Latest Images

PSF-subtracted image of the inner region. The w...

PSF-subtracted image of the inner region. The white lines represent the predicted locati...

Jorge Llop-Sayson et al, The Astronomical Journal 170 4

Left: azimuthal average of the surface brightne...

Left: azimuthal average of the surface brightness as a function of offset from ϵ Eridani...

Jorge Llop-Sayson et al, The Astronomical Journal 170 4

PSF-subtracted images of the observations of ϵ ...

PSF-subtracted images of the observations of ϵ Eridani observations with the JWST/NIRCam...

Jorge Llop-Sayson et al, The Astronomical Journal 170 4

Mass sensitivities from JWST/NIRCam coronagraph...

Mass sensitivities from JWST/NIRCam coronagraphic observations of ϵ Eridani assuming E. ...

Jorge Llop-Sayson et al, The Astronomical Journal 170 4

Sensitivity limits (5σ) in terms of contrast. T...

Sensitivity limits (5σ) in terms of contrast. The result from these observations with JW...

Jorge Llop-Sayson et al, The Astronomical Journal 170 4

Subtraction residuals for each target-PSF pairi...

Subtraction residuals for each target-PSF pairing used in the high SNR reduction (classi...

Jorge Llop-Sayson et al, The Astronomical Journal 170 4

Full-array observation contrast curves. The exp...

Full-array observation contrast curves. The exposure time for this mode was optimized fo...

Jorge Llop-Sayson et al, The Astronomical Journal 170 4

The final F444W image produced via classical RD...

The final F444W image produced via classical RDI optimized for extended source emission ...

Jorge Llop-Sayson et al, The Astronomical Journal 170 4

The radial MAD values of the individual target-...

The radial MAD values of the individual target-SGD PSF pair subtractions for the epoch 2...

Jorge Llop-Sayson et al, The Astronomical Journal 170 4

Planet radius limits for a planet of mass = 0.9...

Planet radius limits for a planet of mass = 0.98 MJ, i.e., the latest mass estimate for ...

Jorge Llop-Sayson et al, The Astronomical Journal 170 4

Contrast curves comparing the performance of th...

Contrast curves comparing the performance of the 3-roll strategy (black) with respect to...

Jorge Llop-Sayson et al, The Astronomical Journal 170 4

Contrast curves for the two epochs of observati...

Contrast curves for the two epochs of observations of δ Eridani, the reference star for ...

Jorge Llop-Sayson et al, The Astronomical Journal 170 4

Spatial distribution of members and gas. The ba...

Spatial distribution of members and gas. The background images were taken from the Digit...

Beomdu Lim et al, The Astronomical Journal 170 4

IGRINS slit positions over one of the southern ...

IGRINS slit positions over one of the southern pillars. The grayscale images represent t...

Beomdu Lim et al, The Astronomical Journal 170 4

Parallaxes (left) and PMs (right) of member can...

Parallaxes (left) and PMs (right) of member candidates. The left panel shows the distrib...

Beomdu Lim et al, The Astronomical Journal 170 4

Radial surface density profile. Poisson statist...

Radial surface density profile. Poisson statistics was assumed to obtain the error for g...

Beomdu Lim et al, The Astronomical Journal 170 4

Color–color diagram of early-type members (blac...

Color–color diagram of early-type members (black dots). The blue solid curve represents ...

Beomdu Lim et al, The Astronomical Journal 170 4

Color–color diagrams of IR sources from the GLI...

Color–color diagrams of IR sources from the GLIMPS survey (E. Churchwell et al. 2009). T...

Beomdu Lim et al, The Astronomical Journal 170 4

CMD of members. Several member candidates (red ...

CMD of members. Several member candidates (red crosses) below the orange solid lines are...

Beomdu Lim et al, The Astronomical Journal 170 4

Rotation of NGC 6611 within rcl. The upper pane...

Rotation of NGC 6611 within rcl. The upper panel represents the spatial variation of mea...

Beomdu Lim et al, The Astronomical Journal 170 4

Kinematics of stars in M16. Left panel: the pro...

Kinematics of stars in M16. Left panel: the proper motion vectors of stars relative to N...

Beomdu Lim et al, The Astronomical Journal 170 4

Map of proper motion vectors (upper) and the Φ ...

Map of proper motion vectors (upper) and the Φ distribution of the cluster members (lowe...

Beomdu Lim et al, The Astronomical Journal 170 4

Integrated intensity maps and position–velocity...

Integrated intensity maps and position–velocity diagrams of stars and gas in Regions 1 (...

Beomdu Lim et al, The Astronomical Journal 170 4

Color excess ratios of the early-type members (...

Color excess ratios of the early-type members (red dots). The black line shows the color...

Beomdu Lim et al, The Astronomical Journal 170 4

CMDs in comparison with the MESA theoretical is...

CMDs in comparison with the MESA theoretical isochrones for three different ages: 1 Myr ...

Beomdu Lim et al, The Astronomical Journal 170 4

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