adsabs/AstroCLIMB huggingface dataset:
Paper: Astrometric Calibration and Performance of the Dark Energy Spectroscopic Instrument Focal Plane
Authors: S. Kent, E. Neilsen, K. Honscheid, D. Rabinowitz, E. F. Schlafly, J. Guy, D. Schlegel, J. García-Bellido, T. S. Li, E. Sanchez, J. Silber, J. Aguilar, S. Ahlen, D. Brooks, T. Claybaugh, A. de la Macorra, P. Doel, D. J. Eisenstein, K. Fanning, A. Font-Ribera, J. E. Forero-Romero, S. Gontcho A. Gontcho, J. Jimenez, D. Kirkby, T. Kisner, A. Kremin, M. Landriau, L. Le Guillou, M. E. Levi, C. Magneville, M. Manera, P. Martini, A. Meisner, R. Miquel, J. Moustakas, J. Nie, N. Palanque-Delabrouille, W. J. Percival, C. Poppett, M. Rezaie, A. J. Ross, G. Rossi, M. Schubnell, H. Seo, Gregory Tarlé, B. A. Weaver, R. Zhou, Z. Zhou, H. Zou
Figure caption: Portion of an FVC image of the focal plane with positioner fibers and fiducials (FIFs and GIFs) back-illuminated. The fiducials have a 4-spot pattern to aid in their identification. The approximate location of a GFA CCD is also shown.
Paper: Astrometric Calibration and Performance of the Dark Energy Spectroscopic Instrument Focal Plane
Authors: S. Kent, E. Neilsen, K. Honscheid, D. Rabinowitz, E. F. Schlafly, J. Guy, D. Schlegel, J. García-Bellido, T. S. Li, E. Sanchez, J. Silber, J. Aguilar, S. Ahlen, D. Brooks, T. Claybaugh, A. de la Macorra, P. Doel, D. J. Eisenstein, K. Fanning, A. Font-Ribera, J. E. Forero-Romero, S. Gontcho A. Gontcho, J. Jimenez, D. Kirkby, T. Kisner, A. Kremin, M. Landriau, L. Le Guillou, M. E. Levi, C. Magneville, M. Manera, P. Martini, A. Meisner, R. Miquel, J. Moustakas, J. Nie, N. Palanque-Delabrouille, W. J. Percival, C. Poppett, M. Rezaie, A. J. Ross, G. Rossi, M. Schubnell, H. Seo, Gregory Tarlé, B. A. Weaver, R. Zhou, Z. Zhou, H. Zou
Figure caption: Radial distortion (in microns) in B (green points) and R (red points) channels relative to the Z channel as measured by the dither tests. Open circles are the optical model predictions.
Paper: Astrometric Calibration and Performance of the Dark Energy Spectroscopic Instrument Focal Plane
Authors: S. Kent, E. Neilsen, K. Honscheid, D. Rabinowitz, E. F. Schlafly, J. Guy, D. Schlegel, J. García-Bellido, T. S. Li, E. Sanchez, J. Silber, J. Aguilar, S. Ahlen, D. Brooks, T. Claybaugh, A. de la Macorra, P. Doel, D. J. Eisenstein, K. Fanning, A. Font-Ribera, J. E. Forero-Romero, S. Gontcho A. Gontcho, J. Jimenez, D. Kirkby, T. Kisner, A. Kremin, M. Landriau, L. Le Guillou, M. E. Levi, C. Magneville, M. Manera, P. Martini, A. Meisner, R. Miquel, J. Moustakas, J. Nie, N. Palanque-Delabrouille, W. J. Percival, C. Poppett, M. Rezaie, A. J. Ross, G. Rossi, M. Schubnell, H. Seo, Gregory Tarlé, B. A. Weaver, R. Zhou, Z. Zhou, H. Zou
Figure caption: Comparison of telescope field center offsets, determined for each exposure in a dither sequence, to offsets measured by guide stars at the same time.
