Article
Astronomy & Astrophysics
A. Morales-Vargas, J. P. Torres-Papaqui, F. F. Rosales-Ortega, M. Chow-Martinez, J. J. Trejo-Alonso, R. A. Ortega-Minakata, A. C. Robleto-Orus, F. J. Romero-Cruz, D. M. Neri-Larios
Summary: The study reveals that tidal interactions influence star formation in galaxies, with higher star-formation rates and lower oxygen abundances in tidally perturbed regions. Statistical analysis confirms these observations, suggesting a link between tidal interactions and galaxy evolution.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2021)
Article
Astronomy & Astrophysics
P. Bonfini, A. Zezas, M. L. N. Ashby, S. P. Willner, A. Maragkoudakis, K. Kouroumpatzakis, P. H. Sell, K. Kovlakas
Summary: The study uses the Star Formation Reference Survey to constrain the mass distribution in nearby star-forming galaxies and measure the integrated luminosity density and total stellar mass density. The results indicate that discs dominate the mass density budget and recent star formation primarily happened in massive systems within the discs.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2021)
Article
Astronomy & Astrophysics
Mallory D. Thorp, Sara L. Ellison, Hsi-An Pan, Lihwai Lin, David R. Patton, Asa F. L. Bluck, Dan Walters, Jillian M. Scudder
Summary: This work presents spatially resolved measurements of CO emission collected with ALMA for mergers selected from the MaNGA and AlMaQUEST surveys. The study finds that merger-induced star formation can be driven by a variety of mechanisms, both within a galaxy and between different mergers, regardless of interaction stage.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2022)
Article
Astronomy & Astrophysics
Kearn Grisdale
Summary: The choice of star formation criteria impacts both galactic and giant molecular cloud scales in a Milky Way-like galaxy simulation. Using a turbulent, self-gravitating star formation criteria leads to increased gas density and larger cloud sizes, affecting the location and distribution of star formation. Despite the differences, relationships between cloud properties remain unaffected.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2021)
Article
Astronomy & Astrophysics
R. A. P. Oliveira, F. F. S. Maia, B. Barbuy, B. Dias, J. F. C. Santos Jr, S. O. Souza, L. O. Kerber, E. Bica, D. Sanmartim, B. Quint, L. Fraga, T. Armond, D. Minniti, M. C. Parisi, O. J. Katime Santrich, M. S. Angelo, A. Perez-Villegas, B. J. De Bortoli
Summary: This study analyzes 33 star clusters in the Magellanic Bridge and finds two main groups: older clusters with lower metallicities, possibly formed before the Magellanic Clouds encounter, and younger clusters with higher metallicities, likely formed in situ during the formation of the Bridge. The study also discovers two metallicity dips in the age-metallicity relation of the Bridge, indicating possible chemical signatures of its formation.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2023)
Article
Astronomy & Astrophysics
Michael W. Topping, Daniel P. Stark, Ryan Endsley, Rychard J. Bouwens, Sander Schouws, Renske Smit, Mauro Stefanon, Hanae Inami, Rebecca A. A. Bowler, Pascal Oesch, Valentino Gonzalez, Pratika Dayal, Elisabete da Cunha, Hiddo Algera, Paul van Der Werf, Andrea Pallottini, Laia Barrufet, Raffaella Schneider, Ilse De Looze, Laura Sommovigo, Lily Whitler, Luca Graziani, Yoshinobu Fudamoto, Andrea Ferrara
Summary: This study presents specific star formation rates (sSFRs) for 40 UV-bright galaxies at high redshifts, using improved SFR calibrations and SED-based stellar masses. The results show that the sSFRs derived from far-infrared continuum emission are higher than those derived from UV+optical SEDs. The study also suggests the possibility of spatial variations in dust across these galaxies and finds that sSFRs increase rapidly with redshifts, consistent with expectations from baryon accretion rates.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2022)
Article
Astronomy & Astrophysics
R. M. Gonzalez Delgado, J. E. Rodriguez-Martin, L. A. Diaz-Garcia, A. de Amorim, R. Garcia-Benito, G. Martinez-Solaeche, P. A. A. Lopes, M. Maturi, E. Perez, R. Cid Fernandes, A. Cortesi, A. Finoguenov, E. R. Carrasco, A. Hernan-Caballero, L. R. Abramo, J. Alcaniz, N. Benitez, S. Bonoli, A. J. Cenarro, D. Cristobal-Hornillos, J. M. Diego, R. A. Dupke, A. Ederoclite, J. A. Fernandez-Ontiveros, C. Lopez-Sanjuan, A. Marin-Franch, I Marquez, C. Mendes de Oliveira, M. Moles, I Pintos, L. Sodre, K. Taylor, J. Varela, H. Vazquez Ramio, J. M. Vilchez
Summary: This study demonstrates the potential of J-PAS in detecting and characterizing galaxy populations within galaxy clusters, showing that the proportion of red and quiescent galaxies in clusters increases with stellar mass, while the abundance excess of transition galaxies is modest at lower stellar masses.
