Search Results - "Smith, Martin C."
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The biggest splash
Published in Monthly notices of the Royal Astronomical Society (21-05-2020)“…ABSTRACT Using a large sample of bright nearby stars with accurate Gaia Data Release 2 astrometry and auxiliary spectroscopy we map out the properties of the…”
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Young stars as tracers of a barred-spiral Milky Way
Published in Monthly notices of the Royal Astronomical Society (01-01-2020)“…Abstract Identifying the structure of our Galaxy has always been fraught with difficulties, and while modern surveys continue to make progress building a map…”
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The Pisces Plume and the Magellanic wake
Published in Monthly notices of the Royal Astronomical Society. Letters (01-09-2019)“…ABSTRACT Using RR Lyrae stars in the Gaia Data Release 2 and Pan-STARRS1 we study the properties of the Pisces overdensity, a diffuse substructure in the outer…”
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Blending in gravitational microlensing experiments: source confusion and related systematics
Published in Monthly notices of the Royal Astronomical Society (11-09-2007)“…Gravitational microlensing surveys target very dense stellar fields in the local group. As a consequence, the microlensed source stars are often blended with…”
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The tale of the tail – disentangling the high transverse velocity stars in Gaia DR2
Published in Monthly notices of the Royal Astronomical Society (01-03-2020)“…ABSTRACT Although the stellar halo accounts for just ∼1 per cent of the total stellar mass of the Milky Way, the kinematics of halo stars encode valuable…”
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Using microlensed quasars to probe the structure of the Milky Way
Published in Monthly notices of the Royal Astronomical Society (01-01-2011)“…This paper presents an investigation into the gravitational microlensing of quasars by stars and stellar remnants in the Milky Way. We present predictions for…”
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Chemodynamical properties of the Anticentre Stream: a surviving disc fossil from a past satellite interaction
Published in Monthly notices of the Royal Astronomical Society. Letters (11-02-2020)“…ABSTRACT Using Gaia second data release (DR2), we trace the Anticentre Stream (ACS) in various stellar populations across the sky and find that it is…”
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RESONANT ORBITS AND THE HIGH VELOCITY PEAKS TOWARD THE BULGE
Published in The Astrophysical journal (20-10-2015)“…ABSTRACT We extract the resonant orbits from an N-body bar that is a good representation of the Milky Way, using the method recently introduced by Molloy et…”
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The velocity ellipsoid in the Galactic disc using Gaia DR1
Published in Monthly notices of the Royal Astronomical Society (01-02-2018)“…Abstract The stellar velocity ellipsoid of the solar neighbour (d < 200 pc) is re-examined using intermediate-old mono-abundance stellar groups with…”
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The Lives of Stars: Insights from the TGAS-RAVE-LAMOST Data Set
Published in The Astrophysical journal (20-06-2018)“…In this paper, we investigate how the chemical and kinematic properties of stars vary as a function of age. Using data from a variety of photometric,…”
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A LAMOST BHB Catalog and Kinematics Therein. I. Catalog and Halo Properties
Published in The Astrophysical journal (01-05-2021)“…Abstract In this paper, we collect a sample of stars observed both in LAMOST and Gaia, which have colors implying a temperature hotter than 7000 K. We train a…”
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THE K GIANT STARS FROM THE LAMOST SURVEY DATA. I. IDENTIFICATION, METALLICITY, AND DISTANCE
Published in The Astrophysical journal (01-08-2014)“…We present a support vector machine classifier to identify the K giant stars from the LAMOST survey directly using their spectral line features. The…”
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LAMOST observations in the K2 fields: project and observation progress
Published in EPJ Web of Conferences (01-01-2017)“…To complement the time-series observations of the Kepler space mission in the K2 fields, spectroscopic observations for hundreds of thousands of stars in these…”
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Journal Article Conference Proceeding -
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Modelling the Galactic bar using OGLE-II red clump giant stars
Published in Monthly notices of the Royal Astronomical Society (01-07-2007)“…Red clump giant (RCG) stars can be used as distance indicators to trace the mass distribution of the Galactic bar. We use RCG stars from 44 bulge fields from…”
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RED RUNAWAYS II: LOW-MASS HILLS STARS IN SDSS STRIPE 82
Published in The Astrophysical journal (20-11-2016)“…ABSTRACT Stars ejected from the Galactic Center can be used to place important constraints on the Milky Way potential. Since existing hypervelocity stars are…”
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SELECTING M GIANTS WITH INFRARED PHOTOMETRY: DISTANCES, METALLICITIES, AND THE SAGITTARIUS STREAM
Published in The Astrophysical journal (20-05-2016)“…ABSTRACT Using a spectroscopically confirmed sample of M giants, M dwarfs, and quasars from the LAMOST survey, we assess how well Wide-field Infrared Survey…”
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RESONANT CLUMPING AND SUBSTRUCTURE IN GALACTIC DISKS
Published in The Astrophysical journal (10-05-2015)“…ABSTRACT We describe a method to extract resonant orbits from N-body simulations, exploiting the fact that they close in frames rotating with a constant…”
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SLICING AND DICING THE MILKY WAY DISK IN THE SLOAN DIGITAL SKY SURVEY
Published in The Astrophysical journal (20-02-2012)“…We use the Stripe 82 proper-motion catalog of Bramich et al. to study the kinematics of Galactic disk stars in the solar neighborhood. We select samples of…”
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Searching Extra-tidal Features around the Globular Cluster Whiting 1
Published in The Astrophysical journal (01-05-2022)“…Abstract Whiting 1 is a faint and young globular cluster in the halo of the Milky Way, and was suggested to have originated in the Sagittarius spherical dwarf…”
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The Tilt of the Halo Velocity Ellipsoid and the Shape of the Milky Way Halo
Published in The Astrophysical journal (20-06-2009)“…A sample of ~1800 halo subdwarf stars with radial velocities and proper motions is assembled from Bramich et al.'s light-motion catalog of 2008. This is based…”
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