adsabs/AstroCLIMB huggingface dataset:
Paper: Discovery of a Nearby Habitable Zone Super-Earth Candidate Amenable to Direct Imaging
Authors: Corey Beard, Paul Robertson, Jack Lubin, Eric B. Ford, Suvrath Mahadevan, Gudmundur Stefansson, Jason T. Wright, Eric Wolf, Vincent Kofman, Vidya Venkatesan, Ravi Kopparapu, Roan Arendtsz, Rae Holcomb, Raquel A. Martinez, Stephanie Sallum, Jacob K. Luhn, Chad F. Bender, Cullen H. Blake, William D. Cochran, Megan Delamer, Scott A. Diddams, Michael Endl, Samuel Halverson, Shubham Kanodia, Daniel M. Krolikowski, Andrea S. J. Lin, Sarah E. Logsdon, Michael W. McElwain, Andrew Monson, Joe P. Ninan, Jayadev Rajagopal, Arpita Roy, Christian Schwab, Ryan C. Terrien
Figure caption: Linewidth, Hα, Ca IRT, KI, and dET activity indicators of GJ 251. CARMENES/NEID line widths show strong signals near the rotation period, 68/72 days, and at longer periods. IRT I, II, and III show significant powers near 130 days, likely the rotation period of GJ 251. Meanwhile, dET shows significant peaks near 40 and 60 days, likely the second and first harmonics of the rotation period. Significantly, 14 and 54 day signals never appear in the activity indicators, except in KI, though neither are the dominant signal nor significant in power. Signals of interest highlighted are at 14, 54, 68, 73, 120, and 130 days.
Paper: Discovery of a Nearby Habitable Zone Super-Earth Candidate Amenable to Direct Imaging
Authors: Corey Beard, Paul Robertson, Jack Lubin, Eric B. Ford, Suvrath Mahadevan, Gudmundur Stefansson, Jason T. Wright, Eric Wolf, Vincent Kofman, Vidya Venkatesan, Ravi Kopparapu, Roan Arendtsz, Rae Holcomb, Raquel A. Martinez, Stephanie Sallum, Jacob K. Luhn, Chad F. Bender, Cullen H. Blake, William D. Cochran, Megan Delamer, Scott A. Diddams, Michael Endl, Samuel Halverson, Shubham Kanodia, Daniel M. Krolikowski, Andrea S. J. Lin, Sarah E. Logsdon, Michael W. McElwain, Andrew Monson, Joe P. Ninan, Jayadev Rajagopal, Arpita Roy, Christian Schwab, Ryan C. Terrien
Figure caption: A BFP created using the Agatha software package (F. Feng et al. 2017). These periodograms use an MA red-noise model to more accurately identify coherent, periodic signals. The BFP first identifies a very significant signal at 14 days, planet b. It then identifies a significant signal at 53.6 days, our purported planet c. Next, it identifies a 73 day signal which we discuss in Section 6. The final plot identifies no additional significant signals. We designate a Bayes factor of 5 as the threshold for a significant signal (R. E. Kass & A. E. Raftery 1995). Signals of interest highlighted are at 14, 54, 68, 73, 120, and 130 days.
Paper: Discovery of a Nearby Habitable Zone Super-Earth Candidate Amenable to Direct Imaging
Authors: Corey Beard, Paul Robertson, Jack Lubin, Eric B. Ford, Suvrath Mahadevan, Gudmundur Stefansson, Jason T. Wright, Eric Wolf, Vincent Kofman, Vidya Venkatesan, Ravi Kopparapu, Roan Arendtsz, Rae Holcomb, Raquel A. Martinez, Stephanie Sallum, Jacob K. Luhn, Chad F. Bender, Cullen H. Blake, William D. Cochran, Megan Delamer, Scott A. Diddams, Michael Endl, Samuel Halverson, Shubham Kanodia, Daniel M. Krolikowski, Andrea S. J. Lin, Sarah E. Logsdon, Michael W. McElwain, Andrew Monson, Joe P. Ninan, Jayadev Rajagopal, Arpita Roy, Christian Schwab, Ryan C. Terrien
Figure caption: Pixel-by-pixel periodogram of the TESS photometry of GJ 251 during TESS Sector 20. Each plot corresponds to a pixel of the TESS CCD, and the solid blue line is the aperture used by the PDCSAP pipeline during the generation of the GJ 251 light curve. A gold star highlights the pixel that contains GJ 251. This plot can help us discover the source of the periodic variability seen in the GJ 251 light curve. It is clear that the ∼4 hr periodicity originates not from GJ 251 but from other, neighboring pixels, which we highlight in red. Consequently, we can rule out the signal as fast rotation of GJ 251.
