adsabs/AstroCLIMB huggingface dataset:
Paper: HD 35843: A Sun-like Star Hosting a Long-period Sub-Neptune and Inner Super-Earth
Authors: Katharine Hesse, Ismael Mireles, François Bouchy, Diana Dragomir, Solène Ulmer-Moll, Nora L. Eisner, Keivan G. Stassun, Samuel N. Quinn, Hugh P. Osborn, Sergio G. Sousa, Cristilyn N. Watkins, Karen A. Collins, Edward M. Bryant, Jonathan M. Irwin, Coel Hellier, Marshall C. Johnson, Carl Ziegler, Steve B. Howell, David R. Anderson, Daniel Bayliss, Allyson Bieryla, César Briceño, R. Paul Butler, David Charbonneau, Ryan Cloutier, Jeffrey Crane, Jason Dittmann, Jason D. Eastman, Sebastián A. Freigeiro, Benjamin J. Fulton, Samuel Gill, Maximilian Günther, Haedam Im, Jon M. Jenkins, Michelle Kunimoto, Baptiste Lavie, Monika Lendl, Michael B. Lund, Andrew W. Mann, Belinda Nicholson, David Osip, Martin Paegert, Nuno C. Santos, Richard P. Schwarz, Sara Seager, Stephen Shectman, Johanna Teske, Joseph D. Twicken, Stéphane Udry, Vincent Van Eylen, José Vinés, Sharon X. Wang, Peter J. Wheatley, Joshua N. Winn, Edward E. Zuidema
Figure caption: Transit injection and recovery for the TESS light curve of HD 35843 made using tkmatrix (M. Dévora-Pajares & F. J. Pozuelos 2022) showing that an additional transiting planet at a period shorter than 20 days or a radius larger than 1.5 R⊕ should have been detected if present.
Paper: HD 35843: A Sun-like Star Hosting a Long-period Sub-Neptune and Inner Super-Earth
Authors: Katharine Hesse, Ismael Mireles, François Bouchy, Diana Dragomir, Solène Ulmer-Moll, Nora L. Eisner, Keivan G. Stassun, Samuel N. Quinn, Hugh P. Osborn, Sergio G. Sousa, Cristilyn N. Watkins, Karen A. Collins, Edward M. Bryant, Jonathan M. Irwin, Coel Hellier, Marshall C. Johnson, Carl Ziegler, Steve B. Howell, David R. Anderson, Daniel Bayliss, Allyson Bieryla, César Briceño, R. Paul Butler, David Charbonneau, Ryan Cloutier, Jeffrey Crane, Jason Dittmann, Jason D. Eastman, Sebastián A. Freigeiro, Benjamin J. Fulton, Samuel Gill, Maximilian Günther, Haedam Im, Jon M. Jenkins, Michelle Kunimoto, Baptiste Lavie, Monika Lendl, Michael B. Lund, Andrew W. Mann, Belinda Nicholson, David Osip, Martin Paegert, Nuno C. Santos, Richard P. Schwarz, Sara Seager, Stephen Shectman, Johanna Teske, Joseph D. Twicken, Stéphane Udry, Vincent Van Eylen, José Vinés, Sharon X. Wang, Peter J. Wheatley, Joshua N. Winn, Edward E. Zuidema
Figure caption: Top row: from left to right, we create stacked periodograms for (1) the full set of ESPRESSO RV points, (2) the ESPRESSO RV points with the 47 day signal removed, and (3) the RV points with both the 47 day and 10 day signals removed. The color scale corresponds to logarithm of the probability of the period. Bottom row: SNR of the highest peak of periodicity for the same three sets of data. The SNR increases with the number of observations for both planet signals (left and center), which is consistent with a stable planetary signal.
