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Protecting stable biological nomenclatural systems enables universal communication: A collective international appeal

Jiménez-Mejías, Pedro ; Manzano, Saúl ; Gowda, Vinita ; [et al.]

Oxford University Press (OUP) ; 2024

In: BioScience ( 2024-06-19)

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In: BioScience, Oxford University Press (OUP), ( 2024-06-19)

Abstract: The fundamental value of universal nomenclatural systems in biology is that they enable unambiguous scientific communication. However, the stability of these systems is threatened by recent discussions asking for a fairer nomenclature, raising the possibility of bulk revision processes for “inappropriate” names. It is evident that such proposals come from very deep feelings, but we show how they can irreparably damage the foundation of biological communication and, in turn, the sciences that depend on it. There are four essential consequences of objective codes of nomenclature: universality, stability, neutrality, and transculturality. These codes provide fair and impartial guides to the principles governing biological nomenclature and allow unambiguous universal communication in biology. Accordingly, no subjective proposals should be allowed to undermine them.

Type of Medium: Online Resource

ISSN: 0006-3568 , 1525-3244

URL: Article

DOI: 10.1093/biosci/biae043

RVK:

WA 15000

Language: English

Publisher: Oxford University Press (OUP)

Publication Date: 2024

detail.hit.zdb_id: 2066019-4

SSG: 12

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Measurement of the mean central optical depth of galaxy clusters via the pairwise kinematic Sunyaev-Zel’dovich effect with SPT-3G and DES

Schiappucci, E. ; Bianchini, F. ; Aguena, M. ; [et al.]

American Physical Society (APS) ; 2023

In: Physical Review D Vol. 107, No. 4 ( 2023-2-21)

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In: Physical Review D, American Physical Society (APS), Vol. 107, No. 4 ( 2023-2-21)

Type of Medium: Online Resource

ISSN: 2470-0010 , 2470-0029

URL: Article

DOI: 10.1103/PhysRevD.107.042004

Language: English

Publisher: American Physical Society (APS)

Publication Date: 2023

detail.hit.zdb_id: 2844732-3

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Measurements of the E -mode polarization and temperature- E -mode correlation of the CMB from SPT-3G 2018 data

Dutcher, D. ; Balkenhol, L. ; Ade, P. A. R. ; [et al.]

American Physical Society (APS) ; 2021

In: Physical Review D Vol. 104, No. 2 ( 2021-7-13)

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In: Physical Review D, American Physical Society (APS), Vol. 104, No. 2 ( 2021-7-13)

Type of Medium: Online Resource

ISSN: 2470-0010 , 2470-0029

URL: Article

DOI: 10.1103/PhysRevD.104.022003

Language: English

Publisher: American Physical Society (APS)

Publication Date: 2021

detail.hit.zdb_id: 2844732-3

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Right on track? Performance of satellite telemetry in terrestrial wildlife research

Hofman, M. P. G. ; Hayward, M. W. ; Heim, M. ; [et al.]

Public Library of Science (PLoS) ; 2019

In: PLOS ONE Vol. 14, No. 5 ( 2019-5-9), p. e0216223-

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In: PLOS ONE, Public Library of Science (PLoS), Vol. 14, No. 5 ( 2019-5-9), p. e0216223-

