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researcher

A. Deutsch

4 papers here

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • first author1
  • middle author2

Across the 3 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.CO3
  • astro-ph.IM1
same name
  • A. Deutsch — 16 papers, h 41
  • A. Deutsch — 4 papers, h 40
  • A. Deutsch — 1 paper
  • A. Deutsch — 1 paper, h 4
  • A. Deutsch — 1 paper
  • A. Deutsch — 1 paper, h 5

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

collaborators

4 papers

astro-ph.CO2018

Primordial gravitational wave phenomenology with polarized Sunyaev Zel'dovich tomography

Anne-Sylvie Deutsch, Emanuela Dimastrogiovanni, Matteo Fasiello +2

The detection and characterization of primordial gravitational waves through their impact on the polarization anisotropies of the cosmic microwave background (CMB) is a primary sci…

astro-ph.IM2018

Methods for the detection of gravitational waves from sub-solar mass ultracompact binaries

Ryan Magee, Anne-Sylvie Deutsch, Phoebe McClincy +6

We describe detection methods for extensions of gravitational wave searches to sub-solar mass compact binaries. Sub-solar mass searches were previously carried out using Initial LI…

astro-ph.CO2018

Search for sub-solar mass ultracompact binaries in Advanced LIGO's first observing run

B. P. Abbott, R. Abbott, T. D. Abbott +1135

We present the first Advanced LIGO and Advanced Virgo search for ultracompact binary systems with component masses between 0.2 M⊙​ - 1.0 M⊙​ using data taken between Se…

astro-ph.CO2018

Statistical anisotropies in temperature and polarization fluctuations from a scale-dependent trispectrum

Saroj Adhikari, Anne-Sylvie Deutsch, Sarah Shandera

We study statistical anisotropies generated in the observed two-point function of the cosmic microwave background (CMB) fluctuations if the primordial statistics are non-Gaussian.…

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