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A. Tikhomirov

6 papers hereh-index 107.9k citations16 works total

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

author position
  • middle author4

Across the 4 of 6 papers where every author was matched, so the position is known.

fields
  • astro-ph.IM4
  • astro-ph.CO2
same name
  • A. Tikhomirov — 27 papers, h 11
  • A. Tikhomirov — 20 papers, h 20
  • A. Tikhomirov — 6 papers, h 7
  • A. Tikhomirov — 2 papers, h 8
  • A. Tikhomirov — 1 paper, h 11
  • A. Tikhomirov — 1 paper, h 1

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
20132022
most citedThe POLARBEAR-2 and the Simons Array Experiment

163 citations · 472 across the 6 of their papers we have counts for

collaborators
Showing astro-ph.IMShow all

4 papers · 1 filter

astro-ph.IM2022★ 37 cited

The POLARBEAR-2 and Simons Array Focal Plane Fabrication Status

B. Westbrook, P. A. R. Ade, M. Aguilar +90

We present on the status of POLARBEAR-2 A (PB2-A) focal plane fabrication. The PB2-A is the first of three telescopes in the Simon Array (SA), which is an array of three cosmic mic…

astro-ph.IM2016★ 38 cited

POLARBEAR-2: an instrument for CMB polarization measurements

Y. Inoue, P. Ade, Y. Akiba +83

POLARBEAR-2 (PB-2) is a cosmic microwave background (CMB) polarization experiment that will be located in the Atacama highland in Chile at an altitude of 5200 m. Its science goals…

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.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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