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Band center positions of the 0.9 μm absorption ...

Band center positions of the 0.9 μm absorption feature as a function of grain size. Mete...

David C. Cantillo et al, The Planetary Science Journal 7 6

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VNIR spectra of the three distinct main belt E-...

VNIR spectra of the three distinct main belt E-type lithologies (B. E. Clark et al. 2004...

David C. Cantillo et al, The Planetary Science Journal 7 6

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The 9.0 μm Reststrahlen band (R. B.) maxima off...

The 9.0 μm Reststrahlen band (R. B.) maxima offset relative to each meteorite’s 45–90 μm...

David C. Cantillo et al, The Planetary Science Journal 7 6

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Bus–DeMeo principal component values for all ei...

Bus–DeMeo principal component values for all eight aubrite meteorites and their associat...

David C. Cantillo et al, The Planetary Science Journal 7 6

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Christiansen feature (C. F.) minima offset rela...

Christiansen feature (C. F.) minima offset relative to each individual meteorite’s 45–90...

David C. Cantillo et al, The Planetary Science Journal 7 6

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VNIR spectra of two end-member grain sizes of N...

VNIR spectra of two end-member grain sizes of Norton County (slab and <45 μm powder) plo...

David C. Cantillo et al, The Planetary Science Journal 7 6

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Spectral slope from 0.8 to 1.8 μm as a function...

Spectral slope from 0.8 to 1.8 μm as a function of grain size for our eight aubrite mete...

David C. Cantillo et al, The Planetary Science Journal 7 6

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R. B. contrast as a function of grain size for ...

R. B. contrast as a function of grain size for our eight aubrites. Finer <45 μm samples ...

David C. Cantillo et al, The Planetary Science Journal 7 6

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The telescopic spectrum of NEA 2023 DZ2 compare...

The telescopic spectrum of NEA 2023 DZ2 compared two selected grain sizes of Norton Coun...

David C. Cantillo et al, The Planetary Science Journal 7 6

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Absorption depth of the 0.9 μm low-iron pyroxen...

Absorption depth of the 0.9 μm low-iron pyroxene feature as a function of grain size for...

David C. Cantillo et al, The Planetary Science Journal 7 6

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Normalized reflectance of the seven grain size ...

Normalized reflectance of the seven grain size bins from our eight aubrite meteorites ac...

David C. Cantillo et al, The Planetary Science Journal 7 6

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Absolute reflectance of the seven grain size bi...

Absolute reflectance of the seven grain size bins from our eight aubrite meteorites acro...

David C. Cantillo et al, The Planetary Science Journal 7 6

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Absolute reflectance (top row) and normalized r...

Absolute reflectance (top row) and normalized reflectance (bottom row) of our eight aubr...

David C. Cantillo et al, The Planetary Science Journal 7 6

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Absorption depth of the 0.5 μm feature as a fun...

Absorption depth of the 0.5 μm feature as a function of grain size for our aubrite meteo...

David C. Cantillo et al, The Planetary Science Journal 7 6

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Absolute reflectance values at 0.55 μm (photome...

Absolute reflectance values at 0.55 μm (photometric (V) filter) plotted as a function of...

David C. Cantillo et al, The Planetary Science Journal 7 6

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Visual representation of the analysis of MIR fe...

Visual representation of the analysis of MIR features and spectral contrast for our aubr...

David C. Cantillo et al, The Planetary Science Journal 7 6

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VNIR spectra of the two Rantila grain size end-...

VNIR spectra of the two Rantila grain size end-members (slab and <45 μm) plotted against...

David C. Cantillo et al, The Planetary Science Journal 7 6

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Surface brightness estimates of the ICL at r = ...

Surface brightness estimates of the ICL at r = 100 kpc for 11 individual clusters (blue)...

Kailin Kang and Michael McDonald, Research Notes of the AAS 10 6

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All-sky density plot of the number of identifie...

All-sky density plot of the number of identified solar analogs within 7°.

Quanzhi Ye and 泉志叶, Research Notes of the AAS 10 6

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(a) TESS TPF of TOI-2155 (TIC 461591646) from S...

(a) TESS TPF of TOI-2155 (TIC 461591646) from Sector 60, illustrating the pixel-level fl...

Md Redyan Ahmed et al, The Astronomical Journal 172 1

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Position of TOI-2155 in the Teff–luminosity pla...

Position of TOI-2155 in the Teff–luminosity plane. The luminosity is derived from SED mo...

Md Redyan Ahmed et al, The Astronomical Journal 172 1

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(a) TESS phase-folded data (gray points) with A...

(a) TESS phase-folded data (gray points) with Allesfitter model (red curve), and binned ...

Md Redyan Ahmed et al, The Astronomical Journal 172 1

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SED of TOI-2155. Red symbols represent the obse...

SED of TOI-2155. Red symbols represent the observed photometric measurements, with horiz...

Md Redyan Ahmed et al, The Astronomical Journal 172 1

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Lomb–Scargle periodogram of the out-of-transit ...

Lomb–Scargle periodogram of the out-of-transit TESS light curve of TOI-2155 of sector 52...

Md Redyan Ahmed et al, The Astronomical Journal 172 1

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Data of TOI-2155 b from 13 TESS sectors. Panel ...

Data of TOI-2155 b from 13 TESS sectors. Panel (a) shows the detrended light curve from ...

Md Redyan Ahmed et al, The Astronomical Journal 172 1

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