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Spatially resolved dust properties and quasar-galaxy decomposition of a hyper-luminous infrared galaxy at z = 4.4
DOI: 10.1093/mnras/stad1464 Bibcode: 2023MNRAS.523.4654T

Krumholz, Mark R.; Wisnioski, Emily; Tsukui, Takafumi +1 more

We report spatially resolved dust properties of the quasar host galaxy BRI1335-0417 at redshift z = 4.4 constrained by the Atacama Large Millimetre/submillimetre Array observations. The dust temperature map, derived from a greybody fit to rest frame 90 and 161 µm continuum images, shows a steep increase towards the centre, reaching 57.1 ± 0.…

2023 Monthly Notices of the Royal Astronomical Society
Gaia Herschel eHST 25
Direct observations of a complex coronal web driving highly structured slow solar wind
DOI: 10.1038/s41550-022-01834-5 Bibcode: 2023NatAs...7..133C

Chitta, L. P.; Seaton, D. B.; DeForest, C. E. +2 more

The solar wind consists of continuous streams of charged particles that escape into the heliosphere from the Sun, and is split into fast and slow components, with the fast wind emerging from the interiors of coronal holes. Near the ecliptic plane, the fast wind from low-latitude coronal holes is interspersed with a highly structured slow solar win…

2023 Nature Astronomy
SOHO 25
Gaia Data Release 3. The Gaia Andromeda Photometric Survey
DOI: 10.1051/0004-6361/202244204 Bibcode: 2023A&A...674A...4E

Audard, M.; Rimoldini, L.; Holl, B. +14 more

Context. As part of Gaia Data Release 3 (Gaia DR3), epoch photometry has been released for 1.2 million sources centred on M 31. This is a taster for Gaia Data Release 4 where all the epoch photometry will be released.
Aims: In this paper, the content of the Gaia Andromeda Photometric Survey (GAPS) is described, including statistics to assess …

2023 Astronomy and Astrophysics
Gaia 25
CEERS: Spatially Resolved UV and Mid-infrared Star Formation in Galaxies at 0.2 < z < 2.5: The Picture from the Hubble and James Webb Space Telescopes
DOI: 10.3847/1538-4357/acc944 Bibcode: 2023ApJ...950....7S

Papovich, Casey; Yang, Guang; Finkelstein, Steven L. +38 more

We present the mid-infrared (MIR) morphologies for 64 star-forming galaxies (SFGs) at 0.2 < z < 2.5 with stellar mass M * > 109 M using James Webb Space Telescope (JWST) Mid-Infrared Instrument (MIRI) observations from the Cosmic Evolution Early Release Science survey. The MIRI bands span the MIR (7.7-21…

2023 The Astrophysical Journal
eHST JWST 25
X-Ray Polarization of the BL Lacertae Type Blazar 1ES 0229+200
DOI: 10.3847/1538-4357/ad05c4 Bibcode: 2023ApJ...959...61E

Kaaret, Philip; Wu, Kinwah; Enoto, Teruaki +111 more

We present polarization measurements in the 2-8 keV band from blazar 1ES 0229+200, the first extreme high synchrotron peaked source to be observed by the Imaging X-ray Polarimetry Explorer (IXPE). Combining two exposures separated by about two weeks, we find the degree of polarization to be ΠX = 17.9% ± 2.8% at an electric-vector positi…

2023 The Astrophysical Journal
XMM-Newton 25
Pegasus W: An Ultrafaint Dwarf Galaxy Outside the Halo of M31 Not Quenched by Reionization
DOI: 10.3847/1538-4357/acaec9 Bibcode: 2023ApJ...944...14M

McQuinn, Kristen B. W.; Dolphin, Andrew E.; Cohen, Roger E. +3 more

We report the discovery of an ultrafaint dwarf (UFD) galaxy, Pegasus W, located on the far side of the Milky Way-M31 system and outside the virial radius of M31. The distance to the galaxy is ${915}_{-91}^{+60}$ kpc, measured using the luminosity of horizontal branch stars identified in Hubble Space Telescope optical imaging. The galaxy has a half…

2023 The Astrophysical Journal
eHST 25
The stellar halo in Local Group Hestia simulations. I. The in situ component and the effect of mergers
DOI: 10.1051/0004-6361/202244232 Bibcode: 2023A&A...677A..89K

Vogelsberger, Mark; Steinmetz, Matthias; Grand, Robert J. J. +12 more

Theory suggests that mergers play an important role in shaping galactic discs and stellar haloes, which was observationally confirmed in the Milky Way (MW) thanks to Gaia data. In this work, aiming to probe the contribution of mergers to the in situ stellar halo formation, we analyse six M 31 and MW analogues from the HESTIA suite of cosmological …

2023 Astronomy and Astrophysics
Gaia 25
Do Central Compact Objects have Carbon Atmospheres?
DOI: 10.3847/1538-4357/acaf55 Bibcode: 2023ApJ...944...36A

Halpern, J. P.; Alford, J. A. J.

Only three of the dozen central compact objects (CCOs) in supernova remnants (SNRs) show thermal X-ray pulsations due to nonuniform surface temperature (hot spots). The absence of X-ray pulsations from several unpulsed CCOs has motivated suggestions that they have uniform-temperature carbon atmospheres (UTCAs), which adequately fit their spectra w…

2023 The Astrophysical Journal
XMM-Newton 25
V-LoTSS: The circularly polarised LOFAR Two-metre Sky Survey
DOI: 10.1051/0004-6361/202245567 Bibcode: 2023A&A...670A.124C

White, G. J.; Bomans, D. J.; Ray, T. P. +44 more

We present the detection of 68 sources from the most sensitive radio survey in circular polarisation conducted to date. We used the second data release of the 144 MHz LOFAR Two-metre Sky Survey to produce circularly polarised maps with a median noise of 140 µJy beam−1 and resolution of 20″ for ≈27% of the northern sky (5634 deg2

2023 Astronomy and Astrophysics
Gaia 25
PHANGS-JWST First Results: The 21 µm Compact Source Population
DOI: 10.3847/2041-8213/aca8ab Bibcode: 2023ApJ...944L..21H

Sandstrom, Karin M.; Kruijssen, J. M. Diederik; Leroy, Adam K. +24 more

We use PHANGS-James Webb Space Telescope (JWST) data to identify and classify 1271 compact 21 µm sources in four nearby galaxies using MIRI F2100W data. We identify sources using a dendrogram-based algorithm, and we measure the background-subtracted flux densities for JWST bands from 2 to 21 µm. Using the spectral energy distribution (…

2023 The Astrophysical Journal
eHST JWST 25