adsabs/AstroCLIMB huggingface dataset:
Paper: The Disks In Scorpius–Centaurus Survey (DISCS). I. Four Newly Resolved Debris Disks in Polarized Intensity Light
Authors: Justin Hom, Thomas M. Esposito, Katie A. Crotts, Gaspard Duchêne, Jennifer Patience, Johan Mazoyer, Robert J. De Rosa, Christine H. Chen, Paul Kalas, Bruce Macintosh, Brenda C. Matthews
Figure caption: Ansae flux ratio measurements of Sco-Cen debris disk targets as a function of 1.24 mm continuum emission from J. Lieman-Sifry et al. (2016; or 1.33 mm continuum emission in triangular points, from A. Moór et al. 2017 and A. J. Fehr et al. 2022) normalized by system distance, with color indicating logLIR/L*. The solid line represents the median likelihood result with 1σ uncertainties from linear bootstrap fitting (gray lines) of Sco-Cen systems. Ansae flux ratio increases slowly as a function of continuum emission at a lower rate than the IR excess, but there is large scatter in the measurements. The HD 109832 measurement is an upper limit and is not included in the bootstrapping fit. The 1.33 mm continuum measurements of non-Sco-Cen systems are also plotted as squares, showing an offset similar to Figure 7. Non-Sco-Cen measurement references: A. Bayo et al. (2019), G. M. Kennedy et al. (2018), M. A. MacGregor et al. (2013), M. A. MacGregor et al. (2018), L. Matrà et al. (2019b).
Paper: The Disks In Scorpius–Centaurus Survey (DISCS). I. Four Newly Resolved Debris Disks in Polarized Intensity Light
Authors: Justin Hom, Thomas M. Esposito, Katie A. Crotts, Gaspard Duchêne, Jennifer Patience, Johan Mazoyer, Robert J. De Rosa, Christine H. Chen, Paul Kalas, Bruce Macintosh, Brenda C. Matthews
Figure caption: Fans/F* (left) and IR excess (right) as a function of host star Teff. The two dashed lines in the left panel represent the median likelihood line parameters with 1σ uncertainties from separate linear bootstrapping fits (in light blue and red). No correlation appears present between Teff and LIR/L*, but a positive correlation is seen between Teff and Fans/F* for non-Sco-Cen systems. Curiously, the division between Sco-Cen and non-Sco-Cen systems is even more apparent, with a negative correlation for Sco-Cen targets compared to the rest of the GPI debris disk sample.
Paper: The Disks In Scorpius–Centaurus Survey (DISCS). I. Four Newly Resolved Debris Disks in Polarized Intensity Light
Authors: Justin Hom, Thomas M. Esposito, Katie A. Crotts, Gaspard Duchêne, Jennifer Patience, Johan Mazoyer, Robert J. De Rosa, Christine H. Chen, Paul Kalas, Bruce Macintosh, Brenda C. Matthews
Figure caption: Fans/F* as a function of SCO (normalized by distance). The systems highlighted in this work (HD 98363, HD 109832, HD 112810, and HD 146181) do not have confirmed detections of gas. The only systems with confirmed CO gas detections are β Pic, CE Ant, HD 32297, HD 110058, HD 131835, HD 146897, and HD 156623, with all other measurements being 3σ upper limits. Due to the small sample size, it is difficult to extrapolate on how Fans/F* may correlate with the presence of gas. While a negative trend appears among the detected sample, the upper limits for other systems complicate this observation.
Paper: The Disks In Scorpius–Centaurus Survey (DISCS). I. Four Newly Resolved Debris Disks in Polarized Intensity Light
Authors: Justin Hom, Thomas M. Esposito, Katie A. Crotts, Gaspard Duchêne, Jennifer Patience, Johan Mazoyer, Robert J. De Rosa, Christine H. Chen, Paul Kalas, Bruce Macintosh, Brenda C. Matthews
Figure caption: Fans/F* as a function of system inclination and LIR/L*. Similar ranges in inclination are observed between both the Sco-Cen and non-Sco-Cen samples, also indicated by the K-S test p-value. Overall, this suggests that inclination and limb brightening are not significant factors in accentuating the differences in Fans/F* between Sco-Cen and non-Sco-Cen objects.
