adsabs/AstroCLIMB huggingface dataset:
Paper: TOI-1452 b: SPIRou and TESS Reveal a Super-Earth in a Temperate Orbit Transiting an M4 Dwarf
Authors: Charles Cadieux, René Doyon, Mykhaylo Plotnykov, Guillaume Hébrard, Farbod Jahandar, Étienne Artigau, Diana Valencia, Neil J. Cook, Eder Martioli, Thomas Vandal, Jean-François Donati, Ryan Cloutier, Norio Narita, Akihiko Fukui, Teruyuki Hirano, François Bouchy, Nicolas B. Cowan, Erica J. Gonzales, David R. Ciardi, Keivan G. Stassun, Luc Arnold, Björn Benneke, Isabelle Boisse, Xavier Bonfils, Andrés Carmona, Pía Cortés-Zuleta, Xavier Delfosse, Thierry Forveille, Pascal Fouqué, João Gomes da Silva, Jon M. Jenkins, Flavien Kiefer, Ágnes Kóspál, David Lafrenière, Jorge H. C. Martins, Claire Moutou, J.-D. do Nascimento, Merwan Ould-Elhkim, Stefan Pelletier, Joseph D. Twicken, Luke G. Bouma, Scott Cartwright, Antoine Darveau-Bernier, Konstantin Grankin, Masahiro Ikoma, Taiki Kagetani, Kiyoe Kawauchi, Takanori Kodama, Takayuki Kotani, David W. Latham, Kristen Menou, George Ricker, Sara Seager, Motohide Tamura, Roland Vanderspek, Noriharu Watanabe
Figure caption: Bayesian log-evidence (﹩\mathrm{ln}Z﹩) for different joint transit RV models (﹩{ \mathcal M }﹩) and RV data sets. The typical uncertainty on the ﹩{\rm{\Delta }}\mathrm{ln}Z﹩ is 0.7. The “zero”-planet model ﹩{{ \mathcal M }}_{0{\rm{p}}}﹩ has a fixed K = 0 m s−1. Single-planet models ﹩{{ \mathcal M }}_{1\mathrm{cp}}﹩ and ﹩{{ \mathcal M }}_{1\mathrm{ep}}﹩ correspond to an RV component with a circular (e = 0, ω = 90°) or eccentric (free e, ω) orbit, respectively. Models ﹩{{ \mathcal M }}_{1\mathrm{cp}+\mathrm{GP}}﹩ and ﹩{{ \mathcal M }}_{1\mathrm{ep}+\mathrm{GP}}﹩ add a Gaussian process to remove correlated noise in the RV data.
Paper: TOI-1452 b: SPIRou and TESS Reveal a Super-Earth in a Temperate Orbit Transiting an M4 Dwarf
Authors: Charles Cadieux, René Doyon, Mykhaylo Plotnykov, Guillaume Hébrard, Farbod Jahandar, Étienne Artigau, Diana Valencia, Neil J. Cook, Eder Martioli, Thomas Vandal, Jean-François Donati, Ryan Cloutier, Norio Narita, Akihiko Fukui, Teruyuki Hirano, François Bouchy, Nicolas B. Cowan, Erica J. Gonzales, David R. Ciardi, Keivan G. Stassun, Luc Arnold, Björn Benneke, Isabelle Boisse, Xavier Bonfils, Andrés Carmona, Pía Cortés-Zuleta, Xavier Delfosse, Thierry Forveille, Pascal Fouqué, João Gomes da Silva, Jon M. Jenkins, Flavien Kiefer, Ágnes Kóspál, David Lafrenière, Jorge H. C. Martins, Claire Moutou, J.-D. do Nascimento, Merwan Ould-Elhkim, Stefan Pelletier, Joseph D. Twicken, Luke G. Bouma, Scott Cartwright, Antoine Darveau-Bernier, Konstantin Grankin, Masahiro Ikoma, Taiki Kagetani, Kiyoe Kawauchi, Takanori Kodama, Takayuki Kotani, David W. Latham, Kristen Menou, George Ricker, Sara Seager, Motohide Tamura, Roland Vanderspek, Noriharu Watanabe
Figure caption: SEDs of TOI-1452 and TIC 420112587 fitted with a NextGen atmospheric model, respectively depicted with a black and a cyan line. Photometric measurements are represented with red (TOI-1452) and blue (TIC 420112587) error bars, where the horizontal bars represent the effective widths of the bandpasses and the small blue dots represent the model fluxes of TOI-1452 for comparison to the red symbols. The WISE measurements (3.4, 4.6, 12, and 22 μm), excluded from this analysis for including both star fluxes, agree with the sum of the two SEDs (green).
