Difference between revisions of "Multi-wavelength facilities and contacts"

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| J, FELH1500 (15200-16700Å)  
 
| J, FELH1500 (15200-16700Å)  
 
| https://telescope.livjm.ac.uk/web_submission/  
 
| https://telescope.livjm.ac.uk/web_submission/  
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| ltphase1@ljmu.ac.uk (questions about applying for time on the LT or to ask about time allocation policies) <br>ltsupport_astronomer@ljmu.ac.uk (questions on preparing LT observations using the Phase 2 GUI, data retrieval and telescope use, and for any other general questions)
 
| Relatively fast reaction through the Reactive Time form of the link.
 
| Relatively fast reaction through the Reactive Time form of the link.
 
|-
 
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Revision as of 12:45, 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

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

Size

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 2m IO:O (SDSS ugriz, Bessell BV)
RISE (V+R filter)
MOPTOP (BVRI and open)
SPRAT (4020–8100Å spectroscopy)
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)
ltsupport_astronomer@ljmu.ac.uk (questions on preparing LT observations using the Phase 2 GUI, data retrieval and telescope use, and for any other general questions)
Relatively fast reaction through the Reactive Time form of the link.
Photometry with IO:O and MOPTOP, polarimetry with MOPTOP, spectroscopy with SPRAT
NOT XXX XXX XXX XXX XXX

IR

Instrument

Size

Filters/Energy range

Webpage

Contact information

Notes

Canica XXX XXX XXX XXX XXX
Liverpool Telescope 2.0m J, FELH1500 (15200-16700Å) https://telescope.livjm.ac.uk/web_submission/ ltphase1@ljmu.ac.uk (questions about applying for time on the LT or to ask about time allocation policies)
ltsupport_astronomer@ljmu.ac.uk (questions on preparing LT observations using the Phase 2 GUI, data retrieval and telescope use, and for any other general questions)
Relatively fast reaction through the Reactive Time form of the link.
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