Paper: HD 35843: A Sun-like Star Hosting a Long-period Sub-Neptune and Inner Super-Earth
Authors: Katharine Hesse, Ismael Mireles, François Bouchy, Diana Dragomir, Solène Ulmer-Moll, Nora L. Eisner, Keivan G. Stassun, Samuel N. Quinn, Hugh P. Osborn, Sergio G. Sousa, Cristilyn N. Watkins, Karen A. Collins, Edward M. Bryant, Jonathan M. Irwin, Coel Hellier, Marshall C. Johnson, Carl Ziegler, Steve B. Howell, David R. Anderson, Daniel Bayliss, Allyson Bieryla, César Briceño, R. Paul Butler, David Charbonneau, Ryan Cloutier, Jeffrey Crane, Jason Dittmann, Jason D. Eastman, Sebastián A. Freigeiro, Benjamin J. Fulton, Samuel Gill, Maximilian Günther, Haedam Im, Jon M. Jenkins, Michelle Kunimoto, Baptiste Lavie, Monika Lendl, Michael B. Lund, Andrew W. Mann, Belinda Nicholson, David Osip, Martin Paegert, Nuno C. Santos, Richard P. Schwarz, Sara Seager, Stephen Shectman, Johanna Teske, Joseph D. Twicken, Stéphane Udry, Vincent Van Eylen, José Vinés, Sharon X. Wang, Peter J. Wheatley, Joshua N. Winn, Edward E. Zuidema
Figure caption: GLS periodogram for the ESPRESSO RVs before (top) and after subtracting out the 46.96 day planet (middle) and both planets (bottom). The peak near 10 days becomes more significant after this subtraction. The peaks near 1 day and those past 100 days are artifacts of the window function of the observation times. The magenta line marks the 46.96 day planet and the yellow line marks the peak near 10 days.
Paper: HD 35843: A Sun-like Star Hosting a Long-period Sub-Neptune and Inner Super-Earth
Authors: Katharine Hesse, Ismael Mireles, François Bouchy, Diana Dragomir, Solène Ulmer-Moll, Nora L. Eisner, Keivan G. Stassun, Samuel N. Quinn, Hugh P. Osborn, Sergio G. Sousa, Cristilyn N. Watkins, Karen A. Collins, Edward M. Bryant, Jonathan M. Irwin, Coel Hellier, Marshall C. Johnson, Carl Ziegler, Steve B. Howell, David R. Anderson, Daniel Bayliss, Allyson Bieryla, César Briceño, R. Paul Butler, David Charbonneau, Ryan Cloutier, Jeffrey Crane, Jason Dittmann, Jason D. Eastman, Sebastián A. Freigeiro, Benjamin J. Fulton, Samuel Gill, Maximilian Günther, Haedam Im, Jon M. Jenkins, Michelle Kunimoto, Baptiste Lavie, Monika Lendl, Michael B. Lund, Andrew W. Mann, Belinda Nicholson, David Osip, Martin Paegert, Nuno C. Santos, Richard P. Schwarz, Sara Seager, Stephen Shectman, Johanna Teske, Joseph D. Twicken, Stéphane Udry, Vincent Van Eylen, José Vinés, Sharon X. Wang, Peter J. Wheatley, Joshua N. Winn, Edward E. Zuidema
Figure caption: SED of TOI 4189. Red symbols represent the observed photometric measurements, where the horizontal bars represent the effective width of the passband. Blue symbols are the model fluxes from the best-fit Kurucz atmosphere model (black).
Paper: HD 35843: A Sun-like Star Hosting a Long-period Sub-Neptune and Inner Super-Earth
Authors: Katharine Hesse, Ismael Mireles, François Bouchy, Diana Dragomir, Solène Ulmer-Moll, Nora L. Eisner, Keivan G. Stassun, Samuel N. Quinn, Hugh P. Osborn, Sergio G. Sousa, Cristilyn N. Watkins, Karen A. Collins, Edward M. Bryant, Jonathan M. Irwin, Coel Hellier, Marshall C. Johnson, Carl Ziegler, Steve B. Howell, David R. Anderson, Daniel Bayliss, Allyson Bieryla, César Briceño, R. Paul Butler, David Charbonneau, Ryan Cloutier, Jeffrey Crane, Jason Dittmann, Jason D. Eastman, Sebastián A. Freigeiro, Benjamin J. Fulton, Samuel Gill, Maximilian Günther, Haedam Im, Jon M. Jenkins, Michelle Kunimoto, Baptiste Lavie, Monika Lendl, Michael B. Lund, Andrew W. Mann, Belinda Nicholson, David Osip, Martin Paegert, Nuno C. Santos, Richard P. Schwarz, Sara Seager, Stephen Shectman, Johanna Teske, Joseph D. Twicken, Stéphane Udry, Vincent Van Eylen, José Vinés, Sharon X. Wang, Peter J. Wheatley, Joshua N. Winn, Edward E. Zuidema
Figure caption: GLS periodogram for the ESPRESSO RVs and various activity indicators. There is a significant peak near 47 days in the RVs (marked in red) and a less significant peak near 10 days (marked in yellow). The bisector span, FWHM, and contrast all show peaks of varying significance near 25 days.
