Astronomy Image Explorer

Latest Images

The first two rows show density profiles (densi...

The first two rows show density profiles (density versus position) at constant 1283 reso...

Isabel Barrios Lombardi and Ryan Jeffrey Farber, Research Notes of the AAS 10 11

Image Details View Article

Euclidean-normalized number counts for the Hers...

Euclidean-normalized number counts for the Herschel-SPIRE Dark Field at 250 μm (top left...

Rebecca Hughes et al, Research Notes of the AAS 10 11

Image Details View Article

Validation on the planetary microlensing event ...

Validation on the planetary microlensing event MOA-2022-BLG-091. Panels (a) and (c) show...

Michael Hippke, Research Notes of the AAS 10 11

Image Details View Article

(a) H I column density map of NGC 4214 from the...

(a) H I column density map of NGC 4214 from the FAST observation shown as black contours...

Shulan Yan et al, The Astrophysical Journal Letters 1011 2

Image Details View Article

(a) VLA H I spectrum of the central region with...

(a) VLA H I spectrum of the central region with COS observations. The data and the fitte...

Shulan Yan et al, The Astrophysical Journal Letters 1011 2

Image Details View Article

3D warped-disk model of H I data. The data, mod...

3D warped-disk model of H I data. The data, model, and residual are shown in (a), (b), a...

Shulan Yan et al, The Astrophysical Journal Letters 1011 2

Image Details View Article

Distribution of total density n = ni + ne, J/ec...

Distribution of total density n = ni + ne, J/ec, charge, and electron density ne for B0/...

Daniel Humphrey et al, The Astrophysical Journal Letters 1011 2

Image Details View Article

On the left, the electron density ne and the ve...

On the left, the electron density ne and the velocity associated with the current Δv = J...

Daniel Humphrey et al, The Astrophysical Journal Letters 1011 2

Image Details View Article

γ distribution for PIC particles in the case of...

γ distribution for PIC particles in the case of B0/δB0 = 10, as well as the bulk Lorentz...

Daniel Humphrey et al, The Astrophysical Journal Letters 1011 2

Image Details View Article

Distribution of total density n = ni + ne, J/ec...

Distribution of total density n = ni + ne, J/ec, charge, and electron density ne for B0/...

Daniel Humphrey et al, The Astrophysical Journal Letters 1011 2

Image Details View Article

Average pitch angles as a function of energy sh...

Average pitch angles as a function of energy shown for PIC particles over the whole simu...

Daniel Humphrey et al, The Astrophysical Journal Letters 1011 2

Image Details View Article

The normalized, conditional expectation value o...

The normalized, conditional expectation value of particle energy density as a function o...

Daniel Humphrey et al, The Astrophysical Journal Letters 1011 2

Image Details View Article

The prompt X-ray (0.4–2 keV) light curve of EP2...

The prompt X-ray (0.4–2 keV) light curve of EP260321a. The EP-WXT and EP-FXT data are ta...

Zhuo Li et al, The Astrophysical Journal Letters 1011 2

Image Details View Article

Schematic description of the geometry of the ej...

Schematic description of the geometry of the ejecta–wind interaction in an SN wind break...

Zhuo Li et al, The Astrophysical Journal Letters 1011 2

Image Details View Article

Multiband early optical light curves of EP26032...

Multiband early optical light curves of EP260321a/SN 26gzf within 30 ks after the start ...

Zhuo Li et al, The Astrophysical Journal Letters 1011 2

Image Details View Article

Optical spectrum of EP260321a/SN 26gzf observed...

Optical spectrum of EP260321a/SN 26gzf observed at 8500 s since the start time T0. The m...

Zhuo Li et al, The Astrophysical Journal Letters 1011 2

Image Details View Article

Top panel: 2025 white light curve covering the ...

Top panel: 2025 white light curve covering the same wavelength range as the HST/WFC3 whi...

Elena Manjavacas et al, The Astrophysical Journal Letters 1011 2

Image Details View Article

Top panel: median combination of the 20 maximum...

Top panel: median combination of the 20 maximum flux (blue) and 20 minimum flux spectra ...

Elena Manjavacas et al, The Astrophysical Journal Letters 1011 2

Image Details View Article

White light curve (1.10–1.63 μm, blue, panel (a...

White light curve (1.10–1.63 μm, blue, panel (a)), J- (green, panel (b)), H- (pink, pane...

Elena Manjavacas et al, The Astrophysical Journal Letters 1011 2

Image Details View Article

Phase-folded light curves using the P ∼ 5.7 hr ...

Phase-folded light curves using the P ∼ 5.7 hr rotational period (left panels) and the P...

Elena Manjavacas et al, The Astrophysical Journal Letters 1011 2

Image Details View Article

Classification and dynamic changes of the Zhuro...

Classification and dynamic changes of the Zhurong plume-disturbed zone. (a) Various regi...

Zhibin Li et al, The Astronomical Journal 172 6

Image Details View Article

Radiometric cross calibration and normalization...

Radiometric cross calibration and normalization analysis for HiRIC and HiRISE data. (a) ...

Zhibin Li et al, The Astronomical Journal 172 6

Image Details View Article

Meteorological environmental comparisons at mul...

Meteorological environmental comparisons at multiple Martian landing sites based on the ...

Zhibin Li et al, The Astronomical Journal 172 6

Image Details View Article

Schematic diagram of the variations of the pass...

Schematic diagram of the variations of the passivation-affected region. (a) Before the l...

Zhibin Li et al, The Astronomical Journal 172 6

Image Details View Article

Timeline of all HiRISE and HiRIC observations u...

Timeline of all HiRISE and HiRIC observations used in this study, illustrating the obser...

Zhibin Li et al, The Astronomical Journal 172 6

Image Details View Article

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!