WFRF:(Tartaglia D.)
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| Fältnamn | Indikatorer | Metadata |
|---|---|---|
| 000 | 05723naa a2200889 4500 | |
| 001 | oai:DiVA.org:su-215785 | |
| 003 | SwePub | |
| 008 | 230331s2023 | |||||||||||000 ||eng| | |
| 009 | oai:DiVA.org:kth-325097 | |
| 024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-2157852 URI |
| 024 | 7 | a https://doi.org/10.3847/1538-4357/aca1612 DOI |
| 024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-3250972 URI |
| 040 | a (SwePub)sud (SwePub)kth | |
| 041 | a engb eng | |
| 042 | 9 SwePub | |
| 072 | 7 | a ref2 swepub-contenttype |
| 072 | 7 | a art2 swepub-publicationtype |
| 100 | 1 | a Chen, Z. H.u Tsinghua Univ, Phys Dept, Beijing 100084, Peoples R China.;Tsinghua Univ, Tsinghua Ctr Astrophys THCA, Beijing 100084, Peoples R China.4 aut |
| 245 | 1 0 | a The Hydrogen-poor Superluminous Supernovae from the Zwicky Transient Facility Phase I Survey. I. Light Curves and Measurements |
| 264 | c 2023-01-24 | |
| 264 | 1 | b American Astronomical Society,c 2023 |
| 338 | a print2 rdacarrier | |
| 500 | a QC 20230329 | |
| 520 | a During the Zwicky Transient Facility (ZTF) Phase I operations, 78 hydrogen-poor superluminous supernovae (SLSNe-I) were discovered in less than 3 yr, constituting the largest sample from a single survey. This paper (Paper I) presents the data, including the optical/UV light curves and classification spectra, while Paper II in this series will focus on the detailed analysis of the light curves and modeling. Our photometry is primarily taken by ZTF in the g, r, and i bands, and with additional data from other ground-based facilities and Swift. The events of our sample cover a redshift range of z = 0.06 − 0.67, with a median and 1σ error (16% and 84% percentiles) of zmed=0.265. The peak luminosity covers −22.8 mag ≤ Mg,peak ≤ −19.8 mag, with a median value of -21.48. The light curves evolve slowly with a mean rest-frame rise time of trise = 41.9 ± 17.8 days. The luminosity and timescale distributions suggest that low-luminosity SLSNe-I with a peak luminosity ∼−20 mag or extremely fast-rising events (<10 days) exist, but are rare. We confirm previous findings that slowly rising SLSNe-I also tend to fade slowly. The rest-frame color and temperature evolution show large scatters, suggesting that the SLSN-I population may have diverse spectral energy distributions. The peak rest-frame color shows a moderate correlation with the peak absolute magnitude, i.e., brighter SLSNe-I tend to have bluer colors. With optical and UV photometry, we construct the bolometric luminosity and derive a bolometric correction relation that is generally applicable for converting g, r-band photometry to the bolometric luminosity for SLSNe-I. | |
| 650 | 7 | a NATURVETENSKAPx Fysikx Astronomi, astrofysik och kosmologi0 (SwePub)103052 hsv//swe |
| 650 | 7 | a NATURAL SCIENCESx Physical Sciencesx Astronomy, Astrophysics and Cosmology0 (SwePub)103052 hsv//eng |
| 650 | 7 | a NATURVETENSKAPx Fysik0 (SwePub)1032 hsv//swe |
| 650 | 7 | a NATURAL SCIENCESx Physical Sciences0 (SwePub)1032 hsv//eng |