Paper: HD 35843: A Sun-like Star Hosting a Long-period Sub-Neptune and Inner Super-Earth
Authors: Katharine Hesse, Ismael Mireles, François Bouchy, Diana Dragomir, Solène Ulmer-Moll, Nora L. Eisner, Keivan G. Stassun, Samuel N. Quinn, Hugh P. Osborn, Sergio G. Sousa, Cristilyn N. Watkins, Karen A. Collins, Edward M. Bryant, Jonathan M. Irwin, Coel Hellier, Marshall C. Johnson, Carl Ziegler, Steve B. Howell, David R. Anderson, Daniel Bayliss, Allyson Bieryla, César Briceño, R. Paul Butler, David Charbonneau, Ryan Cloutier, Jeffrey Crane, Jason Dittmann, Jason D. Eastman, Sebastián A. Freigeiro, Benjamin J. Fulton, Samuel Gill, Maximilian Günther, Haedam Im, Jon M. Jenkins, Michelle Kunimoto, Baptiste Lavie, Monika Lendl, Michael B. Lund, Andrew W. Mann, Belinda Nicholson, David Osip, Martin Paegert, Nuno C. Santos, Richard P. Schwarz, Sara Seager, Stephen Shectman, Johanna Teske, Joseph D. Twicken, Stéphane Udry, Vincent Van Eylen, José Vinés, Sharon X. Wang, Peter J. Wheatley, Joshua N. Winn, Edward E. Zuidema
Figure caption: ESPRESSO residual RVs (46.96 day planet subtracted) vs. various activity indicators showing no significant correlations. The plots show the Pearson correlation coefficient and corresponding p-value.
Paper: HD 35843: A Sun-like Star Hosting a Long-period Sub-Neptune and Inner Super-Earth
Authors: Katharine Hesse, Ismael Mireles, François Bouchy, Diana Dragomir, Solène Ulmer-Moll, Nora L. Eisner, Keivan G. Stassun, Samuel N. Quinn, Hugh P. Osborn, Sergio G. Sousa, Cristilyn N. Watkins, Karen A. Collins, Edward M. Bryant, Jonathan M. Irwin, Coel Hellier, Marshall C. Johnson, Carl Ziegler, Steve B. Howell, David R. Anderson, Daniel Bayliss, Allyson Bieryla, César Briceño, R. Paul Butler, David Charbonneau, Ryan Cloutier, Jeffrey Crane, Jason Dittmann, Jason D. Eastman, Sebastián A. Freigeiro, Benjamin J. Fulton, Samuel Gill, Maximilian Günther, Haedam Im, Jon M. Jenkins, Michelle Kunimoto, Baptiste Lavie, Monika Lendl, Michael B. Lund, Andrew W. Mann, Belinda Nicholson, David Osip, Martin Paegert, Nuno C. Santos, Richard P. Schwarz, Sara Seager, Stephen Shectman, Johanna Teske, Joseph D. Twicken, Stéphane Udry, Vincent Van Eylen, José Vinés, Sharon X. Wang, Peter J. Wheatley, Joshua N. Winn, Edward E. Zuidema
Figure caption: Phase folded and offset-subtracted ESPRESSO RVs with the modeled best-fit allesfitter RV curve for HD 35843 b (left) and HD 35843 c (right), with residuals plotted on the bottom. Stellar jitter has been added in quadrature with the measurement uncertainties.
Paper: HD 35843: A Sun-like Star Hosting a Long-period Sub-Neptune and Inner Super-Earth
Authors: Katharine Hesse, Ismael Mireles, François Bouchy, Diana Dragomir, Solène Ulmer-Moll, Nora L. Eisner, Keivan G. Stassun, Samuel N. Quinn, Hugh P. Osborn, Sergio G. Sousa, Cristilyn N. Watkins, Karen A. Collins, Edward M. Bryant, Jonathan M. Irwin, Coel Hellier, Marshall C. Johnson, Carl Ziegler, Steve B. Howell, David R. Anderson, Daniel Bayliss, Allyson Bieryla, César Briceño, R. Paul Butler, David Charbonneau, Ryan Cloutier, Jeffrey Crane, Jason Dittmann, Jason D. Eastman, Sebastián A. Freigeiro, Benjamin J. Fulton, Samuel Gill, Maximilian Günther, Haedam Im, Jon M. Jenkins, Michelle Kunimoto, Baptiste Lavie, Monika Lendl, Michael B. Lund, Andrew W. Mann, Belinda Nicholson, David Osip, Martin Paegert, Nuno C. Santos, Richard P. Schwarz, Sara Seager, Stephen Shectman, Johanna Teske, Joseph D. Twicken, Stéphane Udry, Vincent Van Eylen, José Vinés, Sharon X. Wang, Peter J. Wheatley, Joshua N. Winn, Edward E. Zuidema
Figure caption: Phase folded TESS transit data with the modeled best-fit allesfitter light curve, and residuals plot on the bottom.
