Difference between revisions of "Multi-wavelength facilities and contacts"
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'''To go back to the EGal wikipage, use [[Extragalactic_Working_Group|this link]]''' <br> | '''To go back to the EGal wikipage, use [[Extragalactic_Working_Group|this link]]''' <br> | ||
| − | == X-rays == | + | == Facilities with possibility of ToO/follow up == |
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| + | === X-rays === | ||
{| class="wikitable" | {| class="wikitable" | ||
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| − | == UV == | + | === UV === |
{| class="wikitable" | {| class="wikitable" | ||
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| − | == Optical == | + | === Optical === |
{| class="wikitable" | {| class="wikitable" | ||
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| − | == IR == | + | === IR === |
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| − | == Radio/mm == | + | === Radio/mm === |
{| class="wikitable" | {| class="wikitable" | ||
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| XXX | | XXX | ||
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| + | == Monitoring programs to look for archival data or automatic observations == | ||
Revision as of 12:49, 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
Facilities with possibility of ToO/follow up
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, 1.0m | 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 | 2.0m | IO:O (SDSS ugriz, Bessell BV) RISE (V+R filter) MOPTOP (BVRI and open) SPRAT (4020–8100Å spectroscopy) LIRIC (R, also IR) |
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, LIRIC 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. |
| Kanata | 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 |
