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Comparison of the posteriors (solid lines) from...

Comparison of the posteriors (solid lines) from our four different fiducial models, labe...

David Kipping, The Astronomical Journal 171 4

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Network architecture of the real–bogus classifi...

Network architecture of the real–bogus classifier used in this work. (Above) Input image...

A. Inada et al, The Astronomical Journal 171 4

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ROC curve for the autoScan dataset with and wit...

ROC curve for the autoScan dataset with and without using the difference image. The netw...

A. Inada et al, The Astronomical Journal 171 4

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Stamps from the no-Diff dataset. Positive (labe...

Stamps from the no-Diff dataset. Positive (label = 1) and negative (label = 0) examples ...

A. Inada et al, The Astronomical Journal 171 4

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Fake recovery rate (true-positive rate) analysi...

Fake recovery rate (true-positive rate) analysis on the autoScan test data. (Left) Fake ...

A. Inada et al, The Astronomical Journal 171 4

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The difference in accuracy between search–templ...

The difference in accuracy between search–template–difference network and search–templat...

A. Inada et al, The Astronomical Journal 171 4

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ROC Curve for the no-Diff test dataset.

ROC Curve for the no-Diff test dataset.

A. Inada et al, The Astronomical Journal 171 4

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Fake recovery rate (true-positive rate) analysi...

Fake recovery rate (true-positive rate) analysis on the no-Diff dataset. (Left) Fake rec...

A. Inada et al, The Astronomical Journal 171 4

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Infrared spectral variability of CVSO 1942. The...

Infrared spectral variability of CVSO 1942. The blue, orange, and red lines are observat...

Thanawuth Thanathibodee et al, The Astrophysical Journal Letters 999 2

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Left: the light curve of CVSO 1942 from the ALL...

Left: the light curve of CVSO 1942 from the ALLWISE (2010–2011) and NEOWISE (2014-2024) ...

Thanawuth Thanathibodee et al, The Astrophysical Journal Letters 999 2

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Optical light curves of CVSO 1942. Top/middle: ...

Optical light curves of CVSO 1942. Top/middle: The photometry from ZTF DR23 in the g and...

Thanawuth Thanathibodee et al, The Astrophysical Journal Letters 999 2

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Hα profiles of CVSO 1942 across 15 yr. The blue...

Hα profiles of CVSO 1942 across 15 yr. The blue lines represent the observations, the re...

Thanawuth Thanathibodee et al, The Astrophysical Journal Letters 999 2

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Binary disruption timescale (left) and v∞,smbh ...

Binary disruption timescale (left) and v∞,smbh (right) as a function of Hills disruption...

Matthew W. Hosek et al, The Astrophysical Journal Letters 999 2

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The orbit of IRS 9, integrated for the past 0.4...

The orbit of IRS 9, integrated for the past 0.4 Myr and assuming dlos = 0 pc. In each pa...

Matthew W. Hosek et al, The Astrophysical Journal Letters 999 2

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The observed v3d distribution of 32 stars with ...

The observed v3d distribution of 32 stars with projected radii within ±1″ of IRS 9 (blac...

Matthew W. Hosek et al, The Astrophysical Journal Letters 999 2

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The 23 SiO masers examined in this study, overl...

The 23 SiO masers examined in this study, overlaid on an HST F153M image. The green squa...

Matthew W. Hosek et al, The Astrophysical Journal Letters 999 2

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Maser v3d as a function of r2d. A model for ...

Maser v3d as a function of r2d. A model for ﹩{v}_{{\rm{esc}},{\rm{\max }}}﹩ and the corr...

Matthew W. Hosek et al, The Astrophysical Journal Letters 999 2

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HST proper-motion error as a function of magnit...

HST proper-motion error as a function of magnitude for the SiO masers compared to the HS...

Matthew W. Hosek et al, The Astrophysical Journal Letters 999 2

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A comparison of the HST and radio proper-motion...

A comparison of the HST and radio proper-motion measurements for the masers (left panel)...

Matthew W. Hosek et al, The Astrophysical Journal Letters 999 2

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Different calculated properties for the orbit o...

Different calculated properties for the orbit of IRS 9 as a function of dlos. Left: v∞,s...

Matthew W. Hosek et al, The Astrophysical Journal Letters 999 2

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DM velocity profiles as a function of radial di...

DM velocity profiles as a function of radial distance from the GC for the velocity dispe...

Shyam Balaji et al, The Astrophysical Journal Letters 999 2

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511 keV line longitude profile (left panel) and...

511 keV line longitude profile (left panel) and latitude profiles (right panel) for XDM ...

Shyam Balaji et al, The Astrophysical Journal Letters 999 2

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511 keV line longitude profiles (left panel) an...

511 keV line longitude profiles (left panel) and latitude profiles (right panel) compare...

Shyam Balaji et al, The Astrophysical Journal Letters 999 2

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Similar to Figure 2 but for mχ = 1.5 TeV and va...

Similar to Figure 2 but for mχ = 1.5 TeV and varied Δm, for the respective 511 keV fit c...

Shyam Balaji et al, The Astrophysical Journal Letters 999 2

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Same as in Figure 1, but for a fixed mass of mχ...

Same as in Figure 1, but for a fixed mass of mχ = 1.5 TeV with different variations of Δ...

Shyam Balaji et al, The Astrophysical Journal Letters 999 2

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