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Potential scientific synergies in weak lensing studies between the CSST and Euclid space probes
DOI: 10.1051/0004-6361/202243978 Bibcode: 2023A&A...669A.128L

Schrabback, T.; Zhang, J.; Kneib, J. P. +24 more


Aims: With the next generation of large surveys poised to join the ranks of observational cosmology in the near future, it is important to explore their potential synergies and to maximize their scientific outcomes. In this study, we aim to investigate the complementarity of two upcoming space missions: Euclid and the China Space Station Tele…

2023 Astronomy and Astrophysics
eHST 16
The Pristine dwarf galaxy survey-V. The edges of the dwarf galaxy Hercules
DOI: 10.1093/mnras/stad2227 Bibcode: 2023MNRAS.525.3086L

Sestito, Federico; Martin, Nicolas; Malhan, Khyati +6 more

We present a new spectroscopic study of 175 stars in the vicinity of the dwarf galaxy Hercules (d ~ 132 kpc) with data from the Anglo-Australian Telescope and its AAOmega spectrograph together with the Two Degree Field multi-object system to solve the conundrum that whether Hercules is tidally disrupting. We combine broad-band photometry, proper m…

2023 Monthly Notices of the Royal Astronomical Society
Gaia 16
Spectroscopy of QUBRICS quasar candidates: 1672 new redshifts and a golden sample for the Sandage test of the redshift drift
DOI: 10.1093/mnras/stad1007 Bibcode: 2023MNRAS.522.2019C

Grazian, Andrea; Boutsia, Konstantina; Cupani, Guido +10 more

The QUBRICS (QUasars as BRIght beacons for Cosmology in the Southern hemisphere) survey aims at constructing a sample of the brightest quasars with $z \lower.5ex\hbox{$\,\, \buildrel\gt \over \sim \,\,$}2.5$, observable with facilities in the Southern Hemisphere. QUBRICS makes use of the available optical and IR wide-field surveys in the South and…

2023 Monthly Notices of the Royal Astronomical Society
Gaia 16
JWST photometry of globular cluster populations in Abell 2744 at z = 0.3
DOI: 10.1093/mnras/stad2903 Bibcode: 2023MNRAS.526.2696H

Harris, William E.; Reina-Campos, Marta

JWST imaging of the rich galaxy cluster Abell 2744 at z = 0.308 has been used by the UNCOVER team to construct mosaic images in the NIRCam filters. The exceptionally deep images in the (F115W, F150W, and F200W) bands reveal a large population of unresolved point-like sources across the field, the vast majority of which are globular clusters (GCs) …

2023 Monthly Notices of the Royal Astronomical Society
JWST 16
A Measurement of the Cosmic Optical Background and Diffuse Galactic Light Scaling from the R < 50 au New Horizons-LORRI Data
DOI: 10.3847/1538-4357/acaa37 Bibcode: 2023ApJ...945...45S

Cooray, Asantha; Zemcov, Michael; Symons, Teresa +2 more

Direct photometric measurements of the cosmic optical background (COB) provide an important point of comparison to both other measurement methodologies and models of cosmic structure formation, and permit a cosmic consistency test with the potential to reveal additional diffuse sources of emission. The COB has been challenging to measure from Eart…

2023 The Astrophysical Journal
Gaia eHST 16
Magnetic Activity Evolution of Solar-like Stars. I. S ph-Age Relation Derived from Kepler Observations
DOI: 10.3847/1538-4357/acd118 Bibcode: 2023ApJ...952..131M

van Saders, Jennifer; García, Rafael A.; Breton, Sylvain N. +9 more

The ages of solar-like stars have been at the center of many studies such as exoplanet characterization or Galactic-archeology. While ages are usually computed from stellar evolution models, relations linking ages to other stellar properties, such as rotation and magnetic activity, have been investigated. With the large catalog of 55,232 rotation …

2023 The Astrophysical Journal
Gaia 16
A New Study on a Type Iax Stellar Remnant and its Probable Association with SN 1181
DOI: 10.3847/1538-4357/acb138 Bibcode: 2023ApJ...944..120L

Hillier, D. John; Parker, Quentin A.; Ritter, Andreas +4 more

We report observations and modeling of the stellar remnant and presumed double-degenerate merger of Type Iax supernova Pa 30, which is the probable remnant of SN 1181 AD. It is the only known bound stellar SN remnant and the only star with Wolf-Rayet features that is neither a planetary nebula central star nor a massive Population I progenitor. We…

2023 The Astrophysical Journal
AKARI Gaia INTEGRAL XMM-Newton eHST 16
The CGM2 Survey: Quenching and the Transformation of the Circumgalactic Medium
DOI: 10.3847/1538-4357/acc86a Bibcode: 2023ApJ...949...41T

Tripp, Todd M.; Prochaska, J. Xavier; Tejos, Nicolas +9 more

This study addresses how the incidence rate of strong O VI absorbers in a galaxy's circumgalactic medium (CGM) depends on galaxy mass and, independently, on the amount of star formation in the galaxy. We use Hubble Space Telescope/Cosmic Origins Spectrograph absorption spectroscopy of quasars to measure O VI absorption within 400 projected kpc and…

2023 The Astrophysical Journal
eHST 16
Analysis of the Young Open Cluster Trumpler 2 Using Gaia DR3 Data
DOI: 10.26650/PAR.2023.00001 Bibcode: 2023PARep...1....1T

Yontan, Talar; Tasdemir, Seval

We present an investigation of the open cluster Trumpler 2 using Gaia DR3 photometric, astrometric and spectroscopic data. 92 stars were identified as likely members of the cluster, with membership probabilities greater than 0.5. The mean proper-motion components of the cluster are derived as ($\mu_{\alpha}\cos \delta$, $\mu_{\delta}$)=($1.494 \pm…

2023 Physics and Astronomy Reports
Gaia 16
The first catalogue of spectroscopically confirmed red nuggets at z ∼ 0.7 from the VIPERS survey. Linking high-z red nuggets and local relics
DOI: 10.1051/0004-6361/202243616 Bibcode: 2023A&A...669A..95L

Pollo, Agnieszka; Małek, Katarzyna; Siudek, Małgorzata +4 more

Context. Red nuggets are a rare population of passive compact massive galaxies thought to be the first massive galaxies that formed in the Universe. First found at z ∼ 3, they are even less abundant at lower redshifts, and it is believed that with time they mostly transformed through mergers into today's giant ellipticals. The red nuggets that man…

2023 Astronomy and Astrophysics
eHST 16