Pour vous authentifier, privilégiez eduGAIN / To authenticate, prefer eduGAINeu

S'authentifier

3rd Astro-COLIBRI multi-messenger astrophysics workshop

16–20 sept. 2024
Institut Pascal
Fuseau horaire Europe/Paris

Contact

Liste des contributions

41 / 41
37. Welcome
Fabian Schüssler (IRFU / CEA Paris-Saclay)
16/09/2024 10:00
34. Participants presentations
16/09/2024 10:15
35. Multi-messenger theory and modelling
Frédéric DAIGNE (Institut d'Astrophysique de Paris - Sorbonne University)
16/09/2024 11:00
36. The Multi-Messenger Astronomy Followup Ecosystem
Curtis McCully
16/09/2024 11:45

The Multi-Messenger Astrophysics (MMA) era has necessitated that we coordinate the community at an entirely new level. Many of these events (e.g., gravitational wave and neutrino sources) are not localized enough to unambiguously identify the electromagnetic counterpart. Instead, large-scale searches are necessary to localize the source to combine the information from the different...
57. Swift
Phil Evans
16/09/2024 14:00
60. NITRATES / GUANO
Jimmy DeLaunay
16/09/2024 14:15

Alerts and results from Swift-BAT GUANO data and the NITRATES analysis

In 2019 the Gamma-ray Urgent Archiver for Novel Opportunities (GUANO) was implemented, allowing for time-tagged event data for the Swift Burst Alert Telescope (BAT) to be saved on command around times of interest. This allows for more sensitive analyses to be performed on the ground. The most sensitive being, the...
58. Einstein Probe
Erik Kuulkers
16/09/2024 14:30

Einstein probe: searching the Universe for cosmic variable objects and transient phenomena shining in X-ray light

The Einstein Probe (EP) is a mission of the Chinese Academy of Sciences (CAS) in collaboration with ESA, MPE and CNES dedicated to time-domain high-energy astrophysics. Its primary goals are to discover high-energy transients and monitor variable objects. To achieve this, EP...
59. SVOM
Damien Turpin
16/09/2024 14:45
61. Fermi
Deirdre Horan
16/09/2024 15:00
62. IACTs
Alessio Berti (Max Planck Institute for Physics)
16/09/2024 15:15

Multimessenger astrophysics recently provided groundbreaking results, in many cases involving transient sources. The study of this type of objects can be challenging, especially from an observational point of view. In particular, in the electromagnetic domain, the very-high-energy gamma-ray band (E>~100 GeV) can provide vital information on the sources themselves and their environment. In this...
53. TESS
Kyle Hart
16/09/2024 16:00

TESS Transient Light Curve Patrol
The Transiting Exoplanet Survey Satellite (TESS) is a space telescope mission developed by NASA with the goal of detecting exoplanets. Over the duration of it's mission, TESS has trained its wide-field imaging array on dozens of sky sectors, and identified thousands of candidate targets. Our team has developed a a subtraction pipeline for these full frame...
54. ATLAS
Heloise Stevance
16/09/2024 16:15
55. LAST
Ruslan Konno (Weizmann Institute)
16/09/2024 16:30
56. Argus Array
Hank Corbett
16/09/2024 16:45

Data products, public access, and survey optimization for the Argus Array

The Argus Array will be a 900-telescope optical survey instrument with a combined collecting area equivalent to a 5-meter telescope and an 8000 sq. deg simultaneous field of view, currently slated for first light in 2027. Operating at depths comparable to those of the deepest active sky surveys, Argus will capture a...
9. Current version and features
16/09/2024 17:00
65. Multi-Messenger Online Data Analysis and Galaxy platform
Andrii Neronov
17/09/2024 09:00

Multi-Messenger Online Data Analysis platform (MMODA) and Galaxy platforms provide services for on-the-fly analysis of publicly available data astronomical and astroparticle data for a range of telescopes. The platforms also provide a possibility for users to add new services based on user-contributed analysis workflows formulated in the form of python notebooks.
64. ACROSS: The Astrophysics CRoss Observatory Science Support Initiative
Jamie Kennea
17/09/2024 09:15

In October 2022, NASA HQ directed the Physics of the Cosmos program office initiated a study to identify requirements and formulate implementation options for a TDAMM Guest of Observer Facility, in response to Astro2020 TDAMM recommendations. Phase 1 of the study investigated the coordination of NASA space-based missions. As a result of this study, NASA approved a pilot program for The...
63. Fast Radio Burst Alerts : frb-voe and the CHIME/FRB Virtual Observatory Event Service
Thomas Abbott
17/09/2024 09:30

Discovered in 2007, fast radio bursts (FRBs) are luminous, millisecond duration radio bursts that have quickly become one of the most fascinating classes of radio transients. The progenitor of FRBs remains a mystery, however, through observations like that of the FRB-like bursts detected from a galactic magnetar, SGR 1935+2154, it has been shown that collaborative efforts from multiple...
66. Predicting the topics of a follow-up Astronomical Telegram using knowledge graphs and natural language processing
Andrei Variu
17/09/2024 09:45

