| 单词 | bolometric |
| 例句 | We determined the points on the bolometric light curve at epochs when K-band or ultraviolet observations were available. A kilonova as the electromagnetic counterpart to a gravitational-wave source : Nature : Nature Research 2017-10-15T04:00:00Z We compare the individual band magnitudes from this fit, using the bolometric corrections supplied by the model and find that they are redder than the observations. Optical emission from a kilonova following a gravitational-wave-detected neutron-star merger : Nature : Nature Research 2017-10-15T04:00:00Z Therefore this is a robust result independent of any time-varying bolometric correction. Corrigendum: Slowly fading super-luminous supernovae that are not pair-instability explosions : Nature : Nature Research 2016-10-04T04:00:00Z Its visible portion covers a range of about one octave; bolometric indications already in 1884 comprised between three and four. A Popular History of Astronomy During the Nineteenth Century Fourth Edition The numerical models were tailored to fit Vriw bands, but not the g band, which is driving the high bolometric luminosity at early times. Optical emission from a kilonova following a gravitational-wave-detected neutron-star merger : Nature : Nature Research 2017-10-15T04:00:00Z Thus, their contribution to the bolometric light curve is largely proportional to their masses. A kilonova as the electromagnetic counterpart to a gravitational-wave source : Nature : Nature Research 2017-10-15T04:00:00Z The numerical models were tailored to fit Vriw bands, but not the g band, which is driving the high bolometric luminosity at early times. Optical emission from a kilonova following a gravitational-wave-detected neutron-star merger : Nature : Nature Research 2017-10-15T04:00:00Z The parameters of our magnetar-powered fit to the corrected bolometric light curve shown in Fig. Corrigendum: Slowly fading super-luminous supernovae that are not pair-instability explosions : Nature : Nature Research 2016-10-04T04:00:00Z It is important to note that the large discrepancy compared to pair-instability models does not rely solely on bolometric comparisons: the difference was clearly apparent in the r-band light curves in our original Fig. Corrigendum: Slowly fading super-luminous supernovae that are not pair-instability explosions : Nature : Nature Research 2016-10-04T04:00:00Z To construct the bolometric light curve, we transformed the Swift data into Vega magnitudes, and then converted all photometry to fluxes. Corrigendum: Slowly fading super-luminous supernovae that are not pair-instability explosions : Nature : Nature Research 2016-10-04T04:00:00Z These reddening corrections were applied to the photometry to calculate absolute magnitudes and bolometric luminosities. A kilonova as the electromagnetic counterpart to a gravitational-wave source : Nature : Nature Research 2017-10-15T04:00:00Z This allows us to match the per-band light curves, rather than the bolometric luminosity. Optical emission from a kilonova following a gravitational-wave-detected neutron-star merger : Nature : Nature Research 2017-10-15T04:00:00Z If anything, the improved bolometric light curve strengthens our main conclusion—that PTF 12dam was not a pair-instability supernova—because the brighter light curve peak results in an even steeper rise to maximum. Corrigendum: Slowly fading super-luminous supernovae that are not pair-instability explosions : Nature : Nature Research 2016-10-04T04:00:00Z Here we present updated figures and model fits with the correct bolometric luminosity. Corrigendum: Slowly fading super-luminous supernovae that are not pair-instability explosions : Nature : Nature Research 2016-10-04T04:00:00Z |
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