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Differential light curves for CD Cyg using a pe...

Photometric Measurements of Hα in the C...

Differential light curves for CD Cyg using a period of 17.073967 days. The different pan...

Research Notes of the AAS 3 4 63

Top-left panel: slit-reconstructed intensity ma...

Recovering Thermodynamics from Spectral...

Top-left panel: slit-reconstructed intensity map of NOAA AR 12480 observed by IRIS at Mg...

The Astrophysical Journal Letters 875 2 L18

Top panels: (first row) T for NOAA AR 12480 at ...

Recovering Thermodynamics from Spectral...

Top panels: (first row) T for NOAA AR 12480 at log(τ) = −4 provided by STiC (left), IRIS...

The Astrophysical Journal Letters 875 2 L18

Some thermodynamic quantities recovered by STiC...

Recovering Thermodynamics from Spectral...

Some thermodynamic quantities recovered by STiC (left), IRIS2 (center), and deepIRIS2 (r...

The Astrophysical Journal Letters 875 2 L18

For the full FoV (FFOV, blue line) and the RoIs...

Recovering Thermodynamics from Spectral...

For the full FoV (FFOV, blue line) and the RoIs framed in Figure 2. Top: T along the opt...

The Astrophysical Journal Letters 875 2 L18

Uncertainty multiplication factor (UMFp, see Eq...

Recovering Thermodynamics from Spectral...

Uncertainty multiplication factor (UMFp, see Equation (3)) for vlos (top), vturb (center...

The Astrophysical Journal Letters 875 2 L18

Flux upper limits of FRB 180814.J0422+73 in the...

Second Repeating FRB 180814.J0422+73: T...

Flux upper limits of FRB 180814.J0422+73 in the 100 MeV–10 GeV band. The time range is f...

The Astrophysical Journal Letters 875 2 L19

Constraints of the initial spin period and the ...

Second Repeating FRB 180814.J0422+73: T...

Constraints of the initial spin period and the surface magnetic field of a putative magn...

The Astrophysical Journal Letters 875 2 L19

Constraints on the isotropic kinetic energy of ...

Second Repeating FRB 180814.J0422+73: T...

Constraints on the isotropic kinetic energy of the blastwave and the luminosity distance...

The Astrophysical Journal Letters 875 2 L19

Stacked TESS images of the 11 × 11 pixel stamps...

TESS Full Orbital Phase Curve of the WA...

Stacked TESS images of the 11 × 11 pixel stamps centered around WASP-18 (red cross) for ...

The Astronomical Journal 157 5 178

Plot of the median-normalized and outlier-remov...

TESS Full Orbital Phase Curve of the WA...

Plot of the median-normalized and outlier-removed PDC sector 2 and 3 light curves of the...

The Astronomical Journal 157 5 178

Top panel: phase-folded light curve, after corr...

TESS Full Orbital Phase Curve of the WA...

Top panel: phase-folded light curve, after correcting for long-term trends, binned in 5 ...

The Astronomical Journal 157 5 178

Lomb–Scargle (top) and double-harmonic (bottom)...

TESS Full Orbital Phase Curve of the WA...

Lomb–Scargle (top) and double-harmonic (bottom) periodograms of the light curves, where ...

The Astronomical Journal 157 5 178

Long-term (left panel) and short-term (right pa...

TESS Full Orbital Phase Curve of the WA...

Long-term (left panel) and short-term (right panel) TTV search. Both panels show the res...

The Astronomical Journal 157 5 178

Period ratios of adjacent transiting planets wh...

Ultra-short-period Planets from Secular...

Period ratios of adjacent transiting planets where the inner planet has a period less th...

The Astronomical Journal 157 5 180

Expected multiplicity ratio (...

Ultra-short-period Planets from Secular...

Expected multiplicity ratio (﹩\left\langle {f}_{\gt 1}/{f}_{1}\right\rangle ﹩ in Equatio...

The Astronomical Journal 157 5 180

Expected multiplicity ratio ...

Ultra-short-period Planets from Secular...

Expected multiplicity ratio ...

The Astronomical Journal 157 5 180

Contours of the minimum eccentricity and inclin...

Ultra-short-period Planets from Secular...

Contours of the minimum eccentricity and inclination dispersions expressed as ...

The Astronomical Journal 157 5 180

Example of a possible evolution to produce a sy...

Ultra-short-period Planets from Secular...

Example of a possible evolution to produce a system like Kepler-10. The upper panel (a) ...

The Astronomical Journal 157 5 180

Maximum eccentricities reached by a Kepler-10b-...

Ultra-short-period Planets from Secular...

Maximum eccentricities reached by a Kepler-10b-like planet after 106 yr, for different i...

The Astronomical Journal 157 5 180

Fraction of USP planets formed (i.e., reaching ...

Ultra-short-period Planets from Secular...

Fraction of USP planets formed (i.e., reaching ﹩{a}_{1}(1-{e}_{1}^{2})\lt 0.02﹩ au) as a...

The Astronomical Journal 157 5 180

Inclination distributions for Kepler-10b from o...

Ultra-short-period Planets from Secular...

Inclination distributions for Kepler-10b from our fiducial simulation (initial e, i from...

The Astronomical Journal 157 5 180

Eccentricity distributions for the Kepler-10b p...

Ultra-short-period Planets from Secular...

Eccentricity distributions for the Kepler-10b planets that do not reach the threshold ...

The Astronomical Journal 157 5 180

Initial period from which the USP planets start...

Ultra-short-period Planets from Secular...

Initial period from which the USP planets started tidal migration if only asynchronous e...

The Astronomical Journal 157 5 180

Altitude ranges for which the S/N is at detecta...

Modeling the Altitude Distribution of M...

Altitude ranges for which the S/N is at detectable levels for the Arecibo (panel a), PFI...

The Astronomical Journal 157 5 179

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