Paper: Discovery of a Nearby Habitable Zone Super-Earth Candidate Amenable to Direct Imaging
Authors: Corey Beard, Paul Robertson, Jack Lubin, Eric B. Ford, Suvrath Mahadevan, Gudmundur Stefansson, Jason T. Wright, Eric Wolf, Vincent Kofman, Vidya Venkatesan, Ravi Kopparapu, Roan Arendtsz, Rae Holcomb, Raquel A. Martinez, Stephanie Sallum, Jacob K. Luhn, Chad F. Bender, Cullen H. Blake, William D. Cochran, Megan Delamer, Scott A. Diddams, Michael Endl, Samuel Halverson, Shubham Kanodia, Daniel M. Krolikowski, Andrea S. J. Lin, Sarah E. Logsdon, Michael W. McElwain, Andrew Monson, Joe P. Ninan, Jayadev Rajagopal, Arpita Roy, Christian Schwab, Ryan C. Terrien
Figure caption: A closer look at the chromatic GP used in our white NEID fits for a particularly dense region of RVs. The solid lines indicate the GP + two-planet model. Unlike most other GP models, which typically calculate a covariance matrix for each instrument separately, and later combine the likelihoods, the Chromatic kernels for B. L. Cale et al. (2021) calculate covariances across instruments. This relationship is most clear when examining the different predictions from each instrument: they follow the same periodic structure, with deviations mostly due to different amplitudes. It is also notable that the bluer instruments are consistently larger in amplitude, while the redder instruments have smaller GP amplitudes.
Paper: Discovery of a Nearby Habitable Zone Super-Earth Candidate Amenable to Direct Imaging
Authors: Corey Beard, Paul Robertson, Jack Lubin, Eric B. Ford, Suvrath Mahadevan, Gudmundur Stefansson, Jason T. Wright, Eric Wolf, Vincent Kofman, Vidya Venkatesan, Ravi Kopparapu, Roan Arendtsz, Rae Holcomb, Raquel A. Martinez, Stephanie Sallum, Jacob K. Luhn, Chad F. Bender, Cullen H. Blake, William D. Cochran, Megan Delamer, Scott A. Diddams, Michael Endl, Samuel Halverson, Shubham Kanodia, Daniel M. Krolikowski, Andrea S. J. Lin, Sarah E. Logsdon, Michael W. McElwain, Andrew Monson, Joe P. Ninan, Jayadev Rajagopal, Arpita Roy, Christian Schwab, Ryan C. Terrien
Figure caption: Short cadence photometry of GJ 251 taken by TESS during sectors 20, 45, 47, 60, 71, and 72. Overlaid is the transit ephemeris of GJ 251 b and c as determined from our RV fits. Sectors 71 and 72 strongly suggest that GJ 251 b does not transit. GJ 251 c, with its 54 days period and less precise ephemeris, is difficult to constrain with short-baseline TESS photometry. One predicted transit time does fall into Sector 20 photometry, though the uncertainty is so large as to be fairly uninformative. We detect no transits in the TESS photometry of GJ 251.
