adsabs/AstroCLIMB huggingface dataset:
Paper: Dynamical Origin for the Collinder 132–Gulliver 21 Stream: A Mixture of Three Comoving Populations with an Age Difference of 250 Myr
Authors: Xiaoying Pang, Yuqian Li, Shih-Yun Tang, Long Wang, Yanshu Wang, Zhao-Yu Li, Danchen Wang, M. B. N. Kouwenhoven, Mario Pasquato
Figure caption: 3D morphology of the Collinder 132–Gulliver 21 stream in Galactocentric Cartesian coordinates after distance correction via a Bayesian approach (Pang et al. 2021a). The black solid curve represents the Local Arm center, and the Local Arm edge is denoted as the black dotted curve. The position of the Sun is taken at (X, Y, Z) = (−8150, 0, 5.5) pc (Reid et al. 2019). The age of each subgroup is indicated in panel (b) to show that the oldest population is surrounded by young populations.
Paper: Dynamical Origin for the Collinder 132–Gulliver 21 Stream: A Mixture of Three Comoving Populations with an Age Difference of 250 Myr
Authors: Xiaoying Pang, Yuqian Li, Shih-Yun Tang, Long Wang, Yanshu Wang, Zhao-Yu Li, Danchen Wang, M. B. N. Kouwenhoven, Mario Pasquato
Figure caption: IRAS-IRIS infrared image of the 60 μm band (Miville-Deschênes & Lagache 2005). Members of the eight subgroups in the Collinder 132–Gulliver 21 stream are displayed as colored circles. The background bubble structure is apparent.
Paper: Sodium Distribution on the Moon
Authors: S. Narendranath, Netra S. Pillai, Srikar P. Tadepalli, Menelaos Sarantos, K. Vadodariya, A. Sarwade, Radhakrishna V, A. Tyagi
Figure caption: (a) Na wt% and (b) Mg wt% derived from CLASS data using Chandrayaan-2 XSM and GOES-16 XRS, which show consistency in the derived values.
Paper: Sodium Distribution on the Moon
Authors: S. Narendranath, Netra S. Pillai, Srikar P. Tadepalli, Menelaos Sarantos, K. Vadodariya, A. Sarwade, Radhakrishna V, A. Tyagi
Figure caption: Lunar X-ray spectra from a mare region (above) and a farside non-mare region (below) are shown with the nominal background on the nightside (summed over a month). Along with the major elements from O to Fe, Ti, a minor element in these regions, is also detected.
Paper: Sodium Distribution on the Moon
Authors: S. Narendranath, Netra S. Pillai, Srikar P. Tadepalli, Menelaos Sarantos, K. Vadodariya, A. Sarwade, Radhakrishna V, A. Tyagi
Figure caption: Lunar X-ray spectrum from a region in Mare Tranquillitatis showing the detection of minor elements Cr and Mn. The nominal background spectrum from the nightside (summed over a month) is also plotted.
Paper: Sodium Distribution on the Moon
Authors: S. Narendranath, Netra S. Pillai, Srikar P. Tadepalli, Menelaos Sarantos, K. Vadodariya, A. Sarwade, Radhakrishna V, A. Tyagi
Figure caption: Lunar X-ray spectrum triggered by solar flares of two different classes showing the better detection of the sodium line in the weaker flare (C class). The slope of the scattered continuum is steep (more low-energy photons compared to high-energy) and high at low energies for stronger flares because the Na-Kα line to continuum ratio is very low.
Paper: Sodium Distribution on the Moon
Authors: S. Narendranath, Netra S. Pillai, Srikar P. Tadepalli, Menelaos Sarantos, K. Vadodariya, A. Sarwade, Radhakrishna V, A. Tyagi
Figure caption: Spectral fits to lunar X-ray spectra showing two cases with and without sodium. Spectrum (a) shows the case when Na is detected and (b) where it is not. The deconvolved spectra are plotted in (c) and (d), showing the solar scattered component and XRF lines.
Paper: Sodium Distribution on the Moon
Authors: S. Narendranath, Netra S. Pillai, Srikar P. Tadepalli, Menelaos Sarantos, K. Vadodariya, A. Sarwade, Radhakrishna V, A. Tyagi
Figure caption: Sodium abundance in weight% overlaid on a LROC WAC global albedo map. Abundance increases toward higher latitudes for a given longitude.
Paper: A Low-inclination Neutral Trans-Neptunian Object in an Extreme Orbit
Authors: Ying-Tung Chen, 英同 陳, Marielle R. Eduardo, Marco A. Muñoz-Gutiérrez, Shiang-Yu Wang, 祥宇 王, Matthew J. Lehner, Chan-Kao Chang, 展誥 章
Figure caption: Left panel: gri colors of 2016 SD106, selected extreme TNOs, and objects from Sheppard (2010) and Sheppard (2012), which include most of the dynamically excited TNO populations. The colors of high-perihelion objects mentioned in Bannister et al. (2017) are indicated by triangles, and the solar color is indicated by the yellow star. The dashed lines roughly indicate the different color regions. Right panel: BVRI colors of 2016 SD106, the particularly neutral plutino 2004 EW95 (Perna et al. 2013), and plutinos, SDOs, and DOs from MBOSS (Hainaut et al. 2012). The BVRI color of 2016 SD106 was transformed from the original Sloan colors using the equations from Smith et al. (2002).
Paper: Sodium Distribution on the Moon
Authors: S. Narendranath, Netra S. Pillai, Srikar P. Tadepalli, Menelaos Sarantos, K. Vadodariya, A. Sarwade, Radhakrishna V, A. Tyagi
Figure caption: A two-component model (c) that consists of a regolith component and a surface adsorbate is fitted to the Na wt% data. The plot shows the variation of the Na/Mg XRF line flux ratio (a) with Na wt%, if the Na was only in the soil, and (b) with an adsorbate layer thickness if there is a component from a surface adsorbate layer as well. The red line in (c) is the best fit which gives an adsorbate component of 21%. The blue data points in (c) are not included in the fit and follow a trend of a higher fraction of adsorbate component.
Paper: Sodium Distribution on the Moon
Authors: S. Narendranath, Netra S. Pillai, Srikar P. Tadepalli, Menelaos Sarantos, K. Vadodariya, A. Sarwade, Radhakrishna V, A. Tyagi
Figure caption: Variation of Na with Al does not show any correlation similar to the trend in the returned soil samples. The CLASS pixel containing the Apollo-17 landing site is marked separately.
Paper: Sodium Distribution on the Moon
Authors: S. Narendranath, Netra S. Pillai, Srikar P. Tadepalli, Menelaos Sarantos, K. Vadodariya, A. Sarwade, Radhakrishna V, A. Tyagi
Figure caption: A histogram of the Na wt% is shown here. Ground pixels intersecting mare are colored in dark blue. There is no trend that suggests a different distribution in mare regions.
Paper: Sodium Distribution on the Moon
Authors: S. Narendranath, Netra S. Pillai, Srikar P. Tadepalli, Menelaos Sarantos, K. Vadodariya, A. Sarwade, Radhakrishna V, A. Tyagi
Figure caption: The global average of the latitudinal trend shows a north–south asymmetry.