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The spatial relation between young star clusters and molecular clouds in M51 with LEGUS (2018)
Journal Article
Grasha, K., Calzetti, D., Adamo, A., Kennicutt, R., Elmegreen, B., Messa, M., …Meidt, S. (2019). The spatial relation between young star clusters and molecular clouds in M51 with LEGUS. Monthly Notices of the Royal Astronomical Society, 483(4), 4707-4723. https://doi.org/10.1093/mnras/sty3424

We present a study correlating the spatial locations of young star clusters with those of molecular clouds in NGC 5194, in order to investigate the time-scale over which clusters separate from their birth clouds. The star cluster catalogues are from... Read More about The spatial relation between young star clusters and molecular clouds in M51 with LEGUS.

Overdensity of submillimeter galaxies around the z ≃ 2.3 MAMMOTH-1 nebula (2018)
Journal Article
Arrigoni Battaia, F., Chen, C., Fumagalli, M., Cai, Z., Calistro Rivera, G., Xu, J., …De Breuck, C. (2018). Overdensity of submillimeter galaxies around the z ≃ 2.3 MAMMOTH-1 nebula. Astronomy & Astrophysics, 620, Article A202. https://doi.org/10.1051/0004-6361/201834195

In the hierarchical model of structure formation, giant elliptical galaxies form through merging processes within the highest density peaks known as protoclusters. While high-redshift radio galaxies usually pinpoint the location of these environments... Read More about Overdensity of submillimeter galaxies around the z ≃ 2.3 MAMMOTH-1 nebula.

A Virgo Environmental Survey Tracing Ionised Gas Emission (VESTIGE): IV. a tail of ionised gas in the merger remnant NGC4424 (2018)
Journal Article
Boselli, A., Fossati, M., Consolandi, G., Amram, P., Ge, C., Sun, M., …Vollmer, B. (2018). A Virgo Environmental Survey Tracing Ionised Gas Emission (VESTIGE): IV. a tail of ionised gas in the merger remnant NGC4424. Astronomy & Astrophysics, 620, Article A164. https://doi.org/10.1051/0004-6361/201833914

We observed the late-type peculiar galaxy NGC 4424 during the Virgo Environmental Survey Tracing Galaxy Evolution (VESTIGE), a blind narrow-band Hα+[NII] imaging survey of the Virgo cluster carried out with MegaCam at the Canada-French-Hawaii Telesco... Read More about A Virgo Environmental Survey Tracing Ionised Gas Emission (VESTIGE): IV. a tail of ionised gas in the merger remnant NGC4424.

The core of the massive cluster merger MACS J0417.5-1154 as seen by VLT/MUSE (2018)
Journal Article
Jauzac, M., Mahler, G., Edge, A. C., Sharon, K., Gillman, S., Ebeling, H., …Salomé, P. (2018). The core of the massive cluster merger MACS J0417.5-1154 as seen by VLT/MUSE. Monthly Notices of the Royal Astronomical Society, 483(3), 3082-3097. https://doi.org/10.1093/mnras/sty3312

We present a multiwavelength analysis of the core of the massive galaxy cluster MACS J0417.5−1154 (⁠z = 0.441). Our analysis takes advantage of Very Large Telescope/Multi-Unit Spectroscopic Explorer observations which allow the spectroscopic confirma... Read More about The core of the massive cluster merger MACS J0417.5-1154 as seen by VLT/MUSE.

Exploring the origins of a new, apparently metal-free gas cloud at z = 4.4 (2018)
Journal Article
Robert, P. F., Murphy, M. T., O’Meara, J. M., Crighton, N. H., & Fumagalli, M. (2019). Exploring the origins of a new, apparently metal-free gas cloud at z = 4.4. Monthly Notices of the Royal Astronomical Society, 483(2), 2736-2747. https://doi.org/10.1093/mnras/sty3287

We report the discovery and analysis of only the third Lyman-limit system in which a high-quality resolution, echelle spectrum reveals no metal absorption lines, implying a metallicity ≲1/10 000 solar. Our HIRES spectrum of the background quasar, PSS... Read More about Exploring the origins of a new, apparently metal-free gas cloud at z = 4.4.

