The 5σ upper limits as a function of sky position for GW200105_162426, the marginal GW w...

The 5σ flux upper limit as a function of sky position for the six GWs from O3 identified...

The 5σ flux upper limit as a function of sky position for the six GWs from O3 identified...

The redshift-corrected NIRSpec spectrum of D40. The top two panels provide the full spec...

Detection pipeline as performed on GRB180807A. Left: events detected by the pipeline on ...

Distribution of detected stellar flares over Galactic latitude in random trials across 6...

Cumulative distribution functions of the (left) binary and single star population, (midd...

Gaussian fits for M35 for stars within a 0.°5 radius from the cluster center. These fits...

Binary fraction with respect to distance from the cluster center. We plot the binary fra...

Color–magnitude diagram of M35, including the entire sample we downloaded from the Gaia ...

Cumulative distribution functions of the binary and single star population of M35 for st...

Cluster fits for NGC 2682 for stars within a 0.°35 radius from the cluster center. In pi...

King (1962) model fits using only ML-MS stars within r eff. We plot...

Binary fraction plotted against primary-star mass (left) and radius from the cluster cen...

Normalized CDFs of all ML-MS binaries in black and ML-MS single stars in red vs. distanc...

Top: the reconstructed image and contrast curve for 2MASS J08313759+1923395 and its comp...

Percentage of stellar companions detectable within our speckle images vs. distance. Circ...

Top: background-subtracted and normalized light curves of 0.512 s binned Fermi-GBM TTE d...

The 95% credible level for the fifth-force strength ﹩\tilde{\alpha }﹩ derived from the N...

Sky maps showing the GLADE+ K-band apparent magnitude threshold, m ...

The observer-frame (z = 1.49) broadband light curves at 5000–7000 Å of SN Refsdal and th...

Inferred SEDs of three separate underlying components at the positions of the images of ...

Photometry of the five images of SN Refsdal and light-curve fits using the fiducial ligh...

Distributions of total magnification of images S1–S4 and SX of SN Refsdal from microlens...

Simulated source-plane magnification maps for random realizations of stellar microlenses...