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25 Jul 2024: Toggle menu. Latest news.

25 Jul 2024: Toggle menu. Reseach group. Meet the members of the research group. Toggle menu. Cosmic Dawn Lab is a research group spread across the Institute of Astronomy, Kavli Institute for Cosmology and Cavendish Laboratory at the University of Cambridge

29 Jan 2024: Our twitter feed has uptodate news on campaigns. If you wish to contact me about a bullying issue in Cambridge University, please use this email.. ... I have developed new mechanisms for hypervelocity stars. In theoretical physics, I pioneered the study

25 Jul 2024: July 17, 2024. less than 1 minute read. During the past few months, we have had a number of PhD vivas in the group, namely those of Stefan, Thomas and Tibor. In order to celebrate these achievements, the group gathered for an evening at a board

25 Jul 2024: Five Astronomers At The Ioa. July 24, 2024. less than 1 minute read. Check out this video from the Institute of Astronomy, featuring group members Anastasia Fialkov and Tibor Dome, as well as other astronomers at the IoA! Updated:. July 24, 2024.

2 May 2024: Current Research Projects. Cosmology with Strongly Lensed Supernovae. In light of the Hubble tension, astronomy is looking to new probes, which are independent of the local distance ladder, with which to ... systems. The study of strongly lensed

25 Jul 2024: Toggle menu. Quick Links. Quick links to the group’s latest research publications. Toggle menu. Publications. 2024. On the constraints on superconducting cosmic strings from 21-cm cosmology. T. Gessey-Jones, S. Pochinda, H. T. J. Bevins, et al.,

17 Jul 2024: FitteR for Accretion ProPErties of T Tauri stars (FRAPPE): A new approach to use Class III spectra to derive stellar and accretion properties. ... An ALMA Survey of M-dwarfs in the Beta Pictoris Moving Group with Two New Debris Disc Detections.

25 Jul 2024: We implement increasingly more sophisticated and realistic processes, explore new statistical tools (using e.g.

28 Jun 2024: in order to determine whether the acceleration requires a new form Dark Energy or modifications to General Relativity on large (Giga light year) scales. ... Gravitationally lensed quasars in Gaia: III. 22 new lensed quasars from Gaia data release 2, Lemon

2 May 2024: The researchers give a presentation about their science and then help the students create art which visualizes the data from the presentation in a new way.

22 Mar 2024: Therefore, tackling a prime objective of exoplanet science and understanding how unique or common planets like our Earth are in our galactic neighborhood will require a new, dedicated approach. ... below). 15. 2.3 Timing for a space-based mid-infrared

9 Apr 2024: The new ALMA observa-tion is marked as a black circle, and the blue circle represents the fluxat the stellar position. ... Con-sequently, the broad structure of the Herschel observations seessmaller grains whose distribution is modified by radiation

22 Mar 2024: Science (New York, N.Y.) 233,869–72 (1986). [21] Maurette, M., Brack, A., Kurat, G., Perreau, M. &

22 Mar 2024: We describethe new mid-IR observations of Beta Pic in Section 2 and the datareduction procedures in Section 3. ... 5 DISCUSSION. In the following sections, we discuss new constraints that can beobtained in light of the newobservations under theories

22 Mar 2024: In order to do so, we de-velop a new extension of Frankenstein (Jennings et al. ... The new version of frank includes now an option to consider opticallythin or thick emission.

22 Mar 2024: any detections of circumstellar dust emission. These data provide new limits on dust belt fractional luminosities and. ... 2007a). Najita et al. (2022) used new coagulation models to assess the possibility that the observed population of cold debris.

22 Mar 2024: An ALMA Survey of M-dwarfs in the Beta Pictoris Moving Group withTwo New Debris Disc Detections. ... 2018),further solidifying the BPMG as a good candidate sample to searchfor new discs.

22 Mar 2024: Large surveys provided new insights about the frequency and properties of massive sub-stellar companions withseparations from 5 to 300 au.Aims. ... A new planetary characterisation algorithm, based on the RSM framework, is developed and testedsuccessfully

22 Mar 2024: In 2 we present and describe a new model thattakes into account photodissociation, vertical diffusion, ionisation,and viscous evolution of gas continuously released in a planetesi-mal belt.