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X-ORIGINAL-URL:https://www.atnf.csiro.au
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DTSTART:20230401T160000
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DTSTART:20230930T160000
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DTSTART:20240406T160000
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DTSTART:20241005T160000
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DTSTART:20250405T160000
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BEGIN:VEVENT
DTSTART;TZID=Australia/Sydney:20240612T150000
DTEND;TZID=Australia/Sydney:20240612T160000
DTSTAMP:20260525T024311
CREATED:20250819T053726Z
LAST-MODIFIED:20250819T053727Z
UID:14869-1718204400-1718208000@www.atnf.csiro.au
SUMMARY:S&A Colloquium: Susmita Sett (Curtin)
DESCRIPTION:Imaging pulsar census of the Galactic Plane using MWA VCS data\n\nAbstract\n\nPulsars play a crucial role in exploring a wide range of physics and astrophysics\, such as probing dense-matter physics and testing strong-field gravity. Traditional pulsar surveys have mostly used time-domain periodicity searches\, but these methods can be hindered by scattering\, eclipses\, and orbital motion\, especially at low radio frequencies (<300 MHz). In contrast\, image domain searches for pulsars are more effective against these effects\, enabling new discoveries in the parameter space unreachable by traditional methods. To exploit the capability of image-based pulsar searches\, a pipeline has been developed to form 1-second full Stokes images from high-time-resolution data (Voltage Capture System\, VCS) from the Murchison Widefield Array (MWA). This led to the exploration of image-based techniques for identifying new pulsar candidates. In this talk\, I will describe a low-frequency image-based pulsar census of the Galactic Plane (GP) with the MWA focused on detecting the known pulsars in the observed region of the sky using both image-based and beamformed methods. This effort led to our detection of known pulsars\, with some being detected for the first time at low-frequency (150 MHz). The continuum flux densities of the pulsars detected in our image-based GP survey are significantly more reliable than the timing flux densities and therefore offer an additional benefit as flux densities are not readily available or are unreliable for many known pulsars at low frequencies. Therefore\, imaging is an effective approach for discovering new pulsars in less-explored regions of the DM space and improving the spectral modelling of the known detected pulsars. Upcoming facilities like SKA-Low will enhance the success of such image-based pulsar searches and aid in identifying new pulsar candidates. \nWatch recording\nEvent details\nDownload iCal\nCategory\nColearnia
URL:https://www.atnf.csiro.au/event/sa-colloquium-susmita-sett-curtin/
CATEGORIES:Colloquia
ATTACH;FMTTYPE=image/jpeg:https://www.atnf.csiro.au/wp-content/uploads/2024/12/Colloq-12062024.jpg
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Australia/Sydney:20240626T150000
DTEND;TZID=Australia/Sydney:20240626T160000
DTSTAMP:20260525T024311
CREATED:20250819T053632Z
LAST-MODIFIED:20250819T053633Z
UID:14870-1719414000-1719417600@www.atnf.csiro.au
SUMMARY:S&A Colloquium: Benjamin Roberts (University of Queensland)
DESCRIPTION:A brief history of time(keeping): atomic clocks at the precision frontier of fundamental physics\n\nAbstract\n\nAtomic clocks are the most precise instrucments ever constructed. The best atomic clocks today have a precision that corresponds to losing no more than a second over the lifetime of the universe. In this talk\, I’ll discuss the role of atomic clocks at the forefront of fundamental physics\, with a particular focus on dark matter\, and how precision atomic physics allows us to extend the search for dark matter (and other exotic physics) to lower and lower masses. (Image credit: N. Hanacek\, NIST) \nWatch recording\nEvent details\nDownload iCal\nCategory\nColearnia
URL:https://www.atnf.csiro.au/event/sa-colloquium-benjamin-roberts-university-of-queensland/
CATEGORIES:Colloquia
ATTACH;FMTTYPE=image/jpeg:https://www.atnf.csiro.au/wp-content/uploads/2024/12/Colloq-26062024-scaled.jpg
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Australia/Sydney:20240703T150000
DTEND;TZID=Australia/Sydney:20240703T160000
DTSTAMP:20260525T024311
CREATED:20250819T053558Z
LAST-MODIFIED:20250819T053558Z
UID:14871-1720018800-1720022400@www.atnf.csiro.au
SUMMARY:S&A Colloquium: Monserrat Martinez (Swinburne)
DESCRIPTION:The role of AGN in regulating galaxy evolution in massive z~3-4 galaxies\n\nAbstract\n\nAn excess of massive quiescent galaxies (MQGs) is found at the early universe (z~3-4). MQGs at this epoch suggest their stellar content was already in place in the first 1.5 Gyr of the Universe. These findings indicate that MQGs must have experienced an event that caused rapid quenching. Although observational evidence is scarce\, AGNs are the most suitable candidate for quenching these galaxies. In this talk\, we present a sample of massive galaxies (10 < log(𝑀★/𝑀⊙ ) < 11) at 3 < z < 4 from JWST NIRSpec and the ZFOURGE survey with K–band spectra of the Keck/MOSFIRE\, VLT/KMOS. We find that a large fraction have strong [OIII]5007 and H𝛽 emission lines with large line widths (𝜎 100 – 450 km/s). These results show a significantly high AGN fraction in massive galaxies\, ranging from 60–70%\, pointing to the period between 3 < z < 4 being a time of heightened activity for the development of supermassive black holes in the massive end of the galaxy population and provide evidence for their role in the emergence of the first massive quenched galaxies at this epoch. \nWatch recording\nEvent details\nDownload iCal\nCategory\nColearnia
