Search Publications

Nearly all the sky is covered by Lyman-α emission around high-redshift galaxies
DOI: 10.1038/s41586-018-0564-6 Bibcode: 2018Natur.562..229W

Inami, H.; Steinmetz, M.; Richard, J. +22 more

Galaxies are surrounded by large reservoirs of gas, mostly hydrogen, that are fed by inflows from the intergalactic medium and by outflows from galactic winds. Absorption-line measurements along the lines of sight to bright and rare background quasars indicate that this circumgalactic medium extends far beyond the starlight seen in galaxies, but v…

2018 Nature
eHST 145
Deep Learning Based Solar Flare Forecasting Model. I. Results for Line-of-sight Magnetograms
DOI: 10.3847/1538-4357/aaae00 Bibcode: 2018ApJ...856....7H

Xu, Long; Huang, Xin; Wang, Huaning +3 more

Solar flares originate from the release of the energy stored in the magnetic field of solar active regions, the triggering mechanism for these flares, however, remains unknown. For this reason, the conventional solar flare forecast is essentially based on the statistic relationship between solar flares and measures extracted from observational dat…

2018 The Astrophysical Journal
SOHO 144
The VLA Nascent Disk and Multiplicity Survey of Perseus Protostars (VANDAM). IV. Free-Free Emission from Protostars: Links to Infrared Properties, Outflow Tracers, and Protostellar Disk Masses
DOI: 10.3847/1538-4365/aaceae Bibcode: 2018ApJS..238...19T

Dunham, Michael M.; Kratter, Kaitlin M.; Li, Zhi-Yun +11 more

Emission from protostars at centimeter radio wavelengths has been shown to trace the free-free emission arising from ionizing shocks as a result of jets and outflows driven by protostars. Therefore, measuring properties of protostars at radio frequencies can provide valuable insights into the nature of their outflows and jets. We present a C-band …

2018 The Astrophysical Journal Supplement Series
Herschel XMM-Newton 144
The Opacity of the Intergalactic Medium Measured along Quasar Sightlines at z ∼ 6
DOI: 10.3847/1538-4357/aad4fd Bibcode: 2018ApJ...864...53E

Hennawi, Joseph F.; Davies, Frederick B.; Eilers, Anna-Christina

We publicly release a new sample of 34 medium resolution quasar spectra at 5.77 ≤ z em ≤ 6.54 observed with the Echellette Spectrograph and Imager on the Keck telescope. This quasar sample represents an ideal laboratory to study the intergalactic medium (IGM) during the end stages of the epoch of reionization, and constrain the timing a…

2018 The Astrophysical Journal
eHST 144
Light Curves of Hydrogen-poor Superluminous Supernovae from the Palomar Transient Factory
DOI: 10.3847/1538-4357/aab9b6 Bibcode: 2018ApJ...860..100D

Cenko, S. B.; Sollerman, J.; Spyromilio, J. +24 more

We investigate the light-curve properties of a sample of 26 spectroscopically confirmed hydrogen-poor superluminous supernovae (SLSNe-I) in the Palomar Transient Factory survey. These events are brighter than SNe Ib/c and SNe Ic-BL, on average, by about 4 and 2 mag, respectively. The peak absolute magnitudes of SLSNe-I in rest-frame g band span -2…

2018 The Astrophysical Journal
eHST 143
Gaia Data Release 2. Processing of the photometric data
DOI: 10.1051/0004-6361/201832712 Bibcode: 2018A&A...616A...3R

Jordi, C.; Evans, D. W.; van Leeuwen, F. +13 more

Context. The second Gaia data release is based on 22 months of mission data with an average of 0.9 billion individual CCD observations per day. A data volume of this size and granularity requires a robust and reliable but still flexible system to achieve the demanding accuracy and precision constraints that Gaia is capable of delivering.
Aims…

2018 Astronomy and Astrophysics
Gaia 143
Measuring Radial Orbit Migration in the Galactic Disk
DOI: 10.3847/1538-4357/aadba5 Bibcode: 2018ApJ...865...96F

Ting, Yuan-Sen; Hogg, David W.; Rix, Hans-Walter +2 more

We develop and apply a model to quantify the global efficiency of radial orbit migration among stars in the Milky Way disk. This model parameterizes the possible star formation and enrichment histories and radial birth profiles, and combines them with a migration model that relates present-day orbital radii to birth radii through a Gaussian probab…

2018 The Astrophysical Journal
Gaia 143
The Habitability of Proxima Centauri b: Environmental States and Observational Discriminants
DOI: 10.1089/ast.2016.1589 Bibcode: 2018AsBio..18..133M

Lustig-Yaeger, Jacob; Meadows, Victoria S.; Arney, Giada N. +11 more

Proxima Centauri b provides an unprecedented opportunity to understand the evolution and nature of terrestrial planets orbiting M dwarfs. Although Proxima Cen b orbits within its star's habitable zone, multiple plausible evolutionary paths could have generated different environments that may or may not be habitable. Here, we use 1-D coupled climat…

2018 Astrobiology
IUE eHST 143
Violation of the equivalence principle from light scalar dark matter
DOI: 10.1103/PhysRevD.98.064051 Bibcode: 2018PhRvD..98f4051H

Wolf, Peter; Hees, Aurélien; Minazzoli, Olivier +2 more

In this paper, we study the local observational consequences of a violation of the Einstein equivalence principle induced by models of light scalar dark matter (DM). We focus on two different models where the scalar field couples linearly or quadratically to the standard model of matter fields. For both these cases, we derive the solutions of the …

2018 Physical Review D
MICROSCOPE 143
Evidence for Pulsar-like Emission Components in the Broadband ULX Sample
DOI: 10.3847/1538-4357/aab610 Bibcode: 2018ApJ...856..128W

Harrison, F. A.; Stern, D.; Fabian, A. C. +7 more

We present broadband X-ray analyses of a sample of bright ultraluminous X-ray sources (ULX) with the goal of investigating the spectral similarity of this population to the known ULX pulsars, M82 X-2, NGC 7793 P13, and NGC 5907 ULX. We perform a phase-resolved analysis of the broadband XMM-Newton+NuSTAR data set of NGC 5907 ULX, finding that the p…

2018 The Astrophysical Journal
XMM-Newton 142