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- ID:
- ivo://jvo/isas/darts/akari/AKARI-IRC_Spectrum_Pointed_SlitlessMIR_spectrum_1.0
- Title:
- AKARI/IRC MIR-S slit-less spectroscopic catalogue
- Short Name:
- AKARI_IRC_SPEC_V1
- Date:
- 07 Feb 2023 00:55:14
- Publisher:
- JVO
- Description:
- A catalogue of mid-infrared slit-less spectra (5.5-12.5 ?m) extracted from the AKARI/IRC MIR-S spectroscopic observation data. All 886 MIR-S spectroscopic data obtained in Phases 1&2 are analyzed, and 862 spectra of 604 individual sources that are little contaminated by nearby sources are catalogued. We also present a 9 ?m point source catalogue generated as a by-product. The point source catalogue contains 42,387 sources brighter than 0.3 mJy.
- ID:
- ivo://jvo/isas/darts/akari/AKARI-IRC_Spectrum_Pointed_DiffuseSkyPatch_1.0
- Title:
- AKARI/IRC NIR Low-resolution Spectral Catalogue of Diffuse Sky Patches
- Short Name:
- AKARI_IRC_SPEC_DSP
- Date:
- 07 Feb 2023 00:53:40
- Publisher:
- JVO
- Description:
- This catalog contains the 278 low-resolution (R~20) near-infrared (1.8-5.3 micron) spectra of diffuse sky covering a wide range of galactic and ecliptic latitudes with the Infrared Camera (IRC) onboard AKARI before the exhaustion of liquid-helium (from September 2006 to May 2007). Advanced reduction methods specialized for the slit spectroscopy of diffuse sky spectra are developed for constructing this spectral catalog.
- ID:
- ivo://jvo/isas/darts/akari/AKARI-IRC_Spectrum_Pointed_GALPN_1.0
- Title:
- AKARI/IRC NIR Spectral Atlas of Galactic Planetary Nebulae
- Short Name:
- AKARI_IRC_SPEC_GALPN
- Date:
- 07 Feb 2023 00:54:25
- Publisher:
- JVO
- Description:
- This catalog contains near-infrared (2.5--5.0 micron) low-resolution (R ~ 100) spectra of 72 Galactic Planetary Nebulae (PNe), obtained with the InfraRed Camera (IRC) onboard the AKARI satellite in the post-helium phase. The objects were treated as almost point sources for the IRC. Grism spectroscopy was carried out in the 1-arcmin window. The near-infrared spectra were obtained in a slit-less mode without any flux loss due to a slit. The spectra show emission features including hydrogen recombination lines, helium recombination lines, the 3.3--3.5 micron hydrocarbon features, [MgIV] at 4.49 micron, and [ArVI] at 4.53 micron. This catalog also contains the intensity and equivalent width of these emission features measured by spectral fitting. The source list (source.dat) summarizes observations. As ancillary data, the magnitudes in the V- and Ks-band, the extinction at V-band toward the objects, and the effective temperature collected from literature are listed in another table (misc.dat). The intensities and the equivalent widths of the emission features are tabulated in different tables (intens.dat and equivw.dat). Each object is identified by the PNG ID (PNG) or an observation ID (Obs-ID). One-dimensional near-infrared spectra are stored in a directory (spc/). Each spectrum is identified by the observation ID.
- ID:
- ivo://svo.cab/models/cond00
- Title:
- Allard, COND 2000
- Short Name:
- COND00
- Date:
- 04 Sep 2019 08:27:24
- Publisher:
- SVO CAB
- Description:
- The COND00 Model grid of theoretical spectra (Lyon group)
- ID:
- ivo://svo.cab/models/dusty00
- Title:
- Allard, DUSTY 2000
- Short Name:
- DUSTY00
- Date:
- 04 Sep 2019 08:28:21
- Publisher:
- SVO CAB
- Description:
- The DUSTY00 Model grid of theoretical spectra (Lyon group)
- ID:
- ivo://svo.cab/arches
- Title:
- ARCHES fully calibrated spectral energy distributions (SEDs)
- Short Name:
- ARCHES SED
- Date:
- 04 Sep 2019 00:05:08
- Publisher:
- ARCHES - Astronomical Resource Cross-matching for High Energy Studies.
- Description:
- This service provides access to the spectral energy distributions of the objects included in the enhanced 3XMM catalogue
- ID:
- ivo://fai.kz/spectra_agn_archive/q/ssa
- Title:
- Archive of AGN spectral observations
- Short Name:
- spectra_agn_archive SSAP
- Date:
- 04 May 2024 09:44:08
- Publisher:
- Fesenkov Astrophysical Institute
- Description:
- The archive of AGN spectral observations is obtained on AZT-8 telescope at the Fesenkov Astrophysical Institute (FAI), Almaty, Kazakhstan. It represents the result of observations for abot 25 years - from 1970 to 1995. All observations were carried out at AZT-8 (D = 700 mm, F[main] = 2800 mm, F[Cassegrain] = 11000 mm) with a high-power spectrograph. In 1967-68, on the basis of the image intensifier (https://doi.org/10.1080/1055679031000084795a) developed and assembled the spectrograph of the original design in the workshops of the FAI. To use the spectra, please, download raw .fit file of required object, date and exposure. The open 'Calibration frames' in Related links and then use them to calibrate object spectra frames. For more information about calibration process please visit https://github.com/ill-i/Spectra-Reduction.
- ID:
- ivo://svo.cab/models/atmo2020/ceq
- Title:
- ATMO 2020, CEQ
- Short Name:
- ATMO-CEQ
- Date:
- 27 Sep 2022 00:50:15
- Publisher:
- SVO CAB
- Description:
- A set of atmosphere models for cool T-Y brown dwarfs and giant exoplanets. Equilibrium chemistry. Valid temperature range: 200-2000K. Only for solar metallicity.
- ID:
- ivo://svo.cab/models/atmo2020/neq_strong
- Title:
- ATMO 2020, NEQ strong
- Short Name:
- ATMO-NEQs
- Date:
- 27 Sep 2022 13:17:57
- Publisher:
- SVO CAB
- Description:
- A set of atmosphere models for cool T-Y brown dwarfs and giant exoplanets. Non equilibrium chemistry (strong). Valid temperature range: 200-2000K. Only for solar metallicity.
- ID:
- ivo://svo.cab/models/atmo2020/neq_weak
- Title:
- ATMO 2020, NEQ weak
- Short Name:
- ATMO-NEQw
- Date:
- 27 Sep 2022 13:18:30
- Publisher:
- SVO CAB
- Description:
- A set of atmosphere models for cool T-Y brown dwarfs and giant exoplanets. Non equilibrium chemistry (weak). Valid temperature range: 200-2000K. Only for solar metallicity.
- ID:
- ivo://mast.stsci/ssap/befs
- Title:
- Berkeley Extreme and Far-UV Spectrometer
- Short Name:
- BEFS
- Date:
- 03 Feb 2021 15:45:57
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- The Berkeley Extreme and Far-UV Spectrometer (BEFS), flew on the Orbiting and Retrievable Far and Extreme Ultraviolet Spectrograph (ORFEUS)-SPAS I and II space shuttle missions in 1993 and 1996, returning high-resolution (/3000) FUV spectra (900-1200 Å) of 75 astrophysical objects from the first flight and more than 100 from the second. EUV spectra (400-900 Å) were obtained for a subset of these targets.
