Swift-XRT Follow-up of Gravitational-wave Triggers in the Second Advanced LIGO/Virgo Observing Run Article Swipe
N. J. Klingler
,
J. A. Kennea
,
P. A. Evans
,
A. Tohuvavohu
,
S. B. Cenko
,
S. D. Barthelmy
,
A. P. Beardmore
,
A. A. Breeveld
,
P. J. Brown
,
D. N. Burrows
,
S. Campana
,
G. Cusumano
,
A. D’Aì
,
P. D’Avanzo
,
V. D’Elia
,
M. de Pasquale
,
S. W. K. Emery
,
Javier A. García
,
P. Giommi
,
C. Gronwall
,
D. H. Hartmann
,
H. A. Krimm
,
N. P. M. Kuin
,
A. Y. Lien
,
D. Malesani
,
F. E. Marshall
,
A. Melandri
,
J. A. Nousek
,
S. R. Oates
,
P. T. O’Brien
,
J. P. Osborne
,
K. L. Page
,
D. M. Palmer
,
M. Perri
,
J. L. Racusin
,
M. H. Siegel
,
T. Sakamoto
,
B. Sbarufatti
,
G. Tagliaferri
,
E. Troja
·
YOU?
·
· 2019
· Open Access
·
· DOI: https://doi.org/10.3847/1538-4365/ab4ea2
YOU?
·
· 2019
· Open Access
·
· DOI: https://doi.org/10.3847/1538-4365/ab4ea2
The Neil Gehrels Swift Observatory carried out prompt searches for gravitational-wave (GW) events detected by the LIGO/Virgo Collaboration (LVC) during the second observing run (“O2”). Swift performed extensive tiling of eight LVC triggers, two of which had very low false-alarm rates (GW170814 and the epochal GW170817), indicating a high confidence of being astrophysical in origin; the latter was the first GW event to have an electromagnetic counterpart detected. In this paper we describe the follow-up performed during O2 and the results of our searches. No GW electromagnetic counterparts were detected; this result is expected, as GW170817 remained the only astrophysical event containing at least one neutron star after LVC’s later retraction of some events. A number of X-ray sources were detected, with the majority of identified sources being active galactic nuclei. We discuss the detection rate of transient X-ray sources and their implications in the O2 tiling searches. Finally, we describe the lessons learned during O2 and how these are being used to improve the Swift follow-up of GW events. In particular, we simulate a population of gamma-ray burst afterglows to evaluate our source ranking system’s ability to differentiate them from unrelated and uncataloged X-ray sources. We find that ≈60%–70% of afterglows whose jets are oriented toward Earth will be given high rank (i.e., “interesting” designation) by the completion of our second follow-up phase (assuming that their location in the sky was observed), but that this fraction can be increased to nearly 100% by performing a third follow-up observation of sources exhibiting fading behavior.
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- Type
- article
- Language
- en
- Landing Page
- https://doi.org/10.3847/1538-4365/ab4ea2
- https://iopscience.iop.org/article/10.3847/1538-4365/ab4ea2/pdf
- OA Status
- bronze
- Cited By
- 19
- References
- 88
- Related Works
- 10
- OpenAlex ID
- https://openalex.org/W2985582156
All OpenAlex metadata
Raw OpenAlex JSON
- OpenAlex ID
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https://openalex.org/W2985582156Canonical identifier for this work in OpenAlex
- DOI
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https://doi.org/10.3847/1538-4365/ab4ea2Digital Object Identifier
- Title
-
Swift-XRT Follow-up of Gravitational-wave Triggers in the Second Advanced LIGO/Virgo Observing RunWork title
- Type
-
articleOpenAlex work type
- Language
-
enPrimary language
- Publication year
-
2019Year of publication
- Publication date
-
2019-11-01Full publication date if available
- Authors
-
N. J. Klingler, J. A. Kennea, P. A. Evans, A. Tohuvavohu, S. B. Cenko, S. D. Barthelmy, A. P. Beardmore, A. A. Breeveld, P. J. Brown, D. N. Burrows, S. Campana, G. Cusumano, A. D’Aì, P. D’Avanzo, V. D’Elia, M. de Pasquale, S. W. K. Emery, Javier A. García, P. Giommi, C. Gronwall, D. H. Hartmann, H. A. Krimm, N. P. M. Kuin, A. Y. Lien, D. Malesani, F. E. Marshall, A. Melandri, J. A. Nousek, S. R. Oates, P. T. O’Brien, J. P. Osborne, K. L. Page, D. M. Palmer, M. Perri, J. L. Racusin, M. H. Siegel, T. Sakamoto, B. Sbarufatti, G. Tagliaferri, E. TrojaList of authors in order
- Landing page
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https://doi.org/10.3847/1538-4365/ab4ea2Publisher landing page
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https://iopscience.iop.org/article/10.3847/1538-4365/ab4ea2/pdfDirect link to full text PDF
- Open access
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YesWhether a free full text is available
- OA status
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bronzeOpen access status per OpenAlex
- OA URL
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https://iopscience.iop.org/article/10.3847/1538-4365/ab4ea2/pdfDirect OA link when available
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LIGO, Swift, Gravitational wave, Physics, Astronomy, AstrophysicsTop concepts (fields/topics) attached by OpenAlex
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19Total citation count in OpenAlex
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2025: 1, 2024: 2, 2023: 1, 2022: 7, 2021: 5Per-year citation counts (last 5 years)
- References (count)
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88Number of works referenced by this work
- Related works (count)
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10Other works algorithmically related by OpenAlex
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