Paper: The Disks In Scorpius–Centaurus Survey (DISCS). I. Four Newly Resolved Debris Disks in Polarized Intensity Light
Authors: Justin Hom, Thomas M. Esposito, Katie A. Crotts, Gaspard Duchêne, Jennifer Patience, Johan Mazoyer, Robert J. De Rosa, Christine H. Chen, Paul Kalas, Bruce Macintosh, Brenda C. Matthews
Figure caption: Total intensity images of all sample targets, in surface brightness units of mJy arcsec−2. The HD 98363 image was produced using LOCI, while all other target images were produced using KLIP. As marked by the white arrows, all polarized-intensity-detected systems have some level of detection in total intensity, with HD 109832 providing the clearest, highest-SNR detection. As the images were processed with ADI, surface brightness is underestimated owing to self-subtraction (J. Milli et al. 2012). HD 108904, HD 113556, and HD 119718 show bright candidate companions, with the candidates identified in HD 108904 and HD 113556 confirmed to be background sources (see Appendix A).
Paper: The Disks In Scorpius–Centaurus Survey (DISCS). I. Four Newly Resolved Debris Disks in Polarized Intensity Light
Authors: Justin Hom, Thomas M. Esposito, Katie A. Crotts, Gaspard Duchêne, Jennifer Patience, Johan Mazoyer, Robert J. De Rosa, Christine H. Chen, Paul Kalas, Bruce Macintosh, Brenda C. Matthews
Figure caption: Best-fitting ellipse models for the spine-fitting analysis of all four detected systems overlaid on the disk images. Geometric asymmetries appear present to some degree in all systems, with the strongest asymmetries apparent in HD 98363 and HD 109832.
Paper: The Disks In Scorpius–Centaurus Survey (DISCS). I. Four Newly Resolved Debris Disks in Polarized Intensity Light
Authors: Justin Hom, Thomas M. Esposito, Katie A. Crotts, Gaspard Duchêne, Jennifer Patience, Johan Mazoyer, Robert J. De Rosa, Christine H. Chen, Paul Kalas, Bruce Macintosh, Brenda C. Matthews
Figure caption: Measured surface brightness profiles for all four detected systems.
Paper: The Disks In Scorpius–Centaurus Survey (DISCS). I. Four Newly Resolved Debris Disks in Polarized Intensity Light
Authors: Justin Hom, Thomas M. Esposito, Katie A. Crotts, Gaspard Duchêne, Jennifer Patience, Johan Mazoyer, Robert J. De Rosa, Christine H. Chen, Paul Kalas, Bruce Macintosh, Brenda C. Matthews
Figure caption: 5σ contrast measurements in ΔH magnitudes for all targets, calibrated against self-subtraction.
Paper: The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems
Authors: Mark R. Giovinazzi, Cullen H. Blake, Paul Robertson, Andrea S. J. Lin, Arvind F. Gupta, Suvrath Mahadevan, Jason T. Wright, Daniella Bardalez Gagliuffi, Jiayin Dong, Rachel B. Fernandes, Evan Fitzmaurice, Samuel Halverson, Shubham Kanodia, Sarah E. Logsdon, Jacob K. Luhn, Michael W. McElwain, Andy Monson, Joe P. Ninan, Jayadev Rajagopal, Arpita Roy, Christian Schwab, Gudmundur Stefánsson, Ryan Terrien, Jason D. Eastman, Jonathan Horner, Peter Plavchan, Sharon X. Wang, Maurice L. Wilson, Robert A. Wittenmyer
Figure caption: Same as Figure A1, but for HD 4614 AB.
Paper: The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems
Authors: Mark R. Giovinazzi, Cullen H. Blake, Paul Robertson, Andrea S. J. Lin, Arvind F. Gupta, Suvrath Mahadevan, Jason T. Wright, Daniella Bardalez Gagliuffi, Jiayin Dong, Rachel B. Fernandes, Evan Fitzmaurice, Samuel Halverson, Shubham Kanodia, Sarah E. Logsdon, Jacob K. Luhn, Michael W. McElwain, Andy Monson, Joe P. Ninan, Jayadev Rajagopal, Arpita Roy, Christian Schwab, Gudmundur Stefánsson, Ryan Terrien, Jason D. Eastman, Jonathan Horner, Peter Plavchan, Sharon X. Wang, Maurice L. Wilson, Robert A. Wittenmyer
Figure caption: Posterior solution set for the orbital parameters of the HD 68017 binary star system. From left to right in the corner plot, the physical properties are primary mass, secondary mass, semimajor axis, eccentricity, and inclination.