13. Be Stars Spectra
- ID:
- ivo://vopdc.obspm/lesia/BeStars/BeSS
- Title:
- Be Stars Spectra
- Short Name:
- BeSS
- Date:
- 10 Jan 2017
- Publisher:
- Paris Astronomical Data Centre - LESIA
- Description:
- The BeSS database assembles classical Be star spectra obtained by professional and amateur astronomers at any wavelength, epoch, and spectral resolution.
- ID:
- ivo://org.gavo.dc/onebigb/q/ssap
- Title:
- 1BIGB: First Brazil-ICRANet Gamma-Ray Blazar Catalogue
- Short Name:
- 1BIGB SSAP
- Date:
- 23 Mar 2022 13:13:03
- Publisher:
- The GAVO DC team
- Description:
- This catalog presents the 1-100 GeV spectral energy distribution (SED) for a population of 148 high-synchrotron-peaked blazars (HSPs) recently detected with Fermi-LAT as part of the First Brazil-ICRANet Gamma-ray Blazar catalogue (1BIGB). A series of two works describe details on the broadband analysis: :bibcode:`2017A&A...598A.134A`, and the calculation of the gamma-ray SEDs :bibcode:`2018MNRAS.480.2165A`. The 1BIGB sample was originally selected from an excess signal in the 0.3-500 GeV band The flux estimates presented here are derived considering PASS8 data, integrating over more than 9 years of Fermi-LAT observations. The full broadband fit between 0.3-500 GeV presented in paper 1 for all sources was reevaluated in paper 2, updating the power-law parameters with currently
15. Black Body
- ID:
- ivo://svo.cab/models/bbody
- Title:
- Black Body
- Short Name:
- Black Body
- Date:
- 04 Sep 2019 08:31:00
- Publisher:
- SVO CAB
- Description:
- Black Body flux. Teff from 10 to 200000 K
- ID:
- ivo://org.gavo.dc/bgds/l/ssa
- Title:
- Bochum Galactic Disk Survey (BGDS) light curves
- Short Name:
- BGDS TS SSAP
- Date:
- 09 Feb 2023 14:30:36
- Publisher:
- The GAVO DC team
- Description:
- This service exposes the light curves of stars produced by the Bochum Galactic Disk Survey; several million light curves are provided in the SDSS i and r bands. The lightcurves are published per-band and are also available through obscore.
17. BT-COND
- ID:
- ivo://svo.cab/models/bt-cond
- Title:
- BT-COND
- Short Name:
- BT-COND
- Date:
- 04 Sep 2019 08:31:00
- Publisher:
- SVO CAB
- Description:
- The BT-COND Model grid of theoretical spectra. Brown dwarfs/extrasolar planets atmosphere models without irradiation and no dust opacity (no dust settling) but updated abundances. Wavelengths have been converted to air wavelengths.
18. BT-DUSTY
- ID:
- ivo://svo.cab/models/bt-dusty
- Title:
- BT-DUSTY
- Short Name:
- BT-DUSTY
- Date:
- 04 Sep 2019 08:31:00
- Publisher:
- SVO CAB
- Description:
- The BT-DUSTY Model grid of theoretical spectra. Brown dwarfs/extrasolar planets atmosphere models without irradiation but including dust opacity (fully efficient dust settling) and updated abundances. Wavelengths have been converted to air wavelengths.
- ID:
- ivo://svo.cab/models/bt-nextgen-agss2009
- Title:
- BT-NextGen (AGSS2009)
- Short Name:
- BT-NextGen-AGSS
- Date:
- 04 Sep 2019 08:31:00
- Publisher:
- SVO CAB
- Description:
- The NextGen Model grid of theoretical spectra; Gas phase only, valid for Teff > 2700 K. Updated opacities. Wavelengths have been converted to air wavelengths.
- ID:
- ivo://svo.cab/models/bt-nextgen-gns93
- Title:
- BT-NextGen (GNS93)
- Short Name:
- BT-NextGen-GNS93
- Date:
- 04 Sep 2019 08:31:00
- Publisher:
- SVO CAB
- Description:
- The NextGen Model grid of theoretical spectra; Gas phase only, valid for Teff > 2700 K. Updated opacities. Wavelengths have been converted to air wavelengths.
21. BT-Settl
- ID:
- ivo://svo.cab/models/bt-settl
- Title:
- BT-Settl
- Short Name:
- BT-Settl
- Date:
- 04 Sep 2019 08:31:00
- Publisher:
- SVO CAB
- Description:
- The BT-Settl Model grid of theoretical spectra; With a cloud model, valid across the entire parameter range. Wavelengths have been converted to air wavelengths.
- ID:
- ivo://svo.cab/models/bt-settl-agss2009
- Title:
- BT-Settl (AGSS2009)
- Short Name:
- BT-Settl-AGSS
- Date:
- 04 Sep 2019 08:31:00
- Publisher:
- SVO CAB
- Description:
- The BT-Settl Model grid of theoretical spectra; With a cloud model, valid across the entire parameter range. Using AGSS2009 abundances. Wavelengths have been converted to air wavelengths.
- ID:
- ivo://svo.cab/models/bt-settl-cifist
- Title:
- BT-Settl (CIFIST)
- Short Name:
- BT-Settl-CIFIST
- Date:
- 04 Sep 2019 08:31:00
- Publisher:
- SVO CAB
- Description:
- The BT-Settl Model grid of theoretical spectra. With a cloud model, valid across the entire parameter range and using the Caffau et al. (2011) solar abundances. Wavelengths have been converted to air wavelengths.
24. BT-Settl (GNS93)
- ID:
- ivo://svo.cab/models/bt-settl-gns93
- Title:
- BT-Settl (GNS93)
- Short Name:
- BT-Settl-GNS93
- Date:
- 27 Sep 2022 13:34:35
- Publisher:
- SVO CAB
- Description:
- The BT-Settl Model grid of theoretical spectra; With a cloud model, valid across the entire parameter range. Using GNS93 abundances. Wavelengths have been converted to air wavelengths.
25. CALIFA DR3
- ID:
- ivo://org.gavo.dc/califa/q3/s
- Title:
- CALIFA DR3
- Short Name:
- califa ssa
- Date:
- 20 Apr 2023 00:19:47
- Publisher:
- The GAVO DC team
- Description:
- Split spectra from the CALIFA DR3 cubes. This service serves one spectrum each per pixel in each cube where there is at least one valid spaxel. Where both V500 and COMB data is available, COMB spectra are served. WARNING: The individual spectra are not independent. Also, error estimates over wide spectral ranges based on the error estimates served here are unreliable.
