Astronomy Image Explorer

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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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Measured η over time for Ceres and Vesta observ...

Measured η over time for Ceres and Vesta observed with SOFIA FORCAST and analyzed in the...

Anicia Arredondo et al, The Planetary Science Journal 7 9

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Slope of the G227 filter compared to (A) orbita...

Slope of the G227 filter compared to (A) orbital position, (B) subobserver longitude, (C...

Anicia Arredondo et al, The Planetary Science Journal 7 9

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(Top) The original data (gray) were scaled to t...

(Top) The original data (gray) were scaled to the NEATM model (black) calculated with a ...

Anicia Arredondo et al, The Planetary Science Journal 7 9

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Comparison of slopes between 22 and 28 μm found...

Comparison of slopes between 22 and 28 μm found while letting η vary as in Section 5.2 a...

Anicia Arredondo et al, The Planetary Science Journal 7 9

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The complete figure set (17 images) is availabl...

The complete figure set (17 images) is available in the online journal. Left: NEATM fit ...

Anicia Arredondo et al, The Planetary Science Journal 7 9

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Comparison between original emissivity (gray li...

Comparison between original emissivity (gray lines, same as Figure 3) and emissivity fou...

Anicia Arredondo et al, The Planetary Science Journal 7 9

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Spitzer Data Fusion Sky Coverage in Galactic (T...

Spitzer Data Fusion Sky Coverage in Galactic (Top Panel) and Equatorial (Bottom Panel) C...

Mattia Vaccari, Research Notes of the AAS 10 9

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Marginalized 1D and 2D constraints on the param...

Marginalized 1D and 2D constraints on the parameters A, ns, ABAO, kBAO, α, γ, and β from...

Pierros Ntelis et al, The Astrophysical Journal 1009 2

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Comparison of theoretical predictions and simul...

Comparison of theoretical predictions and simulated data. Left: monopole ξ0(s) (solid) a...

Pierros Ntelis et al, The Astrophysical Journal 1009 2

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Schematic illustration of the dipole contributi...

Schematic illustration of the dipole contributions. LPI (green): oscillatory shape with ...

Pierros Ntelis et al, The Astrophysical Journal 1009 2

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Sketch of different redshift contributions: cos...

Sketch of different redshift contributions: cosmological (zcosmo), LPI violation (zgrav(...

Pierros Ntelis et al, The Astrophysical Journal 1009 2

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Dipole of the two-point correlation function ξ1...

Dipole of the two-point correlation function ξ1(s) for different violation scenarios. Le...

Pierros Ntelis et al, The Astrophysical Journal 1009 2

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Best-fit model (magenta) to the GHOST spectrum ...

Best-fit model (magenta) to the GHOST spectrum of AF Lep A (cyan), shown for (Left) the ...

Aneesh Baburaj et al, The Astronomical Journal 172 4

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Posteriors for MARCS–C/S grid fit to spectral o...

Posteriors for MARCS–C/S grid fit to spectral order #51 with the S I feature at 6757 Å. ...

Aneesh Baburaj et al, The Astronomical Journal 172 4

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Best-fit MARCS-C/O model (magenta) to the GHOST...

Best-fit MARCS-C/O model (magenta) to the GHOST spectrum of ϵ Indi A (cyan), shown for C...

Aneesh Baburaj et al, The Astronomical Journal 172 4

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Posteriors for MARCS–C/O grid fit to spectral o...

Posteriors for MARCS–C/O grid fit to spectral order with C I lines between 7110 and 7119...

Aneesh Baburaj et al, The Astronomical Journal 172 4

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The luminosity deficit in core galaxies may be ...

The luminosity deficit in core galaxies may be estimated by taking the integrated differ...

C. J. Harris et al, The Astrophysical Journal 1009 2

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The plot shows hardening time in years on the y...

The plot shows hardening time in years on the y-axis and binary separation in parsecs on...

C. J. Harris et al, The Astrophysical Journal 1009 2

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Plotted are the distributions of stellar mass d...

Plotted are the distributions of stellar mass deficit as a fraction of total galaxy stel...

C. J. Harris et al, The Astrophysical Journal 1009 2

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Coalescence time plotted against the average bi...

Coalescence time plotted against the average binary hardening parameter, s = d(1/a)/dt. ...

C. J. Harris et al, The Astrophysical Journal 1009 2

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Here we plot the posterior distribution of coal...

Here we plot the posterior distribution of coalescence times for the SBHBs in our best-f...

C. J. Harris et al, The Astrophysical Journal 1009 2

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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!