Paper: Discovery of a Nearby Habitable Zone Super-Earth Candidate Amenable to Direct Imaging
Authors: Corey Beard, Paul Robertson, Jack Lubin, Eric B. Ford, Suvrath Mahadevan, Gudmundur Stefansson, Jason T. Wright, Eric Wolf, Vincent Kofman, Vidya Venkatesan, Ravi Kopparapu, Roan Arendtsz, Rae Holcomb, Raquel A. Martinez, Stephanie Sallum, Jacob K. Luhn, Chad F. Bender, Cullen H. Blake, William D. Cochran, Megan Delamer, Scott A. Diddams, Michael Endl, Samuel Halverson, Shubham Kanodia, Daniel M. Krolikowski, Andrea S. J. Lin, Sarah E. Logsdon, Michael W. McElwain, Andrew Monson, Joe P. Ninan, Jayadev Rajagopal, Arpita Roy, Christian Schwab, Ryan C. Terrien
Figure caption: GLS periodograms of GJ 251 RV data as we sequentially remove the most prominent signals. Black plots include white NEID data, while red plots include red NEID data. GJ 251 b is the most significant by far at first, but its subtraction reveals several other prominent signals. Eventually, subtracting signals only adds noise to the periodograms, so we cease our analysis. False alarm probabilities are estimated using methods in P. A. Sturrock & J. D. Scargle (2010). Signals of interest highlighted are at 14, 54, 68, 73, 120, and 130 days.
Paper: Discovery of a Nearby Habitable Zone Super-Earth Candidate Amenable to Direct Imaging
Authors: Corey Beard, Paul Robertson, Jack Lubin, Eric B. Ford, Suvrath Mahadevan, Gudmundur Stefansson, Jason T. Wright, Eric Wolf, Vincent Kofman, Vidya Venkatesan, Ravi Kopparapu, Roan Arendtsz, Rae Holcomb, Raquel A. Martinez, Stephanie Sallum, Jacob K. Luhn, Chad F. Bender, Cullen H. Blake, William D. Cochran, Megan Delamer, Scott A. Diddams, Michael Endl, Samuel Halverson, Shubham Kanodia, Daniel M. Krolikowski, Andrea S. J. Lin, Sarah E. Logsdon, Michael W. McElwain, Andrew Monson, Joe P. Ninan, Jayadev Rajagopal, Arpita Roy, Christian Schwab, Ryan C. Terrien
Figure caption: Top: RV time series of GJ 251, with GP + two-planet model overlaid for each instrument. Middle: Residuals to a GP + two-planet model. Bottom: RVs folded to the phase of GJ 251 b and c.(The data used to create this figure are available in the online article.)(The data used to create this figure are available.)
Paper: Discovery of a Nearby Habitable Zone Super-Earth Candidate Amenable to Direct Imaging
Authors: Corey Beard, Paul Robertson, Jack Lubin, Eric B. Ford, Suvrath Mahadevan, Gudmundur Stefansson, Jason T. Wright, Eric Wolf, Vincent Kofman, Vidya Venkatesan, Ravi Kopparapu, Roan Arendtsz, Rae Holcomb, Raquel A. Martinez, Stephanie Sallum, Jacob K. Luhn, Chad F. Bender, Cullen H. Blake, William D. Cochran, Megan Delamer, Scott A. Diddams, Michael Endl, Samuel Halverson, Shubham Kanodia, Daniel M. Krolikowski, Andrea S. J. Lin, Sarah E. Logsdon, Michael W. McElwain, Andrew Monson, Joe P. Ninan, Jayadev Rajagopal, Arpita Roy, Christian Schwab, Ryan C. Terrien
Figure caption: The posterior values for Kc, Pc, and Tc, and their uncertainties, are shown from top to bottom. Fits divided by instrument on the left, and divided by observing region on the right. A gray bar highlights the posterior value of our best all-data fit and its 1σ confidence interval.
Paper: Discovery of a Nearby Habitable Zone Super-Earth Candidate Amenable to Direct Imaging
Authors: Corey Beard, Paul Robertson, Jack Lubin, Eric B. Ford, Suvrath Mahadevan, Gudmundur Stefansson, Jason T. Wright, Eric Wolf, Vincent Kofman, Vidya Venkatesan, Ravi Kopparapu, Roan Arendtsz, Rae Holcomb, Raquel A. Martinez, Stephanie Sallum, Jacob K. Luhn, Chad F. Bender, Cullen H. Blake, William D. Cochran, Megan Delamer, Scott A. Diddams, Michael Endl, Samuel Halverson, Shubham Kanodia, Daniel M. Krolikowski, Andrea S. J. Lin, Sarah E. Logsdon, Michael W. McElwain, Andrew Monson, Joe P. Ninan, Jayadev Rajagopal, Arpita Roy, Christian Schwab, Ryan C. Terrien
Figure caption: Two histograms highlighting the results of model comparisons on simulated data sets. After generating 200 fake one-planet and 200 fake two-planet data sets, we performed nested sampling fits for one- and two-planet models, and computed the difference in BF. When the fake data include only one injected planet, it is very rare that a two-planet model is preferred. On the other hand, when the generated data include two injected planets, a two-planet model is often preferred, with the BF in the real data falling on the center of this distribution.
