Astronomy Image Explorer

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First row, right panel: unsharp-masked WFPC2/F5...

First row, right panel: unsharp-masked WFPC2/F555W image of the double nucleus in NGC 44...

Behzad Tahmasebzadeh et al, The Astrophysical Journal Letters 1001 1

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Trajectories of the BH that is kicked from the ...

Trajectories of the BH that is kicked from the center of NGC 4486B. The different-colore...

Behzad Tahmasebzadeh et al, The Astrophysical Journal Letters 1001 1

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Expected GW recoil kick magnitude, Vkick, as a ...

Expected GW recoil kick magnitude, Vkick, as a function of the premerger BH mass ratio, ...

Behzad Tahmasebzadeh et al, The Astrophysical Journal Letters 1001 1

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Top: radial profile of the retrograde orbit fra...

Top: radial profile of the retrograde orbit fraction from the best-fit Schwarzschild mod...

Behzad Tahmasebzadeh et al, The Astrophysical Journal Letters 1001 1

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The top panel presents the projected luminosity...

The top panel presents the projected luminosity density of NGC 4486B (black dots) derive...

Behzad Tahmasebzadeh et al, The Astrophysical Journal Letters 1001 1

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Trajectory of the BH that is placed at the cent...

Trajectory of the BH that is placed at the center of NGC 4486B without any recoil kick. ...

Behzad Tahmasebzadeh et al, The Astrophysical Journal Letters 1001 1

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Time evolution of the galaxy and the SMBH binar...

Time evolution of the galaxy and the SMBH binary parameters. Top left: volume–density pr...

Behzad Tahmasebzadeh et al, The Astrophysical Journal Letters 1001 1

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Best-fit Schwarzschild models with (top) and wi...

Best-fit Schwarzschild models with (top) and without (bottom) retrograde orbits, each an...

Behzad Tahmasebzadeh et al, The Astrophysical Journal Letters 1001 1

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Examples of a metric type II radio burst event ...

Examples of a metric type II radio burst event on 2015 November 4. The spectrum was chos...

X.-N. Wang et al, The Astrophysical Journal 1001 1

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The CME and its driven shock from the SOHO LASC...

The CME and its driven shock from the SOHO LASCO/C2 instruments on 2000 December 18. The...

X.-N. Wang et al, The Astrophysical Journal 1001 1

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Evolving log ΣSFR–log ...

Evolving log ΣSFR–log ﹩{{\rm{\Sigma }}}_{{M}_{\ast }}﹩correlations for UVCANDELS IDs 053...

Charlotte Olsen et al, The Astrophysical Journal 1001 1

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Similar to Figure 17, we show the evolution of ...

Similar to Figure 17, we show the evolution of regions within UVCANDELS IDs 08218, 22456...

Charlotte Olsen et al, The Astrophysical Journal 1001 1

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Within the UVCANDELS 23475 postage stamps, the ...

Within the UVCANDELS 23475 postage stamps, the galaxy’s spiral arms are clearest in F435...

Charlotte Olsen et al, The Astrophysical Journal 1001 1

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UVCANDELS 22456 is an inclined spiral galaxy. S...

UVCANDELS 22456 is an inclined spiral galaxy. Strong clumps trace the spiral arms in F43...

Charlotte Olsen et al, The Astrophysical Journal 1001 1

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The projected radial profile of UVCANDELS ID 10...

The projected radial profile of UVCANDELS ID 10335 shows similar shapes for all properti...

Charlotte Olsen et al, The Astrophysical Journal 1001 1

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The “center” of UVCANDELS ID 05386 is defined a...

The “center” of UVCANDELS ID 05386 is defined as the brightest point in the object on th...

Charlotte Olsen et al, The Astrophysical Journal 1001 1

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Both log ΣSFR and log sSFR show a crossing beha...

Both log ΣSFR and log sSFR show a crossing behavior where the values at the time of obse...

Charlotte Olsen et al, The Astrophysical Journal 1001 1

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Radial profiles for 08062 in log ΣSFR, log sSFR...

Radial profiles for 08062 in log ΣSFR, log sSFR, AV, and tx mass formation times show si...

Charlotte Olsen et al, The Astrophysical Journal 1001 1

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The log ΣSFR radial profile for UVCANDELS ID 08...

The log ΣSFR radial profile for UVCANDELS ID 08218 shows little evolution over the last ...

Charlotte Olsen et al, The Astrophysical Journal 1001 1

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Shown are postage stamps and property maps of 1...

Shown are postage stamps and property maps of 10335 in pixel coordinates. Top: HST F275W...

Charlotte Olsen et al, The Astrophysical Journal 1001 1

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Evolution of the log ΣSFR–log ...

Evolution of the log ΣSFR–log ﹩{{\rm{\Sigma }}}_{{M}_{\ast }}﹩correlation over the past ...

Charlotte Olsen et al, The Astrophysical Journal 1001 1

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The two panels show how the slope, normalizatio...

The two panels show how the slope, normalization, and redshift vary between each galaxy’...

Charlotte Olsen et al, The Astrophysical Journal 1001 1

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log ΣSFR–log ﹩{{\rm{\Sigma }}}_{{M}_{\ast }}﹩co...

log ΣSFR–log ﹩{{\rm{\Sigma }}}_{{M}_{\ast }}﹩correlation fit lines for all galaxies are ...

Charlotte Olsen et al, The Astrophysical Journal 1001 1

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The two panels show how the slope, normalizatio...

The two panels show how the slope, normalization, and scatter of each galaxy’s regional ...

Charlotte Olsen et al, The Astrophysical Journal 1001 1

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UVCANDELS 05386 is cataloged as a pair, with th...

UVCANDELS 05386 is cataloged as a pair, with the dimmer object to the right likely a com...

Charlotte Olsen et al, The Astrophysical Journal 1001 1

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