URL:https://www.atnf.csiro.au/event/sa-colloquium-monserrat-martinez-swinburne/
CATEGORIES:Colloquia
ATTACH;FMTTYPE=image/jpeg:https://www.atnf.csiro.au/wp-content/uploads/2024/12/Colloq-03072024.jpg
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Australia/Sydney:20240710T150000
DTEND;TZID=Australia/Sydney:20240710T160000
DTSTAMP:20260525T024311
CREATED:20250819T053450Z
LAST-MODIFIED:20250819T053450Z
UID:14872-1720623600-1720627200@www.atnf.csiro.au
SUMMARY:S&A Colloquium: Patricia Forster
DESCRIPTION:Western Australia Aboriginal Astronomy\n\nAbstract\n\nTraditionally\, Aboriginal people used objects in the sky to establish direction\, guide navigation\, predict seasons and as calendars for planning social life. Their narratives linked objects in the sky to life and landforms on earth and frequently included a moral element. This talk will draw on less publicized aspects of WA Aboriginal Astronomy from my review of the topic published by Cambridge University Press for the Astronomical Society of Australia. \nWatch recording\nEvent details\nDownload iCal\nCategory\nColearnia
URL:https://www.atnf.csiro.au/event/sa-colloquium-patricia-forster/
CATEGORIES:Colloquia
ATTACH;FMTTYPE=image/jpeg:https://www.atnf.csiro.au/wp-content/uploads/2024/12/Colloq-10072024.jpg
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Australia/Sydney:20240717T150000
DTEND;TZID=Australia/Sydney:20240717T160000
DTSTAMP:20260525T024311
CREATED:20250819T053315Z
LAST-MODIFIED:20250819T053315Z
UID:14873-1721228400-1721232000@www.atnf.csiro.au
SUMMARY:S&A Colloquium: Apurba Bera (ICRAR/Curtin)
DESCRIPTION:The curious case of twin fast radio bursts detected in the ASKAP-CRAFT survey\n\nAbstract\n\nFast radio bursts (FRBs) are brilliant short-duration flashes of radio emission originating at cosmological distances. Vast diversity in the properties of currently known FRBs\, complex spectro-temporal structures and the fleeting nature of these events make it difficult to understand their progenitors and emission mechanism. The Commensal Real-time ASKAP Fast Transients (CRAFT) survey\, with the Australian Square Kilometre Array Pathfinder (ASKAP) radio telescope\, enables high time resolution spectro-polarimetric study of FRBs that helps us probe the physics of the emission source and its surrounding medium. In the currently available CRAFT FRB sample we identified two apparently unrelated FRBs that show remarkable resemblance in pulse shape\, rest-frame emission time-scales and polarization properties — which indicates that these two events are likely to have very similar progenitors. In this talk I will describe the observed properties of these two FRBs and discuss their possible interpretations. \nWatch recording\nEvent details\nDownload iCal\nCategory\nColearnia
URL:https://www.atnf.csiro.au/event/sa-colloquium-apurba-bera-icrar-curtin/
CATEGORIES:Colloquia
ATTACH;FMTTYPE=image/jpeg:https://www.atnf.csiro.au/wp-content/uploads/2024/12/Colloq-17072024.jpg
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Australia/Sydney:20240731T150000
DTEND;TZID=Australia/Sydney:20240731T160000
DTSTAMP:20260525T024311
CREATED:20250819T053237Z
LAST-MODIFIED:20250819T053238Z
UID:14874-1722438000-1722441600@www.atnf.csiro.au
SUMMARY:S&A Colloquium: Hao Ding (NAOJ)
DESCRIPTION:Enhancing the studies of reference frame ties and millisecond pulsar formation channels with LBA astrometry of millisecond pulsars\n\nAbstract\n\nMillisecond pulsars (MSPs) are the fastest-spinning neutron stars. Thanks to their superbtime-keeping ability\, MSPs have provided sharp tests of gravitational theories\, and have been collectively used to constrain the stochastic gravitational-wave background (GWB). Precise astrometric studies of MSPs are desired in many ways. In this talk\, I will mainly focus on two scientific prospects promised by MSP astrometry. Firstly\, as I will explain in the talk\, the velocity distribution of MSPs is likely multi-modal. VLBI astrometry of MSPs holds the key to constraining the MSP velocity distribution\, which is directly linked to the formation channels of MSPs. Secondly\, VLBI and timing observations of MSPs can jointly refine the connection between the kinematic and dynamic reference frames\, which would betterquantify the systematics in pulsar timing array studies. As the major VLBI network in the southern hemisphere\, the Australian Long Baseline Array is crucial for significantly enriching the astrometrically studied MSP sample. I will introduce a new LBA program focusing on MSP astrometry\, and update its progress. Alongside the scientific discussions\, I will describe the main challenges the two studies are facing\, and outline some innovations in data reduction and analysis that may help us overcome the challenges. \nWatch recording\nEvent details\nDownload iCal\nCategory\nColearnia
URL:https://www.atnf.csiro.au/event/sa-colloquium-hao-ding-naoj/
CATEGORIES:Colloquia
ATTACH;FMTTYPE=image/jpeg:https://www.atnf.csiro.au/wp-content/uploads/2024/12/Colloq-31072024.jpg
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Australia/Sydney:20240802T150000
DTEND;TZID=Australia/Sydney:20240802T160000
DTSTAMP:20260525T024311
CREATED:20250819T053148Z
LAST-MODIFIED:20250819T053149Z
UID:14875-1722610800-1722614400@www.atnf.csiro.au
SUMMARY:S&A Colloquium: Tasso Tzioumis (CSIRO)
DESCRIPTION:34 years with CSIRO\n\nAbstract\n\nOn the occasion of his retirement from CSIRO\, Tasso Tzioumis will look back over his 34 year career in the Australia Telescope National Facility. \nWatch recording\nEvent details\nDownload iCal\nCategory\nColearnia
