activity
20142024
most citedHigh resolution transmission spectrum of the Earth's atmosphere -- Seeing Earth as an exoplanet using a lunar eclipse

51 citations · 142 across the 11 of their papers we have counts for

collaborators

11 papers

astro-ph.EP2024

The Terminator Region Atmosphere of the hot Jupiter WASP-77Ab with ESPRESSO/VLT observations

Zewen Jiang, Wei Wang, Guo Chen +5

Atmospheric studies are essential for elucidating the formation history, evolutionary processes, and atmospheric dynamics of exoplanets. High-resolution transmission spectroscopy o…

astro-ph.SR2023★ 11 cited

Photometric calibration of the Stellar Abundance and Galactic Evolution Survey (SAGES): Nanshan One-meter Wide-field Telescope g, r, and i band imaging data

Kai Xiao, Haibo Yuan, Bowen Huang +16

In this paper, a total of approximately 2.6 million dwarfs were constructed as standard stars, with an accuracy of about 0.01-0.02 mag for each band, by combining spectroscopic dat…

astro-ph.EP2023★ 7 cited

The Tianlin Mission: a 6m UV/Opt/IR space telescope to explore the habitable worlds and the universe

Wei Wang, Meng Zhai, Gang Zhao +7

[Abridged] It is expected that the ongoing and future space-borne planet survey missions including TESS, PLATO, and Earth 2.0 will detect thousands of small to medium-sized planets…

astro-ph.GA2023

Beyond spectroscopy. II. Stellar parameters for over twenty million stars in the northern sky from SAGES DR1 and Gaia DR3

Yang Huang, Timothy C. Beers, Hai-Bo Yuan +18

We present precise photometric estimates of stellar parameters, including effective temperature, metallicity, luminosity classification, distance, and stellar age, for nearly 26 mi…

astro-ph.GA2023

The Stellar Abundances and Galactic Evolution Survey (SAGES) -- -- I. General Description and the First Data Release (DR1)

Zhou Fan, Gang Zhao, Wei Wang +35

The Stellar Abundances and Galactic Evolution Survey (SAGES) of the northern sky is a specifically-designed multi-band photometric survey aiming to provide reliable stellar paramet…

astro-ph.EP2023★ 10 cited

Detection of rubidium and samarium in the atmosphere of the ultra-hot Jupiter MASCARA-4b

Zewen Jiang, Wei Wang, Gang Zhao +5

Ultra-hot Jupiters (UHJs) possess the most extreme environments among various types of exoplanets, making them ideal laboratories to study the chemical composition and kinetics pro…

astro-ph.EP2023★ 14 cited

Detection of TiO and VO in the atmosphere of WASP-121b and Evidence for its temporal variation

Qinglin Ouyang, Wei Wang, Meng Zhai +6

We report the transit observations of the ultra hot Jupiter WASP-121b using the Goodman High Throughput Spectrograph (GHTS) at the 4-meter ground-based telescope Southern Astrophys…

astro-ph.EP2023★ 9 cited

Thermal Emission from the hot Jupiter WASP-103b in J and Ks Bands

Yaqing Shi, Wei Wang, Gang Zhao +8

Hot Jupiters, particularly those with temperature higher than 2000 K are the best sample of planets that allow in-depth characterization of their atmospheres. We present here a the…

astro-ph.EP2023★ 10 cited

Tentative detection of titanium oxide in the atmosphere of WASP-69 b with a 4m ground-based telescope

Qinglin Ouyang, Wei Wang, Meng Zhai +6

Transiting planets provide unique opportunities for the atmospheric characterization of exoplanets as they can reveal composition and the temperature structures at the day-night te…

astro-ph.EP2023★ 30 cited

The Masses of a Sample of Radial-Velocity Exoplanets with Astrometric Measurements

Guang-Yao Xiao, Yu-Juan Liu, Huan-Yu Teng +6

Being one of the most fundamental physical parameter of astronomical objects, mass plays a vital role in the study of exoplanets, including their temperature structure, chemical co…

astro-ph.EP2014★ 51 cited

High resolution transmission spectrum of the Earth's atmosphere -- Seeing Earth as an exoplanet using a lunar eclipse

Fei Yan, Robert A. E. Fosbury, Monika G. Petr-Gotzens +5

With the rapid developments in the exoplanet field, more and more terrestrial exoplanets are being detected. Characterising their atmospheres using transit observations will become…