activity
20192026
most citedThe Atacama Cosmology Telescope: DR6 Gravitational Lensing Map and Cosmological Parameters

347 citations · 679 across the 15 of their papers we have counts for

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Showing astro-ph.IMShow all

12 papers · 1 filter

astro-ph.IM2026

Status of BICEP Array and Integration of the 220/270 GHz Receiver

A. Steiger, P. A. R. Ade, Z. Ahmed +83

Measurements of the polarization of the cosmic microwave background are critical for modern cosmology as they constrain the physics of the early universe and cosmic inflation. BICE…

astro-ph.IM2026

Advanced Time-Division Multiplexed Readout Chain for the BICEP Array 90/150 GHz Receiver

B. Cantrall, P. A. R. Ade, Z. Ahmed +89

This work presents the current performance of the advanced time-division multiplexed (TDM) readout chain for the BICEP Array 90/150 GHz receiver. BA4-90/150, scheduled for deployme…

astro-ph.IM2026

Optical characterization of the BICEP array 150 and 220/270GHz CMB polarimeters in the 2026 season

M. Izquierdo Poza, P. A. R. Ade, Z. Ahmed +82

BICEP Array (BA) is the current-generation instrument in the BICEP series of small-aperture, on-axis refracting telescopes at the South Pole, designed to constrain the tensor-to-sc…

astro-ph.IM2026

Overview and status of BICEP Array's BA4-90/150 CMB polarimeter

M. A. Petroff, P. A. R. Ade, Z. Ahmed +83

The inflation paradigm postulates a period of rapid expansion in the early Universe, which would generate gravitational waves. These tensor perturbations would produce a faint B-mo…

astro-ph.IM2023

End-to-End Modeling of the TDM Readout System for CMB-S4

David C. Goldfinger, Zeeshan Ahmed, Darcy R. Barron +13

The CMB-S4 experiment is developing next-generation ground-based microwave telescopes to observe the Cosmic Microwave Background with unprecedented sensitivity. This will require a…

astro-ph.IM2023★ 7 cited

Crosstalk effects in microwave SQUID multiplexed TES bolometer readout

John C. Groh, Zeeshan Ahmed, Shawn W. Henderson +5

Transition-edge sensor (TES) bolometers are broadly used for background-limited astrophysical measurements from the far-infrared to mm-waves. Many planned future instruments requir…