URL:https://www.atnf.csiro.au/event/sa-colloquium-tasso-tzioumis-csiro/
CATEGORIES:Colloquia
ATTACH;FMTTYPE=image/jpeg:https://www.atnf.csiro.au/wp-content/uploads/2024/12/Colloq-02082024-scaled.jpg
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Australia/Sydney:20240807T150000
DTEND;TZID=Australia/Sydney:20240807T160000
DTSTAMP:20260525T024311
CREATED:20250819T053112Z
LAST-MODIFIED:20250819T053112Z
UID:14876-1723042800-1723046400@www.atnf.csiro.au
SUMMARY:S&A Colloquium: Laura Driessen (University of Sydney)
DESCRIPTION:The Sydney Radio Star Catalogue: a new catalogue of radio stars\n\nAbstract\n\nI will present a new catalogue of 839 radio stars detected < 3 GHz: the Sydney Radio Star Catalogue (SRSC). Most of these stars were identified using ASKAP. The ASKAP stars in the SRSC were found using a range of techniques: circular polarisation searches\, proper-motion searches\, variability searches and multiwavelength cross-matching. We have also included published radio stars from e.g. MeerKAT and V-LoTSS in the SRSC. The catalogue contains stars from across the Hertzsprung-Russell diagram\, from ultra-cool dwarfs to blue supergiants to Wolf Rayets. The previous best-known radio star catalogue\, the Wendker catalogue\, contained 228 radio stars detected < 3GHz. Hence the SRSC is a big leap forward in our understanding of the population and characteristics of radio stars. I will present an overview of the SRSC catalogue\, including the search methods\, the properties and types of stars\, the X-ray-radio characteristics using eROSITA_DE observations\, and the circular polarisation properties. I will also highlight some individual objects of particular interest. I will also present a short summary of ASKAP VAST\, with some recent updates. \nWatch recording\nEvent details\nDownload iCal\nCategory\nColearnia
URL:https://www.atnf.csiro.au/event/sa-colloquium-laura-driessen-university-of-sydney/
CATEGORIES:Colloquia
ATTACH;FMTTYPE=image/jpeg:https://www.atnf.csiro.au/wp-content/uploads/2024/12/Colloq-07082024.jpg
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Australia/Sydney:20240814T150000
DTEND;TZID=Australia/Sydney:20240814T160000
DTSTAMP:20260525T024311
CREATED:20250819T053020Z
LAST-MODIFIED:20250819T053020Z
UID:14877-1723647600-1723651200@www.atnf.csiro.au
SUMMARY:S&A Colloquium: Orsola De Marco (AAL)
DESCRIPTION:AAL member update to CSIRO Space & Astronomy\n\nAbstract\n\nAAL is a not-for-profit organisation\, whose members are Australian universities and institutions with a significant astronomical research capability. CSIRO Space & Astronomy is one of our member institutions and we are so pleased to be delivering our member update to you all in person once more this year. During our presentation\, we will provide a quick introduction on who we are\, where our funding money comes from and where it goes. We will discuss some of our key projects\, the bid for full membership of ESO and AAL’s strategy moving forward over the next 12 to 24 months. \nWatch recording\nEvent details\nDownload iCal\nCategory\nColearnia
URL:https://www.atnf.csiro.au/event/sa-colloquium-orsola-de-marco-aal/
CATEGORIES:Colloquia
ATTACH;FMTTYPE=image/jpeg:https://www.atnf.csiro.au/wp-content/uploads/2024/12/Colloq-14082024.jpg
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Australia/Sydney:20240821T150000
DTEND;TZID=Australia/Sydney:20240821T160000
DTSTAMP:20260525T024311
CREATED:20250819T052823Z
LAST-MODIFIED:20250819T052823Z
UID:14878-1724252400-1724256000@www.atnf.csiro.au
SUMMARY:S&A Colloquium: Pascal Keller (Leiden Observatory)
DESCRIPTION:Investigating the Epoch of Reionisation with Radio Interferometers\n\nAbstract\n\nThe Epoch of Reionisation (EoR) marks the cosmic period during which the neutral hydrogen that pervaded the Universe transitioned to an almost entirely ionised state. The most promising probe of the EoR is the redshifted 21 cm line\, which has the potential to characterise the 3-dimensional distribution of neutral hydrogen. The statistical detection of its spatial fluctuations is a prime objective of modern low-frequency radio interferometers\, though instrumental systematics and calibration errors pose an immense challenge. In this talk\, I will discuss a calibration-independent method of detecting the cosmological signal fluctuations using the interferometric closure phase. I discuss recent developments in the interpretation of the closure phase delay power spectrum and present constraints on it obtained from a full season of HERA observations. \n\n Additionally\, I present the results of a VLA L-Band survey of 138 optically confirmed reionisation-era quasars. The survey aimed at finding quasars suitable for measuring the cosmological 21 cm signal in absorption to their bright radio emissions. The survey was further used to constrain the statistical properties of the high-redshift quasar population and their cosmic evolution. \n\n Together\, these efforts extend the required groundwork for detecting the cosmological 21 cm signal from the EoR. \nWatch recording\nEvent details\nDownload iCal\nCategory\nColearnia
URL:https://www.atnf.csiro.au/event/sa-colloquium-pascal-keller-leiden-observatory/
CATEGORIES:Colloquia
ATTACH;FMTTYPE=image/png:https://www.atnf.csiro.au/wp-content/uploads/2024/12/Colloq-21082024.png
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Australia/Sydney:20240828T150000
DTEND;TZID=Australia/Sydney:20240828T160000
DTSTAMP:20260525T024311
CREATED:20250819T052729Z
LAST-MODIFIED:20250819T052730Z
UID:14879-1724857200-1724860800@www.atnf.csiro.au
SUMMARY:S&A Colloquium: Oliver Oayda (University of Sydney)
