adsabs/AstroCLIMB huggingface dataset:
Paper: CWISE J105512.11+544328.3: A Nearby Y Dwarf Spectroscopically Confirmed with Keck/NIRES
Authors: Grady Robbins, Aaron M. Meisner, Adam C. Schneider, Adam J. Burgasser, J. Davy Kirkpatrick, Jonathan Gagné, Chih-Chun Hsu, Leslie Moranta, Sarah Casewell, Federico Marocco, Roman Gerasimov, Jacqueline K. Faherty, Marc J. Kuchner, Dan Caselden, Michael C. Cushing, Sherelyn Alejandro
Figure caption: Keck/NIRES near-infrared spectrum of CWISE J105512.11+544328.3 (black) plotted against spectral standards: T7 (Burgasser et al. 2006), T8 (Burgasser et al. 2004), T9 (Cushing et al. 2011), Y0 (Cushing et al. 2011), and Y1 (Kirkpatrick et al. 2012).
Paper: CWISE J105512.11+544328.3: A Nearby Y Dwarf Spectroscopically Confirmed with Keck/NIRES
Authors: Grady Robbins, Aaron M. Meisner, Adam C. Schneider, Adam J. Burgasser, J. Davy Kirkpatrick, Jonathan Gagné, Chih-Chun Hsu, Leslie Moranta, Sarah Casewell, Federico Marocco, Roman Gerasimov, Jacqueline K. Faherty, Marc J. Kuchner, Dan Caselden, Michael C. Cushing, Sherelyn Alejandro
Figure caption: Spitzer ch1−ch2 color plotted against spectral type for the LTY dwarfs in Kirkpatrick et al. (2021), where the blue star is W1055+5443, the purple star is WISEA J153429.75−104303.3 (a.k.a. The Accident; Meisner et al. 2020; Kirkpatrick et al. 2021), the green star is WISEA J114156.67−332635.5, and the black star is Y dwarf WISE 0855−0714. Cases of objects with Spitzer limits rather than detections in ch1 and/or ch2 are excluded. See Section 3 for our spectral typing of W1055+5443.
Paper: CWISE J105512.11+544328.3: A Nearby Y Dwarf Spectroscopically Confirmed with Keck/NIRES
Authors: Grady Robbins, Aaron M. Meisner, Adam C. Schneider, Adam J. Burgasser, J. Davy Kirkpatrick, Jonathan Gagné, Chih-Chun Hsu, Leslie Moranta, Sarah Casewell, Federico Marocco, Roman Gerasimov, Jacqueline K. Faherty, Marc J. Kuchner, Dan Caselden, Michael C. Cushing, Sherelyn Alejandro
Figure caption: Eighteen T8 to Y2 dwarfs from Schneider et al. (2015) plotted with W1055+5443 (blue star). Left panel: Delorme et al. (2008) NH3-H index vs. spectral type. Right panel: Delorme et al. (2008) NH3-H index plotted against W  J  index. In both panels, spectral type defines each data point’s color and square symbols are spectral standards.
Paper: CWISE J105512.11+544328.3: A Nearby Y Dwarf Spectroscopically Confirmed with Keck/NIRES
Authors: Grady Robbins, Aaron M. Meisner, Adam C. Schneider, Adam J. Burgasser, J. Davy Kirkpatrick, Jonathan Gagné, Chih-Chun Hsu, Leslie Moranta, Sarah Casewell, Federico Marocco, Roman Gerasimov, Jacqueline K. Faherty, Marc J. Kuchner, Dan Caselden, Michael C. Cushing, Sherelyn Alejandro
Figure caption: Spitzer ch2 absolute magnitude (M ch2) plotted against Spitzer ch1−ch2 color for the LTY dwarfs in Kirkpatrick et al. (2021), where the blue star is W1055+5443, the purple star is WISEA J153429.75−104303.3 (a.k.a. The Accident), the green star is WISEA J114156.67−332635.5, and the black star is Y dwarf WISE 0855−0714. Cases of objects with Spitzer limits rather than detections in ch1 and/or ch2 are excluded, as are dwarfs without parallax measurements available.
