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Per-sector TESS multi-pipeline analysis of Gaia...

Per-sector TESS multi-pipeline analysis of Gaia DR3 3183786280737192704 (TIC 43488669). ...

Scott Greenberg, Research Notes of the AAS 10 5

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Schematic illustration of the geometry of secul...

Schematic illustration of the geometry of secular acceleration. The star moves with cons...

Szilárd Csizmadia, Research Notes of the AAS 10 5

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The ratio of the standard deviation (SD) to the...

The ratio of the standard deviation (SD) to the mean error (σ) of the NEOWISE epoch medi...

Zihan Kang et al, The Astrophysical Journal Supplement Series 284 2

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Distribution of cross-correlation coefficients ...

Distribution of cross-correlation coefficients derived from a preliminary simulation. Th...

Zihan Kang et al, The Astrophysical Journal Supplement Series 284 2

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The left panel illustrates the distribution of ...

The left panel illustrates the distribution of the cluster results derived from the algo...

Zihan Kang et al, The Astrophysical Journal Supplement Series 284 2

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Two primary types of artificial variable light ...

Two primary types of artificial variable light curves. The left panel illustrates the ar...

Zihan Kang et al, The Astrophysical Journal Supplement Series 284 2

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The criteria for filtering out the two types of...

The criteria for filtering out the two types of artifacts. The left panel displays the r...

Zihan Kang et al, The Astrophysical Journal Supplement Series 284 2

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The distribution of amplitude and minimum ampli...

The distribution of amplitude and minimum amplitude at different magnitudes in our sampl...

Zihan Kang et al, The Astrophysical Journal Supplement Series 284 2

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The architecture of the autoencoder neural netw...

The architecture of the autoencoder neural network to extract morphological features of ...

Zihan Kang et al, The Astrophysical Journal Supplement Series 284 2

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The anomaly scores’ distribution of different a...

The anomaly scores’ distribution of different algorithms at both bands. A large score me...

Zihan Kang et al, The Astrophysical Journal Supplement Series 284 2

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Some example light curves for the identified ou...

Some example light curves for the identified outliers. The quoted anomaly scores come fr...

Zihan Kang et al, The Astrophysical Journal Supplement Series 284 2

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The spectra of our broad-line AGN and the best-...

The spectra of our broad-line AGN and the best-fit result. For each source, the top pane...

Qinyue Fei et al, The Astrophysical Journal 1003 2

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Location of broad-line AGNs in the survey field...

Location of broad-line AGNs in the survey field. The NIRSpec footprint is indicated by t...

Qinyue Fei et al, The Astrophysical Journal 1003 2

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Example of the best-fit galaxy and AGN composit...

Example of the best-fit galaxy and AGN composite SED of our sample, ID13131. The red dat...

Qinyue Fei et al, The Astrophysical Journal 1003 2

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Panel (a) displays the 2D NIRSpec spectrum, whi...

Panel (a) displays the 2D NIRSpec spectrum, while panel (b) shows the corresponding 1D s...

Qinyue Fei et al, The Astrophysical Journal 1003 2

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BHMF derived from this study. Left: the measure...

BHMF derived from this study. Left: the measured BHMF and the empirical relation. Our so...

Qinyue Fei et al, The Astrophysical Journal 1003 2

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Completeness of broad Hα emission line detectio...

Completeness of broad Hα emission line detection. The colored contours denote 0.1, 0.5, ...

Qinyue Fei et al, The Astrophysical Journal 1003 2

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Relation between BH mass and galaxies’ stellar ...

Relation between BH mass and galaxies’ stellar mass for our sources. Our sources are sho...

Qinyue Fei et al, The Astrophysical Journal 1003 2

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BPT diagrams of our targets. The distribution o...

BPT diagrams of our targets. The distribution of local galaxies from the Sloan Digital S...

Qinyue Fei et al, The Astrophysical Journal 1003 2

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Illustration of our mock spectrum. Panel (a) di...

Illustration of our mock spectrum. Panel (a) displays the mock spectrum of the. In this ...

Qinyue Fei et al, The Astrophysical Journal 1003 2

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Accuracy of our BH mass measurement. Top: outpu...

Accuracy of our BH mass measurement. Top: output BH masses compared to the input BH mass...

Qinyue Fei et al, The Astrophysical Journal 1003 2

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BH mass and UV magnitude of our selected broad-...

BH mass and UV magnitude of our selected broad-line AGNs (red circles), where filled cir...

Qinyue Fei et al, The Astrophysical Journal 1003 2

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Fitting results. Similar to those shown in Figu...

Fitting results. Similar to those shown in Figure B1.

Qinyue Fei et al, The Astrophysical Journal 1003 2

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Comparison between M* derived from two differen...

Comparison between M* derived from two different methods. Two outliers, ID 5536 and ID 7...

Qinyue Fei et al, The Astrophysical Journal 1003 2

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CIGALE fitting result for all our sources. Labe...

CIGALE fitting result for all our sources. Labels in this plot are the same as those in ...

Qinyue Fei et al, The Astrophysical Journal 1003 2

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