Paper: Astrometric Calibration and Performance of the Dark Energy Spectroscopic Instrument Focal Plane
Authors: S. Kent, E. Neilsen, K. Honscheid, D. Rabinowitz, E. F. Schlafly, J. Guy, D. Schlegel, J. García-Bellido, T. S. Li, E. Sanchez, J. Silber, J. Aguilar, S. Ahlen, D. Brooks, T. Claybaugh, A. de la Macorra, P. Doel, D. J. Eisenstein, K. Fanning, A. Font-Ribera, J. E. Forero-Romero, S. Gontcho A. Gontcho, J. Jimenez, D. Kirkby, T. Kisner, A. Kremin, M. Landriau, L. Le Guillou, M. E. Levi, C. Magneville, M. Manera, P. Martini, A. Meisner, R. Miquel, J. Moustakas, J. Nie, N. Palanque-Delabrouille, W. J. Percival, C. Poppett, M. Rezaie, A. J. Ross, G. Rossi, M. Schubnell, H. Seo, Gregory Tarlé, B. A. Weaver, R. Zhou, Z. Zhou, H. Zou
Figure caption: Residual positioner offsets in a typical dither sequence as a function of the focal plane coordinates. (Note that 0.″11 corresponds to 7.7 μm.)
Paper: Astrometric Calibration and Performance of the Dark Energy Spectroscopic Instrument Focal Plane
Authors: S. Kent, E. Neilsen, K. Honscheid, D. Rabinowitz, E. F. Schlafly, J. Guy, D. Schlegel, J. García-Bellido, T. S. Li, E. Sanchez, J. Silber, J. Aguilar, S. Ahlen, D. Brooks, T. Claybaugh, A. de la Macorra, P. Doel, D. J. Eisenstein, K. Fanning, A. Font-Ribera, J. E. Forero-Romero, S. Gontcho A. Gontcho, J. Jimenez, D. Kirkby, T. Kisner, A. Kremin, M. Landriau, L. Le Guillou, M. E. Levi, C. Magneville, M. Manera, P. Martini, A. Meisner, R. Miquel, J. Moustakas, J. Nie, N. Palanque-Delabrouille, W. J. Percival, C. Poppett, M. Rezaie, A. J. Ross, G. Rossi, M. Schubnell, H. Seo, Gregory Tarlé, B. A. Weaver, R. Zhou, Z. Zhou, H. Zou
Figure caption: Temperature dependence of the FVC astrometric scale factor. The scale factor is in units of angular degrees per FVC pixel.
Paper: Astrometric Calibration and Performance of the Dark Energy Spectroscopic Instrument Focal Plane
Authors: S. Kent, E. Neilsen, K. Honscheid, D. Rabinowitz, E. F. Schlafly, J. Guy, D. Schlegel, J. García-Bellido, T. S. Li, E. Sanchez, J. Silber, J. Aguilar, S. Ahlen, D. Brooks, T. Claybaugh, A. de la Macorra, P. Doel, D. J. Eisenstein, K. Fanning, A. Font-Ribera, J. E. Forero-Romero, S. Gontcho A. Gontcho, J. Jimenez, D. Kirkby, T. Kisner, A. Kremin, M. Landriau, L. Le Guillou, M. E. Levi, C. Magneville, M. Manera, P. Martini, A. Meisner, R. Miquel, J. Moustakas, J. Nie, N. Palanque-Delabrouille, W. J. Percival, C. Poppett, M. Rezaie, A. J. Ross, G. Rossi, M. Schubnell, H. Seo, Gregory Tarlé, B. A. Weaver, R. Zhou, Z. Zhou, H. Zou
Figure caption: Quiver pattern as a function of the focal plane coordinates used to correct positioner fibers for residual uncorrected distortion in the PM model.
Paper: A Crater Chronology for the Jupiter’s Trojan Asteroids
Authors: S. Marchi, D. Nesvorný, D. Vokrouhlický, W. F. Bottke, H. Levison
Figure caption: Calculated final crater sizes on an assumed 100 km Trojan asteroid. Scaling laws are from Equation (2) for cohesive soils (CS) and porous materials (P), cratering strength Y as indicated (see text). Other parameters assumed are: density of target and projectile 1 g cm−3. We assumed average impact velocity for Trojans–Trojans collisions (4.6 km s−1; Table 1). Here we use a 45 deg impact angle. The material parameters are (Holsapple & Housen 2007): ν = 0.4, μ = 0.41, k = 1.03 (CS); and ν = 0.4, μ = 0.4, k = 0.725 (P). Gray lines indicate craters with diameters equal to 1x and 10x the impactor size.
