J-type Carbon Stars: A Dominant Source ...

Isotopic compositions of C, N, and Si of AB2 and MS SiC grains from this study are compa...

J-type Carbon Stars: A Dominant Source ...

A Mo three-isotope plot of δ94Mo vs. δ92Mo for SiC AB2 and MS grains from this study and...

J-type Carbon Stars: A Dominant Source ...

The Mo isotope pattern of the most anomalous AB2 grain M2-A1-G554, in comparison to the ...

J-type Carbon Stars: A Dominant Source ...

Plot of δ135Ba vs. δ92Mo for MS SiC grains from this study and the same set of Torino AG...

Wayne—A Simulator for HST  WFC3 IR Gris...

Simplified overview of the steps performed by Wayne to generate a visit. Steps are shown...

Wayne—A Simulator for HST  WFC3 IR Gris...

The light-curve model of HD 209458b generated by PyLightcurve using the parameters descr...

Wayne—A Simulator for HST  WFC3 IR Gris...

WFC3 G102 and G141 grism sensitivity as calculated by Kuntschner et al. (2011). This ste...

Wayne—A Simulator for HST  WFC3 IR Gris...

Quantum efficiency of the WFC3 IR detector. The black lines indicate the edges of the wa...

Wayne—A Simulator for HST  WFC3 IR Gris...

Trace positions of the G102 and G141 grisms given by the field-dependent wavelength solu...

Wayne—A Simulator for HST  WFC3 IR Gris...

The PSF parameters with wavelength for the WFC3 IR channel.

Wayne—A Simulator for HST  WFC3 IR Gris...

Cropped exposure of a simulation of a staring mode frame for HD 209458b using Wayne with...

Wayne—A Simulator for HST  WFC3 IR Gris...

Flat-field cube from Kuntschner et al. (2011) for the G141 grism and 256 subarray.

Wayne—A Simulator for HST  WFC3 IR Gris...

Master sky image from Kümmel et al. (2011) for the G141 grism and 256 subarray.

Wayne—A Simulator for HST  WFC3 IR Gris...

WFC3 IR superdark u4819493i_drk.fits for a 256 subarray at NSAMP 5 in SPARS10 mode cover...

Wayne—A Simulator for HST  WFC3 IR Gris...

The initial bias frame for the 256 subarray mode used for the zero-read. The frame is in...

Wayne—A Simulator for HST  WFC3 IR Gris...

Measuring scan speed variations from orbit 3 of HD 209458b. The upper plot shows the fir...

Wayne—A Simulator for HST  WFC3 IR Gris...

Comparison of a real raw frame (ibh726meq_raw.fits) of HD 209458 from proposal 12181 (up...

Wayne—A Simulator for HST  WFC3 IR Gris...

Retrieved position shifts (dots) compared to the input values (crosses) and residuals fo...

Wayne—A Simulator for HST  WFC3 IR Gris...

Top: the wavelength-dependent photon positions (colored points) as the star moves along ...

Wayne—A Simulator for HST  WFC3 IR Gris...

1D spectra extracted from a real and a simulated spatially scanned frame, compared with ...

Wayne—A Simulator for HST  WFC3 IR Gris...

Top: white light curve, as extracted from the real and the simulated data sets. Bottom: ...

Wayne—A Simulator for HST  WFC3 IR Gris...

High-resolution input spectrum of HD 209458b and the extracted data from the simulation....

The Densities of Planets in Multiple St...

Fractional change of planet density vs. fractional change of planet radius. The subscrip...

The Densities of Planets in Multiple St...

Radius vs. mass for confirmed Kepler planets whose host stars have stellar companions wi...

The Densities of Planets in Multiple St...

Similar to Figure 2; the black circles are measurements (for clarity, uncertainties are ...