ASTRONOMY & ASTROPHYSICS
(2022)
Article
Astronomy & Astrophysics
Marvin Blank, Andrea Maccio, Xi Kang, Keri L. Dixon, Nadine H. Soliman
Summary: This study investigates the transition of high-mass galaxies from being blue and star-forming to being red and dead, and finds that the crossing time through the green valley is mainly determined by the ageing of the current stellar population and the residual star formation in the green valley.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2022)
Article
Astronomy & Astrophysics
A. Capetti, B. Balmaverde, C. Tadhunter, A. Marconi, G. Venturi, M. Chiaberge, R. D. Baldi, S. Baum, R. Gilli, P. Grandi, E. T. Meyer, G. Miley, C. O'Dea, W. Sparks, E. Torresi, G. Tremblay
Summary: Observations using the VLT/MUSE optical integral field spectrograph were conducted on the radio source 3C 277.3, which is associated with the galaxy Coma A and has a redshift of 0.085. A emission line region was found to completely surround the double-lobed radio source, with a size of approximately 60 kpc x 90 kpc. Based on emission line ratios, five compact knots were identified where the gas ionization is powered by young stars located as far as about 60 kpc from the host. The emission line filaments surrounding the radio emission are likely ionized by fast shocks, but star formation at the edges of the radio source may also contribute.
ASTRONOMY & ASTROPHYSICS
(2022)
Article
Astronomy & Astrophysics
R. K. Cochrane, R. Kondapally, P. N. Best, J. Sabater, K. J. Duncan, D. J. B. Smith, M. J. Hardcastle, H. J. A. Rottgering, I Prandoni, P. Haskell, G. Guerkan, G. K. Miley
Summary: We conducted a detailed study of the cosmic star formation history using deep, radio continuum observations and high-quality ancillary data. By constructing radio luminosity functions and deriving the cosmic star formation rate density, we found that our measurements are generally in good agreement with previous studies and provide new insights into the star formation rates at different redshifts.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2023)
Article
Astronomy & Astrophysics
J. K. Barrera-Ballesteros, S. F. Sanchez, T. Heckman, T. Wong, A. Bolatto, E. Ostriker, E. Rosolowsky, L. Carigi, S. Vogel, R. C. Levy, D. Colombo, Yufeng Luo, Yixian Cao
Summary: The study reveals a tight correlation between star formation rate density Σ(SFR) and hydrostatic mid-plane pressure P-h, with an increase in effective feedback momentum per unit stellar mass (p(*) / m(*)) in actively star-forming regions as P-h increases. There is a significant negative correlation with total stellar mass, stellar age, and metallicity.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2021)
Article
Astronomy & Astrophysics
Rose A. Finn, Benedetta Vulcani, Gregory Rudnick, Michael L. Balogh, Vandana Desai, Pascale Jablonka, Dennis Zaritsky
Summary: We investigate the role of dense environments in suppressing star formation by studying galaxies with log(10)(M- * / M-?) > 9.7 in nine clusters from the Local Cluster Survey. We find that SFR suppression increases with increasing bulge-to-total ratio in all environments. In addition, cluster and infall galaxies have more suppressed SFRs compared to field counterparts at all values of B/T, suggesting an additional mechanism in dense environments.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2023)
Article
Astronomy & Astrophysics
Stephen M. Wilkins, Aswin P. Vijayan, Christopher C. Lovell, William J. Roper, Erik Zackrisson, Dimitrios Irodotou, Louise T. C. Seeyave, Jussi K. Kuusisto, Peter A. Thomas, Joseph Caruana, Christopher J. Conselice
