kava kasi.re.kr

Welcom to KaVA

KVN and VERA Array. Guidelines of KaVA observation preparation. Guidelines of KaVA data analysis. KaVAKVN and VERA Array is a combined VLBI array with KVN Korean VLBI Network and VERA VLBI Exploration of Radio Astrometry operated by Korea Astronomy and Space Science Institute KASI and National Astronomical Observatory of Japan NAOJ, respectively. More. First fringe between KVN and VERA array. The first VLBI image of Class-I 44 GHz methanol maser with KaVA! UST-GUAS Radio astronomy winter school.
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This web site kava.kasi.re.kr presently has an average traffic classification of zero (the lower the more traffic). We have evaluated one page inside the website kava.kasi.re.kr and found two websites linking to kava.kasi.re.kr.
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KAVA.KASI.RE.KR HOST

Our web crawlers diagnosed that a single root page on kava.kasi.re.kr took four thousand five hundred and forty-seven milliseconds to load. Our web crawlers could not observe a SSL certificate, so our parsers consider this site not secure.
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SSL
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Internet Address
210.219.33.102

SERVER OPERATING SYSTEM AND ENCODING

I revealed that this domain is utilizing the Apache/2.2.15 (Red Hat) operating system.

TITLE

Welcom to KaVA

DESCRIPTION

KVN and VERA Array. Guidelines of KaVA observation preparation. Guidelines of KaVA data analysis. KaVAKVN and VERA Array is a combined VLBI array with KVN Korean VLBI Network and VERA VLBI Exploration of Radio Astrometry operated by Korea Astronomy and Space Science Institute KASI and National Astronomical Observatory of Japan NAOJ, respectively. More. First fringe between KVN and VERA array. The first VLBI image of Class-I 44 GHz methanol maser with KaVA! UST-GUAS Radio astronomy winter school.

CONTENT

This web site has the following in the web site, "Guidelines of KaVA observation preparation." Our analyzers noticed that the web page also stated " Guidelines of KaVA data analysis." The Website also said " KaVAKVN and VERA Array is a combined VLBI array with KVN Korean VLBI Network and VERA VLBI Exploration of Radio Astrometry operated by Korea Astronomy and Space Science Institute KASI and National Astronomical Observatory of Japan NAOJ, respectively. First fringe between KVN and VERA array. The first VLBI image of Class-I 44 GHz methanol maser with KaVA! UST-GUAS Radio astronomy winter school."

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