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Simultaneous X-Ray, Gamma-Ray, and Radio Observations of the Repeating Fast Radio Burst FRB 121102
DOI: 10.3847/1538-4357/aa8456 Bibcode: 2017ApJ...846...80S

Ransom, S. M.; Chatterjee, S.; Cordes, J. M. +19 more

We undertook coordinated campaigns with the Green Bank, Effelsberg, and Arecibo radio telescopes during Chandra X-ray Observatory and XMM-Newton observations of the repeating fast radio burst FRB 121102 to search for simultaneous radio and X-ray bursts. We find 12 radio bursts from FRB 121102 during 70 ks total of X-ray observations. We detect no …

2017 The Astrophysical Journal
XMM-Newton 127
CANDELS Multi-wavelength Catalogs: Source Identification and Photometry in the CANDELS COSMOS Survey Field
DOI: 10.3847/1538-4365/228/1/7 Bibcode: 2017ApJS..228....7N

Wuyts, S.; Dickinson, M.; Ferguson, H. C. +36 more

We present a multi-wavelength photometric catalog in the COSMOS field as part of the observations by the Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey. The catalog is based on Hubble Space Telescope Wide Field Camera 3 (HST/WFC3) and Advanced Camera for Surveys observations of the COSMOS field (centered at R.A.: {10}{{h

2017 The Astrophysical Journal Supplement Series
eHST 127
The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/Virgo GW170817. VII. Properties of the Host Galaxy and Constraints on the Merger Timescale
DOI: 10.3847/2041-8213/aa9055 Bibcode: 2017ApJ...848L..22B

Berger, E.; Rest, A.; Annis, J. +21 more

We present the properties of NGC 4993, the host galaxy of GW170817, the first gravitational-wave (GW) event from the merger of a binary neutron star (BNS) system and the first with an electromagnetic (EM) counterpart. We use both archival photometry and new optical/near-IR imaging and spectroscopy, together with stellar population synthesis models…

2017 The Astrophysical Journal
eHST 126
Two-season Atacama Cosmology Telescope polarimeter lensing power spectrum
DOI: 10.1103/PhysRevD.95.123529 Bibcode: 2017PhRvD..95l3529S

Hasselfield, Matthew; Battaglia, Nicholas; Aiola, Simone +43 more

We report a measurement of the power spectrum of cosmic microwave background (CMB) lensing from two seasons of Atacama Cosmology Telescope polarimeter (ACTPol) CMB data. The CMB lensing power spectrum is extracted from both temperature and polarization data using quadratic estimators. We obtain results that are consistent with the expectation from…

2017 Physical Review D
Planck 126
The Herschel-ATLAS: a sample of 500 µm-selected lensed galaxies over 600 deg2
DOI: 10.1093/mnras/stw2911 Bibcode: 2017MNRAS.465.3558N

Ivison, R. J.; Omont, A.; Danese, L. +43 more

We present a sample of 80 candidate strongly lensed galaxies with flux density above 100 mJy at 500 µm extracted from the Herschel Astrophysical Terahertz Large Area Survey, over an area of 600 deg2. Available imaging and spectroscopic data allow us to confirm the strong lensing in 20 cases and to reject it in one case. For other …

2017 Monthly Notices of the Royal Astronomical Society
Herschel eHST 126
Structure of Herbig AeBe disks at the milliarcsecond scale . A statistical survey in the H band using PIONIER-VLTI
DOI: 10.1051/0004-6361/201629305 Bibcode: 2017A&A...599A..85L

Pinte, C.; Ménard, F.; Absil, O. +26 more

Context. It is now generally accepted that the near-infrared excess of Herbig AeBe stars originates in the dust of a circumstellar disk.
Aims: The aims of this article are to infer the radial and vertical structure of these disks at scales of order 1 au, and the properties of the dust grains.
Methods: The program objects (51 in total) we…

2017 Astronomy and Astrophysics
Gaia 125
Hitomi Constraints on the 3.5 keV Line in the Perseus Galaxy Cluster
DOI: 10.3847/2041-8213/aa61fa Bibcode: 2017ApJ...837L..15A

Mukai, K.; Yamaguchi, H.; Koyama, K. +215 more

High-resolution X-ray spectroscopy with Hitomi was expected to resolve the origin of the faint unidentified E≈ 3.5 {keV} emission line reported in several low-resolution studies of various massive systems, such as galaxies and clusters, including the Perseus cluster. We have analyzed the Hitomi first-light observation of the Perseus cluster. The e…

2017 The Astrophysical Journal
Hitomi 124
Global Energetics of Solar Flares. V. Energy Closure in Flares and Coronal Mass Ejections
DOI: 10.3847/1538-4357/836/1/17 Bibcode: 2017ApJ...836...17A

Xu, Yan; Jing, Ju; Warren, Harry P. +11 more

In this study we synthesize the results of four previous studies on the global energetics of solar flares and associated coronal mass ejections (CMEs), which include magnetic, thermal, nonthermal, and CME energies in 399 solar M- and X-class flare events observed during the first 3.5 yr of the Solar Dynamics Observatory (SDO) mission. Our findings…

2017 The Astrophysical Journal
SOHO 124
The composition of cometary ices
DOI: 10.1098/rsta.2016.0252 Bibcode: 2017RSPTA.37560252B

Biver, N.; Bockelée-Morvan, D.

The chemical composition of cometary ices provides clues for the conditions of formation and evolution of the early Solar System. A large number of molecules have been identified in cometary atmospheres, from both ground-based observations and space, including in situ investigations. This includes large organic molecules, which are also observed i…

2017 Philosophical Transactions of the Royal Society of London Series A
Rosetta 124
The Distance to NGC 4993: The Host Galaxy of the Gravitational-wave Event GW170817
DOI: 10.3847/2041-8213/aa9110 Bibcode: 2017ApJ...848L..31H

Gall, Christa; Hjorth, Jens; Tanvir, Nial R. +6 more

The historic detection of gravitational waves from a binary neutron star merger (GW170817) and its electromagnetic counterpart led to the first accurate (sub-arcsecond) localization of a gravitational-wave event. The transient was found to be ∼10″ from the nucleus of the S0 galaxy NGC 4993. We report here the luminosity distance to this galaxy usi…

2017 The Astrophysical Journal
eHST 124