Latest Images

Relation between B − V color and the stellar ma...

Color-Mass-to-light-ratio Relations for...

Relation between B − V color and the stellar mass-to-light ratio in the V band (left), I...

McGaugh & Schombert, The Astronomical Journal 148 5 77

Stellar masses (Table 3) estimated by populatio...

Color-Mass-to-light-ratio Relations for...

Stellar masses (Table 3) estimated by population synthesis models (Bell et al. 2003; Por...

McGaugh & Schombert, The Astronomical Journal 148 5 77

Stellar mass-to-light ratios in the I band (ope...

Color-Mass-to-light-ratio Relations for...

Stellar mass-to-light ratios in the I band (open circles) and [3.6] (filled circles) as ...

McGaugh & Schombert, The Astronomical Journal 148 5 77

Stellar mass-to-light ratios in the I band (ope...

Color-Mass-to-light-ratio Relations for...

Stellar mass-to-light ratios in the I band (open circles) and [3.6] (filled circles) as ...

McGaugh & Schombert, The Astronomical Journal 148 5 77

Stellar mass-to-light ratios in the I band (ope...

Color-Mass-to-light-ratio Relations for...

Stellar mass-to-light ratios in the I band (open circles) and [3.6] (filled circles) as ...

McGaugh & Schombert, The Astronomical Journal 148 5 77

Relation between B − V color and the stellar ma...

Color-Mass-to-light-ratio Relations for...

Relation between B − V color and the stellar mass-to-light ratio in the V band (left), I...

McGaugh & Schombert, The Astronomical Journal 148 5 77

Offset in mass-to-light ratios in the I-band (t...

Color-Mass-to-light-ratio Relations for...

Offset in mass-to-light ratios in the I-band (top row) and [3.6] (bottom row) as a funct...

McGaugh & Schombert, The Astronomical Journal 148 5 77

Stellar mass-to-light ratios in the I band (ope...

Color-Mass-to-light-ratio Relations for...

Stellar mass-to-light ratios in the I band (open circles) and [3.6] (filled circles) as ...

McGaugh & Schombert, The Astronomical Journal 148 5 77

Map of the ATLAS-CDFS field (third data release...

Bent-tailed Radio Sources in the Austra...

Map of the ATLAS-CDFS field (third data release) showing the location of detected halos,...

Dehghan et al., The Astronomical Journal 148 5 75

Detected sources in the ATLAS-CDFS field. Radio...

Bent-tailed Radio Sources in the Austra...

Detected sources in the ATLAS-CDFS field. Radio structure of the detected sources based ...

Dehghan et al., The Astronomical Journal 148 5 75

Detected sources in the ATLAS-CDFS field. Radio...

Bent-tailed Radio Sources in the Austra...

Detected sources in the ATLAS-CDFS field. Radio structure of the detected sources based ...

Dehghan et al., The Astronomical Journal 148 5 75

Detected sources in the ATLAS-CDFS field. Radio...

Bent-tailed Radio Sources in the Austra...

Detected sources in the ATLAS-CDFS field. Radio structure of the detected sources based ...

Dehghan et al., The Astronomical Journal 148 5 75

Top panel: the comparative radio structure of I...

Bent-tailed Radio Sources in the Austra...

Top panel: the comparative radio structure of ID 11 detected via the ATLAS data and the ...

Dehghan et al., The Astronomical Journal 148 5 75

Spatial distribution of galaxies surrounding ID...

Bent-tailed Radio Sources in the Austra...

Spatial distribution of galaxies surrounding ID 53, including the galaxy cluster APMCC 4...

Dehghan et al., The Astronomical Journal 148 5 75

Left panel: the rest-frame 1.4 GHz luminosity–r...

Bent-tailed Radio Sources in the Austra...

Left panel: the rest-frame 1.4 GHz luminosity–redshift relation for the detected BTs. Th...

Dehghan et al., The Astronomical Journal 148 5 75

Target stars with detected companions within 1″...

Adaptive Optics Images. III. 87 Kepler ...

Target stars with detected companions within 1″. Each box is 2″ by 2″. The color scaling...

Dressing et al., The Astronomical Journal 148 5 78

Target stars with detected companions between 1...

Adaptive Optics Images. III. 87 Kepler ...

Target stars with detected companions between 1″ and 2″. Each box is 4″ by 4″. The color...

Dressing et al., The Astronomical Journal 148 5 78

Target stars with detected companions between 2...

Adaptive Optics Images. III. 87 Kepler ...

Target stars with detected companions between 2″ and 4″. Each box is 12″ by 12″. KOI 266...

Dressing et al., The Astronomical Journal 148 5 78

Detected nearby stars (black crosses or stars) ...

Adaptive Optics Images. III. 87 Kepler ...

Detected nearby stars (black crosses or stars) and detection limits (lines) on the prese...

Dressing et al., The Astronomical Journal 148 5 78

Kepler magnitudes of host stars vs. the radii o...

Adaptive Optics Images. III. 87 Kepler ...

Kepler magnitudes of host stars vs. the radii of associated planet candidates for the KO...

Dressing et al., The Astronomical Journal 148 5 78

Galactic latitude distribution of AO targets (b...

Adaptive Optics Images. III. 87 Kepler ...

Galactic latitude distribution of AO targets (black solid line), AO targets without iden...

Dressing et al., The Astronomical Journal 148 5 78

Radii and periods for the planet candidates (cr...

Adaptive Optics Images. III. 87 Kepler ...

Radii and periods for the planet candidates (crosses), confirmed planets (stars), and fa...

Dressing et al., The Astronomical Journal 148 5 78

Voyager 2 Doppler residuals.

The Orbits of the Uranian Satellites an...

Voyager 2 Doppler residuals.

Jacobson, The Astronomical Journal 148 5 76

Pole Right Ascension change.

The Orbits of the Uranian Satellites an...

Pole Right Ascension change.

Jacobson, The Astronomical Journal 148 5 76

Pole declination change.

The Orbits of the Uranian Satellites an...

Pole declination change.

Jacobson, The Astronomical Journal 148 5 76

Contour plots showing the time taken for the rm...

On Asymmetric Distributions of Satellit...

Contour plots showing the time taken for the rms Δϕ to reach 2π as a function of dispers...

Bowden, Evans, & Belokurov, The Astrophysical Journal Letters 793 2 L42

Plot showing the number of orbits required for ...

On Asymmetric Distributions of Satellit...

Plot showing the number of orbits required for a Gaussian clump to phase mix as a functi...

Bowden, Evans, & Belokurov, The Astrophysical Journal Letters 793 2 L42

Hubble parameter (left panel) and the effective...

Model-independent Evidence for Dark Ene...

Hubble parameter (left panel) and the effective equation of state of dark energy (right ...

Sahni, Shafieloo, & Starobinsky, The Astrophysical Journal Letters 793 2 L40

Spectrum of Himalia from 2.2 to 3.8 μm. The sho...

The 3 μm Spectrum of Jupiter's Irregula...

Spectrum of Himalia from 2.2 to 3.8 μm. The shorter and longer wavelength NIRSPEC settin...

Brown & Rhoden, The Astrophysical Journal Letters 793 2 L44

Spectrum of Himalia compared to the spectrum of...

The 3 μm Spectrum of Jupiter's Irregula...

Spectrum of Himalia compared to the spectrum of the 52 Europa (blue), the prototype of t...

Brown & Rhoden, The Astrophysical Journal Letters 793 2 L44

SEARCH TERM(S)

PUBLICATIONS

  • 79754
  • 370585
  • 36873
  • 50074

YEAR RANGE:

1995
2014

CONTENT TYPE

AUTHOR