2022-W42-2

Galaxy

2210.03754

  • To See or Not to See a z\sim13 Galaxy? That is the Question

2210.03747

  • Rapid Quenching of Galaxies at Cosmic Noon

2210.04350

  • The evolution of CNO elements in galaxies

2210.04736

  • On the typical width of Herschel filaments

TDE

2210.04115

  • The Study of Dust Formation of Six Tidal Disruption Events

Changing-look AGN

2210.03928

  • Accretion and Host-Galaxy Properties of 14 New "Changing-Look'' Active Galactic Nuclei Identified from the SDSS-V Survey

blazar

2210.04663

  • Modeling the time variable spectral energy distribution of the blazar CTA 102 from 2008 to 2022

FRB

2210.04401

  • Polarisation of magnetospheric curvature radiation in repeating fast radio bursts

GRB

2210.03870

  • The closure relations in optical Afterglow of Gamma-Ray Bursts

UV

2210.04119

  • The UV Excesses of Supernovae and the Implications for Studying Supernovae and Other Optical Transients

JWST

2210.04812

  • The JWST High Redshift Observations and Primordial Non-Gaussianity

2210.04647

  • The Obscured Nucleus and Shocked Environment of VV 114E Revealed by JWST/MIRI Spectroscopy

MUSE

2210.04786

  • MUSE crowded field 3D spectroscopy in NGC 300 III. Characterizing extremely faint HII regions and diffuse ionized gas

LISA

2210.04407

  • Probing Formation of Double Neutron Star Binaries around 1mHz with LISA

Gaia

2210.04721

  • The Gaia-ESO Survey: Lithium measurements and new curves of growth

熟悉的人或源

2210.04190

  • A possible 250-second X-ray quasi-periodicity in the fast blue optical transient AT2018cow
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