Number of results to display per page
Search Results
- 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:
- 27 Dec 2024 08:31:03
- 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:
- 16 Jan 2024 19:46:29
- 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:
- 07 Mar 2025
- 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 .
