Search Publications

Probing the Origin of Changing-look Quasar Transitions with Chandra
DOI: 10.3847/1538-4357/acdedd Bibcode: 2023ApJ...953...61Y

Green, Paul J.; Anderson, Scott F.; Bieryla, Allyson +9 more

Extremely variable quasars can also show strong changes in broad-line emission strength and are known as changing-look quasars (CLQs). To study the CLQ transition mechanism, we present a pilot sample of CLQs with X-ray observations in both the bright and faint states. From a sample of quasars with bright-state archival SDSS spectra and (Chandra or…

2023 The Astrophysical Journal
XMM-Newton 21
An R V Map of the Milky Way Revealed by LAMOST
DOI: 10.3847/1538-4365/acf764 Bibcode: 2023ApJS..269....6Z

Chen, Bingqiu; Yuan, Haibo; Zhang, Ruoyi

The total-to-selective extinction ratio, R V, is a key parameter for tracing the properties of interstellar dust, as it directly determines the variation of the extinction curve with wavelength. By utilizing accurate color excess measurements from the optical to the mid-infrared range, we have derived R V values for approxima…

2023 The Astrophysical Journal Supplement Series
Gaia 21
The data center for the Spectrometer and Telescope for Imaging X-rays (STIX) on board Solar Orbiter
DOI: 10.1051/0004-6361/202346031 Bibcode: 2023A&A...673A.142X

Massa, Paolo; Krucker, Säm; Piana, Michele +12 more

Context. The Spectrometer and Telescope for Imaging X-rays (STIX) on board Solar Orbiter observes solar X-ray emission in the range of 4-150 keV and produces spectra and images of solar flares over a wide range of flare magnitudes. During nominal operation, STIX continuously generates data. A constant data flow requires fully automated data-proces…

2023 Astronomy and Astrophysics
SolarOrbiter 21
Inferring the presence of very massive stars in local star-forming regions
DOI: 10.1051/0004-6361/202346732 Bibcode: 2023A&A...678A.159M

Schaerer, D.; Martins, F.; Marques-Chaves, R. +1 more

Context. Very massive stars (VMS) have masses in excess of 100 M and are rare. However, owing to their powerful winds, very high luminosity, and efficient nucleosynthesis, they are key players of star-forming regions. In particular, their strong ionizing fluxes impact the surrounding interstellar medium.
Aims: We aim at detecting …

2023 Astronomy and Astrophysics
eHST 21
The JWST PEARLS View of the El Gordo Galaxy Cluster and of the Structure It Magnifies
DOI: 10.3847/1538-4357/acd929 Bibcode: 2023ApJ...952...81F

Grogin, Norman A.; Koekemoer, Anton M.; Pirzkal, Nor +41 more

The massive galaxy cluster El Gordo (z = 0.87) imprints multitudes of gravitationally lensed arcs onto James Webb Space Telescope Near-Infrared Camera (NIRCam) images. Eight bands of NIRCam imaging were obtained in the "Prime Extragalactic Areas for Reionization and Lensing Science" ("PEARLS") program. Point-spread function-matched photometry acro…

2023 The Astrophysical Journal
eHST JWST 21
Delving deep: A population of extremely dusty dwarfs observed by JWST
DOI: 10.1051/0004-6361/202346219 Bibcode: 2023A&A...676A..76B

Rodighiero, G.; Kartaltepe, J. S.; Dickinson, M. +21 more


Aims: We take advantage of the NIRCam photometric observations available as part of the Cosmic Evolution Early Release Science survey (CEERS) to identify and analyse very red sources in an effort to discover very dusty star forming galaxies.
Methods: We select red galaxies as objects with a S/N > 3 at 4.4 µm and a S/N < 2 in …

2023 Astronomy and Astrophysics
eHST JWST 21
Unifying High- and Low-resolution Observations to Constrain the Dayside Atmosphere of KELT-20b/MASCARA-2b
DOI: 10.3847/1538-3881/ac9f40 Bibcode: 2023AJ....165....7K

Fu, Guangwei; Brogi, Matteo; Désert, Jean-Michel +10 more

We present high-resolution dayside thermal emission observations of the exoplanet KELT-20b/MASCARA-2b using the MAROON-X spectrograph. Applying the cross-correlation method with both empirical and theoretical masks and a retrieval analysis, we confirm previous detections of Fe I emission lines and we detect Ni I for the first time in the planet (a…

2023 The Astronomical Journal
eHST 21
Uncovering the stellar structure of the dusty star-forming galaxy GN20 at z = 4.055 with MIRI/JWST
DOI: 10.1051/0004-6361/202346535 Bibcode: 2023A&A...673L...6C

Ilbert, O.; Nørgaard-Nielsen, H. U.; Östlin, G. +35 more

Luminous infrared galaxies at high redshifts (z > 4) include extreme starbursts that build their stellar mass over short periods of time, that is, of 100 Myr or less. These galaxies are considered to be the progenitors of massive quiescent galaxies at intermediate redshifts (z ∼ 2) but their stellar structure and buildup is unknown. Here, we pr…

2023 Astronomy and Astrophysics
Gaia eHST JWST 21
2023 Astrophotonics Roadmap: pathways to realizing multi-functional integrated astrophotonic instruments
DOI: 10.1088/2515-7647/ace869 Bibcode: 2023JPhP....5d2501J

Monnier, John D.; Anugu, Narsireddy; Kraus, Stefan +77 more

Photonic technologies offer numerous functionalities that can be used to realize astrophotonic instruments. The most spectacular example to date is the ESO Gravity instrument at the Very Large Telescope in Chile that combines the light-gathering power of four 8 m telescopes through a complex photonic interferometer. Fully integrated astrophotonic …

2023 Journal of Physics: Photonics
Gaia 21
TOI-3235 b: A Transiting Giant Planet around an M4 Dwarf Star
DOI: 10.3847/2041-8213/acbd9a Bibcode: 2023ApJ...946L...4H

Vanderburg, Andrew; Latham, David W.; Jordán, Andrés +34 more

We present the discovery of TOI-3235 b, a short-period Jupiter orbiting an M dwarf with a stellar mass close to the critical mass at which stars transition from partially to fully convective. TOI-3235 b was first identified as a candidate from TESS photometry and confirmed with radial velocities from ESPRESSO and ground-based photometry from HATSo…

2023 The Astrophysical Journal
Gaia 20