Type of Medium: Online Resource

ISSN: 1932-6203

URL: Article

DOI: 10.1371/journal.pone.0216223

DOI: 10.1371/journal.pone.0216223.g001

DOI: 10.1371/journal.pone.0216223.g002

DOI: 10.1371/journal.pone.0216223.g003

DOI: 10.1371/journal.pone.0216223.g004

DOI: 10.1371/journal.pone.0216223.g005

DOI: 10.1371/journal.pone.0216223.g006

DOI: 10.1371/journal.pone.0216223.t001

DOI: 10.1371/journal.pone.0216223.t002

DOI: 10.1371/journal.pone.0216223.t003

DOI: 10.1371/journal.pone.0216223.s001

DOI: 10.1371/journal.pone.0216223.s002

DOI: 10.1371/journal.pone.0216223.s003

DOI: 10.1371/journal.pone.0216223.s004

DOI: 10.1371/journal.pone.0216223.s005

DOI: 10.1371/journal.pone.0216223.s006

DOI: 10.1371/journal.pone.0216223.s007

DOI: 10.1371/journal.pone.0216223.s008

DOI: 10.1371/journal.pone.0216223.s009

DOI: 10.1371/journal.pone.0216223.s010

DOI: 10.1371/journal.pone.0216223.s011

DOI: 10.1371/journal.pone.0216223.s012

DOI: 10.1371/journal.pone.0216223.s013

Language: English

Publisher: Public Library of Science (PLoS)

Publication Date: 2019

detail.hit.zdb_id: 2267670-3

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Asteroid Measurements at Millimeter Wavelengths with the South Pole Telescope

Chichura, P. M. ; Foster, A. ; Patel, C. ; [et al.]

American Astronomical Society ; 2022

In: The Astrophysical Journal Vol. 936, No. 2 ( 2022-09-01), p. 173-

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In: The Astrophysical Journal, American Astronomical Society, Vol. 936, No. 2 ( 2022-09-01), p. 173-

Abstract: We present the first measurements of asteroids in millimeter wavelength data from the South Pole Telescope (SPT), which is used primarily to study the cosmic microwave background (CMB). We analyze maps of two ∼270 deg 2 sky regions near the ecliptic plane, each observed with the SPTpol camera ∼100 times over 1 month. We subtract the mean of all maps of a given field, removing static sky signal, and then average the mean-subtracted maps at known asteroid locations. We detect three asteroids—(324) Bamberga, (13) Egeria, and (22) Kalliope—with signal-to-noise ratios (S/N) of 11.2, 10.4, and 6.1, respectively, at 2.0 mm (150 GHz); we also detect (324) Bamberga with an S/N of 4.1 at 3.2 mm (95 GHz). We place constraints on these asteroids’ effective emissivities, brightness temperatures, and light-curve modulation amplitude. Our flux density measurements of (324) Bamberga and (13) Egeria roughly agree with predictions, while our measurements of (22) Kalliope suggest lower flux, corresponding to effective emissivities of 0.64 ± 0.11 at 2.0 and 〈 0.47 at 3.2 mm. We predict the asteroids detectable in other SPT data sets and find good agreement with detections of (772) Tanete and (1093) Freda in recent data from the SPT-3G camera, which has ∼10× the mapping speed of SPTpol. This work is the first focused analysis of asteroids in data from CMB surveys, and it demonstrates we can repurpose historic and future data sets for asteroid studies. Future SPT measurements can help constrain the distribution of surface properties over a larger asteroid population.

Type of Medium: Online Resource

ISSN: 0004-637X , 1538-4357

URL: Article

DOI: 10.3847/1538-4357/ac89ec

RVK:

UA 1000

Language: Unknown

Publisher: American Astronomical Society

Publication Date: 2022

detail.hit.zdb_id: 2207648-7

detail.hit.zdb_id: 1473835-1

SSG: 16,12

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Detection of Galactic and Extragalactic Millimeter-wavelength Transient Sources with SPT-3G

Guns, S. ; Foster, A. ; Daley, C. ; [et al.]

American Astronomical Society ; 2021

In: The Astrophysical Journal Vol. 916, No. 2 ( 2021-08-01), p. 98-

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In: The Astrophysical Journal, American Astronomical Society, Vol. 916, No. 2 ( 2021-08-01), p. 98-

Type of Medium: Online Resource

ISSN: 0004-637X , 1538-4357

URL: Article

DOI: 10.3847/1538-4357/ac06a3

RVK:

UA 1000

Language: Unknown

Publisher: American Astronomical Society

Publication Date: 2021

detail.hit.zdb_id: 2207648-7

detail.hit.zdb_id: 1473835-1

SSG: 16,12

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The Design and Integrated Performance of SPT-3G

Sobrin, J. A. ; Anderson, A. J. ; Bender, A. N. ; [et al.]