- ID:
- ivo://svo.cab/CARMENES_Reiners2018
- Title:
- CARMENES_Reiners2018
- Short Name:
- CARMENES_Reiners
- Date:
- 13 Apr 2018 00:40:19
- Publisher:
- SVO CAB
- Description:
- CARMENES_Reiners2018
- ID:
- ivo://svo.cab/cat/catlib
- Title:
- CaT library. Empirical Calibration of the Near-IR Ca II Triplet
- Short Name:
- CaT library
- Date:
- 03 Jun 2020 15:33:59
- Publisher:
- SVO/CAB
- Description:
- CaT library, Empirical Calibration of the Near-IR Ca II Triplet
- ID:
- ivo://asu.cas.cz/ccd700/q/ssa
- Title:
- CCD700 Ondrejov Spectra
- Short Name:
- CCD700 SSAP
- Date:
- 30 Nov 2017 10:39:24
- Publisher:
- Stellar Department of Astronomical Institute of the Academy of Sciences of the Czech Republic
- Description:
- CCD700 SSAP service
- ID:
- ivo://cfa.tdc/hectospec/hectospec_public.ssap.q/ssa
- Title:
- CfA Hectospec Spectra
- Short Name:
- CfA Hectospec
- Date:
- 26 Jun 2018 14:04:17
- Publisher:
- Smithsonian Astrophysical Observatory Telescope Data Center
- Description:
- Optical spectra collected with the multi-fiber Hectospec Spectrograph at the MMT 6.5m telescope
- ID:
- ivo://nasa.heasarc/chanmaster
- Title:
- Chandra Observations
- Short Name:
- Chandra
- Date:
- 03 May 2024
- Publisher:
- NASA/GSFC HEASARC
- Description:
- This database table contains all of the observations made by the Chandra X-Ray Observatory (CXO, formerly known as the Advanced X-ray Astrophysics Facility or AXAF) as part of the Performance Verification and Calibration (PVC) phase and also contains all of the subsequent Cycles' Guaranteed Time Observers (GTO) and General Observer (GO) targets, and any Director's Discretionary Time (DDT) targets that have been observed. It also includes scheduled and as-yet-not-scheduled targets. The HEASARC updates this database table on a twice-weekly basis by querying the database table at the Chandra X-Ray Center (CXC) website, as discussed in the Provenance section. For observations whose status is 'archived', data products can be retrieved from the HEASARC's mirror of the CXC's Chandra Data Archive (CDA). The CXC should be acknowledged as the source of Chandra data. The PVC phase was during the first few months of the CXO mission; some of the calibration observations that are for monitoring purposes will be performed in later mission cycles. All calibration data (entries with Type = CAL in this database) are placed immediately into the CXO public data archive at the Chandra X-Ray Observatory Center (CXC); please see the Web page at <a href="http://asc.harvard.edu/">http://asc.harvard.edu/</a> for more information on the CXC data archive). GTO observations during Cycle 1 or any subsequent Cycle will probably occupy 100% of months 3-4, 30% of months 5-22, and 15% of the available time for the remainder of the mission. Guaranteed Time Observers will have the same proprietary data rights as General Observers (i.e., their data will be placed in the public CXC archive 12 months after they have received the data in usable form). For detailed information on the Chandra Observatory and datasets see: <pre> <a href="http://cxc.harvard.edu/">http://cxc.harvard.edu/</a> for general Chandra information <a href="http://cxc.harvard.edu/cda/">http://cxc.harvard.edu/cda/</a> for the Chandra Data Archive <a href="http://cxc.harvard.edu/cal/">http://cxc.harvard.edu/cal/</a> for calibration information <a href="http://cxc.harvard.edu/caldb/">http://cxc.harvard.edu/caldb/</a> for the calibration database <a href="http://cxc.harvard.edu/ciao/">http://cxc.harvard.edu/ciao/</a> for data analysis <a href="http://cxc.harvard.edu/ciao/download/">http://cxc.harvard.edu/ciao/download/</a> for analysis software <a href="http://cxc.harvard.edu/ciao/threads/">http://cxc.harvard.edu/ciao/threads/</a> for analysis threads <a href="http://cda.harvard.edu/chaser/">http://cda.harvard.edu/chaser/</a> for WebChaSeR </pre> The HEASARC updates this database table on a twice-weekly basis based on information obtained from the Chandra Data Archive at the CXC website. This is a service provided by NASA HEASARC .
- ID:
- ivo://svo.cab/models/coelho_highres
- Title:
- Coelho 2014 (highres)
- Short Name:
- Coelho (highres)
- Date:
- 04 Sep 2019 08:31:00
- Publisher:
- SVO CAB
- Description:
- High resolution theoretical stellar spectra covering 250 to 900nm, fully described in Coelho (2014).
- ID:
- ivo://svo.cab/models/coelho_sed
- Title:
- Coelho 2014 (SEDs)
- Short Name:
- Coelho (SEDs)
- Date:
- 04 Sep 2019 08:31:00
- Publisher:
- SVO CAB
- Description:
- Low resolution theoretical fluxes covering 130nm to 100micron, fully described in Coelho (2014).
- ID:
- ivo://org.gavo.dc/k2c9vst/q/ssa
- Title:
- Coordinated microlensing survey observations with Kepler K2/C9 using VST
- Short Name:
- k2c9vst ssap
- Date:
- 23 Mar 2022 13:13:09
- Publisher:
- The GAVO DC team
- Description:
- The Kepler satellite has observed the Galactic center in a campaign lasting from April until the end of June 2016 (K2/C9). The main objective of the 99 hours for the microlensing program 097.C-0261(A) using the ESO VLT Survey Telescope (VST) was to monitor the superstamp (i.e., the actually downloaded region of K2/C9) in service mode for improving the event coverage and securing some color-information. Due to weather conditions, the majority of images were taken in the red band. These are part of the present release. The exact pointing strategy was adjusted to cover the superstamp with 6 pointings and to contain as many microlensing events from earlier seasons as possible. In addition, a two-point dither was requested to reduce the impact of bad pixels and detector gaps. Consequently, some events were getting more coverage and have been observed with different CCDs. The large footprint of roughly 1 square degree and the complementary weather conditions at Cerro Paranal have lead to the coverage of 147 events (this resource's events table), but ~60 of those were already at baseline.
- ID:
- ivo://au.csiro/casda/SSA
- Title:
- CSIRO ASKAP Science Data Archive Spectrum Access Service
- Short Name:
- CSIRO ASKAP SSA
- Date:
- 29 Apr 2022 07:59:11
- Publisher:
- CSIRO
- Description:
- Simple Spectral Access service for querying spectra from ASKAP radio astronomy observations
35. Data Central SSA
- ID:
- ivo://purx/datacentral-ssa
- Title:
- Data Central SSA
- Short Name:
- DCSSA
- Date:
- 08 Jun 2021 09:24:53
- Publisher:
- Data Central
- Description:
- Spectra from surveys hosted by Data Central. Most spectra were taken with the multi-object spectroscopy facilities 2dF (Anglo-Australian Telescope) and 6dF (UK Schmidt Telescope).
- ID:
- ivo://wfau.roe.ac.uk/6dF-ssap
- Title:
- 6dF DR3 Simple Spectra Access
- Short Name:
- 6dF Spectra
- Date:
- 18 Sep 2013 16:43:53
- Publisher:
- WFAU, Institute for Astronomy, University of Edinburgh
- Description:
- The 6dF Galaxy Survey (6dFGS) aims to measure the redshifts of around 150 000 galaxies, and the peculiar velocities of a 15 000-member subsample, over almost the entire southern sky. The table called Spectra contains the redshifts and qualities of all the observations. When complete, it will be the largest redshift survey of the nearby Universe, reaching out to about z ~ 0.15, and more than an order of magnitude larger than any peculiar velocity survey to date. The targets are all galaxies brighter than K tot = 12.75 in the 2MASS Extended Source Catalog (XSC), supplemented by 2MASS and SuperCOSMOS galaxies that complete the sample to limits of (H, J , r F, bJ) = (13.05, 13.75, 15.6, 16.75). This is the Data Release 3 version.
