Difference between revisions of "Multi-wavelength facilities and contacts"
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Revision as of 13:08, 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.
Information on monitoring/automatically running programs that may contain blazar data for sources of interest is also included here.
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, running blazar monitoring program by Jose Acosta and Jorge Otero |
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, running blazar monitoring program by Jose Acosta and Jorge Otero |
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), time can be allocated through the MAPCAT program (https://home.iaa.csic.es/~iagudo/research/MAPCAT/MAPCAT.html) |
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, time can be allocated through the MAPCAT program (https://home.iaa.csic.es/~iagudo/research/MAPCAT/MAPCAT.html) |
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 | 2.1m | JHK | https://astro.inaoep.mx/en/observatories/oagh/near-infrared-imaging-camera-canica | Luis Carrasco () | Blazar observations by Luis Carrasco, contact directly for collaboration/data |
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 |
Size |
Filters/Energy range |
Webpage |
Contact information |
Notes |
SMA | XXX | XXX | XXX | XXX | XXX |
Effelsberg | XXX | XXX | XXX | XXX | XXX |
IRAM | 30m | 3.5mm, 1.3mm | https://iram-institute.org/observatories/30-meter-telescope/ | Iván Agudo (iagudo@iaa.es) | Limited observing nights, time can be allocated through the POLAMI program (see https://polami.iaa.es) |
Metsahövi | 14m | 37 GHz | https://www.aalto.fi/en/metsahovi-radio-observatory/active-galaxies | agn-metsahovi@aalto.fi | Regular monitoring, possibility of increased cadence during interesting events, data requests to the contact email |
Monitoring programs to look for archival data and/or automatic observations
Program |
Filters/Energy range |
Webpage |
Contact information |
Notes |
ASAS-SN | Sloan g, Johnson V | https://asas-sn.osu.edu | -- | Supernova database, monitors the sky, aperture photometry of blazars available, currently running (since 2011) |