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researcher

J. May

7 papers hereh-index 320 citations9 works total

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

author position
  • first author2
  • middle author4

Across the 6 of 7 papers where every author was matched, so the position is known.

fields
  • astro-ph.IM4
  • physics.ins-det2
  • astro-ph.CO1
same name
  • J. May — 12 papers, h 23
  • J. May — 3 papers
  • J. May — 2 papers, h 5
  • J. May — 2 papers, h 24
  • J. May — 1 paper, h 4
  • J. May — 1 paper

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
20242026
collaborators
Showing astro-ph.IMShow all

4 papers · 1 filter

astro-ph.IM2026

picoMUX: microcontroller based time-domain multiplexing readout for kilopixel TES arrays

Simon Tartakovsky, Alexandre E. Adler, Jason E. Austermann +23

Advances in cryogenic SQUID-based time-domain multiplexing (TDM) have outpaced their warm readout electronics. Next generation CMB telescopes are baselining kilopixel TES arrays wi…

astro-ph.IM2026

Sub-Kelvin Cryogenics for a Super-Pressure Balloon-Borne CMB Polarimeter: Taurus

Jared L. May, Alexandre E. Adler, Jason E. Austermann +23

Taurus is a balloon-borne cosmic microwave background (CMB) experiment designed to operate more than 10,000 transition-edge sensor bolometers at a base temperature near 100 mK duri…

astro-ph.IM2024★ 1 cited

In-Flight Performance of Spider's 280 GHz Receivers

Elle C. Shaw, P. A. R. Ade, S. Akers +84

SPIDER is a balloon-borne instrument designed to map the cosmic microwave background at degree-angular scales in the presence of Galactic foregrounds. SPIDER has mapped a large sky…

astro-ph.IM2024

Instrument Overview of Taurus: A Balloon-borne CMB and Dust Polarization Experiment

Jared L. May, Alexandre E. Adler, Jason E. Austermann +20

Taurus is a balloon-borne cosmic microwave background (CMB) experiment optimized to map the E-mode polarization and Galactic foregrounds at the largest angular scales (ℓ <…

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