Search Publications

ALMA Reveals Potential Evidence for Spiral Arms, Bars, and Rings in High-redshift Submillimeter Galaxies
DOI: 10.3847/1538-4357/ab1846 Bibcode: 2019ApJ...876..130H

Smail, I.; Menten, K. M.; Brandt, W. N. +19 more

We present subkiloparsec-scale mapping of the 870 µm ALMA continuum emission in six luminous (L IR ∼ 5 × 1012 L ) submillimeter galaxies (SMGs) from the ALESS survey of the Extended Chandra Deep Field South. Our high-fidelity 0.″07-resolution imaging (∼500 pc) reveals robust evidence for structures with deco…

2019 The Astrophysical Journal
Gaia eHST 133
Mapping the Stellar Halo with the H3 Spectroscopic Survey
DOI: 10.3847/1538-4357/ab38b8 Bibcode: 2019ApJ...883..107C

Conroy, Charlie; Johnson, Benjamin D.; Berlind, Perry +12 more

Modern theories of galaxy formation predict that the Galactic stellar halo was hierarchically assembled from the accretion and disruption of smaller systems. This hierarchical assembly is expected to produce a high degree of structure in the combined phase and chemistry space; this structure should provide a relatively direct probe of the accretio…

2019 The Astrophysical Journal
Gaia 132
General relativistic orbital decay in a seven-minute-orbital-period eclipsing binary system
DOI: 10.1038/s41586-019-1403-0 Bibcode: 2019Natur.571..528B

Kulkarni, S. R.; Duev, Dmitry A.; Riddle, Reed +23 more

General relativity1 predicts that short-orbital-period binaries emit considerable amounts of gravitational radiation. The upcoming Laser Interferometer Space Antenna2 (LISA) is expected to detect tens of thousands of such systems3 but few have been identified4, of which only one5 is eclipsing—…

2019 Nature
Gaia XMM-Newton 132
New constraints on sterile neutrino dark matter from NuSTAR M31 observations
DOI: 10.1103/PhysRevD.99.083005 Bibcode: 2019PhRvD..99h3005N

Wik, Daniel R.; Krivonos, Roman; Beacom, John F. +4 more

We use a combined 1.2 Ms of NuSTAR observations of M31 to search for x-ray lines from sterile neutrino dark matter decay. For the first time in a NuSTAR analysis, we consistently take into account the signal contribution from both the focused and unfocused fields of view. We also reduce the modeling systematic uncertainty by performing spectral fi…

2019 Physical Review D
XMM-Newton 132
Half-mass Radii for ∼7000 Galaxies at 1.0 ≤ z ≤ 2.5: Most of the Evolution in the Mass-Size Relation Is Due to Color Gradients
DOI: 10.3847/1538-4357/ab1bda Bibcode: 2019ApJ...877..103S

Barro, Guillermo; Kriek, Mariska; Price, Sedona H. +1 more

Radial mass-to-light ratio gradients cause the half-mass and half-light radii of galaxies to differ, potentially biasing studies that use half-light radii. Here we present the largest catalog to date of galaxy half-mass radii at z > 1: 7006 galaxies in the CANDELS fields at 1.0 ≤ z ≤ 2.5. The sample includes both star-forming and quiescent gala…

2019 The Astrophysical Journal
eHST 131
On the dust temperatures of high-redshift galaxies
DOI: 10.1093/mnras/stz2134 Bibcode: 2019MNRAS.489.1397L

Faucher-Giguère, Claude-André; Hayward, Christopher C.; Hopkins, Philip F. +7 more

Dust temperature is an important property of the interstellar medium (ISM) of galaxies. It is required when converting (sub)millimetre broad-band flux to total infrared luminosity (LIR), and hence star formation rate, in high-redshift galaxies. However, different definitions of dust temperatures have been used in the literature, leading…

2019 Monthly Notices of the Royal Astronomical Society
Herschel 130
Is the dark-matter halo spin a predictor of galaxy spin and size?
DOI: 10.1093/mnras/stz1952 Bibcode: 2019MNRAS.488.4801J

Somerville, Rachel S.; Genel, Shy; Dekel, Avishai +8 more

The similarity between the distributions of spins for galaxies (λgal) and for dark-matter haloes (λhalo), indicated both by simulations and observations, is naively interpreted as a one-to-one correlation between the spins of a galaxy and its host halo. This is used to predict galaxy sizes in semi-analytic models via Re<…

2019 Monthly Notices of the Royal Astronomical Society
eHST 130
A radio ridge connecting two galaxy clusters in a filament of the cosmic web
DOI: 10.1126/science.aat7500 Bibcode: 2019Sci...364..981G

Brunetti, G.; Enßlin, T. A.; Shimwell, T. W. +26 more

Galaxy clusters are the most massive gravitationally bound structures in the Universe. They grow by accreting smaller structures in a merging process that produces shocks and turbulence in the intracluster gas. We observed a ridge of radio emission connecting the merging galaxy clusters Abell 0399 and Abell 0401 with the Low-Frequency Array (LOFAR…

2019 Science
XMM-Newton 130
The Chemical Evolution of Carbon, Nitrogen, and Oxygen in Metal-poor Dwarf Galaxies
DOI: 10.3847/1538-4357/ab020a Bibcode: 2019ApJ...874...93B

McQuinn, Kristen B. W.; Skillman, Evan D.; Erb, Dawn K. +2 more

Ultraviolet nebular emission lines are important for understanding the time evolution and nucleosynthetic origins of their associated elements, but the underlying trends of their relative abundances are unclear. We present UV spectroscopy of 20 nearby low-metallicity, high-ionization dwarf galaxies obtained using the Hubble Space Telescope. Buildi…

2019 The Astrophysical Journal
eHST 130
Gravitational lensing reveals ionizing ultraviolet photons escaping from a distant galaxy
DOI: 10.1126/science.aaw0978 Bibcode: 2019Sci...366..738R

Mahler, Guillaume; Chisholm, John; Rigby, Jane R. +7 more

During the epoch of reionization, neutral gas in the early Universe was ionized by hard ultraviolet radiation emitted by young stars in the first galaxies. To do so, ionizing ultraviolet photons must escape from the host galaxy. We present Hubble Space Telescope observations of the gravitationally lensed post-reionization galaxy PSZ1-ARC G311.6602…

2019 Science
eHST 130