- ID:
- ivo://org.gavo.dc/dfbsspec/q/getssa
- Title:
- Digitized First Byurakan Survey (DFBS) Spectra Query Service
- Short Name:
- DFBS SSAP
- Date:
- 06 Feb 2024 09:11:09
- Publisher:
- The GAVO DC team
- Description:
- The First Byurakan Survey (FBS) is the largest and the first systematic objective prism survey of the extragalactic sky. It covers 17,000 sq.deg. in the Northern sky together with a high galactic latitudes region in the Southern sky. The FBS has been carried out by B.E. Markarian, V.A. Lipovetski and J.A. Stepanian in 1965-1980 with the Byurakan Observatory 102/132/213 cm (40"/52"/84") Schmidt telescope using 1.5 deg. prism. Each FBS plate contains low-dispersion spectra of some 15,000-20,000 objects; the whole survey consists of about 20,000,000 objects.
- ID:
- ivo://byu.arvo/dfbsspec/q/getssa
- Title:
- Digitized First Byurakan Survey (DFBS) Spectra Query Service
- Short Name:
- DFBS SSAP
- Date:
- 24 Aug 2020 16:45:07
- Publisher:
- The staff at the ArVO Data Center
- Description:
- The First Byurakan Survey (FBS) is the largest and the first systematic objective prism survey of the extragalactic sky. It covers 17,000 sq.deg. in the Northern sky together with a high galactic latitudes region in the Southern sky. The FBS has been carried out by B.E. Markarian, V.A. Lipovetski and J.A. Stepanian in 1965-1980 with the Byurakan Observatory 102/132/213 cm (40"/52"/84") Schmidt telescope using 1.5 deg. prism. Each FBS plate contains low-dispersion spectra of some 15,000-20,000 objects; the whole survey consists of about 20,000,000 objects.
39. DK-154 objects
- ID:
- ivo://asu.cas.cz/extract_apr18/q/ssa
- Title:
- DK-154 objects
- Short Name:
- DK-154 LCs
- Date:
- 18 Apr 2018 11:50:00
- Publisher:
- Stellar Department of Astronomical Institute of the Academy of Sciences of the Czech Republic
- Description:
- DK-154 SSAP interpreted lightcurves
40. DK-154 objects
- ID:
- ivo://asu.cas.cz/extract_jan18/q/ssa
- Title:
- DK-154 objects
- Short Name:
- DK-154 LCs
- Date:
- 08 Jan 2018 15:30:12
- Publisher:
- Stellar Department of Astronomical Institute of the Academy of Sciences of the Czech Republic
- Description:
- DK-154 SSAP interpreted lightcurves
41. DK-154 objects
- ID:
- ivo://asu.cas.cz/extract_dec17/q/ssa
- Title:
- DK-154 objects
- Short Name:
- DK-154 LCs
- Date:
- 08 Jan 2018 15:30:12
- Publisher:
- Stellar Department of Astronomical Institute of the Academy of Sciences of the Czech Republic
- Description:
- DK-154 SSAP interpreted lightcurves
42. DK-154 objects
- ID:
- ivo://asu.cas.cz/extract_jan16/q/ssa
- Title:
- DK-154 objects
- Short Name:
- DK-154 LC
- Date:
- 30 Nov 2017 09:39:26
- Publisher:
- Stellar Department of Astronomical Institute of the Academy of Sciences of the Czech Republic
- Description:
- SSAP interpreted lightcurves
43. DK-154 objects
- ID:
- ivo://asu.cas.cz/extract_jul16/q/ssa
- Title:
- DK-154 objects
- Short Name:
- DK-154 LCs
- Date:
- 19 May 2017 01:42:07
- Publisher:
- Stellar Department of Astronomical Institute of the Academy of Sciences of the Czech Republic
- Description:
- DK-154 SSAP interpreted lightcurves
- ID:
- ivo://svo.cab/models/drift
- Title:
- DRIFT-PHOENIX models
- Short Name:
- DRIFT-PHOENIX
- Date:
- 04 Sep 2019 08:28:05
- Publisher:
- SVO CAB
- Description:
- Drift-Phoenix is a computer code that simulates the structure of an atmosphere including the formation of clouds. The code is part of the Phoenix-code family. Drift describes the formation of mineral clouds and allows to predict cloud details, like the size of the cloud particles and their composition.
- ID:
- ivo://lam.cesam.aspic/el_cosmos_dr1/q/ssa
- Title:
- EL COSMOS DR1 spectra
- Short Name:
- ELCOSMOS1 SSAP
- Date:
- 28 Apr 2022 21:55:18
- Publisher:
- The CeSAM VO team
- Description:
- Synthetic spectra of COSMOS2015 sources
46. ELODIE archive
- ID:
- ivo://obs-hp.fr/elodie/ssa
- Title:
- ELODIE archive
- Short Name:
- ELODIE
- Date:
- 15 Apr 2008 20:18:49
- Publisher:
- Observatoire de Haute-Provence
- Description:
- The science archive of the ELODIE spectrograph contains all the spectra collected by the instrument between 1993 and 2006 (total life time of the instrument). ELODIE is an echelle spectrograph providing a resolution R=42000 in the spectral range 390-680 nm. The web interface of the archive distribute a variety of products, and the SSA service gives the reconnected 1D spectra in instrumental flux (not physical). This service is given for test: The spectra cannot be viewved with VOSpec because they are not flux-calibrated.
- ID:
- ivo://xcatdb/4xmm/epicssa
- Title:
- Epic Spectra SSAP of the SSC Interface for the 4XMM Catalogue
- Short Name:
- 4XMM-SSA
- Date:
- 07 Apr 2021 13:40:35
- Publisher:
- Observatory of Strasbourg, SSC Team
- Description:
- The 4XMM-DR10 catalogue contains source detections drawn from 11647 XMM-Newton EPIC observations, covering an energy interval from 0.2 keV to 12 keV. These observations were made between 2000 February 3 and 2019 December 14 and all datasets were publicly available by 2020 December 10, but not all public observations are included in this catalogue . This version of the XMM-Newton EPIC Serendipitous Source Catalogue, 4XMM-DR10 includes 748670 clean detections which relate to 575158 unique sources from 11647 observations that were public by 2020 December 10. 3XMM-DR7 covers a total sky area of ~1192 square degrees if overlaps are taken into account, where some regions of the sky have been pointed as many as 50 times. The median flux in the total photon energy band (0.2 - 12 keV) of the catalogue detections is ~ 8.3 × 10-14 erg cm-2 s-1; in the soft energy band (0.2 - 2 keV) the median flux is ~ 5.3 × 10-15, and in the hard band (2 - 12 keV) it is ~ 1.2 × 10-14. About 23% of the sources have total fluxes below 1 × 10-14 erg cm-2 s-1.
- ID:
- ivo://eso.org/ssap
- Title:
- ESO 1D reduced spectra
- Short Name:
- ESO SSAP
- Date:
- 29 Mar 2022 09:14:37
- Publisher:
- European Southern Observatory
- Description:
- The ESO Simple Spectral Access service provides access to the 1D reduced spectra generated either by the principal investigators of ESO observations, or by an unattended ESO processing-pipeline that makes use of certified master calibrations. The spectra are FITS files adhering to the ESO Science Data Product standard, based on the Virtual Observatory Spectral Data Model standard (v1.0 for some spectra, and v2.0 for some others, use the VOCLASS FITS keyword to discern the two).
