adsabs/AstroCLIMB huggingface dataset:
Paper: Surface Conditions and Resource Accessibility at Potential Artemis Landing Sites 007 and 011
Authors: Nandita Kumari, Jordan M. Bretzfelder, Indujaa Ganesh, Antonio Lang, David A. Kring
Figure caption: Hillshade image of the two sites derived from a LOLA digital elevation model.
Paper: NaCl and KCl in Io’s Atmosphere
Authors: Erin Redwing, Imke de Pater, Statia Luszcz-Cook, Katherine de Kleer, Arielle Moullet, Patricio M. Rojo
Figure caption: All ALMA images used in this study. The top row is the NaCl lines, and the bottom row is the KCl lines. The middle columns are dates where NaCl and KCl were observed concurrently. In these images (as well as all images in this paper), Io north is up, the bottom left white circle is the HPBW of the synthesized beam (spatial resolution), the center white circle is the outline of the disk of Io taken from continuum maps of Io observed simultaneously, and the black circles are the apertures analyzed in this study. Identification of each aperture (i.e., apertures 1, 2, etc.) is summarized in Figures 12 and 13 in the Appendix. The rms error for each image, calculated from emission off Io’s disk, is noted in the bottom right corner of each image. The radius of the apertures was determined by the smaller axis of the HPBW for each image (see Table 2).
Paper: A Near-surface Temperature Model of Arrokoth
Authors: Orkan M. Umurhan, William M. Grundy, Michael K. Bird, Ross Beyer, James T. Keane, Ivan R. Linscott, Samuel Birch, Carver Bierson, Leslie A. Young, S. Alan Stern, Carey M. Lisse, Carly J. A. Howett, Silvia Protopapa, John R. Spencer, Richard P. Binzel, William B. McKinnon, Tod R. Lauer, Harold A. Weaver, Catherine B. Olkin, Kelsi N. Singer, Anne J. Verbiscer, Alex H. Parker
Figure caption: Predicted brightness temperatures T  b  for the CA08 observation. For input values of ﹩\varepsilon ^{\prime} \equiv \mathrm{Re}(\varepsilon )﹩ and 〈E eff〉 predicted T  b  shown as a function of ﹩\varepsilon ^{\prime\prime} \equiv \mathrm{Im}(\varepsilon )﹩ and ﹩{ \mathcal I }﹩: (left column) ﹩\varepsilon ^{\prime} =1.04﹩ and (right column) ﹩\varepsilon ^{\prime} =3.50﹩. Successive rows corresponding to decreasing values of 〈E eff〉. Black contours denote T  b  = 29 K, while the dotted black contours represent T  b  = 24 K and 34 K levels. The right column might be considered representative of pure methanol ice of zero porosity, while the left column could be the same with a porosity of 60%.
Paper: A Near-surface Temperature Model of Arrokoth
Authors: Orkan M. Umurhan, William M. Grundy, Michael K. Bird, Ross Beyer, James T. Keane, Ivan R. Linscott, Samuel Birch, Carver Bierson, Leslie A. Young, S. Alan Stern, Carey M. Lisse, Carly J. A. Howett, Silvia Protopapa, John R. Spencer, Richard P. Binzel, William B. McKinnon, Tod R. Lauer, Harold A. Weaver, Catherine B. Olkin, Kelsi N. Singer, Anne J. Verbiscer, Alex H. Parker
Figure caption: Histogram plots for various orbital-scale quantities. The model assumes ﹩{ \mathcal I }=2.54﹩ tiu, A = 0.06, and ε = 0.9. The vertical axis corresponds to the number of facets. The panels are (left panel) percent of body self-obscuration in reference to Figure 3, (middle left) orbitally averaged surface temperature T int,i , (middle right) orbitally averaged flux temperature T a,i , and (right) minimum surface temperature over the course of one orbit.
Paper: A Near-surface Temperature Model of Arrokoth
Authors: Orkan M. Umurhan, William M. Grundy, Michael K. Bird, Ross Beyer, James T. Keane, Ivan R. Linscott, Samuel Birch, Carver Bierson, Leslie A. Young, S. Alan Stern, Carey M. Lisse, Carly J. A. Howett, Silvia Protopapa, John R. Spencer, Richard P. Binzel, William B. McKinnon, Tod R. Lauer, Harold A. Weaver, Catherine B. Olkin, Kelsi N. Singer, Anne J. Verbiscer, Alex H. Parker
Figure caption: Four views of the absolute minimum surface temperature of each facet over the course of one orbit. The four views are in the same orientation as those shown in Figure 6. The range of temperatures is shown with arrows; see also Figure 12. Note the higher temperatures running within the equatorial zone and occasionally outlining the putative rims of cratered morphology lying in the tropical zone.
