All Outputs (74)

Revealing Prostate Calcification Heterogeneity through Their Elemental Distribution (2025)
Journal Article
Gosling, S. B., Arnold, E. L., Adams, L., Cool, P., Geraki, K., Kitchen, M. O., Lyburn, I. D., Rogers, K. D., Snow, T., Stone, N., & Greenwood, C. E. (2025). Revealing Prostate Calcification Heterogeneity through Their Elemental Distribution. Chemical & Biomedical Imaging, https://doi.org/10.1021/cbmi.5c00050

Calcifications across the body offer snapshots of the surrounding ionic environment at the time of their formation. Links between prostate calcification chemistry and cancer are becoming of increasing interest, particularly in identifying biomarkers... Read More about Revealing Prostate Calcification Heterogeneity through Their Elemental Distribution.

Eleven New Transiting Brown Dwarfs and Very-low-mass Stars from TESS (2025)
Journal Article
Vowell, N., Rodriguez, J. E., Latham, D. W., Quinn, S. N., Schulte, J., Eastman, J. D., Bieryla, A., Barkaoui, K., Ciardi, D. R., Collins, K. A., Girardin, E., Hébrard, G., Heldridge, E., Jafariyazani, M., Kotten, B., Mancini, L., Murgas, F., Narita, N., Radford, D. J., Relles, H. M., …Winn, J. N. (2025). Eleven New Transiting Brown Dwarfs and Very-low-mass Stars from TESS. Astronomical Journal, 170(2), Article 68. https://doi.org/10.3847/1538-3881/addd17

We present the discovery of 11 new transiting brown dwarfs (BDs) and low-mass M dwarfs from NASA’s Transiting Exoplanet Survey Satellite (TESS) mission: TOI-2844, TOI-3122, TOI-3577, TOI-3755, TOI-4462, TOI-4635, TOI-4737, TOI-4759, TOI-5240, TOI-546... Read More about Eleven New Transiting Brown Dwarfs and Very-low-mass Stars from TESS.

Equivalent Width of the Interstellar Na i D 1 and D 2 Absorption Lines for Stars with E ( B − V ) < 0.15 (2025)
Journal Article
Maxted, P. F. L. (2025). Equivalent Width of the Interstellar Na i D 1 and D 2 Absorption Lines for Stars with E ( B − V ) < 0.15. Research Notes of the American Astronomical Society, 9(6), 1-5. https://doi.org/10.3847/2515-5172/ade39b

New measurements of the equivalent width of the interstellar Na i D1 and D2 absorption lines for 62 bright B-type stars with E(B − V) < 0.15 are used to recalibrate the relation between these quantities in this low-reddening regime, and to quantify t... Read More about Equivalent Width of the Interstellar Na i D 1 and D 2 Absorption Lines for Stars with E ( B − V ) < 0.15.

Chemical synthesis of glycosaminoglycan mimetics for targeting endoglycosidase activity (2025)
Thesis
Wootton, H. S. (2025). Chemical synthesis of glycosaminoglycan mimetics for targeting endoglycosidase activity. (Thesis). Keele University. https://keele-repository.worktribe.com/output/1279726

Glycosaminoglycans are a family of extraordinary, long-chain polysaccharides that are highly abundant on the mammalian cell surface and in the extracellular matrix. These linear chains exist as proteoglycans which perform critical roles in many biolo... Read More about Chemical synthesis of glycosaminoglycan mimetics for targeting endoglycosidase activity.

Chemical Synthesis of S-linked Glycosaminoglycans (2025)
Thesis
O’Shea, C. (2025). Chemical Synthesis of S-linked Glycosaminoglycans. (Thesis). Keele University. https://keele-repository.worktribe.com/output/1280018

Heparan sulfate (HS), a sulfated linear carbohydrate that decorates the cell surface and extracellular matrix, is ubiquitously distributed throughout the animal kingdom and represents a key regulator of biological processes. An example of a glycosami... Read More about Chemical Synthesis of S-linked Glycosaminoglycans.

The Isaac Newton Telescope Monitoring Survey of Local Group Dwarf Galaxies. VII. Long-period Variable Stars in the Nearest Starburst Dwarf Galaxy, IC 10 (2025)
Journal Article
Gholami, M., Javadi, A., Mahani, H., van Loon, J. T., Khosroshahi, H., Saremi, E., McDonald, I., Eftekhari, S., Ren, Y., & Altafi, H. (2025). The Isaac Newton Telescope Monitoring Survey of Local Group Dwarf Galaxies. VII. Long-period Variable Stars in the Nearest Starburst Dwarf Galaxy, IC 10. Astronomical Journal, 170(1), Article 54. https://doi.org/10.3847/1538-3881/adda2b

To identify long-period variable (LPV) stars in IC 10—the nearest starburst galaxy of the Local Group—we conducted an optical monitoring survey using the 2.5 m Isaac Newton Telescope with the wide-field camera (WFC) in the i band and V band from 2015... Read More about The Isaac Newton Telescope Monitoring Survey of Local Group Dwarf Galaxies. VII. Long-period Variable Stars in the Nearest Starburst Dwarf Galaxy, IC 10.

