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(a) Plot of LPC orbital period vs. perihelion p...

(a) Plot of LPC orbital period vs. perihelion passage time for LPCs making their first p...

Nathan A. Kaib and Sean N. Raymond, The Planetary Science Journal 7 7

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(a) For the Flyby_7943 simulation, the distribu...

(a) For the Flyby_7943 simulation, the distribution of s2ω at t = 1 Myr is shown for q ...

Nathan A. Kaib and Sean N. Raymond, The Planetary Science Journal 7 7

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(a) The cumulative distribution of s2ω is shown...

(a) The cumulative distribution of s2ω is shown for observed LPCs (thick lines) and simu...

Nathan A. Kaib and Sean N. Raymond, The Planetary Science Journal 7 7

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The cumulative distribution of s2ω is shown for...

The cumulative distribution of s2ω is shown for observed LPCs (thick lines) and simulate...

Nathan A. Kaib and Sean N. Raymond, The Planetary Science Journal 7 7

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Estimated uncertainty of LPC original semimajor...

Estimated uncertainty of LPC original semimajor axis vs. LPC discovery year for dynamica...

Nathan A. Kaib and Sean N. Raymond, The Planetary Science Journal 7 7

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(a) Distribution of inverse original semimajor ...

(a) Distribution of inverse original semimajor axes of dynamically new (a > 104 au) LPCs...

Nathan A. Kaib and Sean N. Raymond, The Planetary Science Journal 7 7

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The distribution of s2ω for Oort cloud orbits i...

The distribution of s2ω for Oort cloud orbits in 10 coadded snapshots of our TIDE simula...

Nathan A. Kaib and Sean N. Raymond, The Planetary Science Journal 7 7

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Distributions of s2ω are shown for LPCs making ...

Distributions of s2ω are shown for LPCs making perihelion passages inside 4 au with a > ...

Nathan A. Kaib and Sean N. Raymond, The Planetary Science Journal 7 7

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Plot of the mean new LPC flux into the inner so...

Plot of the mean new LPC flux into the inner solar system against the impact parameter o...

Nathan A. Kaib and Sean N. Raymond, The Planetary Science Journal 7 7

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Relative Sun-spacecraft geometry at 23: 30 UT o...

Relative Sun-spacecraft geometry at 23: 30 UT on 2024 March 19. The polar plot (J. Giese...

Sabrina Guastavino et al, The Astrophysical Journal Letters 1005 2

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Zoomed-in crop of the flaring site on 2024 Marc...

Zoomed-in crop of the flaring site on 2024 March 19, at a solar-referenced time of 23: 1...

Sabrina Guastavino et al, The Astrophysical Journal Letters 1005 2

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Pixel-level light curves at the intersection be...

Pixel-level light curves at the intersection between the EUI/HRIEUV validity mask and th...

Sabrina Guastavino et al, The Astrophysical Journal Letters 1005 2

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Comparison between SDO/AIA 171 Å and Solar Orbi...

Comparison between SDO/AIA 171 Å and Solar Orbiter/EUI/HRIEUV views of the same solar fl...

Sabrina Guastavino et al, The Astrophysical Journal Letters 1005 2

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Same as Figure 3, but for a solar-referenced ti...

Same as Figure 3, but for a solar-referenced time of 23: 21: 53 UT.

Sabrina Guastavino et al, The Astrophysical Journal Letters 1005 2

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Same as Figure 1, but the spectra are shown on ...

Same as Figure 1, but the spectra are shown on a narrower band to illustrate additional ...

Jon M. Miller et al, The Astrophysical Journal Letters 1005 2

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Swift/XRT spectra of NGC 4151 obtained as part ...

Swift/XRT spectra of NGC 4151 obtained as part of our 2 month continuum monitoring campa...

Jon M. Miller et al, The Astrophysical Journal Letters 1005 2

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The cross-correlation centroid lag probability ...

The cross-correlation centroid lag probability distributions that result from running py...

Jon M. Miller et al, The Astrophysical Journal Letters 1005 2

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Upper panel: the unabsorbed X-ray flux in the f...

Upper panel: the unabsorbed X-ray flux in the full XRISM/Resolve band (2.2–17.4 keV), as...

Jon M. Miller et al, The Astrophysical Journal Letters 1005 2

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Continuum and BLR line flux trends, relative to...

Continuum and BLR line flux trends, relative to local mean values. The XRISM data are ve...

Jon M. Miller et al, The Astrophysical Journal Letters 1005 2

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The nine XRISM spectra of NGC 4151, centered on...

The nine XRISM spectra of NGC 4151, centered on the narrow Fe K − α emission line. The d...

Jon M. Miller et al, The Astrophysical Journal Letters 1005 2

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(a) Modeling of the KR for Sample 1 (n > 1.5)....

(a) Modeling of the KR for Sample 1 (n > 1.5). Top: the marginalized posterior distribu...

Anshuman Borgohain and Kanak Saha, The Astrophysical Journal Letters 1005 2

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(a) False-color images of a few z ≥ 6 galaxies ...

(a) False-color images of a few z ≥ 6 galaxies from our sample that are best fit with a ...

Anshuman Borgohain and Kanak Saha, The Astrophysical Journal Letters 1005 2

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Comparison between structural parameters obtain...

Comparison between structural parameters obtained from unconstrained and constrained GAL...

Anshuman Borgohain and Kanak Saha, The Astrophysical Journal Letters 1005 2

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Kormendy relations derived after excluding all ...

Kormendy relations derived after excluding all DJA-catalog galaxies from the Samples 1 a...

Anshuman Borgohain and Kanak Saha, The Astrophysical Journal Letters 1005 2

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The Kormendy relation for the Sample 1 (n > 1...

The Kormendy relation for the Sample 1 (n > 1.5) galaxies color-coded by stellar mass....

Anshuman Borgohain and Kanak Saha, The Astrophysical Journal Letters 1005 2

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