- ID:
- ivo://esavo/hst/ssap
- Title:
- European HST Archive SSAP service
- Short Name:
- Hubble SSAP ESA
- Date:
- 07 Feb 2024 10:19:58
- Publisher:
- European Space Agency
- Description:
- Science spectra from the HST collection hosted at ESAC/ESA. All public HST observations in calibrated and science-ready form are synchronised with the MAST services for HST reprocessed public data and corresponding metadata. The European HST archive interface can be accessed at https://hst.esac.esa.int/ehst
- ID:
- ivo://mast.stsci/ssap/euve
- Title:
- Extreme Ultraviolet Explorer Merged Spectra
- Short Name:
- EUVE
- Date:
- 22 Jul 2020 21:49:27
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- The Extreme Ultraviolet Explorer (EUVE) was a NASA-funded satellite launched in June 1992 which obtained extreme ultraviolet spectra (70 - 760 Angstroms) of over 350 unique astronomical targets. The science payload, was designed and built at the Space Sciences Laboratory at the University of California, Berkeley, under the direction of Dr. Roger F. Malina. The program ended in January, 2001. These particular spectra were extracted by Damian Christian, formerly of the EUVE project, and reformatted by MAST staff.
- ID:
- ivo://mast.stsci/ssap/fuse
- Title:
- Far Ultraviolet Spectroscopic Explorer
- Short Name:
- FUSE
- Date:
- 22 Jul 2020 21:53:56
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- The Far Ultraviolet Spectroscopic Explorer (FUSE), launched on June 24, 1999, covers the 905-1187 Å spectral region and obtains high resolution spectra of hot and cool stars, AGNs, supernova remnants, planetary nebulae, solar system objects as well as perform detailed studies of the interstellar medium. This service provides access to the FUSE spectra reprocessed using CalFUSE 3.2 and reformatted to be VO-compatible.
- ID:
- ivo://org.gavo.dc/feros/q/ssa
- Title:
- FEROS Public Spectra
- Short Name:
- FEROS SSAP
- Date:
- 20 Apr 2023 00:19:48
- Publisher:
- The GAVO DC team
- Description:
- Spectra from FEROS spectrograph at La Silla's 1.5m telescope as obtained during commissioning and guaranteed time.
- ID:
- ivo://org.gavo.dc/flashheros/q/echssa
- Title:
- Flash/Heros Split-Order SSAP Service
- Short Name:
- F/H Orders SSAP
- Date:
- 31 Mar 2023 10:58:42
- Publisher:
- The GAVO DC team
- Description:
- Spectra from the Flash and Heros Echelle spectrographs developed at Landessternwarte Heidelberg and mounted at La Silla and various other observatories. The data mostly contains spectra of OB stars. Heros was the name of the instrument after Flash got a second channel in 1995.
54. Flash/Heros SSAP
- ID:
- ivo://org.gavo.dc/flashheros/q/ssa
- Title:
- Flash/Heros SSAP
- Short Name:
- Flash/Heros SSAP
- Date:
- 31 Mar 2023 10:58:42
- Publisher:
- The GAVO DC team
- Description:
- Spectra from the Flash and Heros Echelle spectrographs developed at Landessternwarte Heidelberg and mounted at La Silla and various other observatories. The data mostly contains spectra of OB stars. Heros was the name of the instrument after Flash got a second channel in 1995.
- ID:
- ivo://org.gavo.dc/gaia/q2/ssa
- Title:
- Gaia DR2 light curves SSA
- Short Name:
- GDR2 TS SSAP
- Date:
- 23 Mar 2022 13:13:05
- Publisher:
- The GAVO DC team
- Description:
- This service exposes about 0.5 million light curves of stars classified as variable by the Gaia analysis system through the VO SSAP protocol. The lightcurves are published per-band and are also available through obscore.
- ID:
- ivo://org.gavo.dc/gaia/s3/ssa
- Title:
- Gaia DR3 MC sampled XP spectra SSA
- Short Name:
- gdr3spec SSAP
- Date:
- 12 Sep 2023 14:56:39
- Publisher:
- The GAVO DC team
- Description:
- This is a re-publication the Gaia DR3 RP/BP spectra in the IVOA Spectral Data Model. It presents the continous spectra in sampled form, using a Monte Carlo scheme to decorrelate errors, elaborated in this resource's reference URL. The underlying tables are also available for querying through TAP, which opens some powerful methods for mass-analysing the data.
- ID:
- ivo://lam.cesam.aspic/gama_dr3/q/ssa
- Title:
- GAMA DR3 - Simple Spectrum Access
- Short Name:
- GAMA3 SSAP
- Date:
- 20 May 2021 06:32:29
- Publisher:
- The CeSAM VO team
- Description:
- Spectra from the third data release (DR3) of GAMA.
58. Goyal (local)
- ID:
- ivo://svo.cab/models/goyal_local
- Title:
- Goyal (local)
- Short Name:
- Goyal_local
- Date:
- 27 Sep 2022 14:11:28
- Publisher:
- SVO CAB
- Description:
- Fully scalable forward model grid of exoplanet transmission spectra. Considering local condensation only.
59. Goyal (rainout)
- ID:
- ivo://svo.cab/models/goyal_rainout
- Title:
- Goyal (rainout)
- Short Name:
- Goyal_rainout
- Date:
- 27 Sep 2022 14:11:56
- Publisher:
- SVO CAB
- Description:
- Fully scalable forward model grid of exoplanet transmission spectra. Considering global condensation and removal of species from the atmospheric column (rainout).
- ID:
- ivo://svo.cab/models/grams_cgrid
- Title:
- GRAMS, C-rich grid
- Short Name:
- GRAMS-Crich
- Date:
- 04 Sep 2019 08:31:00
- Publisher:
- SVO CAB
- Description:
- GRAMS (Grid of Red supergiant and Asymptotic giant ModelS) is a grid of radiative transfer (RT) models for dust shells around red supergiant (RSG) and asymptotic giant branch (AGB) stars. This is the model grid for Carbon-rich stars
- ID:
- ivo://svo.cab/models/grams_ogrid
- Title:
- GRAMS, O-rich original grid
- Short Name:
- GRAMS-Orich
- Date:
- 04 Sep 2019 08:31:00
- Publisher:
- SVO CAB
- Description:
- GRAMS (Grid of Red supergiant and Asymptotic giant ModelS) is a grid of radiative transfer (RT) models for dust shells around red supergiant (RSG) and asymptotic giant branch (AGB) stars. This is the model grid for Oxygen-rich stars
- ID:
- ivo://nrao/GBTSA
- Title:
- Green Bank Spectral Archive
- Short Name:
- NRAO.GBTSA
- Date:
- 19 Jun 2019 18:46:24
- Publisher:
- National Radio Astronomy Observatory
- Description:
- High frequency water maser and HI spectra are available through this web service. The water maser phenomena are found in active galactic nuclei (AGN) and have been surveyed with the NRAO Green Bank Telescope. HI spectra are measured mostly from galaxies in the local Universe.
- ID:
- ivo://esavo/hsa/ssap
- Title:
- Herschel ESA Archive SSAP
- Short Name:
- Herschel SSAP
- Date:
- 07 Feb 2024 10:19:03
- Publisher:
- ESA
- Description:
- Herschel standard data products were systematically generated by the Herschel Data Processing pipeline and made available to the users through the Herschel Science Archive (HSA) typically 1-2 days after an observation had been executed. Today all Herschel science data (~23,400 hours of observing, ~37,000 AORs) are publicly available, and there are science calibration observations (~2600 hours of observing, ~6600 AORs) available too. In addition "User Provided Data Products" (UPDPs) are also being served by the HSA.
