output
20022026
most citedThe Gaia mission

7.1k citations

Showing 2023 · astro-ph.IMShow all

23 papers · 2 filters

astro-ph.IM2023★ 15 cited

: An Accurate Photometric Classifier for Tidal Disruption Events

Robert Stein, Ashish Mahabal, Simeon Reusch +12

Optical surveys have become increasingly adept at identifying candidate Tidal Disruption Events (TDEs) in large numbers, but classifying these generally requires extensive spectros…

astro-ph.IM2023★ 8 cited

Polarization-dependent beam shifts upon metallic reflection in high-contrast imagers and telescopes

R. G. van Holstein, C. U. Keller, F. Snik +1

(Abridged) Context. To directly image rocky exoplanets in reflected (polarized) light, future space- and ground-based high-contrast imagers and telescopes aim to reach extreme cont…

astro-ph.IM2023★ 2 cited

Integrated photonic-based coronagraphic systems for future space telescopes

Niyati Desai, Lorenzo König, Emiel Por +38

The detection and characterization of Earth-like exoplanets around Sun-like stars is a primary science motivation for the Habitable Worlds Observatory. However, the current best te…

astro-ph.IM2023★ 8 cited

1-arcsecond imaging of ELAIS-N1 field at 144MHz using the LoTSS survey with international LOFAR telescope

Haoyang Ye, Frits Sweijen, Reinout van Weeren +10

We present the first wide area (2.5 x 2.5 deg^2) LOFAR High Band Antenna image at a resolution of 1.2'' x 2'' with a median noise of approximately 80 microJy per beam. It was made…

astro-ph.IM2023★ 14 cited

Water ice: temperature-dependent refractive indexes and their astrophysical implications

W. R. M. Rocha, M. G. Rachid, M. K. McClure +2

Interstellar ices are largely composed of frozen water. It is important to derive fundamental parameters for HO ice such as absorption and scattering opacities for which accura…

astro-ph.IM2023★ 4 cited

A novel radio imaging method for physical spectral index modelling

E. Ceccotti, A. R. Offringa, L. V. E. Koopmans +9

We present a new method, called "forced-spectrum fitting", for physically-based spectral modelling of radio sources during deconvolution. This improves upon current common deconvol…