CreditsVOSA uses some external services and theoretical models that you might want to cite or acknowledge if your science benefits from the use of this tool.
You can find below the description and, when appropiate, the bibliographic reference corresponding to all of them.
When you download the results obtained by VOSA two files will be included: info/refs.dat with the references to all the services used to obtain the results and info/refs.bibtex.bib with the bibtex entries corresponding to all those references.
VOSA- Please include the following in any published material that makes use of VOSA:
This publication makes use of VOSA, developed under the Spanish Virtual Observatory (https://svo.cab.inta-csic.es) project funded by MCIN/AEI/10.13039/501100011033/ through grant PID2020-112949GB-I00. - If your research benefits from the use of VOSA, we would appreciate if you could include the following reference in your publication:
Bayo, A., Rodrigo, C., Barrado y Navascués, D., Solano, E., Gutiérrez, R., Morales-Calderón, M., Allard, F. 2008, A&A 492,277B.
Theoretical Spectra.- NextGen
- Computed infrared absorption properties of hot water vapour.
Schryber, Miller & Tennyson 1995 - The NextGen Model Atmosphere Grid for 3000<=T_eff<=10,000 K
Hauschildt et al 1999, ApJ 512, 377 - A revision of the solar abundance of dysprosium
Grevesse et al. 1993, A&A 271, 587 - Evolutionary models for solar metallicity low-mass stars: mass-magnitude relationships and color-magnitude diagrams
Baraffe et al 1998, A&A 337, 403B - Evolutionary models for metal-poor low-mass stars. Lower main sequence of globular clusters and halo field stars
Baraffe et al 1997, A&A 327, 1054 - Model Atmospheres of Very Low Mass Stars and Brown Dwarfs
Allard et al 1997, ARA&A 35, 137 - Star, Brown Dwarf & Planet Simulator
- AMES-Dusty 2000
- AMES-Cond 2000
- Kurucz ODFNEW /NOVER models
- Kurucz ODFNEW /NOVER, alpha: 0.0 (2003)
- Kurucz ODFNEW /NOVER, alpha: 0.4 (2003)
- BT-Settl
- A high-accuracy computed water line list
Barber et al 2006, MNRAS 368, 1087 - The Chemical Composition of the Sun
Asplund et al. 2009, A&A 47, 481 - Progress in modeling very low mass stars, brown dwarfs, and planetary mass objects.
Allard et al. 2013, MSAIS 24, 128 - Models of very-low-mass stars, brown dwarfs and exoplanets
Allard et al 2012, RSPTA 370. 2765A - Model Atmospheres From Very Low Mass Stars to Brown Dwarfs
Allard et al 2011, ASPC 448, 91A - K-H2 quasi-molecular absorption detected in the T-dwarf \varepsilon Indi Ba
Allard et al 2007, A&A 474L, 21 - Model Atmospheres and Spectra: The Role of Dust
Allard et al 2003, IAUS 211, 325 - Star, Brown Dwarf & Planet Simulator
- BT-Settl (AGSS2009)
- A high-accuracy computed water line list
Barber et al 2006, MNRAS 368, 1087 - The Chemical Composition of the Sun
Asplund et al. 2009, A&A 47, 481 - Progress in modeling very low mass stars, brown dwarfs, and planetary mass objects.
Allard et al. 2013, MSAIS 24, 128 - Models of very-low-mass stars, brown dwarfs and exoplanets
Allard et al 2012, RSPTA 370. 2765A - Model Atmospheres From Very Low Mass Stars to Brown Dwarfs
Allard et al 2011, ASPC 448, 91A - K-H2 quasi-molecular absorption detected in the T-dwarf \varepsilon Indi Ba
Allard et al 2007, A&A 474L, 21 - Model Atmospheres and Spectra: The Role of Dust
Allard et al 2003, IAUS 211, 325 - Star, Brown Dwarf & Planet Simulator
- BT-Settl (CIFIST)
- Solar Chemical Abundances Determined with a CO5BOLD 3D Model Atmosphere
Caffau et al. 2011, SoPh 268, 255 - A high-accuracy computed water line list
Barber et al 2006, MNRAS 368, 1087 - Progress in modeling very low mass stars, brown dwarfs, and planetary mass objects.