Paper: The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems
Authors: Mark R. Giovinazzi, Cullen H. Blake, Paul Robertson, Andrea S. J. Lin, Arvind F. Gupta, Suvrath Mahadevan, Jason T. Wright, Daniella Bardalez Gagliuffi, Jiayin Dong, Rachel B. Fernandes, Evan Fitzmaurice, Samuel Halverson, Shubham Kanodia, Sarah E. Logsdon, Jacob K. Luhn, Michael W. McElwain, Andy Monson, Joe P. Ninan, Jayadev Rajagopal, Arpita Roy, Christian Schwab, Gudmundur Stefánsson, Ryan Terrien, Jason D. Eastman, Jonathan Horner, Peter Plavchan, Sharon X. Wang, Maurice L. Wilson, Robert A. Wittenmyer
Figure caption: Same as Figure A1, but for HD 24496 AB.
Paper: The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems
Authors: Mark R. Giovinazzi, Cullen H. Blake, Paul Robertson, Andrea S. J. Lin, Arvind F. Gupta, Suvrath Mahadevan, Jason T. Wright, Daniella Bardalez Gagliuffi, Jiayin Dong, Rachel B. Fernandes, Evan Fitzmaurice, Samuel Halverson, Shubham Kanodia, Sarah E. Logsdon, Jacob K. Luhn, Michael W. McElwain, Andy Monson, Joe P. Ninan, Jayadev Rajagopal, Arpita Roy, Christian Schwab, Gudmundur Stefánsson, Ryan Terrien, Jason D. Eastman, Jonathan Horner, Peter Plavchan, Sharon X. Wang, Maurice L. Wilson, Robert A. Wittenmyer
Figure caption: Same as Figure 14 but for HD 190360.
Paper: The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems
Authors: Mark R. Giovinazzi, Cullen H. Blake, Paul Robertson, Andrea S. J. Lin, Arvind F. Gupta, Suvrath Mahadevan, Jason T. Wright, Daniella Bardalez Gagliuffi, Jiayin Dong, Rachel B. Fernandes, Evan Fitzmaurice, Samuel Halverson, Shubham Kanodia, Sarah E. Logsdon, Jacob K. Luhn, Michael W. McElwain, Andy Monson, Joe P. Ninan, Jayadev Rajagopal, Arpita Roy, Christian Schwab, Gudmundur Stefánsson, Ryan Terrien, Jason D. Eastman, Jonathan Horner, Peter Plavchan, Sharon X. Wang, Maurice L. Wilson, Robert A. Wittenmyer
Figure caption: Same as Figure A1, but for 61 Cygni AB.
Paper: The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems
Authors: Mark R. Giovinazzi, Cullen H. Blake, Paul Robertson, Andrea S. J. Lin, Arvind F. Gupta, Suvrath Mahadevan, Jason T. Wright, Daniella Bardalez Gagliuffi, Jiayin Dong, Rachel B. Fernandes, Evan Fitzmaurice, Samuel Halverson, Shubham Kanodia, Sarah E. Logsdon, Jacob K. Luhn, Michael W. McElwain, Andy Monson, Joe P. Ninan, Jayadev Rajagopal, Arpita Roy, Christian Schwab, Gudmundur Stefánsson, Ryan Terrien, Jason D. Eastman, Jonathan Horner, Peter Plavchan, Sharon X. Wang, Maurice L. Wilson, Robert A. Wittenmyer
Figure caption: Same as Figure 14 but for 61 Cygni A.
Paper: The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems
Authors: Mark R. Giovinazzi, Cullen H. Blake, Paul Robertson, Andrea S. J. Lin, Arvind F. Gupta, Suvrath Mahadevan, Jason T. Wright, Daniella Bardalez Gagliuffi, Jiayin Dong, Rachel B. Fernandes, Evan Fitzmaurice, Samuel Halverson, Shubham Kanodia, Sarah E. Logsdon, Jacob K. Luhn, Michael W. McElwain, Andy Monson, Joe P. Ninan, Jayadev Rajagopal, Arpita Roy, Christian Schwab, Gudmundur Stefánsson, Ryan Terrien, Jason D. Eastman, Jonathan Horner, Peter Plavchan, Sharon X. Wang, Maurice L. Wilson, Robert A. Wittenmyer
Figure caption: Same as Figure 14 but for HD 154345.
