Search Publications

The NuSTAR Serendipitous Survey: Hunting for the Most Extreme Obscured AGN at >10 keV
DOI: 10.3847/1538-4357/aa8176 Bibcode: 2017ApJ...846...20L

Harrison, F. A.; Stern, D.; Alexander, D. M. +27 more

We identify sources with extremely hard X-ray spectra (I.e., with photon indices of {{Γ }}≲ 0.6) in the 13 deg2 NuSTAR serendipitous survey, to search for the most highly obscured active galactic nuclei (AGNs) detected at > 10 {keV}. Eight extreme NuSTAR sources are identified, and we use the NuSTAR data in combination with lower-ene…

2017 The Astrophysical Journal
XMM-Newton 49
Interpreting the Strongly Lensed Supernova iPTF16geu: Time Delay Predictions, Microlensing, and Lensing Rates
DOI: 10.3847/2041-8213/835/2/L25 Bibcode: 2017ApJ...835L..25M

Lee, Chien-Hsiu; Oguri, Masamune; Suyu, Sherry H. +2 more

We present predictions for time delays between multiple images of the gravitationally lensed supernova, iPTF16geu, which was recently discovered from the intermediate Palomar Transient Factory (iPTF). As the supernova is of Type Ia where the intrinsic luminosity is usually well known, accurately measured time delays of the multiple images could pr…

2017 The Astrophysical Journal
eHST 49
Observations of the GRB Afterglow ATLAS17aeu and Its Possible Association with GW 170104
DOI: 10.3847/1538-4357/aa95c1 Bibcode: 2017ApJ...850..149S

Inserra, C.; Rest, A.; Smartt, S. J. +26 more

We report the discovery and multiwavelength data analysis of the peculiar optical transient, ATLAS17aeu. This transient was identified in the sky map of the LIGO gravitational wave event GW 170104 by our ATLAS and Pan-STARRS coverage. ATLAS17aeu was discovered 23.1 hr after GW 170104 and rapidly faded over the next three nights, with a spectrum re…

2017 The Astrophysical Journal
INTEGRAL 49
Halogens as tracers of protosolar nebula material in comet 67P/Churyumov-Gerasimenko
DOI: 10.1093/mnras/stx1911 Bibcode: 2017MNRAS.472.1336D

Neefs, Eddy; Mall, Urs; De Keyser, Johan +26 more

We report the first in situ detection of halogens in a cometary coma, that of 67P/Churyumov-Gerasimenko. Neutral gas mass spectra collected by the European Space Agency's Rosetta spacecraft during four periods of interest from the first comet encounter up to perihelion indicate that the main halogen-bearing compounds are HF, HCl and HBr. The bulk …

2017 Monthly Notices of the Royal Astronomical Society
Rosetta 49
The puzzling case of the radio-loud QSO 3C 186: a gravitational wave recoiling black hole in a young radio source?
DOI: 10.1051/0004-6361/201629522 Bibcode: 2017A&A...600A..57C

Bianchi, S.; Macchetto, F. D.; Capetti, A. +14 more

Context. Radio-loud active galactic nuclei with powerful relativistic jets are thought to be associated with rapidly spinning black holes (BHs). BH spin-up may result from a number of processes, including accretion of matter onto the BH itself, and catastrophic events such as BH-BH mergers.
Aims: We study the intriguing properties of the powe…

2017 Astronomy and Astrophysics
eHST 49
The Very Low Albedo of WASP-12b from Spectral Eclipse Observations with Hubble
DOI: 10.3847/2041-8213/aa876c Bibcode: 2017ApJ...847L...2B

Nikolov, Nikolay; Gibson, Neale P.; Sing, David K. +11 more

We present an optical eclipse observation of the hot Jupiter WASP-12b using the Space Telescope Imaging Spectrograph on board the Hubble Space Telescope. These spectra allow us to place an upper limit of {A}g< 0.064 (97.5% confidence level) on the planet’s white light geometric albedo across 290-570 nm. Using six wavelength bins acro…

2017 The Astrophysical Journal
eHST 49
Witnessing galaxy assembly in an extended z≈3 structure
DOI: 10.1093/mnras/stx1896 Bibcode: 2017MNRAS.471.3686F

Prochaska, J. Xavier; Rafelski, Marc; Fumagalli, Michele +9 more

We present new observations acquired with the Multi Unit Spectroscopic Explorer instrument on the Very Large Telescope in a quasar field that hosts a high column density damped Lyα absorber (DLA) at z ≈ 3.25. We detect Lyα emission from a nebula at the redshift of the DLA with line luminosity (27 ± 1) × 1041 erg s- 1, which e…

2017 Monthly Notices of the Royal Astronomical Society
eHST 49
Detection of the Ultraviolet Spectrum of the Hot Subdwarf Companion of 60 Cygni (B1 Ve) from a Survey of IUE Spectra of Be Stars
DOI: 10.3847/1538-4357/aa740a Bibcode: 2017ApJ...843...60W

Gies, Douglas R.; Wang, Luqian; Peters, Geraldine J.

We used archival International Ultraviolet Explorer (IUE) high-dispersion, short wavelength spectra data to search for evidence of the spectra of hot subdwarf companions of six rapidly rotating Be stars in binary systems. We searched for the signature of a hot companion through an analysis of the cross-correlation functions (CCFs) of observed and …

2017 The Astrophysical Journal
Gaia IUE 49
The relationship between star formation activity and galaxy structural properties in CANDELS and a semi-analytic model
DOI: 10.1093/mnras/stw2690 Bibcode: 2017MNRAS.465..619B

Barro, Guillermo; Bell, Eric F.; Ferguson, Henry C. +13 more

We study the correlation of galaxy structural properties with their location relative to the SFR-M* correlation, also known as the star formation `star-forming main sequence' (SFMS), in the Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey and Galaxy and Mass Assembly Survey and in a semi-analytic model (SAM) of galaxy form…

2017 Monthly Notices of the Royal Astronomical Society
eHST 49
The Herschel-ATLAS Data Release 2, Paper I. Submillimeter and Far-infrared Images of the South and North Galactic Poles: The Largest Herschel Survey of the Extragalactic Sky
DOI: 10.3847/1538-4365/aa9b35 Bibcode: 2017ApJS..233...26S

Smith, Matthew W. L.; Dunne, Loretta; Viaene, Sébastien +11 more

We present the largest submillimeter images that have been made of the extragalactic sky. The Herschel Astrophysical Terahertz Large Area Survey (H-ATLAS) is a survey of 660 deg2 with the PACS and SPIRE cameras in five photometric bands: 100, 160, 250, 350, and 500 µm. In this paper we present the images from our two largest field…

2017 The Astrophysical Journal Supplement Series
Herschel Planck 49