activity
20122020
most cited197 Candidates and 104 Validated Planets in K2's First Five Fields

214 citations · 3.2k across the 79 of their papers we have counts for

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17 papers · 1 filter

astro-ph.SR2020★ 10 cited

EPIC 216747137: a new HW Vir eclipsing binary with a massive sdOB primary and a low-mass M-dwarf companion

R. Silvotti, V. Schaffenroth, U. Heber +8

EPIC 216747137 is a new HW~Virginis system discovered by the Kepler spacecraft during its K2 "second life". Like the other HW Vir systems, EPIC 216747137 is a post-common-envelope…

astro-ph.SR2019★ 11 cited

The PDS 110 observing campaign - photometric and spectroscopic observations reveal eclipses are aperiodic

Hugh P. Osborn, Matthew Kenworthy, Joseph E. Rodriguez +71

PDS 110 is a young disk-hosting star in the Orion OB1A association. Two dimming events of similar depth and duration were seen in 2008 (WASP) and 2011 (KELT), consistent with an ob…

astro-ph.SR2018★ 8 cited

Radial velocity survey of spatially resolved young, low-mass binaries

Stephen Durkan, Markus Janson, Simona Ciceri +6

The identification and characterisation of low-mass binaries is of importance for a range of astrophysical investigations. Low-mass binaries in young ( Myr) moving g…

astro-ph.SR2018★ 33 cited

Microlensing Parallax for OGLE-2017-BLG-0896 Reveals a Counter-Rotating Low-Mass Brown Dwarf

Yossi Shvartzvald, Jennifer C. Yee, Jan Skowron +63

The kinematics of isolated brown dwarfs in the Galaxy, beyond the solar neighborhood, is virtually unknown. Microlensing has the potential to probe this hidden population, as it ca…

astro-ph.SR2018★ 6 cited

OGLE-2017-BLG-0329L: A Microlensing Binary Characterized with Dramatically Enhanced Precision Using Data from Space-based Observations

C. Han, S. Calchi Novati, A. Udalski +54

Mass measurements of gravitational microlenses require one to determine the microlens parallax $\pie$, but precise $\pie$ measurement, in many cases, is hampered due to the subtlet…

astro-ph.SR2017★ 28 cited

Stellar & Planetary Parameters for K2's Late Type Dwarf Systems from C1 to C5

Arturo O. Martinez, Ian J. M. Crossfield, Joshua E. Schlieder +12

The NASA K2 mission uses photometry to find planets transiting stars of various types. M dwarfs are of high interest since they host more short period planets than any other type o…

astro-ph.SR2016★ 25 cited

OGLE-2015-BLG-0479LA,B: Binary Gravitational Microlens Characterized by Simultaneous Ground-based and Space-based Observation

C. Han, A. Udalski, A. Gould +60

We present a combined analysis of the observations of the gravitational microlensing event OGLE-2015-BLG-0479 taken both from the ground and by the {\it Spitzer Space Telescope}. T…

astro-ph.SR2016★ 8 cited

Many new variable stars discovered in the core of the globular cluster NGC 6715 (M54) with EMCCD observations

R. Figuera Jaimes, D. M. Bramich, N. Kains +38

We show the benefits of using Electron-Multiplying CCDs and the shift-and-add technique as a tool to minimise the effects of the atmospheric turbulence such as blending between sta…

astro-ph.SR2015

Exploring the crowded central region of 10 Galactic globular clusters using EMCCDs. Variable star searches and new discoveries

R. Figuera Jaimes, D. M. Bramich, J. Skottfelt +31

Obtain time-series photometry of the very crowded central regions of Galactic globular clusters with better angular resolution than previously achieved with conventional CCDs on gr…

astro-ph.SR2015★ 23 cited

Spitzer Microlensing Program as a Probe for Globular Cluster Planets. Analysis of OGLE-2015-BLG-0448

Radosław Poleski, Wei Zhu, Grant W. Christie +83

The microlensing event OGLE-2015-BLG-0448 was observed by Spitzer and lay within the tidal radius of the globular cluster NGC 6558. The event had moderate magnification and was int…

astro-ph.SR2015★ 14 cited

Rotation periods and astrometric motions of the Luhman 16AB brown dwarfs by high-resolution lucky-imaging monitoring

L. Mancini, P. Giacobbe, S. P. Littlefair +33

Context. Photometric monitoring of the variability of brown dwarfs can provide useful information about the structure of clouds in their cold atmospheres. The brown-dwarf binary sy…

astro-ph.SR2015★ 54 cited

Mass Measurements of Isolated Objects from Space-based Microlensing

Wei Zhu, S. Calchi Novati, A. Gould +78

We report on the mass and distance measurements of two single-lens events from the 2015 \emph{Spitzer} microlensing campaign. With both finite-source effect and microlens parallax…

astro-ph.SR2015

A 0.24+0.18 Msun double-lined eclipsing binary from the HATSouth survey

G. Zhou, D. Bayliss, J. D. Hartman +21

We report the discovery and characterisation of a new M-dwarf binary, with component masses and radii of M1 = 0.244 -0.003/+0.003 Msun, R1 = 0.261 -0.009/+0.006 Rsun, M2 = 0.179 -0…

astro-ph.SR2015★ 24 cited

A Census of Variability in Globular Cluster M68 (NGC 4590)

N. Kains, A. Arellano Ferro, R. Figuera Jaimes +32

We analyse 20 nights of CCD observations in the V and I bands of the globular cluster M68 (NGC 4590), using these to detect variable objects. We also obtained electron-multiplying…

astro-ph.SR2014★ 29 cited

Searching for variable stars in the cores of five metal rich globular clusters using EMCCD observations

Jesper Skottfelt, D. M. Bramich, R. Figuera Jaimes +31

In this paper, we present the analysis of time-series observations from 2013 and 2014 of five metal rich ([Fe/H] -1) globular clusters: NGC~6388, NGC~6441, NGC~6528, NGC~6638,…

astro-ph.SR2013★ 95 cited

Weather on the Nearest Brown Dwarfs: Resolved Simultaneous Multi-Wavelength Variability Monitoring of WISE J104915.57-531906.1AB

Beth A. Biller, Ian J. M. Crossfield, Luigi Mancini +15

We present two epochs of MPG/ESO 2.2m GROND simultaneous 6-band () photometric monitoring of the closest known L/T transition brown dwarf binary WISE J104915.57-531906.1…

astro-ph.SR2013★ 139 cited

The GAPS programme with HARPS-N at TNG. I: Observations of the Rossiter-McLaughlin effect and characterisation of the transiting system Qatar-1

E. Covino, M. Esposito, M. Barbieri +67

A long-term multi-purpose observational programme has started with HARPS-N@TNG aimed to characterise the global architectural properties of exoplanetary systems. In this first pape…