Allard et al. 2013, MSAIS 24, 128 - Models of very-low-mass stars, brown dwarfs and exoplanets
Allard et al 2012, RSPTA 370. 2765A - Model Atmospheres From Very Low Mass Stars to Brown Dwarfs
Allard et al 2011, ASPC 448, 91A - K-H2 quasi-molecular absorption detected in the T-dwarf \varepsilon Indi Ba
Allard et al 2007, A&A 474L, 21 - Model Atmospheres and Spectra: The Role of Dust
Allard et al 2003, IAUS 211, 325 - Star, Brown Dwarf & Planet Simulator
- BT-Settl (GNS93)
- A revision of the solar abundance of dysprosium
Grevesse et al. 1993, A&A 271, 587 - A high-accuracy computed water line list
Barber et al 2006, MNRAS 368, 1087 - Progress in modeling very low mass stars, brown dwarfs, and planetary mass objects.
Allard et al. 2013, MSAIS 24, 128 - Models of very-low-mass stars, brown dwarfs and exoplanets
Allard et al 2012, RSPTA 370. 2765A - Model Atmospheres From Very Low Mass Stars to Brown Dwarfs
Allard et al 2011, ASPC 448, 91A - K-H2 quasi-molecular absorption detected in the T-dwarf \varepsilon Indi Ba
Allard et al 2007, A&A 474L, 21 - Model Atmospheres and Spectra: The Role of Dust
Allard et al 2003, IAUS 211, 325 - You could want to take a look also to Grevesse & Noels, 1993 for more information about solar abundances.
- Star, Brown Dwarf & Planet Simulator
- BT-COND
- BT-DUSTY
- BT-NextGen (AGSS2009)
- BT-NextGen (GNS93)
- A revision of the solar abundance of dysprosium
Grevesse et al. 1993, A&A 271, 587 - A high-accuracy computed water line list
Barber et al 2006, MNRAS 368, 1087 - Models of very-low-mass stars, brown dwarfs and exoplanets
Allard et al 2012, RSPTA 370. 2765A - Model Atmospheres From Very Low Mass Stars to Brown Dwarfs
Allard et al 2011, ASPC 448, 91A - You could want to take a look also to Grevesse & Noels, 1993 for more information about solar abundances.
- Star, Brown Dwarf & Planet Simulator
- Black Body
- Coelho Synthetic stellar library (SEDs)
- Koester WD models
- Levenhagen 2017
- DRIFT-PHOENIX
- Dust in brown dwarfs. II. The coupled problem of dust formation and sedimentation
Woitke P., Helling C., 2003, A&A, 399, 297 - Dust in brown dwarfs and extra-solar planets. III. Testing synthetic spectra on observations
Witte et al. 2011, A&A, 529, A44 - Dust in brown dwarfs and extra-solar planets. II. Cloud formation for cosmologically evolving abundances
Witte et al. 2009, A&A, 506, 1367 - Consistent Simulations of Substellar Atmospheres and Nonequilibrium Dust Cloud Formation
Helling et al. 2008, ApJL, 675, L105 - Dust in brown dwarfs and extra-solar planets. I. Chemical composition and spectral appearance of quasi-static cloud layers
Helling et al. 2008, A&A, 485, 547 - Dust in brown dwarfs. V. Growth and evaporation of dirty dust grains
Helling C., Woitke P., 2006, A&A, 455, 325 - Numerical solution of the expanding stellar atmosphere problem
Hauschildt & Baron 1999, JCoAM 109, 41 - Highlights of Stellar Modeling with PHOENIX
Baron et al. 2003, IAU 210, 19 - Dust in brown dwarfs. III. Formation and structure of quasi-static cloud layers
Woitke P., Helling C., 2004, A&A, 414, 335
- Morley 2012
- Morley 2014
- ATMO 2020, CEQ
- ATMO 2020, NEQ strong
- ATMO 2020, NEQ weak
- Saumon 2012
- TMAP (Grid 1)
- TMAP (Grid 2)
- TMAP (Grid 3)
- TMAP (Grid 4)
- TMAP
- TMAP - Tubingen
- GRAMS, C-rich grid
- GRAMS, O-rich original grid
- The Mass-loss Return from Evolved Stars to the Large Magellanic Cloud. IV. Construction and Validation of a Grid of Models for Oxygen-rich AGB Stars, Red Supergiants, and Extreme AGB Stars
Sargent et al 2011, ApJ 728, 93
- Husfeld et al models for non-LTE Helium-rich stars
- Pacheco et al 2021
- TLUSTY OSTAR2002+BSTAR2006
- A Grid of NLTE Line-blanketed Model Atmospheres of Early B-Type Stars.
