Receiver
FINER受信システムの仕様(2023年6月現在)
General | |
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バンド数 | 2 (アルマ2のバンド4+5受信機,およびバンド6+7受信機に相当) |
1バンドあたりのビーム数 | 1 |
1バンドあたりの偏波数 | 2 |
1バンドあたりのサイドバンド数 | 2 |
項目 | 低周波バンド(Band 4+5) | 高周波バンド(Band 6+7) |
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観測周波数(RF) | 125−210 GHz | 210−350 GHz |
中間周波数(IF) | 4-20.48 GHz | 4-20.48 GHz |
受信機雑音温度 | 45 K | 75 K |
システムの概要
FINER consists of low- and high-frequency band SIS receivers, each of which covers the ALMA’s Band 4+5 (120-210 GHz) and Band 6+7 (210-350 GHz), respectively. The front-end receivers are followed by the back-end spectrometers with wide-band and high-dispersion modes.
Figure. Block diagram.
光学系
A dual-polarization single beam from each receiver band is coupled with the LMT’s optics. The FINER warm optics is planed to have a beam-switching mechanism which allows a quick (~1 Hz) position switching for atmospheric removal. The spatial resolution (i.e. PSF size) is 7 arcsec X (frequency/200 GHz)^-1, depending on observing frequency.
フロントエンド受信機
The front-end receiver exploits the high critical current density SIS mixer technology (Kojima et al. 2017, 2020) for ALMA 2 (wideband sensitivity upgrade, WSU), which allows us to have a wide instantaneous frequency coverage.
バックエンド分光計
FINER has two sets of digital spectrometers with different spectral resolutions and bandwidths.
- Wide-band spectrometers (DRS4, ELECS Inc.). Analog IF input is digitized by a set of 3-bit 20.48 GSa/s analog-to-digital converters (ADCs), each of which offers a 10.24 GHz bandwidth with a 20 MHz spectral resolution.
- High-resolution spectrometers (XFFTS, RPG). spectroscopy is offered by the array of 2.5-GHz digital spectrometers, XFFTS (RPG).
データ処理
技術文書
Document | Version | Download |
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Proposal | 1-May-2023 | (in prep.) |
Overview | 1-May-2023 | (in prep.) |