DESCRIPTION:Probing the Cosmic Dipole in the Radio Sky using ASKAP for Cosmology\n\nAbstract\n\nThe dipole of the Cosmic Microwave Background (“CMB”) is conventionally understood to be due to our heliocentric motion through the Universe at a speed of about 370 km/s. It is therefore called the kinematic dipole. If this interpretation is correct\, this motion should impact other observables\, for example large-scale radio galaxy surveys surveyed up to some limiting flux density. Our motion is anticipated to induce a variation in galaxy source density described by a dipole — the “cosmic dipole”. Analysing the consistency between this dipole and the kinematic dipole functions as a test of the cosmological principle\, which is the assumption that our Universe is homogeneous and isotropic on large scales. We present a Bayesian analysis of two radio galaxy surveys — RACS-low and NVSS — and find that\, even after accounting for local sources\, the dipole points roughly in the same direction as the kinematic dipole but has an amplitude 2 to 3 times larger than anticipated. This accords with other studies in the literature and represents an ongoing challenge to the kinematic interpretation of the CMB\, and therefore the cosmological principle. \nWatch recording\nEvent details\nDownload iCal\nCategory\nColearnia
URL:https://www.atnf.csiro.au/event/sa-colloquium-oliver-oayda-university-of-sydney/
CATEGORIES:Colloquia
ATTACH;FMTTYPE=image/jpeg:https://www.atnf.csiro.au/wp-content/uploads/2024/12/Colloq-28082024-scaled.jpg
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Australia/Sydney:20240918T150000
DTEND;TZID=Australia/Sydney:20240918T160000
DTSTAMP:20260525T024311
CREATED:20250819T052601Z
LAST-MODIFIED:20250819T052602Z
UID:14880-1726671600-1726675200@www.atnf.csiro.au
SUMMARY:S&A Colloquium: Dongjin Kim (CSIRO)
DESCRIPTION:Radio Jet and Obscuring Torus of Active Galactic Nuclei Revealed by VLBI\n\nAbstract\n\nActive Galactic Nuclei (AGNs) are believed to play a significant role in the formation and evolution of galaxies through their energetic jet outflows. However\, observational constraints are still limited when it comes to understanding how radio jets are triggered and how jet feedback operates in different types of AGNs. To gain insights into these processes\, it is crucial to study both the continuum radio jet and the circumnuclear gas in AGNs. This presentation will review high-angular-resolution VLBI studies on AGN radio jets and their immediate surroundings. Specifically\, I will emphasize spectroscopic studies of AGNs using molecular absorption and highlight promising scientific opportunities that can be achieved with current and future mm/sub-mm VLBI arrays. These studies provide valuable insights into the nuclear environments of AGNs\, offering a better understanding of the triggering and feedback mechanisms driving radio jet outflows. \nWatch recording\nEvent details\nDownload iCal\nCategory\nColearnia
URL:https://www.atnf.csiro.au/event/sa-colloquium-dongjin-kim-csiro/
CATEGORIES:Colloquia
ATTACH;FMTTYPE=image/jpeg:https://www.atnf.csiro.au/wp-content/uploads/2024/12/Colloq-18092024.jpg
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Australia/Sydney:20240930T080000
DTEND;TZID=Australia/Sydney:20240930T170000
DTSTAMP:20260525T024311
CREATED:20240928T013534Z
LAST-MODIFIED:20240829T044043Z
UID:2018-1727683200-1727715600@www.atnf.csiro.au
SUMMARY:Meet monazite\, a pathfinder to rare earth elements
DESCRIPTION:Overview\n\nEvent summary text (summary text is slightly larger than regular text) … \n\nDescribe the details of your event here … \nLearn more\nLocation\n\nOrganiser\n\nEvent details\nDownload iCal\nCategory\nColearnia
URL:https://www.atnf.csiro.au/event/meet-monazite-a-pathfinder-to-rare-earth-elements/
LOCATION:Kensington Lecture Theatre\, WA\, Australia
CATEGORIES:Public lecture
ORGANIZER;CN="Steve Gartner":MAILTO:steve.gartner@csiro.au
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Australia/Sydney:20241002T140000
DTEND;TZID=Australia/Sydney:20241002T150000
DTSTAMP:20260525T024311
CREATED:20241029T034040Z
LAST-MODIFIED:20250821T003227Z
UID:2966-1727877600-1727881200@www.atnf.csiro.au
SUMMARY:Colloquium: Rhea–Silvia Remus and Lucas Kimmig (LMU Munich)
DESCRIPTION:From Cosmic Dawn to Present-Day: Galaxy Formation and Evolution from Simulations\n\nAbstract: \n\nObservations of galaxies have revealed a puzzle of different properties seen from redshifts of z=10 or higher to present-day\, using multi-wavebands and integral field spectroscopy to probe the stellar light\, the gas\, but also infer the dark matter content of galaxies at different epochs of time. However\, as observations represent snapshots in time\, connecting the puzzle pieces in their evolution requires simulations to bridge our understanding of galaxy formation at early and late times. We will present the results of this endeavour using one of the largest sets of fully hydrodynamical cosmological simulations\, the Magneticum Pathfinder simulation suite and its adjacent simulations\, going from the earliest formation of galaxies to their present-day counterparts. We will highlight how metals in the stars reveal a galaxy’s assembly history\, show that most present day main sequence galaxies have experienced episodes of quiescence and rejuvenation\, and demonstrate how kinematics and low surface brightness features are connected. We invite you to join us on this journey of galaxy formation through cosmic time\, and discover how simulations and observations together shed light on how structures have formed in our Universe. \nTeams meeting\nPhysical location\n\nOnline location\n\nOrganiser\n\nEvent details\nDownload iCal\nCategory\nColearnia
