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Zeta-Payne: A Fully Automated Spectrum Analysis Algorithm for the Milky Way Mapper Program of the SDSS-V Survey
DOI: 10.3847/1538-3881/ac5f49 Bibcode: 2022AJ....163..236S

Xiang, Maosheng; Ting, Yuan-Sen; Kollmeier, Juna A. +13 more

The Sloan Digital Sky Survey (SDSS) has recently initiated its fifth survey generation (SDSS-V), with a central focus on stellar spectroscopy. In particular, SDSS-V's Milky Way Mapper program will deliver multiepoch optical and near-infrared spectra for more than 5 × 106 stars across the entire sky, covering a large range in stellar mas…

2022 The Astronomical Journal
Gaia 13
Searching for TESS Photometric Variability of Possible JWST Spectrophotometric Standard Stars
DOI: 10.3847/1538-3881/ac4bce Bibcode: 2022AJ....163..136M

Gordon, Karl D.; Hermes, J. J.; Fleming, Scott W. +7 more

We use data from the Transiting Exoplanet Survey Satellite (TESS) to search for, and set limits on, optical to near-infrared photometric variability of the well-vetted, candidate James Webb Space Telescope (JWST) spectrophotometric standards. Our search of 37 of these candidate standards has revealed measurable periodic variability in 15 stars. Th…

2022 The Astronomical Journal
Gaia 13
Improved Orbital Constraints and Hα Photometric Monitoring of the Directly Imaged Protoplanet Analog HD 142527 B
DOI: 10.3847/1538-3881/ac73f4 Bibcode: 2022AJ....164...29B

Weinberger, Alycia J.; De Rosa, Robert J.; Pueyo, Laurent +9 more

Companions embedded in the cavities of transitional circumstellar disks have been observed to exhibit excess luminosity at Hα, an indication that they are actively accreting. We report 5 yr (2013-2018) of monitoring of the position and Hα excess luminosity of the embedded, accreting low-mass stellar companion HD 142527 B from the MagAO/VisAO instr…

2022 The Astronomical Journal
Gaia 13
Dynamical Star-forming History of Per OB2
DOI: 10.3847/1538-3881/ac7951 Bibcode: 2022AJ....164...57K

Stassun, Keivan G.; Kounkel, Marina; Deng, TingYan

We analyze the internal dynamics of young stars toward Perseus using Gaia EDR3 data, including Per OB2 and California Cloud. Interpreting the current dynamics, we speculate that Per OB2 may have formed from two separate clouds that have begun forming stars in close proximity to each other. IC 348 is caught in the middle between the two of them, in…

2022 The Astronomical Journal
Gaia 13
TOI-1670 b and c: An Inner Sub-Neptune with an Outer Warm Jupiter Unlikely to Have Originated from High-eccentricity Migration
DOI: 10.3847/1538-3881/ac5c4f Bibcode: 2022AJ....163..225T

Latham, David W.; Quinn, Samuel N.; Cochran, William D. +38 more

We report the discovery of two transiting planets around the bright (V = 9.9 mag) main-sequence F7 star TOI-1670 by the Transiting Exoplanet Survey Satellite. TOI-1670 b is a sub-Neptune ( ${R}_{{\rm{b}}}={2.06}_{-0.15}^{+0.19}$ R ) on a 10.9 day orbit, and TOI-1670 c is a warm Jupiter ( ${R}_{{\rm{c}}}={0.987}_{-0.025}^{+0.025}$ R

2022 The Astronomical Journal
Gaia 13
The TESS-Keck Survey. XI. Mass Measurements for Four Transiting Sub-Neptunes Orbiting K Dwarf TOI-1246
DOI: 10.3847/1538-3881/ac69e5 Bibcode: 2022AJ....163..293T

Lester, Kathryn V.; Bieryla, Allyson; Latham, David W. +78 more

Multiplanet systems are valuable arenas for investigating exoplanet architectures and comparing planetary siblings. TOI-1246 is one such system, with a moderately bright K dwarf (V = 11.6, K = 9.9) and four transiting sub-Neptunes identified by TESS with orbital periods of 4.31, 5.90, 18.66, and 37.92 days. We collected 130 radial velocity observa…

2022 The Astronomical Journal
Gaia 12
pterodactyls: A Tool to Uniformly Search and Vet for Young Transiting Planets in TESS Primary Mission Photometry
DOI: 10.3847/1538-3881/ac7b29 Bibcode: 2022AJ....164...78F

Pascucci, Ilaria; Ciardi, David R.; Giacalone, Steven +8 more

Kepler's short-period exoplanet population has revealed evolutionary features such as the Radius Valley and the Hot Neptune desert that are likely sculpted by atmospheric loss over time. These findings suggest that the primordial planet population is different from the Gyr-old Kepler population, and motivates exoplanet searches around young stars.…

2022 The Astronomical Journal
Gaia 12
Atmospheric Characterization of Hot Jupiter CoRoT-1 b Using the Wide Field Camera 3 on the Hubble Space Telescope
DOI: 10.3847/1538-3881/ac6cdb Bibcode: 2022AJ....164...19G

Deming, Drake; Zhou, Yifan; Schlawin, Everett +3 more

Exoplanet CoRoT-1 b is intriguing because we predict it to be a transitional planet between hot Jupiters (equilibrium temperatures ~1500 K) and ultrahot Jupiters (equilibrium temperatures >2000 K). In 2012, observations of CoRoT-1 b included one primary transit and three secondary eclipses with the Hubble Space Telescope (HST) Wide Field Camera…

2022 The Astronomical Journal
eHST 12
TOI-1696: A Nearby M4 Dwarf with a 3 R Planet in the Neptunian Desert
DOI: 10.3847/1538-3881/ac6bf8 Bibcode: 2022AJ....163..298M

Ikuta, Kai; Bieryla, Allyson; Latham, David W. +59 more

We present the discovery and validation of a temperate sub-Neptune around the nearby mid-M dwarf TIC 470381900 (TOI-1696), with a radius of 3.09 ± 0.11 R and an orbital period of 2.5 days, using a combination of Transiting Exoplanets Survey Satellite (TESS) and follow-up observations using ground-based telescopes. Joint analysis of mu…

2022 The Astronomical Journal
Gaia 12
Revisiting BD-06 1339b: A Likely False Positive Caused by Stellar Activity
DOI: 10.3847/1538-3881/ac5d41 Bibcode: 2022AJ....163..215S

Kane, Stephen R.; Pepper, Joshua; Fetherolf, Tara +3 more

As long as astronomers have searched for exoplanets, the intrinsic variability of host stars has interfered with the ability to reliably detect and confirm exoplanets. One particular source of false positives is the presence of stellar magnetic or chromospheric activity that can mimic the radial velocity reflex motion of a planet. Here we present …

2022 The Astronomical Journal
Gaia 12