Paper: A Crater Chronology for the Jupiter’s Trojan Asteroids
Authors: S. Marchi, D. Nesvorný, D. Vokrouhlický, W. F. Bottke, H. Levison
Figure caption: Population size-frequency distribution assumed in this work (see text for details). Note that Trojan SFD is only for one cloud, either L4 or L5. We also report MBAs for reference (taken from Bottke et al. 2020).
Paper: A Crater Chronology for the Jupiter’s Trojan Asteroids
Authors: S. Marchi, D. Nesvorný, D. Vokrouhlický, W. F. Bottke, H. Levison
Figure caption: Chronology function used in this work (see text for details). For reference, a chronology for MBAs is also reported (O’Brien et al. 2014). All curves are normalized for a better comparison at the present time (t = 10−9 Gyr ago). Because of the normalization, JFCs appear to have more impacts than the other chronologies, but in reality this is not the case as explained in the text.
Paper: A Crater Chronology for the Jupiter’s Trojan Asteroids
Authors: S. Marchi, D. Nesvorný, D. Vokrouhlický, W. F. Bottke, H. Levison
Figure caption: Computed impact velocity distributions for Trojans–Trojans and Comets–Trojans collisions, indicated with Trojans and JFCs, respectively. For Trojans–Trojans, velocities are computed using a subset of numbered Trojan asteroids (Marzari et al. 1996). For Comets–Trojans, we considered a representative Trojan asteroid at 5.2 au (with zero inclination and eccentricity), and use an Opik approximation to compute impact velocities with crossing comtes.
Paper: An Exploration of AGN and Stellar Feedback Effects in the Intergalactic Medium via the Low-redshift Lyα Forest
Authors: Megan Taylor Tillman, Blakesley Burkhart, Stephanie Tonnesen, Simeon Bird, Greg L. Bryan, Daniel Anglés-Alcázar, Sultan Hassan, Rachel S. Somerville, Romeel Davé, Federico Marinacci, Lars Hernquist, Mark Vogelsberger
Figure caption: The Simba and TNG CDDs at z = 0.1 for the CAMELS 1P set varying the AGN feedback parameters (left two plots) and stellar feedback parameters (right four plots). The blue scatter points are observational data from D16. The blue lines represent a decrease in the parameter value (labeled in corresponding color bars), while the red lines represent an increase. The dashed black lines are the fiducial results. The panel below each plot displays the ratio, Δ, of the parameter variation result to the observed D16 data. The gray shaded region corresponds to the observational error bars. The TNG results when varying the AGN feedback parameters are not shown, as no changes in the CDD are seen.
Paper: An Exploration of AGN and Stellar Feedback Effects in the Intergalactic Medium via the Low-redshift Lyα Forest
Authors: Megan Taylor Tillman, Blakesley Burkhart, Stephanie Tonnesen, Simeon Bird, Greg L. Bryan, Daniel Anglés-Alcázar, Sultan Hassan, Rachel S. Somerville, Romeel Davé, Federico Marinacci, Lars Hernquist, Mark Vogelsberger
Figure caption: Simba temperature and column density projections of a single absorber slice as defined in this study (525 kpc h−1; see text in 2.3 and 3.1 for justification of this value). The top plots display the projected mean temperature weighted by mass. The bottom plots display the integrated H I column density of the slice. We show projections for varying AGN momentum flux (A AGN1) and AGN jet speed (A AGN2). The left plots are the lowest value for the parameter, the right plots are for the highest value, and the middle plots are the fiducial results. The projections help visualize the effect of varying the AGN feedback parameters.
Paper: An Exploration of AGN and Stellar Feedback Effects in the Intergalactic Medium via the Low-redshift Lyα Forest
Authors: Megan Taylor Tillman, Blakesley Burkhart, Stephanie Tonnesen, Simeon Bird, Greg L. Bryan, Daniel Anglés-Alcázar, Sultan Hassan, Rachel S. Somerville, Romeel Davé, Federico Marinacci, Lars Hernquist, Mark Vogelsberger
Figure caption: BH accretion rate density in the jet mode and overall number of SMBHs in the jet mode when varying different feedback parameters in the CAMELS-Simba simulations. All plots: the black lines correspond to fiducial results, the blue lines correspond to the smallest value for the parameter varied, and the red lines correspond to the largest value for the parameter varied. Top row: The SMBH accretion rate density ﹩{\dot{\rho }}_{\mathrm{BH}}﹩ in the AGN jet feedback mode vs. redshift for different values of the parameters. Bottom row: the number of SMBHs producing jet-mode feedback for parameter variations.
