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Spatial distribution of the RRLSs and AC stars ...

Spatial distribution of the RRLSs and AC stars in planar coordinates with the center of ...

A. Katherina Vivas et al, The Astronomical Journal 171 2

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Spatial coverage of our DECam observations of C...

Spatial coverage of our DECam observations of CraII in equatorial coordinates. The gray ...

A. Katherina Vivas et al, The Astronomical Journal 171 2

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Location of the RRLSs and AC stars in the CMD o...

Location of the RRLSs and AC stars in the CMD of CraII. The left panel shows with colore...

A. Katherina Vivas et al, The Astronomical Journal 171 2

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The complete figure set (96 images) is availabl...

The complete figure set (96 images) is available in the online journal.

A. Katherina Vivas et al, The Astronomical Journal 171 2

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Equatorial coordinates of the different types o...

Equatorial coordinates of the different types of RRLSs and AC stars in CraII (V20) and i...

A. Katherina Vivas et al, The Astronomical Journal 171 2

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Number of RRLSs in CraII along the axis of the ...

Number of RRLSs in CraII along the axis of the tails, in bins of ...

A. Katherina Vivas et al, The Astronomical Journal 171 2

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Distribution of extinction-corrected g magnitud...

Distribution of extinction-corrected g magnitudes in the central field of CraII (from V2...

A. Katherina Vivas et al, The Astronomical Journal 171 2

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Left: distance to the RRLSs along the stream as...

Left: distance to the RRLSs along the stream as defined by the line in Figure 6 (right p...

A. Katherina Vivas et al, The Astronomical Journal 171 2

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Proper motion of radial velocity members of Cra...

Proper motion of radial velocity members of CraII (gray asterisks) and AC stars in the c...

A. Katherina Vivas et al, The Astronomical Journal 171 2

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Absolute magnitude vs. period for the AC stars ...

Absolute magnitude vs. period for the AC stars in the central field of CraII (black circ...

A. Katherina Vivas et al, The Astronomical Journal 171 2

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Temporal evolution of the best-fitting blackbod...

Temporal evolution of the best-fitting blackbody temperature T, radius R, bolometric lum...

Natalie LeBaron et al, The Astrophysical Journal Letters 997 1

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AT 2024wpp is the most luminous LFBOT discovere...

AT 2024wpp is the most luminous LFBOT discovered to date. (a) AT 2024wpp in the phase sp...

Natalie LeBaron et al, The Astrophysical Journal Letters 997 1

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Left: collated AT 2024wpp optical spectral seri...

Left: collated AT 2024wpp optical spectral series spanning from +4.1 to +63.0 days from ...

Natalie LeBaron et al, The Astrophysical Journal Letters 997 1

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Left: AT 2024wpp NIR spectral series from +10.0...

Left: AT 2024wpp NIR spectral series from +10.0 to +24.2 days after t0. Spectra are plot...

Natalie LeBaron et al, The Astrophysical Journal Letters 997 1

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UVOIR light curve of AT 2024wpp corrected for ...

UVOIR light curve of AT 2024wpp corrected for Galactic extinction. Offsets are applied ...

Natalie LeBaron et al, The Astrophysical Journal Letters 997 1

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By +35 days, AT 2024wpp shows the emergence of...

By +35 days, AT 2024wpp shows the emergence of clear Hα and He features blueshifted by ...

Natalie LeBaron et al, The Astrophysical Journal Letters 997 1

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Soft X-ray (0.3–10 keV; LX, dark-blue circles),...

Soft X-ray (0.3–10 keV; LX, dark-blue circles), broadband X-ray (0.3–30 keV; LXtot, oran...

Natalie LeBaron et al, The Astrophysical Journal Letters 997 1

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Ratio of the soft (0.3–10 keV) X-ray luminosity...

Ratio of the soft (0.3–10 keV) X-ray luminosity (LX) to LUVOIR (shades of orange) and LN...

Natalie LeBaron et al, The Astrophysical Journal Letters 997 1

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Evolution of the Hα line in AT 2024wpp (left) ...

Evolution of the Hα line in AT 2024wpp (left) and CSS161010 (right; C. P. Gutiérrez et ...

Natalie LeBaron et al, The Astrophysical Journal Letters 997 1

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Assuming that the observed LUVOIR is purely due...

Assuming that the observed LUVOIR is purely due to radiative processing of X-rays (B. D....

Natalie LeBaron et al, The Astrophysical Journal Letters 997 1

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Evolution of the FWHM (top panel), velocity off...

Evolution of the FWHM (top panel), velocity offset (middle panel; i.e., blueshift or red...

Natalie LeBaron et al, The Astrophysical Journal Letters 997 1

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Top panel: blackbody fits to the observed photo...

Top panel: blackbody fits to the observed photometry (blue points) at various epochs (ob...

Natalie LeBaron et al, The Astrophysical Journal Letters 997 1

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Color evolution of AT 2024wpp. The black dashed...

Color evolution of AT 2024wpp. The black dashed lines are extrapolations of the w1–r and...

Natalie LeBaron et al, The Astrophysical Journal Letters 997 1

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Left: multiwavelength light curves for GRB 2308...

Left: multiwavelength light curves for GRB 230815A. The radio data points are represente...

James K. Leung et al, The Astrophysical Journal Letters 997 1

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Radio SEDs of GRB 230815A at the 12 different e...

Radio SEDs of GRB 230815A at the 12 different epochs constructed from the temporal windo...

James K. Leung et al, The Astrophysical Journal Letters 997 1

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