Paper: TOI-1452 b: SPIRou and TESS Reveal a Super-Earth in a Temperate Orbit Transiting an M4 Dwarf
Authors: Charles Cadieux, René Doyon, Mykhaylo Plotnykov, Guillaume Hébrard, Farbod Jahandar, Étienne Artigau, Diana Valencia, Neil J. Cook, Eder Martioli, Thomas Vandal, Jean-François Donati, Ryan Cloutier, Norio Narita, Akihiko Fukui, Teruyuki Hirano, François Bouchy, Nicolas B. Cowan, Erica J. Gonzales, David R. Ciardi, Keivan G. Stassun, Luc Arnold, Björn Benneke, Isabelle Boisse, Xavier Bonfils, Andrés Carmona, Pía Cortés-Zuleta, Xavier Delfosse, Thierry Forveille, Pascal Fouqué, João Gomes da Silva, Jon M. Jenkins, Flavien Kiefer, Ágnes Kóspál, David Lafrenière, Jorge H. C. Martins, Claire Moutou, J.-D. do Nascimento, Merwan Ould-Elhkim, Stefan Pelletier, Joseph D. Twicken, Luke G. Bouma, Scott Cartwright, Antoine Darveau-Bernier, Konstantin Grankin, Masahiro Ikoma, Taiki Kagetani, Kiyoe Kawauchi, Takanori Kodama, Takayuki Kotani, David W. Latham, Kristen Menou, George Ricker, Sara Seager, Motohide Tamura, Roland Vanderspek, Noriharu Watanabe
Figure caption: Ground-based transit follow-up of TOI-1452.01 on 2021 September 8 UT with the multifilter (﹩{g}^{{\prime} }﹩, ﹩{r}^{{\prime} }﹩, ﹩{i}^{{\prime} }﹩, z s) MuSCAT3 instrument installed on LCO-FTN at Haleakala Observatory. For each corresponding filter, the black points depict the binned photometry (8 minute temporal bin). The color coded curves correspond to each filter’s best-fit transit model (described in Section 4.3), with their respective 68% confidence interval envelope in lighter shade. The residuals are shown below each phase-folded transit.
Paper: TOI-1452 b: SPIRou and TESS Reveal a Super-Earth in a Temperate Orbit Transiting an M4 Dwarf
Authors: Charles Cadieux, René Doyon, Mykhaylo Plotnykov, Guillaume Hébrard, Farbod Jahandar, Étienne Artigau, Diana Valencia, Neil J. Cook, Eder Martioli, Thomas Vandal, Jean-François Donati, Ryan Cloutier, Norio Narita, Akihiko Fukui, Teruyuki Hirano, François Bouchy, Nicolas B. Cowan, Erica J. Gonzales, David R. Ciardi, Keivan G. Stassun, Luc Arnold, Björn Benneke, Isabelle Boisse, Xavier Bonfils, Andrés Carmona, Pía Cortés-Zuleta, Xavier Delfosse, Thierry Forveille, Pascal Fouqué, João Gomes da Silva, Jon M. Jenkins, Flavien Kiefer, Ágnes Kóspál, David Lafrenière, Jorge H. C. Martins, Claire Moutou, J.-D. do Nascimento, Merwan Ould-Elhkim, Stefan Pelletier, Joseph D. Twicken, Luke G. Bouma, Scott Cartwright, Antoine Darveau-Bernier, Konstantin Grankin, Masahiro Ikoma, Taiki Kagetani, Kiyoe Kawauchi, Takanori Kodama, Takayuki Kotani, David W. Latham, Kristen Menou, George Ricker, Sara Seager, Motohide Tamura, Roland Vanderspek, Noriharu Watanabe
Figure caption: SPIRou observation of the Al I line (1675.514 nm) of TOI-1452 (black dashed line). Top panel: The solid lines represent the ACES models for a fixed metallicity of 0.1 dex and T eff values of 3060 K, 3160 K, and 3260 K. Bottom panel: Same as top panel, but the ACES models have a fixed T eff = 3160 K and metallicity values of −0.2 dex, 0.1 dex and 0.5 dex. These plots illustrate the good sensitivity of near-IR high-resolution spectroscopy for constraining both the metallicity and effective temperature of M dwarfs.