Paper: The Compositions of Rocky Planets in Close-in Orbits Tend to Be Earth-like
Authors: Casey L. Brinkman, Lauren M. Weiss, Daniel Huber, Rena A. Lee, Jared Kolecki, Gwyneth Tenn, Jingwen Zhang, Suchitra Narayanan, Alex S. Polanski, Fei Dai, Jacob L. Bean, Corey Beard, Madison Brady, Max Brodheim, Matt Brown, Ashley Chontos, William Deich, Jerry Edelstein, Benjamin J. Fulton, Steven Giacalone, Steven R. Gibson, Gregory J. Gilbert, Samuel Halverson, Luke Handley, Grant M. Hill, Rae Holcomb, Bradford Holden, Aaron Householder, Andrew W. Howard, Howard Isaacson, Stephen Kaye, Russ R. Laher, Kyle Lanclos, J. M. Joel Ong, Joel Payne, Erik A. Petigura, Daria Pidhorodetska, Claire Poppett, Arpita Roy, Ryan Rubenzahl, Nicholas Saunders, Christian Schwab, Andreas Seifahrt, Abby P. Shaum, Martin M. Sirk, Chris Smith, Roger Smith, Guđmundur Stefánsson, Julian Stürmer, Jim Thorne, Emma V. Turtelboom, Dakotah Tyler, John Valliant, Judah Van Zandt, Josh Walawender, Samuel W. Yee, Sherry Yeh, Jon Zink
Figure caption: RVs phase folded at the period of each planet, after subtracting the RV components from the other three planets based on our best-fit model. The model RV curve for each planet is overplotted in gray, with the model period, semiamplitude (K), and standard deviation in semiamplitude (σ) shown. The gold points are the binned weighted median values with standard deviation of binned RVs as uncertainties.
Paper: The Compositions of Rocky Planets in Close-in Orbits Tend to Be Earth-like
Authors: Casey L. Brinkman, Lauren M. Weiss, Daniel Huber, Rena A. Lee, Jared Kolecki, Gwyneth Tenn, Jingwen Zhang, Suchitra Narayanan, Alex S. Polanski, Fei Dai, Jacob L. Bean, Corey Beard, Madison Brady, Max Brodheim, Matt Brown, Ashley Chontos, William Deich, Jerry Edelstein, Benjamin J. Fulton, Steven Giacalone, Steven R. Gibson, Gregory J. Gilbert, Samuel Halverson, Luke Handley, Grant M. Hill, Rae Holcomb, Bradford Holden, Aaron Householder, Andrew W. Howard, Howard Isaacson, Stephen Kaye, Russ R. Laher, Kyle Lanclos, J. M. Joel Ong, Joel Payne, Erik A. Petigura, Daria Pidhorodetska, Claire Poppett, Arpita Roy, Ryan Rubenzahl, Nicholas Saunders, Christian Schwab, Andreas Seifahrt, Abby P. Shaum, Martin M. Sirk, Chris Smith, Roger Smith, Guđmundur Stefánsson, Julian Stürmer, Jim Thorne, Emma V. Turtelboom, Dakotah Tyler, John Valliant, Judah Van Zandt, Josh Walawender, Samuel W. Yee, Sherry Yeh, Jon Zink
Figure caption: Effective temperature vs. luminosity is shown for all stars in our sample (colored stars), along with a larger sample of exoplanet host stars from the SPOCS catalog (J. M. Brewer & D. A. Fischer 2018). Stars of spectral type G are shown in the pink shaded region (center), those of type F in the purple shaded region (left), and K in the blue shaded region (right).
