首页> 外文OA文献 >A 1.4 GHz radio continuum and polarization survey at medium Galactic latitudes: I. Observation and reduction technique
【2h】

A 1.4 GHz radio continuum and polarization survey at medium Galactic latitudes: I. Observation and reduction technique

机译:中型银河系的1.4 GHz无线电连续谱和极化测量   纬度:I。观察和减少技术

代理获取
本网站仅为用户提供外文OA文献查询和代理获取服务,本网站没有原文。下单后我们将采用程序或人工为您竭诚获取高质量的原文,但由于OA文献来源多样且变更频繁,仍可能出现获取不到、文献不完整或与标题不符等情况,如果获取不到我们将提供退款服务。请知悉。

摘要

A radio continuum survey at medium Galactic latitudes with the Effelsberg100-m telescope is being carried out at a centre frequency of 1.4 GHz in totalpower and linear polarization. Areas up to +/- 20 degree of Galactic latitudeare now being observed at a sensitivity of 15 mK TB total intensity and 8 mK TBin linear polarization with an angular resolution of 9'35. This paper describesthe observing and reduction technique applied which results in absolutelycalibrated maps. The methods are illustrated by examples of images from thesurvey.
机译:目前正在使用Effelsberg100米望远镜在银河系中纬度进行连续波无线电调查,其总功率和线性极化的中心频率为1.4 GHz。现在,在总极化强度为15 mK TB和线性极化为8 mK TB且灵敏度为9'35的情况下,观测到的银河纬度范围达+/- 20度。本文介绍了观测和归约技术的应用,它可以产生绝对校准的地图。通过来自调查的图像示例来说明这些方法。

著录项

相似文献

  • 外文文献
  • 中文文献
  • 专利
代理获取

客服邮箱:kefu@zhangqiaokeyan.com

京公网安备:11010802029741号 ICP备案号:京ICP备15016152号-6 六维联合信息科技 (北京) 有限公司©版权所有
  • 客服微信

  • 服务号