Paper: TOI-1452 b: SPIRou and TESS Reveal a Super-Earth in a Temperate Orbit Transiting an M4 Dwarf
Authors: Charles Cadieux, René Doyon, Mykhaylo Plotnykov, Guillaume Hébrard, Farbod Jahandar, Étienne Artigau, Diana Valencia, Neil J. Cook, Eder Martioli, Thomas Vandal, Jean-François Donati, Ryan Cloutier, Norio Narita, Akihiko Fukui, Teruyuki Hirano, François Bouchy, Nicolas B. Cowan, Erica J. Gonzales, David R. Ciardi, Keivan G. Stassun, Luc Arnold, Björn Benneke, Isabelle Boisse, Xavier Bonfils, Andrés Carmona, Pía Cortés-Zuleta, Xavier Delfosse, Thierry Forveille, Pascal Fouqué, João Gomes da Silva, Jon M. Jenkins, Flavien Kiefer, Ágnes Kóspál, David Lafrenière, Jorge H. C. Martins, Claire Moutou, J.-D. do Nascimento, Merwan Ould-Elhkim, Stefan Pelletier, Joseph D. Twicken, Luke G. Bouma, Scott Cartwright, Antoine Darveau-Bernier, Konstantin Grankin, Masahiro Ikoma, Taiki Kagetani, Kiyoe Kawauchi, Takanori Kodama, Takayuki Kotani, David W. Latham, Kristen Menou, George Ricker, Sara Seager, Motohide Tamura, Roland Vanderspek, Noriharu Watanabe
Figure caption: Distribution of OH abundance measurements from 72 isolated OH lines in the SPIRou combined spectrum of TOI-1452. The inherent, per-line uncertainty (0.13 dex) is inferred from a Gaussian fit of this distribution. This uncertainty does not take into account possible systematic errors of the stellar atmosphere models.
Paper: TOI-1452 b: SPIRou and TESS Reveal a Super-Earth in a Temperate Orbit Transiting an M4 Dwarf
Authors: Charles Cadieux, René Doyon, Mykhaylo Plotnykov, Guillaume Hébrard, Farbod Jahandar, Étienne Artigau, Diana Valencia, Neil J. Cook, Eder Martioli, Thomas Vandal, Jean-François Donati, Ryan Cloutier, Norio Narita, Akihiko Fukui, Teruyuki Hirano, François Bouchy, Nicolas B. Cowan, Erica J. Gonzales, David R. Ciardi, Keivan G. Stassun, Luc Arnold, Björn Benneke, Isabelle Boisse, Xavier Bonfils, Andrés Carmona, Pía Cortés-Zuleta, Xavier Delfosse, Thierry Forveille, Pascal Fouqué, João Gomes da Silva, Jon M. Jenkins, Flavien Kiefer, Ágnes Kóspál, David Lafrenière, Jorge H. C. Martins, Claire Moutou, J.-D. do Nascimento, Merwan Ould-Elhkim, Stefan Pelletier, Joseph D. Twicken, Luke G. Bouma, Scott Cartwright, Antoine Darveau-Bernier, Konstantin Grankin, Masahiro Ikoma, Taiki Kagetani, Kiyoe Kawauchi, Takanori Kodama, Takayuki Kotani, David W. Latham, Kristen Menou, George Ricker, Sara Seager, Motohide Tamura, Roland Vanderspek, Noriharu Watanabe
Figure caption: PSF photometry relative light curve (TOI-1452 to TIC 420112587 flux ratio) from OMM-PESTO on 2020 February 22. The dotted black lines represent the ingress and egress of the transit estimated from contemporaneous TESS sector 22 data. The light curve is normalized with the out-of-transit median. A flux deficit comparable to the TESS transit depth is detected on TOI-1452 during transit.