| 653 | a Supernovae | |
| 700 | 1 | a Yan, Lin4 aut |
| 700 | 1 | a Kangas, Tuomasu KTH,Partikel- och astropartikelfysik,Albanova VinnExcellence Center for Protein Technology, ProNova,Oskar Klein Ctr4 aut0 (Swepub:kth)u1m7rsjb |
| 700 | 1 | a Lunnan, Ragnhildu Stockholms universitet,Institutionen för astronomi,Oskar Klein-centrum för kosmopartikelfysik (OKC)4 aut0 (Swepub:su)rlunn |
| 700 | 1 | a Schulze, Steveu Stockholms universitet,Oskar Klein-centrum för kosmopartikelfysik (OKC),Fysikum4 aut0 (Swepub:su)stsc6413 |
| 700 | 1 | a Sollerman, Jesper,d 1968-u Stockholms universitet,Institutionen för astronomi,Oskar Klein-centrum för kosmopartikelfysik (OKC)4 aut0 (Swepub:su)solle |
| 700 | 1 | a Perley, D. A.4 aut |
| 700 | 1 | a Chen, Ting-Wanu Stockholms universitet,Institutionen för astronomi,Oskar Klein-centrum för kosmopartikelfysik (OKC)4 aut0 (Swepub:su)jach1916 |
| 700 | 1 | a Taggart, K.4 aut |
| 700 | 1 | a Hinds, K. R.4 aut |
| 700 | 1 | a Gal-Yam, A.4 aut |
| 700 | 1 | a Wang, X. F.4 aut |
| 700 | 1 | a Andreoni, I.4 aut |
| 700 | 1 | a Bellm, E.4 aut |
| 700 | 1 | a Bloom, J. S.4 aut |
| 700 | 1 | a Burdge, K.4 aut |
| 700 | 1 | a Burgos, A.4 aut |
| 700 | 1 | a Cook, D.4 aut |
| 700 | 1 | a Dahiwale, A.4 aut |
| 700 | 1 | a De, K.4 aut |
| 700 | 1 | a Dekany, R.4 aut |
| 700 | 1 | a Dugas, A.4 aut |
| 700 | 1 | a Frederik, S.4 aut |
| 700 | 1 | a Fremling, C.4 aut |
| 700 | 1 | a Graham, M.4 aut |
| 700 | 1 | a Hankins, M.4 aut |
| 700 | 1 | a Ho, A.4 aut |
| 700 | 1 | a Jencson, J.4 aut |
| 700 | 1 | a Karambelkar, V.4 aut |
| 700 | 1 | a Kasliwal, M.4 aut |
| 700 | 1 | a Kulkarni, S.4 aut |
| 700 | 1 | a Laher, R.4 aut |
| 700 | 1 | a Rusholme, B.4 aut |
| 700 | 1 | a Sharma, Y.4 aut |
| 700 | 1 | a Taddia, F.4 aut |
| 700 | 1 | a Tartaglia, L.4 aut |
| 700 | 1 | a Thomas, B. P.4 aut |
| 700 | 1 | a Tzanidakis, A.4 aut |
| 700 | 1 | a Van Roestel, J.4 aut |
| 700 | 1 | a Walter, R.4 aut |
| 700 | 1 | a Yang, Y.4 aut |
| 700 | 1 | a Yao, Y. H.4 aut |
| 700 | 1 | a Yaron, O.u Weizmann Inst Sci, Dept Particle Phys & Astrophys, IL-76100 Rehovot, Israel.4 aut |
| 710 | 2 | a Tsinghua Univ, Phys Dept, Beijing 100084, Peoples R China.;Tsinghua Univ, Tsinghua Ctr Astrophys THCA, Beijing 100084, Peoples R China.b Partikel- och astropartikelfysik4 org |
| 773 | 0 | t Astrophysical Journald : American Astronomical Societyg 943:1q 943:1x 0004-637Xx 1538-4357 |
| 856 | 4 | u https://doi.org/10.3847/1538-4357/aca161y Fulltext |
| 856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-215785 |
| 856 | 4 8 | u https://doi.org/10.3847/1538-4357/aca161 |
| 856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-325097 |
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- Bellm, E.
- Bloom, J. S.
- Burdge, K.
- Burgos, A.
- Cook, D.
- Dahiwale, A.
- De, K.
- Dekany, R.
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- Hankins, M.
- Ho, A.
- Jencson, J.
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- Kulkarni, S.
- Laher, R.
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- Taddia, F.
- Tartaglia, L.
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