URL:https://www.atnf.csiro.au/event/colloquium-rhea-silvia-remus-and-lucas-kimmig-lmu-munich/
LOCATION:Kensington Lecture Theatre\, WA\, Australia
CATEGORIES:Colloquia
ATTACH;FMTTYPE=image/jpeg:https://www.atnf.csiro.au/wp-content/uploads/2024/10/askapdataflow_Jul10.jpg
ORGANIZER;CN="Nikhel Gupta":MAILTO:nikhel.gupta@csiro.au
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Australia/Sydney:20241009T150000
DTEND;TZID=Australia/Sydney:20241009T160000
DTSTAMP:20260525T024311
CREATED:20250820T013415Z
LAST-MODIFIED:20250820T013416Z
UID:15095-1728486000-1728489600@www.atnf.csiro.au
SUMMARY:S&A Colloquium: Manasvee Saraf (UWA)
DESCRIPTION:Constraining neutral hydrogen and its environment using radio interferometry\n\nAbstract\n\nIn this talk\, I will present an overview of my PhD research\, conducted over the past three and a half years as a CSIRO co-supervised student. My thesis investigates the relationship between neutral atomic hydrogen gas (HI) and its environment using radio interferometric observations. I will highlight my discovery of HI absorption in the brightest cluster galaxy (BCG) of the Norma cluster\, based on ATCA data\, which supports the BCG’s recent arrival into the cluster core. Additionally\, I will discuss my detection of 25 HI emission detections towards Norma using ASKAP data\, alongside my contribution to and findings from the optimisation of the WALLABY data-processing and HI source-finding pipelines in the presence of bright continuum sources. Finally\, I will contextualise my findings within a broader range of environments\, focusing on my analysis of the scatter in the HI-halo mass relation of central galaxies from the xGASS survey\, where I found a strong correlation with stellar specific angular momentum\, offering key insights for simulations. \nWatch recording\nEvent details\nDownload iCal\nCategory\nColearnia
URL:https://www.atnf.csiro.au/event/sa-colloquium-manasvee-saraf-uwa/
CATEGORIES:Colloquia
ATTACH;FMTTYPE=image/jpeg:https://www.atnf.csiro.au/wp-content/uploads/2024/12/Colloq-09102024.jpg
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Australia/Sydney:20241010T150000
DTEND;TZID=Australia/Sydney:20241010T160000
DTSTAMP:20260525T024311
CREATED:20250820T013649Z
LAST-MODIFIED:20250820T013650Z
UID:15094-1728572400-1728576000@www.atnf.csiro.au
SUMMARY:De Laeter Colloquium: Ron Ekers (CSIRO)
DESCRIPTION:Exploring the nature of scientific discoveries with examples from radio astronomy\n\nAbstract\n\nI will discuss the nature of scientific discoveries which are a key driver for the advancement of science. In the 90-year history of radio astronomy many of the most significant advances in our understanding of the Universe have resulted from technology enabled serendipity. I will discuss a few of these cases (quasars\, pulsars and the galactic centre) in detail to illustrate how the path to discovery can be very different from the widely accepted scientific methodology. I will also comment on how the vision to explore the unknown has influenced the development of the SKA and its precursors. (Image credit: Daily Telegraph) \n\n The de Laeter Colloquium series features distinguished national and international scientists as speakers\, aimed at enhancing interaction between CSIRO\, SKAO\, the two ICRAR nodes\, and high-profile centres of astronomical research around the world. \nWatch recording\nEvent details\nDownload iCal\nCategory\nColearnia
URL:https://www.atnf.csiro.au/event/de-laeter-colloquium-ron-ekers-csiro/
CATEGORIES:Colloquia
ATTACH;FMTTYPE=image/jpeg:https://www.atnf.csiro.au/wp-content/uploads/2024/12/Colloq-10102024.jpg
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Australia/Sydney:20241017T120000
DTEND;TZID=Australia/Sydney:20241017T123000
DTSTAMP:20260525T024311
CREATED:20241128T042123Z
LAST-MODIFIED:20241128T042124Z
UID:6186-1729166400-1729168200@www.atnf.csiro.au
SUMMARY:Colearnium: Jordan Collier (CSIRO)
DESCRIPTION:CARTA – Cube Analysis and Rendering Tool for Astronomy\n\nThis week Jordan Collier will present on “CARTA – Cube Analysis and Rendering Tool for Astronomy”. \n\nPlease let me know if you’re willing to present at a future co-learnium or have requests for specific talks\, thanks! \n\nKind regards\, \n\nSamuel (On behalf of the co-learnium organisers) \n\nTeams meeting link below: \nTeams Meeting\nOrganiser\n\nEvent details\nDownload iCal\nCategory\nColearnia
URL:https://www.atnf.csiro.au/event/colearnium-jordan-collier-csiro/
CATEGORIES:Colearnia
ORGANIZER;CN="Stefan Duchesne":MAILTO:Stefan.Duchesne@csiro.au
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Australia/Sydney:20241023T150000
DTEND;TZID=Australia/Sydney:20241023T160000
DTSTAMP:20260525T024311
CREATED:20250820T013728Z
LAST-MODIFIED:20250820T013729Z
UID:15093-1729695600-1729699200@www.atnf.csiro.au
SUMMARY:S&A Colloquium: Simon Weng (University of Sydney)
DESCRIPTION:The Distribution of Cool Gas In and Around Galaxies\n\nAbstract\n\nUnraveling the evolutionary paths of galaxies remains a key focus in astronomy. Over the past decade\, the circumgalactic medium (CGM) has been recognised as a pivotal component in this research\, serving as a record keeper of the processes of accretion and outflows\, which move gas to and from the interstellar medium. In this talk\, I will explore the CGM properties of galaxies\, linking these properties to their stellar properties and using simulations to guide the interpretation of the observational findings. \nWatch recording\nEvent details\nDownload iCal\nCategory\nColearnia
URL:https://www.atnf.csiro.au/event/sa-colloquium-simon-weng-university-of-sydney/
CATEGORIES:Colloquia
ATTACH;FMTTYPE=image/jpeg:https://www.atnf.csiro.au/wp-content/uploads/2024/12/Colloq-23102024.jpg