Paper: TOI-1452 b: SPIRou and TESS Reveal a Super-Earth in a Temperate Orbit Transiting an M4 Dwarf
Authors: Charles Cadieux, René Doyon, Mykhaylo Plotnykov, Guillaume Hébrard, Farbod Jahandar, Étienne Artigau, Diana Valencia, Neil J. Cook, Eder Martioli, Thomas Vandal, Jean-François Donati, Ryan Cloutier, Norio Narita, Akihiko Fukui, Teruyuki Hirano, François Bouchy, Nicolas B. Cowan, Erica J. Gonzales, David R. Ciardi, Keivan G. Stassun, Luc Arnold, Björn Benneke, Isabelle Boisse, Xavier Bonfils, Andrés Carmona, Pía Cortés-Zuleta, Xavier Delfosse, Thierry Forveille, Pascal Fouqué, João Gomes da Silva, Jon M. Jenkins, Flavien Kiefer, Ágnes Kóspál, David Lafrenière, Jorge H. C. Martins, Claire Moutou, J.-D. do Nascimento, Merwan Ould-Elhkim, Stefan Pelletier, Joseph D. Twicken, Luke G. Bouma, Scott Cartwright, Antoine Darveau-Bernier, Konstantin Grankin, Masahiro Ikoma, Taiki Kagetani, Kiyoe Kawauchi, Takanori Kodama, Takayuki Kotani, David W. Latham, Kristen Menou, George Ricker, Sara Seager, Motohide Tamura, Roland Vanderspek, Noriharu Watanabe
Figure caption: Chemical abundances of 12 different elements via line-by-line spectroscopy of 151 spectral features. The dashed line represents the average metallicity of the star corresponding to the average of all elements.
Paper: TOI-1452 b: SPIRou and TESS Reveal a Super-Earth in a Temperate Orbit Transiting an M4 Dwarf
Authors: Charles Cadieux, René Doyon, Mykhaylo Plotnykov, Guillaume Hébrard, Farbod Jahandar, Étienne Artigau, Diana Valencia, Neil J. Cook, Eder Martioli, Thomas Vandal, Jean-François Donati, Ryan Cloutier, Norio Narita, Akihiko Fukui, Teruyuki Hirano, François Bouchy, Nicolas B. Cowan, Erica J. Gonzales, David R. Ciardi, Keivan G. Stassun, Luc Arnold, Björn Benneke, Isabelle Boisse, Xavier Bonfils, Andrés Carmona, Pía Cortés-Zuleta, Xavier Delfosse, Thierry Forveille, Pascal Fouqué, João Gomes da Silva, Jon M. Jenkins, Flavien Kiefer, Ágnes Kóspál, David Lafrenière, Jorge H. C. Martins, Claire Moutou, J.-D. do Nascimento, Merwan Ould-Elhkim, Stefan Pelletier, Joseph D. Twicken, Luke G. Bouma, Scott Cartwright, Antoine Darveau-Bernier, Konstantin Grankin, Masahiro Ikoma, Taiki Kagetani, Kiyoe Kawauchi, Takanori Kodama, Takayuki Kotani, David W. Latham, Kristen Menou, George Ricker, Sara Seager, Motohide Tamura, Roland Vanderspek, Noriharu Watanabe
Figure caption:  K-band 5σ contrast curve of TOI-1452 from Keck II/NIRC2 adaptive optics imaging. No close companion is detected.