Paper: The Compositions of Rocky Planets in Close-in Orbits Tend to Be Earth-like
Authors: Casey L. Brinkman, Lauren M. Weiss, Daniel Huber, Rena A. Lee, Jared Kolecki, Gwyneth Tenn, Jingwen Zhang, Suchitra Narayanan, Alex S. Polanski, Fei Dai, Jacob L. Bean, Corey Beard, Madison Brady, Max Brodheim, Matt Brown, Ashley Chontos, William Deich, Jerry Edelstein, Benjamin J. Fulton, Steven Giacalone, Steven R. Gibson, Gregory J. Gilbert, Samuel Halverson, Luke Handley, Grant M. Hill, Rae Holcomb, Bradford Holden, Aaron Householder, Andrew W. Howard, Howard Isaacson, Stephen Kaye, Russ R. Laher, Kyle Lanclos, J. M. Joel Ong, Joel Payne, Erik A. Petigura, Daria Pidhorodetska, Claire Poppett, Arpita Roy, Ryan Rubenzahl, Nicholas Saunders, Christian Schwab, Andreas Seifahrt, Abby P. Shaum, Martin M. Sirk, Chris Smith, Roger Smith, Guđmundur Stefánsson, Julian Stürmer, Jim Thorne, Emma V. Turtelboom, Dakotah Tyler, John Valliant, Judah Van Zandt, Josh Walawender, Samuel W. Yee, Sherry Yeh, Jon Zink
Figure caption: Planet radius vs. mass for our sample (diamonds) shown in the context of the rocky planet population (circles). Opaque diamonds represent our mass and radius measurements, while translucent diamonds are the previously published values. Lines show mass–radius relations for planets with an Earth-like composition, a purely silicate-rock composition, and a purely iron composition (L. Zeng et al. 2019). Literature values come from the NASA Exoplanet Archive (R. L. Akeson et al. 2013) queried 2024 April 12 for planets with mass and radius measurements with fractional uncertainties <50%, and the circle size is inversely correlated with fractional uncertainty in density. Planets consistent with a rocky composition (mixture of iron and silicate only) are shown in pink. Planets with masses and radii 1σ away from a pure silicate composition (dashed line) are shown in purple and possibly host envelopes made of high mean molecular weight (MMW) species.
Paper: The Compositions of Rocky Planets in Close-in Orbits Tend to Be Earth-like
Authors: Casey L. Brinkman, Lauren M. Weiss, Daniel Huber, Rena A. Lee, Jared Kolecki, Gwyneth Tenn, Jingwen Zhang, Suchitra Narayanan, Alex S. Polanski, Fei Dai, Jacob L. Bean, Corey Beard, Madison Brady, Max Brodheim, Matt Brown, Ashley Chontos, William Deich, Jerry Edelstein, Benjamin J. Fulton, Steven Giacalone, Steven R. Gibson, Gregory J. Gilbert, Samuel Halverson, Luke Handley, Grant M. Hill, Rae Holcomb, Bradford Holden, Aaron Householder, Andrew W. Howard, Howard Isaacson, Stephen Kaye, Russ R. Laher, Kyle Lanclos, J. M. Joel Ong, Joel Payne, Erik A. Petigura, Daria Pidhorodetska, Claire Poppett, Arpita Roy, Ryan Rubenzahl, Nicholas Saunders, Christian Schwab, Andreas Seifahrt, Abby P. Shaum, Martin M. Sirk, Chris Smith, Roger Smith, Guđmundur Stefánsson, Julian Stürmer, Jim Thorne, Emma V. Turtelboom, Dakotah Tyler, John Valliant, Judah Van Zandt, Josh Walawender, Samuel W. Yee, Sherry Yeh, Jon Zink
Figure caption: The CMF of rocky exoplanets vs. equivalent CMF for their host stars is shown for our sample in the context of the sample of rocky planets (from C. L. Brinkman et al. 2024). The CMFs for the four inner solar system planets are shown at the equivalent CMF of the Sun (from top to bottom: Mercury, Earth, Venus, and Mars). The dotted line shows the one-to-one correspondence of CMF in stars and planets, which is where planets would fall if they inherited the exact Fe/Mg ratio from their host star. Our linear best-fit model is shown in indigo (OLS with rejection sampling).