Lanz, T., Hubeny, I. 2007, ApJS, 169, 83 - A Grid of Non-LTE Line-blanketed Model Atmospheres of O-Type Stars
Lanz, T., Hubeny, I. 2003, ApJS, 146, 417 - NLTE line blanketed model atmospheres of hot stars. I. Hybrid Complete Linearization/Accelerated Lambda Iteration Method
Hubeny, I., Lanz, T. 1995, ApJ, 439, 875H - TLusty web page
Template fit- Bayo et al, M types from Collinder 69
- Spectroscopy of very low mass stars and brown dwarfs in the Lambda Orionis star forming region. I. Enlarging the census down to the planetary mass domain in Collinder 69
Bayo et al 2011, A&A 536, 63B
- UVES/VLT
- L and T dwarf data archive
- Near-Infrared Photometry and Spectroscopy of L and T Dwarfs: The Effects of Temperature, Clouds, and Gravity
Knapp et al. 2004, AJ, 127, 3553 - L' and M' Photometry of Ultracool Dwarfs
Golimowski et al. 2004, AJ, 127, 3516 - Seventy-One New L and T Dwarfs from the Sloan Digital Sky Survey
Chiu et al. 2006, AJ, 131, 2722 - L and T dwarf data archive
- Keck LRIS spectra of late-M, L and T dwarfs
- The NIRSPEC Brown Dwarf Spectroscopic Survey
- Kesseli et al.
- An empirical template library of stellar spectra for a wide range of spectral classes, luminosity classes, and metallicities using SDSS BOSS spectra
Kesseli et al 2017
- The SpeX Prism Spectral Libraries
Theoretical Isochrones and Evolutionary Tracks- BT-Settl Isochrones and Evolutionary Tracks
- BHAC15 Isochrones and Evolutionary Tracks
- NextGen Isochrones and Evolutionary Tracks
- COND99 Isochrones and Evolutionary Tracks
- DUSTY99 Isochrones and Evolutionary Tracks
- Siess Isochrones and Evolutionary Tracks
- PARSEC 1.2 Isochrones and Evolutionary Tracks
- Geneva 2011 Isochrones and Evolutionary Tracks (Z=0.014)
- Geneva (Haemmerle 2019) Isochrones and Evolutionary Tracks
- SPOTS (f=0) Isochrones and Evolutionary Tracks
- SPOTS (f=0.17) Isochrones and Evolutionary Tracks
- SPOTS (f=0.34) Isochrones and Evolutionary Tracks
- SPOTS (f=0.51) Isochrones and Evolutionary Tracks
- SPOTS (f=0.68) Isochrones and Evolutionary Tracks
- SPOTS (f=0.85) Isochrones and Evolutionary Tracks
- ATMO2020 (CEQ) Isochrones and Evolutionary Tracks
- ATMO2020 (NEQ strong) Isochrones and Evolutionary Tracks
- ATMO2020 (NEQ weak) Isochrones and Evolutionary Tracks
VO Photometry- 2MASS All-Sky Point Source Catalog
- The Two Micron All Sky Survey (2MASS)
Skrutskie et al, 2006, AJ, 131, 1163S - The VizieR database of astronomical catalogues
Ochsenbein et al 2000, A&AS 143, 221 - Acknowledgement
This publication makes use of data products from the Two Micron All Sky Survey, which is a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation.
