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University of Groningen

Wide band instantaneous coverage receiver concept for ALMA

Adema, Joost; Baryshev, Andrey

DOI:

10.5281/zenodo.3240307

IMPORTANT NOTE: You are advised to consult the publisher's version (publisher's PDF) if you wish to cite from

it. Please check the document version below.

Document Version

Publisher's PDF, also known as Version of record

Publication date:

2019

Link to publication in University of Groningen/UMCG research database

Citation for published version (APA):

Adema, J., & Baryshev, A. (2019). Wide band instantaneous coverage receiver concept for ALMA.

https://doi.org/10.5281/zenodo.3240307

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Downloaded from the University of Groningen/UMCG research database (Pure): http://www.rug.nl/research/portal. For technical reasons the number of authors shown on this cover page is limited to 10 maximum.

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Wide band instantaneous

coverage receiver

concept for ALMA

Andrey Baryshev, Kirill Rudakov, Ronald Hesper,

Andrey Khudchenko, Daniel Montofre, J. Adema,

Rob de Haan Stijkel, Pavel Dmitriev, Valery

(3)

ALMA development workshop

Improve ALMA!

How can we improve current ALMA

system

Ø

Improve sensitivity of SIS mixer (Quantum

limited performance @ 260 GHz)

Ø

Improve instantaneous RF bandwidth (dual

frequency operation = 1

st

step)

Ø

Ultra wide instantaneous coverage

(4)

ALMA development workshop

(5)

ALMA development workshop

Dual frequency ALMA B6/9

Benefits:

ØImproved phase calibration

ØEnabling the highest resolution imaging

with ALMA

ØObservation of transient phenomena

ØHigh redshift resolved cosmic star

formation history

(6)

ALMA development workshop

Frequency Array Receiver

Only small part is covered Instantaneously (one bar) or at best 3 bands for current receivers (3 bars)

Antenna

Superconducting Transmission line

Band Pass Filter

SIS mixer

channel 1 SIS mixerchannel n Load

(7)

ALMA development workshop

Key advantages

n

All atomic/molecular lines are available in one go

in high resolution

n

Much more information is available for

atmospheric transmission correction

n

Possibility to study large spectral features (dust)

n

Possibility to exclude atmospheric line forest –

background limited total power performance

n

Blind red shifted CII, CO, CI search

(SUPERSPEC, DESHIMA science)

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