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Australia/Sydney:20241024T120000
DTEND;TZID=Australia/Sydney:20241024T123000
DTSTAMP:20260525T024311
CREATED:20241128T042033Z
LAST-MODIFIED:20241128T042034Z
UID:6184-1729771200-1729773000@www.atnf.csiro.au
SUMMARY:Colearnium: Phil Edwards (CSIRO)
DESCRIPTION:Parkrun? But I don’t run!\n\nThis week Phil Edwards will present on “Parkrun? But I don’t run!”. \n\nPlease let me know if you’re willing to present at a future co-learnium or have requests for specific talks\, thanks! \n\nKind regards\, \n\nSamuel (On behalf of the co-learnium organisers) \n\nTeams meeting link below: \nTeams Meeting\nOrganiser\n\nEvent details\nDownload iCal\nCategory\nColearnia
URL:https://www.atnf.csiro.au/event/colearnium-phil-edwards-csiro/
CATEGORIES:Colearnia
ORGANIZER;CN="Stefan Duchesne":MAILTO:Stefan.Duchesne@csiro.au
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Australia/Sydney:20241031T120000
DTEND;TZID=Australia/Sydney:20241031T123000
DTSTAMP:20260525T024311
CREATED:20241128T041756Z
LAST-MODIFIED:20241128T041831Z
UID:6181-1730376000-1730377800@www.atnf.csiro.au
SUMMARY:Colearnium: Georgia Stewart (UTas)
DESCRIPTION:An (AGN) Ghost Story\n\nThis week Georgia Stewart will present on “An (AGN) Ghost Story”. \n\nPlease let me know if you’re willing to present at a future co-learnium or have requests for specific talks\, thanks! \n\nKind regards\, \n\nSamuel (On behalf of the co-learnium organisers) \n\nTeams meeting link below: \nTeams Meeting\nOrganiser\n\nEvent details\nDownload iCal\nCategory\nColearnia
URL:https://www.atnf.csiro.au/event/colearnium-georgia-stewart-utas/
CATEGORIES:Colearnia
ORGANIZER;CN="Stefan Duchesne":MAILTO:Stefan.Duchesne@csiro.au
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Australia/Sydney:20241107T120000
DTEND;TZID=Australia/Sydney:20241107T123000
DTSTAMP:20260525T024311
CREATED:20241128T041641Z
LAST-MODIFIED:20241128T041924Z
UID:6178-1730980800-1730982600@www.atnf.csiro.au
SUMMARY:Colearnium: Emily Kerrison (USyd)
DESCRIPTION:2\,000 years of twinkling: lessons learned from a brief history of astronomical scintillation\n\nThis week Emily Kerrison will present on “2\,000 years of twinkling: lessons learned from a brief history of astronomical scintillation”. \n\nPlease let me know if you’re willing to present at a future co-learnium or have requests for specific talks\, thanks! \n\nKind regards\, \n\nSamuel (On behalf of the co-learnium organisers) \n\nTeams meeting link below: \nTeams Meeting\nOrganiser\n\nEvent details\nDownload iCal\nCategory\nColearnia
URL:https://www.atnf.csiro.au/event/colearnium-emily-kerrison-csiro/
CATEGORIES:Colearnia
ORGANIZER;CN="Stefan Duchesne":MAILTO:Stefan.Duchesne@csiro.au
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Australia/Sydney:20241113T150000
DTEND;TZID=Australia/Sydney:20241113T160000
DTSTAMP:20260525T024311
CREATED:20250820T013807Z
LAST-MODIFIED:20250820T013808Z
UID:15092-1731510000-1731513600@www.atnf.csiro.au
SUMMARY:S&A Colloquium: Meriem Behiri (SISSA)
DESCRIPTION:SHORES: Serendipitous H-ATLAS-fields Observations of Radio Extragalactic Sources with the ATCA\n\nAbstract\n\nIn this presentation\, we explore the advantages of integrating data from the radio to the far-infrared (FIR) spectrum for characterizing dusty star-forming galaxies (DS-FGs). These galaxies are believed to be the star-forming progenitors of local massive quiescent galaxies and are pivotal in reconstructing the cosmic star formation rate density up to high redshifts (Talia+21\,Enia+22\,Behiri+23). Due to their heavily obscured nature by dust\, DSFGs are often invisible in near-infrared/optical/UV bands\, necessitating observations at longer wavelengths\, primarily in the FIR band where dust emission occurs\, and in the radio band\, unaffected by dust absorption. By combining data from these spectral regions\, even the most dust-obscured objects can be characterized\, providing insights into their age\, dust temperature\, and star-formation activity\, and enabling differentiation between various galaxy populations evolving throughout cosmic history (Behiri+24). In this context\, we introduce the Serendipitous H-ATLAS fields Observations of Radio Extragalactic Sources (SHORES) survey. SHORES is a newly conducted survey at 2.1 GHz performed with the Australia Telescope Compact Array\, comprising 27 shallow fields and 2 deep fields centered around a candidate lensed galaxy. These fields are complemented by Herschel observations (H-ATLAS sgp) and data from various surveys (KIDS\, VIKING\, Euclid\, DES\, eRosita..)\, as well as SKAO pathfinders surveys (e.g.\, RACS). The extensive 200+ hours of observations with the ATCA interferometer have enabled us to achieve a 33 uJy rms for the shallow fields and 5 uJy rms for the deep fields\, resulting in a collection of more than 3200 sources. To fully characterize the radio spectra\, the SHORES deep field is observed at 5.5\, 9\, and 20 GHz\, providing crucial insights into various radio populations\, including Active Galactic Nuclei (AGN) and Star-Forming Galaxies (SFGs) (Behiri+\, in prep.). Additionally\, all SHORES observations incorporate polarization measurements\, offering a unique opportunity to explore the polarization nature across a substantial sample of AGN and SFGs (Galluzzi+\, in prep.). This comprehensive\, panchromatic approach provides a crucial perspective for unraveling the mysteries of the radio sky. The broad multi-wavelength coverage of the SHORES survey positions it as an ideal candidate for studying the diverse array of objects in the radio zoo\, thereby preparing us for forthcoming SKAO observations. \nWatch recording\nEvent details\nDownload iCal\nCategory\nColearnia