- AKARI/IRC mid-IR all-sky Survey (ISAS/JAXA, 2010)
- The AKARI/IRC mid-infrared all-sky survey
Ishihara et al, 2010, A&A, 514, A1 - The Infrared Astronomical Mission AKARI
Murakami et al, 2007, PASJ 59, S369 - The VizieR database of astronomical catalogues
Ochsenbein et al 2000, A&AS 143, 221 - The Infrared Camera (IRC) for AKARI -- Design and Imaging Performance
Onaka et al, 2007, PASJ, 59, S401
- AKARI/FIS All-Sky Survey Point Source Catalogues (ISAS/JAXA, 2010)
- WISE
- Acknowledgement
This publication makes use of data products from the Wide-field Infrared Survey Explorer, which is a joint project of the University of California, Los Angeles, and the Jet Propulsion Laboratory/California Institute of Technology, funded by the National Aeronautics and Space Administration. - The VizieR database of astronomical catalogues
Ochsenbein et al 2000, A&AS 143, 221 - The Wide-field Infrared Survey Explorer (WISE): Mission Description and Initial On-orbit Performance
Wright et al 2010, AJ 140, 1868W
- DENIS Catalogue
- GLIMPSE Source Catalog (I + II + 3D)
- IRAS Catalog of Point Sources, Version 2.0
- IRAS Faint Source Catalog
- C2D Spitzer and Ancillary Data
- FEPS Catalog
- Taurus Catalog
- MSX6C Infrared Point Source Catalog
- NEOWISE Reactivation
- Initial Performance of the NEOWISE Reactivation Mission
Mainzer et al. 2014, ApJ, 792, 30 - Acknowledgement
This publication makes use of data products from the Near-Earth Object Wide-field Infrared Survey Explorer (NEOWISE), which is a joint project of the Jet Propulsion Laboratory/California Institute of Technology and the University of Arizona. NEOWISE is funded by the National Aeronautics and Space Administration.
- UKIDSS Deep Extragalactic Survey DR10
- The UKIRT wide field camera ZYJHK photometric system: calibration from 2MASS
Hodgkin et ak, 2009, MNRAS, 394, 675 - The UKIRT Infrared Deep Sky Survey ZY JHK photometric system: passbands and synthetic colours
Hewett et al 2006, MNRAS, 367, 454 - The WFCAM Science Archive
Hambly et al 2008, MNRAS 384, 637 - The UKIRT wide-field camera
Casali et al, 2007, A&A, 467, 777 - The UKIRT Infrared Deep Sky Survey (UKIDSS)
Lawrence et al, 2007, MNRAS, 379, 1599
- UKIDSS Galactic Clusters Survey DR10
- The UKIRT wide field camera ZYJHK photometric system: calibration from 2MASS
Hodgkin et ak, 2009, MNRAS, 394, 675 - The UKIRT Infrared Deep Sky Survey ZY JHK photometric system: passbands and synthetic colours
Hewett et al 2006, MNRAS, 367, 454 - The WFCAM Science Archive
Hambly et al 2008, MNRAS 384, 637 - The UKIRT wide-field camera
Casali et al, 2007, A&A, 467, 777 - The UKIRT Infrared Deep Sky Survey (UKIDSS)
Lawrence et al, 2007, MNRAS, 379, 1599
- UKIDSS Galactic Plane Survey DR8
- The UKIRT wide field camera ZYJHK photometric system: calibration from 2MASS
Hodgkin et ak, 2009, MNRAS, 394, 675 - The UKIRT Infrared Deep Sky Survey ZY JHK photometric system: passbands and synthetic colours
Hewett et al 2006, MNRAS, 367, 454 - The WFCAM Science Archive
Hambly et al 2008, MNRAS 384, 637 - The UKIRT wide-field camera
Casali et al, 2007, A&A, 467, 777 - The UKIRT Infrared Deep Sky Survey (UKIDSS)
Lawrence et al, 2007, MNRAS, 379, 1599
- UKIDSS Large Area Survey DR10
- The UKIRT wide field camera ZYJHK photometric system: calibration from 2MASS
Hodgkin et ak, 2009, MNRAS, 394, 675 - The UKIRT Infrared Deep Sky Survey ZY JHK photometric system: passbands and synthetic colours
Hewett et al 2006, MNRAS, 367, 454 - The WFCAM Science Archive
Hambly et al 2008, MNRAS 384, 637 - The UKIRT wide-field camera
