Search Publications

The CO Luminosity Density at High-z (COLDz) Survey: A Sensitive, Large-area Blind Search for Low-J CO Emission from Cold Gas in the Early Universe with the Karl G. Jansky Very Large Array
DOI: 10.3847/1538-4357/aacb79 Bibcode: 2018ApJ...864...49P

Dickinson, Mark; Smail, Ian; Daddi, Emanuele +16 more

We describe the CO Luminosity Density at High-z (COLDz) survey, the first spectral line deep field targeting CO(1-0) emission from galaxies at z = 1.95-2.85 and CO(2-1) at z = 4.91-6.70. The main goal of COLDz is to constrain the cosmic density of molecular gas at the peak epoch of cosmic star formation. By targeting both a wide (∼51 arcmin2<…

2018 The Astrophysical Journal
eHST 91
Hitomi (ASTRO-H) X-ray Astronomy Satellite
DOI: 10.1117/1.JATIS.4.2.021402 Bibcode: 2018JATIS...4b1402T

Done, Chris; Safi-Harb, Samar; Hamaguchi, Kenji +267 more

The Hitomi (ASTRO-H) mission is the sixth Japanese x-ray astronomy satellite developed by a large international collaboration, including Japan, USA, Canada, and Europe. The mission aimed to provide the highest energy resolution ever achieved at E > 2 keV, using a microcalorimeter instrument, and to cover a wide energy range spanning four decade…

2018 Journal of Astronomical Telescopes, Instruments, and Systems
Hitomi 91
The 1.5 Ms observing campaign on IRAS 13224-3809 - I. X-ray spectral analysis
DOI: 10.1093/mnras/sty836 Bibcode: 2018MNRAS.477.3711J

Harrison, F. A.; Fabian, A. C.; Miller, J. M. +16 more

We present a detailed spectral analysis of the recent 1.5 Ms XMM-Newton observing campaign on the narrow-line Seyfert 1 galaxy IRAS 13224-3809, taken simultaneously with 500 ks of NuSTAR data. The X-ray light curve shows three flux peaks, registering at about 100 times the minimum flux seen during the campaign, and rapid variability with a time-sc…

2018 Monthly Notices of the Royal Astronomical Society
XMM-Newton 91
Production of Cool Gas in Thermally Driven Outflows
DOI: 10.3847/1538-4357/aacce1 Bibcode: 2018ApJ...862...56S

Robertson, Brant E.; Thompson, Todd A.; Schneider, Evan E.

Galactic outflows commonly contain multiphase gas, and its physical origin requires explanation. Using the Cholla Galactic OutfLow Simulations suite of high-resolution isolated galaxy models, we demonstrate the viability of rapid radiative cooling as a source of fast-moving (v ∼ 1000 km s-1), cool (104 K) gas observed in abso…

2018 The Astrophysical Journal
eHST 91
Hubble Space Telescope Observations of Extended [O III]λ 5007 Emission in Nearby QSO2s: New Constraints on AGN Host Galaxy Interaction
DOI: 10.3847/1538-4357/aab03e Bibcode: 2018ApJ...856..102F

Turner, T. J.; Kraemer, S. B.; Crenshaw, D. M. +15 more

We present a Hubble Space Telescope survey of extended [O III] λ5007 emission for a sample of 12 nearby (z < 0.12), luminous Type 2 quasars (QSO2s), which we use to measure the extent and kinematics of their AGN-ionized gas. We find that the size of the observed [O III] regions scale with luminosity in comparison to nearby, less luminous Seyfer…

2018 The Astrophysical Journal
eHST 90
Successive X-class Flares and Coronal Mass Ejections Driven by Shearing Motion and Sunspot Rotation in Active Region NOAA 12673
DOI: 10.3847/1538-4357/aab153 Bibcode: 2018ApJ...856...79Y

Feng, X. S.; Yan, X. L.; Xue, Z. K. +5 more

We present a clear case study on the occurrence of two successive X-class flares, including a decade-class flare (X9.3) and two coronal mass ejections (CMEs) triggered by shearing motion and sunspot rotation in active region NOAA 12673 on 2017 September 6. A shearing motion between the main sunspots with opposite polarities began on September 5 an…

2018 The Astrophysical Journal
SOHO 90
High-precision stellar abundances of the elements: methods and applications
DOI: 10.1007/s00159-018-0111-3 Bibcode: 2018A&ARv..26....6N

Nissen, Poul Erik; Gustafsson, Bengt

Efficient spectrographs at large telescopes have made it possible to obtain high-resolution spectra of stars with high signal-to-noise ratio and advances in model atmosphere analyses have enabled estimates of high-precision differential abundances of the elements from these spectra, i.e. with errors in the range 0.01-0.03 dex for F, G, and K stars…

2018 Astronomy and Astrophysics Review
Gaia 90
The Disk Substructures at High Angular Resolution Project (DSHARP). X. Multiple Rings, a Misaligned Inner Disk, and a Bright Arc in the Disk around the T Tauri star HD 143006
DOI: 10.3847/2041-8213/aaf745 Bibcode: 2018ApJ...869L..50P

Wilner, David J.; Andrews, Sean M.; Guzmán, Viviana V. +14 more

We present a detailed analysis of new Atacama Large Millimeter/submillimeter Array (ALMA) observations of the disk around the T-Tauri star HD 143006, which at 46 mas (7.6 au) resolution reveals new substructures in the 1.25 mm continuum emission. The disk resolves into a series of concentric rings and gaps, together with a bright arc exterior to t…

2018 The Astrophysical Journal
Gaia 90
Measuring the Recoverability of Close Binaries in Gaia DR2 with the Robo-AO Kepler Survey
DOI: 10.3847/1538-3881/aad80a Bibcode: 2018AJ....156..259Z

Baranec, Christoph; Law, Nicholas M.; Riddle, Reed +6 more

We use the Robo-AO survey of Kepler planetary candidate host stars, the largest adaptive optics survey yet performed, to measure the recovery rate of close stellar binaries in Gaia DR2. We find that Gaia recovers binaries down to 1″ at magnitude contrasts as large as six; closer systems are not resolved, regardless of secondary brightness. Gaia DR…

2018 The Astronomical Journal
Gaia 90
Distances and Kinematics of Gould Belt Star-forming Regions with Gaia DR2 Results
DOI: 10.3847/1538-4357/aae687 Bibcode: 2018ApJ...867..151D

Rodríguez, Luis F.; Loinard, Laurent; Ortiz-León, Gisela N. +2 more

We present an analysis of the astrometric results from the Gaia second data release (DR2) for young stellar objects (YSOs) in star-forming regions related to the Gould Belt (GB). These regions are Barnard 59, Lupus 1 to 4, Chamaeleon I and II, ɛ Chamaeleontis, the Cepheus flare, IC 5146, and Corona Australis. The mean distance to the YSOs in each …

2018 The Astrophysical Journal
Gaia 90