Paper: Discovery of a Nearby Habitable Zone Super-Earth Candidate Amenable to Direct Imaging
Authors: Corey Beard, Paul Robertson, Jack Lubin, Eric B. Ford, Suvrath Mahadevan, Gudmundur Stefansson, Jason T. Wright, Eric Wolf, Vincent Kofman, Vidya Venkatesan, Ravi Kopparapu, Roan Arendtsz, Rae Holcomb, Raquel A. Martinez, Stephanie Sallum, Jacob K. Luhn, Chad F. Bender, Cullen H. Blake, William D. Cochran, Megan Delamer, Scott A. Diddams, Michael Endl, Samuel Halverson, Shubham Kanodia, Daniel M. Krolikowski, Andrea S. J. Lin, Sarah E. Logsdon, Michael W. McElwain, Andrew Monson, Joe P. Ninan, Jayadev Rajagopal, Arpita Roy, Christian Schwab, Ryan C. Terrien
Figure caption: Time series of RVs for GJ 251, showing how we divided observing “regions” to test the consistency of the candidate planet parameters. We mostly try to divide into observing seasons (R3, R4, R5, R6), though R1, R2, and R7 encompass multiple years of observing due to lower cadence.
Paper: Discovery of a Nearby Habitable Zone Super-Earth Candidate Amenable to Direct Imaging
Authors: Corey Beard, Paul Robertson, Jack Lubin, Eric B. Ford, Suvrath Mahadevan, Gudmundur Stefansson, Jason T. Wright, Eric Wolf, Vincent Kofman, Vidya Venkatesan, Ravi Kopparapu, Roan Arendtsz, Rae Holcomb, Raquel A. Martinez, Stephanie Sallum, Jacob K. Luhn, Chad F. Bender, Cullen H. Blake, William D. Cochran, Megan Delamer, Scott A. Diddams, Michael Endl, Samuel Halverson, Shubham Kanodia, Daniel M. Krolikowski, Andrea S. J. Lin, Sarah E. Logsdon, Michael W. McElwain, Andrew Monson, Joe P. Ninan, Jayadev Rajagopal, Arpita Roy, Christian Schwab, Ryan C. Terrien
Figure caption: Angular separation of the HZ for the closest stars to Earth that have known HZ planets. The conservative inner and outer edges of the system’s HZ are plotted and connected by a gray line. Points are color-coded by stellar effective temperature. Planets that might be terrestrial are highlighted with green diamonds, while gas-dominant planets are marked with an x. We separate these populations at a minimum mass of 5 M⊕ because planets with greater mass become increasingly unlikely to remain terrestrial. We further include a plausible end-goal IWA for next generation 30 meter class telescopes and a curve showing the angle at which a 2 R⊕ planet would be visible at 10−8 contrast with an albedo of 0.5. This curve actually corresponds to a particular physical separation, which correspondingly translates into smaller angular separations for systems further from Earth. The region where both conditions are met is highlighted in green.
Paper: Discovery of a Nearby Habitable Zone Super-Earth Candidate Amenable to Direct Imaging
Authors: Corey Beard, Paul Robertson, Jack Lubin, Eric B. Ford, Suvrath Mahadevan, Gudmundur Stefansson, Jason T. Wright, Eric Wolf, Vincent Kofman, Vidya Venkatesan, Ravi Kopparapu, Roan Arendtsz, Rae Holcomb, Raquel A. Martinez, Stephanie Sallum, Jacob K. Luhn, Chad F. Bender, Cullen H. Blake, William D. Cochran, Megan Delamer, Scott A. Diddams, Michael Endl, Samuel Halverson, Shubham Kanodia, Daniel M. Krolikowski, Andrea S. J. Lin, Sarah E. Logsdon, Michael W. McElwain, Andrew Monson, Joe P. Ninan, Jayadev Rajagopal, Arpita Roy, Christian Schwab, Ryan C. Terrien
Figure caption: Window function of our data for each instrument. Only a periodicity near 30 days, most likely a lunar cycle, seems to be caused by our sampling.
