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The results of near-infrared photometric observations of a transit event of an extrasolar planet HAT-P-54b are presented herein. Precise near-infrared photometry was carried out using the Nayuta 2 m telescope at Nishi-Harima Astronomical Observatory, Japan and Nishi-Harima Infrared Camera (NIC). 170 <em>J-</em>, <em>H-</em>, and <em>Ks</em>-band images were taken in each band in 196 minutes. The flux of the planetary system was observed to decrease during the transit event. While the <em>Ks</em>-band transit depth is similar to that in the <em>r</em>-band, the<em> J</em>- and <em>H</em>-band transits are deeper than those in the <em>Ks</em>-band. We constructed simple models of the planetary atmosphere and found that the observed transit depths are well reproduced by inflated atmosphere containing H<sub>2</sub>S molecule.
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篇名 Near-Infrared Transit Photometry of Extra-Solar Planet HAT-P-54b
来源期刊 天文学与天体物理学国际期刊(英文) 学科 地球科学
关键词 Planetary Systems Infrared: Planetary Systems
年,卷(期) 2020,(2) 所属期刊栏目
研究方向 页码范围 89-96
页数 8页 分类号 P14
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Planetary
Systems
Infrared:
Planetary
Systems
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天文学与天体物理学国际期刊(英文)
季刊
2161-4717
武汉市江夏区汤逊湖北路38号光谷总部空间
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333
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0
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