Search Publications

The evolution of rest-frame UV properties, Ly α EWs, and the SFR-stellar mass relation at z ∼ 2-6 for SC4K LAEs
DOI: 10.1093/mnras/staa093 Bibcode: 2020MNRAS.493..141S

da Cunha, E.; Arrabal Haro, P.; Sobral, D. +6 more

We explore deep rest-frame UV to FIR data in the COSMOS field to measure the individual spectral energy distributions (SED) of the ∼4000 SC4K (Sobral et al.) Lyman α (Ly α) emitters (LAEs) at z ∼ 2-6. We find typical stellar masses of 109.3 ± 0.6 M and star formation rates (SFR) of SFR_SED=4.4^{+10.5}_{-2.4} M yr…

2020 Monthly Notices of the Royal Astronomical Society
Herschel 47
Superflares and variability in solar-type stars with TESS in the Southern hemisphere
DOI: 10.1093/mnras/staa923 Bibcode: 2020MNRAS.494.3596D

Doyle, J. G.; Ramsay, G.; Doyle, L.

Superflares on solar-type stars have been a rapidly developing field ever since the launch of Kepler. Over the years, there have been several studies investigating the statistics of these explosive events. In this study, we present a statistical analysis of stellar flares on solar-type stars made using photometric data in 2-min cadence from Transi…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 47
Multiple chemodynamic stellar populations of the Ursa Minor dwarf spheroidal galaxy
DOI: 10.1093/mnras/staa1419 Bibcode: 2020MNRAS.495.3022P

Djorgovski, S. G.; Geha, Marla; Simon, Joshua D. +6 more

We present a Bayesian method to identify multiple (chemodynamic) stellar populations in dwarf spheroidal galaxies (dSphs) using velocity, metallicity, and positional stellar data without the assumption of spherical symmetry. We apply this method to a new Keck/Deep Imaging Multi-Object Spectrograph (DEIMOS) spectroscopic survey of the Ursa Minor (U…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 47
Stellar Feedback and Resolved Stellar IFU Spectroscopy in the Nearby Spiral Galaxy NGC 300
DOI: 10.3847/1538-4357/ab6d63 Bibcode: 2020ApJ...891...25M

Kruijssen, J. M. Diederik; Longmore, Steven N.; Chevance, Mélanie +7 more

We present MUSE integral field unit (IFU) observations of five individual H II regions in two giant star-forming complexes in the low-metallicity, nearby dwarf spiral galaxy NGC 300. In combination with high spatial resolution Hubble Space Telescope photometry, we demonstrate the extraction of stellar spectra and classification of individual stars…

2020 The Astrophysical Journal
eHST 47
Mapping the Galactic Disk with the LAMOST and Gaia Red Clump Sample. I. Precise Distances, Masses, Ages, and 3D Velocities of ∼140,000 Red Clump Stars
DOI: 10.3847/1538-4365/ab994f Bibcode: 2020ApJS..249...29H

Wu, Yaqian; Xiang, Maosheng; Huang, Yang +10 more

We present a sample of ∼140,000 primary red clump (RC) stars of spectral signal-to-noise ratios higher than 20 from the Large Sky Area Multi-Object Fibre Spectroscopic Telescope (LAMOST) Galactic spectroscopic surveys, selected based on their positions in the metallicity-dependent effective temperature-surface gravity and color-metallicity diagram…

2020 The Astrophysical Journal Supplement Series
Gaia 47
The growth of brightest cluster galaxies and intracluster light over the past 10 billion years
DOI: 10.1093/mnras/stz3236 Bibcode: 2020MNRAS.491.3751D

Donahue, Megan; Mulchaey, John S.; Connor, Thomas +9 more

We constrain the evolution of the brightest cluster galaxy plus intracluster light (BCG + ICL) using an ensemble of 42 galaxy groups and clusters that span redshifts of z = 0.05-1.75 and masses of M500,c= 2 × 1013-1015 M. Specifically, we measure the relationship between the BCG + ICL stellar mass M

2020 Monthly Notices of the Royal Astronomical Society
eHST 47
Candidate Population III stellar complex at z = 6.629 in the MUSE Deep Lensed Field
DOI: 10.1093/mnrasl/slaa041 Bibcode: 2020MNRAS.494L..81V

Treu, T.; Castellano, M.; Pentericci, L. +20 more

We discovered a strongly lensed (µ ≳ 40) Ly α emission at z = 6.629 (S/N ≃ 18) in the MUSE Deep Lensed Field (MDLF) targeting the Hubble Frontier Field (HFF) galaxy cluster MACS J0416. Dedicated lensing simulations imply that the Ly α emitting region necessarily crosses the caustic. The arc-like shape of the Ly α extends 3 arcsec on the obse…

2020 Monthly Notices of the Royal Astronomical Society
eHST 47
Revisiting MOA 2013-BLG-220L: A Solar-type Star with a Cold Super-Jupiter Companion
DOI: 10.3847/1538-3881/aba2d3 Bibcode: 2020AJ....160..121V

Cole, Andrew A.; Beaulieu, Jean-Philippe; Bond, Ian A. +7 more

We present the analysis of high-resolution images of MOA-2013-BLG-220, taken with the Keck adaptive optics system six years after the initial observation, identifying the lens as a solar-type star hosting a super-Jupiter-mass planet. The masses of planets and host stars discovered by microlensing are often not determined from light-curve data, whi…

2020 The Astronomical Journal
Gaia 47
Age demographics of the Milky Way disc and bulge
DOI: 10.1093/mnras/stz3617 Bibcode: 2020MNRAS.492.3128G

Evans, N. W.; Belokurov, V.; Grady, J.

We exploit the extensive Gaia Data Release 2 set of long-period variables to select a sample of O-rich Miras throughout the Milky Way disc and bulge for study. Exploiting the relation between Mira pulsation period and stellar age/chemistry, we slice the stellar density of the Galactic disc and bulge as a function of period. We find that the morpho…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 47
Gamma-Ray Urgent Archiver for Novel Opportunities (GUANO): Swift/BAT Event Data Dumps on Demand to Enable Sensitive Subthreshold GRB Searches
DOI: 10.3847/1538-4357/aba94f Bibcode: 2020ApJ...900...35T

Cenko, S. Bradley; Palmer, David M.; Barthelmy, Scott +3 more

We introduce a new capability of the Neil Gehrels Swift Observatory to provide event-level data from the Burst Alert Telescope (BAT) on demand in response to transients detected by other instruments. We show that the availability of these data can effectively increase the rate of detections and arcminute localizations of gamma-ray bursts (GRB) lik…

2020 The Astrophysical Journal
INTEGRAL 47