Paper: The Compositions of Rocky Planets in Close-in Orbits Tend to Be Earth-like
Authors: Casey L. Brinkman, Lauren M. Weiss, Daniel Huber, Rena A. Lee, Jared Kolecki, Gwyneth Tenn, Jingwen Zhang, Suchitra Narayanan, Alex S. Polanski, Fei Dai, Jacob L. Bean, Corey Beard, Madison Brady, Max Brodheim, Matt Brown, Ashley Chontos, William Deich, Jerry Edelstein, Benjamin J. Fulton, Steven Giacalone, Steven R. Gibson, Gregory J. Gilbert, Samuel Halverson, Luke Handley, Grant M. Hill, Rae Holcomb, Bradford Holden, Aaron Householder, Andrew W. Howard, Howard Isaacson, Stephen Kaye, Russ R. Laher, Kyle Lanclos, J. M. Joel Ong, Joel Payne, Erik A. Petigura, Daria Pidhorodetska, Claire Poppett, Arpita Roy, Ryan Rubenzahl, Nicholas Saunders, Christian Schwab, Andreas Seifahrt, Abby P. Shaum, Martin M. Sirk, Chris Smith, Roger Smith, Guđmundur Stefánsson, Julian Stürmer, Jim Thorne, Emma V. Turtelboom, Dakotah Tyler, John Valliant, Judah Van Zandt, Josh Walawender, Samuel W. Yee, Sherry Yeh, Jon Zink
Figure caption: Alpha abundances [α/Fe] as a function of [Fe/H] for each host star in our sample, along with a larger sample of exoplanet hosts from the SPOCS catalog (J. M. Brewer & D. A. Fischer 2018). The colors of each diamond correspond to the same planet as listed in Figure 5. The black dashed line approximately separates the galactic thin-disk and thick-disk populations (L. M. Weiss et al. 2021). The two stars in our sample that fall above this line and were likely born in the galactic thick disk are labeled.
Paper: The Compositions of Rocky Planets in Close-in Orbits Tend to Be Earth-like
Authors: Casey L. Brinkman, Lauren M. Weiss, Daniel Huber, Rena A. Lee, Jared Kolecki, Gwyneth Tenn, Jingwen Zhang, Suchitra Narayanan, Alex S. Polanski, Fei Dai, Jacob L. Bean, Corey Beard, Madison Brady, Max Brodheim, Matt Brown, Ashley Chontos, William Deich, Jerry Edelstein, Benjamin J. Fulton, Steven Giacalone, Steven R. Gibson, Gregory J. Gilbert, Samuel Halverson, Luke Handley, Grant M. Hill, Rae Holcomb, Bradford Holden, Aaron Householder, Andrew W. Howard, Howard Isaacson, Stephen Kaye, Russ R. Laher, Kyle Lanclos, J. M. Joel Ong, Joel Payne, Erik A. Petigura, Daria Pidhorodetska, Claire Poppett, Arpita Roy, Ryan Rubenzahl, Nicholas Saunders, Christian Schwab, Andreas Seifahrt, Abby P. Shaum, Martin M. Sirk, Chris Smith, Roger Smith, Guđmundur Stefánsson, Julian Stürmer, Jim Thorne, Emma V. Turtelboom, Dakotah Tyler, John Valliant, Judah Van Zandt, Josh Walawender, Samuel W. Yee, Sherry Yeh, Jon Zink
Figure caption: Phase-folded transit light curve of TOI-1011 b from sectors 34 and 61 of TESS photometry. We have binned the phased light curve (black) and show the best-fit transit model in blue. The bottom panel shows the binned residuals after removing the best-fit model.
