Latest Images

Keck LRIS images of PSR J1544+4937, revealing a...

Identification of the Optical Counterpa...

Keck LRIS images of PSR J1544+4937, revealing a variable optical source at the nominal p...

Tang et al., The Astrophysical Journal Letters 791 1 L5

Top: folded optical light curves of PSR J1544+4...

Identification of the Optical Counterpa...

Top: folded optical light curves of PSR J1544+4937. The I, R, g, and B data shown as sol...

Tang et al., The Astrophysical Journal Letters 791 1 L5

One- and two-dimensional distributions of the k...

Identification of the Optical Counterpa...

One- and two-dimensional distributions of the key parameter values resulting from our Ic...

Tang et al., The Astrophysical Journal Letters 791 1 L5

Mass–radius relation for the companion of PSR J...

Identification of the Optical Counterpa...

Mass–radius relation for the companion of PSR J1544+4937 derived from different light cu...

Tang et al., The Astrophysical Journal Letters 791 1 L5

First-moment map of CO J = 3–2 emission (color ...

ALMA Hints at the Presence of two Compa...

First-moment map of CO J = 3–2 emission (color map) overlaid with integrated intensity c...

Walsh et al., The Astrophysical Journal Letters 791 1 L6

Normalized continuum flux at 346 GHz (blue line...

ALMA Hints at the Presence of two Compa...

Normalized continuum flux at 346 GHz (blue lines) and CO J = 3–2 (345.795 GHz) integrate...

Walsh et al., The Astrophysical Journal Letters 791 1 L6

Visibilities as a function of the deprojected b...

ALMA Hints at the Presence of two Compa...

Visibilities as a function of the deprojected baseline overlaid with the best-fit “singl...

Walsh et al., The Astrophysical Journal Letters 791 1 L6

Residual images (color map) and contours (white...

ALMA Hints at the Presence of two Compa...

Residual images (color map) and contours (white lines) overlaid with observed 3σ contour...

Walsh et al., The Astrophysical Journal Letters 791 1 L6

Surface density of millimeter-sized and microme...

ALMA Hints at the Presence of two Compa...

Surface density of millimeter-sized and micrometer-sized grains (top and bottom rows, re...

Walsh et al., The Astrophysical Journal Letters 791 1 L6

GW degeneracies, illustrated by the first princ...

Prospects for Joint Gravitational-wave ...

GW degeneracies, illustrated by the first principal component lines (red) in the MBH–MNS...

Pannarale & Ohme, The Astrophysical Journal Letters 791 1 L7

Second principal component lines in the MBH– pl...

Prospects for Joint Gravitational-wave ...

Second principal component lines in the MBH– plane for constant MChirp, as defined in th...

Pannarale & Ohme, The Astrophysical Journal Letters 791 1 L7

MChirp– combinations for which an EM counterpar...

Prospects for Joint Gravitational-wave ...

MChirp– combinations for which an EM counterpart is not supported (dark gray), EM counte...

Pannarale & Ohme, The Astrophysical Journal Letters 791 1 L7

Top panel: phase shift Δϕ between fluctuations ...

Globular Clusters and Dark Satellite Ga...

Top panel: phase shift Δϕ between fluctuations in the baryons and DM as a function of re...

Naoz & Narayan, The Astrophysical Journal Letters 791 1 L8

Top panel: the vertical axis measures the rarit...

Globular Clusters and Dark Satellite Ga...

Top panel: the vertical axis measures the rarity of fluctuations (“number of σ's”) neede...

Naoz & Narayan, The Astrophysical Journal Letters 791 1 L8

Top left panel: spatial separation between bary...

Globular Clusters and Dark Satellite Ga...

Top left panel: spatial separation between baryon and DM clumps at the redshift of colla...

Naoz & Narayan, The Astrophysical Journal Letters 791 1 L8

Zoomed view of the (a) (mF606W − mF814W; mF606W...

First Evidence of Fully Spatially Mixed...