Paper: TOI-1452 b: SPIRou and TESS Reveal a Super-Earth in a Temperate Orbit Transiting an M4 Dwarf
Authors: Charles Cadieux, René Doyon, Mykhaylo Plotnykov, Guillaume Hébrard, Farbod Jahandar, Étienne Artigau, Diana Valencia, Neil J. Cook, Eder Martioli, Thomas Vandal, Jean-François Donati, Ryan Cloutier, Norio Narita, Akihiko Fukui, Teruyuki Hirano, François Bouchy, Nicolas B. Cowan, Erica J. Gonzales, David R. Ciardi, Keivan G. Stassun, Luc Arnold, Björn Benneke, Isabelle Boisse, Xavier Bonfils, Andrés Carmona, Pía Cortés-Zuleta, Xavier Delfosse, Thierry Forveille, Pascal Fouqué, João Gomes da Silva, Jon M. Jenkins, Flavien Kiefer, Ágnes Kóspál, David Lafrenière, Jorge H. C. Martins, Claire Moutou, J.-D. do Nascimento, Merwan Ould-Elhkim, Stefan Pelletier, Joseph D. Twicken, Luke G. Bouma, Scott Cartwright, Antoine Darveau-Bernier, Konstantin Grankin, Masahiro Ikoma, Taiki Kagetani, Kiyoe Kawauchi, Takanori Kodama, Takayuki Kotani, David W. Latham, Kristen Menou, George Ricker, Sara Seager, Motohide Tamura, Roland Vanderspek, Noriharu Watanabe
Figure caption: Top panel: Monitoring of the longitudinal magnetic field (B  ℓ ) of TOI-1452 with SPIRou. Bottom panel: Lomb–Scargle periodogram of the B  ℓ  time series. No clear periodic signal is detected, suggesting a relatively quiet star.
Paper: Calibration of the IXPE Focal Plane X-Ray Polarimeters to Polarized Radiation
Authors: Alessandro Di Marco, Sergio Fabiani, Fabio La Monaca, Fabio Muleri, John Rankin, Paolo Soffitta, Fei Xie, Fabrizio Amici, Primo attinà, Matteo Bachetti, Luca Baldini, Mattia Barbanera, Wayne Baumgartner, Ronaldo Bellazzini, Fabio Borotto, Alessandro Brez, Daniele Brienza, Ciro Caporale, Claudia Cardelli, Rita Carpentiero, Simone Castellano, Marco Castronuovo, Luca Cavalli, Elisabetta Cavazzuti, Marco Ceccanti, Mauro Centrone, Saverio Citraro, Enrico Costa, Elisa D'Alba, Fabio D'Amico, Ettore Del Monte, Sergio Di Cosimo, Niccolò Di Lalla, Giuseppe Di Persio, Immacolata Donnarumma, Yuri Evangelista, Riccardo Ferrazzoli, Luca Latronico, Carlo Lefevre, Pasqualino Loffredo, Paolo Lorenzi, Leonardo Lucchesi, Carlo Magazzù, Guido Magazzù, Simone Maldera, Alberto Manfreda, Elio Mangraviti, Marco Marengo, Giorgio Matt, Paolo Mereu, Massimo Minuti, Alfredo Morbidini, Federico Mosti, Hikmat Nasimi, Barbara Negri, Alessio Nuti, Stephen L. O'Dell, Leonardo Orsini, Matteo Perri, Melissa Pesce-Rollins, Raffaele Piazzolla, Stefano Pieraccini, Maura Pilia, Michele Pinchera, Alessandro Profeti, Simonetta Puccetti, Brian D. Ramsey, Ajay Ratheesh, Alda Rubini, Francesco Santoli, Paolo Sarra, Emanuele Scalise, Andrea Sciortino, Carmelo Sgrò, Gloria Spandre, Marcello Tardiola, Allyn F. Tennant, Antonino Tobia, Alessio Trois, Marco Vimercati, Martin C. Weisskopf, Davide Zanetti, Francesco Zanetti
Figure caption: Deviation from the expected phase for polarization angle for each DU and energy. Data points are fitted with a constant line (dashed line).
