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Swift observations of the dwarf nova ASASSN-18fs
High Energy Astrophysical Phenomena · Submitted 2 Nov 2018
abstract compiled · 2026-09-23 · no language-model review
The authors' main claim Here we report on the follow-up photometry using the {\it Neil Gehrels Swift Observatory}.
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The abstract, sentence by sentence
The All Sky Automated Survey for SuperNovae (ASAS-SN) reported a possible Galactic dwarf nova ASASSN-18fs on 2018 March 19 at $\sim$13.2 mag in the V band, with a quiescent magnitude of V$>$17.6. Here we report on the follow-up photometry using the {\it Neil Gehrels Swift Observatory}.
background contribution method result interpretation main claim
| # | sentence | role | the authors' own work | states the main conclusion | strength |
|---|---|---|---|---|---|
| s0 | The All Sky Automated Survey for SuperNovae (ASAS-SN) reported a possible Galactic dwarf nova ASASSN-18fs on 2018 March 19 at $\sim$13.2 mag in the V band, with a quiescent magnitude of V$>$17.6. | background 0.97 | 0.06 | 0.06 | hedged possibility 0.98 |
| s1 | Here we report on the follow-up photometry using the {\it Neil Gehrels Swift Observatory}. | contribution 0.69 | 0.92 | 0.04 | asserted 0.91 |
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The paper
Original abstract
The All Sky Automated Survey for SuperNovae (ASAS-SN) reported a possible Galactic dwarf nova ASASSN-18fs on 2018 March 19 at $\sim$13.2 mag in the V band, with a quiescent magnitude of V$>$17.6. Here we report on the follow-up photometry using the {\it Neil Gehrels Swift Observatory}.
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