FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W3119157085> ?p ?o ?g. }

• W3119157085 endingPage "19" @default.
• W3119157085 startingPage "19" @default.
• W3119157085 abstract "Abstract The nova rate in the Milky Way remains largely uncertain, despite its vital importance in constraining models of Galactic chemical evolution as well as understanding progenitor channels for Type Ia supernovae. The rate has been previously estimated to be in the range of ≈10–300 yr −1 , either based on extrapolations from a handful of very bright optical novae or the nova rates in nearby galaxies; both methods are subject to debatable assumptions. The total discovery rate of optical novae remains much smaller (≈5–10 yr −1 ) than these estimates, even with the advent of all-sky optical time-domain surveys. Here, we present a systematic sample of 12 spectroscopically confirmed Galactic novae detected in the first 17 months of Palomar Gattini-IR (PGIR), a wide-field near-infrared time-domain survey. Operating in the J band (≈1.2 μ m), which is significantly less affected by dust extinction compared to optical bands, the extinction distribution of the PGIR sample is highly skewed to a large extinction values (>50% of events obscured by A V ≳ 5 mag). Using recent estimates for the distribution of Galactic mass and dust, we show that the extinction distribution of the PGIR sample is commensurate with dust models. The PGIR extinction distribution is inconsistent with that reported in previous optical searches (null-hypothesis probability <0.01%), suggesting that a large population of highly obscured novae have been systematically missed in previous optical searches. We perform the first quantitative simulation of a 3 π time-domain survey to estimate the Galactic nova rate using PGIR, and derive a rate of <?CDATA $approx {43.7}_{-8.7}^{+19.5}$?> <mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML overflow=scroll> <mml:mo>≈</mml:mo> <mml:msubsup> <mml:mrow> <mml:mn>43.7</mml:mn> </mml:mrow> <mml:mrow> <mml:mo>−</mml:mo> <mml:mn>8.7</mml:mn> </mml:mrow> <mml:mrow> <mml:mo>+</mml:mo> <mml:mn>19.5</mml:mn> </mml:mrow> </mml:msubsup> </mml:math> yr −1 . Our results suggest that all-sky near-infrared time-domain surveys are well poised to uncover the Galactic nova population." @default.
• W3119157085 created "2021-01-18" @default.
• W3119157085 creator A5007384804 @default.
• W3119157085 creator A5011450970 @default.
• W3119157085 creator A5017540414 @default.
• W3119157085 creator A5019618939 @default.
• W3119157085 creator A5023086549 @default.
• W3119157085 creator A5023644739 @default.
• W3119157085 creator A5025429352 @default.
• W3119157085 creator A5025879207 @default.
• W3119157085 creator A5029669315 @default.
• W3119157085 creator A5030458910 @default.
• W3119157085 creator A5030545448 @default.
• W3119157085 creator A5030997784 @default.
• W3119157085 creator A5035180093 @default.
• W3119157085 creator A5037193532 @default.
• W3119157085 creator A5043531190 @default.
• W3119157085 creator A5043629751 @default.
• W3119157085 creator A5046607536 @default.
• W3119157085 creator A5056613271 @default.
• W3119157085 creator A5058319970 @default.
• W3119157085 creator A5059864975 @default.
• W3119157085 creator A5075671855 @default.
• W3119157085 creator A5077781647 @default.
• W3119157085 creator A5078910984 @default.
• W3119157085 creator A5080115868 @default.
• W3119157085 creator A5080324654 @default.
• W3119157085 creator A5083848107 @default.
• W3119157085 creator A5087653554 @default.
• W3119157085 creator A5091335338 @default.
• W3119157085 date "2021-04-30" @default.
• W3119157085 modified "2023-10-17" @default.
• W3119157085 title "A Population of Heavily Reddened, Optically Missed Novae from Palomar Gattini-IR: Constraints on the Galactic Nova Rate" @default.
• W3119157085 cites W1623134403 @default.
• W3119157085 cites W1967092854 @default.
• W3119157085 cites W1977694174 @default.
• W3119157085 cites W1979886931 @default.
• W3119157085 cites W1984348627 @default.
• W3119157085 cites W1992789711 @default.
• W3119157085 cites W1995271373 @default.
• W3119157085 cites W2006843828 @default.
• W3119157085 cites W2010834068 @default.
• W3119157085 cites W2011301426 @default.
• W3119157085 cites W2011489977 @default.
• W3119157085 cites W2011490256 @default.
• W3119157085 cites W2011978559 @default.
• W3119157085 cites W2012282528 @default.
• W3119157085 cites W2015229441 @default.
• W3119157085 cites W2016787743 @default.
• W3119157085 cites W2020087228 @default.
• W3119157085 cites W2029343094 @default.
• W3119157085 cites W2034327354 @default.
• W3119157085 cites W2034817948 @default.
• W3119157085 cites W2037583679 @default.
• W3119157085 cites W2040357841 @default.
• W3119157085 cites W2042185285 @default.
• W3119157085 cites W2044093857 @default.
• W3119157085 cites W2049121849 @default.
• W3119157085 cites W2051997064 @default.
• W3119157085 cites W2063988638 @default.
• W3119157085 cites W2065780061 @default.
• W3119157085 cites W2067110819 @default.
• W3119157085 cites W2072481232 @default.
• W3119157085 cites W2072969507 @default.
• W3119157085 cites W2078050440 @default.
• W3119157085 cites W2082025394 @default.
• W3119157085 cites W2084488312 @default.
• W3119157085 cites W2093928930 @default.
• W3119157085 cites W2135625048 @default.
• W3119157085 cites W2163755141 @default.
• W3119157085 cites W2167635287 @default.
• W3119157085 cites W2170761363 @default.
• W3119157085 cites W2267191465 @default.
• W3119157085 cites W2274731095 @default.
• W3119157085 cites W2276541034 @default.
• W3119157085 cites W2309417010 @default.
• W3119157085 cites W2417087913 @default.
• W3119157085 cites W2485876312 @default.
• W3119157085 cites W2547328913 @default.
• W3119157085 cites W2604157616 @default.
• W3119157085 cites W2788693782 @default.
• W3119157085 cites W2791653656 @default.
• W3119157085 cites W2795732688 @default.
• W3119157085 cites W2890873809 @default.
• W3119157085 cites W2905241809 @default.
• W3119157085 cites W2905450617 @default.
• W3119157085 cites W2907948910 @default.
• W3119157085 cites W2950135604 @default.
• W3119157085 cites W2951303400 @default.
• W3119157085 cites W2951429632 @default.
• W3119157085 cites W2973796999 @default.
• W3119157085 cites W2988879082 @default.
• W3119157085 cites W2994840868 @default.
• W3119157085 cites W3000236346 @default.
• W3119157085 cites W3000717044 @default.
• W3119157085 cites W3016358123 @default.
• W3119157085 cites W3032741400 @default.
• W3119157085 cites W3090339076 @default.

• next