Paper: The Compositions of Rocky Planets in Close-in Orbits Tend to Be Earth-like
Authors: Casey L. Brinkman, Lauren M. Weiss, Daniel Huber, Rena A. Lee, Jared Kolecki, Gwyneth Tenn, Jingwen Zhang, Suchitra Narayanan, Alex S. Polanski, Fei Dai, Jacob L. Bean, Corey Beard, Madison Brady, Max Brodheim, Matt Brown, Ashley Chontos, William Deich, Jerry Edelstein, Benjamin J. Fulton, Steven Giacalone, Steven R. Gibson, Gregory J. Gilbert, Samuel Halverson, Luke Handley, Grant M. Hill, Rae Holcomb, Bradford Holden, Aaron Householder, Andrew W. Howard, Howard Isaacson, Stephen Kaye, Russ R. Laher, Kyle Lanclos, J. M. Joel Ong, Joel Payne, Erik A. Petigura, Daria Pidhorodetska, Claire Poppett, Arpita Roy, Ryan Rubenzahl, Nicholas Saunders, Christian Schwab, Andreas Seifahrt, Abby P. Shaum, Martin M. Sirk, Chris Smith, Roger Smith, Guđmundur Stefánsson, Julian Stürmer, Jim Thorne, Emma V. Turtelboom, Dakotah Tyler, John Valliant, Judah Van Zandt, Josh Walawender, Samuel W. Yee, Sherry Yeh, Jon Zink
Figure caption: The CMF of rocky exoplanets vs. [Fe/H] metallicity for their host stars is shown for our sample in the context of the sample of rocky planets. The colors of each diamond correspond to the same planet as listed in Figure 5. The rocky planet point size is inversely correlated with fractional uncertainty in CMF.
Paper: The Compositions of Rocky Planets in Close-in Orbits Tend to Be Earth-like
Authors: Casey L. Brinkman, Lauren M. Weiss, Daniel Huber, Rena A. Lee, Jared Kolecki, Gwyneth Tenn, Jingwen Zhang, Suchitra Narayanan, Alex S. Polanski, Fei Dai, Jacob L. Bean, Corey Beard, Madison Brady, Max Brodheim, Matt Brown, Ashley Chontos, William Deich, Jerry Edelstein, Benjamin J. Fulton, Steven Giacalone, Steven R. Gibson, Gregory J. Gilbert, Samuel Halverson, Luke Handley, Grant M. Hill, Rae Holcomb, Bradford Holden, Aaron Householder, Andrew W. Howard, Howard Isaacson, Stephen Kaye, Russ R. Laher, Kyle Lanclos, J. M. Joel Ong, Joel Payne, Erik A. Petigura, Daria Pidhorodetska, Claire Poppett, Arpita Roy, Ryan Rubenzahl, Nicholas Saunders, Christian Schwab, Andreas Seifahrt, Abby P. Shaum, Martin M. Sirk, Chris Smith, Roger Smith, Guđmundur Stefánsson, Julian Stürmer, Jim Thorne, Emma V. Turtelboom, Dakotah Tyler, John Valliant, Judah Van Zandt, Josh Walawender, Samuel W. Yee, Sherry Yeh, Jon Zink
Figure caption: Corner plot of key transit model fit parameters for TOI-1011 b.
Paper: Multiple Machine Learning as a Powerful Tool for Star Cluster Analysis
Authors: Denilso Camargo
Figure caption: Gaia-EDR3 optical CMDs for the probable member stars (black circles) within an extraction area of ﹩R=6{0}^{{\prime} }﹩ centered on the coordinates of NGC 1605a (left panels), NGC 1605b (middle panels), and a combination of both (right panels). The heat maps are built by applying the KNN smoothing algorithm smoothing on K = 3 (top panels) and K = 8 nearest neighbors (bottom panels), and they are color coded by the smoothness level. The two clusters are present in both CMDs, and they are highlighted by the isochrone fitting and the smoothing graphs.
Paper: Multiple Machine Learning as a Powerful Tool for Star Cluster Analysis
Authors: Denilso Camargo
Figure caption: Spatial and PM distributions of stars for an extraction area of ﹩R=2{0}^{{\prime} }﹩, centered on the coordinates of NGC 1605a and color coded by the pyUPMASK membership probabilities. Both diagrams reveal multiple substructures, especially the PM distribution.
Paper: Exploring the Wolf Approach to Constraining NIR Extinction Laws in the Corona Australis Molecular Cloud
Authors: Botao Jiang, 博韬 江, Jun Li, 军 李, Xi Chen, 曦 陈
Figure caption: Correlations between extinction values in different NIR bands (AJ vs. AH, AJ vs. ﹩{A}_{{K}_{S}}﹩, and AH vs. ﹩{A}_{{K}_{S}}﹩) for the CrA molecular cloud observed by the VISIONS survey. Each panel explicitly reports the fitted slope coefficient and intercept (zero-point) with associated uncertainties. The color scale indicates the density of data points. Black solid lines represent the best linear fits after removing 3σ outliers, with fit parameters annotated in each panel. Red dashed lines denote the 3σ boundaries, and points identified as outliers are shown in gray. Error bars in each panel represent the characteristic noise levels in the extinction measurements.