Keronopsamides, a New Class of Pigments from Marine Ciliates
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C-1Ј), 117.8 (d, C-4), 116.6 (d, C-6Ј), 113.6 (d, C-7), 111.1 (s, C-2),
105.1 (s, C-3Ј), 101.5 (s, C2Ј) ppm. FT-IR (neat): ν = 3420 (strong,
˜
NH and OH stretching), 1683 (strong, C=O stretching) cm–1. UV
(MeOH): λmax (ε) = 357 nm (29100 mol–1 dm3 cm–1) MALDI-TOF
(negative ion mode) HR-MS: m/z 486.8220Ϯ0.010 (calcd. for
C15H11Br3N2O2: 486.8298). ESI-MS (positive ion mode detection)
m/z: [M + H]+ [M + Na]+ and [M + K]+ as 1:3:3:1 quartets at
[4]
[5]
[6]
[7]
nominal
masses
489:491:493:495,
511:513:515:517
and
527:529:531:533, respectively. ESI-MS (negative ion mode detec-
tion) m/z: [M – H]– as 1:3:3:1 quartet at nominal masses
487:489:491:493.
Keronopsamide B (8): 1H NMR (CD3OD): δ = 7.57 (d, J1,5
=
2.1 Hz, 1 H, 1-H), 7.56 (d, 3J7,8 = 14.7 Hz, 1 H, 8-H), 7.52 (d, 3J5Ј,6Ј
= 15.8 Hz, 1 H, 5Ј-H), 7.51 (d, J4,5 = 8.5 Hz, 1 H, 4-H), 7.30 (dd,
3
J1,5 = 2.1, J4,5 = 8.5. Hz 1 H, 5-H), 7.04 (s, 1Ј-H), 6.50 (d, J5Ј,6Ј
=
3
15.8 Hz, 1 H, 6Ј-H), 6.18 (d, J7,8 = 14.7 Hz, 1 H, 7-H) ppm. UV
(MeOH): λmax (ε) = 379 nm (31000 mol–1 dm3 cm–1). ESI-MS
(negative ion mode detection) m/z: [M – H]– and [M – SO3 – H]–
as 1:3:3:1 quartets at nominal masses 567:569:571:573 and
487:489:491:493, respectively. Compound 8 afforded pure 7 when
treated in NMR tube (CD3OD) with a catalytic amount of tri-
chloroacetic acid.
[8]
[9]
3
Keronopsamide C (9): 1H NMR (CD3OD): δ = 7.56 (d, J7,8
=
[10]
14.7 Hz, 1 H, 8-H), 7.54 (d, J1,5 = 2.1 Hz, 1 H, 1-H), 7.50 (d, J4,5
= 8.5 Hz, 1 H, 4-H), 7.30 (dd, J1,5 = 2.1, J4,5 = 8.5. Hz 1 H, 5-H),
3
3
7.04 (s, 1Ј-H), 6.76 (d, J5Ј,6Ј = 12.1 Hz, 1 H, 5Ј-H), 5.75 (d, J5Ј,6Ј
3
= 12.1 Hz, 1 H, 6Ј-H), 6.18 (d, J7,8 = 14.7 Hz, 1 H, 7-H) ppm.
ESI-MS (negative ion mode detection) m/z: [M – H]– and [M –
SO3 – H]– as 1:3:3:1 quartets at nominal masses 567:569:571:573
and 487:489:491:493, respectively.
[11]
[12]
[13]
[14]
Supporting Information (see also the footnote on the first page of
this article): 400 MHz NMR (CD3COCD3) spectra of keronops-
amide A 7. 1H NMR (Figure S1), COSY full spectrum (Figure S2),
HSQC (Figure S3), HMBC (Figure S4), and NOESY (Figure S5).
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Acknowledgments
This research was supported by the Italian Department of Environ-
ment (Ministero dell’Ambiente e della Tutela del Territorio e del
Mare), projects DPN-2008-005185 and 27/02/08-21/12/07. Ad-
ditional support was provided by funds of University of Trento,
Department of Physics and University of Pisa, Department of Bio-
logy.
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