Paper: A Near-surface Temperature Model of Arrokoth
Authors: Orkan M. Umurhan, William M. Grundy, Michael K. Bird, Ross Beyer, James T. Keane, Ivan R. Linscott, Samuel Birch, Carver Bierson, Leslie A. Young, S. Alan Stern, Carey M. Lisse, Carly J. A. Howett, Silvia Protopapa, John R. Spencer, Richard P. Binzel, William B. McKinnon, Tod R. Lauer, Harold A. Weaver, Catherine B. Olkin, Kelsi N. Singer, Anne J. Verbiscer, Alex H. Parker
Figure caption: Four views of the full temperature variation over the course of one orbit ΔT  i . The four views are in the same orientation as those shown in Figure 6. The far upper-right graph shows a histogram of ΔT  i .
Paper: A Near-surface Temperature Model of Arrokoth
Authors: Orkan M. Umurhan, William M. Grundy, Michael K. Bird, Ross Beyer, James T. Keane, Ivan R. Linscott, Samuel Birch, Carver Bierson, Leslie A. Young, S. Alan Stern, Carey M. Lisse, Carly J. A. Howett, Silvia Protopapa, John R. Spencer, Richard P. Binzel, William B. McKinnon, Tod R. Lauer, Harold A. Weaver, Catherine B. Olkin, Kelsi N. Singer, Anne J. Verbiscer, Alex H. Parker
Figure caption: Value of ﹩{\varepsilon }_{c}^{{\prime\prime} }﹩ that yields T  b  = 29K during CA08 for 〈E eff〉 = 0.9 and 1.0. For these values of 〈E eff〉, this analysis predicts that the material is very nearly transparent in the X band (﹩{\varepsilon }_{c}^{{\prime\prime} }\lessapprox 0.002﹩) for ﹩1\ \mathrm{tiu}\ \lt { \mathcal I }\lt 40﹩ tiu.
Paper: A Near-surface Temperature Model of Arrokoth
Authors: Orkan M. Umurhan, William M. Grundy, Michael K. Bird, Ross Beyer, James T. Keane, Ivan R. Linscott, Samuel Birch, Carver Bierson, Leslie A. Young, S. Alan Stern, Carey M. Lisse, Carly J. A. Howett, Silvia Protopapa, John R. Spencer, Richard P. Binzel, William B. McKinnon, Tod R. Lauer, Harold A. Weaver, Catherine B. Olkin, Kelsi N. Singer, Anne J. Verbiscer, Alex H. Parker
Figure caption: Predicted brightness temperatures based on subsurface radiative transfer analysis for ﹩\left\langle {E}_{\mathrm{eff}}\right\rangle =1﹩. Several values of ﹩{ \mathcal I }﹩ shown. White contours denote several values of electric skin depth. Note the weak dependence on the ﹩\varepsilon ^{\prime} ﹩ (denoted in the graphs as Re (ε)).
Paper: A Near-surface Temperature Model of Arrokoth
Authors: Orkan M. Umurhan, William M. Grundy, Michael K. Bird, Ross Beyer, James T. Keane, Ivan R. Linscott, Samuel Birch, Carver Bierson, Leslie A. Young, S. Alan Stern, Carey M. Lisse, Carly J. A. Howett, Silvia Protopapa, John R. Spencer, Richard P. Binzel, William B. McKinnon, Tod R. Lauer, Harold A. Weaver, Catherine B. Olkin, Kelsi N. Singer, Anne J. Verbiscer, Alex H. Parker
Figure caption: Four views of the orbitally averaged surface temperature. The four views are in the same orientation as those shown in Figure 6. The range of temperatures is shown with arrows; see also Figure 12.
Paper: A Near-surface Temperature Model of Arrokoth
Authors: Orkan M. Umurhan, William M. Grundy, Michael K. Bird, Ross Beyer, James T. Keane, Ivan R. Linscott, Samuel Birch, Carver Bierson, Leslie A. Young, S. Alan Stern, Carey M. Lisse, Carly J. A. Howett, Silvia Protopapa, John R. Spencer, Richard P. Binzel, William B. McKinnon, Tod R. Lauer, Harold A. Weaver, Catherine B. Olkin, Kelsi N. Singer, Anne J. Verbiscer, Alex H. Parker
Figure caption: The disk-averaged “deep” temperature T deep as a function of ﹩{ \mathcal I }﹩, predicted for CA08.
Paper: A Near-surface Temperature Model of Arrokoth
Authors: Orkan M. Umurhan, William M. Grundy, Michael K. Bird, Ross Beyer, James T. Keane, Ivan R. Linscott, Samuel Birch, Carver Bierson, Leslie A. Young, S. Alan Stern, Carey M. Lisse, Carly J. A. Howett, Silvia Protopapa, John R. Spencer, Richard P. Binzel, William B. McKinnon, Tod R. Lauer, Harold A. Weaver, Catherine B. Olkin, Kelsi N. Singer, Anne J. Verbiscer, Alex H. Parker
Figure caption: Four views of the orbitally averaged flux temperature T a,i . The four views are the same orientation as those shown in Figure 6. The range of temperatures is shown with arrows; see also Figure 12.