Astronomy Image Explorer

Latest Images

GW signals (solid lines) versus experimental se...

GW signals (solid lines) versus experimental sensitivity curves as a function of f (dash...

Mian Zhu and Yi-Fu Cai, The Astrophysical Journal Letters 1004 2

Image Details View Article

Left panel: the effective potential ...

Left panel: the effective potential ﹩{M}_{p}^{2}V(\tau )﹩ in inflationary (blue line) an...

Mian Zhu and Yi-Fu Cai, The Astrophysical Journal Letters 1004 2

Image Details View Article

Illustration of the bouncing scenarios.

Illustration of the bouncing scenarios.

Mian Zhu and Yi-Fu Cai, The Astrophysical Journal Letters 1004 2

Image Details View Article

Left: Hα-based SFRs vs. stellar mass for our CE...

Left: Hα-based SFRs vs. stellar mass for our CECILIA Faint sample (pink squares and shad...

Menelaos Raptis et al, The Astrophysical Journal Letters 1004 2

Image Details View Article

Left: O3 vs. ...

Left: O3 vs. ﹩12+\mathrm{log}({\rm{O}}/{\rm{H}})﹩ diagram with O3-based metallicity cali...

Menelaos Raptis et al, The Astrophysical Journal Letters 1004 2

Image Details View Article

Photometry and best-fit SED models for two sour...

Photometry and best-fit SED models for two sources in the CECILIA Faint sample. The uppe...

Menelaos Raptis et al, The Astrophysical Journal Letters 1004 2

Image Details View Article

Left: redshift evolution of the low-mass MZR fr...

Left: redshift evolution of the low-mass MZR from z ∼ 0 to Cosmic Noon. At low redshift,...

Menelaos Raptis et al, The Astrophysical Journal Letters 1004 2

Image Details View Article

MZR for our CECILIA Faint sample (pink squares ...

MZR for our CECILIA Faint sample (pink squares and shaded rectangles as in Figure 2), wi...

Menelaos Raptis et al, The Astrophysical Journal Letters 1004 2

Image Details View Article

A comparison of various low-mass MZR measuremen...

A comparison of various low-mass MZR measurements at Cosmic Noon. The MZR for our CECILI...

Menelaos Raptis et al, The Astrophysical Journal Letters 1004 2

Image Details View Article

Comparison of the CECILIA Faint galaxy metallic...

Comparison of the CECILIA Faint galaxy metallicities (pink squares and shaded rectangles...

Menelaos Raptis et al, The Astrophysical Journal Letters 1004 2

Image Details View Article

MZR for our CECILIA Faint sample compared to in...

MZR for our CECILIA Faint sample compared to individual 1.8 < z < 3.4 lensed dwarf galax...

Menelaos Raptis et al, The Astrophysical Journal Letters 1004 2

Image Details View Article

Dynamical vs. stellar masses for the CECILIA Fa...

Dynamical vs. stellar masses for the CECILIA Faint sample (pink squares) with the 1:1 li...

Menelaos Raptis et al, The Astrophysical Journal Letters 1004 2

Image Details View Article

MZR for the CECILIA Faint sample when including...

MZR for the CECILIA Faint sample when including all galaxies (purple solid line) and whe...

Menelaos Raptis et al, The Astrophysical Journal Letters 1004 2

Image Details View Article

Constraints on physical properties using photoi...

Constraints on physical properties using photoionization modeling. We utilize Cue (Y. Li...

Jakob M. Helton et al, The Astrophysical Journal Letters 1004 2

Image Details View Article

The rest-frame optical spectrum of JADES-GS-z14...

The rest-frame optical spectrum of JADES-GS-z14-0. Top panel: the final MIRI/LRS 2D spec...

Jakob M. Helton et al, The Astrophysical Journal Letters 1004 2

Image Details View Article

Hα line luminosity versus absolute UV magnitude...

Hα line luminosity versus absolute UV magnitude. Left panel: these measurements are show...

Jakob M. Helton et al, The Astrophysical Journal Letters 1004 2

Image Details View Article

Slit locations for four separate visits. Our ta...

Slit locations for four separate visits. Our target, JADES-GS-z14-0, was observed using ...

Jakob M. Helton et al, The Astrophysical Journal Letters 1004 2

Image Details View Article

Zoomed-in views around the strongest rest-frame...

Zoomed-in views around the strongest rest-frame optical emission lines. From left to rig...

Jakob M. Helton et al, The Astrophysical Journal Letters 1004 2

Image Details View Article

Ionizing photon production efficiency versus bo...

Ionizing photon production efficiency versus both spectroscopic redshift and absolute UV...

Jakob M. Helton et al, The Astrophysical Journal Letters 1004 2

Image Details View Article

Carbon-to-oxygen ratio versus gas-phase oxygen ...

Carbon-to-oxygen ratio versus gas-phase oxygen abundance. The inferred chemical abundanc...

Jakob M. Helton et al, The Astrophysical Journal Letters 1004 2

Image Details View Article

Standard strong-line diagnostics with O32 versu...

Standard strong-line diagnostics with O32 versus R3 and R23. Both panels: these emission...

Jakob M. Helton et al, The Astrophysical Journal Letters 1004 2

Image Details View Article

Parallaxes and proper motion fits for G021.87+0...

Parallaxes and proper motion fits for G021.87+00.01, G037.82+00.41, G060.57–00.18, and G...

L. J. Hyland et al, The Astrophysical Journal 1004 2

Image Details View Article

Comparison of parallax distance with maximum li...

Comparison of parallax distance with maximum likelihood distance in the Galactocentric c...

L. J. Hyland et al, The Astrophysical Journal 1004 2

Image Details View Article

Left: the log-periodic spiral arm fits. The sha...

Left: the log-periodic spiral arm fits. The shaded area shows the estimated Perseus arm ...

L. J. Hyland et al, The Astrophysical Journal 1004 2

Image Details View Article

Example of the distance determination process f...

Example of the distance determination process for G070.29+01.60. The Vlsr PDF (dashed re...

L. J. Hyland et al, The Astrophysical Journal 1004 2

Image Details View Article

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!