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The distribution of detection significance ( ) for the 1CGH and 3FHL samp...

The distribution of detection significance ( ) for the 1CGH and 3FHL samp...

Published: 02 May 2025
Figure 1. The distribution of detection significance ( ) for the 1CGH and 3FHL samples (respectively, blue line and red dashed line).
Journal Article
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FLAMINGO: combining kinetic SZ effect and galaxy-galaxy lensing measurements to gauge the impact of feedback on large-scale structure

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Ian G McCarthy and others
Monthly Notices of the Royal Astronomical Society, staf731, https://doi.org/10.1093/mnras/staf731
Published: 02 May 2025
Journal Article
ACCEPTED MANUSCRIPT

Can planet–planet binaries survive in star-forming regions?

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Richard J Parker and others
Monthly Notices of the Royal Astronomical Society: Letters, slaf045, https://doi.org/10.1093/mnrasl/slaf045
Published: 02 May 2025
Journal Article
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A missing palaeomagnetic signal in Middle Devonian pillow lavas

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R A de Boer and others
Geophysical Journal International, ggaf151, https://doi.org/10.1093/gji/ggaf151
Published: 02 May 2025
Journal Article
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Searching for star formation towards the Eos molecular cloud

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Suryansh Saxena and others
Monthly Notices of the Royal Astronomical Society: Letters, slaf044, https://doi.org/10.1093/mnrasl/slaf044
Published: 02 May 2025
Image
The photon index ( ) versus the integral flux in the 10–800 GeV energy ba...

The photon index ( ) versus the integral flux in the 10–800 GeV energy ba...

Published: 02 May 2025
Figure 2. The photon index ( ) versus the integral flux in the 10–800 GeV energy band. The green points represent 1CGH sources with counterparts in both 3FHL and 4FGL-DR4 catalogues; the blue open diamonds represent 1CGH sources with counterparts in 4FGL-DR4 only; and the magenta circles represent new -r
Image
The CGH, showing the highest energy photon versus redshift, based on Fe...

The CGH, showing the highest energy photon versus redshift, based on Fe...

Published: 02 May 2025
Figure 4. The CGH, showing the highest energy photon versus redshift, based on Fermi -LAT ultra-clean events with PSF0 events removed ( evclass = 512 and evtype = 56 ). Sources detected above 10 GeV are represented, with robust (spectroscopic) redshifts marked as filled circles; lower limit redshifts are r
Journal Article

Mapping the cosmic gamma-ray horizon: the 1CGH catalogue of Fermi-LAT detections above 10 GeV

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Bruno Arsioli and others
Monthly Notices of the Royal Astronomical Society, Volume 539, Issue 2, May 2025, Pages 1458–1470, https://doi.org/10.1093/mnras/staf329
Published: 02 May 2025
Image
The redshift distribution for the 1CGH and 3FHL samples. For the 1CGH, the ...

The redshift distribution for the 1CGH and 3FHL samples. For the 1CGH, the ...

Published: 02 May 2025
Figure 3. The redshift distribution for the 1CGH and 3FHL samples. For the 1CGH, the histogram only includes sources with spectroscopic redshift determination ( z-flag  = 1); for the 3FHL catalogue, we include the entire sample.
Image
The CGH, showing the ‘largest energy bin detectable with Fermi-LAT...

The CGH, showing the ‘largest energy bin detectable with Fermi-LAT...

Published: 02 May 2025
Figure 5. The CGH, showing the ‘largest energy bin detectable with Fermi -LAT’ versus redshift. The ‘largest energy bin’ is calculated as the mean energy of the four highest energy source-type events associated with each source, excluding PSF0 events (i.e. evclass = 128 and evtype = 56 ). The opacity regi
Journal Article
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Geometric Mean Algebraic Reconstruction Technique : A tool for ionospheric tomography using GNSS receiver system

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Ajay Potdar and others
RAS Techniques and Instruments, rzaf015, https://doi.org/10.1093/rasti/rzaf015
Published: 02 May 2025
Journal Article
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Exogenic dust inventory in the Saturn system: the Cassini Cosmic Dust Analyzer perspective

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Nicolas Altobelli and others
Monthly Notices of the Royal Astronomical Society, staf656, https://doi.org/10.1093/mnras/staf656
Published: 02 May 2025
Journal Article
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Global distribution of earthquake-fault dip angles

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Roberto Basili and Mara Monica Tiberti
Geophysical Journal International, ggaf158, https://doi.org/10.1093/gji/ggaf158
Published: 02 May 2025
Journal Article
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DESI Peculiar Velocity Survey – Fundamental Plane

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Khaled Said and others
Monthly Notices of the Royal Astronomical Society, staf700, https://doi.org/10.1093/mnras/staf700
Published: 02 May 2025
Journal Article
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Estimating constraints on cosmological parameters via the canonical and the differential redshift drift with SKA HI 21-cm observations

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Jiangang Kang and others
Monthly Notices of the Royal Astronomical Society, staf664, https://doi.org/10.1093/mnras/staf664
Published: 01 May 2025
Journal Article
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High-resolution radio observations of massive protostars in the SARAO MeerKAT Galactic Plane Survey

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W O Obonyo and others
Monthly Notices of the Royal Astronomical Society, staf681, https://doi.org/10.1093/mnras/staf681
Published: 01 May 2025
Journal Article
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TOI-6478 b: a cold under-dense Neptune transiting a fully convective M dwarf from the thick disc

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Madison G Scott and others
Monthly Notices of the Royal Astronomical Society, staf684, https://doi.org/10.1093/mnras/staf684
Published: 01 May 2025
Journal Article
ACCEPTED MANUSCRIPT

Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback

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Piyush Sharda and others
Monthly Notices of the Royal Astronomical Society: Letters, slaf043, https://doi.org/10.1093/mnrasl/slaf043
Published: 01 May 2025
Journal Article
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Resolving the nature and putative nebular emission of GS9422: an obscured AGN without exotic stars

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Sandro Tacchella and others
Monthly Notices of the Royal Astronomical Society, staf718, https://doi.org/10.1093/mnras/staf718
Published: 01 May 2025
Journal Article
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Dust density enhancements and the direct formation of planetary cores in gravitationally unstable discs

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Ken Rice and others
Monthly Notices of the Royal Astronomical Society, staf714, https://doi.org/10.1093/mnras/staf714
Published: 01 May 2025