URL:https://www.atnf.csiro.au/event/sa-colloquium-meriem-behiri-sissa/
CATEGORIES:Colloquia
ATTACH;FMTTYPE=image/jpeg:https://www.atnf.csiro.au/wp-content/uploads/2024/12/Colloq-13112024.jpg
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Australia/Sydney:20241114T120000
DTEND;TZID=Australia/Sydney:20241114T123000
DTSTAMP:20260525T024311
CREATED:20241118T060705Z
LAST-MODIFIED:20241118T060705Z
UID:3631-1731585600-1731587400@www.atnf.csiro.au
SUMMARY:Colearnium: Ivy Wong (CSIRO)
DESCRIPTION:Ivy’s Trip to NRAO\n\nThis week Ivy Wong will present on “Ivy’s Trip to NRAO”. \n\nPlease let me know if you’re willing to present at a future co-learnium or have requests for specific talks\, thanks! \n\nKind regards\, \n\nSamuel (On behalf of the co-learnium organisers) \n\nTeams Meeting link below: \nTeams Meeting\nOrganiser\n\nEvent details\nDownload iCal\nCategory\nColearnia
URL:https://www.atnf.csiro.au/event/colearnium-ivy-wong-csiro/
CATEGORIES:Colearnia
ATTACH;FMTTYPE=image/png:https://www.atnf.csiro.au/wp-content/uploads/2024/11/Screenshot-from-2024-11-18-14-06-38.png
ORGANIZER;CN="Stefan Duchesne":MAILTO:Stefan.Duchesne@csiro.au
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Australia/Sydney:20241118T080000
DTEND;TZID=Australia/Sydney:20241118T170000
DTSTAMP:20260525T024311
CREATED:20241118T051020Z
LAST-MODIFIED:20241118T051021Z
UID:3622-1731916800-1731949200@www.atnf.csiro.au
SUMMARY:Colloquium: Michael (aff)
DESCRIPTION:Radio continuum emission from very massive galaxies\n\nEvent summary text (summary text is slightly larger than regular text) … \n\nDescribe the details of your event here … \nAdd a button here\nLocation\n\nOrganiser\n\nEvent details\nDownload iCal\nCategory\nColloColearnia
URL:https://www.atnf.csiro.au/event/colloquium-michael-aff/
LOCATION:Marsfield Lecture Theatre\, 26 Pembroke Road\, Marsfield\, NSW\, 2122\, Australia
ORGANIZER;CN="Nikhel Gupta":MAILTO:nikhel.gupta@csiro.au
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Australia/Sydney:20241120T150000
DTEND;TZID=Australia/Sydney:20241120T160000
DTSTAMP:20260525T024311
CREATED:20250820T013832Z
LAST-MODIFIED:20250820T013833Z
UID:15091-1732114800-1732118400@www.atnf.csiro.au
SUMMARY:S&A Colloquium: Michael Brown (Monash)
DESCRIPTION:Radio continuum emission from very massive galaxies\n\nAbstract\n\nSome of the first radio continuum radio sources to be identified were powerful radio-loud active galactic nuclei in very massive elliptical galaxies such as M87. As radio surveys have improved over the past seven decades\, an increasing fraction of massive elliptical galaxies have been found to host radio continuum sources. I will present recent work using the Australian Square Kilometre Array Pathfinder to search for radio continuum emission from local very massive galaxies without star formation. We find a very large fraction of very massive galaxies are radio continuum sources. However\, the radio powers of these sources can vary by orders of magnitude (at fixed galaxy mass)\, and there are some tantalising correlations between radio power\, morphology and host galaxy kinematics. \nWatch recording\nEvent details\nDownload iCal\nCategory\nColearnia
URL:https://www.atnf.csiro.au/event/sa-colloquium-michael-brown-monash/
CATEGORIES:Colloquia
ATTACH;FMTTYPE=image/png:https://www.atnf.csiro.au/wp-content/uploads/2024/12/Colloq-20112024.png
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Australia/Sydney:20241121T120000
DTEND;TZID=Australia/Sydney:20241121T123000
DTSTAMP:20260525T024311
CREATED:20241118T061018Z
LAST-MODIFIED:20241118T061019Z
UID:3638-1732190400-1732192200@www.atnf.csiro.au
SUMMARY:Colearnium: Tegan Carter + Carlie Ring + Bev Rose (CSIRO)
DESCRIPTION:Child Safety in Space and Astronomy\n\nThis week Tegan Carter + Carlie Ring + Bev Rose will present on “Child Safety in Space and Astronomy”. \n\nPlease let me know if you’re willing to present at a future co-learnium or have requests for specific talks\, thanks! \n\nKind regards\, \n\nSamuel (On behalf of the co-learnium organisers) \n\nTeams meeting link below: \nTeams Meeting\nOrganiser\n\nEvent details\nDownload iCal\nCategory\nColearnia
URL:https://www.atnf.csiro.au/event/colearnium-tegan-carter-carlie-ring-bev-rose-csiro/
CATEGORIES:Colearnia
ORGANIZER;CN="Stefan Duchesne":MAILTO:Stefan.Duchesne@csiro.au
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Australia/Sydney:20241128T120000
DTEND;TZID=Australia/Sydney:20241128T123000
DTSTAMP:20260525T024311
CREATED:20241128T010048Z
LAST-MODIFIED:20241128T004826Z
UID:5061-1732795200-1732797000@www.atnf.csiro.au
SUMMARY:Colearnium: Li Wang (CSIRO)
DESCRIPTION:Astronomy from a non-Astronomer’s Perspective\n\nThis week Li Wang will present on “Astronomy from a non-Astronomer’s Perspective”. \n\nPlease let me know if you’re willing to present at a future co-learnium or have requests for specific talks\, thanks! \n\nKind regards\, \n\nSamuel (On behalf of the co-learnium organisers) \n\nTeams meeting link below: \nTeams Meeting\nOrganiser\n\nEvent details\nDownload iCal\nCategory\nColearnia
URL:https://www.atnf.csiro.au/event/colearnium-li-wang-csiro/
CATEGORIES:Colearnia
ORGANIZER;CN="Stefan Duchesne":MAILTO:Stefan.Duchesne@csiro.au
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Australia/Sydney:20241203T150000
DTEND;TZID=Australia/Sydney:20241203T160000
DTSTAMP:20260525T024311
CREATED:20241127T172046Z
LAST-MODIFIED:20241127T172048Z
UID:5917-1733238000-1733241600@www.atnf.csiro.au
SUMMARY:Kristine Spekkens Colloquium
