Search Publications

Probing dark matter substructure in the gravitational lens HE 0435-1223 with the WFC3 grism
DOI: 10.1093/mnras/stx1400 Bibcode: 2017MNRAS.471.2224N

Keeton, C. R.; Kochanek, C. S.; Brammer, G. +7 more

Strong gravitational lensing provides a powerful test of cold dark matter (CDM) as it enables the detection and mass measurement of low-mass haloes even if they do not contain baryons. Compact lensed sources such as active galactic nuclei (AGNs) are particularly sensitive to perturbing subhaloes, but their use as a test of CDM has been limited by …

2017 Monthly Notices of the Royal Astronomical Society
eHST 98
ALMA Reveals Metals yet No Dust within Multiple Components in CR7
DOI: 10.3847/1538-4357/aa9931 Bibcode: 2017ApJ...851..145M

Schaerer, D.; Mobasher, B.; Ferrara, A. +8 more

We present spectroscopic follow-up observations of CR7 with ALMA, targeted at constraining the infrared (IR) continuum and [C II]{}158µ {{m}} line-emission at high spatial resolution matched to the HST/WFC3 imaging. CR7 is a luminous Lyα emitting galaxy at z = 6.6 that consists of three separated UV-continuum components. Our obser…

2017 The Astrophysical Journal
eHST 98
Bombs and Flares at the Surface and Lower Atmosphere of the Sun
DOI: 10.3847/1538-4357/aa6844 Bibcode: 2017ApJ...839...22H

Leenaarts, J.; Hansteen, V. H.; Rouppe van der Voort, L. +3 more

A spectacular manifestation of solar activity is the appearance of transient brightenings in the far wings of the Hα line, known as Ellerman bombs (EBs). Recent observations obtained by the Interface Region Imaging Spectrograph have revealed another type of plasma “bombs” (UV bursts) with high temperatures of perhaps up to 8 × 104 K wit…

2017 The Astrophysical Journal
IRIS 98
Falling Outer Rotation Curves of Star-forming Galaxies at 0.6 ≲ z ≲ 2.6 Probed with KMOS3D and SINS/zC-SINF
DOI: 10.3847/1538-4357/aa6d82 Bibcode: 2017ApJ...840...92L

Übler, Hannah; van Dokkum, Pieter G.; Brammer, Gabe +25 more

We exploit the deep, resolved, Hα kinematic data from the KMOS3D and SINS/zC-SINF surveys to examine the largely unexplored outer-disk kinematics of star-forming galaxies (SFGs), out to the peak of cosmic star formation. Our sample contains 101 SFGs, representative of the more massive (9.3≲ {log}{M}* /{M}≲ 11.5) …

2017 The Astrophysical Journal
eHST 98
A Measurement of the Cosmic Microwave Background B-mode Polarization Power Spectrum at Subdegree Scales from Two Years of polarbear Data
DOI: 10.3847/1538-4357/aa8e9f Bibcode: 2017ApJ...848..121P

Ade, P. A. R.; Baccigalupi, C.; Borrill, J. +79 more

We report an improved measurement of the cosmic microwave background B-mode polarization power spectrum with the Polarbear experiment at 150 GHz. By adding new data collected during the second season of observations (2013-2014) to re-analyzed data from the first season (2012-2013), we have reduced twofold the band-power uncertainties. The band pow…

2017 The Astrophysical Journal
Planck 98
A Close-up View of the Young Circumbinary Disk HD 142527
DOI: 10.3847/1538-4357/aa696c Bibcode: 2017ApJ...840...60B

Ricci, L.; Boehler, Y.; Grady, C. +4 more

We present ALMA observations of the 0.88 millimeter dust continuum and the 13CO and C18O J = 3-2 line emission of the circumbinary disk HD 142527 at a spatial resolution of ∼0.″25. This system is characterized by a large central cavity of roughly 120 au in radius, and asymmetric dust and gas emission. By comparing the observa…

2017 The Astrophysical Journal
Gaia 97
Warm inflation dissipative effects: Predictions and constraints from the Planck data
DOI: 10.1103/PhysRevD.95.023517 Bibcode: 2017PhRvD..95b3517B

Benetti, Micol; Ramos, Rudnei O.

We explore the warm inflation scenario theoretical predictions looking at two different dissipative regimes for several representative primordial potentials. As it is well known, warm inflation is able to decrease the tensor-to-scalar ratio value, rehabilitating several primordial potentials ruled out in the cold inflation context by the recent co…

2017 Physical Review D
Planck 97
Characterizing the UV-to-NIR shape of the dust attenuation curve of IR luminous galaxies up to z ∼ 2
DOI: 10.1093/mnras/stx1901 Bibcode: 2017MNRAS.472.1372L

Buat, V.; Burgarella, D.; Efstathiou, A. +4 more

In this work, we investigate the far-ultraviolet (UV) to near-infrared (NIR) shape of the dust attenuation curve of a sample of IR-selected dust obscured (ultra)luminous IR galaxies at z ∼ 2. The spectral energy distributions (SEDs) are fitted with Code Investigating GALaxy Emission, a physically motivated spectral-synthesis model based on energy …

2017 Monthly Notices of the Royal Astronomical Society
Herschel 97
MOSFIRE Spectroscopy of Quiescent Galaxies at 1.5 < z < 2.5. I. Evolution of Structural and Dynamical Properties
DOI: 10.3847/1538-4357/834/1/18 Bibcode: 2017ApJ...834...18B

Ellis, Richard S.; Belli, Sirio; Newman, Andrew B.

We present deep near-infrared spectra for a sample of 24 quiescent galaxies in the redshift range 1.5< z< 2.5 obtained with the MOSFIRE spectrograph at the W. M. Keck Observatory. In conjunction with a similar data set we obtained in the range 1< z< 1.5 with the LRIS spectrograph, we analyze the kinematic and structural properties for …

2017 The Astrophysical Journal
eHST 97
Wide binaries in Tycho-Gaia: search method and the distribution of orbital separations
DOI: 10.1093/mnras/stx2000 Bibcode: 2017MNRAS.472..675A

Agüeros, Marcel A.; Andrews, Jeff J.; Chanamé, Julio

We mine the Tycho-Gaia astrometric solution (TGAS) catalogue for wide stellar binaries by matching positions, proper motions and astrometric parallaxes. We separate genuine binaries from unassociated stellar pairs through a Bayesian formulation that includes correlated uncertainties in the proper motions and parallaxes. Rather than relying on assu…

2017 Monthly Notices of the Royal Astronomical Society
Gaia 97