In mid-October of this year, Comet Tsuchinshan-ATLAS graced the evening sky with its magnificent appearance. Its incredible ...

This project is supported by "Project to Promote Large Scientific Frontiers" of MEXT.

Time, Limited Term (up to three (3) years in duration with possible extension for two (2) more years), RCUH Non-Civil ...

説明 ： Low Res. (84 KB) / Mid. Res. (255 KB) / High Res. (1.5MB) おとめ座の方向にあるNGC 5257 と NGC 5258 は、お互いの重力で相互作用する衝突銀河です。同じような大きさと質量 の渦巻銀河のペアで ...

Domeflat in HSC-g 18693400 - 18695357 The flat pattern has changed from the previous run probably due to WFC lens cleaning. Domeflat in HSC-r2 18756600 - 18758557 The flat pattern has changed from the ...

InfraRed Doppler (IRD), which experienced the first light in 2018, is an infrared instrument used in the search for exoplanets (extrasolar planets). IRD is specialized for finding exoplanets with the ...

NGC 5257 and NGC 5258 are gravitationally interacting galaxies of similar size and mass in the constellation Virgo. The pair of spiral galaxies, also known as Arp 240, has a bridge-like interacting ...

The observatory of the Subaru Telescope was officially established in April 1997, following the completion of its base facility building in Hilo, Hawaii. "Subaru Telescope" can refer to the telescope ...

自然科学研究機構国立天文台ハワイ観測所が運用する 口径 8.2 メートルの光学赤外線望遠鏡です。

スービーだよ。どうぞよろしくね！ すばる 望遠鏡 ぼうえんきょう で 宇宙 うちゅう の 観測 かんそく をするためには たくさんの人々の 協力 きょうりょく が 必要 ひつよう なんだ。

This page is an explanation of the quick reduction of Subaru HDS (High Dispersion Spectrograph) data on sumda system at Subaru summit/remote observation system. Basically, this page describes the ...