Latest Images

Geometry of a hot spot on the surface of a neut...

Constraining the Neutron Star Mass–Radi...

Geometry of a hot spot on the surface of a neutron star rotating at an angular frequency...

The Astrophysical Journal Letters 887 1 L26

Comparison of flux measured at 1 keV for the S+...

Constraining the Neutron Star Mass–Radi...

Comparison of flux measured at 1 keV for the S+D and OS approximations and the exact num...

The Astrophysical Journal Letters 887 1 L26

Comparison of the calculated light ray deflecti...

Constraining the Neutron Star Mass–Radi...

Comparison of the calculated light ray deflection angle from Equation (16) (left panel) ...

The Astrophysical Journal Letters 887 1 L26

Comparison of the calculations of the travel ti...

Constraining the Neutron Star Mass–Radi...

Comparison of the calculations of the travel time delay integral from Equation (18) usin...

The Astrophysical Journal Letters 887 1 L26

Comparisons of the synthetic pulse waveforms fr...

Constraining the Neutron Star Mass–Radi...

Comparisons of the synthetic pulse waveforms from Tests SD1a and SD1b, the slowly spinni...

The Astrophysical Journal Letters 887 1 L26

Same as Figure 5 except for tests SD1c and SD1d...

Constraining the Neutron Star Mass–Radi...

Same as Figure 5 except for tests SD1c and SD1d, which consider more rapid rotation (ν =...

The Astrophysical Journal Letters 887 1 L26

Same as Figure 5 but for comparisons of the syn...

Constraining the Neutron Star Mass–Radi...

Same as Figure 5 but for comparisons of the synthetic pulse waveforms from Tests SD1e an...

The Astrophysical Journal Letters 887 1 L26

Left: results of the emission line tests SD2a–S...

Constraining the Neutron Star Mass–Radi...

Left: results of the emission line tests SD2a–SD2d (from top to bottom, respectively) fo...

The Astrophysical Journal Letters 887 1 L26

Comparisons of the synthetic pulse waveforms fr...

Constraining the Neutron Star Mass–Radi...

Comparisons of the synthetic pulse waveforms from Tests OS1a and OS1b. The point-like (θ...

The Astrophysical Journal Letters 887 1 L26

Same as Figure 9 but for tests OS1c and OS1d.

Constraining the Neutron Star Mass–Radi...

Same as Figure 9 but for tests OS1c and OS1d.

The Astrophysical Journal Letters 887 1 L26

Same as Figure 9 but for tests OS1e and OS1f.

Constraining the Neutron Star Mass–Radi...

Same as Figure 9 but for tests OS1e and OS1f.

The Astrophysical Journal Letters 887 1 L26

Same as Figure 9 but for tests OS1g and OS1h.

Constraining the Neutron Star Mass–Radi...

Same as Figure 9 but for tests OS1g and OS1h.

The Astrophysical Journal Letters 887 1 L26

Same as Figure 9 but for tests OS1i and OS1j.

Constraining the Neutron Star Mass–Radi...

Same as Figure 9 but for tests OS1i and OS1j.

The Astrophysical Journal Letters 887 1 L26

Left: results of the emission line tests OS1k a...

Constraining the Neutron Star Mass–Radi...

Left: results of the emission line tests OS1k and OS1l (from top to bottom, respectively...

The Astrophysical Journal Letters 887 1 L26

Average pulse profile of PSR J0030+0451’s emiss...

A NICER View of PSR J0030+0451: Evidenc...

Average pulse profile of PSR J0030+0451’s emission in three energy bands. Top and bottom...

The Astrophysical Journal Letters 887 1 L23

Cartoon showing both the magnetospheric geometr...

A NICER View of PSR J0030+0451: Evidenc...

Cartoon showing both the magnetospheric geometry inferred from the X-ray pulsations by R...

The Astrophysical Journal Letters 887 1 L23

1D and 2D marginal posterior density distributi...

A NICER View of PSR J0030+0451: Evidenc...

1D and 2D marginal posterior density distributions for the geometric parameters (spheric...

The Astrophysical Journal Letters 887 1 L23

Prior probability distributions for PSR J0030+0...

A Nicer View of PSR J0030+0451: Implica...

Prior probability distributions for PSR J0030+0451 transformed to the joint space of cen...

The Astrophysical Journal Letters 887 1 L22

Marginal posterior distributions of the pressur...

A Nicer View of PSR J0030+0451: Implica...

Marginal posterior distributions of the pressure P conditional on energy density ε, ...

The Astrophysical Journal Letters 887 1 L22

The 68% and 95% highest-density credible region...

A Nicer View of PSR J0030+0451: Implica...

The 68% and 95% highest-density credible regions of the PSR J0030+0451 likelihood functi...

The Astrophysical Journal Letters 887 1 L22

Similar to Figure 3 but for the hypothetical sc...

A Nicer View of PSR J0030+0451: Implica...

Similar to Figure 3 but for the hypothetical scenario where the observing time of PSR J0...

The Astrophysical Journal Letters 887 1 L22

Left panel: effect of spin on the mass vs. equa...

A Nicer View of PSR J0030+0451: Implica...

Left panel: effect of spin on the mass vs. equatorial radius curves for six representati...

The Astrophysical Journal Letters 887 1 L22

Effective area (red line) of the NICER XTI conc...

Constraining the Neutron Star Mass–Radi...

Effective area (red line) of the NICER XTI concentrator optics as a function of photon e...

The Astrophysical Journal Letters 887 1 L25

Folded profiles of PSR J0437–4715 (top left), P...

Constraining the Neutron Star Mass–Radi...

Folded profiles of PSR J0437–4715 (top left), PSR J0030+0451 (top right), PSR J1231−1411...

The Astrophysical Journal Letters 887 1 L25

Two-dimensional histograms of NICER XTI counts ...

Constraining the Neutron Star Mass–Radi...

Two-dimensional histograms of NICER XTI counts vs. pulse phase and photon energy for PSR...

The Astrophysical Journal Letters 887 1 L25

SEARCH TERM(S)

AUTHOR

PUBLICATIONS

  • 528161
  • 105441
  • 66624
  • 48731
  • 2224
  • 598
  • 563
  • 391
  • 197
  • 128
  • 111
  • 46
  • 23
  • 22

YEAR RANGE:

1982
2020

CONTENT TYPE

ADVANCED

ANNOUNCEMENTS

Take the AstroExplorer for a spin!

Be sure to try the search and sorting features, which were added based on user feedback; browse and find the links to videos and interactive figures in our Journal articles; find AAS Research Notes; or notice that new publishers have begun adding their figures to the AIE. Get in touch to hear more!