Red Supergiant Mass Loss and Mass-Loss Rates (2025)
Journal Article
van Loon, J. T. (2025). Red Supergiant Mass Loss and Mass-Loss Rates. Galaxies, 13(4), Article 72. https://doi.org/10.3390/galaxies13040072

This review discusses the causes, nature, importance and observational evidence of mass loss by red supergiants. It arrives at the perception that mass loss finds its origin in the gravity which makes the star a star in the first place, and is a mech... Read More about Red Supergiant Mass Loss and Mass-Loss Rates.

The orbit of WASP-4 b is in decay (2025)
Journal Article
Baştürk, Ö., Kutluay, A. C., Barker, A., Yalçınkaya, S., Southworth, J., Barkaoui, K., Wünsche, A., Burgdorf, M. J., Timmermans, M., Jehin, E., Tregloan-Reed, J., Jaimes, R. F., Hinse, T. C., Duru, B., Hitchcock, J., Longa-Peña, P., Rahvar, S., Sajadian, S., Bretton, M., Selam, S. O., …Mancini, L. (2025). The orbit of WASP-4 b is in decay. Monthly Notices of the Royal Astronomical Society, 541(2), 714-730. https://doi.org/10.1093/mnras/staf1009

WASP-4 b is a hot Jupiter exhibiting a decreasing orbital period, prompting investigations into potential mechanisms driving its evolution. We analysed 173 transit light curves, including 37 new observations, and derived mid-transit timings with exof... Read More about The orbit of WASP-4 b is in decay.

Dusty Stellar Source Classification by Implementing Machine Learning Methods Based on Spectroscopic Observations in the Magellanic Clouds (2025)
Journal Article
Ghaziasgar, S., Abdollahi, M., Javadi, A., van Loon, J. T., McDonald, I., Oliveira, J., Masoudnezhad, A., Khosroshahi, H. G., Foing, B. H., & Fazel Hesar, F. (2025). Dusty Stellar Source Classification by Implementing Machine Learning Methods Based on Spectroscopic Observations in the Magellanic Clouds. The Astrophysical Journal, 986(2), 1-22. https://doi.org/10.3847/1538-4357/adceeb

Dusty stellar point sources are a significant stage in stellar evolution and contribute to the metal enrichment of galaxies. These objects can be classified using photometric and spectroscopic observations using color–magnitude diagrams and infrared... Read More about Dusty Stellar Source Classification by Implementing Machine Learning Methods Based on Spectroscopic Observations in the Magellanic Clouds.

MicroMaps: Ontology-driven Semantic Geospatial Data Fusion Approach for IoT Integration and Decision Making in Smart Cities (2025)
Presentation / Conference Contribution
Rayis, A., Ortolani, M., David, R.-M., Hirschi, R., & Misirli, G. (2025, August). MicroMaps: Ontology-driven Semantic Geospatial Data Fusion Approach for IoT Integration and Decision Making in Smart Cities. Presented at 2025 the 9th International Conference on Cloud, Big Data and Communication Systems (ICCBDCS 2025), Manchester

Smart cities generate large amounts of Internet of
Things data from diverse sources, often presented in varying
formats and with inconsistent quality, complicating effective data
management and interoperability. Despite recent advancements
relate... Read More about MicroMaps: Ontology-driven Semantic Geospatial Data Fusion Approach for IoT Integration and Decision Making in Smart Cities.

Symmetric double-layer capacitor with natural rubber and sodium salt-based solid polymer electrolyte and reduced graphene oxide electrodes (2025)
Presentation / Conference Contribution
Balakrishnan, N. (2025, June). Symmetric double-layer capacitor with natural rubber and sodium salt-based solid polymer electrolyte and reduced graphene oxide electrodes. Presented at International Conference on Sustainable Chemistry for Net Zero, University of St Andrews, Scotland, UK

Solid polymer electrolytes (SPEs) are the key to improving electrochemical devices' energy density and safety. In recent years, natural polymers have received tremendous attention due to the latest advances in green technology for a sustainable futur... Read More about Symmetric double-layer capacitor with natural rubber and sodium salt-based solid polymer electrolyte and reduced graphene oxide electrodes.

