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jra:rings [2017/03/14 14:40]
irottmann
jra:rings [2017/03/14 14:44]
irottmann
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 ===== WP7 JRA RINGS ====== ===== WP7 JRA RINGS ======
-The main objective ​of BRAND EVN (BRoad bAND EVN) is to develop and build a prototype broad-band digital +The main objective ​for RINGS (Radio Interferometry Next Generation Software) is to deliver advanced calibration algorithms for the next generation of radio astronomy facilitiescharacterized by high sensitivity, a high bandwidth and long baselines ​({{:jra:730562_radionet_wp7.pdf|RINGS Description}}).
-receiverwhich will cover frequency range from 1.5 GHz to 15.5 GHz (1:10 rangechosen to include the 2 cm VLBA +
-band). The BRAND frontend can be adapted to different EVN antennas. The backend part can also be used for other +
-receivers with RF frequency or IF range between 0-16 GHz. ({{:jra:730562_radionet_wp6.pdf|BRAND EVN Description}}).+
  
-**The RINGS parter:** MPG, ASTRON, ​INAFOSOUAH-IGNVUC+**The RINGS parter:** MPG, ASTRON, ​JIV-ERICUMANOSODIAS
  
 **The RINGS tasks:** **The RINGS tasks:**
-  * WP6.1: Feasibility survey of EVN antennas ​[UAH, OSO, INAF+  * WP7.1 Methodology and approach ​[ASTRONUMAN OSO, JIV-ERIC, MPG, DIAS
-  * WP6.2: BRAND receiver frontend ​[MPG, INAF, OSO, UAH+  * WP7.2 Polarimetry Conversion ​[OSO, DIAS
-  * WP6.3: BRAND backend ​[INAFMPGASTRON, VUC+  * WP7.3: Multiband and Wide Band Fringe Fitting ​[JIV-ERICDIASMPG
-  * WP6.4: Control, recording and correlation software ​[INAFMPGOSOASTRON+  * WP7.4: Fringe Fitting with dispersive delays ​[UMANASTRONDIASMPG
-  * WP6.5: Integration at telescope and test observation ​[INAF, MPG, OSO, UAH+  * Task 7.5: Advanced calibration algorithms for full-polarization interferometry data [OSO, DIAS
- +  ​* ​ 
-This activity is lead by MPG - Leader ​WAlef.+This activity is lead by ASTRON ​- Leader ​GKruithof.
  
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jra/rings.txt · Last modified: 2021/03/02 09:24 by jcasado