Search Publications

Predicting the Presence of Companions for Stripped-envelope Supernovae: The Case of the Broad-lined Type Ic SN 2002ap
DOI: 10.3847/1538-4357/aa7467 Bibcode: 2017ApJ...842..125Z

Fox, O. D.; Smith, N.; Filippenko, A. V. +10 more

Many young, massive stars are found in close binaries. Using population synthesis simulations we predict the likelihood of a companion star being present when these massive stars end their lives as core-collapse supernovae (SNe). We focus on stripped-envelope SNe, whose progenitors have lost their outer hydrogen and possibly helium layers before e…

2017 The Astrophysical Journal
eHST 60
Whimper of a Bang: Documenting the Final Days of the Nearby Type Ia Supernova 2011fe
DOI: 10.3847/1538-4357/aa6eab Bibcode: 2017ApJ...841...48S

Garnavich, P. M.; Kochanek, C. S.; Stanek, K. Z. +1 more

Using the Hubble Space Telescope (HST) and the Large Binocular Telescope, we followed the evolution of the Type Ia supernova (SN Ia) 2011fe for an unprecedented 1840 days past B-band maximum light and over a factor of 7 million in flux. At 1840 days, the 4000-17000 Å quasi-bolometric luminosity is just (420+/- 20) {L}. By measuring th…

2017 The Astrophysical Journal
eHST 60
A Comparison of Cosmological Parameters Determined from CMB Temperature Power Spectra from the South Pole Telescope and the Planck Satellite
DOI: 10.3847/1538-4357/aa947b Bibcode: 2017ApJ...850..101A

Bleem, L. E.; Stark, A. A.; George, E. M. +42 more

The Planck cosmic microwave background temperature data are best fit with a ΛCDM model that mildly contradicts constraints from other cosmological probes. The South Pole Telescope (SPT) 2540 {\deg }2 SPT-SZ survey offers measurements on sub-degree angular scales (multipoles 650≤slant {\ell }≤slant 2500) with sufficient precision to use …

2017 The Astrophysical Journal
Planck 60
On the Stellar Masses of Giant Clumps in Distant Star-forming Galaxies
DOI: 10.3847/2041-8213/aa5d52 Bibcode: 2017ApJ...836L..22D

Schaerer, Daniel; Cava, Antonio; Mayer, Lucio +2 more

We analyze stellar masses of clumps drawn from a compilation of star-forming galaxies at 1.1 < z < 3.6. Comparing clumps selected in different ways, and in lensed or blank field galaxies, we examine the effects of spatial resolution and sensitivity on the inferred stellar masses. Large differences are found, with median stellar masses rangin…

2017 The Astrophysical Journal
eHST 60
The Grism Lens-Amplified Survey from Space (GLASS). XI. Detection of C IV in Multiple Images of the z = 6.11 Lyα Emitter behind RXC J2248.7-4431
DOI: 10.3847/1538-4357/aa68a3 Bibcode: 2017ApJ...839...17S

Vulcani, B.; Hoag, A.; Bradač, M. +11 more

The C III] and C IV rest-frame UV emission lines are powerful probes of the ionization states of galaxies. They have furthermore been suggested as alternatives for spectroscopic redshift confirmation of objects at the epoch of reionization (z> 6), where the most frequently used redshift indicator, Lyα, is attenuated by the high fraction of neut…

2017 The Astrophysical Journal
eHST 59
Calibration of Ultraviolet, Mid-infrared, and Radio Star Formation Rate Indicators
DOI: 10.3847/1538-4357/aa8ad2 Bibcode: 2017ApJ...847..136B

Imanishi, Masatoshi; Peek, J. E. G.; Kennicutt, Robert C. +12 more

We present calibrations for star formation rate (SFR) indicators in the ultraviolet, mid-infrared, and radio-continuum bands, including one of the first direct calibrations of 150 MHz as an SFR indicator. Our calibrations utilize 66 nearby star-forming galaxies with Balmer-decrement-corrected {{H}}α luminosities, which span five orders of magnitud…

2017 The Astrophysical Journal
Planck 59
Polycyclic Aromatic Hydrocarbons in Protoplanetary Disks around Herbig Ae/Be and T Tauri Stars
DOI: 10.3847/1538-4357/835/2/291 Bibcode: 2017ApJ...835..291S

Seok, Ji Yeon; Li, Aigen

A distinct set of broad emission features at 3.3, 6.2, 7.7, 8.6, 11.3, and 12.7 µm, is often detected in protoplanetary disks (PPDs). These features are commonly attributed to polycyclic aromatic hydrocarbons (PAHs). We model these emission features in the infrared spectra of 69 PPDs around 14 T Tauri and 55 Herbig Ae/Be stars in terms of as…

2017 The Astrophysical Journal
ISO 59
X-Ray Counterpart of Gravitational Waves Due to Binary Neutron Star Mergers: Light Curves, Luminosity Function, and Event Rate Density
DOI: 10.3847/1538-4357/835/1/7 Bibcode: 2017ApJ...835....7S

Sun, Hui; Zhang, Bing; Gao, He

Zhang proposed a type of GRB-less X-ray transient associated with double neutron star (NS-NS) mergers under the conjecture of a rapidly spinning magnetar merger product with the line of sight off the short gamma-ray burst (GRB) jet. We investigate possible light curves of these transients by considering different observers’ viewing angles. We perf…

2017 The Astrophysical Journal
XMM-Newton 58
Forecasting the Impact of Stellar Activity on Transiting Exoplanet Spectra
DOI: 10.3847/1538-4357/aa79f5 Bibcode: 2017ApJ...844...27Z

Line, Michael R.; Zellem, Robert T.; Ciardi, David R. +8 more

Exoplanet host star activity, in the form of unocculted starspots or faculae, alters the observed transmission and emission spectra of the exoplanet. This effect can be exacerbated when combining data from different epochs if the stellar photosphere varies between observations due to activity. Here, we present a method to characterize and correct …

2017 The Astrophysical Journal
eHST 58
Variable Dynamics in the Inner Disk of HD 135344B Revealed with Multi-epoch Scattered Light Imaging
DOI: 10.3847/1538-4357/aa886a Bibcode: 2017ApJ...849..143S

Kraus, Stefan; Milli, Julien; Benisty, Myriam +12 more

We present multi-epoch Very Large Telescope/Spectro-Polarimetric High-contrast Exoplanet REsearch (VLT/SPHERE) observations of the protoplanetary disk around HD 135344B (SAO 206462). The J-band scattered light imagery reveal, with high spatial resolution (∼41 mas, 6.4 au), the disk surface beyond ∼20 au. Temporal variations are identified in the a…

2017 The Astrophysical Journal
Gaia 58