Paper: The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems
Authors: Mark R. Giovinazzi, Cullen H. Blake, Paul Robertson, Andrea S. J. Lin, Arvind F. Gupta, Suvrath Mahadevan, Jason T. Wright, Daniella Bardalez Gagliuffi, Jiayin Dong, Rachel B. Fernandes, Evan Fitzmaurice, Samuel Halverson, Shubham Kanodia, Sarah E. Logsdon, Jacob K. Luhn, Michael W. McElwain, Andy Monson, Joe P. Ninan, Jayadev Rajagopal, Arpita Roy, Christian Schwab, Gudmundur Stefánsson, Ryan Terrien, Jason D. Eastman, Jonathan Horner, Peter Plavchan, Sharon X. Wang, Maurice L. Wilson, Robert A. Wittenmyer
Figure caption: Same as Figure 14 but for HD 4614.
Paper: The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems
Authors: Mark R. Giovinazzi, Cullen H. Blake, Paul Robertson, Andrea S. J. Lin, Arvind F. Gupta, Suvrath Mahadevan, Jason T. Wright, Daniella Bardalez Gagliuffi, Jiayin Dong, Rachel B. Fernandes, Evan Fitzmaurice, Samuel Halverson, Shubham Kanodia, Sarah E. Logsdon, Jacob K. Luhn, Michael W. McElwain, Andy Monson, Joe P. Ninan, Jayadev Rajagopal, Arpita Roy, Christian Schwab, Gudmundur Stefánsson, Ryan Terrien, Jason D. Eastman, Jonathan Horner, Peter Plavchan, Sharon X. Wang, Maurice L. Wilson, Robert A. Wittenmyer
Figure caption: Same as Figure 14 but for HD 24496.
Paper: Searching for GEMS: Confirmation of TOI-5573 b, a Cool, Saturn-like Planet Orbiting an M Dwarf 
Authors: Rachel B. Fernandes, Shubham Kanodia, Megan Delamer, Andrew Hotnisky, Te Han, Caleb I. Cañas, Jessica Libby-Roberts, Varghese Reji, Arvind F. Gupta, Jaime A. Alvarado-Montes, Chad F. Bender, Cullen H. Blake, William D. Cochran, Zoë L. de Beurs, Scott A. Diddams, Jiayin Dong, Mark E. Everett, Eric B. Ford, Samuel Halverson, Jesus Higuera, Henry A. Kobulnicky, Daniel M. Krolikowski, Alexander Larsen, Andrea S.J. Lin, Suvrath Mahadevan, Michael W. McElwain, Andrew Monson, Joe P. Ninan, Leonardo A. Paredes, Yatrik G. Patel, Paul Robertson, Gabrielle Ross, Arpita Roy, Christian Schwab, Gudmundur Stefansson, Daniel J. Stevens, Andrew M. Vanderburg, Jason Wright
Figure caption: The HPF-SpecMatch spectra fit results for order index 5. Top: two plots showing the five best-fit stars (red) selected to compose the spectra. The size and transparency of these five stars and the other library stars (black) are inversely proportional to the calculated χ2 initial value where we compare TOI-5573 spectra to the library star spectra. Larger and darker points signify a lower χ2 initial value, implying a better fit to the target spectrum. Middle: all HPF order index 5 spectra of TOI-5573 (gray) and their best-fit composite (yellow). The highest S/N spectrum is shown in black and its best-fit composite is in red. Bottom: the residuals of the best-fit composites for all spectra (gray) and for the highest S/N spectrum (black). The featureless residuals suggest a high-quality fit.
