2018
DOI: 10.1016/j.molstruc.2018.02.034
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Photoluminescence studies on holmium (III) and praseodymium (III) doped calcium borophosphate (CBP) phosphors

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Cited by 28 publications
(9 citation statements)
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“…3 H i (i = 4, 5, 6) and 3 F j (j=2, 4) (Zhou et al, 2012;Shalapska et al, 2014;Prasad et al, 2018;Runowski et al, 2019). Prasad et al (2018) identified the 1 D 2 state to be the transition origin for the prominent Pr emission at around 600 nm as well as Gaft et al (2005), who also attributed the emission around 500 nm to the same origin. However, the observed positions lie at slightly (around 10 nm) higher emission wavelength that agree better to positions found by e.g.…”
Section: Ree Reference Spectra At 442 Nm Laser Excitationmentioning
confidence: 98%
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“…3 H i (i = 4, 5, 6) and 3 F j (j=2, 4) (Zhou et al, 2012;Shalapska et al, 2014;Prasad et al, 2018;Runowski et al, 2019). Prasad et al (2018) identified the 1 D 2 state to be the transition origin for the prominent Pr emission at around 600 nm as well as Gaft et al (2005), who also attributed the emission around 500 nm to the same origin. However, the observed positions lie at slightly (around 10 nm) higher emission wavelength that agree better to positions found by e.g.…”
Section: Ree Reference Spectra At 442 Nm Laser Excitationmentioning
confidence: 98%
“…6 and Tab. 3) corresponding to the dominant transitions described by Gaft et al (2005) The transitions originate in 3 P 0 or 3 P 1 (Zhou et al, 2012;Prasad et al, 2018;Runowski et al, 2019), where the comparison between reported and observed emission wavelength indicates that both origins are possible and the (relative)…”
Section: Ree Reference Spectra At 442 Nm Laser Excitationmentioning
confidence: 98%
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“…For HoPO 4 , the diagnostic emission line around 540 nm (e.g. Gaft et al, 2005;Qin et al, 2011;Pandey and Swart, 2016) was masked by broad-band luminescence with Ho 3+related absorptions (e.g. Turner et al, 2014;Kokaly et al, 2017) when using 325 and 442 nm laser excitation (see above).…”
Section: Ree Reference Spectra At 532 Nm Laser Excitationmentioning
confidence: 99%
“…The first, relatively weak emission line corresponds to a 5 F 5 to 5 I 8 transition (e.g. Friis et al, 2010;Qin et al, 2011;Pandey and Swart, 2016), while the second, more intense emission cluster results from a 5 F 4 / 5 S 2 to 5 I 7 transition (e.g. Qin et al, 2011;Pandey and Swart, 2016).…”
Section: Ree Reference Spectra At 532 Nm Laser Excitationmentioning
confidence: 99%