DESCRIPTION:Gas-Rich Galaxies as Cosmological Probes\n\n \n\nAbstract \n\nThe atomic gas (HI) content of nearby galaxies provides important insight into how they form and evolve within the standard cosmology. In this talk\, I will highlight some of my group’s recent progress towards building statistical samples of gas-rich galaxies to use as cosmological probes. I will first focus on how sensitive HI searches in optically-selected dwarf and ultra-diffuse galaxy candidates are a powerful tool for measuring their structure and constraining formation models. I will then describe how the widefield WALLABY survey\, now underway on the Australian SKA Pathfinder (ASKAP)\, is delivering the first spatially-resolved populations of HI disks for comparison with cosmological predictions. This work paves the way for probing HI disks across cosmic time using the SKA when it comes online towards the end of this decade. \nAdd a button here\nLocation\n\nOrganiser\n\nEvent details\nDownload iCal\nCategory\nColearnia
URL:https://www.atnf.csiro.au/event/kristine-spekkens-colloquium/
LOCATION:26 Dick Perry Ave\, Kensington WA 6151\, 26 Dick Perry Avenue\, Kensington\, Washington\, 6151
CATEGORIES:Colloquia
ORGANIZER;CN="Nikhel Gupta":MAILTO:nikhel.gupta@csiro.au
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Australia/Sydney:20241204T150000
DTEND;TZID=Australia/Sydney:20241204T160000
DTSTAMP:20260525T024311
CREATED:20241129T001542Z
LAST-MODIFIED:20241129T002459Z
UID:6259-1733324400-1733328000@www.atnf.csiro.au
SUMMARY:S&A Colloquium: Bryan Scott (CIERA\, Northwestern University)
DESCRIPTION:Prospects for Fundamental Physics from Line Intensity Mapping\n\nAbstract \n\nLine Intensity Mapping (LIM) is a technique for quickly performing surveys of large volumes at many frequencies but at low spatial resolution. These large survey volumes make LIM a promising method for constraining fundamental physics\, such as beyond wCDM cosmology or extensions of Einstein Gravity in the coming decade. I will begin this talk with a presentation of LIM and synergies with photometric and spectroscopic galaxy surveys\, in particular the Vera C. Rubin Observatory Legacy Survey of Space & Time (LSST) and surveys with the Subaru Observatory Prime Focus Spectrograph (PFS). After introducing forecasting results for fundamental physics with LIM\, I will discuss how astrophysical uncertainties pose barriers to interpretation and conclude with an overview of prospects for machine learning and improved statistical methods to meet these challenges \nJoin Event on Microsoft Teams\nLocation\n\nOrganiser\n\nEvent details\nDownload iCal\nCategory\nColearnia
URL:https://www.atnf.csiro.au/event/sa-colloquium-bryan-scott-ciera-northwestern-university/
LOCATION:Marsfield Lecture Theatre\, 26 Pembroke Road\, Marsfield\, NSW\, 2122\, Australia
CATEGORIES:Colloquia
ATTACH;FMTTYPE=image/png:https://www.atnf.csiro.au/wp-content/uploads/2024/11/SCR-20241129-kgfz.png
ORGANIZER;CN="Joshua Preston Pritchard":MAILTO:joshua.pritchard@csiro.au
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Australia/Sydney:20241211T150000
DTEND;TZID=Australia/Sydney:20241211T160000
DTSTAMP:20260525T024311
CREATED:20241204T030024Z
LAST-MODIFIED:20241211T024822Z
UID:12379-1733929200-1733932800@www.atnf.csiro.au
SUMMARY:S&A Colloquium: Vincenzo Galluzzi (IRA-INAF\, Bologna)
DESCRIPTION:From Data Archives to Science Gateways: examples of INAF-supported radio facilities.\n\nAbstract \n\nData archives are now rapidly evolving from simple repositories to sophisticated science gateways\, facilitating data discovery\, access\, retrieval\, visualization\, processing\, interoperability (with data at different wavelengths or from different messengers)\, and reuse. This transformation is driven by the increasing volume and complexity of data generated by modern radio astronomy facilities\, which offer unprecedented potential for scientific discovery. \n\nINAF has been at the forefront of this evolution\, actively embracing Open Science principles\, through supporting various initiatives promoted by the International Virtual Observatory Alliance (IVOA) in developing and implementing new standards. From the perspective of the radio astronomical facilities I am working with\, I will present some examples of e-infrastructures or projects at various scales\, including: \n\n\nThe INAF Radio Telescope Data Archive\, a newly operational archive providing access to a wealth of radio astronomical data. In such a context\, I will also briefly address the INAF contribution to the IVOA Radio Interest Groups (RIG)\, which recently proposed an extension of the ObsCore Data Model (ObsCore DM) for bolstering the discovery of radio data.\n\n\n\nThe Additional Representative Images for Legacy (ARI-L) project\, leaded by the Italian node of the ALMA Regional Centre: this project reprocessed ALMA data from earlier cycles (2-4) in order to support archival science projects\, hence adding value to the ALMA Science Archive (ASA) itself.\n\n\n\nThe deployment of the Italian node of the SKA Regional Centre Network (SRCNet): the Team Orange established by the SRC Steering Committee (SRCSC) has been working on a prototype for data visualization\, and recently changed its focus towards deployment activities\, since Italy will host one of the first 9 nodes of the SRCNet.\n\nJoin Event on Microsoft Teams\nLocation\n\nOrganiser\n\nEvent details\nDownload iCal\nCategory\nColearnia
URL:https://www.atnf.csiro.au/event/sa-colloquium-vincenzo-galluzi-ira-inaf-bologna/
LOCATION:Marsfield Lecture Theatre\, 26 Pembroke Road\, Marsfield\, NSW\, 2122\, Australia
CATEGORIES:Colloquia
ATTACH;FMTTYPE=image/png:https://www.atnf.csiro.au/wp-content/uploads/2024/12/ATNF_colloquium_Galluzzi_Vincenzo.png
ORGANIZER;CN="Joshua Preston Pritchard":MAILTO:joshua.pritchard@csiro.au
END:VEVENT
END:VCALENDAR