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TSEBL profiles of the EBL detection as a functi...

TSEBL profiles of the EBL detection as a function of the renormalizing parameter b, for ...

Anuvab Banerjee et al, The Astrophysical Journal 1003 1

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Measurement of the CGRH derived from the EBL op...

Measurement of the CGRH derived from the EBL optical-depth measurements (blue data point...

Anuvab Banerjee et al, The Astrophysical Journal 1003 1

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Illustration of the computation of the optical ...

Illustration of the computation of the optical depth for the 0.70 ≤ z < 0.79 bin and pho...

Anuvab Banerjee et al, The Astrophysical Journal 1003 1

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Measurements of the EBL optical depth, τγγ, as ...

Measurements of the EBL optical depth, τγγ, as a function of energy and redshift. The so...

Anuvab Banerjee et al, The Astrophysical Journal 1003 1

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Redshift distribution of the sources used in th...

Redshift distribution of the sources used in this analysis on a logarithmic scale.

Anuvab Banerjee et al, The Astrophysical Journal 1003 1

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﹩{E}_{{\rm{\max }}}﹩ versus redshift for the b...

﹩{E}_{{\rm{\max }}}﹩ versus redshift for the blazar sample. ﹩{E}_{{\rm{\max }}}﹩ corres...

Anuvab Banerjee et al, The Astrophysical Journal 1003 1

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Light curve of 4FGL J1504.4+1029 produced using...

Light curve of 4FGL J1504.4+1029 produced using a two-week bin. The red line shows the BBs.

Anuvab Banerjee et al, The Astrophysical Journal 1003 1

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The 68% contour EBL intensity results as a func...

The 68% contour EBL intensity results as a function of wavelength at z = 0 for our empir...

Anuvab Banerjee et al, The Astrophysical Journal 1003 1

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The 68% contour luminosity density results as a...

The 68% contour luminosity density results as a function of redshift for three wavelengt...

Anuvab Banerjee et al, The Astrophysical Journal 1003 1

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The 68% contour EBL intensity results as a func...

The 68% contour EBL intensity results as a function of wavelength at z = 0 for our physi...

Anuvab Banerjee et al, The Astrophysical Journal 1003 1

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The orange region shows the 68% contour luminos...

The orange region shows the 68% contour luminosity density results as a function of reds...

Anuvab Banerjee et al, The Astrophysical Journal 1003 1

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The orange region shows the 68% contour luminos...

The orange region shows the 68% contour luminosity density results as a function of wave...

Anuvab Banerjee et al, The Astrophysical Journal 1003 1

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The 68% contour star formation rate density as ...

The 68% contour star formation rate density as a function of density for the physical mo...

Anuvab Banerjee et al, The Astrophysical Journal 1003 1

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Water mixing ratios versus altitude for each of...

Water mixing ratios versus altitude for each of our three profile assumptions (left) and...

S. Rugheimer et al, The Astrophysical Journal 1003 1

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Planet distance (astronomical units) versus wat...

Planet distance (astronomical units) versus water surface mixing ratio (bar) needed to m...

S. Rugheimer et al, The Astrophysical Journal 1003 1

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Mid-IR input spectra at R=100 calculated by pet...

Mid-IR input spectra at R=100 calculated by petitRADTRANS as input to LIFESIM for differ...

S. Rugheimer et al, The Astrophysical Journal 1003 1

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Water posteriors for simulations for a range of...

Water posteriors for simulations for a range of surface H2O abundances from 1 bar to 10−...

S. Rugheimer et al, The Astrophysical Journal 1003 1

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Corner plot for the posterior distributions fro...

Corner plot for the posterior distributions from the retrievals of a 1 bar surface H2O v...

S. Rugheimer et al, The Astrophysical Journal 1003 1

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The same as Figure 5, except showing results fo...

The same as Figure 5, except showing results for the 1 bar surface H2O Earth-like water ...

S. Rugheimer et al, The Astrophysical Journal 1003 1

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The same as Figure 5, except showing results fo...

The same as Figure 5, except showing results for the 10−2 bar surface H2O Earth-like wat...

S. Rugheimer et al, The Astrophysical Journal 1003 1

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The same as Figure 5, except showing results fo...

The same as Figure 5, except showing results for the 10−6 bar surface H2O with diffusion...

S. Rugheimer et al, The Astrophysical Journal 1003 1

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Joint posterior constraints in mc–ac space. The...

Joint posterior constraints in mc–ac space. The dark and light regions indicate, respect...

Haedam Im et al, The Astrophysical Journal 1003 1

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RV measurements and our best-fitting model of t...

RV measurements and our best-fitting model of the GJ 436 system. Panel (a) shows the RV ...

Haedam Im et al, The Astrophysical Journal 1003 1

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Analytic constraints in mc–ac space for three i...

Analytic constraints in mc–ac space for three initial semimajor axes ab = 0.3, 1, and 5 ...

Haedam Im et al, The Astrophysical Journal 1003 1

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Example dynamical history of GJ 436 b via ZLK m...

Example dynamical history of GJ 436 b via ZLK migration with an outer companion of mass ...

Haedam Im et al, The Astrophysical Journal 1003 1

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