Paper: CWISE J105512.11+544328.3: A Nearby Y Dwarf Spectroscopically Confirmed with Keck/NIRES
Authors: Grady Robbins, Aaron M. Meisner, Adam C. Schneider, Adam J. Burgasser, J. Davy Kirkpatrick, Jonathan Gagné, Chih-Chun Hsu, Leslie Moranta, Sarah Casewell, Federico Marocco, Roman Gerasimov, Jacqueline K. Faherty, Marc J. Kuchner, Dan Caselden, Michael C. Cushing, Sherelyn Alejandro
Figure caption: Keck/NIRES near-infrared spectrum for CWISE J105512.11+544328.3: original spectrum (gray) and 5 pixel smoothed spectrum (black). The spectrum is normalized to the J-band peak between 1.27 and 1.29 μm.(The data used to create this figure are available.)
Paper: Shadow Implications: What Does Measuring the Photon Ring Imply for Gravity?
Authors: Avery E. Broderick, Kiana Salehi, Boris Georgiev
Figure caption: Comparison of allowed range of N(r  γ ), ﹩N^{\prime} ({r}_{\gamma })﹩ for a shadow-size measurement with fractional uncertainty σ  R /R = 10% (gray band) and the curves by single-parameter modifications to the metric. Explicitly, those associated with various PN orders, J13 metric orders, MGBK metric orders for γ 1 and γ 4, and RZ metric with a 0 and a 1 varied, holding all other metric expansion parameters fixed at zero (the latter are degenerate with those of the MGBK                         γ 1,2 and γ 1,3 curves, and are otherwise hidden). Thin lines indicate values for which an event horizon does not exist (affecting only the PN expansion examples); the small open and filled points at which the curves terminate show when the photon orbit becomes infinite and degenerate with the event horizon, respectively. The large black point indicates the values corresponding to general relativity.
Paper: Shadow Implications: What Does Measuring the Photon Ring Imply for Gravity?
Authors: Avery E. Broderick, Kiana Salehi, Boris Georgiev
Figure caption: Comparison of allowed range of N(r  γ ), ﹩N^{\prime} ({r}_{\gamma })﹩ for a shadow-size measurement with σ  R /R = 10% (gray band) and the curves associated with the various spherically symmetric alternative spacetimes considered in Kocherlakota & Rezzolla (2020). The small open points at which the curves terminate show when the charge reaches an intrinsic limit, e.g., the solution no longer has an event horizon. The large black point indicates the values corresponding to general relativity.
Paper: Shadow Implications: What Does Measuring the Photon Ring Imply for Gravity?
Authors: Avery E. Broderick, Kiana Salehi, Boris Georgiev
Figure caption: Constraints on N(r  γ ), ﹩N^{\prime} ({r}_{\gamma })﹩, and N″(r  γ )/B 2(r  γ ) arising from the LIGO QNM constraints reported in Abbott et al. (2021). The magenta shaded region shows the 68% confidence region. Illustrative curves associated with the metric expansions in Figure 1 (blue) and alternative spacetimes in Figure 2 (orange) are shown. See Figure 1 for a description of line types.
Paper: Shadow Implications: What Does Measuring the Photon Ring Imply for Gravity?
Authors: Avery E. Broderick, Kiana Salehi, Boris Georgiev
Figure caption: Representative constraints implied by the shadow-size constraints for M87* (left) and Sgr A* (right) published by the EHT. Illustrative curves associated with the metric expansions in Figure 1 (blue) and alternative spacetimes in Figure 2 (orange) are shown. See Figure 1 for a description of line types. In both panels the relevant EHT measurements at 1σ and 2σ are shown by the green bands.