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Data obtained from the differential output of a...

Data obtained from the differential output of a double Bracewell nuller, showing the rec...

Philipp A. Huber et al, The Astronomical Journal 170 4

Definition of the instrumental setup. The obser...

Definition of the instrumental setup. The observed astrophysical scene consists of the s...

Philipp A. Huber et al, The Astronomical Journal 170 4

Differential intensity response, R4 − R3, of a ...

Differential intensity response, R4 − R3, of a double Bracewell nuller in the case of an...

Philipp A. Huber et al, The Astronomical Journal 170 4

Covariance for the bottom panel of Figure 4, co...

Covariance for the bottom panel of Figure 4, confirming strong correlations between wave...

Philipp A. Huber et al, The Astronomical Journal 170 4

Illustration of the effect of the whitening tra...

Illustration of the effect of the whitening transformation on the planetary model (top) ...

Philipp A. Huber et al, The Astronomical Journal 170 4

Intensity response within the angular extent of...

Intensity response within the angular extent of the star (dark gray circle) for an ideal...

Philipp A. Huber et al, The Astronomical Journal 170 4

Correlation maps showing the correlation of the...

Correlation maps showing the correlation of the data with the planetary templates, y...

Philipp A. Huber et al, The Astronomical Journal 170 4

Top: underlying pink power spectrum with a 1/ω ...

Top: underlying pink power spectrum with a 1/ω falloff. Bottom: random time series of an...

Philipp A. Huber et al, The Astronomical Journal 170 4

Planetary SED (left) and the corresponding sign...

Planetary SED (left) and the corresponding signature in the differential output (right) ...

Philipp A. Huber et al, The Astronomical Journal 170 4

Comparison of the 1σ uncertainties of the estim...

Comparison of the 1σ uncertainties of the estimated planetary SED derived from the diago...

Philipp A. Huber et al, The Astronomical Journal 170 4

Estimated SED for the optimistic scenario witho...

Estimated SED for the optimistic scenario without data whitening (top) and with data whi...

Philipp A. Huber et al, The Astronomical Journal 170 4

Distribution of the test statistics, TED (left ...

Distribution of the test statistics, TED (left two plots) and TNP (right two plots), und...

Philipp A. Huber et al, The Astronomical Journal 170 4

Illustrative example of the correlation matrix ...

Illustrative example of the correlation matrix corresponding to the covariance matrix de...

Philipp A. Huber et al, The Astronomical Journal 170 4

Correlations between the estimated planetary SE...

Correlations between the estimated planetary SED and sky coordinates. The correlations g...

Philipp A. Huber et al, The Astronomical Journal 170 4

Correlation maps of the Earth-like planet aroun...

Correlation maps of the Earth-like planet around an M star for the ideal (left), optimis...

Philipp A. Huber et al, The Astronomical Journal 170 4

Additional examples of extracted planetary SEDs...

Additional examples of extracted planetary SEDs with corresponding uncertainties for the...

Philipp A. Huber et al, The Astronomical Journal 170 4

Channel maps of CO (J = 2–1). The upper panels ...

Channel maps of CO (J = 2–1). The upper panels cover ...

Hao-Min Sun et al, The Astronomical Journal 170 4

Continuum emission at 1.3 mm wavelengths. The s...

Continuum emission at 1.3 mm wavelengths. The synthesized beams shown in the lower-left ...

Hao-Min Sun et al, The Astronomical Journal 170 4

Flux density statistics of 13CO and CO moment 0...

Flux density statistics of 13CO and CO moment 0 map in different regions. Left panels: 1...

Hao-Min Sun et al, The Astronomical Journal 170 4

Integrated intensity maps of the CO (J = 2–1) l...

Integrated intensity maps of the CO (J = 2–1) line over two different velocity ranges. T...

Hao-Min Sun et al, The Astronomical Journal 170 4

Three-dimensional mesh geometry of the SHAPE mo...

Three-dimensional mesh geometry of the SHAPE model viewed from two orthogonal directions...

Hao-Min Sun et al, The Astronomical Journal 170 4

SED and two-component fitting of IRAS 06530–0213.

SED and two-component fitting of IRAS 06530–0213.

Hao-Min Sun et al, The Astronomical Journal 170 4

CO (J = 2–1) line profile and its isotopologue ...

CO (J = 2–1) line profile and its isotopologue line profiles detected in IRAS 06530–0213...

Hao-Min Sun et al, The Astronomical Journal 170 4

Same as lower panels of Figure 5, but for 13CO ...

Same as lower panels of Figure 5, but for 13CO J = 2−1.

Hao-Min Sun et al, The Astronomical Journal 170 4

UV coverage acquired by combining the 12A and 1...

UV coverage acquired by combining the 12A and 10D configurations.

Hao-Min Sun et al, The Astronomical Journal 170 4

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