Paper: Searching for GEMS: Confirmation of TOI-5573 b, a Cool, Saturn-like Planet Orbiting an M Dwarf 
Authors: Rachel B. Fernandes, Shubham Kanodia, Megan Delamer, Andrew Hotnisky, Te Han, Caleb I. Cañas, Jessica Libby-Roberts, Varghese Reji, Arvind F. Gupta, Jaime A. Alvarado-Montes, Chad F. Bender, Cullen H. Blake, William D. Cochran, Zoë L. de Beurs, Scott A. Diddams, Jiayin Dong, Mark E. Everett, Eric B. Ford, Samuel Halverson, Jesus Higuera, Henry A. Kobulnicky, Daniel M. Krolikowski, Alexander Larsen, Andrea S.J. Lin, Suvrath Mahadevan, Michael W. McElwain, Andrew Monson, Joe P. Ninan, Leonardo A. Paredes, Yatrik G. Patel, Paul Robertson, Gabrielle Ross, Arpita Roy, Christian Schwab, Gudmundur Stefansson, Daniel J. Stevens, Andrew M. Vanderburg, Jason Wright
Figure caption: The raw (gray) phase-folded light curves of RBO and TGLC TESS sectors 20, 21, 47, and 74 photometry for TOI-5573. The best joint fit model is shown in red, and the 1σ confidence intervals are shown in yellow.
Paper: Searching for GEMS: Confirmation of TOI-5573 b, a Cool, Saturn-like Planet Orbiting an M Dwarf 
Authors: Rachel B. Fernandes, Shubham Kanodia, Megan Delamer, Andrew Hotnisky, Te Han, Caleb I. Cañas, Jessica Libby-Roberts, Varghese Reji, Arvind F. Gupta, Jaime A. Alvarado-Montes, Chad F. Bender, Cullen H. Blake, William D. Cochran, Zoë L. de Beurs, Scott A. Diddams, Jiayin Dong, Mark E. Everett, Eric B. Ford, Samuel Halverson, Jesus Higuera, Henry A. Kobulnicky, Daniel M. Krolikowski, Alexander Larsen, Andrea S.J. Lin, Suvrath Mahadevan, Michael W. McElwain, Andrew Monson, Joe P. Ninan, Leonardo A. Paredes, Yatrik G. Patel, Paul Robertson, Gabrielle Ross, Arpita Roy, Christian Schwab, Gudmundur Stefansson, Daniel J. Stevens, Andrew M. Vanderburg, Jason Wright
Figure caption: The binned HPF (blue) and NEID (orange) RV measurements of TOI-5573. Left: time series binned by each night. Right: phase-folded RV (black). The best-fit model is shown in black, and the 1σ confidence intervals are shown in gray.
Paper: Searching for GEMS: Confirmation of TOI-5573 b, a Cool, Saturn-like Planet Orbiting an M Dwarf 
Authors: Rachel B. Fernandes, Shubham Kanodia, Megan Delamer, Andrew Hotnisky, Te Han, Caleb I. Cañas, Jessica Libby-Roberts, Varghese Reji, Arvind F. Gupta, Jaime A. Alvarado-Montes, Chad F. Bender, Cullen H. Blake, William D. Cochran, Zoë L. de Beurs, Scott A. Diddams, Jiayin Dong, Mark E. Everett, Eric B. Ford, Samuel Halverson, Jesus Higuera, Henry A. Kobulnicky, Daniel M. Krolikowski, Alexander Larsen, Andrea S.J. Lin, Suvrath Mahadevan, Michael W. McElwain, Andrew Monson, Joe P. Ninan, Leonardo A. Paredes, Yatrik G. Patel, Paul Robertson, Gabrielle Ross, Arpita Roy, Christian Schwab, Gudmundur Stefansson, Daniel J. Stevens, Andrew M. Vanderburg, Jason Wright
Figure caption: SED of TOI-5573 showing the broadband photometric measurements from Table 2 in red (the x-error bar is the bandpass width) and the derived MIST model fluxes (as blue circles). A NextGen BT-SETTL spectrum (F. Allard et al. 2012) is overlaid for reference in gray (a smoothed version in black); the model spectrum is not used when fitting the SED.
