(Q58917412)

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Trade-off between angular resolution and straylight contamination in the PLANCK Low Frequency Instrument

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Trade-off between angular resolution and straylight contamination in the PLANCK Low Frequency Instrument (English)

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R. Nesti

3

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Maura Sandri

object named as

M. Sandri

series ordinal

1

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Fabrizio Villa

object named as

F. Villa

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2

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Carlo Burigana

object named as

C. Burigana

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4

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author name string

M. Bersanelli

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5

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N. Mandolesi

series ordinal

6

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language of work or name

English

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publication date

23 November 2004

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published in

Astronomy and Astrophysics

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SIMBAD

volume

428

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issue

1

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page(s)

299–310

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cites work

First‐Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Preliminary Maps and Basic Results

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reference URL

https://api.crossref.org/works/10.1051%2F0004-6361%3A20041435

retrieved

21 January 2018

PLANCK LFI: Comparison between Galaxy Straylight Contamination and other systematic effects

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reference URL

https://api.crossref.org/works/10.1051%2F0004-6361%3A20041435

retrieved

21 January 2018

Trade-off between angular resolution and straylight contamination in the PLANCK Low Frequency Instrument

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stated in

Crossref

reference URL

https://api.crossref.org/works/10.1051%2F0004-6361%3A20041435

retrieved

21 January 2018

On the performance of Planck-like telescopes versus mirror aperture

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Crossref

reference URL

https://api.crossref.org/works/10.1051%2F0004-6361%3A20041435

21 January 2018

1 reference

https://api.crossref.org/works/10.1051%2F0004-6361%3A20041435

retrieved

21 January 2018

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DOI

10.1051/0004-6361:20041435

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(Q58917412)

Trade-off between angular resolution and straylight contamination in the PLANCK Low Frequency Instrument

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