Vitacrystallography: Appearance and Development of Cancer-Induced Structural Biomarkers in a Mouse Model (2025)
Journal Article
Avdieiev, O., Denisov, S. A., Ajeer, A., Adams, L., Greenwood, C., Nesbitt, H., Thomas, K., Rogers, K., Solovyeva, O., Mourokh, L., & Lazarev, P. (2025). Vitacrystallography: Appearance and Development of Cancer-Induced Structural Biomarkers in a Mouse Model. Life, 15(6), Article 904. https://doi.org/10.3390/life15060904

Structural biomarkers determined by X-ray scattering of the tissues can complement conventional diagnostics and provide a pathway for early detection of diseases. In the present study, mouse models were utilized to observe the progression of prostate... Read More about Vitacrystallography: Appearance and Development of Cancer-Induced Structural Biomarkers in a Mouse Model.

Binarity at LOw Metallicity (BLOeM):. Enhanced multiplicity of early B-type dwarfs and giants at Z=0.2 Zsun (2025)
Journal Article
Villaseñor, J., Sana, H., Mahy, L., Shenar, T., Bodensteiner, J., Britavskiy, N., Lennon, D., Moe, M., Patrick, L., Pawlak, M., Bowman, D., Crowther, P., de Mink, S., Deshmukh, K., Evans, C., Fabry, M., Fouesneau, M., Holgado, G., Langer, N., Maíz Apellaniz, J., …Vink, J. (2025). Binarity at LOw Metallicity (BLOeM):. Enhanced multiplicity of early B-type dwarfs and giants at Z=0.2 Zsun. Astronomy & Astrophysics, 698, https://doi.org/10.1051/0004-6361/202453166

Early B-type stars with initial masses between 8 and 15M are frequently found in multiple systems, as is evidenced by multi-epoch spectroscopic campaigns in the Milky Way and the Large Magellanic Cloud (LMC). Previous studies have shown no strong met... Read More about Binarity at LOw Metallicity (BLOeM):. Enhanced multiplicity of early B-type dwarfs and giants at Z=0.2 Zsun.

Binarity at LOw Metallicity (BLOeM): The multiplicity properties and evolution of BAF-type supergiants (2025)
Journal Article
Patrick, L. R., Lennon, D. J., Najarro, F., Shenar, T., Bodensteiner, J., Sana, H., Crowther, P. A., Britavskiy, N., Langer, N., Schootemeijer, A., Evans, C. J., Mahy, L., Götberg, Y., de Mink, S. E., Schneider, F. R. N., O’Grady, A. J. G., Villaseñor, J. I., Bernini-Peron, M., Bowman, D. M., de Koter, A., …Wang, C. (2025). Binarity at LOw Metallicity (BLOeM): The multiplicity properties and evolution of BAF-type supergiants. Astronomy & Astrophysics, 698(June 2025), Article A39. https://doi.org/10.1051/0004-6361/202452949

Given the uncertain evolutionary status of blue supergiant stars, their multiplicity properties hold vital clues to better understand their origin and evolution. As part of The Binarity at LOw Metallicity (BLOeM) campaign in the Small Magellanic Clou... Read More about Binarity at LOw Metallicity (BLOeM): The multiplicity properties and evolution of BAF-type supergiants.

Binarity at LOw Metallicity (BLOeM): Multiplicity of early B-type supergiants in the Small Magellanic Cloud (2025)
Journal Article
Britavskiy, N., Mahy, L., Lennon, D., Patrick, L., Sana, H., Villaseñor, J., Shenar, T., Bodensteiner, J., Bernini-Peron, M., Berlanas, S., Bowman, D., Crowther, P., de Mink, S., Evans, C., Götberg, Y., Holgado, G., Johnston, C., Keszthelyi, Z., Klencki, J., Langer, N., …Vink, J. (2025). Binarity at LOw Metallicity (BLOeM): Multiplicity of early B-type supergiants in the Small Magellanic Cloud. Astronomy & Astrophysics, 698(May 2025), Article A40. https://doi.org/10.1051/0004-6361/202452963

Context. The blue supergiant (BSG) domain contains a large variety of stars whose past and future evolutionary paths are still highly uncertain. Since binary interaction plays a crucial role in the fate of massive stars, investigating the multiplicit... Read More about Binarity at LOw Metallicity (BLOeM): Multiplicity of early B-type supergiants in the Small Magellanic Cloud.

