Latest Images

Left: bulk RV correlation slope (y-axis) vs. li...

Left: bulk RV correlation slope (y-axis) vs. line depth (x-axis) for different line sele...

Abigail Burrows et al, The Astronomical Journal 167 5

Left: LBL bulk velocities with corresponding FF...

Left: LBL bulk velocities with corresponding FF’-based velocities derived using the dept...

Abigail Burrows et al, The Astronomical Journal 167 5

Top: HD 26965 bulk RVs calculated through our L...

Top: HD 26965 bulk RVs calculated through our LBL pipeline (gray) with linear trend remo...

Abigail Burrows et al, The Astronomical Journal 167 5

Left: LBL bulk RV time series when detrended (p...

Left: LBL bulk RV time series when detrended (purple circles) for each metric based on c...

Abigail Burrows et al, The Astronomical Journal 167 5

Example GP-modeled phase lag between S ...

Example GP-modeled phase lag between S HK activity indicator and...

Abigail Burrows et al, The Astronomical Journal 167 5

Posteriors from MCMC best-fit Keplerian periods...

Posteriors from MCMC best-fit Keplerian periods, per, and semiamplitudes, K, for the sym...

Abigail Burrows et al, The Astronomical Journal 167 5

Correlations between bulk RV and each activity ...

Correlations between bulk RV and each activity metric (described in Section 5.1.1). The ...

Abigail Burrows et al, The Astronomical Journal 167 5

Critical points for computing diagnostic symmet...

Critical points for computing diagnostic symmetry metrics are plotted across the spectru...

Abigail Burrows et al, The Astronomical Journal 167 5

NEID bulk RVs of HD 26965 (purple) overlaid on ...

NEID bulk RVs of HD 26965 (purple) overlaid on the best-fit Keplerian solution from Ma e...

Abigail Burrows et al, The Astronomical Journal 167 5

Demonstration of our LBL pipeline on NEID solar...

Demonstration of our LBL pipeline on NEID solar spectra, compared to the standard NEID D...

Abigail Burrows et al, The Astronomical Journal 167 5

Left: NEID data of HD 26965, showing velocities...

Left: NEID data of HD 26965, showing velocities and activity indicator time series for s...

Abigail Burrows et al, The Astronomical Journal 167 5

Phase-folded velocity plots of the best-fit Kep...

Phase-folded velocity plots of the best-fit Keplerians corresponding to the MCMC fits of...

Abigail Burrows et al, The Astronomical Journal 167 5

Overview of FF’ injection recovery experiment, ...

Overview of FF’ injection recovery experiment, applied to the measured bulk RVs of HD 26...

Abigail Burrows et al, The Astronomical Journal 167 5

Line fit carried out to the Paβ line. The top t...

Line fit carried out to the Paβ line. The top two panels show the results after consider...

Alberto Rodríguez-Ardila et al, The Astronomical Journal 167 5

Deblending procedure applied to the Fe II ...

Deblending procedure applied to the Fe II λ10501 line. The left pan...

Alberto Rodríguez-Ardila et al, The Astronomical Journal 167 5

Deblending procedure applied to O I ...

Deblending procedure applied to O I λ11287. The left panel shows th...

Alberto Rodríguez-Ardila et al, The Astronomical Journal 167 5

Top panel: fit applied to the NIR continuum emi...

Top panel: fit applied to the NIR continuum emission (black line) in 1H 0707−495 with a ...

Alberto Rodríguez-Ardila et al, The Astronomical Journal 167 5

Deblending procedure applied to the Fe II ...

Deblending procedure applied to the Fe II λ9997+Paδ blend. The left...

Alberto Rodríguez-Ardila et al, The Astronomical Journal 167 5

NIR spectrum of 1H 0707−495 in rest wavelength ...

NIR spectrum of 1H 0707−495 in rest wavelength already corrected for a Galactic extincti...

Alberto Rodríguez-Ardila et al, The Astronomical Journal 167 5

Line fitting procedure applied to the [S III] λ...

Line fitting procedure applied to the [S III] λ9531 + Pa 8 blend. The left panel shows t...

Alberto Rodríguez-Ardila et al, The Astronomical Journal 167 5

Line fit carried out on the Fe II ...

Line fit carried out on the Fe II λ10501 lines. The left panel show...

Alberto Rodríguez-Ardila et al, The Astronomical Journal 167 5

Line fit carried out on O I ...

Line fit carried out on O I λ11287. The left panel shows the result...

Alberto Rodríguez-Ardila et al, The Astronomical Journal 167 5

Deblending procedure applied to the Fe II ...

Deblending procedure applied to the Fe II λ9997+Paδ blend without a...

Alberto Rodríguez-Ardila et al, The Astronomical Journal 167 5

Similar to Figure A3, but for the [S III] λ9531...

Similar to Figure A3, but for the [S III] λ9531+Pa 8 blend.

Alberto Rodríguez-Ardila et al, The Astronomical Journal 167 5

The distributions of P (left panel) and θ (righ...

The distributions of P (left panel) and θ (right panel) in the B, V, R, and I bands. Dis...

Sadhana Singh et al, The Astronomical Journal 167 5

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