Paper: Discovery of a Nearby Habitable Zone Super-Earth Candidate Amenable to Direct Imaging
Authors: Corey Beard, Paul Robertson, Jack Lubin, Eric B. Ford, Suvrath Mahadevan, Gudmundur Stefansson, Jason T. Wright, Eric Wolf, Vincent Kofman, Vidya Venkatesan, Ravi Kopparapu, Roan Arendtsz, Rae Holcomb, Raquel A. Martinez, Stephanie Sallum, Jacob K. Luhn, Chad F. Bender, Cullen H. Blake, William D. Cochran, Megan Delamer, Scott A. Diddams, Michael Endl, Samuel Halverson, Shubham Kanodia, Daniel M. Krolikowski, Andrea S. J. Lin, Sarah E. Logsdon, Michael W. McElwain, Andrew Monson, Joe P. Ninan, Jayadev Rajagopal, Arpita Roy, Christian Schwab, Ryan C. Terrien
Figure caption: Top panel: Visual representations of the four different climate states simulated for this study, with illuminated portions correlating with albedo. For these cases, the host star’s spectrum was set to a 5770 K blackbody to correspond to the Sun for the purpose of visual interpretation of the atmospheres. Bottom panel: Contrasts of the different atmospheres as a function of wavelength.
Paper: Discovery of a Nearby Habitable Zone Super-Earth Candidate Amenable to Direct Imaging
Authors: Corey Beard, Paul Robertson, Jack Lubin, Eric B. Ford, Suvrath Mahadevan, Gudmundur Stefansson, Jason T. Wright, Eric Wolf, Vincent Kofman, Vidya Venkatesan, Ravi Kopparapu, Roan Arendtsz, Rae Holcomb, Raquel A. Martinez, Stephanie Sallum, Jacob K. Luhn, Chad F. Bender, Cullen H. Blake, William D. Cochran, Megan Delamer, Scott A. Diddams, Michael Endl, Samuel Halverson, Shubham Kanodia, Daniel M. Krolikowski, Andrea S. J. Lin, Sarah E. Logsdon, Michael W. McElwain, Andrew Monson, Joe P. Ninan, Jayadev Rajagopal, Arpita Roy, Christian Schwab, Ryan C. Terrien
Figure caption: RV plot of our best Red NEID fit.(The data used to create this figure are available in the online article.)(The data used to create this figure are available.)
Paper: Discovery of a Nearby Habitable Zone Super-Earth Candidate Amenable to Direct Imaging
Authors: Corey Beard, Paul Robertson, Jack Lubin, Eric B. Ford, Suvrath Mahadevan, Gudmundur Stefansson, Jason T. Wright, Eric Wolf, Vincent Kofman, Vidya Venkatesan, Ravi Kopparapu, Roan Arendtsz, Rae Holcomb, Raquel A. Martinez, Stephanie Sallum, Jacob K. Luhn, Chad F. Bender, Cullen H. Blake, William D. Cochran, Megan Delamer, Scott A. Diddams, Michael Endl, Samuel Halverson, Shubham Kanodia, Daniel M. Krolikowski, Andrea S. J. Lin, Sarah E. Logsdon, Michael W. McElwain, Andrew Monson, Joe P. Ninan, Jayadev Rajagopal, Arpita Roy, Christian Schwab, Ryan C. Terrien
Figure caption: A variety of possible contrast limits for the TMT PSI are plotted as solid, dashed, and dotted lines. Calculated contrasts for GJ 251 c are shown for a variety of planet radius and albedo values. GJ 251 c will test the limitations of PSI, but there are a number of scenarios where its direct imaging will be possible.
