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The observed Day +196.1 SN 2024vjm JWST spect...

The observed Day +196.1 SN 2024vjm JWST spectrum, with tentative line identifications....

E. Baron et al, The Astrophysical Journal Letters 1008 2

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(a) The velocity space extent of the observed [...

(a) The velocity space extent of the observed [Co II] 10.52, [Ne II] 12.81, and [Fe III]...

E. Baron et al, The Astrophysical Journal Letters 1008 2

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(a) The W7-Iax model shown in Figure 7(a) is co...

(a) The W7-Iax model shown in Figure 7(a) is compared to the same model but where the mo...

E. Baron et al, The Astrophysical Journal Letters 1008 2

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The strong intermediate-mass element lines (top...

The strong intermediate-mass element lines (top row) and iron group element lines (botto...

E. Baron et al, The Astrophysical Journal Letters 1008 2

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(a) The observed Day +196.1 SN 2024vjm JWST s...

(a) The observed Day +196.1 SN 2024vjm JWST spectrum plotted against the best-fit blac...

E. Baron et al, The Astrophysical Journal Letters 1008 2

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(a) A simple model, W7-Iax, using W7 abundances...

(a) A simple model, W7-Iax, using W7 abundances with an ejecta mass of 0.42 M⊙ and the v...

E. Baron et al, The Astrophysical Journal Letters 1008 2

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The observed Day +196.1 SN 2024vjm JWST spect...

The observed Day +196.1 SN 2024vjm JWST spectrum plotted against other SNe Ia at simil...

E. Baron et al, The Astrophysical Journal Letters 1008 2

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SED of SN 2024vjm. The raw and smoothed Day +19...

SED of SN 2024vjm. The raw and smoothed Day +196.1 SN 2024vjm JWST spectrum plus the d...

E. Baron et al, The Astrophysical Journal Letters 1008 2

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The SN 2024vjm light curve obtained by ATLAS an...

The SN 2024vjm light curve obtained by ATLAS and POISE.

E. Baron et al, The Astrophysical Journal Letters 1008 2

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(a) The W7-Iax model shown in Figure 7(a), comp...

(a) The W7-Iax model shown in Figure 7(a), compared to the same model with the SiO opaci...

E. Baron et al, The Astrophysical Journal Letters 1008 2

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The mean absolute residuals in [Fe/H] as a func...

The mean absolute residuals in [Fe/H] as a function of aR for stars in different age bin...

Shaunak Modak et al, The Astrophysical Journal Letters 1008 2

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The measured values of σtot(τ), with points col...

The measured values of σtot(τ), with points colored as in Figure 3. Horizontal error bar...

Shaunak Modak et al, The Astrophysical Journal Letters 1008 2

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Absolute metallicity-residual distributions pro...

Absolute metallicity-residual distributions produced by formation and migration processe...

Shaunak Modak et al, The Astrophysical Journal Letters 1008 2

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Absolute residual histograms (with Poisson erro...

Absolute residual histograms (with Poisson error bars) for stars with τ < 2 Gyr in the s...

Shaunak Modak et al, The Astrophysical Journal Letters 1008 2

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Top left: a cumulative distribution function sh...

Top left: a cumulative distribution function showing the burst ages of the QPE host gala...

Margaret Shepherd et al, The Astrophysical Journal Letters 1008 2

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Top: the burst mass fraction of the QPE hosts a...

Top: the burst mass fraction of the QPE hosts and the control galaxies vs. the time sinc...

Margaret Shepherd et al, The Astrophysical Journal Letters 1008 2

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Comparison between the BAGPIPES results for the...

Comparison between the BAGPIPES results for the burst age (left column), burst mass frac...

Margaret Shepherd et al, The Astrophysical Journal Letters 1008 2

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The Hα emission equivalent width and Lick HδA a...

The Hα emission equivalent width and Lick HδA absorption in the optical spectra of QPE h...

Margaret Shepherd et al, The Astrophysical Journal Letters 1008 2

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Light curves for selected novae used for the de...

Light curves for selected novae used for the determination of t2 times. (a) LMCN 1971-03...

Allen W. Shafter, The Astrophysical Journal Supplement Series 286 1

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Light curves for selected novae used for the de...

Light curves for selected novae used for the determination of t2 times. (a) LMCN 2018-05...

Allen W. Shafter, The Astrophysical Journal Supplement Series 286 1

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The positions of the LMC nova candidates. The o...

The positions of the LMC nova candidates. The offsets were computed assuming the center ...

Allen W. Shafter, The Astrophysical Journal Supplement Series 286 1

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The history of nova candidate discoveries in th...

The history of nova candidate discoveries in the LMC plotted in decade-wide bins from 19...

Allen W. Shafter, The Astrophysical Journal Supplement Series 286 1

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Light curves for selected novae used for the de...

Light curves for selected novae used for the determination of t2 times. (a) LMCN 2024-03...

Allen W. Shafter, The Astrophysical Journal Supplement Series 286 1

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The cumulative fractions of the t2 times for th...

The cumulative fractions of the t2 times for the LMC nova sample compared with those of ...

Allen W. Shafter, The Astrophysical Journal Supplement Series 286 1

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Left panel: the MMRD plot for the LMC (blue poi...

Left panel: the MMRD plot for the LMC (blue points: He/N novae; red points: Fe II novae)...

Allen W. Shafter, The Astrophysical Journal Supplement Series 286 1

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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!