Casali et al, 2007, A&A, 467, 777 - The UKIRT Infrared Deep Sky Survey (UKIDSS)
Lawrence et al, 2007, MNRAS, 379, 1599
- UKIDSS Ultra Deep Survey DR10
- The UKIRT wide field camera ZYJHK photometric system: calibration from 2MASS
Hodgkin et ak, 2009, MNRAS, 394, 675 - The UKIRT Infrared Deep Sky Survey ZY JHK photometric system: passbands and synthetic colours
Hewett et al 2006, MNRAS, 367, 454 - The WFCAM Science Archive
Hambly et al 2008, MNRAS 384, 637 - The UKIRT wide-field camera
Casali et al, 2007, A&A, 467, 777 - The UKIRT Infrared Deep Sky Survey (UKIDSS)
Lawrence et al, 2007, MNRAS, 379, 1599
- VHS - VISTA Hemisphere Survey, DR6
- VIDEO - VISTA Deep Extragalactic Observations Survey, DR5
- VIKING - VISTA Kilo-Degree Infrared Galaxy Survey, DR4
- VMC - VISTA Magellanic Survey, DR4
- VVV - VISTA Variables in the Via Lactea, DR4
- ALHAMBRA gold
- Near-Infrared Galaxy Counts and Evolution from the Wide-Field ALHAMBRA Survey
Cristóbal-Hornillos et al. 2009, ApJ 696, 1554 - The Alhambra Survey: a Large Area Multimedium-Band Optical and Near-Infrared Photometric Survey
Moles et al, AJ, 2008, 136, 1325 - The ALHAMBRA Survey: Bayesian photometric redshifts with 23 bands for 3 deg
Molino et al. 2013, MNRAS 441,2891 - The ALHAMBRA Photometric System
Villegas et al. 2010, AJ 139, 1242
- APASS 9
- CMC14
- CMC15
- DARK ENERGY SURVEY, DR1
- The VizieR database of astronomical catalogues
Ochsenbein et al 2000, A&AS 143, 221 - Acknowledgement
This project used public archival data from the Dark Energy Survey (DES). Funding for the DES Projects has been provided by the U.S. Department of Energy, the U.S. National Science Foundation, the Ministry of Science and Education of Spain, the Science and Technology Facilities Council of the United Kingdom, the Higher Education Funding Council for England, the National Center for Supercomputing Applications at the University of Illinois at Urbana–Champaign, the Kavli Institute of Cosmological Physics at the University of Chicago, the Center for Cosmology and Astro-Particle Physics at the Ohio State University, the Mitchell Institute for Fundamental Physics and Astronomy at Texas A&M University, Financiadora de Estudos e Projetos, Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro, Conselho Nacional de Desenvolvimento Científico e Tecnológico and the Ministério da Ciência, Tecnologia e Inovação, the Deutsche Forschungsgemeinschaft and the Collaborating Institutions in the Dark Energy Survey.
The Collaborating Institutions are Argonne National Laboratory, the University of California at Santa Cruz, the University of Cambridge, Centro de Investigaciones Enérgeticas, Medioambientales y Tecnológicas–Madrid, the University of Chicago, University College London, the DES-Brazil Consortium, the University of Edinburgh, the Eidgenössische Technische Hochschule (ETH) Zürich, Fermi National Accelerator Laboratory, the University of Illinois at Urbana-Champaign, the Institut de Ciències de l'Espai (IEEC/CSIC), the Institut de Física d'Altes Energies, Lawrence Berkeley National Laboratory, the Ludwig-Maximilians Universität München and the associated Excellence Cluster Universe, the University of Michigan, the National Optical Astronomy Observatory, the University of Nottingham, The Ohio State University, the OzDES Membership Consortium, the University of Pennsylvania, the University of Portsmouth, SLAC National Accelerator Laboratory, Stanford University, the University of Sussex, and Texas A&M University.