Paper: Discovery of a Nearby Habitable Zone Super-Earth Candidate Amenable to Direct Imaging
Authors: Corey Beard, Paul Robertson, Jack Lubin, Eric B. Ford, Suvrath Mahadevan, Gudmundur Stefansson, Jason T. Wright, Eric Wolf, Vincent Kofman, Vidya Venkatesan, Ravi Kopparapu, Roan Arendtsz, Rae Holcomb, Raquel A. Martinez, Stephanie Sallum, Jacob K. Luhn, Chad F. Bender, Cullen H. Blake, William D. Cochran, Megan Delamer, Scott A. Diddams, Michael Endl, Samuel Halverson, Shubham Kanodia, Daniel M. Krolikowski, Andrea S. J. Lin, Sarah E. Logsdon, Michael W. McElwain, Andrew Monson, Joe P. Ninan, Jayadev Rajagopal, Arpita Roy, Christian Schwab, Ryan C. Terrien
Figure caption: The size of GJ 251 and the orbits of GJ 251 b and c. Stellar size and orbital distances are to scale. In light green, we show the optimistic HZ, and in dark green, the conservative HZ (R. K. Kopparapu et al. 2013, 2014). GJ 251 c orbits directly in a regime where liquid water might be able to exist on its surface.
Paper: Discovery of a Nearby Habitable Zone Super-Earth Candidate Amenable to Direct Imaging
Authors: Corey Beard, Paul Robertson, Jack Lubin, Eric B. Ford, Suvrath Mahadevan, Gudmundur Stefansson, Jason T. Wright, Eric Wolf, Vincent Kofman, Vidya Venkatesan, Ravi Kopparapu, Roan Arendtsz, Rae Holcomb, Raquel A. Martinez, Stephanie Sallum, Jacob K. Luhn, Chad F. Bender, Cullen H. Blake, William D. Cochran, Megan Delamer, Scott A. Diddams, Michael Endl, Samuel Halverson, Shubham Kanodia, Daniel M. Krolikowski, Andrea S. J. Lin, Sarah E. Logsdon, Michael W. McElwain, Andrew Monson, Joe P. Ninan, Jayadev Rajagopal, Arpita Roy, Christian Schwab, Ryan C. Terrien
Figure caption: We show a corner plot of our best fit posteriors. Results are generally well behaved and normally distributed.
Paper: High Proper Motion Discoveries from the UKIRT Hemisphere Survey
Authors: Wings Zhang, Adam C. Schneider, Thomas P. Bickle, Adam J. Burgasser, Emma Softich, Federico Marocco, Daniella Bardalez Gagliuffi, Jacqueline K. Faherty, Aaron M. Meisner, J. Davy Kirkpatrick, Marc J. Kuchner, Martin Kabatnik, Frank Kiwy, Arttu Sainio, Jörg Schümann, Karl Selg-Mann, Nikolaj Stevnbak Andersen, Bruce Baller, Paul Beaulieu, John Bell, Dan Caselden, Guillaume Colin, Alexandru Dereveanco, Christoph Frank, Konstantin Glebov, Léopold Gramaize, Leslie K. Hamlet, David W. Martin, William Pendrill, Stéphane Perlin, Andres Stenner, Christopher Tanner, Melina Thévenot, Vinod Thakur
Figure caption: Color–magnitude diagram comparing the newly discovered high proper motion objects (red) with those from the Gaia Catalog of Nearby Stars (GCNS; gray). Also shown are the median subdwarf colors for sdM0 through sdM9 spectral types (black diamonds) as described in 4.3. The two objects with spectra, as shown in 5, are highlighted with a blue or green star.