Paper: An Exploration of AGN and Stellar Feedback Effects in the Intergalactic Medium via the Low-redshift Lyα Forest
Authors: Megan Taylor Tillman, Blakesley Burkhart, Stephanie Tonnesen, Simeon Bird, Greg L. Bryan, Daniel Anglés-Alcázar, Sultan Hassan, Rachel S. Somerville, Romeel Davé, Federico Marinacci, Lars Hernquist, Mark Vogelsberger
Figure caption: The same temperature projections as seen in Figures 1 and 2, but for the CAMELS IllustrisTNG 1P simulation set feedback parameters. AGN feedback variations are on the left, and stellar feedback variations are on the right. The parameters varied are AGN energy per SMBH accretion rate (A AGN1), AGN burstiness (A AGN2), SN energy per SFR (﹩{A}_{\mathrm{SN}1}﹩), and SN wind speed (﹩{A}_{\mathrm{SN}2}﹩). Column density projections show minimal to no changes and are thus not included. Changes in the temperature projection due to feedback remain close to or confined to the host halos.
Paper: An Exploration of AGN and Stellar Feedback Effects in the Intergalactic Medium via the Low-redshift Lyα Forest
Authors: Megan Taylor Tillman, Blakesley Burkhart, Stephanie Tonnesen, Simeon Bird, Greg L. Bryan, Daniel Anglés-Alcázar, Sultan Hassan, Rachel S. Somerville, Romeel Davé, Federico Marinacci, Lars Hernquist, Mark Vogelsberger
Figure caption: Same as Figure 4 but for the b-value distribution, and here Δ is the ratio of the parameter variation results to the fiducial results. The distribution is normalized to integrate to unity. No change is seen in the b-value distribution for the TNG simulations when varying AGN feedback, so those results are excluded.
Paper: An Exploration of AGN and Stellar Feedback Effects in the Intergalactic Medium via the Low-redshift Lyα Forest
Authors: Megan Taylor Tillman, Blakesley Burkhart, Stephanie Tonnesen, Simeon Bird, Greg L. Bryan, Daniel Anglés-Alcázar, Sultan Hassan, Rachel S. Somerville, Romeel Davé, Federico Marinacci, Lars Hernquist, Mark Vogelsberger
Figure caption: Same as Figure 1, except for variations of the SN mass-loading factor (﹩{A}_{\mathrm{SN}1}﹩) and SN wind speed (﹩{A}_{\mathrm{SN}2}﹩).
Paper: Validating AU Microscopii d with Transit Timing Variations
Authors: Justin M. Wittrock, Peter P. Plavchan, Bryson L. Cale, Thomas Barclay, Mathis R. Ludwig, Richard P. Schwarz, Djamel Mékarnia, Amaury H. M. J. Triaud, Lyu Abe, Olga Suarez, Tristan Guillot, Dennis M. Conti, Karen A. Collins, Ian A. Waite, John F. Kielkopf, Kevin I. Collins, Stefan Dreizler, Mohammed El Mufti, Dax L. Feliz, Eric Gaidos, Claire S. Geneser, Keith D. Horne, Stephen R. Kane, Patrick J. Lowrance, Eder Martioli, Don J. Radford, Michael A. Reefe, Veronica Roccatagliata, Avi Shporer, Keivan G. Stassun, Christopher Stockdale, Thiam-Guan Tan, Angelle M. Tanner, Laura D. Vega
Figure caption: Corner plot of AU Mic b and c’s orbital parameters from Exo-Striker MCMC analysis for P d = 14.1 days.
Paper: Validating AU Microscopii d with Transit Timing Variations
Authors: Justin M. Wittrock, Peter P. Plavchan, Bryson L. Cale, Thomas Barclay, Mathis R. Ludwig, Richard P. Schwarz, Djamel Mékarnia, Amaury H. M. J. Triaud, Lyu Abe, Olga Suarez, Tristan Guillot, Dennis M. Conti, Karen A. Collins, Ian A. Waite, John F. Kielkopf, Kevin I. Collins, Stefan Dreizler, Mohammed El Mufti, Dax L. Feliz, Eric Gaidos, Claire S. Geneser, Keith D. Horne, Stephen R. Kane, Patrick J. Lowrance, Eder Martioli, Don J. Radford, Michael A. Reefe, Veronica Roccatagliata, Avi Shporer, Keivan G. Stassun, Christopher Stockdale, Thiam-Guan Tan, Angelle M. Tanner, Laura D. Vega
Figure caption: Corner plot of AU Mic b and c’s orbital parameters from Exo-Striker MCMC analysis for P d = 5.08 days.