Paper: The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems
Authors: Mark R. Giovinazzi, Cullen H. Blake, Paul Robertson, Andrea S. J. Lin, Arvind F. Gupta, Suvrath Mahadevan, Jason T. Wright, Daniella Bardalez Gagliuffi, Jiayin Dong, Rachel B. Fernandes, Evan Fitzmaurice, Samuel Halverson, Shubham Kanodia, Sarah E. Logsdon, Jacob K. Luhn, Michael W. McElwain, Andy Monson, Joe P. Ninan, Jayadev Rajagopal, Arpita Roy, Christian Schwab, Gudmundur Stefánsson, Ryan Terrien, Jason D. Eastman, Jonathan Horner, Peter Plavchan, Sharon X. Wang, Maurice L. Wilson, Robert A. Wittenmyer
Figure caption: Same as Figure A1, but for HD 190360 b.
Paper: Searching for GEMS: Confirmation of TOI-5573 b, a Cool, Saturn-like Planet Orbiting an M Dwarf 
Authors: Rachel B. Fernandes, Shubham Kanodia, Megan Delamer, Andrew Hotnisky, Te Han, Caleb I. Cañas, Jessica Libby-Roberts, Varghese Reji, Arvind F. Gupta, Jaime A. Alvarado-Montes, Chad F. Bender, Cullen H. Blake, William D. Cochran, Zoë L. de Beurs, Scott A. Diddams, Jiayin Dong, Mark E. Everett, Eric B. Ford, Samuel Halverson, Jesus Higuera, Henry A. Kobulnicky, Daniel M. Krolikowski, Alexander Larsen, Andrea S.J. Lin, Suvrath Mahadevan, Michael W. McElwain, Andrew Monson, Joe P. Ninan, Leonardo A. Paredes, Yatrik G. Patel, Paul Robertson, Gabrielle Ross, Arpita Roy, Christian Schwab, Gudmundur Stefansson, Daniel J. Stevens, Andrew M. Vanderburg, Jason Wright
Figure caption: NESSI Speckle Imaging in r’ and z’ bands in the inset 2﹩\mathop{.}\limits^{\unicode{x02033}}﹩4 across. The curve shows the 5σ contrast curve for TOI-5573 in both z and r bands. The contrast curves indicate that there are no bright companions within 1﹩\mathop{.}\limits^{\unicode{x02033}}﹩2 from the host star.
Paper: The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems
Authors: Mark R. Giovinazzi, Cullen H. Blake, Paul Robertson, Andrea S. J. Lin, Arvind F. Gupta, Suvrath Mahadevan, Jason T. Wright, Daniella Bardalez Gagliuffi, Jiayin Dong, Rachel B. Fernandes, Evan Fitzmaurice, Samuel Halverson, Shubham Kanodia, Sarah E. Logsdon, Jacob K. Luhn, Michael W. McElwain, Andy Monson, Joe P. Ninan, Jayadev Rajagopal, Arpita Roy, Christian Schwab, Gudmundur Stefánsson, Ryan Terrien, Jason D. Eastman, Jonathan Horner, Peter Plavchan, Sharon X. Wang, Maurice L. Wilson, Robert A. Wittenmyer
Figure caption: Same as Figure A1, but for HD 154345 b.
Paper: The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems
Authors: Mark R. Giovinazzi, Cullen H. Blake, Paul Robertson, Andrea S. J. Lin, Arvind F. Gupta, Suvrath Mahadevan, Jason T. Wright, Daniella Bardalez Gagliuffi, Jiayin Dong, Rachel B. Fernandes, Evan Fitzmaurice, Samuel Halverson, Shubham Kanodia, Sarah E. Logsdon, Jacob K. Luhn, Michael W. McElwain, Andy Monson, Joe P. Ninan, Jayadev Rajagopal, Arpita Roy, Christian Schwab, Gudmundur Stefánsson, Ryan Terrien, Jason D. Eastman, Jonathan Horner, Peter Plavchan, Sharon X. Wang, Maurice L. Wilson, Robert A. Wittenmyer
Figure caption: Same as Figure A1, but for HD 217107 c.