Summary: The star formation and metal enrichment histories of galaxies are important properties, and their observation is a core goal in extragalactic astronomy. The lack of proper observations at high redshift has made it difficult to obtain robust constraints, but the upcoming JWST mission is expected to change this. In this study using the FLARES suite, we simulate the star formation and metal enrichment histories of galaxies at z = 5-13, and find a flat relationship between age/specfic star formation rate and stellar mass. We also predict a strong stellar mass-metallicity relation and α-enhancement at z = 10 and beyond.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2023)
Article
Astronomy & Astrophysics
Stephen M. Wilkins, Aswin P. Vijayan, Christopher C. Lovell, William J. Roper, Erik Zackrisson, Dimitrios Irodotou, Louise T. C. Seeyave, Jussi K. Kuusisto, Peter A. Thomas, Joseph Caruana, Christopher J. Conselice
Summary: The star formation and metal enrichment histories of galaxies are crucial properties that are measured in observational extragalactic astronomy. With the advent of JWST, robust constraints on these properties are now possible. Using the flares suite, we explore the star formation and metal enrichment histories of galaxies at high redshifts. Our core results show a flat relationship between age and specific star formation rate with stellar mass, indicating that these properties do not strongly depend on mass. We also predict a strong stellar mass-metallicity relation and alpha-enhancement at high redshifts. Additionally, we find no large-scale environmental dependence of age, specific star formation rate, or metallicity with stellar mass.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2022)
Article
Astronomy & Astrophysics
Mahdieh Navabi, Elham Saremi, Atefeh Javadi, Majedeh Noori, Jacco Th. van Loon, Habib G. Khosroshahi, Iain McDonald, Mina Alizadeh, Arash Danesh, Ghassem Gozaliasl, Alireza Molaeinezhad, Tahere Parto, Mojtaba Raouf
Summary: The study examines the star formation history of Andromeda VII, showing that the main epoch of star formation occurred around 6.2 billion years ago, followed by slow star formation until 500 million years ago. The research results indicate that the star formation rate of And VII varies with cosmic time.
ASTROPHYSICAL JOURNAL
(2021)
Article
Astronomy & Astrophysics
Mirko Curti, Francesco D'Eugenio, Stefano Carniani, Roberto Maiolino, Lester Sandles, Joris Witstok, William M. Baker, Jake S. Bennett, Joanna M. Piotrowska, Sandro Tacchella, Stephane Charlot, Kimihiko Nakajima, Gabriel Maheson, Filippo Mannucci, Amirnezam Amiri, Santiago Arribas, Francesco Belfiore, Nina R. Bonaventura, Andrew J. Bunker, Jacopo Chevallard, Giovanni Cresci, Emma Curtis-Lake, Connor Hayden-Pawson, Gareth C. Jones, Nimisha Kumari, Isaac Laseter, Tobias J. Looser, Alessandro Marconi, Michael Maseda, Jan Scholtz, Renske Smit, Hannah Ubler, Imaan E. B. Wallace
Summary: We analyze the chemical properties of three z similar to 8 galaxies behind the galaxy cluster SMACSJ0723.3-7327 and measure their metallicities using the direct T-e method for the first time at such high redshift. The galaxies show different excitation properties compared to local strong-line metallicity calibrations, suggesting a need for reassessment of the calibrations at these redshifts. The two galaxies at z similar to 7.6 have metallicities consistent with the extrapolation of the mass-metallicity relation, while the least massive galaxy at z similar to 8.5 shows a significantly lower metallicity, indicating a deviation from the equilibrium between gas flows, star formation, and metal enrichment.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2023)
Article
Astronomy & Astrophysics
B. Groves, K. Kreckel, F. Santoro, F. Belfiore, E. Zavodnik, E. Congiu, O. Egorov, E. Emsellem, K. Grasha, A. Leroy, F. Scheuermann, E. Schinnerer, E. J. Watkins, A. T. Barnes, F. Bigiel, D. A. Dale, S. C. O. Glover, I Pessa, P. Sanchez-Blazquez, T. G. Williams