Based in part on observations at Cerro Tololo Inter-American Observatory, National Optical Astronomy Observatory, which is operated by the Association of Universities for Research in Astronomy (AURA) under a cooperative agreement with the National Science Foundation. - The Dark Energy Survey: Data Release 1
Abbott et al. 2018, ApJS 239 18A
- Synt.Phot. from Gaia DR3 (CDS)
- Gaia DR3 (CDS)
- GaiaDR3 J-PAS Synt.Phot.
- Gaia DR3 Doc.
Gaia DR3 Documentation - Gaia DR3 Credit and citation instructions
Gaia DR3 Credit and citation instructions - Gaia Data Release 3: The Galaxy in your preferred colours. Synthetic photometry from Gaia low-resolution spectra
Gaia, Montegriffo et al. 2022 - The Gaia mission
Gaia Collaboration et al. 2016, A&A 595, 1G - Acknowledgement
This work has made use of data from the European Space Agency (ESA) mission Gaia (https://www.cosmos.esa.int/gaia), processed by the Gaia Data Processing and Analysis Consortium (DPAC, https://www.cosmos.esa.int/web/gaia/dpac/consortium). Funding for the DPAC has been provided by national institutions, in particular the institutions participating in the Gaia Multilateral Agreement.
- GTC OSIRIS DR1
- Hipparcos
- IPHAS Catalogue
- J-PLUS DR3
- Stroemgren-Crawford uvbyβ photometry catalog (Paunzen, 2015)
- Pan-Starrs PS1 DR2
- Pan-STARRS Pixel Processing: Detrending, Warping, Stacking
Waters et al 2016, arXiv: 1612.05245 - Pan-STARRS Photometric and Astrometric Calibration
Magnier et al 2016, arXiv:1612.05242 - The Pan-STARRS Data Processing System
Magnier et al 2016, arXiv:1612.05240 - Pan-STARRS Pixel Analysis : Source Detection and Characterization
Magnier et al 2016, arXiv: 1612.05244 - The Pan-STARRS1 Database and Data Products
Flewelling et al 2016, arXiv: 1612.05243 - The Pan-STARRS1 Surveys
Chambers et al 2016, arXiv: 1612.05560 - Acknowledgement
The Pan-STARRS1 Surveys (PS1) and the PS1 public science archive have been made possible through contributions by the Institute for Astronomy, the University of Hawaii, the Pan-STARRS Project Office, the Max-Planck Society and its participating institutes, the Max Planck Institute for Astronomy, Heidelberg and the Max Planck Institute for Extraterrestrial Physics, Garching, The Johns Hopkins University, Durham University, the University of Edinburgh, the Queen's University Belfast, the Harvard-Smithsonian Center for Astrophysics, the Las Cumbres Observatory Global Telescope Network Incorporated, the National Central University of Taiwan, the Space Telescope Science Institute, the National Aeronautics and Space Administration under Grant No. NNX08AR22G issued through the Planetary Science Division of the NASA Science Mission Directorate, the National Science Foundation Grant No. AST-1238877, the University of Maryland, Eotvos Lorand University (ELTE), the Los Alamos National Laboratory, and the Gordon and Betty Moore Foundation.
- SDSS Catalogue, Release 12
- Please, check the SDSS credits page
- The VizieR database of astronomical catalogues
Ochsenbein et al 2000, A&AS 143, 221 - The Eleventh and Twelfth Data Releases of the Sloan Digital Sky Survey: Final Data from SDSS-III
Alam et al., 2015, ApJS, 219, 12A - Acknowledgement
Funding for the SDSS and SDSS-II has been provided by the Alfred P. Sloan Foundation, the Participating Institutions, the National Science Foundation, the U.S. Department of Energy, the National Aeronautics and Space Administration, the Japanese Monbukagakusho, the Max Planck Society, and the Higher Education Funding Council for England. The SDSS Web Site is http://www.sdss.org/.
