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researcher

A. Cukierman

100 papers hereh-index 356.5k citations153 works total

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

author position
  • first author5
  • middle author53

Across the 58 of 100 papers where every author was matched, so the position is known.

fields
  • astro-ph.IM64
  • astro-ph.CO23
  • astro-ph.GA7
  • astro-ph.EP3
  • physics.ins-det2
  • hep-ph1
same name
  • A. Cukierman — 21 papers, h 44
  • A. Cukierman — 2 papers

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

activity
20112026
most citedThe Simons Observatory: Science goals and forecasts

1.5k citations · 5k across the 89 of their papers we have counts for

collaborators
Showing 2015Show all

4 papers · 1 filter

astro-ph.IM2015★ 14 cited

Development of readout electronics for POLARBEAR-2 Cosmic Microwave Background experiment

K. Hattori, Y. Akiba, K. Arnold +18

The readout of transition-edge sensor (TES) bolometers with a large multiplexing factor is key for the next generation Cosmic Microwave Background (CMB) experiment, Polarbear-2, ha…

astro-ph.IM2015★ 163 cited

The POLARBEAR-2 and the Simons Array Experiment

A. Suzuki, P. Ade, Y. Akiba +86

We present an overview of the design and status of the \Pb-2 and the Simons Array experiments. \Pb-2 is a Cosmic Microwave Background polarimetry experiment which aims to character…

astro-ph.CO2015★ 100 cited

POLARBEAR Constraints on Cosmic Birefringence and Primordial Magnetic Fields

POLARBEAR Collaboration, Peter A. R. Ade, Kam Arnold +84

We constrain anisotropic cosmic birefringence using four-point correlations of even-parity E-mode and odd-parity B-mode polarization in the cosmic microwave background measurem…

astro-ph.IM2015★ 40 cited

Modeling atmospheric emission for CMB ground-based observations

J. Errard, P. A. R. Ade, Y. Akiba +72

Atmosphere is one of the most important noise sources for ground-based cosmic microwave background (CMB) experiments. By increasing optical loading on the detectors, it amplifies t…

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