Astronomy Image Explorer

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Top panel: phase-integrated polarization degree...

Top panel: phase-integrated polarization degree and angle in the 2.0–7.5 keV detected by...

Roberto Taverna et al, The Astrophysical Journal Letters 1011 2

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Pulse profile of EP J223759.5+531421 from the I...

Pulse profile of EP J223759.5+531421 from the IXPE-EP joint analysis in the 2.0–7.5 keV ...

Roberto Taverna et al, The Astrophysical Journal Letters 1011 2

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Phase-integrated count spectra (dots with 1σ er...

Phase-integrated count spectra (dots with 1σ error bars) collected by IXPE DU 1 (yellow)...

Roberto Taverna et al, The Astrophysical Journal Letters 1011 2

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Temperature (top) and emitting radius (bottom) ...

Temperature (top) and emitting radius (bottom) of the warm (cyan) and hot (orange) black...

Roberto Taverna et al, The Astrophysical Journal Letters 1011 2

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Phase-dependent polarization degree (top) and a...

Phase-dependent polarization degree (top) and angle (bottom) in the 2.0–7.5 keV band (bl...

Roberto Taverna et al, The Astrophysical Journal Letters 1011 2

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Phase-dependent polarization degree (top) and a...

Phase-dependent polarization degree (top) and angle (bottom) in the 2.0–7.5 (blue), 2.0–...

Roberto Taverna et al, The Astrophysical Journal Letters 1011 2

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Polarization degree and angle measured in the 2...

Polarization degree and angle measured in the 2.0–7.5 keV band by IXPE in the phase bins...

Roberto Taverna et al, The Astrophysical Journal Letters 1011 2

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Top: IXPE 2.0–7.5 keV polarization angle (blue ...

Top: IXPE 2.0–7.5 keV polarization angle (blue points with error bars) fitted with the R...

Roberto Taverna et al, The Astrophysical Journal Letters 1011 2

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Phase-dependent 2.0–7.5 keV (normalized) flux (...

Phase-dependent 2.0–7.5 keV (normalized) flux (top, black lines), polarization degree (c...

Roberto Taverna et al, The Astrophysical Journal Letters 1011 2

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Simulated luminous binary population properties...

Simulated luminous binary population properties (orbital period Porb, parallax ϖ, eccent...

Casey Y. Lam et al, The Astrophysical Journal Supplement Series 287 1

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Roman GBTDS footprint (black outline) with the ...

Roman GBTDS footprint (black outline) with the locations of the simulated fields run in ...

Casey Y. Lam et al, The Astrophysical Journal Supplement Series 287 1

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Top panel: simulated luminosity function (numbe...

Top panel: simulated luminosity function (number of sources per magnitude bin) for the c...

Casey Y. Lam et al, The Astrophysical Journal Supplement Series 287 1

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Schematic of the observational structure of the...

Schematic of the observational structure of the GBTDS. Six fields toward the Galactic bu...

Casey Y. Lam et al, The Astrophysical Journal Supplement Series 287 1

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Simulated astrometry for three binaries. The le...

Simulated astrometry for three binaries. The left panels show the on-sky trajectories; g...

Casey Y. Lam et al, The Astrophysical Journal Supplement Series 287 1

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GBTDS F146 per-exposure astrometric precision σ...

GBTDS F146 per-exposure astrometric precision σast (top panel; solid gray line) and SNR ...

Casey Y. Lam et al, The Astrophysical Journal Supplement Series 287 1

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Distance, orbital period Porb, and F146Vega mag...

Distance, orbital period Porb, and F146Vega magnitude distributions of NS+star and BH+st...

Casey Y. Lam et al, The Astrophysical Journal Supplement Series 287 1

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Detectability of binaries in the contiguous GBT...

Detectability of binaries in the contiguous GBTDS fields, broken down by binary type. Th...

Casey Y. Lam et al, The Astrophysical Journal Supplement Series 287 1

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Distribution of the goodness of fit z1s of sour...

Distribution of the goodness of fit z1s of sources in the GBTDS contiguous field with F1...

Casey Y. Lam et al, The Astrophysical Journal Supplement Series 287 1

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BH+star binaries simulated in the Roman GBTDS c...

BH+star binaries simulated in the Roman GBTDS contiguous fields. All simulated sources a...

Casey Y. Lam et al, The Astrophysical Journal Supplement Series 287 1

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Extraction-consistency diagnostic between adopt...

Extraction-consistency diagnostic between adopted X1D and continuum-peak-centered S3D li...

Siqi Liu et al, The Astrophysical Journal 1011 2

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Leo P aperture-matching test. Left: gray square...

Leo P aperture-matching test. Left: gray squares mark valid public S3D spaxels throughou...

Siqi Liu et al, The Astrophysical Journal 1011 2

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Continuum-window systematic half-width for base...

Continuum-window systematic half-width for baseline X1D detections. Each point summarize...

Siqi Liu et al, The Astrophysical Journal 1011 2

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Summary of the adopted H2 line inventory. Color...

Summary of the adopted H2 line inventory. Colors identify the four targets, as labeled i...

Siqi Liu et al, The Astrophysical Journal 1011 2

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Upper-level populations for the adopted line de...

Upper-level populations for the adopted line decisions. The vertical axis is ...

Siqi Liu et al, The Astrophysical Journal 1011 2

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Focused P0/P1 line windows and R/QA candidates ...

Focused P0/P1 line windows and R/QA candidates used to construct the adopted conservativ...

Siqi Liu et al, The Astrophysical Journal 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!