Paper: Validating AU Microscopii d with Transit Timing Variations
Authors: Justin M. Wittrock, Peter P. Plavchan, Bryson L. Cale, Thomas Barclay, Mathis R. Ludwig, Richard P. Schwarz, Djamel Mékarnia, Amaury H. M. J. Triaud, Lyu Abe, Olga Suarez, Tristan Guillot, Dennis M. Conti, Karen A. Collins, Ian A. Waite, John F. Kielkopf, Kevin I. Collins, Stefan Dreizler, Mohammed El Mufti, Dax L. Feliz, Eric Gaidos, Claire S. Geneser, Keith D. Horne, Stephen R. Kane, Patrick J. Lowrance, Eder Martioli, Don J. Radford, Michael A. Reefe, Veronica Roccatagliata, Avi Shporer, Keivan G. Stassun, Christopher Stockdale, Thiam-Guan Tan, Angelle M. Tanner, Laura D. Vega
Figure caption: Corner plot of AU Mic b and c’s orbital parameters from Exo-Striker MCMC analysis for P d = 12.6 days.
Paper: Validating AU Microscopii d with Transit Timing Variations
Authors: Justin M. Wittrock, Peter P. Plavchan, Bryson L. Cale, Thomas Barclay, Mathis R. Ludwig, Richard P. Schwarz, Djamel Mékarnia, Amaury H. M. J. Triaud, Lyu Abe, Olga Suarez, Tristan Guillot, Dennis M. Conti, Karen A. Collins, Ian A. Waite, John F. Kielkopf, Kevin I. Collins, Stefan Dreizler, Mohammed El Mufti, Dax L. Feliz, Eric Gaidos, Claire S. Geneser, Keith D. Horne, Stephen R. Kane, Patrick J. Lowrance, Eder Martioli, Don J. Radford, Michael A. Reefe, Veronica Roccatagliata, Avi Shporer, Keivan G. Stassun, Christopher Stockdale, Thiam-Guan Tan, Angelle M. Tanner, Laura D. Vega
Figure caption: Corner plot of AU Mic b and c’s orbital parameters from Exo-Striker MCMC analysis for P d = 11.9 days.
Paper: Validating AU Microscopii d with Transit Timing Variations
Authors: Justin M. Wittrock, Peter P. Plavchan, Bryson L. Cale, Thomas Barclay, Mathis R. Ludwig, Richard P. Schwarz, Djamel Mékarnia, Amaury H. M. J. Triaud, Lyu Abe, Olga Suarez, Tristan Guillot, Dennis M. Conti, Karen A. Collins, Ian A. Waite, John F. Kielkopf, Kevin I. Collins, Stefan Dreizler, Mohammed El Mufti, Dax L. Feliz, Eric Gaidos, Claire S. Geneser, Keith D. Horne, Stephen R. Kane, Patrick J. Lowrance, Eder Martioli, Don J. Radford, Michael A. Reefe, Veronica Roccatagliata, Avi Shporer, Keivan G. Stassun, Christopher Stockdale, Thiam-Guan Tan, Angelle M. Tanner, Laura D. Vega
Figure caption: Corner plot of AU Mic b and c’s orbital parameters from Exo-Striker MCMC analysis for P d = 6.20 days.
Paper: Validating AU Microscopii d with Transit Timing Variations
Authors: Justin M. Wittrock, Peter P. Plavchan, Bryson L. Cale, Thomas Barclay, Mathis R. Ludwig, Richard P. Schwarz, Djamel Mékarnia, Amaury H. M. J. Triaud, Lyu Abe, Olga Suarez, Tristan Guillot, Dennis M. Conti, Karen A. Collins, Ian A. Waite, John F. Kielkopf, Kevin I. Collins, Stefan Dreizler, Mohammed El Mufti, Dax L. Feliz, Eric Gaidos, Claire S. Geneser, Keith D. Horne, Stephen R. Kane, Patrick J. Lowrance, Eder Martioli, Don J. Radford, Michael A. Reefe, Veronica Roccatagliata, Avi Shporer, Keivan G. Stassun, Christopher Stockdale, Thiam-Guan Tan, Angelle M. Tanner, Laura D. Vega
Figure caption: Corner plot of AU Mic b and c’s orbital parameters from Exo-Striker MCMC analysis for P d = 5.86 days.
