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PaglalarawanView of the southern spiral NGC 300.jpg
English: This picture of the spectacular southern spiral galaxy NGC 300 was taken using the Wide Field Imager (WFI) at ESO’s La Silla Observatory in Chile. It was assembled from many individual images through a large set of different filters over many observing nights, spanning several years. The main purpose of this extensive observational campaign was to get an unusually thorough census of the stars in the galaxy, counting both the number and varieties of stars and marking regions, or even individual stars, that warrant deeper and more focussed investigation. But such a rich data collection will also have many other uses for years to come.
The images were mostly taken through filters that transmit red, green or blue light. These were supplemented by images through special filters that allow through only the light from ionised hydrogen or oxygen gas and highlight the glowing clouds in the galaxy’s spiral arms. The total exposure time amounted to around 50 hours.
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Araw at oras ng paggawa ng datos
12:00, 8 Setyembre 2010
Haba
7,603 px
Taas
7,603 px
Mga bit bawat komponente
0
306
2
Iskima ng kompresyon
LZW
Komposisyon ng pixel
RGB
Oryentasyon
Karaniwan
Bilang ng mga komponente
3
Pahigang resolusyon
0.086206896551724 dpi
Patayong resolusyon
296,809 dpi
Pagkakaayos ng datos
pagkaayos sa malalaking bahagi (chunky)
Espasyo ng kulay
Hindi nakaakma sa pamantayang sukat
Balidong taas ng larawan
7,603 px
Balidong lapad ng larawan
7,603 px
Ginamit na software
Adobe Photoshop CS3 Windows
Araw at oras ng ginawang digital
15:15, 22 Oktubre 2010
Araw at oras ng pagpapalit ng talaksan
15:15, 22 Oktubre 2010
Petsa kung kailang huling binago ang metadato
15:15, 22 Oktubre 2010
Pinagmulan
European Southern Observatory
Pagbanggit/Tagapagbigay
ESO
Maiksing pamagat
Wide Field Imager view of the southern spiral NGC 300
Pamagat ng larawan
This picture of the spectacular southern spiral galaxy NGC 300 was taken using the Wide Field Imager (WFI) at ESO’s La Silla Observatory in Chile. It was assembled from many individual images through a large set of different filters over many observing nights, spanning several years. The main purpose of this extensive observational campaign was to get an unusually thorough census of the stars in the galaxy,counting both the number and varieties of stars and marking regions, or even individual stars, that warrant deeper and more focussed investigation. But such a rich data collection will also have many other uses for years to come. The images were mostly taken through filters that transmit red, greenor blue light. These were supplemented by images through special filters that allow through only the light from ionised hydrogen or oxygen gas and highlight the glowing clouds in the galaxy’s spiral arms. The total exposure time amounted to around 50 hours.