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No Small-scale Radio Jets Here: Multiepoch Observations of Radio Continuum Structures in NGC 1068 with the VLBA
DOI: 10.3847/1538-4357/ace1f0 Bibcode: 2023ApJ...953...87F

Fischer, Travis C.; Secrest, Nathan J.; Crenshaw, D. Michael +2 more

We present recent Very Long Baseline Array (VLBA) 5 GHz radio observations of the nearby, luminous Seyfert 2 galaxy NGC 1068 for comparison to similar VLBA observations made on 1997 April 26. By cross-correlating the positions of emitting regions across both epochs, we find that spatially resolved extranuclear radio knots in this system have subre…

2023 The Astrophysical Journal
Gaia eHST 15
Sodium Brightening of (3200) Phaethon near Perihelion
DOI: 10.3847/PSJ/acc866 Bibcode: 2023PSJ.....4...70Z

Zhang, Qicheng; Knight, Matthew M.; Battams, Karl +2 more

Sunskirting asteroid (3200) Phaethon has been repeatedly observed in Solar Terrestrial Relations Observatory (STEREO) Heliospheric Imager 1 (HI1) imagery to anomalously brighten and produce an antisunward tail for a few days near each perihelion passage, phenomena previously attributed to the ejection of micron-sized dust grains. Color imaging by …

2023 The Planetary Science Journal
Gaia SOHO 15
Analysing the SEDs of protoplanetary disks with machine learning
DOI: 10.1051/0004-6361/202245461 Bibcode: 2023A&A...672A..30K

Pinte, C.; Woitke, P.; Kamp, I. +2 more

Context. The analysis of spectral energy distributions (SEDs) of protoplanetary disks to determine their physical properties is known to be highly degenerate. Hence, a full Bayesian analysis is required to obtain parameter uncertainties and degeneracies. The main challenge here is computational speed, as one proper full radiative transfer model re…

2023 Astronomy and Astrophysics
Herschel ISO XMM-Newton 15
Contamination in TESS Light Curves: The Case of the Fast Yellow Pulsating Supergiants
DOI: 10.3847/1538-3881/accc31 Bibcode: 2023AJ....165..239P

Bell, Keaton J.; Pedersen, May G.

Given its large plate scale of 21″ pixel-1, analyses of data from the Transiting Exoplanet Survey Satellite (TESS) space telescope must be wary of source confusion from blended light curves, which creates the potential to attribute observed photometric variability to the wrong astrophysical source. We explore the impact of light curve c…

2023 The Astronomical Journal
Gaia 15
Hidden Cooling Flows in clusters of Galaxies II: a wider sample
DOI: 10.1093/mnras/stad507 Bibcode: 2023MNRAS.521.1794F

Fabian, A. C.; Pinto, C.; Ferland, G. J. +3 more

We have recently uncovered Hidden Cooling Flows (HCFs) in the XMM Reflection Grating Spectrometer spectra of three clusters of galaxies; Centaurus, Perseus, and A1835. Here, we search for them in a wider sample of objects: the X-ray brightest group NGC 5044; four moderate X-ray luminosity clusters Sersic 159, A262, A2052, and RX J0821; and three h…

2023 Monthly Notices of the Royal Astronomical Society
XMM-Newton 15
Detection of Carbon Monoxide's 4.6 Micron Fundamental Band Structure in WASP-39b's Atmosphere with JWST NIRSpec G395H
DOI: 10.3847/2041-8213/acd544 Bibcode: 2023ApJ...949L..15G

Mikal-Evans, Thomas; Stevenson, Kevin B.; Kirk, James +29 more

Carbon monoxide (CO) is predicted to be the dominant carbon-bearing molecule in giant planet atmospheres and, along with water, is important for discerning the oxygen and therefore carbon-to-oxygen ratio of these planets. The fundamental absorption mode of CO has a broad, double-branched structure composed of many individual absorption lines from …

2023 The Astrophysical Journal
JWST 14
The Imprint of Clump Formation at High Redshift. II. The Chemistry of the Bulge
DOI: 10.3847/1538-4357/acbb00 Bibcode: 2023ApJ...946..118D

Fisher, Deanne B.; Nidever, David L.; Valenti, Elena +11 more

In Paper I, we showed that clumps in high-redshift galaxies, having a high star formation rate density (ΣSFR), produce disks with two tracks in the [Fe/H]-[α/Fe] chemical space, similar to that of the Milky Way's (MW's) thin+thick disks. Here we investigate the effect of clumps on the bulge's chemistry. The chemistry of the MW's bulge i…

2023 The Astrophysical Journal
Gaia 14
A Southern Photometric Quasar Catalog from the Dark Energy Survey Data Release 2
DOI: 10.3847/1538-4365/ac9ea8 Bibcode: 2023ApJS..264....9Y

Shen, Yue; Yang, Qian

We present a catalog of 1.4 million photometrically selected quasar candidates in the southern hemisphere over the ~5000 deg2 Dark Energy Survey (DES) wide survey area. We combine optical photometry from the DES second data release (DR2) with available near-infrared (NIR) and the all-sky unWISE mid-infrared photometry in the selection. …

2023 The Astrophysical Journal Supplement Series
Gaia 14
The Stellar Mass-Black Hole Mass Relation at z 2 down to {{M }}_{\mathrm{BH}}∼ {10}(7} {M) _{⊙ } Determined by HETDEX
DOI: 10.3847/1538-4357/acc2c2 Bibcode: 2023ApJ...948..103Z

Ono, Yoshiaki; Ouchi, Masami; Finkelstein, Steven L. +14 more

We investigate the stellar mass-black hole mass ( ${{ \mathcal M }}_{* }\mbox{--}{{ \mathcal M }}_{\mathrm{BH}}$ ) relation with type 1 active galactic nuclei (AGNs) down to ${{ \mathcal M }}_{\mathrm{BH}}={10}^{7\,}{M}_{\odot }$ , corresponding to a ≃ -21 absolute magnitude in rest-frame ultraviolet, at z = 2-2.5. Exploiting the deep and large-ar…

2023 The Astrophysical Journal
JWST 14
ED-2: A cold but not so narrow stellar stream crossing the solar neighbourhood
DOI: 10.1051/0004-6361/202347076 Bibcode: 2023A&A...678A.115B

Helmi, A.; Balbinot, E.; Ruiz-Lara, T. +3 more

Context. ED-2 is a stellar stream identified as a compact group in integrals-of-motion space in a local sample of halo stars from the third Gaia data release.
Aims: We investigate its nature and possible association with known halo substructures.
Methods: We explored the current properties of ED-2 members in phase-space and also analysed…

2023 Astronomy and Astrophysics
Gaia 14