Dissecting cold gas in a high-redshift galaxy using a lensed background quasar (2018)
Journal Article
Krogager, J., Noterdaeme, P., O’Meara, J., Fumagalli, M., Fynbo, J., Prochaska, J., …Boissé, P. (2018). Dissecting cold gas in a high-redshift galaxy using a lensed background quasar. Astronomy & Astrophysics, 619, Article A142. https://doi.org/10.1051/0004-6361/201833608

We present a study of cold gas absorption from a damped Lyman-α absorber (DLA) at redshift zabs = 1.946 toward two lensed images of the quasar J144254.78+405535.5 at redshift zQSO = 2.590. The physical separation of the two lines of sight at the abso... Read More about Dissecting cold gas in a high-redshift galaxy using a lensed background quasar.

MCMC determination of the cosmic UV background at z ≃ 0 from Hα fluorescence (2018)
Journal Article
Caruso, D., Haardt, F., Fumagalli, M., & Cantalupo, S. (2019). MCMC determination of the cosmic UV background at z ≃ 0 from Hα fluorescence. Monthly Notices of the Royal Astronomical Society, 482(2), 2833-2837. https://doi.org/10.1093/mnras/sty2956

In a recent paper we reported on the detection of a diffuse H α glow in the outskirts of the nearby, edge-on disc galaxy UGC 7321 observed with the Multi-Unit Spectroscopic Explorer (MUSE) at the ESO Very Large Telescope. By interpreting the H α emis... Read More about MCMC determination of the cosmic UV background at z ≃ 0 from Hα fluorescence.

SLUG IV: A Novel Forward-Modelling Method to Derive the Demographics of Star Clusters (2018)
Journal Article
Krumholz, M., Adamo, A., Fumagalli, M., & Calzetti, D. (2019). SLUG IV: A Novel Forward-Modelling Method to Derive the Demographics of Star Clusters. Monthly Notices of the Royal Astronomical Society, 482(3), 3550-3566. https://doi.org/10.1093/mnras/sty2896

We describe a novel method for determining the demographics of a population of star clusters, for example distributions of cluster mass and age, from unresolved photometry. This method has a number of desirable properties: it fully exploits all the i... Read More about SLUG IV: A Novel Forward-Modelling Method to Derive the Demographics of Star Clusters.

Measurement of the primordial helium abundance from the intergalactic medium (2018)
Journal Article
Cooke, R., & Fumagalli, M. (2018). Measurement of the primordial helium abundance from the intergalactic medium. Nature Astronomy, 2(12), 957-961. https://doi.org/10.1038/s41550-018-0584-z

Almost every helium atom in the Universe was created just a few minutes after the Big Bang through a process commonly referred to as Big Bang nucleosynthesis1,2. The amount of helium that was made during Big Bang nucleosynthesis is determined by comb... Read More about Measurement of the primordial helium abundance from the intergalactic medium.

Connecting young star clusters to CO molecular gas in NGC 7793 with ALMA–LEGUS (2018)
Journal Article
Grasha, K., Calzetti, D., Bittle, L., Johnson, K., Meyer, J., Kennicutt, R., …Smith, L. (2018). Connecting young star clusters to CO molecular gas in NGC 7793 with ALMA–LEGUS. Monthly Notices of the Royal Astronomical Society, 481(1), 1016-1027. https://doi.org/10.1093/mnras/sty2154

We present an investigation of the relationship between giant molecular cloud (GMC) properties and the associated stellar clusters in the nearby flocculent galaxy NGC 7793. We combine the star cluster catalogue from the HST LEGUS (Legacy ExtraGalacti... Read More about Connecting young star clusters to CO molecular gas in NGC 7793 with ALMA–LEGUS.