English
 
Help Privacy Policy Disclaimer
  Advanced SearchBrowse

Item

ITEM ACTIONSEXPORT

Released

Proceedings

Preflight characterization of the BLAST-TNG receiver and detector arrays

MPS-Authors

Lourie,  Nathan P.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Ade,  Peter A. R.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Angile,  Francisco E.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Ashton,  Peter C.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Austermann,  Jason E.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Devlin,  Mark J.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Dober,  Bradley
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Galitzki,  Nicholas
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Gao,  Jiansong
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Gordon,  Sam
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Groppi,  Christopher E.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Klein,  Jeffrey
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Hilton,  Gene C.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Hubmayr,  Johannes
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Li,  Dale
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Lowe,  Ian
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Mani,  Hamdi
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Mauskopf,  Philip
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

McKenney,  Christopher M.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Nati,  Federico
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Novak,  Giles
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Pascale,  Enzo
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Pisano,  Giampaolo
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Sinclair,  Adrian
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Soler,  Juan D.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Tucker,  Carole
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Ullom,  Joel N.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Vissers,  Michael
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Williams,  Paul A.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Fulltext (restricted access)
There are currently no full texts shared for your IP range.
Fulltext (public)
There are no public fulltexts stored in PuRe
Supplementary Material (public)
There is no public supplementary material available
Citation

Lourie, N. P., Ade, P. A. R., Angile, F. E., Ashton, P. C., Austermann, J. E., Devlin, M. J., et al. (2018). Preflight characterization of the BLAST-TNG receiver and detector arrays.


Cite as: https://hdl.handle.net/21.11116/0000-0005-CC6E-B
Abstract
The Next Generation Balloon-borne Large Aperture Submillimeter Telescope (BLAST-TNG) is a submillimeter mapping experiment planned for a 28 day long-duration balloon (LDB) flight from McMurdo Station, Antarctica during the 2018-2019 season. BLAST-TNG will detect submillimeter polarized interstellar dust emission, tracing magnetic fields in galactic molecular clouds. BLAST-TNG will be the first polarimeter with the sensitivity and resolution to probe the 0.1 parsec-scale features that are critical to understanding the origin of structures in the interstellar medium. BLAST-TNG features three detector arrays operating at wavelengths of 250, 350, and 500 m (1200, 857, and 600 GHz) comprised of 918, 469, and 272 dual-polarization pixels, respectively. Each pixel is made up of two crossed microwave kinetic inductance detectors (MKIDs). These arrays are cooled to 275 mK in a cryogenic receiver. Each MKID has a different resonant frequency, allowing hundreds of resonators to be read out on a single transmission line. This inherent ability to be frequency-domain multiplexed simplifies the cryogenic readout hardware, but requires careful optical testing to map out the physical location of each resonator on the focal plane. Receiver-level optical testing was carried out using both a cryogenic source mounted to a movable xy-stage with a shutter, and a beam-filling, heated blackbody source able to provide a 10-50 C temperature chop. The focal plane array noise properties, responsivity, polarization efficiency, instrumental polarization were measured. We present the preflight characterization of the BLAST-TNG cryogenic system and array-level optical testing of the MKID detector arrays in the flight receiver.