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Keck/LRIS spectra of the three extreme WISE-sel...

NuSTAR and XMM-Newton Observa...

Keck/LRIS spectra of the three extreme WISE-selected obscured AGNs at z ∼ 2 which we obs...

Stern et al., The Astrophysical Journal 794 2 102

Gross source counts vs. background counts (scal...

NuSTAR and XMM-Newton Observa...

Gross source counts vs. background counts (scaled to the source region) for WISE J1814+3...

Stern et al., The Astrophysical Journal 794 2 102

Best-fitting SED template models (heavy gray li...

NuSTAR and XMM-Newton Observa...

Best-fitting SED template models (heavy gray line) to the WISE photometry (shown by gree...

Stern et al., The Astrophysical Journal 794 2 102

Rest-frame X-ray luminosity against rest-frame ...

NuSTAR and XMM-Newton Observa...

Rest-frame X-ray luminosity against rest-frame 6 μm luminosity for: (left) 2–10 keV lumi...

Stern et al., The Astrophysical Journal 794 2 102

J-band image of NGC 6822 created from our FourS...

A New Cepheid Distance Measurement and ...

J-band image of NGC 6822 created from our FourStar data with the overlapping Spitzer IRA...

Rich et al., The Astrophysical Journal 794 2 107

Light curve photometry for a typical Cepheid fr...

A New Cepheid Distance Measurement and ...

Light curve photometry for a typical Cepheid from our sample. The average magnitude and ...

Rich et al., The Astrophysical Journal 794 2 107

Period–luminosity relations in all of the bands...

A New Cepheid Distance Measurement and ...

Period–luminosity relations in all of the bands used in this paper; data are in Table 1....

Rich et al., The Astrophysical Journal 794 2 107

First method for calculating a true distance mo...

A New Cepheid Distance Measurement and ...

First method for calculating a true distance modulus, μo and E(B − V). Data points corre...

Rich et al., The Astrophysical Journal 794 2 107

Individual reddening fits applied to each Cephe...

A New Cepheid Distance Measurement and ...

Individual reddening fits applied to each Cepheid, normalized to each star's I-band magn...

Rich et al., The Astrophysical Journal 794 2 107

Same as Figure 5, but without normalization app...

A New Cepheid Distance Measurement and ...

Same as Figure 5, but without normalization applied and individual data points removed. ...

Rich et al., The Astrophysical Journal 794 2 107

Mixture distribution of distance moduli in Tabl...

A New Cepheid Distance Measurement and ...

Mixture distribution of distance moduli in Table 5. Top panel: normal distributions with...

Rich et al., The Astrophysical Journal 794 2 107

Postage stamps of the Cepheids with near-IR mag...

A New Cepheid Distance Measurement and ...

Postage stamps of the Cepheids with near-IR magnitudes measured in our analysis. The ima...

Rich et al., The Astrophysical Journal 794 2 107

Light curves for the GLOESS fits to four Cephei...

A New Cepheid Distance Measurement and ...

Light curves for the GLOESS fits to four Cepheids (CEP001, CEP002, CEP003, CEP004), as i...

Rich et al., The Astrophysical Journal 794 2 107

Same as Figure 9, but for CEP005, CEP006, CEP00...

A New Cepheid Distance Measurement and ...

Same as Figure 9, but for CEP005, CEP006, CEP007, and CEP008.

Rich et al., The Astrophysical Journal 794 2 107

Same as Figure 9, but for CEP009, CEP010, CEP01...

A New Cepheid Distance Measurement and ...

Same as Figure 9, but for CEP009, CEP010, CEP011, and CEP012.

Rich et al., The Astrophysical Journal 794 2 107

Same as Figure 9, but for CEP013, CEP014, CEP01...

A New Cepheid Distance Measurement and ...

Same as Figure 9, but for CEP013, CEP014, CEP015, and CEP016.

Rich et al., The Astrophysical Journal 794 2 107

Same as Figure 9, but for CEP017, CEP018, CEP01...

A New Cepheid Distance Measurement and ...

Same as Figure 9, but for CEP017, CEP018, CEP019, and CEP020.

Rich et al., The Astrophysical Journal 794 2 107

Same as Figure 9, but for CEP021, CEP022, CEP02...

A New Cepheid Distance Measurement and ...

Same as Figure 9, but for CEP021, CEP022, CEP023, and CEP024.

Rich et al., The Astrophysical Journal 794 2 107

Same as Figure 9, but for CEP025, CEP026, CEP02...

A New Cepheid Distance Measurement and ...

Same as Figure 9, but for CEP025, CEP026, CEP027, and CEP028.

Rich et al., The Astrophysical Journal 794 2 107

Same as Figure 9, but for CEP029, CEP030, CEP03...

A New Cepheid Distance Measurement and ...

Same as Figure 9, but for CEP029, CEP030, CEP031, and CEP032.

Rich et al., The Astrophysical Journal 794 2 107

Same as Figure 9, but for CEP033, CEP034, CEP03...

A New Cepheid Distance Measurement and ...

Same as Figure 9, but for CEP033, CEP034, CEP035, and CEP036.

Rich et al., The Astrophysical Journal 794 2 107

Same as Figure 9, but for CEP037, CEP038, and C...

A New Cepheid Distance Measurement and ...

Same as Figure 9, but for CEP037, CEP038, and CEP039.

Rich et al., The Astrophysical Journal 794 2 107

Top panels show the Lagrangian radii for the fo...

On the Distribution of Stellar Remnants...

Top panels show the Lagrangian radii for the four stellar species during the N-body simu...

Antonini, The Astrophysical Journal 794 2 106

Evolution of the density slope, γ ≡ −dlog ρ/dlo...

On the Distribution of Stellar Remnants...

Evolution of the density slope, γ ≡ −dlog ρ/dlog r, of the main-sequence density profile...

Antonini, The Astrophysical Journal 794 2 106

Evolution of the fbh = 0 model Lagrangian radii...

On the Distribution of Stellar Remnants...

Evolution of the fbh = 0 model Lagrangian radii and density profile compared with the ev...

Antonini, The Astrophysical Journal 794 2 106

Top panel shows the evolution of the density of...

On the Distribution of Stellar Remnants...

Top panel shows the evolution of the density of 10 M☉ BHs due to dynamical friction agai...

Antonini, The Astrophysical Journal 794 2 106

Effective radii (Reff) of galaxies plotted agai...

On the Distribution of Stellar Remnants...

Effective radii (Reff) of galaxies plotted against their masses (Mgal). Filled circles a...

Antonini, The Astrophysical Journal 794 2 106

Evolution of the cluster model during the initi...

On the Distribution of Stellar Remnants...

Evolution of the cluster model during the initial N-body integrations used to realize th...

Antonini, The Astrophysical Journal 794 2 106

Inspiral of a ∼106 M☉ globular cluster in a Mil...

On the Distribution of Stellar Remnants...

Inspiral of a ∼106 M☉ globular cluster in a Milky Way model. The linear size of each box...

Antonini, The Astrophysical Journal 794 2 106

Time evolution of galactocentric radius (upper ...

On the Distribution of Stellar Remnants...

Time evolution of galactocentric radius (upper panels) and bound mass (lower panels) of ...

Antonini, The Astrophysical Journal 794 2 106

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