Search Publications

A Terrestrial-mass Rogue Planet Candidate Detected in the Shortest-timescale Microlensing Event
DOI: 10.3847/2041-8213/abbfad Bibcode: 2020ApJ...903L..11M

Han, Cheongho; Udalski, Andrzej; Lee, Chung-Uk +29 more

Some low-mass planets are expected to be ejected from their parent planetary systems during early stages of planetary system formation. According to planet formation theories, such as the core accretion theory, typical masses of ejected planets should be between 0.3 and 1.0 M. Although in practice such objects do not emit any light, th…

2020 The Astrophysical Journal
Gaia 55
HST Imaging of the Ionizing Radiation from a Star-forming Galaxy at z = 3.794
DOI: 10.3847/1538-4357/ab5fdc Bibcode: 2020ApJ...888..109J

Papovich, Casey; Castellano, Marco; Ferguson, Henry C. +17 more

We report on the Hubble Space Telescope (HST) detection of the Lyman-continuum (LyC) radiation emitted by a galaxy at redshift z = 3.794 dubbed Ion1. The LyC from Ion1 is detected at 820-890 Å with HST WFC3/UVIS in the F410M band (m410 = 27.60 ± 0.36 mAB, peak signal-to-noise ratio (S/N) = 4.17 in an r = 0"12 aperture) and 70…

2020 The Astrophysical Journal
eHST 54
PopSyCLE: A New Population Synthesis Code for Compact Object Microlensing Events
DOI: 10.3847/1538-4357/ab5fd3 Bibcode: 2020ApJ...889...31L

Hosek, Matthew W., Jr.; Lu, Jessica R.; Dawson, William A. +2 more

We present a new Milky Way microlensing simulation code, dubbed PopSyCLE (Population Synthesis for Compact object Lensing Events). PopSyCLE is the first resolved microlensing simulation to include a compact object distribution derived from numerical supernova explosion models and both astrometric and photometric microlensing effects. We demonstrat…

2020 The Astrophysical Journal
Gaia 54
Probing the Bright End of the Rest-frame Ultraviolet Luminosity Function at z = 8-10 with Hubble Pure-parallel Imaging
DOI: 10.3847/1538-4357/ab7659 Bibcode: 2020ApJ...891..146R

Finkelstein, Steven L.; Bagley, Micaela B.; Rojas-Ruiz, Sofía +5 more

Looking for bright galaxies born in the early universe is fundamental to investigating the Epoch of Reionization, the era when the first stars and galaxies ionized the intergalactic medium. We utilize Hubble Space Telescope pure-parallel imaging to select galaxy candidates at a time 500-650 million years after the Big Bang, which corresponds to re…

2020 The Astrophysical Journal
eHST 54
Chemical Evolution in the Milky Way: Rotation-based Ages for APOGEE-Kepler Cool Dwarf Stars
DOI: 10.3847/1538-4357/ab5c24 Bibcode: 2020ApJ...888...43C

van Saders, Jennifer L.; García, Rafael A.; Claytor, Zachary R. +5 more

We use models of stellar angular momentum evolution to determine ages for ∼500 stars in the APOGEE-Kepler Cool Dwarfs sample. We focus on lower-main-sequence stars, where other age-dating tools become ineffective. Our age distributions are compared to those derived from asteroseismic and giant samples and solar analogs. We are able to recover gyro…

2020 The Astrophysical Journal
Gaia 54
CLEAR. II. Evidence for Early Formation of the Most Compact Quiescent Galaxies at High Redshift
DOI: 10.3847/1538-4357/aba004 Bibcode: 2020ApJ...898..171E

Papovich, Casey; Finkelstein, Steven L.; Cleri, Nikko J. +11 more

The origin of the correlations between mass, morphology, quenched fraction, and formation history in galaxies is difficult to define, primarily due to the uncertainties in galaxy star formation histories (SFHs). SFHs are better constrained for higher redshift galaxies, observed closer to their formation and quenching epochs. Here we use "nonparame…

2020 The Astrophysical Journal
eHST 53
Microwave Spectral Imaging of an Erupting Magnetic Flux Rope: Implications for the Standard Solar Flare Model in Three Dimensions
DOI: 10.3847/2041-8213/ab901a Bibcode: 2020ApJ...895L..50C

Reeves, Katharine K.; Chen, Bin; Yu, Sijie +1 more

We report microwave spectral imaging observations of an erupting magnetic flux rope during the early impulsive phase of the X8.2-class limb flare on 2017 September 10, obtained by the Expanded Owens Valley Solar Array. A few days prior to the eruption, when viewed against the disk, the flux rope appeared as a reverse S-shaped dark filament along t…

2020 The Astrophysical Journal
Hinode 53
Multiwavelength Variability of BL Lacertae Measured with High Time Resolution
DOI: 10.3847/1538-4357/aba693 Bibcode: 2020ApJ...900..137W

Chen, W. P.; Villata, M.; Carnerero, M. I. +54 more

In an effort to locate the sites of emission at different frequencies and physical processes causing variability in blazar jets, we have obtained high time-resolution observations of BL Lacertae over a wide wavelength range: with the Transiting Exoplanet Survey Satellite (TESS) at 6000-10000 Å with 2 minute cadence; with the Neil Gehrels Swift sat…

2020 The Astrophysical Journal
Gaia 53
An Evolutionary Study of Volatile Chemistry in Protoplanetary Disks
DOI: 10.3847/1538-4357/ab9e71 Bibcode: 2020ApJ...898...97B

Wilner, David J.; Cleeves, L. Ilsedore; Andrews, Sean M. +11 more

The volatile composition of a planet is determined by the inventory of gas and ice in the parent disk. The volatile chemistry in the disk is expected to evolve over time, though this evolution is poorly constrained observationally. We present Atacama Large Millimeter/submillimeter Array observations of C18O, C2H, and the isot…

2020 The Astrophysical Journal
Gaia 53
A Very Young Radio-loud Magnetar
DOI: 10.3847/2041-8213/ab9742 Bibcode: 2020ApJ...896L..30E

Campana, S.; Tiengo, A.; Götz, D. +20 more

The magnetar Swift J1818.0-1607 was discovered in 2020 March when Swift detected a 9 ms hard X-ray burst and a long-lived outburst. Prompt X-ray observations revealed a spin period of 1.36 s, soon confirmed by the discovery of radio pulsations. We report here on the analysis of the Swift burst and follow-up X-ray and radio observations. The burst …

2020 The Astrophysical Journal
XMM-Newton 53