Difference between revisions of "Multi-wavelength facilities and contacts"
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| XXX | | XXX | ||
| Regular monitoring, possibility of increased cadence during interesting events | | Regular monitoring, possibility of increased cadence during interesting events | ||
+ | |- | ||
+ | | Kanata | ||
+ | | XXX | ||
+ | | XXX | ||
+ | | XXX | ||
+ | | XXX | ||
+ | | XXX | ||
+ | |- | ||
+ | | Liverpool telescope | ||
+ | | XXX | ||
+ | | 2m | ||
+ | | https://telescope.livjm.ac.uk/PropInst/Reactive/ | ||
+ | | ltphase1@ljmu.ac.uk (questions about applying for time on the LT or to ask about time allocation policies) | ||
+ | | Relatively fast reaction through the Reactive Time form of the link | ||
+ | |- | ||
+ | | NOT | ||
+ | | XXX | ||
+ | | XXX | ||
+ | | XXX | ||
+ | | XXX | ||
+ | | XXX | ||
|} | |} | ||
Revision as of 12:35, 10 April 2024
This wikipage will serve as a summary of available multi-wavelength facilities that can be contacted in case of needing broadband follow-up observations of ToO/observing campaigns.
To go back to the EGal wikipage, use this link
Contents
X-rays
Instrument |
Filters/Energy range |
Webpage |
Contact information |
Notes |
Swift-XRT | 0.2-10 keV | https://www.swift.psu.edu/toop/request.php | -- | ToOs through ToO form in the webpage link |
XMM-Newton | 0.1-10 keV | https://www.cosmos.esa.int/web/xmm-newton/too-alert | -- | ToOs through ToO form in the webpage link |
NuSTAR | 3-79 keV | https://nustarsoc.caltech.edu/NuSTAR_Public/GO/GOsubmit.php | -- | ToOs through ToO form in the webpage link |
UV
Instrument |
Filters/Energy range |
Webpage |
Contact information |
Notes |
Swift-UVOT | b, v, u, w1, m2, w2 | https://www.swift.psu.edu/toop/request.php | -- | ToOs through ToO form in the webpage link |
Optical
Instrument |
Telescope |
Filters/Energy range |
Webpage |
Contact information |
Notes |
Las Cumbres | 0.4m, 1m | Johnson-Cousins/Bessell UBVRI SDSS/PanSTARRS u’g’r’i’zsYw |
https://lco.global/about/ | Jose Acosta Pulido (jose.acosta@iac.es) Jorge Otero Santos (joteros@iaa.es) |
Only photometry, schedule relatively flexible |
IAC80 | 0.8m | Johnson UBVRI Sloan grizy |
https://www.iac.es/es/observatorios-de-canarias/telescopios-y-experimentos/iac80-telescope | Jose Acosta Pulido (jose.acosta@iac.es) Jorge Otero Santos (joteros@iaa.es) |
Only photometry |
Sierra Nevada Observatory | 0.9m, 1.5m | UBVRI | https://www.osn.iaa.csic.es/en | Jorge Otero Santos (joteros@iaa.es) Iván Agudo (iagudo@iaa.es) |
BVRI photo-polarimetry (most of the photometry at the 1.5m, polarimetry at the 0.9m) |
Calar Alto Observatory | 2.2m | UBVRI | http://www.caha.es | Jorge Otero Santos (joteros@iaa.es) Iván Agudo (iagudo@iaa.es) |
Very limited nights and ToO triggers |
Tuorla monitoring | XXX | R | https://users.utu.fi/kani/1m/index.html | XXX | Regular monitoring, possibility of increased cadence during interesting events |
Kanata | XXX | XXX | XXX | XXX | XXX |
Liverpool telescope | XXX | 2m | https://telescope.livjm.ac.uk/PropInst/Reactive/ | ltphase1@ljmu.ac.uk (questions about applying for time on the LT or to ask about time allocation policies) | Relatively fast reaction through the Reactive Time form of the link |
NOT | XXX | XXX | XXX | XXX | XXX |
IR
Instrument |
Filters/Energy range |
Webpage |
Contact information |
Notes |
Canica | XXX | XXX | XXX | XXX |
XXX | XXX | XXX | XXX | XXX |
XXX | XXX | XXX | XXX | XXX |
Radio/mm
Instrument |
Filters/Energy range |
Webpage |
Contact information |
Notes |
SMA/Effelsberg | XXX | XXX | XXX | XXX |
IRAM | XXX | XXX | XXX | XXX |
Metsahövi | XXX | XXX | XXX | XXX |