Search Publications

New Fe I Level Energies and Line Identifications from Stellar Spectra. II. Initial Results from New Ultraviolet Spectra of Metal-poor Stars
DOI: 10.3847/1538-4365/aa6253 Bibcode: 2017ApJS..229...23P

Ayres, Thomas R.; Peterson, Ruth C.; Kurucz, Robert L.

The Fe I spectrum is critical to many areas of astrophysics, yet many of the high-lying levels remain uncharacterized. To remedy this deficiency, Peterson & Kurucz identified Fe I lines in archival ultraviolet and optical spectra of metal-poor stars, whose warm temperatures favor moderate Fe I excitation. Sixty-five new levels were recovered, …

2017 The Astrophysical Journal Supplement Series
eHST 17
Insights from Synthetic Star-forming Regions. I. Reliable Mock Observations from SPH Simulations
DOI: 10.3847/1538-4365/233/1/1 Bibcode: 2017ApJS..233....1K

Dale, James E.; Robitaille, Thomas P.; Koepferl, Christine M. +1 more

Through synthetic observations of a hydrodynamical simulation of an evolving star-forming region, we assess how the choice of observational techniques affects the measurements of properties that trace star formation. Testing and calibrating observational measurements requires synthetic observations that are as realistic as possible. In this part o…

2017 The Astrophysical Journal Supplement Series
Herschel 15
Wayne—A Simulator for HST WFC3 IR Grism Spectroscopy
DOI: 10.3847/1538-4365/aa7750 Bibcode: 2017ApJS..231...13V

Tsiaras, A.; Varley, R.; Karpouzas, K.

Wayne is an algorithm that simulates Hubble Space Telescope Wide Field Camera 3 (WFC3) grism spectroscopic frames, including sources of noise and systematics. It can simulate both staring and spatial scan modes, and observations such as the transit and the eclipse of an exoplanet. Unlike many other instrument simulators, the focus of Wayne is on c…

2017 The Astrophysical Journal Supplement Series
eHST 14
A Large Catalog of Homogeneous Ultra-Violet/Optical GRB Afterglows: Temporal and Spectral Evolution
DOI: 10.3847/1538-4365/228/2/13 Bibcode: 2017ApJS..228...13R

Gronwall, Caryl; Kuin, N. P. M.; Roming, Peter W. A. +10 more

We present the second Swift Ultra-Violet/Optical Telescope (UVOT) gamma-ray burst (GRB) afterglow catalog, greatly expanding on the first Swift UVOT GRB afterglow catalog. The second catalog is constructed from a database containing over 120,000 independent UVOT observations of 538 GRBs first detected by Swift, the High Energy Transient Explorer 2…

2017 The Astrophysical Journal Supplement Series
INTEGRAL 13
Galactic Sources Detected in the NuSTAR Serendipitous Survey
DOI: 10.3847/1538-4365/aa7517 Bibcode: 2017ApJS..230...25T

Hailey, Charles J.; Mori, Kaya; Aird, James +13 more

The Nuclear Spectroscopic Telescope Array (NuSTAR) provides an improvement in sensitivity at energies above 10 keV by two orders of magnitude over non-focusing satellites, making it possible to probe deeper into the Galaxy and universe. Lansbury and collaborators recently completed a catalog of 497 sources serendipitously detected in the 3-24 keV …

2017 The Astrophysical Journal Supplement Series
Gaia XMM-Newton 9
Star Formation Conditions in a Planck Galactic Cold Clump, G108.84-00.81
DOI: 10.3847/1538-4365/aa7b31 Bibcode: 2017ApJS..231....9K

Kim, Kee-Tae; Lee, Jeong-Eun; Liu, Tie +6 more

We present the results from a series of ground-based radio observations toward a Planck Galactic Cold Clump (PGCC), PGCC G108.84-00.81, which is located in one curved filamentary cloud in the vicinity of an extended H II region Sh2-152 and SNR G109.1-1.0. PGCC G108.84-00.81 is mainly composed of two clumps, “G108-N” and “G108-S”. In the 850 µ…

2017 The Astrophysical Journal Supplement Series
AKARI Planck 9
Exploring the SDSS Data Set with Linked Scatter Plots. I. EMP, CEMP, and CV Stars
DOI: 10.3847/1538-4365/228/2/19 Bibcode: 2017ApJS..228...19C

Carbon, Duane F.; Henze, Christopher; Nelson, Bron C.

We present the results of a search for extremely metal-poor (EMP), carbon-enhanced metal-poor (CEMP), and cataclysmic variable (CV) stars using a new exploration tool based on linked scatter plots (LSPs). Our approach is especially designed to work with very large spectrum data sets such as the SDSS, LAMOST, RAVE, and Gaia data sets, and it can be…

2017 The Astrophysical Journal Supplement Series
Gaia 8
An Improved Method for Determining the Integrated Properties of Nuclear Rings: NGC 1512
DOI: 10.3847/1538-4365/aa709e Bibcode: 2017ApJS..230...14M

Ho, Luis C.; de Grijs, Richard; Ma, Chao

The integrated properties of nuclear rings are correlated with the secular evolution and dynamics of the host galaxies of the rings, as well as with the formation and evolution of the rings’ star cluster population(s). Here we present a new method to accurately measure the spectral energy distribution and current star formation rate (SFR) of the n…

2017 The Astrophysical Journal Supplement Series
eHST 8
The InterPlanetary Network Supplement to the Second Fermi GBM Catalog of Cosmic Gamma-Ray Bursts
DOI: 10.3847/1538-4365/229/2/31 Bibcode: 2017ApJS..229...31H

Zhang, X.; Cline, T.; Hurley, K. +32 more

InterPlanetary Network (IPN) data are presented for the gamma-ray bursts in the second Fermi Gamma-Ray Burst Monitor (GBM) catalog. Of the 462 bursts in that catalog between 2010 July 12 and 2012 July 11, 428, or 93%, were observed by at least 1 other instrument in the 9-spacecraft IPN. Of the 428, the localizations of 165 could be improved by tri…

2017 The Astrophysical Journal Supplement Series
INTEGRAL 7
Measuring Filament Orientation: A New Quantitative, Local Approach
DOI: 10.3847/1538-4365/aa8507 Bibcode: 2017ApJS..232....6G

Green, C. -E.; Dawson, J. R.; Cunningham, M. R. +3 more

The relative orientation between filamentary structures in molecular clouds and the ambient magnetic field provides insight into filament formation and stability. To calculate the relative orientation, a measurement of filament orientation is first required. We propose a new method to calculate the orientation of the one-pixel-wide filament skelet…

2017 The Astrophysical Journal Supplement Series
Herschel 3