L-BASS: a project to produce an absolutely calibrated 1.4 GHz sky map I – Scientific rationale and system overview

ABSTRACT L-BASS is an instrument designed to produce an absolutely calibrated map of the sky at a wavelength of 21 cm (L-band) with a radiometric accuracy of $\le 0.1$ K and with an angular resolution of $23^{\circ }$. The prime motivations are to improve the temperature calibration of higher resolution maps and to investigate the steep spectrum radio background proposed by the ARCADE 2 team. The instrument consists of a pair of conical horn antennas which can scan independently in elevation; each antenna produces a circularly polarized output. The difference in signals from the antennas is measured with a continuous-comparison receiver connected to a digital spectrometer sampling the signal from 1400 to 1425 MHz within the protected radio astronomy band. We describe the astrophysical motivation for the project, the design requirements, and how these will be attained.

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Publication Details

Journal
RAS Techniques and Instruments
Published
2025-01-01
DOI
https://doi.org/10.1093/rasti/rzaf017
Citations
3
Primary Topic
Radio Astronomy Observations and Technology
Type
article
Field-Weighted Citation Impact
3.46

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article

L-BASS: a project to produce an absolutely calibrated 1.4 GHz sky map I – Scientific rationale and system overview

J. P. Leahy, Christopher Radcliffe, I. W. A. Browne, P. N. Wilkinson et al.
3 citations
RAS Techniques and Instruments
Radio Astronomy Observations and Technology
3.46
article

L-BASS: a project to produce an absolutely calibrated 1.4 GHz sky map I – Scientific rationale and system overview

J. P. Leahy, Christopher Radcliffe, I. W. A. Browne, P. N. Wilkinson, Peter Black, D P Zerafa
article en
3 citations

Abstract

ABSTRACT L-BASS is an instrument designed to produce an absolutely calibrated map of the sky at a wavelength of 21 cm (L-band) with a radiometric accuracy of $\le 0.1$ K and with an angular resolution of $23^{\circ }$. The prime motivations are to improve the temperature calibration of higher resolution maps and to investigate the steep spectrum radio background proposed by the ARCADE 2 team. The instrument consists of a pair of conical horn antennas which can scan independently in elevation; each antenna produces a circularly polarized output. The difference in signals from the antennas is measured with a continuous-comparison receiver connected to a digital spectrometer sampling the signal from 1400 to 1425 MHz within the protected radio astronomy band. We describe the astrophysical motivation for the project, the design requirements, and how these will be attained.

RAS Techniques and InstrumentsVol. 4
Age UK (GB), University of Manchester (GB)
Science and Technology Facilities Council
Openalex Percentile: Top 8%
Radio Astronomy Observations and Technology
3.46
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L-BASS: a project to produce an absolutely calibrated 1.4 GHz sky map I – Scientific rationale and system overview — J. P. Leahy, Christopher Radcliffe, et al. · RAS Techniques and Instruments (2025) | TGRS Research Map | TGRS