Search Publications

Blanco DECam Bulge Survey (BDBS) II: project performance, data analysis, and early science results
DOI: 10.1093/mnras/staa2393 Bibcode: 2020MNRAS.499.2357J

Clarkson, William I.; Kunder, Andrea; Johnson, Christian I. +7 more

The Blanco DECam Bulge Survey (BDBS) imaged more than 200 sq deg of the Southern Galactic bulge using the ugrizY filters of the Dark Energy Camera, and produced point spread function photometry of approximately 250 million unique sources. In this paper, we present details regarding the construction and collation of survey catalogues, and also disc…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 30
NGTS-10b: the shortest period hot Jupiter yet discovered
DOI: 10.1093/mnras/staa115 Bibcode: 2020MNRAS.493..126M

Smalley, Barry; Jackman, James A. G.; Wheatley, Peter J. +44 more

We report the discovery of a new ultrashort period (USP) transiting hot Jupiter from the Next Generation Transit Survey (NGTS). NGTS-10b has a mass and radius of 2.162 ^{+0.092}_{-0.107} MJ and 1.205 ^{+0.117}_{-0.083} RJ and orbits its host star with a period of 0.7668944 ± 0.0000003 d, making it the shortest period hot Jupi…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 30
Probing the circumnuclear absorbing medium of the buried AGN in NGC 1068 through NuSTAR observations
DOI: 10.1093/mnras/staa107 Bibcode: 2020MNRAS.492.3872Z

Bauer, F. E.; Brandt, W. N.; Bianchi, S. +9 more

We present the results of the latest NuSTAR monitoring campaign of the Compton-thick Seyfert 2 galaxy NGC 1068, composed of four ∼50 ks observations performed between 2017 July and 2018 February to search for flux and spectral variability on time-scales from 1 to 6 months. We detect one unveiling and one eclipsing event with time-scales less than …

2020 Monthly Notices of the Royal Astronomical Society
XMM-Newton 29
The distribution of relative proper motions of wide binaries in Gaia DR2: MOND or multiplicity?
DOI: 10.1093/mnrasl/slz161 Bibcode: 2020MNRAS.491L..72C

Clarke, C. J.

We examine the distribution of on-sky relative velocities for wide binaries previously assembled from theGaia DR2 data and focus on the origin of the high-velocity tail of apparently unbound systems, which may be interpreted as evidence for non-Newtonian gravity in the weak field limit. We argue that this tail is instead explicable in terms of a p…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 29
Inverse stellar population age gradients of post-starburst galaxies at z = 0.8 with LEGA-C
DOI: 10.1093/mnras/staa1937 Bibcode: 2020MNRAS.497..389D

Bell, Eric F.; D'Eugenio, Francesco; Franx, Marijn +13 more

We use deep, spatially resolved spectroscopy from the Large Early Galaxy Astrophysics Census Survey to study radial variations in the stellar population of 17 spectroscopically selected post-starburst (PSB) galaxies. We use spectral fitting to measure two Lick indices, H δA and Fe 4383 , and find that, on average, PSB galaxies have radi…

2020 Monthly Notices of the Royal Astronomical Society
eHST 29
Unsupervised machine learning for transient discovery in deeper, wider, faster light curves
DOI: 10.1093/mnras/staa2395 Bibcode: 2020MNRAS.498.3077W

Andreoni, Igor; Mahabal, Ashish; Cooke, Jeff +7 more

Identification of anomalous light curves within time-domain surveys is often challenging. In addition, with the growing number of wide-field surveys and the volume of data produced exceeding astronomers' ability for manual evaluation, outlier and anomaly detection is becoming vital for transient science. We present an unsupervised method for trans…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 29
Atmospheric compositions and observability of nitrogen-dominated ultra-short-period super-Earths
DOI: 10.1093/mnras/staa724 Bibcode: 2020MNRAS.494.1490Z

Mollière, Paul; Tsai, Shang-Min; Miguel, Yamila +1 more

We explore the chemistry and observability of nitrogen-dominated atmospheres for ultra-short-period super-Earths. We base the assumption that super-Earths could have nitrogen-filled atmospheres on observations of 55 Cancri e that favour a scenario with a high-mean-molecular-weight atmosphere. We take Titan's elemental budget as our starting point …

2020 Monthly Notices of the Royal Astronomical Society
IUE 28
Lithium and beryllium in the Gaia-Enceladus galaxy
DOI: 10.1093/mnras/staa1653 Bibcode: 2020MNRAS.496.2902M

Molaro, P.; Cescutti, G.; Fu, X.

Data from Gaia DR2 and The Apache Point Observatory Galactic Evolution Experiment surveys revealed a relatively new component in the inner Galactic halo, which is likely the dynamical remnant of a disrupted dwarf galaxy named Gaia-Enceladus that collided with the Milky Way about 10 Gyr ago. This merging event offers an extraordinary opportunity to…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 28
SMASHing the low surface brightness SMC
DOI: 10.1093/mnras/staa2451 Bibcode: 2020MNRAS.498.1034M

Bell, Eric F.; Monachesi, Antonela; Choi, Yumi +22 more

The periphery of the Small Magellanic Cloud (SMC) can unlock important information regarding galaxy formation and evolution in interacting systems. Here, we present a detailed study of the extended stellar structure of the SMC using deep colour-magnitude diagrams, obtained as part of the Survey of the MAgellanic Stellar History (SMASH). Special ca…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 28
Crystalline silicate absorption at 11.1 µm: ubiquitous and abundant in embedded YSOs and the interstellar medium
DOI: 10.1093/mnras/staa396 Bibcode: 2020MNRAS.493.4463D

Wright, Christopher M.; Fujiyoshi, Takuya; Siebenmorgen, Ralf +5 more

Utilizing several instruments on 4-8 m telescopes, we have observed a large sample of objects in the mid-infrared (8-13 µm). These comprise a few evolved stars, multiple envelopes of embedded young stellar objects (YSOs) or compact H-II regions, and several sightlines through the interstellar medium (ISM). The latter is where dust resides - …

2020 Monthly Notices of the Royal Astronomical Society
ISO 28