Paper: Validating AU Microscopii d with Transit Timing Variations
Authors: Justin M. Wittrock, Peter P. Plavchan, Bryson L. Cale, Thomas Barclay, Mathis R. Ludwig, Richard P. Schwarz, Djamel Mékarnia, Amaury H. M. J. Triaud, Lyu Abe, Olga Suarez, Tristan Guillot, Dennis M. Conti, Karen A. Collins, Ian A. Waite, John F. Kielkopf, Kevin I. Collins, Stefan Dreizler, Mohammed El Mufti, Dax L. Feliz, Eric Gaidos, Claire S. Geneser, Keith D. Horne, Stephen R. Kane, Patrick J. Lowrance, Eder Martioli, Don J. Radford, Michael A. Reefe, Veronica Roccatagliata, Avi Shporer, Keivan G. Stassun, Christopher Stockdale, Thiam-Guan Tan, Angelle M. Tanner, Laura D. Vega
Figure caption: Corner plot of AU Mic b and c’s orbital parameters from Exo-Striker MCMC analysis for P d = 5.39 days.
Paper: Validating AU Microscopii d with Transit Timing Variations
Authors: Justin M. Wittrock, Peter P. Plavchan, Bryson L. Cale, Thomas Barclay, Mathis R. Ludwig, Richard P. Schwarz, Djamel Mékarnia, Amaury H. M. J. Triaud, Lyu Abe, Olga Suarez, Tristan Guillot, Dennis M. Conti, Karen A. Collins, Ian A. Waite, John F. Kielkopf, Kevin I. Collins, Stefan Dreizler, Mohammed El Mufti, Dax L. Feliz, Eric Gaidos, Claire S. Geneser, Keith D. Horne, Stephen R. Kane, Patrick J. Lowrance, Eder Martioli, Don J. Radford, Michael A. Reefe, Veronica Roccatagliata, Avi Shporer, Keivan G. Stassun, Christopher Stockdale, Thiam-Guan Tan, Angelle M. Tanner, Laura D. Vega
Figure caption: Corner plot of AU Mic b and c’s orbital parameters from Exo-Striker MCMC analysis for P d = 5.64 days.
Paper: Validating AU Microscopii d with Transit Timing Variations
Authors: Justin M. Wittrock, Peter P. Plavchan, Bryson L. Cale, Thomas Barclay, Mathis R. Ludwig, Richard P. Schwarz, Djamel Mékarnia, Amaury H. M. J. Triaud, Lyu Abe, Olga Suarez, Tristan Guillot, Dennis M. Conti, Karen A. Collins, Ian A. Waite, John F. Kielkopf, Kevin I. Collins, Stefan Dreizler, Mohammed El Mufti, Dax L. Feliz, Eric Gaidos, Claire S. Geneser, Keith D. Horne, Stephen R. Kane, Patrick J. Lowrance, Eder Martioli, Don J. Radford, Michael A. Reefe, Veronica Roccatagliata, Avi Shporer, Keivan G. Stassun, Christopher Stockdale, Thiam-Guan Tan, Angelle M. Tanner, Laura D. Vega
Figure caption: Corner plot of AU Mic b and c’s orbital parameters from Exo-Striker MCMC analysis for P d = 6.47 days.
Paper: Validating AU Microscopii d with Transit Timing Variations
Authors: Justin M. Wittrock, Peter P. Plavchan, Bryson L. Cale, Thomas Barclay, Mathis R. Ludwig, Richard P. Schwarz, Djamel Mékarnia, Amaury H. M. J. Triaud, Lyu Abe, Olga Suarez, Tristan Guillot, Dennis M. Conti, Karen A. Collins, Ian A. Waite, John F. Kielkopf, Kevin I. Collins, Stefan Dreizler, Mohammed El Mufti, Dax L. Feliz, Eric Gaidos, Claire S. Geneser, Keith D. Horne, Stephen R. Kane, Patrick J. Lowrance, Eder Martioli, Don J. Radford, Michael A. Reefe, Veronica Roccatagliata, Avi Shporer, Keivan G. Stassun, Christopher Stockdale, Thiam-Guan Tan, Angelle M. Tanner, Laura D. Vega
Figure caption: Raw TESS photometry of AU Mic overlaid with observed transits of AU Mic b (red) and c (blue) and a range of predicted transit midpoint times for AU Mic d (green), with P d = 5.07 days (first row), 5.39 days (second row), 5.64 days (third row), 5.86 days (fourth row), 6.20 days (fifth row), 6.47 days (sixth row), 11.9 days (seventh row), 12.6 days (eighth row), and 14.1 days (ninth row). Left column is from Cycle 1, and right column is from Cycle 3. Owing to AU Mic d’s estimated 160 ppm depth and AU Mic’s intense stellar activity, the potential transit signatures from AU Mic d are not obvious in these plots.
