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LoS geometry of M53A relative to Galactic bubbl...

LoS geometry of M53A relative to Galactic bubble structures. Top: composite all-sky map ...

Qiuyi He et al, The Astrophysical Journal Letters 1010 2

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DM and scintillation drift variations of M53A. ...

DM and scintillation drift variations of M53A. From top to bottom: DM measurements from ...

Qiuyi He et al, The Astrophysical Journal Letters 1010 2

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Dynamic spectra of the globular cluster pulsar ...

Dynamic spectra of the globular cluster pulsar M53A at different observing epochs. The h...

Qiuyi He et al, The Astrophysical Journal Letters 1010 2

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Scintillation-arc curvature of M53A referenced ...

Scintillation-arc curvature of M53A referenced to 1.5 GHz. Black points show the measure...

Qiuyi He et al, The Astrophysical Journal Letters 1010 2

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Secondary spectra of the globular cluster pulsa...

Secondary spectra of the globular cluster pulsar M53A at different observing epochs, whe...

Qiuyi He et al, The Astrophysical Journal Letters 1010 2

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Posterior distributions and pairwise correlatio...

Posterior distributions and pairwise correlations of the annual-modulation parameters fo...

Qiuyi He et al, The Astrophysical Journal Letters 1010 2

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Representative illustrations of the SFT pairs u...

Representative illustrations of the SFT pairs used in constructing the cross-correlation...

A. G. Abac et al, The Astrophysical Journal Letters 1010 2

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Ratios of follow-up statistics for candidates f...

Ratios of follow-up statistics for candidates from the search, and from simulated signal...

A. G. Abac et al, The Astrophysical Journal Letters 1010 2

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The search region (black parallelogram) for the...

The search region (black parallelogram) for the present analysis, defined by ...

A. G. Abac et al, The Astrophysical Journal Letters 1010 2

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Selection of follow-up threshold as a function ...

Selection of follow-up threshold as a function of GW frequency. The blue dots represent ...

A. G. Abac et al, The Astrophysical Journal Letters 1010 2

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Upper limits from cross-correlation searches fo...

Upper limits from cross-correlation searches for Sco X-1 in Advanced LIGO data. Left: th...

A. G. Abac et al, The Astrophysical Journal Letters 1010 2

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The marginalized upper limits from Figure 5, co...

The marginalized upper limits from Figure 5, converted to limits on the ellipticity ...

A. G. Abac et al, The Astrophysical Journal Letters 1010 2

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The marginalized upper limits from Figure 5, ex...

The marginalized upper limits from Figure 5, expressed in terms of the quantity known as...

A. G. Abac et al, The Astrophysical Journal Letters 1010 2

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Posterior probability density for the ﹩v\sin i﹩...

Posterior probability density for the ﹩v\sin i﹩ and λ. Blue contours are the 68% and 95%...

Joshua N. Winn et al, The Astrophysical Journal Letters 1010 2

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KPF cross-correlation functions (CCFs) for HD 3...

KPF cross-correlation functions (CCFs) for HD 3167 and four comparison stars with simila...

Joshua N. Winn et al, The Astrophysical Journal Letters 1010 2

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The left panel shows the apparent radial veloci...

The left panel shows the apparent radial velocities of HD 3167 b spanning five separate ...

Joshua N. Winn et al, The Astrophysical Journal Letters 1010 2

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Original V 885 Per discovery plot from A. V. Kh...

Original V 885 Per discovery plot from A. V. Khruslov (2007) (top panel) and my recovery...

Mikhail Yu. Kovalev and Кoвaлёв Mиxaил Юpьeвич, The Astronomical Journal 172 5

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Same as Figure 4, but with analysis of simulate...

Same as Figure 4, but with analysis of simulated TESS data assuming different mass ratio...

Mikhail Yu. Kovalev and Кoвaлёв Mиxaил Юpьeвич, The Astronomical Journal 172 5

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TESS data modeled with W-D.

TESS data modeled with W-D.

Mikhail Yu. Kovalev and Кoвaлёв Mиxaил Юpьeвич, The Astronomical Journal 172 5

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Panels (a) and (b): spectral fitting example in...

Panels (a) and (b): spectral fitting example in two iteration (inner binary phase ϕ = 0....

Mikhail Yu. Kovalev and Кoвaлёв Mиxaил Юpьeвич, The Astronomical Journal 172 5

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SED fit for V 885 Per. Red line shows combined ...

SED fit for V 885 Per. Red line shows combined SED for all three components. Black line ...

Mikhail Yu. Kovalev and Кoвaлёв Mиxaил Юpьeвич, The Astronomical Journal 172 5

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Comparison of ETV measurements with template fi...

Comparison of ETV measurements with template fitting and KvW methods for LC from three T...

Mikhail Yu. Kovalev and Кoвaлёв Mиxaил Юpьeвич, The Astronomical Journal 172 5

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KOREL output for two configurations: three dise...

KOREL output for two configurations: three disentangled components (top), line-strength ...

Mikhail Yu. Kovalev and Кoвaлёв Mиxaил Юpьeвич, The Astronomical Journal 172 5

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O − C curve fit using parabola (dashed line) pl...

O − C curve fit using parabola (dashed line) plus Keplerian orbit (solid line). Gray lin...

Mikhail Yu. Kovalev and Кoвaлёв Mиxaил Юpьeвич, The Astronomical Journal 172 5

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W-D solution for ASAS-SN g LC and “Matryoshka” ...

W-D solution for ASAS-SN g LC and “Matryoshka” based RVs.

Mikhail Yu. Kovalev and Кoвaлёв Mиxaил Юpьeвич, The Astronomical Journal 172 5

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Updated Search and Sort

We have updated the search and sort algorithm to return records in reverse chronological order based on the date/time that the images were uploaded to the Astronomy Image Explorer. This is potentially but rarely different from the publication date. Thank you!