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Spectroscopic Quadrupole Moments in Sr-96,Sr-98: Evidence for Shape Coexistence in Neutron-Rich Strontium Isotopes at N = 60 (vol 116, 022701, 2016) (2016)
Journal Article
Clement, E., Zielinska, M., Gorgen, A., Korten, W., Peru, S., Libert, J., …Wrzosek-Lipska, K. (2016). Spectroscopic Quadrupole Moments in Sr-96,Sr-98: Evidence for Shape Coexistence in Neutron-Rich Strontium Isotopes at N = 60 (vol 116, 022701, 2016). Physical Review Letters, 117(9), Article 099902. https://doi.org/10.1103/physrevlett.117.099902

Color-singlet production at NNLO in MCFM (2016)
Journal Article
Boughezal, R., Campbell, J. M., Ellis, R. K., Focke, C., Giele, W., Liu, X., …Williams, C. (2017). Color-singlet production at NNLO in MCFM. The European Physical Journal C, 77(1), Article 7. https://doi.org/10.1140/epjc/s10052-016-4558-y

We present the implementation of several color-singlet final-state processes at Next-to-Next-to Leading Order (NNLO) accuracy in QCD to the publicly available parton-level Monte Carlo program MCFM. Specifically we discuss the processes pp→Hpp→H , pp→... Read More about Color-singlet production at NNLO in MCFM.

On the ultimate precision of meson mixing observables (2016)
Journal Article
Jubb, T., Kirk, M., & Lenz, A. (2017). On the ultimate precision of meson mixing observables. Nuclear Physics B, 915, 431-453. https://doi.org/10.1016/j.nuclphysb.2016.12.020

Meson mixing is considered to be an ideal testing ground for new physics searches. Experimental precision has greatly increased over the recent years, exceeding in several cases the theoretical precision. A possible limit in the theoretical accuracy... Read More about On the ultimate precision of meson mixing observables.

The GCT camera for the Cherenkov Telescope Array (2016)
Journal Article
Lapington, J., Abchiche, A., Allan, D., Amans, J., Armstrong, T., Balzer, A., …Zorn, J. (2017). The GCT camera for the Cherenkov Telescope Array. Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, 876, 1-4. https://doi.org/10.1016/j.nima.2016.12.010

The Gamma Cherenkov Telescope (GCT) is one of the designs proposed for the Small Sized Telescope (SST) section of the Cherenkov Telescope Array (CTA). The GCT uses dual-mirror optics, resulting in a compact telescope with good image quality and a lar... Read More about The GCT camera for the Cherenkov Telescope Array.

Nature of the warm absorber outflow in NGC 4051 (2016)
Journal Article
Mizumoto, M., & Ebisawa, K. (2017). Nature of the warm absorber outflow in NGC 4051. Monthly Notices of the Royal Astronomical Society, 466(3), 3259-3271. https://doi.org/10.1093/mnras/stw3364

The narrow-line Seyfert 1 galaxy NGC 4051 is known to exhibit significant X-ray spectral/flux variations and have a number of emission/absorption features. X-ray observations have revealed that these absorption features are blueshifted, which indicat... Read More about Nature of the warm absorber outflow in NGC 4051.

The Chandra Deep Field-South Survey: 7 Ms Source Catalogs (2016)
Journal Article
Luo, B., Brandt, W., Xue, Y., Lehmer, B., Alexander, D., Bauer, F., …Wang, J. (2017). The Chandra Deep Field-South Survey: 7 Ms Source Catalogs. Astrophysical Journal Supplement, 228(1), Article 2. https://doi.org/10.3847/1538-4365/228/1/2

We present X-ray source catalogs for the ≈7 Ms exposure of the Chandra Deep Field-South (CDF-S), which covers a total area of 484.2 arcmin2. Utilizing wavdetect for initial source detection and ACIS Extract for photometric extraction and significance... Read More about The Chandra Deep Field-South Survey: 7 Ms Source Catalogs.

The distribution of radioactive 44Ti in Cassiopeia A (2016)
Journal Article
Grefenstette, B. W., Fryer, C. L., Harrison, F. A., Boggs, S. E., DeLaney, T., Laming, J. M., …Zoglauer, A. (2017). The distribution of radioactive 44Ti in Cassiopeia A. Astrophysical Journal, 834(1), Article 19. https://doi.org/10.3847/1538-4357/834/1/19

The distribution of elements produced in the innermost layers of a supernova explosion is a key diagnostic for studying the collapse of massive stars. Here we present the results of a 2.4 Ms NuSTAR observing campaign aimed at studying the supernova r... Read More about The distribution of radioactive 44Ti in Cassiopeia A.