Paper: Calibration of the IXPE Focal Plane X-Ray Polarimeters to Polarized Radiation
Authors: Alessandro Di Marco, Sergio Fabiani, Fabio La Monaca, Fabio Muleri, John Rankin, Paolo Soffitta, Fei Xie, Fabrizio Amici, Primo attinà, Matteo Bachetti, Luca Baldini, Mattia Barbanera, Wayne Baumgartner, Ronaldo Bellazzini, Fabio Borotto, Alessandro Brez, Daniele Brienza, Ciro Caporale, Claudia Cardelli, Rita Carpentiero, Simone Castellano, Marco Castronuovo, Luca Cavalli, Elisabetta Cavazzuti, Marco Ceccanti, Mauro Centrone, Saverio Citraro, Enrico Costa, Elisa D'Alba, Fabio D'Amico, Ettore Del Monte, Sergio Di Cosimo, Niccolò Di Lalla, Giuseppe Di Persio, Immacolata Donnarumma, Yuri Evangelista, Riccardo Ferrazzoli, Luca Latronico, Carlo Lefevre, Pasqualino Loffredo, Paolo Lorenzi, Leonardo Lucchesi, Carlo Magazzù, Guido Magazzù, Simone Maldera, Alberto Manfreda, Elio Mangraviti, Marco Marengo, Giorgio Matt, Paolo Mereu, Massimo Minuti, Alfredo Morbidini, Federico Mosti, Hikmat Nasimi, Barbara Negri, Alessio Nuti, Stephen L. O'Dell, Leonardo Orsini, Matteo Perri, Melissa Pesce-Rollins, Raffaele Piazzolla, Stefano Pieraccini, Maura Pilia, Michele Pinchera, Alessandro Profeti, Simonetta Puccetti, Brian D. Ramsey, Ajay Ratheesh, Alda Rubini, Francesco Santoli, Paolo Sarra, Emanuele Scalise, Andrea Sciortino, Carmelo Sgrò, Gloria Spandre, Marcello Tardiola, Allyn F. Tennant, Antonino Tobia, Alessio Trois, Marco Vimercati, Martin C. Weisskopf, Davide Zanetti, Francesco Zanetti
Figure caption: Modulation factor (top) and polarization angle systematic (bottom) as a function of energy. IXPE scientific requirements are reported in black. Mean values for the polarization angle systematic for each DU is reported as a dashed line.
Paper: Calibration of the IXPE Focal Plane X-Ray Polarimeters to Polarized Radiation
Authors: Alessandro Di Marco, Sergio Fabiani, Fabio La Monaca, Fabio Muleri, John Rankin, Paolo Soffitta, Fei Xie, Fabrizio Amici, Primo attinà, Matteo Bachetti, Luca Baldini, Mattia Barbanera, Wayne Baumgartner, Ronaldo Bellazzini, Fabio Borotto, Alessandro Brez, Daniele Brienza, Ciro Caporale, Claudia Cardelli, Rita Carpentiero, Simone Castellano, Marco Castronuovo, Luca Cavalli, Elisabetta Cavazzuti, Marco Ceccanti, Mauro Centrone, Saverio Citraro, Enrico Costa, Elisa D'Alba, Fabio D'Amico, Ettore Del Monte, Sergio Di Cosimo, Niccolò Di Lalla, Giuseppe Di Persio, Immacolata Donnarumma, Yuri Evangelista, Riccardo Ferrazzoli, Luca Latronico, Carlo Lefevre, Pasqualino Loffredo, Paolo Lorenzi, Leonardo Lucchesi, Carlo Magazzù, Guido Magazzù, Simone Maldera, Alberto Manfreda, Elio Mangraviti, Marco Marengo, Giorgio Matt, Paolo Mereu, Massimo Minuti, Alfredo Morbidini, Federico Mosti, Hikmat Nasimi, Barbara Negri, Alessio Nuti, Stephen L. O'Dell, Leonardo Orsini, Matteo Perri, Melissa Pesce-Rollins, Raffaele Piazzolla, Stefano Pieraccini, Maura Pilia, Michele Pinchera, Alessandro Profeti, Simonetta Puccetti, Brian D. Ramsey, Ajay Ratheesh, Alda Rubini, Francesco Santoli, Paolo Sarra, Emanuele Scalise, Andrea Sciortino, Carmelo Sgrò, Gloria Spandre, Marcello Tardiola, Allyn F. Tennant, Antonino Tobia, Alessio Trois, Marco Vimercati, Martin C. Weisskopf, Davide Zanetti, Francesco Zanetti
Figure caption: Modulation factor as a function of the expected polarization angle for the four DUs. Dashed lines represent the modulation factor mean values.
