Electromagnetic Follow-up to Gravitational Wave Events with the UltraViolet EXplorer (UVEX)
Fuente:
arXiv
Guardado en:
| Autores principales: | , , , , , , , , , , , |
|---|---|
| Formato: | Preprint |
| Publicado: |
2025
|
| Materias: | |
| Acceso en línea: | |
| Etiquetas: |
Agregar Etiqueta
Sin Etiquetas, Sea el primero en etiquetar este registro!
|
| _version_ | 1866909599334924288 |
|---|---|
| author | Criswell, Alexander W. Leggio, Sydney C. Coughlin, Michael W. Singer, Leo P. Kiendrebeogo, R. Weizmann Andreoni, Igor Toivonen, Andrew Earnshaw, Hannah P. Gezari, Suvi Grefenstette, Brian W. Harrison, Fiona A. Kasliwal, Mansi M. |
| author_facet | Criswell, Alexander W. Leggio, Sydney C. Coughlin, Michael W. Singer, Leo P. Kiendrebeogo, R. Weizmann Andreoni, Igor Toivonen, Andrew Earnshaw, Hannah P. Gezari, Suvi Grefenstette, Brian W. Harrison, Fiona A. Kasliwal, Mansi M. |
| contents | The Ultraviolet Explorer (UVEX) is expected to fly in 2030 and will have the opportunity -- and the rapid near/far ultraviolet (UV) capabilities -- to glean unprecedented insight into the bright UV emission present in kilonovae like that of AT 170817gfo, the electromagnetic counterpart to binary neutron star merger GW170817. To do so, it will need to perform prompt target-of-opportunity observations following detection of binary neutron star mergers by the LIGO-Virgo-KAGRA gravitational observatories. We present initial simulations to develop UVEX target-of-opportunity strategies for such events and provide the community with detailed initial estimates of the prospects for and characteristics of UVEX target-of-opportunity observations following gravitational-wave events, considering fiducial scenarios for the fifth and sixth LIGO-Virgo-KAGRA observing runs. Additionally, in light of the relatively few binary neutron star mergers observed since GW170817, we consider variant target-of-opportunity strategies for UVEX to maximize scientific gain in the case of a lowered binary neutron star merger rate. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2501_14109 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | Electromagnetic Follow-up to Gravitational Wave Events with the UltraViolet EXplorer (UVEX) Criswell, Alexander W. Leggio, Sydney C. Coughlin, Michael W. Singer, Leo P. Kiendrebeogo, R. Weizmann Andreoni, Igor Toivonen, Andrew Earnshaw, Hannah P. Gezari, Suvi Grefenstette, Brian W. Harrison, Fiona A. Kasliwal, Mansi M. High Energy Astrophysical Phenomena The Ultraviolet Explorer (UVEX) is expected to fly in 2030 and will have the opportunity -- and the rapid near/far ultraviolet (UV) capabilities -- to glean unprecedented insight into the bright UV emission present in kilonovae like that of AT 170817gfo, the electromagnetic counterpart to binary neutron star merger GW170817. To do so, it will need to perform prompt target-of-opportunity observations following detection of binary neutron star mergers by the LIGO-Virgo-KAGRA gravitational observatories. We present initial simulations to develop UVEX target-of-opportunity strategies for such events and provide the community with detailed initial estimates of the prospects for and characteristics of UVEX target-of-opportunity observations following gravitational-wave events, considering fiducial scenarios for the fifth and sixth LIGO-Virgo-KAGRA observing runs. Additionally, in light of the relatively few binary neutron star mergers observed since GW170817, we consider variant target-of-opportunity strategies for UVEX to maximize scientific gain in the case of a lowered binary neutron star merger rate. |
| title | Electromagnetic Follow-up to Gravitational Wave Events with the UltraViolet EXplorer (UVEX) |
| topic | High Energy Astrophysical Phenomena |
| url | https://arxiv.org/abs/2501.14109 |