Astronomy Image Explorer

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Distribution of the 5σ limiting magnitude (dept...

Distribution of the 5σ limiting magnitude (depth) measured within a 0...

Kimi C. Kreilgaard et al, The Astrophysical Journal 1009 2

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Histogram showing the absolute UV magnitudes fo...

Histogram showing the absolute UV magnitudes for galaxy candidates in each of the three ...

Kimi C. Kreilgaard et al, The Astrophysical Journal 1009 2

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Sky distribution of the 36 fields included in B...

Sky distribution of the 36 fields included in BEACON DR2 (orange circles), overlaid on a...

Kimi C. Kreilgaard et al, The Astrophysical Journal 1009 2

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Binned UV LFs inferred from our F090W- (left pa...

Binned UV LFs inferred from our F090W- (left panel), F115W- (middle panel), and F150W-dr...

Kimi C. Kreilgaard et al, The Astrophysical Journal 1009 2

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The cosmic UV luminosity density, ρUV, resultin...

The cosmic UV luminosity density, ρUV, resulting from integrating our best-fit Schechter...

Kimi C. Kreilgaard et al, The Astrophysical Journal 1009 2

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A comparison of the number densities measured f...

A comparison of the number densities measured from BEACON DR2 (orange scatter points) fo...

Kimi C. Kreilgaard et al, The Astrophysical Journal 1009 2

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Distributions of the probability of observing N...

Distributions of the probability of observing Nobs sources or more in a field where ...

Kimi C. Kreilgaard et al, The Astrophysical Journal 1009 2

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Relative overdensity probability, P(overdense ∣...

Relative overdensity probability, P(overdense ∣ M > Mh)/P(overdense), as a function of h...

Kimi C. Kreilgaard et al, The Astrophysical Journal 1009 2

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Examples of our observed photometry and SED fit...

Examples of our observed photometry and SED fitting results for two F090W dropouts (purp...

Kimi C. Kreilgaard et al, The Astrophysical Journal 1009 2

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Comparison between the photometric redshifts, a...

Comparison between the photometric redshifts, as estimated from the EAZY SED fit, and th...

Kimi C. Kreilgaard et al, The Astrophysical Journal 1009 2

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Example of the completeness matrix for each of ...

Example of the completeness matrix for each of the three dropout selections, as a functi...

Kimi C. Kreilgaard et al, The Astrophysical Journal 1009 2

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Nuclear composition of the accreted material at...

Nuclear composition of the accreted material at the neutron star surface (blue line) and...

I. Sultana et al, The Astrophysical Journal 1009 2

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Model light curves for the baseline calculation...

Model light curves for the baseline calculation using the REACLIB v2.2 reaction rates (b...

I. Sultana et al, The Astrophysical Journal 1009 2

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Baseline XRB light curves for 32 systems. Panel...

Baseline XRB light curves for 32 systems. Panels are arranged so that XH,ign decreases f...

I. Sultana et al, The Astrophysical Journal 1009 2

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(a) Hydrogen mass fraction at ignition (XH,ign)...

(a) Hydrogen mass fraction at ignition (XH,ign) as a function of accreted hydrogen fract...

I. Sultana et al, The Astrophysical Journal 1009 2

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Baseline isotopic abundance distributions for t...

Baseline isotopic abundance distributions for the same 32 systems, using the identical p...

I. Sultana et al, The Astrophysical Journal 1009 2

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Visualization of the impact of individual nucle...

Visualization of the impact of individual nuclear reaction rates across all 32 systems i...

I. Sultana et al, The Astrophysical Journal 1009 2

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Mass number change as a function of target mass...

Mass number change as a function of target mass of the reaction nuclei. The color bar re...

I. Sultana et al, The Astrophysical Journal 1009 2

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Same as Figure 9. The top panels show system H3...

Same as Figure 9. The top panels show system H30Z2M90, and the bottom panels show system...

I. Sultana et al, The Astrophysical Journal 1009 2

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Same as Figure 6. The impactful reaction rate v...

Same as Figure 6. The impactful reaction rate variation changes the final abundances pro...

I. Sultana et al, The Astrophysical Journal 1009 2

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Temperature and density profiles of the accrete...

Temperature and density profiles of the accreted envelope as functions of column depth. ...

I. Sultana et al, The Astrophysical Journal 1009 2

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(Left) NEATM fit (maroon) to the photometric po...

(Left) NEATM fit (maroon) to the photometric points (blue) for flight F435. The red poin...

Anicia Arredondo et al, The Planetary Science Journal 7 9

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The gray line indicates Ceres’s orbital path ar...

The gray line indicates Ceres’s orbital path around the Sun (yellow star). The location ...

Anicia Arredondo et al, The Planetary Science Journal 7 9

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Emissivity spectra for G227 and G329 found by d...

Emissivity spectra for G227 and G329 found by dividing the observed flux by the NEATM mo...

Anicia Arredondo et al, The Planetary Science Journal 7 9

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Changes in η with (A) orbital position, (B) sub...

Changes in η with (A) orbital position, (B) subobserver longitude, (C) date, and (D) pha...

Anicia Arredondo et al, The Planetary Science Journal 7 9

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ANNOUNCEMENTS

Updated Search and Sort

We have updated the search and sort algorithm to return records in reverse chronological order based on the date/time that the images were uploaded to the Astronomy Image Explorer. This is potentially but rarely different from the publication date. Thank you!