Paper: Calibration of the IXPE Focal Plane X-Ray Polarimeters to Polarized Radiation
Authors: Alessandro Di Marco, Sergio Fabiani, Fabio La Monaca, Fabio Muleri, John Rankin, Paolo Soffitta, Fei Xie, Fabrizio Amici, Primo attinà, Matteo Bachetti, Luca Baldini, Mattia Barbanera, Wayne Baumgartner, Ronaldo Bellazzini, Fabio Borotto, Alessandro Brez, Daniele Brienza, Ciro Caporale, Claudia Cardelli, Rita Carpentiero, Simone Castellano, Marco Castronuovo, Luca Cavalli, Elisabetta Cavazzuti, Marco Ceccanti, Mauro Centrone, Saverio Citraro, Enrico Costa, Elisa D'Alba, Fabio D'Amico, Ettore Del Monte, Sergio Di Cosimo, Niccolò Di Lalla, Giuseppe Di Persio, Immacolata Donnarumma, Yuri Evangelista, Riccardo Ferrazzoli, Luca Latronico, Carlo Lefevre, Pasqualino Loffredo, Paolo Lorenzi, Leonardo Lucchesi, Carlo Magazzù, Guido Magazzù, Simone Maldera, Alberto Manfreda, Elio Mangraviti, Marco Marengo, Giorgio Matt, Paolo Mereu, Massimo Minuti, Alfredo Morbidini, Federico Mosti, Hikmat Nasimi, Barbara Negri, Alessio Nuti, Stephen L. O'Dell, Leonardo Orsini, Matteo Perri, Melissa Pesce-Rollins, Raffaele Piazzolla, Stefano Pieraccini, Maura Pilia, Michele Pinchera, Alessandro Profeti, Simonetta Puccetti, Brian D. Ramsey, Ajay Ratheesh, Alda Rubini, Francesco Santoli, Paolo Sarra, Emanuele Scalise, Andrea Sciortino, Carmelo Sgrò, Gloria Spandre, Marcello Tardiola, Allyn F. Tennant, Antonino Tobia, Alessio Trois, Marco Vimercati, Martin C. Weisskopf, Davide Zanetti, Francesco Zanetti
Figure caption: Modulation factor for the inclined measurements at 2.7 keV. They are compatible with a constant as expected.
Paper: Gap Opening and Inner Disk Structure in the Strongly Accreting Transition Disk of DM Tau
Authors: Logan Francis, Nienke van der Marel, Doug Johnstone, Eiji Akiyama, Simon Bruderer, Ruobing Dong, Jun Hashimoto, Hauyu Baobab Liu, Takayuki Muto, Yi Yang
Figure caption: Comparison of the fiducial DM Tau DALI model and a model with no inner dust disk (δ dust1 = δ dust2 = 10−50) with the DM Tau observations, as described in Section 5.2.1. Top row: deprojected and azimuthally averaged millimeter-continuum intensity, and SED zoomed in on the near-to-mid infrared region. Middle row: deprojected and azimuthally averaged intensity for the moment 0 maps of the 12CO, 13CO, and C18O lines.