Paper: High Proper Motion Discoveries from the UKIRT Hemisphere Survey
Authors: Wings Zhang, Adam C. Schneider, Thomas P. Bickle, Adam J. Burgasser, Emma Softich, Federico Marocco, Daniella Bardalez Gagliuffi, Jacqueline K. Faherty, Aaron M. Meisner, J. Davy Kirkpatrick, Marc J. Kuchner, Martin Kabatnik, Frank Kiwy, Arttu Sainio, Jörg Schümann, Karl Selg-Mann, Nikolaj Stevnbak Andersen, Bruce Baller, Paul Beaulieu, John Bell, Dan Caselden, Guillaume Colin, Alexandru Dereveanco, Christoph Frank, Konstantin Glebov, Léopold Gramaize, Leslie K. Hamlet, David W. Martin, William Pendrill, Stéphane Perlin, Andres Stenner, Christopher Tanner, Melina Thévenot, Vinod Thakur
Figure caption: Lick/KAST spectra (black) of J1803+1516 (top) and UHS J1855+4054 (bottom). The best fitting spectral standards from J. J. Bochanski et al. (2007) and/or S. Lépine et al. (2007) are shown as colored lines and labeled in each panel. All spectra are normalized at 7500 Å.
Paper: High Proper Motion Discoveries from the UKIRT Hemisphere Survey
Authors: Wings Zhang, Adam C. Schneider, Thomas P. Bickle, Adam J. Burgasser, Emma Softich, Federico Marocco, Daniella Bardalez Gagliuffi, Jacqueline K. Faherty, Aaron M. Meisner, J. Davy Kirkpatrick, Marc J. Kuchner, Martin Kabatnik, Frank Kiwy, Arttu Sainio, Jörg Schümann, Karl Selg-Mann, Nikolaj Stevnbak Andersen, Bruce Baller, Paul Beaulieu, John Bell, Dan Caselden, Guillaume Colin, Alexandru Dereveanco, Christoph Frank, Konstantin Glebov, Léopold Gramaize, Leslie K. Hamlet, David W. Martin, William Pendrill, Stéphane Perlin, Andres Stenner, Christopher Tanner, Melina Thévenot, Vinod Thakur
Figure caption: Example finder chart of a new high proper motion discovery identified in this work. The circles in the left three panels indicate the measured J-band position (blue), H-band position (green), and K-band position (red). Note the red color in the Pan-STARRS image, indicating a very red optical color and therefore a likely cold effective temperature.
Paper: High Proper Motion Discoveries from the UKIRT Hemisphere Survey
Authors: Wings Zhang, Adam C. Schneider, Thomas P. Bickle, Adam J. Burgasser, Emma Softich, Federico Marocco, Daniella Bardalez Gagliuffi, Jacqueline K. Faherty, Aaron M. Meisner, J. Davy Kirkpatrick, Marc J. Kuchner, Martin Kabatnik, Frank Kiwy, Arttu Sainio, Jörg Schümann, Karl Selg-Mann, Nikolaj Stevnbak Andersen, Bruce Baller, Paul Beaulieu, John Bell, Dan Caselden, Guillaume Colin, Alexandru Dereveanco, Christoph Frank, Konstantin Glebov, Léopold Gramaize, Leslie K. Hamlet, David W. Martin, William Pendrill, Stéphane Perlin, Andres Stenner, Christopher Tanner, Melina Thévenot, Vinod Thakur
Figure caption: A comparison of the measured proper motion components from UHS DR3 and Gaia DR3. The solid black line indicates a ratio of unity.
Paper: High Proper Motion Discoveries from the UKIRT Hemisphere Survey
Authors: Wings Zhang, Adam C. Schneider, Thomas P. Bickle, Adam J. Burgasser, Emma Softich, Federico Marocco, Daniella Bardalez Gagliuffi, Jacqueline K. Faherty, Aaron M. Meisner, J. Davy Kirkpatrick, Marc J. Kuchner, Martin Kabatnik, Frank Kiwy, Arttu Sainio, Jörg Schümann, Karl Selg-Mann, Nikolaj Stevnbak Andersen, Bruce Baller, Paul Beaulieu, John Bell, Dan Caselden, Guillaume Colin, Alexandru Dereveanco, Christoph Frank, Konstantin Glebov, Léopold Gramaize, Leslie K. Hamlet, David W. Martin, William Pendrill, Stéphane Perlin, Andres Stenner, Christopher Tanner, Melina Thévenot, Vinod Thakur
Figure caption: Reduced proper motion diagram comparing the non-Gaia discoveries from this work to the sample of known L and T dwarfs within the UHS survey from A. C. Schneider et al. (2023).