Search Publications

Discovery of a Close-separation Binary Quasar at the Heart of a z ∼ 0.2 Merging Galaxy and Its Implications for Low-frequency Gravitational Waves
DOI: 10.3847/2041-8213/ab2a14 Bibcode: 2019ApJ...879L..21G

Strauss, Michael A.; Mingarelli, Chiara M. F.; Greene, Jenny E. +3 more

Supermassive black hole (SMBH) binaries with masses of ∼108-109 M are expected to dominate the contribution to the as-yet undetected gravitational wave background (GWB) signal at the nanohertz frequencies accessible to pulsar timing arrays. We currently lack firm empirical constraints on the amplitude of the GWB …

2019 The Astrophysical Journal
eHST 53
Fine-scale Explosive Energy Release at Sites of Prospective Magnetic Flux Cancellation in the Core of the Solar Active Region Observed by Hi-C 2.1, IRIS, and SDO
DOI: 10.3847/1538-4357/ab54c1 Bibcode: 2019ApJ...887...56T

Tiwari, Sanjiv K.; Golub, Leon; Winebarger, Amy R. +14 more

The second Hi-C flight (Hi-C 2.1) provided unprecedentedly high spatial and temporal resolution (∼250 km, 4.4 s) coronal EUV images of Fe IX/X emission at 172 Å of AR 12712 on 2018 May 29, during 18:56:21-19:01:56 UT. Three morphologically different types (I: dot-like; II: loop-like; III: surge/jet-like) of fine-scale sudden-brightening events (ti…

2019 The Astrophysical Journal
IRIS 52
Using Surface Brightness Fluctuations to Study Nearby Satellite Galaxy Systems: Calibration and Methodology
DOI: 10.3847/1538-4357/ab22c1 Bibcode: 2019ApJ...879...13C

Greene, Jenny E.; Beaton, Rachael L.; Carlsten, Scott G. +1 more

We explore the use of ground-based surface brightness fluctuation (SBF) measurements to constrain distances to nearby dwarf galaxies. Using archival CFHT Megacam imaging data for a sample of 28 nearby dwarfs, we demonstrate that reliable SBF measurements and distances accurate to 15% are possible even for very low surface brightness (µ

2019 The Astrophysical Journal
eHST 52
The Proper-motion Field along the Magellanic Bridge: A New Probe of the LMC-SMC Interaction
DOI: 10.3847/1538-4357/ab0554 Bibcode: 2019ApJ...874...78Z

van der Marel, Roeland P.; Anderson, J.; Besla, Gurtina +6 more

We present the first detailed kinematic analysis of the proper motions (PMs) of stars in the Magellanic Bridge, from both the Gaia Data Release 2 catalog and from Hubble Space Telescope (HST) Advanced Camera for Surveys data. For the Gaia data, we identify and select two populations of stars in the Bridge region, young main-sequence (MS) and red g…

2019 The Astrophysical Journal
Gaia eHST 52
Fast Outflows Identified in Early Star-forming Galaxies at z = 5-6
DOI: 10.3847/1538-4357/ab49fe Bibcode: 2019ApJ...886...29S

Ouchi, Masami; Blaizot, Jérémy; Bouché, Nicolas +3 more

We present velocities of galactic outflows in seven star-forming galaxies at z = 5-6 with stellar masses of M * ∼ 1010.1 {M}. Although it is challenging to observationally determine the outflow velocities, we overcome this by using ALMA [C II] 158 µm emission lines for systemic velocities and deep Keck spec…

2019 The Astrophysical Journal
eHST 52
The Largest M Dwarf Flares from ASAS-SN
DOI: 10.3847/1538-4357/ab148d Bibcode: 2019ApJ...876..115S

Drout, Maria R.; Kochanek, C. S.; Madore, Barry F. +13 more

The All-sky Automated Survey for Supernovae (ASAS-SN) is the only project in existence to scan the entire sky in optical light approximately every day, reaching a depth of g ∼ 18 mag. Over the course of its first 4 yr of transient alerts (2013-2016), ASAS-SN observed 53 events classified as likely M dwarf flares. We present follow-up photometry an…

2019 The Astrophysical Journal
Gaia 52
On the Gas Content, Star Formation Efficiency, and Environmental Quenching of Massive Galaxies in Protoclusters at z ≈ 2.0-2.5
DOI: 10.3847/1538-4357/ab5302 Bibcode: 2019ApJ...887..183Z

Treister, E.; Toft, S.; Scoville, N. +10 more

We present ALMA Band 6 (ν = 233 GHz, λ = 1.3 mm) continuum observations toward 68 “normal” star-forming galaxies within two Coma-like progenitor structures at z = 2.10 and 2.47, from which ISM masses are derived, providing the largest census of molecular gas mass in overdense environments at these redshifts. Our sample comprises galaxies with a st…

2019 The Astrophysical Journal
eHST 52
A Comparison of Flare Forecasting Methods. III. Systematic Behaviors of Operational Solar Flare Forecasting Systems
DOI: 10.3847/1538-4357/ab2e11 Bibcode: 2019ApJ...881..101L

Leka, K. D.; Gallagher, Peter T.; Murray, Sophie A. +21 more

A workshop was recently held at Nagoya University (2017 October 31-November 2), sponsored by the Center for International Collaborative Research, at the Institute for Space-Earth Environmental Research, Nagoya University, Japan, to quantitatively compare the performance of today’s operational solar flare forecasting facilities. Building upon Paper…

2019 The Astrophysical Journal
SOHO 51
Relationship between the Metallicity of the Circumgalactic Medium and Galaxy Orientation
DOI: 10.3847/1538-4357/ab3b0e Bibcode: 2019ApJ...883...78P

Charlton, Jane C.; Kacprzak, Glenn G.; Churchill, Christopher W. +4 more

We investigate the geometric distribution of gas metallicities in the circumgalactic medium (CGM) around 47, z < 0.7 galaxies from the “Multiphase Galaxy Halos” Survey. Using a combination of quasar spectra from Hubble Space Telescope (HST)/COS and from Keck/HIRES or Very Large Telescope/UVES, we measure column densities of, or determine limits…

2019 The Astrophysical Journal
eHST 51
Far-infrared Properties of the Bright, Gravitationally Lensed Quasar J0439+1634 at z = 6.5
DOI: 10.3847/1538-4357/ab2a02 Bibcode: 2019ApJ...880..153Y

Fan, Xiaohui; Keeton, Charles R.; Walter, Fabian +11 more

We present IRAM NOrthern Extended Millimeter Array, James Clerk Maxwell Telescope/Submillimetre Common-User Bolometer Array-2 and Very Large Array (VLA) observations of the most distant known gravitationally lensed quasar, J0439+1634 at z = 6.5. We detect strong dust emission, [C II] 158 µm, [C I] 369 µm, [O I] 146 µm, CO(6-5), C…

2019 The Astrophysical Journal
eHST 51