Loading…

Development of Aluminum LEKIDs for Balloon-Borne Far-IR Spectroscopy

We are developing lumped-element kinetic inductance detectors (LEKIDs) designed to achieve background-limited sensitivity for far-infrared (FIR) spectroscopy on a stratospheric balloon. The spectroscopic terahertz airborne receiver for far-infrared exploration will study the evolution of dusty galax...

Full description

Saved in:
Bibliographic Details
Published in:Journal of low temperature physics 2018-12, Vol.193 (5-6), p.968-975
Main Authors: Hailey-Dunsheath, S., Barlis, A. C. M., Aguirre, J. E., Bradford, C. M., Redford, J. G., Billings, T. S., LeDuc, H. G., McKenney, C. M., Hollister, M. I.
Format: Article
Language:English
Subjects:
Citations: Items that this one cites
Items that cite this one
Online Access:Get full text
Tags: Add Tag
No Tags, Be the first to tag this record!
Description
Summary:We are developing lumped-element kinetic inductance detectors (LEKIDs) designed to achieve background-limited sensitivity for far-infrared (FIR) spectroscopy on a stratospheric balloon. The spectroscopic terahertz airborne receiver for far-infrared exploration will study the evolution of dusty galaxies with observations of the [CII] 158 μ m and other atomic fine-structure transitions at z = 0.5 –1.5, both through direct observations of individual luminous infrared galaxies, and in blind surveys using the technique of line intensity mapping. The spectrometer will require large format ( ∼  1800 detectors) arrays of dual-polarization sensitive detectors with NEPs of 1 × 10 - 17 W Hz - 1 / 2 . The low-volume LEKIDs are fabricated with a single layer of aluminum (20-nm-thick) deposited on a crystalline silicon wafer, with resonance frequencies of 100–250 MHz. The inductor is a single meander with a linewidth of 0.4 μ m , patterned in a grid to absorb optical power in both polarizations. The meander is coupled to a circular waveguide, fed by a conical feedhorn. Initial testing of a small array prototype has demonstrated good yield and a median NEP of 4 × 10 - 18 W Hz - 1 / 2 .
ISSN:0022-2291
1573-7357
DOI:10.1007/s10909-018-1927-y