Paper: Gap Opening and Inner Disk Structure in the Strongly Accreting Transition Disk of DM Tau
Authors: Logan Francis, Nienke van der Marel, Doug Johnstone, Eiji Akiyama, Simon Bruderer, Ruobing Dong, Jun Hashimoto, Hauyu Baobab Liu, Takayuki Muto, Yi Yang
Figure caption: Gas temperature in the fiducial DALI DM Tau model at the τ = 1 surface for the 12CO, 13CO, and C18O emission (red lines). The dashed vertical gray lines are at the inner cavity at 3.5 au and main dust cavity at 21 au, while the shaded blue region shows the CO freeze-out temperature range.
Paper: Gap Opening and Inner Disk Structure in the Strongly Accreting Transition Disk of DM Tau
Authors: Logan Francis, Nienke van der Marel, Doug Johnstone, Eiji Akiyama, Simon Bruderer, Ruobing Dong, Jun Hashimoto, Hauyu Baobab Liu, Takayuki Muto, Yi Yang
Figure caption: Comparison of the DM Tau observations (black lines and red circles for SED photometry) and fiducial model (blue lines). Top row: deprojected and azimuthally averaged millimeter-continuum intensity, overall SED, and SED zoomed in on the near-to-mid infrared region. Middle row: deprojected and azimuthally averaged intensity for the moment 0 maps of the 12CO, 13CO, and C18O lines. Bottom row: flux integrated over the disk vs. velocity for the 12CO, 13CO, and C18O line cubes. The spectral resolution of the observed line cubes is 1 km s−1, while the models are sampled in 0.5 km s−1 steps.
Paper: Gap Opening and Inner Disk Structure in the Strongly Accreting Transition Disk of DM Tau
Authors: Logan Francis, Nienke van der Marel, Doug Johnstone, Eiji Akiyama, Simon Bruderer, Ruobing Dong, Jun Hashimoto, Hauyu Baobab Liu, Takayuki Muto, Yi Yang
Figure caption: Surface density structure and selected 2D physical quantities from the fiducial DM Tau model plotted from 0 to 30 au. The τ = 1 surfaces for the 12CO, 13CO, and C18O lines are overlaid on each 2D DALI panel as the solid, dashed, and dotted lines, respectively, while the approximate freeze-out temperature of CO (25.5 K) is overlaid as the orange contour on the CO abundance panels.
Paper: Gap Opening and Inner Disk Structure in the Strongly Accreting Transition Disk of DM Tau
Authors: Logan Francis, Nienke van der Marel, Doug Johnstone, Eiji Akiyama, Simon Bruderer, Ruobing Dong, Jun Hashimoto, Hauyu Baobab Liu, Takayuki Muto, Yi Yang
Figure caption: The same fiducial DALI model as Figure 6, but zoomed in on the inner disk from 0 to 5 au.
Paper: Gap Opening and Inner Disk Structure in the Strongly Accreting Transition Disk of DM Tau
Authors: Logan Francis, Nienke van der Marel, Doug Johnstone, Eiji Akiyama, Simon Bruderer, Ruobing Dong, Jun Hashimoto, Hauyu Baobab Liu, Takayuki Muto, Yi Yang
Figure caption: Same as Figure 9, but for the effects of changing the gas surface density depletion within 21 au in the DALI model described in Section 5.2.3.
Paper: Gap Opening and Inner Disk Structure in the Strongly Accreting Transition Disk of DM Tau
Authors: Logan Francis, Nienke van der Marel, Doug Johnstone, Eiji Akiyama, Simon Bruderer, Ruobing Dong, Jun Hashimoto, Hauyu Baobab Liu, Takayuki Muto, Yi Yang
Figure caption: As Figure 9, but for the effects of changing the dust depletion within 3.5 au in the DALI model described in Section 5.2.2.
Paper: Gap Opening and Inner Disk Structure in the Strongly Accreting Transition Disk of DM Tau
Authors: Logan Francis, Nienke van der Marel, Doug Johnstone, Eiji Akiyama, Simon Bruderer, Ruobing Dong, Jun Hashimoto, Hauyu Baobab Liu, Takayuki Muto, Yi Yang
Figure caption: Same as Figure 9, but for the effects of changing the radius of the inner edge of the interior dust ring (r inner) in the DALI model described in Section 5.2.2.