64. hess_ssa
- ID:
- ivo://padc.obspm.astro/hess_ssa/q/web
- Title:
- hess_ssa
- Short Name:
- HESS spectra Web
- Date:
- 02 Apr 2022 00:38:58
- Publisher:
- Paris Astronomical Data Centre
- Description:
- The release consists of event lists and instrument response functions for observations of various well-known gamma-ray sources (the Crab nebula, PKS 2155-304, MSH 15-52, RX J1713.7-3946) as well as observations of empty fields for background modeling.
- ID:
- ivo://vopdc.obspm/gepi/h1g
- Title:
- HI Extragalactic Database
- Short Name:
- HIG
- Date:
- 10 Jan 2017
- Publisher:
- Paris Astronomical Data Centre - GEPI
- Description:
- HI Extragalactic database is a collection of calibrated 21cm hydrogen line profiles for several thousands galaxies.
- ID:
- ivo://vopdc.obspm/luth/hess
- Title:
- High Energy Stereoscopic System
- Short Name:
- H.E.S.S.
- Date:
- 10 Jan 2017
- Publisher:
- Paris Astronomical Data Centre - LUTH
- Description:
- H.E.S.S. is a system of Imaging Atmospheric Cherenkov Telescopes that investigates cosmic gamma rays in the 100 GeV to 100 TeV energy range. The name H.E.S.S. stands for High Energy Stereoscopic System.
- ID:
- ivo://ar.nova/fcaglp/q/ssa
- Title:
- High-resolution optical spectra of HD165052 (Ferrero+, 2013) at NOVA
- Short Name:
- NOVA HD 165052
- Date:
- 14 Aug 2014 17:03:24
- Publisher:
- Nova
- Description:
- This is a set of high-resolution high-S/N optical spectra of the massive binary star HD 165 052 (O7Vz + O7.5Vz) taken between 2008 April and 2011 May with echelle spectrographs at CASLEO (mainly), LCO and ESO. Each one covers the spectral range 3700-6000 A with a resolution varying between ~13000 and ~45000 @ 5000A according to the instrument. Originally, the spectra were secured for radial velocity measurements. More details about observations, instrument configurations and reduction process can be found in documentation section.
- ID:
- ivo://nasa.heasarc/hitomaster
- Title:
- Hitomi Master Catalog
- Short Name:
- HITOMASTER
- Date:
- 03 May 2024
- Publisher:
- NASA/GSFC HEASARC
- Description:
- This table records high-level information for the observations obtained with Hitomi and provides access to the data archive. The Hitomi mission was launched on a JAXA H-IIA into low Earth orbit on February 17, 2016, at 5:45 pm JPS from Tanegashima Space Center. Hitomi was equipped with four different instruments that together cover a wide energy range 0.3-600 keV. The Soft X-ray Spectrometer (SXS), which combined a lightweight Soft X-ray Telescope paired with a X-ray Calorimeter Spectrometer, provided non-dispersive 7-eV resolution in the 0.3-10 keV bandpass with a field of view of about 3 arcminutes. The Soft X-ray Imager (SXI) expanded the field of view with a new generation CCD camera in the energy range of 0.5-12 keV at the focus of the second lightweights Soft X-ray Telescope; the Hard X-ray Imager (HXI, two units) performed sensitive imaging spectroscopy in the 5-80 keV band; the non-imaging Soft Gamma-ray Detector (SGD, two units) extended Hitomi's energy band to 600 keV. On March 27, 2016, JAXA lost contact with the satellite and, on April 28, announced the cessation of the efforts to restore mission operations. At that time Hitomi was in check-out phase and had started the calibration observations. Data were collected from six celestial objects (Perseus, N132D, IGR_J16318-4848, RXJ1856.5-3754, G21.5-0.9, and Crab) as well as black sky for a total of about one month of data. The data from these observations were divided into intervals of one day if the observation of a specific pointing was longer that one day. A sequence number was assigned to each observing day and within data from all instruments are included. The day division was mainly to limit the data size within a sequence number. There are in total 42 sequences, and each record in this database table is dedicated to a single sequence. The early observations do not contain data from all instruments and in cases the object was not always placed at the aim point. This database contains parameters to indicate which instrument was on and if the celestial source was in the field of view. The SXS was the first instrument to turn on and therefore all observations contain SXS data, although the thermal equilibrium was reached after March 4 2016. The second instrument was the SXI followed by the HXIs and, finally, the two SGDs. This database table was generated at the Hitomi Science Data Center processing site (Angelini, L., Terada, Y, et al., 2016, SPIE 9905E, 14) with additions to indicate which instrument was on and if the source was in the FOV. It was ingested into the HEASARC database in June 2017. This is a service provided by NASA HEASARC .
- ID:
- ivo://mast.stsci/ssap/hut
- Title:
- Hopkins Ultraviolet Telescope
- Short Name:
- HUT
- Date:
- 22 Jul 2020 21:48:21
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- The Hopkins Ultraviolet Telescope (HUT) was one of three ultraviolet instruments of the ASTRO-1 mission flown on the space shuttle Columbia during 2-10 December 1990. 106 spectrophotometric observations of 77 targets were obtained in the far-UV (i.e., 912-1850 Ã…) at a resolution of ~3 Ã…. A few sources were observed in the 415-912 Ã… region with a 1.5 Ã… resolution. The same three instruments were later flown on the space shuttle Endeavour from 3-17 March 1995 as part of the ASTRO-2 mission. During the longer ASTRO-2 mission, 385 observations of 265 targets were obtained.
- ID:
- ivo://mast.stsci/ssap/hst/stis
- Title:
- HST Space Telescope Imaging Spectrograph
- Short Name:
- HST STIS Spectra
- Date:
- 22 Jul 2020 21:58:09
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- MAST-produced spectral container files for STIS spectra. STIS spectra range from 1150 to 10,300 at low to medium spectral resolution, high spatial resolution echelle spectroscopy in the ultraviolet. STIS began operation in 1997. (Note the included echelle spectra are technically not yet supported by the SSAP.)
- ID:
- ivo://mast.stsci/ssap/hst/fos
- Title:
- Hubble Space Telescope Faint Object Spectrograph
- Short Name:
- HST.FOS Spectra
- Date:
- 22 Jul 2020 21:50:21
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- Spectra from the HST FOS instrument (processed by ESO and CADC) in the 1,150 - 8,500 Å range, resolution ~ 250 and 1,300, V_max ~ 20, 1990 - 1997. Links point to VO-compatible FITS files created by MAST staff.
- ID:
- ivo://mast.stsci/ssap/hst/ghrs
- Title:
- Hubble Space Telescope Goddard High Resolution Spectrograph
- Short Name:
- HST.GHRS Spectra
- Date:
- 22 Jul 2020 21:54:42
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- Spectra from the HST GHRS instrument (processed by ESO and CADC) in the 1,100 - 3,300 Å range, resolution ~ 2,000, 25,000, and 80,000 (echelle), V_max ~ 18, 16, and 12 respectively, 1990 - 1997. Links point to VO-compatible FITS files created by MAST staff.
- ID:
- ivo://mast.stsci/ssap/hst
- Title:
- Hubble Space Telescope Spectra
- Short Name:
- HST Spectra
- Date:
- 22 Jul 2020 21:49:04
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- Spectra from the following HST instruments are available: GHRS (processed by CADC), FOS (processed by ECF), and STIS (1st order). Separate SSAP services are registered for each instrument. VO-compatible FITS files were created by MAST staff.
