Search Publications

The PAU Survey: Photometric redshifts using transfer learning from simulations
DOI: 10.1093/mnras/staa2265 Bibcode: 2020MNRAS.497.4565E

Carretero, J.; Castander, F. J.; Gaztanaga, E. +15 more

In this paper, we introduce the DEEPZ deep learning photometric redshift (photo-z) code. As a test case, we apply the code to the PAU survey (PAUS) data in the COSMOS field. DEEPZ reduces the σ68 scatter statistic by 50 per cent at iAB = 22.5 compared to existing algorithms. This improvement is achieved through various method…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 31
New and improved rotational periods of magnetic CP stars from ASAS-3, KELT, and MASCARA data
DOI: 10.1093/mnras/staa462 Bibcode: 2020MNRAS.493.3293B

Paunzen, Ernst; Hümmerich, Stefan; Bernhard, Klaus

Magnetic chemically peculiar (mCP) stars allow the investigation of such diverse phenomena as atomic diffusion, magnetic fields, and stellar rotation. The aim of the present investigation is to enhance our knowledge of the rotational properties of mCP stars by increasing the sample of objects with accurately determined rotational periods. To this …

2020 Monthly Notices of the Royal Astronomical Society
Gaia 31
Precise astrometry and diameters of asteroids from occultations - a data set of observations and their interpretation
DOI: 10.1093/mnras/staa3077 Bibcode: 2020MNRAS.499.4570H

Herald, David; Gault, David; Anderson, Robert +10 more

Occultations of stars by asteroids have been observed since 1961, increasing from a very small number to now over 500 annually. We have created and regularly maintain a growing data set of more than 5000 observed asteroidal occultations. The data set includes the raw observations, astrometry at the 1 mas level based on centre of mass or figure (no…

2020 Monthly Notices of the Royal Astronomical Society
AKARI 30
A SkyMapper view of the Large Magellanic Cloud: the dynamics of stellar populations
DOI: 10.1093/mnras/stz3493 Bibcode: 2020MNRAS.492..782W

Lewis, Geraint F.; Ibata, Rodrigo A.; Mackey, Dougal +2 more

We present the first SkyMapper stellar population analysis of the Large Magellanic Cloud (hereafter LMC), including the identification of 3578 candidate Carbon Stars through their extremely red g - r colours. Coupled with Gaia astrometry, we analyse the distribution and kinematics of this Carbon Star population, finding the LMC to be centred at (R…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 30
Blue straggler populations of seven open clusters with Gaia DR2
DOI: 10.1093/mnras/staa1667 Bibcode: 2020MNRAS.496.2402V

Vaidya, Kaushar; Rao, Khushboo K.; Agarwal, Manan +1 more

Blue straggler stars (BSS) are well studied in globular clusters but their systematic study with secure membership determination is lacking in open clusters. We use Gaia DR2 data to determine accurate stellar membership for four intermediate-age open clusters, namely Melotte 66, NGC 2158, NGC 2506, and NGC 6819, and three old open clusters, namely…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 30
Survey of planetesimal belts with ALMA: gas detected around the Sun-like star HD 129590
DOI: 10.1093/mnras/staa2038 Bibcode: 2020MNRAS.497.2811K

Kral, Quentin; Wyatt, Mark C.; Kennedy, Grant M. +2 more

Gas detection around main-sequence stars is becoming more common with around 20 systems showing the presence of CO. However, more detections are needed, especially around later spectral type stars to better understand the origin of this gas and refine our models. To do so, we carried out a survey of 10 stars with predicted high likelihoods of seco…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 30
Recipes for bolometric corrections and Gaia luminosities of B-type stars: application to an asteroseismic sample
DOI: 10.1093/mnras/staa1292 Bibcode: 2020MNRAS.495.2738P

Aerts, Conny; Escorza, Ana; Pedersen, May G. +1 more

We provide three statistical model prescriptions for the bolometric corrections appropriate for B-type stars as a function of (I) Teff, (II) Teff and log g, and (III)Teff, log g and [M/H]. These statistical models have been calculated for 27 different filters, including those of the Gaia space mission, and were der…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 30
The SUrvey for Pulsars and Extragalactic Radio Bursts - IV. Discovery and polarimetry of a 12.1-s radio pulsar
DOI: 10.1093/mnras/staa321 Bibcode: 2020MNRAS.493.1165M

Ray, P. S.; Kramer, M.; Johnston, S. +19 more

We report the discovery of PSR J2251-3711, a radio pulsar with a spin period of 12.1 s, the second longest currently known. Its timing parameters imply a characteristic age of 15 Myr, a surface magnetic field of 1.3 × 1013 G, and a spin-down luminosity of 2.9 × 1029 erg s-1. Its dispersion measure of 12.12(1) pc cm…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 30
Core-collapse supernovae in binaries as the origin of galactic hyper-runaway stars
DOI: 10.1093/mnras/staa2334 Bibcode: 2020MNRAS.497.5344E

Rossi, E. M.; Renzo, M.; Evans, F. A.

Several stars detected moving at velocities near to or exceeding the Galactic escape speed likely originated in the Milky Way disc. We quantitatively explore the 'binary supernova scenario' hypothesis, wherein these 'hyper-runaway' stars are ejected at large peculiar velocities when their close, massive binary companions undergo a core-collapse su…

2020 Monthly Notices of the Royal Astronomical Society
Gaia eHST 30
MKT J170456.2-482100: the first transient discovered by MeerKAT
DOI: 10.1093/mnras/stz3027 Bibcode: 2020MNRAS.491..560D

Heywood, I.; Wijers, R. A. M. J.; Woudt, P. A. +19 more

We report the discovery of the first transient with MeerKAT, MKT J170456.2-482100, discovered in ThunderKAT images of the low-mass X-ray binary GX339-4. MKT J170456.2-482100 is variable in the radio, reaching a maximum flux density of 0.71± 0.11 mJy on 2019 October 12, and is undetected in 15 out of 48 ThunderKAT epochs. MKT J170456.2-482100 is co…

2020 Monthly Notices of the Royal Astronomical Society
Gaia Hipparcos 30