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Confirmation of a Star Formation Bias in Type Ia Supernova Distances and its Effect on Measurement of the Hubble Constant
M. Rigault, G. Aldering, M. Kowalski +35
Previously we used the Nearby Supernova Factory sample to show that SNe~Ia having locally star-forming environments are dimmer than SNe~Ia having locally passive environments.Here…
IceCube-Gen2: A Vision for the Future of Neutrino Astronomy in Antarctica
Gen2 Collaboration, M. G. Aartsen, M. Ackermann +325
The recent observation by the IceCube neutrino observatory of an astrophysical flux of neutrinos represents the "first light" in the nascent field of neutrino astronomy. The observ…
Type Ia Supernova Distance Modulus Bias and Dispersion From K-correction Errors: A Direct Measurement Using Lightcurve Fits to Observed Spectral Time Series
C. Saunders, G. Aldering, P. Antilogus +34
We estimate systematic errors due to K-corrections in standard photometric analyses of high redshift Type Ia supernovae. Errors due to K-correction occur when the spectral template…
Search for Prompt Neutrino Emission from Gamma-Ray Bursts with IceCube
IceCube Collaboration, M. G. Aartsen, M. Ackermann +300
We present constraints derived from a search of four years of IceCube data for a prompt neutrino flux from gamma-ray bursts (GRBs). A single low-significance neutrino, compatible w…
Status of High-Energy Neutrino Astronomy
Marek Kowalski
With the recent discovery of high-energy neutrinos of extra-terrestrial origin by the IceCube neutrino observatory, neutrino-astronomy is entering a new era. This review will cover…
A flux calibration device for the SuperNova Integral Field Spectrograph (SNIFS)
Simona Lombardo, Greg Aldering, Akos Hoffmann +4
Observational cosmology employing optical surveys often require precise flux calibration. In this context we present SNIFS Calibration Apparatus (SCALA), a flux calibration system…
Determining neutrino oscillation parameters from atmospheric muon neutrino disappearance with three years of IceCube DeepCore data
IceCube Collaboration, M. G. Aartsen, M. Ackermann +301
We present a measurement of neutrino oscillations via atmospheric muon neutrino disappearance with three years of data of the completed IceCube neutrino detector. DeepCore, a regio…
Atmospheric and Astrophysical Neutrinos above 1 TeV Interacting in IceCube
M. G. Aartsen, M. Ackermann, J. Adams +301
The IceCube Neutrino Observatory was designed primarily to search for high-energy (TeV--PeV) neutrinos produced in distant astrophysical objects. A search for ~TeV neu…
Hidden Photon Dark Matter Search with a Large Metallic Mirror
Babette Döbrich, Kai Daumiller, Ralph Engel +4
If Dark Matter is composed of hidden-sector photons that kinetically mix with photons of the visible sector, then Dark Matter has a tiny oscillating electric field component. Its p…
Development of a General Analysis and Unfolding Scheme and its Application to Measure the Energy Spectrum of Atmospheric Neutrinos with IceCube
M. G. Aartsen, M. Ackermann, J. Adams +301
We present the development and application of a generic analysis scheme for the measurement of neutrino spectra with the IceCube detector. This scheme is based on regularized unfol…
Searches for small-scale anisotropies from neutrino point sources with three years of IceCube data
IceCube Collaboration, M. G. Aartsen, M. Ackermann +300
Recently, IceCube found evidence for a diffuse signal of astrophysical neutrinos in an energy range of to the -scale. The origin of those events, b…
Observation of High-Energy Astrophysical Neutrinos in Three Years of IceCube Data
M. G. Aartsen, M. Ackermann, J. Adams +294
A search for high-energy neutrinos interacting within the IceCube detector between 2010 and 2012 provided the first evidence for a high-energy neutrino flux of extraterrestrial ori…
Searches for Extended and Point-like Neutrino Sources with Four Years of IceCube Data
IceCube Collaboration, M. G. Aartsen, M. Ackermann +301
We present results on searches for point-like sources of neutrinos using four years of IceCube data, including the first year of data from the completed 86-string detector. The tot…
Multipole analysis of IceCube data to search for dark matter accumulated in the Galactic halo
IceCube Collaboration, M. G. Aartsen, M. Ackermann +299
Dark matter which is bound in the Galactic halo might self-annihilate and produce a flux of stable final state particles, e.g. high energy neutrinos. These neutrinos can be detecte…
Type Ia supernova bolometric light curves and ejected mass estimates from the Nearby Supernova Factory
R. Scalzo, G. Aldering, P. Antilogus +32
We present a sample of normal type Ia supernovae from the Nearby Supernova Factory dataset with spectrophotometry at sufficiently late phases to estimate the ejected mass using the…
Search for non-relativistic Magnetic Monopoles with IceCube
IceCube Collaboration, M. G. Aartsen, R. Abbasi +288
The IceCube Neutrino Observatory is a large Cherenkov detector instrumenting of Antarctic ice. The detector can be used to search for signatures of particle phys…
Type Ia Supernova Hubble Residuals and Host-Galaxy Properties
A. G. Kim, G. Aldering, P. Antilogus +33
Kim et al. (2013) [K13] introduced a new methodology for determining peak-brightness absolute magnitudes of type Ia supernovae from multi-band light curves. We examine the relation…
Letter of Intent: The Precision IceCube Next Generation Upgrade (PINGU)
PINGU Collaboration
The Precision IceCube Next Generation Upgrade (PINGU) is a proposed low-energy in-fill array of the IceCube Neutrino Observatory. Leveraging technology proven with IceCube, PINGU w…