- ID:
- ivo://svo.cab/models/husfeld
- Title:
- Husfeld et al models for non-LTE Helium-rich stars
- Short Name:
- Husfeld
- Date:
- 04 Sep 2019 08:28:51
- Publisher:
- SVO CAB
- Description:
- Husfeld et al models for non-LTE Helium-rich stars
- ID:
- ivo://obs-lyon.fr/hfa/ssa
- Title:
- HyperLeda FITS Archive Simple Spectrum Data Access(HFA SSA)
- Short Name:
- HFA
- Date:
- 15 Apr 2008 20:18:49
- Publisher:
- CRAL-Observatoire de Lyon
- Description:
- A compilation of 1D reference spectra of stars and galaxies. Spectra from several archives and libraries have been collected, re-documented and re-formatted. The spectral resolution is between R=100 and 250000. Some spectra give the physical flux, either or not corrected for the Galactic extinction, and some others are normalized to the pseudo-continuum. Some are given in physical units, and some are momalized to some particular wavelengths (often 5500 A).
- ID:
- ivo://iacvo/iacob
- Title:
- IACOB Spectroscopic Database
- Short Name:
- iacob
- Date:
- 05 Feb 2024 17:22:56
- Publisher:
- Instituto de Astrofisica de Canarias (IAC) - Sergio Simon
- Description:
- OB-stars multi-epoch optical spectra from FIES@NOT and Hermes@Mecator at ORM/La Palma
- ID:
- ivo://svo.cab/ines
- Title:
- INES: The IUE Newly Extracted Spectra
- Short Name:
- INES ARCHIVE
- Date:
- 04 Sep 2019 08:25:20
- Publisher:
- SVO
- Description:
- IUE (International Ultraviolet Explorer) performed UV spectrophotometry at resolutions of 0.2 and 6 Angstroms from 1150 to 3350 Angstroms, acquiring more than 104000 spectra of some 9600 objects.
- ID:
- ivo://esavo/new-iso/ssap
- Title:
- Infrared Space Observatory (ISO) SSAP
- Short Name:
- ISO SSAP
- Date:
- 07 Feb 2024 10:20:50
- Publisher:
- European Space Agency
- Description:
- The Infrared Space Observatory (ISO) was the world's first true orbiting infrared observatory. Equipped with four highly-sophisticated and versatile scientific instruments, it was launched by Ariane in November 1995 and provided astronomers world-wide with a facility of unprecedented sensitivity and capabilities for a detailed exploration of the Universe at infrared wavelengths. The two spectrometers (SWS and LWS), a camera (ISOCAM) and an imaging photo-polarimeter (ISOPHOT) jointly covered wavelengths from 2.5 to around 240 microns with spatial resolutions ranging from 1.5 arcseconds (at the shortest wavelengths) to 90 arcseconds (at the longer wavelengths). Its 60 cm diameter telescope was cooled by superfluid liquid helium to temperatures of 2-4 K.
- ID:
- ivo://nasa.heasarc/intbsc
- Title:
- INTEGRAL Bright Source Catalog
- Short Name:
- INTEGRAL/BSC
- Date:
- 03 May 2024
- Publisher:
- NASA/GSFC HEASARC
- Description:
- The INTEGRAL Bright Source Catalog is based on publicly available data from the two main instruments (IBIS and SPI) on board INTEGRAL (see Winkler et al. 2003, A&A, 411, L1 for a description of the INTEGRAL spacecraft and instrument packages). INTEGRAL began collecting data in October 2002. This catalog will be regularly updated as data become public (~14 months after they are obtained). The Bright Source Catalog is a collaborative effort between the INTEGRAL Science Data Center (ISDC) in Switzerland and the NASA Goddard Space Flight Center (GSFC) INTEGRAL Guest Observer Facility (GOF). The results presented here are a result of a semi-automated analysis and they should be considered as approximate: they are intended to serve as a guideline to those interested in pursuing more detailed follow-up analyses. The data from the imager ISGRI (Lebrun et al. 2003, A&A, 411, L141) have been analyzed at the INTEGRAL Science Data Centre (ISDC), while the SPI (Vedrenne et al. 2003, A&A, 411, L63) data analysis was performed at GSFC as a service of the INTEGRAL GOF. This database table was first created in September 2004. It is based on the online web page maintained by the INTEGRAL GOF at the URL <a href="http://heasarc.gsfc.nasa.gov/docs/integral/INTEGRAL_bright_sources.html">http://heasarc.gsfc.nasa.gov/docs/integral/INTEGRAL_bright_sources.html</a> and is updated on a weekly basis whenever the web page is updated. This is a service provided by NASA HEASARC .
- ID:
- ivo://mast.stsci/ssap/iue
- Title:
- International Ultraviolet Explorer
- Short Name:
- IUE
- Date:
- 22 Jul 2020 21:56:49
- Publisher:
- Space Telescope Science Institute Archive
- Description:
- The International Ultraviolet Explorer (IUE) performed spectrophotometry at high (0.1-0.3 Å) and low (6-7 Å) resolution between 1150 Å and 3200 Å. This service currently provides access to the low dispersion "NEWSIPS" data, reformatted to be VO-compatible.
- ID:
- ivo://irsa.ipac/SSA
- Title:
- IRSA Simple Spectral Access (SSA) Protocol Service
- Short Name:
- IRSA SSA
- Date:
- 06 May 2021 17:44:00
- Publisher:
- NASA/IPAC Infrared Science Archive
- Description:
- This is IRSA's implementation of the IVOA Simple Spectral Access (SSA) protocol. Our SSA service allows a rich variety of searches against IRSA's varied holdings.
- ID:
- ivo://svo.cab/iue/ssap3
- Title:
- IUE highly processed spectra
- Date:
- 04 Sep 2019 08:25:52
- Publisher:
- SVO CAB
- Description:
- IUE HPDP spectra
- ID:
- ivo://svo.cab/models/kurucz2003all
- Title:
- Kurucz ODFNEW /NOVER (2003)
- Short Name:
- Kurucz2003all
- Date:
- 27 Sep 2022 13:40:47
- Publisher:
- SVO CAB
- Description:
- ATLAS9 Kurucz ODFNEW /NOVER models. Newly computed ODFs with better opacities and better abundances have been used.
- ID:
- ivo://svo.cab/models/kurucz2003alp
- Title:
- Kurucz ODFNEW /NOVER (2003) alpha:0.4
- Short Name:
- Kurucz2003a04
- Date:
- 27 Sep 2022 13:46:53
- Publisher:
- SVO CAB
- Description:
- ATLAS9 Kurucz ODFNEW /NOVER models. Newly computed ODFs with better opacities and better abundances have been used.
- ID:
- ivo://svo.cab/models/kurucz2003
- Title:
- Kurucz ODFNEW /NOVER (2003) alpha:0.0
- Short Name:
- Kurucz2003
- Date:
- 27 Sep 2022 13:46:24
- Publisher:
- SVO CAB
- Description:
- ATLAS9 Kurucz ODFNEW /NOVER models. Newly computed ODFs with better opacities and better abundances have been used.
- ID:
- ivo://svo.cab/models/kurucz
- Title:
- Kurucz ODFNEW /NOVER models
- Short Name:
- Kurucz
- Date:
- 04 Sep 2019 08:29:03
- Publisher:
- SVO CAB
- Description:
- Kurucz ODFNEW /NOVER models. Newly computed ODFs with better opacities and better abundances have been used. (The convective treatment is described in Castelli et al. 1997, AA 318, 841.)
