reveals an isotropic outer disc inclination distribution for young dipper stars
DOI: 10.1093/mnras/stz3361 Bibcode: 2020MNRAS.492..572A

Tazzari, M.; Williams, J. P.; Ansdell, M. +12 more

Dippers are a common class of young variable star exhibiting day-long dimmings with depths of up to several tens of per cent. A standard explanation is that dippers host nearly edge-on (Id ≈ 70°) protoplanetary discs that allow close-in (<1 au) dust lifted slightly out of the mid-plane to partially occult the star. The identification…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 56
Varstrometry for Off-nucleus and Dual Subkiloparsec AGN (VODKA): Methodology and Initial Results with Gaia DR2
DOI: 10.3847/1538-4357/ab5c1a Bibcode: 2020ApJ...888...73H

Shen, Yue; Hwang, Hsiang-Chih; Liu, Xin +1 more

Gaia’s precision astrometry allows systematic identification of optically selected subkiloparsec dual active galactic nuclei (AGNs), off-nucleus AGNs, and small-scale lensed quasars by “varstrometry”—where variability-induced astrometric jitter, I.e., temporal displacements of photocenter in unresolved sources, can be reasonably well detected or c…

2020 The Astrophysical Journal
Gaia 56
Globular clusters in the inner Galaxy classified from dynamical orbital criteria
DOI: 10.1093/mnras/stz3162 Bibcode: 2020MNRAS.491.3251P

Barbuy, Beatriz; Bica, Eduardo; Pérez-Villegas, Angeles +3 more

Globular clusters (GCs) are the most ancient stellar systems in the Milky Way. Therefore, they play a key role in the understanding of the early chemical and dynamical evolution of our Galaxy. Around 40 per cent of them are placed within ∼4 kpc from the Galactic centre. In that region, all Galactic components overlap, making their disentanglement …

2020 Monthly Notices of the Royal Astronomical Society
Gaia 56
Cluster Difference Imaging Photometric Survey. II. TOI 837: A Young Validated Planet in IC 2602
DOI: 10.3847/1538-3881/abb9ab Bibcode: 2020AJ....160..239B

Barbieri, M.; Henning, T.; Winn, J. N. +42 more

We report the discovery of TOI 837b and its validation as a transiting planet. We characterize the system using data from the NASA Transiting Exoplanet Survey Satellite mission, the ESA Gaia mission, ground-based photometry from El Sauce and ASTEP400, and spectroscopy from CHIRON, FEROS, and Veloce. We find that TOI 837 is a T = 9.9 mag G0/F9 dwar…

2020 The Astronomical Journal
Gaia 56
Three Lyα Emitting Galaxies within a Quasar Proximity Zone at z ∼ 5.8
DOI: 10.3847/1538-4357/ab85cd Bibcode: 2020ApJ...896...49B

Ellis, Richard S.; Bosman, Sarah E. I.; Meyer, Romain A. +3 more

Quasar proximity zones at $z\gt 5.5$ correspond to overdense and overionized environments. Galaxies found inside proximity zones can therefore display features that would otherwise be masked by absorption in the intergalactic medium. We demonstrate the utility of this quasar-galaxy synergy by reporting the discovery of the first three "proximate L…

2020 The Astrophysical Journal
eHST 56