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The BSS and upper main-sequence regions of the ...

The BSS and upper main-sequence regions of the M67, NGC 188, and NGC 6791 CMDs. The BSS ...

Evan Linck and Robert D. Mathieu, The Astrophysical Journal Letters 1005 1

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The BSS ﹩v\sin i﹩ distribution by effective tem...

The BSS ﹩v\sin i﹩ distribution by effective temperature, color coded by cluster (M67: re...

Evan Linck and Robert D. Mathieu, The Astrophysical Journal Letters 1005 1

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The rotation periods of the BSSs and blue lurke...

The rotation periods of the BSSs and blue lurkers (BLs) vs. Teff. BSSs and BLs with know...

Evan Linck and Robert D. Mathieu, The Astrophysical Journal Letters 1005 1

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We show the Teff–﹩v\sin i﹩ distribution of BSSs...

We show the Teff–﹩v\sin i﹩ distribution of BSSs in open clusters (upper panel, in red, f...

Evan Linck and Robert D. Mathieu, The Astrophysical Journal Letters 1005 1

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Comparison of the rotational velocity distribut...

Comparison of the rotational velocity distributions of open and globular clusters using ...

Evan Linck and Robert D. Mathieu, The Astrophysical Journal Letters 1005 1

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Intuition for the peak-ranking step that underp...

Intuition for the peak-ranking step that underpins the decomposition. The descending wat...

Carlos Vera-Ciro, The Astronomical Journal 172 1

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Survey-scale products derived from the decompos...

Survey-scale products derived from the decomposition (GRS tiles 26–34, ℓ ≈ 25°–35°). All...

Carlos Vera-Ciro, The Astronomical Journal 172 1

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Representative PHSPECTRA decompositions at β = ...

Representative PHSPECTRA decompositions at β = 3.5. Each panel shows the data (gray step...

Carlos Vera-Ciro, The Astronomical Journal 172 1

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Head-to-head comparison on real data. Per-spect...

Head-to-head comparison on real data. Per-spectrum residual rms: PHSPECTRA versus GAUSSP...

Carlos Vera-Ciro, The Astronomical Journal 172 1

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Normalized distributions of velocity separation...

Normalized distributions of velocity separations Δv between adjacent fitted components, ...

Carlos Vera-Ciro, The Astronomical Journal 172 1

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Robustness to the sole free parameter. F1 score...

Robustness to the sole free parameter. F1 score versus β for each synthetic benchmark ca...

Carlos Vera-Ciro, The Astronomical Journal 172 1

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PHSPECTRA pipeline.

PHSPECTRA pipeline.

Carlos Vera-Ciro, The Astronomical Journal 172 1

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The input sample of the modeled planet populati...

The input sample of the modeled planet population for our mission simulations. These mod...

George Zhou et al, The Astronomical Journal 172 1

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Top: one of the Orion target fields is shown in...

Top: one of the Orion target fields is shown in the Two Micron All Sky Survey (2MASS) J ...

George Zhou et al, The Astronomical Journal 172 1

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Survey fields of EVE aligned to the distributio...

Survey fields of EVE aligned to the distribution of young stars. EVE will survey ≈30 sep...

George Zhou et al, The Astronomical Journal 172 1

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The stellar property distribution encompassed w...

The stellar property distribution encompassed within the EVE fields is plotted over the ...

George Zhou et al, The Astronomical Journal 172 1

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The modeled photometric scatter of EVE in the o...

The modeled photometric scatter of EVE in the optical (blue) and NIR (maroon), compared ...

George Zhou et al, The Astronomical Journal 172 1

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Expected planet yield of a simultaneous NUV, op...

Expected planet yield of a simultaneous NUV, optical, and NIR wide-field survey, assumin...

George Zhou et al, The Astronomical Journal 172 1

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Planet recovery probability given transit SNR. ...

Planet recovery probability given transit SNR. Each line shows the probability of recove...

George Zhou et al, The Astronomical Journal 172 1

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Distribution of expected EVE planets from the g...

Distribution of expected EVE planets from the gas-dwarf model shown with Galactic coordi...

George Zhou et al, The Astronomical Journal 172 1

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The optical and NIR channels make nearly equal ...

The optical and NIR channels make nearly equal contributions to the total planet yield o...

George Zhou et al, The Astronomical Journal 172 1

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EVE will probe transit depth differences in the...

EVE will probe transit depth differences in the optical and infrared. Spectral models of...

George Zhou et al, The Astronomical Journal 172 1

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The distribution of simulated planet detections...

The distribution of simulated planet detections in radius, period, and age. Known young ...

George Zhou et al, The Astronomical Journal 172 1

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Expected yield for late formation scenarios for...

Expected yield for late formation scenarios for systems <50 Myr old. Planet yields are s...

George Zhou et al, The Astronomical Journal 172 1

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The simulated mission can determine the planet ...

The simulated mission can determine the planet occurrence rate of the young planet popul...

George Zhou et al, The Astronomical Journal 172 1

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