Zoomed view of the (a) (mF606W − mF814W; mF606W) and (b) (mF336W − mF336W; mF606W) CMDs ...

Dalessandro et al., The Astrophysical Journal Letters 791 1 L4

Δ(mF336W − mF606W) color distribution of RGB st...

First Evidence of Fully Spatially Mixed...

Δ(mF336W − mF606W) color distribution of RGB stars (left panel) and Δ(mF336W) magnitude ...

Dalessandro et al., The Astrophysical Journal Letters 791 1 L4

Different CMDs obtained combining the F336W fil...

First Evidence of Fully Spatially Mixed...

Different CMDs obtained combining the F336W filter with all the other bands of the HST s...

Dalessandro et al., The Astrophysical Journal Letters 791 1 L4

Optical (left panel) and NUV (right panel) CMD ...

First Evidence of Fully Spatially Mixed...

Optical (left panel) and NUV (right panel) CMD of the WFI sample for r < 300″. Red and b...

Dalessandro et al., The Astrophysical Journal Letters 791 1 L4

Upper panel: cumulative radial distribution of ...

First Evidence of Fully Spatially Mixed...

Upper panel: cumulative radial distribution of SG (red) and FG (blue) stars selected as ...

Dalessandro et al., The Astrophysical Journal Letters 791 1 L4

Peak flux of neutral helium observed by IBEX on...

Warm Breeze from the Starboard Bow: a N...

Peak flux of neutral helium observed by IBEX on orbits 54 through 68 during the 2010 obs...

Kubiak et al., The Astrophysical Journal Supplement Series 213 2 29

Data used in the analysis. Gray dots with error...

Warm Breeze from the Starboard Bow: a N...

Data used in the analysis. Gray dots with error bars represent count rates averaged over...

Kubiak et al., The Astrophysical Journal Supplement Series 213 2 29

Estimated background levels for seasons 2009 th...

Warm Breeze from the Starboard Bow: a N...

Estimated background levels for seasons 2009 through 2012, shown in counts per second pe...

Kubiak et al., The Astrophysical Journal Supplement Series 213 2 29

Optimized values of the merit function χ2 for v...

Warm Breeze from the Starboard Bow: a N...

Optimized values of the merit function χ2 for various values of the Warm Breeze inflow d...

Kubiak et al., The Astrophysical Journal Supplement Series 213 2 29

Approximate areas in the parameter space where ...

Warm Breeze from the Starboard Bow: a N...

Approximate areas in the parameter space where the χ2 values are within one of the minim...

Kubiak et al., The Astrophysical Journal Supplement Series 213 2 29

Data used for fitting (dark blue symbols with e...

Warm Breeze from the Starboard Bow: a N...

Data used for fitting (dark blue symbols with error bars), compared with the best-fittin...

Kubiak et al., The Astrophysical Journal Supplement Series 213 2 29

Data used for fitting (dark blue symbols with e...

Warm Breeze from the Starboard Bow: a N...

Data used for fitting (dark blue symbols with error bars), compared with the best-fittin...

Kubiak et al., The Astrophysical Journal Supplement Series 213 2 29

Comparison of simulated peak heights for the or...

Warm Breeze from the Starboard Bow: a N...

Comparison of simulated peak heights for the orbits used in the analysis for a Maxwellia...

Kubiak et al., The Astrophysical Journal Supplement Series 213 2 29

Data vs. simulations (NIS He + Warm Breeze) dif...

Warm Breeze from the Starboard Bow: a N...

Data vs. simulations (NIS He + Warm Breeze) differing by the lower limit of the integrat...

Kubiak et al., The Astrophysical Journal Supplement Series 213 2 29

Expected signal from the NIS He population for ...

Warm Breeze from the Starboard Bow: a N...

Expected signal from the NIS He population for orbits 54 through 59, i.e., from the cros...

Kubiak et al., The Astrophysical Journal Supplement Series 213 2 29

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