Search Publications

Astronomical Test with CMOS on the 60 cm Telescope at the Xinglong Observatory, NAOC
DOI: 10.1088/1674-4527/ad359a Bibcode: 2024RAA....24e5009M

Fan, Zhou; Zhang, Yu; Wu, Hong +2 more

This work shows details of an evaluation of an observational system comprising a complementary metal-oxide-semiconductor detector, 60 cm telescope and filter complement. The system's photometric precision and differential photometric precision, and extinction coefficients were assessed through observations of Supersky flat fields, open clusters, s…

2024 Research in Astronomy and Astrophysics
Gaia 1
JWST Observations Constrain the Time Evolution of Fine Structure Constants and Dark Energy-electromagnetic Coupling
DOI: 10.1088/1674-4527/ad9198 Bibcode: 2024RAA....24l5012W

Feng, Lei; Lei, Lei; Fan, Yi-Zhong +1 more

It was hypothesized in the literature that some physical parameters may be time-evolving and the astrophysical data can serve as a probe. Recently, the James Webb Space Telescope (JWST) released its early observations. In this work, we select the JWST spectroscopic observations of the high redshift (z > 7.1) galaxies with strong [O III] (λ = 49…

2024 Research in Astronomy and Astrophysics
JWST 1
BSN: The First Light Curve Analysis of the Total Eclipse Binary System EL Tuc
DOI: 10.1088/1674-4527/ad7793 Bibcode: 2024RAA....24j5002S

Poro, Atila; Sarvari, Elham; Fernández Lajús, Eduardo

We conducted the first light curve study of the binary star EL Tuc within the Binary Systems of South and North project's framework. The photometric observations were made using standard multiband BVR c I c filters at an observatory in Argentina. We presented a new ephemeris for EL Tuc and a linear fit to the O – C diagra…

2024 Research in Astronomy and Astrophysics
Gaia 1
Long-term Variation of the Solar Polar Magnetic Fields at Different Latitudes
DOI: 10.1088/1674-4527/ad539a Bibcode: 2024RAA....24g5015Y

Hou, Yijun; Li, Ting; Yang, Shuhong +10 more

The polar magnetic fields of the Sun play an important role in governing solar activity and powering fast solar wind. However, because our view of the Sun is limited in the ecliptic plane, the polar regions remain largely uncharted. Using the high spatial resolution and polarimetric precision vector magnetograms observed by Hinode from 2012 to 202…

2024 Research in Astronomy and Astrophysics
Hinode 1
The Astrometric Performance of the China Space Station Telescope (CSST) Sky Survey in Extending the Gaia Celestial Reference Frame
DOI: 10.1088/1674-4527/ad621e Bibcode: 2024RAA....24h5011Y

Zhu, Zi; Yao, Jun; Liu, Niu +2 more

The multi-color imaging sky survey conducted by the China Space Station Telescope (CSST) holds significant promise for advancing the development of the celestial reference frame. In this study, we focus on assessing the astrometric performance of the CSST celestial reference frame (CSST-CRF) in extending the Gaia Celestial Reference Frame 3 (Gaia-…

2024 Research in Astronomy and Astrophysics
Gaia 1
Investigation of WZ Sge-type Dwarf Nova ASASSN-19oc: Optical Spectroscopy and Multicolor Light Curve Analysis
DOI: 10.1088/1674-4527/ad59ec Bibcode: 2024RAA....24h5002K

Krushevska, Viktoriia; Shugarov, Sergey; Ochner, Paolo +3 more

In this study, we present an investigation of the newly discovered dwarf nova ASASSN-19oc during its superoutburst on 2019 June 2. We carried out detailed UBVR c I c -photometric observations and also obtained a spectrum on day 7 of the outburst, which shows the presence of hydrogen absorption lines commonly found in dwarf…

2024 Research in Astronomy and Astrophysics
Gaia 0
A Preliminary Comparative Study on the Centering Algorithms for Cassini-ISS NAC Images
DOI: 10.1088/1674-4527/ad7822 Bibcode: 2024RAA....24j5001L

Zhang, Q. -F.; Liang, T.; Liu, G. -M. +2 more

Obtaining high precision is an important consideration for astrometric studies using images from the Narrow Angle Camera (NAC) of the Cassini Imaging Science Subsystem (ISS). Selecting the best centering algorithm is key to enhancing astrometric accuracy. In this study, we compared the accuracy of five centering algorithms: Gaussian fitting, the m…

2024 Research in Astronomy and Astrophysics
Gaia 0
Ensemble Learning for Stellar Classification and Radius Estimation from Multimodal Data
DOI: 10.1088/1674-4527/ad86a6 Bibcode: 2024RAA....24k5019D

Luo, A. -Li; Kong, Xiao; Li, Xiang-Ru +2 more

Stellar classification and radius estimation are crucial for understanding the structure of the Universe and stellar evolution. With the advent of the era of astronomical big data, multimodal data are available and theoretically effective for stellar classification and radius estimation. A problem is how to improve the performance of this task by …

2024 Research in Astronomy and Astrophysics
Gaia 0
VLBI with SKA: Possible Arrays and Astrometric Science
DOI: 10.1088/1674-4527/ad420c Bibcode: 2024RAA....24g2001L

Xu, Ye; Liu, Dejian; Hao, Chaojie +4 more

The next generation of very long baseline interferometry (VLBI) is stepping into the era of microarcsecond (µas) astronomy, and pushing astronomy, especially astrometry, to new heights. VLBI with the Square Kilometre Array (SKA), SKA-VLBI, will increase current sensitivity by an order of magnitude, and reach astrometric precision routinely b…

2024 Research in Astronomy and Astrophysics
Gaia 0
V0405 Dra: A New Deep and Low Mass Ratio Contact Binary with Extremely Fast Decrease in the Orbital Period
DOI: 10.1088/1674-4527/ad47dd Bibcode: 2024RAA....24f5023L

Zheng, Jie; Jiang, Lin-Qiao; Tian, Xiao-Man +5 more

V0405 Dra is a W UMa-type binary star. Based on the TESS data, we have conducted an orbital period study and performed a light curve analysis for the system. The orbital period study reveals that the O ‑ C curve for V0405 Dra exhibits secular decrease at an extremely high rate of dP/dt = ‑2.71 × 10‑6 day year‑1, along with pe…

2024 Research in Astronomy and Astrophysics
Gaia 0