Solar full-disk images from the Chromospheric Telescope (ChroTel)
Short Name:
chrotel.epn_core
Date:
13 Jun 2024 15:22:09
Publisher:
Leibniz Institute for Solar Physics KIS
Description:
Chromospheric Telescope (ChroTel) at the Observatorio del Teide on
Tenerife is a multi-wavelength imaging telescope for full-disk
synoptic observations of the solar chromosphere. ChroTel observations
are conducted using Lyot-type filters for the chromospheric lines of
Ca, H, and He. The instrument operates autonomically and gathers
imaging data in all three channels with a cadence of down to one
minute.
In this EPN-TAP table, we provide ChroTel data starting in 2012. Data
becomes public one year after the observeration.
Catalogues of solar observations held at MSSL/UCL. Datasets available are SOHO CDS, SOHO EIT, Yohkoh SXT. URL links to data files are provided (EIT data files provided by SDAC, NASA). Reference: http://www.mssl.ucl.ac.uk/www_solar/surfindex.html
Catalogues of solar observations held at MSSL/UCL. Datasets available are SOHO CDS, SOHO EIT, Yohkoh SXT. URL links to data files are provided (EIT data files provided by SDAC, NASA). Reference: http://www.mssl.ucl.ac.uk/www_solar/surfindex.html
Solar Radio Emission Observations at “Orbita” Radio Polygon
Short Name:
solar_flux data
Date:
12 Dec 2024 19:58:36
Publisher:
Fesenkov Astrophysical Institute
Description:
The “Orbita” Radio Polygon at an altitude of 2750 meters conducts solar radio emission observations using state-of-the-art equipment. This includes instruments for monitoring solar radio flux at frequencies of 1 GHz and 2.8 GHz, as well as the Callisto solar radio spectrograph, which is part of the international e-Callisto network. These tools enable the detection of solar radio bursts of types II, III, IV, and V, and provide valuable insights for forecasting the geo-effectiveness of solar flare activity.
The provided dataset consists of daily tables, where each table corresponds to a single observation day. The data includes two columns:
- **timestamp**: The time of observation at the detector.
- **SFU**: The solar flux unit measurement, representing the intensity of solar radio emission in SFU (Solar Flux Units).
The data is collected and provided by the Institute of Ionosphere (https://ionos.kz/).
Solar Spectra from the Gregor Infrared Spectrograph (GRIS)
Short Name:
gris.epn_core
Date:
14 Jun 2024 14:28:15
Publisher:
Leibniz Institute for Solar Physics KIS
Description:
GRIS (GREGOR Infrared Spectrograph) is the grating spectrograph
installed at the GREGOR solar telescope. The spectrograph is mostly
used in combination with the infrared detector of the Tenerife
Infrared Polarimeter (TIP-II) to study the sun's photosphere and
chromosphere. The slit length corresponds to some 60 arcsec, with a
sampling of 0.13 arcsec.
In this EPN-TAP table, we provide GRIS scans starting in 2014. Data
becomes public one year after the observeration.
Solar spectra from the Laser Absolute Reference Spectrograph (LARS)
Short Name:
lars.epn_core
Date:
14 Jun 2024 10:10:51
Publisher:
Leibniz Institute for Solar Physics KIS
Description:
The Laser Absolute Reference Spectrograph (LARS) at the Vaccuum Tower
Telescope (VTT), Observatorio del Teide on Tenerife is a
high-resolution echelle spectrograph capable of providing absolutely
calibrated solar spectra in the visible 480nm to 750nm range.
In this EPN-TAP table, we provide LARS data starting in 2016. Data
becomes public one year after the observeration.
Southern GOODS Field: VLT ISAAC Observations, H band
Short Name:
GOODS ISAAC H
Date:
07 Mar 2025
Publisher:
NASA/GSFC HEASARC
Description:
As part of the Great Observatories Origins Deep Survey (GOODS),
near-infrared imaging observations of the Chandra Deep Field South (CDF-S)
were carried out in J, H, Ks bands, using the ISAAC instrument mounted at
the Antu Unit Telescope of the VLT at ESO's Cerro Paranal Observatory, Chile.