Paper: Five New Sirius-like White Dwarf–Main-sequence Star Systems with MagAO-X
Authors: Logan A. Pearce, Jared R. Males, Sebastiaan Y. Haffert, Laird M. Close, Joseph D. Long, Eden A. McEwen, Joshua Liberman, Maggie Y. Kautz, Jay K. Kueny, Alycia J. Weinberger, Jialin Li, Elena Tonucci, Katie Twitchell, Avalon L. McLeod, Warren B. Foster, Olivier Guyon, Alexander D. Hedglen, Kyle Van Gorkom, Jennifer Lumbres, Lauren Schatz, Victor Gasho, Katie M. Morzinski, Phil M. Hinz
Figure caption: PMa plots for the four stars with nondetections with Hipparcos and Gaia astrometry, generated using the methodology of P. Kervella et al. (2022). The blue curve shows the mass of an unresolved companion that would cause the observed acceleration as a function of separation. The orange region marks where our imaging is sensitive. The inset axes shows the flux contrast corresponding to those minimum masses (purple) and our 3σ contrast limit (red). The gray vertical lines mark where they cross, the gray horizontal line marks the minimum mass at that limit. Our contrast curves rule out at 3σ companions within the orange region beyond the gray vertical line. (a) HD 146740, (b) HD 109439, (c) HD 7918, and (d) HD 680.
Paper: Ultradeep Imaging of Nearby Dwarf Irregular Galaxies: Young Objects in the Far Outer Disk
Authors: Deidre A. Hunter, Hong-Xin Zhang, Bruce G. Elmegreen, Ella R. Castelloe, Hannah Michaye Ledford, Ishara Nisley, Ryuga Hatano
Figure caption: CMDs and CCDs for far outer disk objects in DDO 43 with FUV emission. Quantities are corrected for foreground extinction. Dashed lines are single-age stellar population Z = 0.008 metallicity models from G. Bruzual & S. Charlot (2003), one scaled to a cluster of 3000 M⊙ and the other to 100 M⊙. The red ×'s mark the age of the model cluster in gigayears, so the first four from the left are 1, 3, 10, and 30 Myr.
Paper: Ultradeep Imaging of Nearby Dwarf Irregular Galaxies: Young Objects in the Far Outer Disk
Authors: Deidre A. Hunter, Hong-Xin Zhang, Bruce G. Elmegreen, Ella R. Castelloe, Hannah Michaye Ledford, Ishara Nisley, Ryuga Hatano
Figure caption: DDO 210 with far disk objects circled in blue on the V image (top). The red ellipses are as in Figure 4. The FUV image is also shown although there are no objects in the far outer disk with FUV emission.
Paper: Ultradeep Imaging of Nearby Dwarf Irregular Galaxies: Young Objects in the Far Outer Disk
Authors: Deidre A. Hunter, Hong-Xin Zhang, Bruce G. Elmegreen, Ella R. Castelloe, Hannah Michaye Ledford, Ishara Nisley, Ryuga Hatano
Figure caption: NGC 3738 with far disk objects circled in blue on the V image. The red ellipses are as in Figure 4. The FUV image is also shown although there are no objects in the far outer disk with FUV emission.
Paper: Ultradeep Imaging of Nearby Dwarf Irregular Galaxies: Young Objects in the Far Outer Disk
Authors: Deidre A. Hunter, Hong-Xin Zhang, Bruce G. Elmegreen, Ella R. Castelloe, Hannah Michaye Ledford, Ishara Nisley, Ryuga Hatano
Figure caption: F564-V3 with far disk objects circled in blue on the V image. The red ellipses are as in Figure 4. The FUV image is also shown although there are no objects in the far outer disk with FUV emission.
Paper: Ultradeep Imaging of Nearby Dwarf Irregular Galaxies: Young Objects in the Far Outer Disk
Authors: Deidre A. Hunter, Hong-Xin Zhang, Bruce G. Elmegreen, Ella R. Castelloe, Hannah Michaye Ledford, Ishara Nisley, Ryuga Hatano
Figure caption: DDO 216 with far disk objects circled in blue on the V image. The red ellipses are as in Figure 4. The FUV image is also shown although there are no objects in the far outer disk with FUV emission.
Paper: Ultradeep Imaging of Nearby Dwarf Irregular Galaxies: Young Objects in the Far Outer Disk
Authors: Deidre A. Hunter, Hong-Xin Zhang, Bruce G. Elmegreen, Ella R. Castelloe, Hannah Michaye Ledford, Ishara Nisley, Ryuga Hatano
Figure caption: LGS3 with far disk objects circled in blue on the V image. The red ellipses are as in Figure 4. The FUV image is also shown although there are no objects in the far outer disk with FUV emission.