Summary: Ionized nebulae provide critical insights into the conditions of the interstellar medium (ISM). The PHANGS-MUSE survey has produced optical spectroscopic coverage of the central star-forming discs of nearby galaxies, identifying thousands of nebulae per galaxy. Using diagnostic line ratios, the physical properties and environmental characteristics of each nebula are determined, providing a rich database for ISM studies.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2023)
Article
Astronomy & Astrophysics
William M. Baker, Roberto Maiolino, Francesco Belfiore, Mirko Curti, Asa F. L. Bluck, Lihwai Lin, Sara L. Ellison, Mallory Thorp, Hsi-An Pan
Summary: In this study, we investigated the scaling relations between gas-phase metallicity, stellar mass surface density, star formation rate surface density, and molecular gas surface density in local star-forming galaxies. We found that local metallicity is primarily determined by stellar mass surface density, with a secondary anticorrelation with star formation rate surface density. The impact of molecular gas surface density on local metallicity is less significant. Additionally, we observed that global galaxy properties, such as total stellar mass and total star formation rate, also influence local metallicity.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2023)
Article
Astronomy & Astrophysics
William M. Baker, Roberto Maiolino, Francesco Belfiore, Asa F. L. Bluck, Mirko Curti, Dominika Wylezalek, Caroline Bertemes, M. S. Bothwell, Lihwai Lin, Mallory Thorp, Hsi-An Pan
Summary: We investigate the relationships between SFR, M-*, and MH2 for local star-forming galaxies, high-z galaxies, and AGN host galaxies. The SK relation and MGMS are intrinsic primary relations for all three types of galaxies, while the SFMS is an indirect byproduct. The MGMS and SK relation evolve over cosmic time, with higher redshifts associated with greater MH2 and star formation efficiency. We provide parametrizations of the evolution of the MGMS and SK relation, showing how they contribute to the observed evolution of the SFMS. In addition, AGN host galaxies follow an AGN-MGMS relation, offsetting the MGMS to lower MH2 compared to local star-forming galaxies.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2023)
Article
Astronomy & Astrophysics
Enrico Congiu, Guillermo A. Blanc, Francesco Belfiore, Francesco Santoro, Fabian Scheuermann, Kathryn Kreckel, Eric Emsellem, Brent Groves, Hsi-An Pan, Frank Bigiel, Daniel A. Dale, Simon C. O. Glover, Kathryn Grasha, Oleg V. Egorov, Adam Leroy, Eva Schinnerer, Elizabeth J. Watkins, Thomas G. Williams
Summary: We present a new catalogue of ionised nebulae distributed across 19 galaxies observed by the PHANGS-MUSE survey. The nebulae were classified using a new model-comparison-based algorithm and the resulting catalogue is the largest containing complete spectral and spatial information for ionised nebulae. The algorithm performs well in selecting H II regions and identifies a significant population of shock-ionised regions, but has limitations in detecting planetary nebulae.
ASTRONOMY & ASTROPHYSICS
(2023)
Article
Astronomy & Astrophysics
Regina Sarmiento, Marc Huertas-Company, Johan H. Knapen, Hector Ibarra-Medel, Annalisa Pillepich, Sebastian F. Sanchez, Alina Boecker
Summary: Modern astronomical observations provide valuable information about nearby galaxies, but they can only capture the present-day state of the Universe. Cosmological simulations allow us to study the past processes that galaxies have undergone. This study aims to connect the past events with present-day galactic properties by using hydro-cosmological simulations to generate a mock MaNGA sample for stellar population analysis.