<p>
These data were obtained as part of the ESO Large Programme 168.A-0485 (PI: C. Cesarsky).
Data covering four ISAAC fields in J and Ks bands were also drawn from the ESO programmes 64.O-0643, 66.A-0572 and 68.A-0544 (PI: E.Giallongo),
which were part of the previous data releases.
<p>
This data release covers 172.4, 159.6, and 173.1 arcmin2 of the GOODS/CDF-S
region in J, H and Ks respectively. More than 50% of the images reach a 5-sigma depth
for point sources of at least 25.2 mag (J), 24.7 mag (H and Ks) in the AB system ("median depth").
<p>
This final GOODS/ISAAC data release accumulates observational data which have
been acquired in 12814 science integrations between October 1999 and January 2007
totaling 1.3 Msec integration time.
[Above adapted from reference website.]
<p>
<i> SkyView</i> uses the mosaic files provided in this delivery. The Version 1.5 mosaic
is used for the KS band. Provenance: Data downloaded from VLT archive. This is a service of NASA HEASARC.
Southern GOODS Field: VLT VIMOS Observations, R band
Short Name:
GOODS VIMOS R
Date:
07 Mar 2025
Publisher:
NASA/GSFC HEASARC
Description:
As part of the Great Observatories Origins Deep Survey (GOODS),
deep imaging in the Chandra Deep Field South (CDF-S) has been carried out,
using the VIMOS instrument mounted at the Melipal Unit Telescope of
the VLT at ESO's Cerro Paranal Observatory, Chile.
<p>
This data release contains the coadded images in U band from the ESO large programme
168.A-0485 (P.I. C. Cesarsky) which have been obtained in
service mode observations between August 2004 and fall 2006.
The 1-sigma depth for VIMOS U band in the area covered by the GOODS-ACS observations
is ~30 AB (within an aperture of 1" radius, ranging from 29.5 and 30.2 AB).
The PSF of the VIMOS U band mosaic is ~0.8" FWHM, but varies over the field.
<p>
Also included in this data release is a coadded image in R band obtained from
data retrieved from the ESO archive. Due to the different observing strategies
adopted in the programmes the resulting coverage of the GOODS-ACS
area is more complex than for the U band.
The depth of the VIMOS R band mosaic over the ACS area ranges from ~28 AB to 29 AB
(1-sigma, 1" aperture radius).
The PSF of the VIMOS R band mosaic is ~0".7 FWHM and varies over the field.
[Adapted from reference website.] Provenance: Data downloaded from VLT archive. This is a service of NASA HEASARC.
Space Telescope A901/902 Galaxy Evolution Survey (STAGES)
Short Name:
HST.STAGES
Date:
23 Jul 2020 19:41:16
Publisher:
Space Telescope Science Institute Archive
Description:
STAGES is a large area (0.5x0.5 degree) survey of the complex Abell 901(a,b)/902 multiple-cluster system at z=0.165. An 80-tile imaging mosaic in F606W was conducted in HST cycle 13 with the HST/ACS instrument.
The Space Telescope Imaging Spectrograph (STIS) was installed in HST on Feb. 14, 1997, replacing the GHRS spectrograph. STIS provides spectra and images at ultraviolet and visible wavelengths, probing the Universe from our solar system out to cosmological distances.
![the Fornax VST Survey is licensed under the `Creative Commons Attribution 4.0 License <http://creativecommons.org/licenses/by/4.0/>`_ .. image:: /static/img/ccby.png :alt: [CC-BY]](/registry-search/?f%5Brights_facet%5D%5B%5D=the+Fornax+VST+Survey+is+licensed+under+the+%60Creative+Commons+Attribution+4.0+License+%3Chttp%3A%2F%2Fcreativecommons.org%2Flicenses%2Fby%2F4.0%2F%3E%60_%0A%0A..+image%3A%3A+%2Fstatic%2Fimg%2Fccby.png%0A+++%3Aalt%3A+%5BCC-BY%5D%0A%0A&f%5Btype_facet%5D%5B%5D=Archive){kind=link}