Binarity at LOw Metallicity (BLOeM): Multiplicity properties of Oe and Be stars (2025)
Journal Article
Bodensteiner, J., Shenar, T., Sana, H., Britavskiy, N., Crowther, P., Langer, N., Lennon, D., Mahy, L., Patrick, L., Villaseñor, J., Abdul-Masih, M., Bowman, D., de Koter, A., de Mink, S., Deshmukh, K., Fabry, M., Gilkis, A., Götberg, Y., Holgado, G., Izzard, R., …Xu, X.-T. (2025). Binarity at LOw Metallicity (BLOeM): Multiplicity properties of Oe and Be stars. Astronomy & Astrophysics, https://doi.org/10.1051/0004-6361/202452623

Context. Rapidly rotating classical OBe stars have been proposed as the products of binary interactions, and the fraction of Be stars with compact companions implies that at least some are. However, to constrain the interaction physics spinning up th... Read More about Binarity at LOw Metallicity (BLOeM): Multiplicity properties of Oe and Be stars.

EBLM XV – Revised dynamical masses for the circumbinary planet host Kepler-16 AB, using the SOPHIE spectrograph (2025)
Journal Article
Sebastian, D., Boisse, I., Santerne, A., Triaud, A. H. M. J., Baycroft, T. A., Davis, Y. T., Deleuil, M., Grouffal, S., Hébrard, G., Heidari, N., Martin, D. V., Maxted, P. F. L., Nelson, R. P., Lalitha, S., Scott, M. G., Scutt, O. J., & Standing, M. (in press). EBLM XV – Revised dynamical masses for the circumbinary planet host Kepler-16 AB, using the SOPHIE spectrograph. Monthly Notices of the Royal Astronomical Society, https://doi.org/10.1093/mnras/staf863

Eclipsing binaries are perfect laboratories to measure precise, accurate and model-independent stellar radii and stellar masses, so long as both components are spectroscopically resolved. Resolving both components is difficult in high-contrast binari... Read More about EBLM XV – Revised dynamical masses for the circumbinary planet host Kepler-16 AB, using the SOPHIE spectrograph.

A Swarm of WASP Planets: Nine Giant Planets Identified by the WASP Survey (2025)
Journal Article
Schanche, N., Hébrard, G., Stassun, K. G., Hord, B., Barkaoui, K., Bieryla, A., Ciardi, D., Collins, K. A., Collier Cameron, A., Hartman, J., Heidari, N., Hellier, C., Howell, S. B., Lendl, M., McCormac, J., McLeod, K. K., Parviainen, H., Radford, D., Rajpurohit, A. S., Relles, H., …Winn, J. (2025). A Swarm of WASP Planets: Nine Giant Planets Identified by the WASP Survey. Astronomical Journal, 169(6), Article 334. https://doi.org/10.3847/1538-3881/adccc6

The Wide Angle Search for Planets (WASP) survey provided some of the first transiting hot Jupiter candidates. With the addition of the Transiting Exoplanet Survey Satellite (TESS), many WASP planet candidates have now been revisited and given updated... Read More about A Swarm of WASP Planets: Nine Giant Planets Identified by the WASP Survey.

Systematic studies toward the synthesis of d -galactosamine-containing coumarin glycosides † (2025)
Journal Article
Wootton, H. S., & Miller, G. J. (2025). Systematic studies toward the synthesis of d -galactosamine-containing coumarin glycosides †. Organic and Biomolecular Chemistry, https://doi.org/10.1039/d5ob00746a

An O-glycosylation method for accessing coumarin glycosides is presented. We report the reaction of 6,8-difluoro-7-hydroxy-4-methylcoumarin and 4-methylumbelliferone with a variety of glycosyl imidate donors using BF3·Et2O as activator to access a se... Read More about Systematic studies toward the synthesis of d -galactosamine-containing coumarin glycosides †.

Near-infrared spectroscopy of the recurrent nova M31N 2008-12a (2025)
Journal Article
Banerjee, D. P. K., Geballe, T. R., Evans, A., Woodward, C. E., Page, K. L., & Starrfield, S. (2025). Near-infrared spectroscopy of the recurrent nova M31N 2008-12a. Monthly Notices of the Royal Astronomical Society, 540(2 - June 2025), 1780-1785. https://doi.org/10.1093/mnras/staf817

Near-infrared (NIR) 0.9–2.5 m spectra of the remarkable recurrent nova (RN) M31N 2008-12a were obtained on days 6.3 and 10.3 after discovery of its 2024 outburst, and are the first NIR spectra of this object. The only prominent line seen in the spect... Read More about Near-infrared spectroscopy of the recurrent nova M31N 2008-12a.