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@ARTICLE{RubieraGimeno:627850,
author = {Rubiera Gimeno, José Alejandro and Isleif,
Katharina-Sophie and Januschek, Friederike and Lindner, Axel
and Meyer, Manuel and Othman, Gulden and Rivasto, Elmeri and
Shah, Rikhav and Schwemmbauer, Christina},
title = {{S}imulation and measurement of {B}lack {B}ody {R}adiation
background in a {T}ransition {E}dge {S}ensor},
journal = {Physical review / D},
volume = {112},
number = {3},
issn = {2470-0010},
address = {Ridge, NY},
publisher = {American Physical Society},
reportid = {PUBDB-2025-01633, arXiv:2505.08555},
pages = {032001},
year = {2025},
note = {13 pages, 11 figures},
abstract = {The Any Light Particle Search II (ALPS II) experiment at
DESY, Hamburg, is a Light-Shining-through-a-Wall (LSW)
experiment aiming to probe the existence of axions and
axion-like particles (ALPs), which are candidates for dark
matter. Data collection in ALPS II is underway utilizing a
heterodyne-based detection scheme. A complementary run for
confirmation or as an alternative method is planned using
single photon detection, requiring a sensor capable of
measuring low-energy photons ($1064\,\mathrm{nm}$,
$1.165\,\mathrm{eV}$) with high efficiency (higher than
$50\,\\%$) and a low background rate (below
$7.7\cdot10^{-6}\,\mathrm{cps}$). To meet these
requirements, we are investigating a tungsten Transition
Edge Sensor (TES) provided by NIST, which operates in its
superconducting transition region at millikelvin
temperatures. This sensor exploits the drastic change in
resistance caused by the absorption of a single photon.We
find that the background observed in the setup with a
fiber-coupled TES is consistent with Black Body Radiation
(BBR) as the primary background contributor.A framework was
developed to simulate BBR propagation to the TES under
realistic conditions.The framework not only allows the
exploration of background reduction strategies, such as
improving the TES energy resolution, but also reproduces,
within uncertainties, the spectral distribution of the
observed background.These simulations have been validated
with experimental data, in agreement with the modeled
background distribution, and show that the improved energy
resolution reduces the background rate in the
$1064\,\mathrm{nm}$ signal region by one order of magnitude,
to approximately $10^{-4}\,\mathrm{cps}$. However, this rate
must be reduced further to meet the ALPS II requirements.},
cin = {ALPS},
ddc = {530},
cid = {I:(DE-H253)ALPS-20130318},
pnm = {611 - Fundamental Particles and Forces (POF4-611) / DFG
project G:(GEPRIS)390833306 - EXC 2121: Quantum Universe
(390833306) / AxionDM - Searching for axion and
axion-like-particle dark matter in the laboratory and with
high-energy astrophysical observations (948689)},
pid = {G:(DE-HGF)POF4-611 / G:(GEPRIS)390833306 /
G:(EU-Grant)948689},
experiment = {EXP:(DE-H253)ALPS-20150101},
typ = {PUB:(DE-HGF)16},
eprint = {2505.08555},
howpublished = {arXiv:2505.08555},
archivePrefix = {arXiv},
SLACcitation = {$\%\%CITATION$ = $arXiv:2505.08555;\%\%$},
doi = {10.1103/hqmt-vq1g},
url = {https://bib-pubdb1.desy.de/record/627850},
}