Callum Donnan (@CdonnanAstro) header
Callum Donnan (@CdonnanAstro) profile picture

Postdoc at NOIRLab. Galaxy formation/evolution at high z.

Tucson, AZ
Joined February 2022
Photo by Callum Donnan (@CdonnanAstro)Photo by Callum Donnan (@CdonnanAstro)Photo by Callum Donnan (@CdonnanAstro)Photo by Callum Donnan (@CdonnanAstro)Photo by Callum Donnan (@CdonnanAstro)Photo by Callum Donnan (@CdonnanAstro)Photo by Callum Donnan (@CdonnanAstro)Photo by Callum Donnan (@CdonnanAstro)Photo by Callum Donnan (@CdonnanAstro)Photo by Callum Donnan (@CdonnanAstro)
The School awards annual prizes to postgraduate research students who have produced the best PhD thesis. Many congratulations to the latest winners: · Jordan Marsh · Matteo Sergola · Ryan Begley · Massi Hamadouche · Ivan Lobaskin 🙌 Full story: edin.ac/4ihORaa
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New paper today!🤠 For a sample of star-forming galaxies at z ≈ 4 from the EXCELS survey, we measure the electron temperatures, densities, and the Ar/O and Ne/O abundance ratios. Our main result is that Ar/O is lower at high-z compared to local sources! arxiv.org/abs/2411.11837
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Callum Donnan retweeted
My first lead-author paper is on arxiv today! 🤠 By measuring the O and Fe abundances of star-forming galaxies at z≈3.5, we constrain the stellar + gas-phase mass-metallicity relationships and find our galaxies have ubiquitously supersolar O/Fe ratios! arxiv.org/abs/2405.00774
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I'm happy to present our new paper on the UV luminosity function at z=9-15! We use a combination of the PRIMER, JADES and NGDEEP surveys covering 370 sq.arcmin. and reaching depths of 30 AB mag in the deepest region. 1/6 arxiv.org/abs/2403.03171
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Finally, we construct a simple model based on the halo mass function and find that our results do not need any alteration to LCDM, the dust content or the SF efficiency at high-z. Rather a trend towards younger stellar ages at increasing z is enough to match the observations. 5/6
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Many thanks to everyone who helped get this paper completed as well as to all of the work that went into designing and observing for the surveys! 6/6
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Callum Donnan retweeted
Excited to be presenting a poster at nam 2023, showing preliminary results from the joint analysis of rest-frame optical and UV spectra of star-forming galaxies at z~3.5, with the aim of investigating how oxygen/iron abundances scale with galaxy properties, and alpha enhancement.
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Callum Donnan retweeted
New paper Day! arxiv.org/abs/2306.03916 We've used VANDELS photometry+spectra to estimate fesc(Lya), confirming a (>10sig) EW(Lya)-fesc(Lya) correlation at z~4-5. From ISM line measurements in composite spectra, we then find fesc(LyC) ~ 0.15 fesc(Lya). Go read for all the details!
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Callum Donnan retweeted
For me, a huge takeaway from working with these public datasets is that we have an incredible chance to collaborate, rather than compete, with each other. This project was a lot more fun working together!
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I can barely think of words to tweet after what we have done these last 2.5 days... 🫠 But here you have the first results of the greatly awaited DDT observations 😃 (Spoiler: two new spectroscopically confirmed z > 10 galaxies! 😱) arxiv.org/abs/2303.15431
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Our paper on the DDT program led by @Richarwirman is on arxiv! We spectroscopically confirm 2 bright galaxies at z>10. This reinforces the large abundance of bright galaxies at z>10 while showing the importance of spectroscopic verification: arxiv.org/abs/2303.15431
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The true solution is a strong emission line galaxy which we and other groups suggested as a secondary solution from the photometry. H-alpha contaminates 3 filters at this precise redshift allowing it to imitate the blue photometry expected in these filters for a z=16 candidate.
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This is an exceptional example and not typical of high-z galaxies followed up with NIRSpec. We have shown the incredible power of JWST to find and then verify many bright galaxies at z>10. There is clearly a large number of luminous galaxies in the very young universe!
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It is very exciting that @Richarwirman’s @ceers_jwst DDT observations of #Maisiesgalaxy and @CdonnanAstro’s galaxy were obtained overnight. The @ceers_jwst and Edinburgh teams are hard at work on a joint paper, and we will be excited to share our results here when we submit!
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Guys, not long until we hear about that redshift 16.4 galaxy. Observations scheduled this Friday! Is it z~5 or z~16? Can't wait to find out!
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