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Top panel: Γ is the astrophysical/source-frame ...

Top panel: Γ is the astrophysical/source-frame merger-rate density per unit primary mass...

Elizabeth Flanagan et al, The Astrophysical Journal Letters 1011 2

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Inferred effective-spin distributions across th...

Inferred effective-spin distributions across the four mass intervals identified from the...

Elizabeth Flanagan et al, The Astrophysical Journal Letters 1011 2

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Summary statistics of the inferred effective-sp...

Summary statistics of the inferred effective-spin distributions across the four mass int...

Elizabeth Flanagan et al, The Astrophysical Journal Letters 1011 2

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The merger rate as a function of mass ratio q f...

The merger rate as a function of mass ratio q for each mass interval. The shaded region ...

Elizabeth Flanagan et al, The Astrophysical Journal Letters 1011 2

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Posterior support for the minimum and maximum e...

Posterior support for the minimum and maximum extent of the inferred effective-spin dist...

Elizabeth Flanagan et al, The Astrophysical Journal Letters 1011 2

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Comparison between the inferred effective-spin ...

Comparison between the inferred effective-spin support of the high-mass BBH population a...

Elizabeth Flanagan et al, The Astrophysical Journal Letters 1011 2

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The mass transitions of each region have been s...

The mass transitions of each region have been shifted from the original choices. We see ...

Elizabeth Flanagan et al, The Astrophysical Journal Letters 1011 2

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Inferred effective-spin distributions for diffe...

Inferred effective-spin distributions for different choices of the transition mass scale...

Elizabeth Flanagan et al, The Astrophysical Journal Letters 1011 2

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The evolution of the inferred effective-spin di...

The evolution of the inferred effective-spin distributions as a function of the transiti...

Elizabeth Flanagan et al, The Astrophysical Journal Letters 1011 2

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Posterior distributions of hyperparameters for ...

Posterior distributions of hyperparameters for the mass-interval population models of Se...

Elizabeth Flanagan et al, The Astrophysical Journal Letters 1011 2

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Illustrative time snapshots (columns) of four s...

Illustrative time snapshots (columns) of four separate SPH simulations with different at...

Matthew J. Roche et al, The Astrophysical Journal Letters 1011 2

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The cumulative effect of many giant impacts dur...

The cumulative effect of many giant impacts during planet formation can lead to large va...

Matthew J. Roche et al, The Astrophysical Journal Letters 1011 2

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Earth could have lost significant portions of i...

Earth could have lost significant portions of its atmosphere during the Moon-forming gia...

Matthew J. Roche et al, The Astrophysical Journal Letters 1011 2

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Atmospheric loss increases with decreasing atmo...

Atmospheric loss increases with decreasing atmosphere mass fraction, but follows previou...

Matthew J. Roche et al, The Astrophysical Journal Letters 1011 2

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Our new scaling law captures the effects of atm...

Our new scaling law captures the effects of atmospheric mass on loss and can predict the...

Matthew J. Roche et al, The Astrophysical Journal Letters 1011 2

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The same as Figure 2 but showing atmospheric lo...

The same as Figure 2 but showing atmospheric loss from the far field only. The gray soli...

Matthew J. Roche et al, The Astrophysical Journal Letters 1011 2

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The same as Figure 2 but showing atmospheric lo...

The same as Figure 2 but showing atmospheric loss from the near field only. The gray sol...

Matthew J. Roche et al, The Astrophysical Journal Letters 1011 2

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PCH-L fast wind stream measured at 3 points in ...

PCH-L fast wind stream measured at 3 points in the inner heliosphere. (A) An EUV 211 Å i...

Samuel T. Badman et al, The Astrophysical Journal Letters 1011 2

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In situ measurements of the bulk stream propert...

In situ measurements of the bulk stream properties as a function of heliographic longitu...

Samuel T. Badman et al, The Astrophysical Journal Letters 1011 2

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Properties of the peak of the stream as a funct...

Properties of the peak of the stream as a function of heliocentric distance in historica...

Samuel T. Badman et al, The Astrophysical Journal Letters 1011 2

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Evolution of velocity fluctuations in the fast ...

Evolution of velocity fluctuations in the fast wind stream. Measured vector components o...

Samuel T. Badman et al, The Astrophysical Journal Letters 1011 2

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Discovery and confirmation plots of three new p...

Discovery and confirmation plots of three new pulsars in the Large Magellanic Cloud. Top...

Rahul Sengar et al, The Astrophysical Journal Letters 1011 2

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Discovery and confirmation plots of PSR J0443−6...

Discovery and confirmation plots of PSR J0443−68. Top row: a discovery observation showi...

Rahul Sengar et al, The Astrophysical Journal Letters 1011 2

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Cumulative distributions of radio luminosity fo...

Cumulative distributions of radio luminosity for Galactic pulsars (gray circles) and MC ...

Rahul Sengar et al, The Astrophysical Journal Letters 1011 2

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Discovery and confirmation plots of PSR J0506−6...

Discovery and confirmation plots of PSR J0506−66. Top row: a discovery observation showi...

Rahul Sengar et al, The Astrophysical Journal Letters 1011 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!