We have developed an automatic pipeline to predict the topics of a follow-up ATel and to assign data-analysis workflows, that will be publicly available at https://www.astro.unige.ch/mmoda/. To achieve this, we have created an ontology of telescopes, observatories and instruments in order to detect them in Astronimical Telegrams. Studying the occurances of these telescopes in the ATels, we...
69. Accretion and ejection in binary systems
Sylvain Chaty (Université Paris Cité)
17/09/2024 10:30

I will review accretion and ejection phenomena in low-mass and high-mass X-ray binary systems
72. Online analyses in KM3NeT
Silvia Celli
17/09/2024 10:45
67. Constraining Astrophysical Observables using Gravitational Wave Background
Musfar Muhamed Kozhikkal
17/09/2024 11:00

Pulsar Timing Array (PTA) is close to detecting Gravitational Wave Background (GWB) in the frequency range of nHz to µHZ. We present an extended analytic model to describe the characteristic spectrum of the GWB using the merger rate of supermassive black hole binary (SMBHB) in the Universe. Astrophysical observables (Galaxy stellar mass function (GSMF), pair fraction, merger timescale and mass...
71. Investigate the impact of magnetar on the kilonova afterglow emission in short GRBs through late-time radio observations
Ankur Gosh
17/09/2024 11:15

The coincident detection of Gravitational Wave (GW~170817) and short Gamma Ray Burst (GRB~170817A) confirmed their common origin from the coalescence of binary neutron stars (BNS). Depending on the BNS masses and equations of state, the outcome could be a black hole or a millisecond magnetar. In the presence of a magnetar, a significant portion of its rotational energy is transferred to the...
68. TBC (Stellar Physics & Ground-based observation & data analysis)
Merieme Chadid
17/09/2024 11:30
40. IceCube
Erik Blaufuss
17/09/2024 13:30
41. KM3NeT
Jean-Grégoire Ducoin
17/09/2024 13:45
42. SuperK-SN
Barry Pointon
17/09/2024 14:00

The detection of SN burst neutrinos from a nearby/Galactic core-collapse supernova (SN) can provide an early warning to the multi-messenger astronomy community. As the world’s largest water-Cherenkov detector, Super-Kamiokande (SK) maintains an independent SN alert system, “SNWatch”, and also contributes to SNEWS. Recent upgrades to the SK detector and SNWatch have increased the capabilities...
46. SNEWS
Jeff Tseng
17/09/2024 14:15

The Supernova Early Warning System (SNEWS) is a network of neutrino and dark matter detectors which aims to detect coincident neutrino signals in multiple detectors and alert the worldwide observer community. It has been in automated operation since 2005, but is now undergoing a significant upgrade with goals including increasing sensitivity for both neutrino bursts as well as pre-supernova...
43. LIGO-Virgo-KAGRA
Monica Seglar Arroyo (IFAE)
17/09/2024 14:30
44. Redback
Nikhil Sarin
17/09/2024 14:45
45. Neutrino sources
Foteini Oikonomou (Norwegian University of Science and Technology (NTNU))
17/09/2024 15:00
47. GCN
Vidushi Sharma
17/09/2024 15:45

General Coordinates Network (GCN): NASA's Next Generation Time-Domain and Multimessenger Astronomy Alert SystemA

The General Coordinates Network (GCN) is a public collaboration platform run by NASA for the astronomy research community to share alerts and rapid communications about high-energy, multimessenger, and transient phenomena. Over the past 30 years, GCN has helped enable many...
48. TNS
Ofer Yaron
17/09/2024 16:00
50. FINK
Julien Peloton (CNRS-IJCLab)
17/09/2024 16:15
51. TreasureMap
Samuel Wyatt
17/09/2024 16:30

The Gravitational Wave Treasure Map is designed to help coordinate electromagnetic followup of gravitational-wave (GW) events. It allows observers to easily report their planned and executed observations in search of counterparts to GW events, and to query the reports of other observers, in a programatic way. The goal is to enable coordination between observatories in order to minimize...
52. BHTOM
Lukasz Wyrzykowski
17/09/2024 16:45
38. RAPAS
Thierry Midavaine
17/09/2024 17:00

RAPAS project : 2024 status

The RAPAS project is on its third year of development. We will present the photometric accuracy of the network and the first results we got from the two spectrograph prototypes to deliver photometric and spectral energy distribution on alerts. A first Astro-COLIBRI filter is connected to the RAPAS network to disseminate alect selection then monitoring.
39. WIVONA
Jean-Paul Godard
17/09/2024 17:15

Implementing Astro-Colibry query in PRISM and Sharcap

Wivona is a PRO/AM collaboration to develop access to and usage of the Virtual Observatory data in the amateur's Community.
Transients related data are part of the aim .
PRISM and Sharpcap have been choosen to initiate the developments. Related Software will be open source and support will be provided to requesting developpers.
33. Conclusions
Fabian Schüssler (IRFU / CEA Paris-Saclay)
20/09/2024 12:00
49. AMPEL
70. DLT40 + short plateau SNe (tbc)
Darshana Mehta
Fonctionne avec Indico v3.3.3