The SDSS is managed by the Astrophysical Research Consortium for the Participating Institutions. The Participating Institutions are the American Museum of Natural History, Astrophysical Institute Potsdam, University of Basel, University of Cambridge, Case Western Reserve University, University of Chicago, Drexel University, Fermilab, the Institute for Advanced Study, the Japan Participation Group, Johns Hopkins University, the Joint Institute for Nuclear Astrophysics, the Kavli Institute for Particle Astrophysics and Cosmology, the Korean Scientist Group, the Chinese Academy of Sciences (LAMOST), Los Alamos National Laboratory, the Max-Planck-Institute for Astronomy (MPIA), the Max-Planck-Institute for Astrophysics (MPA), New Mexico State University, Ohio State University, University of Pittsburgh, University of Portsmouth, Princeton University, the United States Naval Observatory, and the University of Washington.
- Stromgren uvby-beta Catalogue (Hauck+ 1997)
- Tycho-2 Catalogue
- Homogeneous Means in the UBV System (Mermilliod 1991)
- VPHAS+ DR2
- ZTF DR12
- The Zwicky Transient Facility: Data Processing, Products, and Archive
Masci et al. 2019, PASP 131, 995 - Acknowledgement
Based on observations obtained with the Samuel Oschin Telescope 48-inch and the 60-inch Telescope at the Palomar Observatory as part of the Zwicky Transient Facility project. ZTF is supported by the National Science Foundation under Grants No. AST-1440341 and AST-2034437 and a collaboration including current partners Caltech, IPAC, the Weizmann Institute for Science, the Oskar Klein Center at Stockholm University, the University of Maryland, Deutsches Elektronen-Synchrotron and Humboldt University, the TANGO Consortium of Taiwan, the University of Wisconsin at Milwaukee, Trinity College Dublin, Lawrence Livermore National Laboratories, IN2P3, University of Warwick, Ruhr University Bochum, Northwestern University and former partners the University of Washington, Los Alamos National Laboratories, and Lawrence Berkeley National Laboratories. Operations are conducted by COO, IPAC, and UW.
- Galaxy Evolution Explorer [Galex-DR5 MIS]
- Galaxy Evolution Explorer [GALEX-GR6+7]
- IUE HPDP photometry
- SpecPhot
Object coordinates- Simbad
- Acknowledgement
This research has made use of the SIMBAD database,
operated at CDS, Strasbourg, France - The SIMBAD astronomical database. The CDS reference database for astronomical objects
Wenger et al. 2000, A&AS 143, 9W
Object distance VO services- GAIA DR2
- Gaia Data Release 2. Summary of the contents and survey properties
Gaia Collaboration et al. 2018, A&A 616, A1 - The Gaia mission
Gaia Collaboration et al. 2016, A&A 595, 1G - Gaia Data Release 2. Photometric content and validation
Evans et al. 2018, A&A 616 A4 - Acknowledgement
This work has made use of data from the European Space Agency (ESA) mission Gaia (https://www.cosmos.esa.int/gaia), processed by the Gaia Data Processing and Analysis Consortium (DPAC, https://www.cosmos.esa.int/web/gaia/dpac/consortium). Funding for the DPAC has been provided by national institutions, in particular the institutions participating in the Gaia Multilateral Agreement.
- GAIA DR3 (vizier)
Dereddening- For dereddening the SEDs we make use of the extinction law by Fitzpatrick (1999) improved by Indebetouw et al (2005) in the infrared.
Extinction properties VO services- GaiaDR3 (vizier)
- UBV Photometry of O & B Stars in Vela (Denoyelle 1977)
- Optically visible open clusters and Candidates (Dias+ 2002-2010)
- SAI Open Clusters Catalog (Glushkova+, 2009)
- Guarinos, 1992
- Stellar Spectrophotometric Atlas
- 6dF galaxy survey final redshift release (Jones+, 2009)
- Photometric Catalog of Northern Bright Galaxies (Kodaira+ 1992)
- Reddening and extinction at high galactic latitude (Larson+, 2005)
- RR Lyrae Metallicities (Layden 1994)
- STELIB: A library of stellar spectra at R~2000 (Le Borgne+, 2003)
- UV Interstellar Extinction (Savage+ 1985)
- Extinction map. Morales+, 2006
- The Rv extinction factor, Morales+, 2006
- SWIRE Photometric Redshift Catalogue
- Kainulainen+ 2009
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