ASTRONOMY & ASTROPHYSICS
(2023)
Article
Astronomy & Astrophysics
Asa F. L. Bluck, Joanna M. Piotrowska, Roberto Maiolino
Summary: We used a machine-learning approach to investigate the intrinsic dependence of star formation quenching on galactic and environmental parameters. Our results showed that black hole mass is the most important parameter in predicting the quenching of central galaxies, while black hole accretion rate has little predictive power. This is important for observational studies, as it suggests that current AGN state cannot be used as a proxy for the impact of AGN feedback.
ASTROPHYSICAL JOURNAL
(2023)
Article
Astronomy & Astrophysics
Fabian Scheuermann, Kathryn Kreckel, Ashley T. Barnes, Francesco Belfiore, Brent Groves, Stephen Hannon, Janice C. Lee, Rebecca Minsley, Erik Rosolowsky, Frank Bigiel, Guillermo A. Blanc, Mederic Boquien, Daniel A. Dale, Sinan Deger, Oleg Egorov, Eric Emsellem, Simon C. O. Glover, Kathryn Grasha, Hamid Hassani, Sarah M. R. Jeffreson, Ralf S. Klessen, J. M. Diederik Kruijssen, Kirsten L. Larson, Adam K. Leroy, Laura A. Lopez, Hsi-An Pan, Patricia Sanchez-Blazquez, Francesco Santoro, Eva Schinnerer, David A. Thilker, Bradley C. Whitmore, Elizabeth J. Watkins, Thomas G. Williams
Summary: Connecting the gas in H II regions to the underlying ionizing radiation source helps us understand stellar feedback and the evolution of H II regions. Using PHANGS-MUSE, we detect and measure physical properties of nearly 24,000 H II regions across 19 galaxies. By analyzing associations with ionizing sources, we find correlations between association ages and various properties, suggesting an evolutionary sequence. We also observe correlations with local metallicity variations, indicating preferential star formation in metal-rich areas.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2023)
Article
Astronomy & Astrophysics
Lukas Neumann, Molly J. Gallagher, Frank Bigiel, Adam K. Leroy, Ashley T. Barnes, Antonio Usero, Jakob S. den Brok, Francesco Belfiore, Ivana Beslic, Yixian Cao, Melanie Chevance, Daniel A. Dale, Cosima Eibensteiner, Simon C. O. Glover, Kathryn Grasha, Jonathan D. Henshaw, Maria J. Jimenez-Donaire, Ralf S. Klessen, J. M. Diederik Kruijssen, Daizhong Liu, Sharon Meidt, Jerome Pety, Johannes Puschnig, Miguel Querejeta, Erik Rosolowsky, Eva Schinnerer, Andreas Schruba, Mattia C. Sormani, Jiayi Sun, Yu-Hsuan Teng, Thomas G. Williams
Summary: In this study, new HCN (1-0) data from the ALMOND survey and CO (2-1) data from the PHANGS-ALMA survey were used to examine the molecular gas density structure and star formation rate in nearby galaxies. The study found positive correlations (negative) between the HCN/CO (SFR/HCN) ratio and the surface density, velocity dispersion, and internal turbulent pressure of the molecular gas. Overall, these findings indicate a close relationship between molecular gas density, molecular cloud properties, and star formation.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2023)
Article
Astronomy & Astrophysics
Francesco Belfiore, Adam K. Leroy, Thomas G. Williams, Ashley T. Barnes, Frank Bigiel, Mederic Boquien, Yixian Cao, Jeremy Chastenet, Enrico Congiu, Daniel A. Dale, Oleg V. Egorov, Cosima Eibensteiner, Eric Emsellem, Simon C. O. Glover, Brent Groves, Hamid Hassani, Ralf S. Klessen, Kathryn Kreckel, Lukas Neumann, Justus Neumann, Miguel Querejeta, Erik Rosolowsky, Patricia Sanchez-Blazquez, Karin Sandstrom, Eva Schinnerer, Jiayi Sun, Jessica Sutter, Elizabeth J. Watkins
Summary: Measurements of star formation activity on cloud scales are crucial to understanding molecular cloud physics and stellar feedback in galaxies. In this study, we used infrared emission and PAH-tracing bands to investigate obscured star formation in nearby galaxies. Our results show that the 21 μm emission is the best tracer of dust attenuation, while the PAH-tracing bands underestimate the correction for bright H II regions and suffer from contamination from diffuse IR background in fainter H II regions.
