Search Publications

Gaia and the Galactic Center Origin of Hypervelocity Stars
DOI: 10.3847/1538-4357/aadb8e Bibcode: 2018ApJ...866...39B

Geller, Margaret J.; Brown, Warren R.; Kenyon, Scott J. +1 more

We use new Gaia measurements to explore the origin of the highest velocity stars in the hypervelocity star (HVS) survey. The measurements reveal a clear pattern in B-type stars. Halo stars dominate the sample at speeds of ≃100 km s-1 below Galactic escape velocity. Disk runaway stars have speeds up to ≃100 km s-1 above Galact…

2018 The Astrophysical Journal
Gaia eHST 66
LensFlow: A Convolutional Neural Network in Search of Strong Gravitational Lenses
DOI: 10.3847/1538-4357/aaae6a Bibcode: 2018ApJ...856...68P

Cooray, Asantha; Nayyeri, Hooshang; Pourrahmani, Milad

In this work, we present our machine learning classification algorithm for identifying strong gravitational lenses from wide-area surveys using convolutional neural networks; LENSFLOW. We train and test the algorithm using a wide variety of strong gravitational lens configurations from simulations of lensing events. Images are processed through mu…

2018 The Astrophysical Journal
eHST 65
Three-dimensional motions in the Sculptor dwarf galaxy as a glimpse of a new era
DOI: 10.1038/s41550-017-0322-y Bibcode: 2018NatAs...2..156M

Massari, D.; Helmi, A.; Brown, A. G. A. +3 more

The three-dimensional motions of stars in small galaxies beyond our own are minute, yet they are crucial for understanding the nature of gravity and dark matter1,2. Even for the dwarf galaxy Sculptor—one of the best-studied systems, which is inferred to be strongly dark matter dominated3,4—there are conflicting reports5-…

2018 Nature Astronomy
Gaia eHST 65
Detection of Reflection Features in the Neutron Star Low-mass X-Ray Binary Serpens X-1 with NICER
DOI: 10.3847/2041-8213/aabee6 Bibcode: 2018ApJ...858L...5L

Fabian, A. C.; Miller, J. M.; Homan, J. +17 more

We present Neutron Star Interior Composition Explorer (NICER) observations of the neutron star (NS) low-mass X-ray binary Serpens X-1 during the early mission phase in 2017. With the high spectral sensitivity and low-energy X-ray passband of NICER, we are able to detect the Fe L line complex in addition to the signature broad, asymmetric Fe K line…

2018 The Astrophysical Journal
XMM-Newton 65
Results from a Systematic Survey of X-Ray Emission from Hydrogen-poor Superluminous SNe
DOI: 10.3847/1538-4357/aad2df Bibcode: 2018ApJ...864...45M

Berger, E.; Chornock, R.; Lunnan, R. +11 more

We present the results from a sensitive X-ray survey of 26 nearby hydrogen-poor superluminous supernovae (SLSNe-I) with Swift, Chandra, and XMM. This data set constrains the SLSN evolution from a few days until ∼2000 days after explosion, reaching a luminosity limit L x ∼ 1040 erg s-1 and revealing the presence o…

2018 The Astrophysical Journal
XMM-Newton 65
MICROSCOPE limits for new long-range forces and implications for unified theories
DOI: 10.1103/PhysRevD.97.055039 Bibcode: 2018PhRvD..97e5039F

Fayet, Pierre

Many theories beyond the standard model involve an extra U (1 ) gauge group. The resulting gauge boson U , in general mixed with the Z and the photon, may be massless or very light and very weakly coupled. It may be viewed as a generalized dark photon interacting with matter through a linear combination [ɛQQ +ɛBB +ɛL

2018 Physical Review D
MICROSCOPE 65
RELICS: Strong Lens Models for Five Galaxy Clusters from the Reionization Lensing Cluster Survey
DOI: 10.3847/1538-4357/aabe7b Bibcode: 2018ApJ...859..159C

Frye, Brenda L.; Bradač, Maruša; Lovisari, Lorenzo +31 more

Strong gravitational lensing by galaxy clusters magnifies background galaxies, enhancing our ability to discover statistically significant samples of galaxies at {\boldsymbol{z}}> 6, in order to constrain the high-redshift galaxy luminosity functions. Here, we present the first five lens models out of the Reionization Lensing Cluster Survey (RE…

2018 The Astrophysical Journal
eHST 65
Constraining warm inflation with CMB data
DOI: 10.1088/1475-7516/2018/02/054 Bibcode: 2018JCAP...02..054B

Bhattacharya, Sukannya; Dutta, Koushik; Gangopadhyay, Mayukh Raj +1 more

We confront the warm inflation observational predictions directly with the latest CMB data. We focus on a linear temperature (T) dissipative coefficient combined with the simplest model of inflation, a quartic chaotic potential. Although excluded in its standard cold inflation version, dissipation reduces the tensor-to-scalar ratio and brings the …

2018 Journal of Cosmology and Astroparticle Physics
Planck 65
A 3.5 million Solar masses black hole in the centre of the ultracompact dwarf galaxy fornax UCD3
DOI: 10.1093/mnras/sty913 Bibcode: 2018MNRAS.477.4856A

Romanowsky, Aaron J.; Neumayer, Nadine; Strader, Jay +16 more

The origin of ultracompact dwarfs (UCDs), a class of compact stellar systems discovered two decades ago, still remains a matter of debate. Recent discoveries of central supermassive black holes in UCDs likely inherited from their massive progenitor galaxies provide support for the tidal stripping hypothesis. At the same time, on statistical ground…

2018 Monthly Notices of the Royal Astronomical Society
eHST 65
Identifying Typical Mg II Flare Spectra Using Machine Learning
DOI: 10.3847/1538-4357/aac779 Bibcode: 2018ApJ...861...62P

Krucker, Säm; Kleint, Lucia; Panos, Brandon +4 more

The Interface Region Imaging Spectrograph (IRIS) performs solar observations over a large range of atmospheric heights, including the chromosphere where the majority of flare energy is dissipated. The strong Mg II h&k spectral lines are capable of providing excellent atmospheric diagnostics, but have not been fully utilized for flaring atmosph…

2018 The Astrophysical Journal
IRIS 65