B − V (z-axis) and V − i (y-axis) multicolor evolution of the KSP Type Ia SNe along the ...

A comparison of the multiwavelength observations of the Sticks cloud used in this analys...

Magnetic ambient field lines of the 2021 March 21 event. The left panel shows the topolo...

Optical lightcurves of HD 251108. Error bars are omitted for clarity. Top: DASCH lightcu...

Dissociation point selection criteria (Interactive figure). The top panel shows the SOS1...

Simulation of the evolution of the Orpheus Association over the next 60 Myr, presented i...

The same as Figure 18, but for the Cinyras Association. An interactive version of this f...

The same as Figure 18, but for the Cupavo Association. An interactive version of this fi...

Overview plot for the Orpheus Association, showing the distribution of groups in l/b sky...

Environment of Hedgehog. We show the distribution of neighboring galaxies from Karachent...

Three-dimensional images of the ray-trace for a source with a continuum spectrum over a ...

Ray-trace like Figure 4, but for a tilted Rowland torus setup. See Figure 4 for an expla...

Ray-trace like Figure 4, but for a tilted Rowland torus setup with four channels with of...

Postage stamps of the 100 brightest of our Tier 1 sources in an emission filter. All ima...

Multiwavelength image of the 3C 220.3 system. F606W, F814W, and F160W are shown in blue,...

Projected maps showing the coverage of the data used in the work at a healpix resolution...

Histograms illustrating the wavelength coverage of the data used in this work that serve...

The N H from the APED fits plotted vs. the N ...

The surface flux plotted against the modeled age of the ONC stars The ages are taken fro...

The measured line widths from the single line fits. Gray boxes show the regions where th...

The coronal temperatures from the APED fits vs. the surface flux. An interactive version...

The emission measures from the APED fits plotted vs. the temperatures from the fits. Thi...

The mean number density of stars in (overlapping) distance bins ranging from d = 0–50 kp...

As Figure 11, but now showing the ratio between the data and the prior. This highlights ...

As Figure 11, but now showing the expected distribution of sources from the Galactic pri...