ASTRONOMY & ASTROPHYSICS
(2023)
Article
Astronomy & Astrophysics
Yeny Garay-Solis, Jorge K. Barrera-Ballesteros, Dario Colombo, Sebastian F. Sanchez, Alejandra Z. Lugo-Aranda, Vicente Villanueva, Tony Wong, Alberto D. Bolatto
Summary: Galactic interactions and mergers play a crucial role in galaxy evolution. Analyzing the data from 236 star-forming CALIFA galaxies, we find that interactions and mergers lead to an increase in the fraction of molecular gas in the center of galaxies compared to isolated ones. Our results suggest that the change in star formation efficiency is the main driver for the enhancement or suppression of central star formation, except in merging galaxies where the increased star formation appears to be driven by an increase in molecular gas. We propose that gravitational torques from interactions and mergers transport cold molecular gas inwards, increasing the gas fraction without necessarily increasing star formation.
ASTROPHYSICAL JOURNAL
(2023)
Article
Astronomy & Astrophysics
Hung-Yu Jian, Lihwai Lin, Bau-Ching Hsieh, Keiichi Umetsu, Carlos Lopez-Coba, Masamune Oguri, Connor Bottrell, Yoshiki Toba, Yusei Koyama, Yu-Yen Chang, Tadayuki Kodama, Yutaka Komiyama, Surhud More, Kai-Yang Lin, Atsushi J. Nishizawa, Ichi Tanaka
Summary: This study examines the impact of cluster environments on galaxy properties and finds a slow quenching mechanism at work, with radial and density-related quenching processes equally crucial for low-mass cluster galaxies.
ASTROPHYSICAL JOURNAL
(2023)
Article
Astronomy & Astrophysics
Caleb Lammers, Kartheik G. Iyer, Hector Ibarra-Medel, Camilla Pacifici, Sebastian F. Sanchez, Sandro Tacchella, Joanna Woo
Summary: By comparing 279 low-redshift AGN galaxies with inactive control galaxies, researchers reconstructed nonparametric star formation histories and found that AGN feedback can suppress star formation in the central regions.
ASTROPHYSICAL JOURNAL
(2023)
Article
Astronomy & Astrophysics
Yixian Cao, Tony Wong, Alberto D. Bolatto, Adam K. Leroy, Erik Rosolowsky, Dyas Utomo, Sebastian F. Sanchez, Jorge K. Barrera-Ballesteros, Rebecca C. Levy, Dario Colombo, Leo Blitz, Stuart N. Vogel, Johannes Puschnig, Vicente Villanueva, Monica Rubio
Summary: This article presents (CO)-C-13 (J=1->0) observations for the EDGE-CALIFA survey, detecting (CO)-C-13 in 41 galaxies via integrated line flux and in 30 galaxies via integrated line intensity. The line ratio R-12/13 is systematically compared with the properties of stars and ionized gas, with higher R-12/13 values found in interacting galaxies. The global R-12/13 slightly increases with infrared color but appears insensitive to other host-galaxy properties. The radial profiles of R-12/13 are flat across the sample and show a weak correlation with gas and stellar properties. These findings suggest that R-12/13 is not a sensitive tracer for ISM properties in complex galaxy environments.
ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES
(2023)
Correction
Astronomy & Astrophysics
Ryan Chow, Laura Parker, Christine D. Wilson, Toby Brown, Fraser Evans, Yang Gao, Ho Seong Hwang, Lihwai Lin, Amelie Saintonge, Mark Sargent, Matthew Smith, Ting Xiao
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2023)
