Sökning: WFRF:(Ofek E. O.) > (2019) > Nugent P. E. > A Six-year Image-su...
Fältnamn | Indikatorer | Metadata |
---|---|---|
000 | 02861naa a2200493 4500 | |
001 | oai:DiVA.org:su-168317 | |
003 | SwePub | |
008 | 190510s2019 | |||||||||||000 ||eng| | |
024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-1683172 URI |
024 | 7 | a https://doi.org/10.1088/1538-3873/ab0a192 DOI |
040 | a (SwePub)su | |
041 | a engb eng | |
042 | 9 SwePub | |
072 | 7 | a ref2 swepub-contenttype |
072 | 7 | a art2 swepub-publicationtype |
100 | 1 | a Ofek, E. O.4 aut |
245 | 1 0 | a A Six-year Image-subtraction Light Curve of SN 2010jl |
264 | c 2019-04-12 | |
264 | 1 | b IOP Publishing,c 2019 |
338 | a print2 rdacarrier | |
520 | a SN 2010jl was a luminous Type Lin supernova (SN), detected in radio, optical, X-ray and hard X-rays. Here we report on its six-year R- and g-band light curves obtained using the Palomar Transient Factory. The light curve was generated using a pipeline based on the proper image-subtraction method and we discuss the algorithm performances. As noted before, the R-band light curve, up to about 300 days after maximum light is well described by a power-law decline with a power-law index of alpha approximate to -0.5. Between day 300 and day 2300 after maximum light, it is consistent with a power-law decline, with a power-law index of about alpha approximate to -3.4. The longevity of the light curve suggests that the massive circumstellar material around the progenitor was ejected on timescales of at least tens of years prior to the progenitor explosion. | |
650 | 7 | a NATURVETENSKAPx Fysik0 (SwePub)1032 hsv//swe |
650 | 7 | a NATURAL SCIENCESx Physical Sciences0 (SwePub)1032 hsv//eng |
653 | a methods: statistical | |
653 | a stars: mass-loss | |
653 | a (stars:) supernovae: general | |
653 | a (stars:) supernovae: individual (... | |
653 | a ...) | |
700 | 1 | a Zackay, B.4 aut |
700 | 1 | a Gal-Yam, A.4 aut |
700 | 1 | a Sollerman, Jesperu Stockholms universitet,Institutionen för astronomi,Oskar Klein-centrum för kosmopartikelfysik (OKC)4 aut0 (Swepub:su)solle |
700 | 1 | a Fransson, Claesu Stockholms universitet,Institutionen för astronomi,Oskar Klein-centrum för kosmopartikelfysik (OKC)4 aut0 (Swepub:su)frans |
700 | 1 | a Fremling, C.4 aut |
700 | 1 | a Kulkarni, S. R.4 aut |
700 | 1 | a Nugent, P. E.4 aut |
700 | 1 | a Yaron, O.4 aut |
700 | 1 | a Kasliwal, M. M.4 aut |
700 | 1 | a Masci, F.4 aut |
700 | 1 | a Laher, R.4 aut |
710 | 2 | a Stockholms universitetb Institutionen för astronomi4 org |
773 | 0 | t Publications of the Astronomical Society of the Pacificd : IOP Publishingg 131:999q 131:999x 0004-6280x 1538-3873 |
856 | 4 | u https://authors.library.caltech.edu/94687/2/1903.02016.pdf |
856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-168317 |
856 | 4 8 | u https://doi.org/10.1088/1538-3873/ab0a19 |
Kungliga biblioteket hanterar dina personuppgifter i enlighet med EU:s dataskyddsförordning (2018), GDPR. Läs mer om hur det funkar här.
Så här hanterar KB dina uppgifter vid användning av denna tjänst.
Kopiera och spara länken för att återkomma till aktuell vy