Event calendar file
21-22 September 2020
Max Planck Institute for Radio Astronomy
Europe/Berlin timezone
Session 4
Place
Location: Max Planck Institute for Radio Astronomy
Address: Auf dem Huegel 69
53123 Bonn
GERMANY
Room: Lecture Hall 0.02
Date:
22 Sep 10:55 - 12:35
Description
Multi pixel cameras. Chair: Dr. Alessandro Orfei
Timetable | Contribution List
Displaying 4
contributions
out of
4
Session:
Session 4
Pulsar studies are generally carried out at centimetre wavelengths and high-energies (X-ray, Gamma-ray), where pulsars are brighter and the available instrumentation is well adapted to fast time-domain science. In the last years, pulsar astronomy in the millimetre band has intensified, supported mainly by large-bandwidth instrumentation with fast-sampling capabilities at the IRAM 30-m telescope. H
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Presented by Dr. Pablo TORNE
on
22/9/2020
at
9:45
Session:
Session 4
QUBIC is an experiment dedicated to the measurement of the B-mode polarization from
the Cosmic Microwave Background (CMB), using a novel technology: Bolometric
Interferometry. The instrument will have 2 focal planes at 150 GHz and 220 GHz. Thanks
to its unique spectroimaging capabilities, QUBIC will also be a powerful instrument to
constrain foreground contamination (thermal galaxy dust emissi
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Presented by Louise MOUSSET
on
22/9/2020
at
8:55
Session:
Session 4
We present the analysis of the optical system of the STRIP instrument, the ground-based telescope of the Large Scale Polarization (LSPE) experiment, which aims at polarization measurements of the Cosmic Microwave Background on large angular scales.
STRIP will observe the polarized emission from the "Observatorio del Teide" in Tenerife, starting in late 2021. The instrument consists of an array of
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Presented by Ms. Sabrina REALINI
on
22/9/2020
at
9:20
Session:
Session 4
We have presented the idea at past meetings to use the mirror arrays of concentrating solar power stations as vast collecting areas for high-sensitivity radio astronomy. Since the signals do not combine coherently they will produce an extended speckle pattern over the focal region that requires a large phased array feed to collect and combine in-phase. The 4000 element EMBRACE array developed un
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Presented by Alan ROY, Olaf WUCKNITZ
on
22/9/2020
at
10:10
