The DOI matches its Crossref record; 21 of the 21 references it cites were found in a registry or an index.
WISeREP—An Interactive Supernova Data Repository
Open accessAbstract
We have entered an era of massive data sets in astronomy. In particular, the number of supernova (SN) discoveries and classifications has substantially increased over the years from few tens to thousands per year. It is no longer the case that observations of a few prototypical events encapsulate most spectroscopic information about SNe, motivating the development of modern tools to collect, archive, organize, and distribute spectra in general and SN spectra in particular. For this reason, we have developed the Weizmann Interactive Supernova Data Repository (WISeREP)—an SQL-based database (DB) with an interactive Web-based graphical interface. The system serves as an archive of high-quality SN spectra, including both historical (legacy) data and data that are accumulated by ongoing modern programs. The archive provides information about objects, their spectra, and related metadata. Utilizing interactive plots, we provide a graphical interface to visualize data, perform line identification of the major relevant species, determine object redshifts, classify SNe, and measure expansion velocities. Guest users may view and download spectra or other data that have been placed in the public domain. Registered users may also view and download data that are proprietary to specific programs with which they are associated. The DB currently holds more than 8000 spectra, of which more than 5000 are public; the latter include published spectra from the Palomar Transient Factory (PTF), all of the SUSPECT (Supernova Spectrum) archive, the Caltech-Core-Collapse Program (CCCP), the CfA SN spectra archive, and published spectra from the University of California, Berkeley, SNDB repository. It offers an efficient and convenient way to archive data and share it with colleagues, and we expect that data stored in this way will be easy to access, increasing its visibility, usefulness, and scientific impact. We encourage the SN community worldwide to make use of the data and tools provided by WISeREP and to contribute data to be made globally available and archived for posterity.
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Filippenko, A. V. (1997) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev.astro.35.1.309 · Cited by 1,824
The Palomar Transient Factory: System Overview, Performance, and First Results
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Self-citationExploring the Optical Transient Sky with the Palomar Transient Factory
Rau, A., Kulkarni, S. R., Law, N. M., Bloom, J. S., Ciardi, D., Djorgovski, G. S., Fox, D. B., Gal-Yam, A., Grillmair, C. C., Kasliwal, M. M., et al. (2009) · Publications of the Astronomical Society of the Pacific · doi:10.1086/605911 · Cited by 736
Self-citationGuy, J., Sullivan, M., Conley, A., Regnault, N., Astier, P., Balland, C., Basa, S., Carlberg, R. G., Fouchez, D., Hardin, D., et al. (2010) · Astronomy & Astrophysics · doi:10.1051/0004-6361/201014468 · Cited by 571
Hydrogen-poor superluminous stellar explosions
Quimby, R. M., Kulkarni, S. R., Kasliwal, M. M., Gal-Yam, A., Arcavi, I., Sullivan, M., Nugent, P., Thomas, R., Howell, D. A., Nakar, E., et al. (2011) · Nature · doi:10.1038/nature10095 · Cited by 546
Self-citationDetermining the Type, Redshift, and Age of a Supernova Spectrum
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Supernova SN 2011fe from an exploding carbon–oxygen white dwarf star
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Self-citationA faint type of supernova from a white dwarf with a helium-rich companion
Perets, H. B., Gal-Yam, A., Mazzali, P. A., Arnett, D., Kagan, D., Filippenko, A. V., Li, W., Arcavi, I., Cenko, S. B., Fox, D. B., et al. (2010) · Nature · doi:10.1038/nature09056 · Cited by 346
Self-citationTHE SPECTROSCOPIC DIVERSITY OF TYPE Ia SUPERNOVAE
Blondin, S., Matheson, T., Kirshner, R. P., Mandel, K. S., Berlind, P., Calkins, M., Challis, P., Garnavich, P. M., Jha, S. W., Modjaz, M., et al. (2012) · The Astronomical Journal · doi:10.1088/0004-6256/143/5/126 · Cited by 306
On the Progenitor of SN 2005gl and the Nature of Type IIn Supernovae
Gal‐Yam, A., Leonard, D. C., Fox, D. B., Cenko, S. B., Soderberg, A. M., Moon, D. ‐., Sand, D. J., Program), (. C. C., Li, W., Filippenko, A. V., et al. (2007) · The Astrophysical Journal · doi:10.1086/510523 · Cited by 298
Self-citation
Cited by
A very luminous magnetar-powered supernova associated with an ultra-long γ-ray burst
Greiner, J., Mazzali, P. A., Kann, D. A., Krühler, T., Pian, E., Prentice, S., Olivares E., F., Rossi, A., Klose, S., Taubenberger, S., et al. (2015) · Nature · doi:10.1038/nature14579 · Cited by 300
Phillips, M. M., Simon, J. D., Morrell, N., Burns, C. R., Cox, N. L. J., Foley, R. J., Karakas, A. I., Patat, F., Sternberg, A., Williams, R. E., et al. (2013) · The Astrophysical Journal · doi:10.1088/0004-637x/779/1/38 · Cited by 275
Self-citationYao, Y., Ravi, V., Gezari, S., van Velzen, S., Lu, W., Schulze, S., Somalwar, J. J., Kulkarni, S. R., Hammerstein, E., Nicholl, M., et al. (2023) · The Astrophysical Journal Letters · doi:10.3847/2041-8213/acf216 · Cited by 219
Metadata
- Authors
- Yaron, O., & Gal-Yam, A.
- Venue
- Publications of the Astronomical Society of the Pacific
- Publisher
- IOP Publishing
- Published
- 2012-07
- Volume
- 124
- Issue
- 917
- Pages
- 668-681
- ISSN
- 0004-6280 (ISSN-L)
- 1538-3873
- OpenAlex
- W2158146204
- Cited by
- 772
- References
- 21
- FWCI
- 22.15
- Type
- journal article
- Language
- en
- Open access
- green
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