Paper: Validating AU Microscopii d with Transit Timing Variations
Authors: Justin M. Wittrock, Peter P. Plavchan, Bryson L. Cale, Thomas Barclay, Mathis R. Ludwig, Richard P. Schwarz, Djamel Mékarnia, Amaury H. M. J. Triaud, Lyu Abe, Olga Suarez, Tristan Guillot, Dennis M. Conti, Karen A. Collins, Ian A. Waite, John F. Kielkopf, Kevin I. Collins, Stefan Dreizler, Mohammed El Mufti, Dax L. Feliz, Eric Gaidos, Claire S. Geneser, Keith D. Horne, Stephen R. Kane, Patrick J. Lowrance, Eder Martioli, Don J. Radford, Michael A. Reefe, Veronica Roccatagliata, Avi Shporer, Keivan G. Stassun, Christopher Stockdale, Thiam-Guan Tan, Angelle M. Tanner, Laura D. Vega
Figure caption:  Exo-Striker-generated TTV models of AU Mic b (left) and c (right) projected over 10 yr since last observed transit of the AU Mic system. The observed TTVs (green) are included with the model (black), with P d = 5.07 days (first row), 5.39 days (second row), 5.64 days (third row), 5.86 days (fourth row), 6.20 days (fifth row), 6.47 days (sixth row), 11.9 days (seventh row), 12.6 days (eighth row), and 14.1 days (ninth row).
Paper: Validating AU Microscopii d with Transit Timing Variations
Authors: Justin M. Wittrock, Peter P. Plavchan, Bryson L. Cale, Thomas Barclay, Mathis R. Ludwig, Richard P. Schwarz, Djamel Mékarnia, Amaury H. M. J. Triaud, Lyu Abe, Olga Suarez, Tristan Guillot, Dennis M. Conti, Karen A. Collins, Ian A. Waite, John F. Kielkopf, Kevin I. Collins, Stefan Dreizler, Mohammed El Mufti, Dax L. Feliz, Eric Gaidos, Claire S. Geneser, Keith D. Horne, Stephen R. Kane, Patrick J. Lowrance, Eder Martioli, Don J. Radford, Michael A. Reefe, Veronica Roccatagliata, Avi Shporer, Keivan G. Stassun, Christopher Stockdale, Thiam-Guan Tan, Angelle M. Tanner, Laura D. Vega
Figure caption:  rebound models of the stability of the AU Mic system on a timescale of 2 Myr for P d = 5.08 days (first row left), 5.39 days (first row right), 5.64 days (second row left), 5.86 days (second row right), 6.20 days (third row left), 6.47 days (third row right), 11.9 days (fourth row left), 12.6 days (fourth row right), and 14.1 days (fifth row).
Paper: Lensing in the Blue. II. Estimating the Sensitivity of Stratospheric Balloons to Weak Gravitational Lensing
Authors: Jacqueline E. McCleary, Spencer W. Everett, Mohamed M. Shaaban, Ajay S. Gill, Georgios N. Vassilakis, Eric M. Huff, Richard J. Massey, Steven J. Benton, Anthony M. Brown, Paul Clark, Bradley Holder, Aurelien A. Fraisse, Mathilde Jauzac, William C. Jones, David Lagattuta, Jason S.-Y. Leung, Lun Li, Thuy Vy T. Luu, Johanna M. Nagy, C. Barth Netterfield, Emaad Paracha, Susan F. Redmond, Jason D. Rhodes, Jürgen Schmoll, Ellen Sirks, Sut Ieng Tam
Figure caption:  SUPERBIT transmission across the six filters planned for the 2023 flight and the now-deprecated shape-band, which will not be flown but is included here for comparative purposes.