- ID:
- ivo://org.gavo.dc/lamost6/q/svc_lrs
- Title:
- LAMOST DR6 Low Resolution Spectra
- Short Name:
- LM6 LRS SSAP
- Date:
- 30 May 2022 13:40:13
- Publisher:
- The GAVO DC team
- Description:
- A machine-readable interface to the LAMOST6 low resolution spectra based on SSAP and datalink.
- ID:
- ivo://org.gavo.dc/lamost6/q/svc_mrs
- Title:
- LAMOST DR6 Medium Resolution Spectra
- Short Name:
- LM6 MRS SSAP
- Date:
- 30 May 2022 13:40:13
- Publisher:
- The GAVO DC team
- Description:
- A machine-readable interface to the LAMOST6 medium resolution spectra based on SSAP and datalink.
- ID:
- ivo://cvo.naoc/data/lamost/dr1/ssa
- Title:
- LAMOST DR1 SPECTRUM CATALOG SERVICE
- Short Name:
- LAMOST.DR1.SSAP
- Date:
- 17 Jun 2019 15:22:03
- Publisher:
- China-VO
- Description:
- LAMOST DR1 totally releases 2,204,860 spectra, include 717,660 objects of the pilot survey (2011-10-24~2012-06-30), and 1,487,200 objects of the regular survey (2012-09-28~2013-06-30). DR1 includes two types of data: optical spectra (flux- and wavelength-calibrated, sky-subtracted), and catalog data, which includes both parameters measure from spectra, such as redshifts and signal to noise ratios, and parameters inherited from input catalogs. You should keep in mind that LAMOST is a spectral survey telescope, and the parameters related to photometry, which you get here, all come from other surveys.
- ID:
- ivo://org.gavo.dc/lamost5/q/ssa
- Title:
- LAMOST DR5 survey spectra
- Short Name:
- LAMOST DR5 SSAP
- Date:
- 23 Mar 2022 13:13:19
- Publisher:
- The GAVO DC team
- Description:
- This services provides 1D spectra from DR5 of LAMOST (Large Sky Area Multi-Object Fiber Spectroscopic Telescope) through SSAP and Obscore; data is served both in VO-standard SDM and, via datalink, the original SDSS-inspired FITS described in http://dr5.lamost.org/doc/data-production-description .
- ID:
- ivo://asu.cas.cz/lamost_dr2/q/ssa
- Title:
- LAMOST DR2 survey spectra
- Short Name:
- LAMOST DR2 SSAP
- Date:
- 23 Nov 2018 01:03:06
- Publisher:
- Stellar Department of Astronomical Institute of the Academy of Sciences of the Czech Republic
- Description:
- LAMOST DR2 SSAP service
- ID:
- ivo://asu.cas.cz/lamost_dr3/q/ssa
- Title:
- LAMOST DR3 survey spectra
- Short Name:
- LAMOST DR3 SSAP
- Date:
- 01 Nov 2018 15:51:24
- Publisher:
- Stellar Department of Astronomical Institute of the Academy of Sciences of the Czech Republic
- Description:
- LAMOST DR3 SSAP service
- ID:
- ivo://asu.cas.cz/lamost_dr1/q/ssa
- Title:
- LAMOST DR1 survey spectra
- Short Name:
- LAMOST DR1 SSAP
- Date:
- 01 Nov 2018 15:49:30
- Publisher:
- Stellar Department of Astronomical Institute of the Academy of Sciences of the Czech Republic
- Description:
- LAMOST DR1 SSAP service
- ID:
- ivo://svo.cab/cat/chiu06
- Title:
- L and T dwarf (Chiu et al. 2006)
- Short Name:
- Chiu2006
- Date:
- 03 Jun 2020 15:34:07
- Publisher:
- SVO/CAB
- Description:
- L and T dwarf (Chiu et al. 2006)
95. Levenhagen 2017
- ID:
- ivo://svo.cab/models/levenhagen
- Title:
- Levenhagen 2017
- Short Name:
- Levenhagen
- Date:
- 04 Sep 2019 08:31:00
- Publisher:
- SVO CAB
- Description:
- A grid of LTE and non-LTE synthetic spectra of hot DA white dwarfs. It covers Teff from 17,000 K to 100,000 K and log(g) from 7.0 to 9.5. The stellar models are built for pure hydrogen and the spectra cover a wavelength range from 90 nm to 2.5 micron.
- ID:
- ivo://org.gavo.dc/lotsspol/q/ssa
- Title:
- LoTSS DR2 Polarization spectra
- Short Name:
- lotsspol SSAP
- Date:
- 20 Jan 2023 07:33:07
- Publisher:
- The GAVO DC team
- Description:
- The LOFAR Two Meter Sky Survey LoTSS DR2 (:bibcode:`2022A&A...659A...1S`) obtained radio data from 27% of the northern sky between 120 and 168 MHz in the year 2014 through 2020. This service publishes polarization spectra of extragalactic radio sources (radio galaxies and blazars) and the rotation measures derived from them. We also give redshifts for all sources. The data has a spatial resolution of 20 arcsec.
- ID:
- ivo://org.gavo.dc/magic/q/ssa
- Title:
- Magic Public Spectra
- Short Name:
- Magic SSAP
- Date:
- 23 Mar 2022 13:13:10
- Publisher:
- The GAVO DC team
- Description:
- The MAGIC project observes the VHE sky (GeV~TeV) through Cherenkov radiation events. The project is operating since 2004 and with the support from the Spain-VO team they provide data access through a VO-SSAP and web services. This service re-publishes the data with homogeneized in flux units (given here in 'erg/(s.cm2)'). Photon energy values in are transfomred to frequencies.
- ID:
- ivo://bsdc.icranet.org/magic/q/ssa
- Title:
- Magic Public Spectra SSAP Interface
- Short Name:
- Magic SSAP
- Date:
- 17 May 2017 10:12:24
- Publisher:
- BSDC
- Description:
- The MAGIC project observes the VHE sky (GeV~TeV) through Cherenkov radiation events. The project is operating since 2004 and with the support from the Spain-VO team they provide data access through a VO-SSAP and web services. Our goal here is to provide the same kind of service with the difference that the data is transformed and homogeneized in its flux units, to values in 'erg/(s.cm2)', and photon energy values in equivalent 'Hz' frequency values.
- ID:
- ivo://wfau.roe.ac.uk/HEAVENS_at_ISDC/light-curves
- Title:
- Mining the HEAVENS with the Virtual Observatory
- Short Name:
- HEAVENS @ ISDC
- Date:
- 03 May 2012 15:51:44
- Publisher:
- WFAU
- Description:
- With time, all HEAVENS products should become available on the Virtual Observatory. In some cases this requires an enhancement of the Virtual Observatory standards. For now the following HEAVENS services are available through the VO: - SIAP Image cutout service for INTEGRAL/ISGRI and JEM-X - Timeseries service for INTEGRAL/ISGRI, JEM-X and OMC Wished features include: - Extended Query Parameters for time intervals - Extended Query Parameters for energy bands - Timeseries service for INTEGRAL/IREM and SPI-ACS - Spectra service for all INTEGRAL instruments
100. Morley 2012
- ID:
- ivo://svo.cab/models/morley12
- Title:
- Morley 2012
- Short Name:
- Morley 2012
- Date:
- 04 Sep 2019 08:31:00
- Publisher:
- SVO CAB
- Description:
- Morley et al. 2012 T/Y dwarf models