American Astronomical Society ; 2022

In: The Astrophysical Journal Supplement Series Vol. 258, No. 2 ( 2022-02-01), p. 42-

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In: The Astrophysical Journal Supplement Series, American Astronomical Society, Vol. 258, No. 2 ( 2022-02-01), p. 42-

Abstract: SPT-3G is the third survey receiver operating on the South Pole Telescope dedicated to high-resolution observations of the cosmic microwave background (CMB). Sensitive measurements of the temperature and polarization anisotropies of the CMB provide a powerful data set for constraining cosmology. Additionally, CMB surveys with arcminute-scale resolution are capable of detecting galaxy clusters, millimeter-wave bright galaxies, and a variety of transient phenomena. The SPT-3G instrument provides a significant improvement in mapping speed over its predecessors, SPT-SZ and SPTpol. The broadband optics design of the instrument achieves a 430 mm diameter image plane across observing bands of 95, 150, and 220 GHz, with 1.2′ FWHM beam response at 150 GHz. In the receiver, this image plane is populated with 2690 dual-polarization, trichroic pixels (∼16,000 detectors) read out using a 68× digital frequency-domain multiplexing readout system. In 2018, SPT-3G began a multiyear survey of 1500 deg 2 of the southern sky. We summarize the unique optical, cryogenic, detector, and readout technologies employed in SPT-3G, and we report on the integrated performance of the instrument.

Type of Medium: Online Resource

ISSN: 0067-0049 , 1538-4365

URL: Article

DOI: 10.3847/1538-4365/ac374f

RVK:

UA 1000

Language: Unknown

Publisher: American Astronomical Society

Publication Date: 2022

detail.hit.zdb_id: 2006860-8

detail.hit.zdb_id: 2207650-5

SSG: 16,12

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Searching for anisotropic cosmic birefringence with polarization data from SPTpol

Bianchini, F. ; Wu, W. L. K. ; Ade, P. A. R. ; [et al.]

American Physical Society (APS) ; 2020

In: Physical Review D Vol. 102, No. 8 ( 2020-10-2)

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In: Physical Review D, American Physical Society (APS), Vol. 102, No. 8 ( 2020-10-2)

Type of Medium: Online Resource

ISSN: 2470-0010 , 2470-0029

URL: Article

DOI: 10.1103/PhysRevD.102.083504

Language: English

Publisher: American Physical Society (APS)

Publication Date: 2020

detail.hit.zdb_id: 2844732-3

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Improving Cosmological Constraints from Galaxy Cluster Number Counts with CMB-cluster-lensing Data: Results from the SPT-SZ Survey and Forecasts for the Future

Chaubal, P. S. ; Reichardt, C. L. ; Gupta, N. ; [et al.]

American Astronomical Society ; 2022

In: The Astrophysical Journal Vol. 931, No. 2 ( 2022-06-01), p. 139-

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In: The Astrophysical Journal, American Astronomical Society, Vol. 931, No. 2 ( 2022-06-01), p. 139-

Abstract: We show the improvement to cosmological constraints from galaxy cluster surveys with the addition of cosmic microwave background (CMB)-cluster lensing data. We explore the cosmological implications of adding mass information from the 3.1 σ detection of gravitational lensing of the CMB by galaxy clusters to the Sunyaev–Zel’dovich (SZ) selected galaxy cluster sample from the 2500 deg 2 SPT-SZ survey and targeted optical and X-ray follow-up data. In the ΛCDM model, the combination of the cluster sample with the Planck power spectrum measurements prefers σ 8 Ω m / 0.3 0.5 = 0.831 ± 0.020 . Adding the cluster data reduces the uncertainty on this quantity by a factor of 1.4, which is unchanged whether the 3.1 σ CMB-cluster lensing measurement is included or not. We then forecast the impact of CMB-cluster lensing measurements with future cluster catalogs. Adding CMB-cluster lensing measurements to the SZ cluster catalog of the ongoing SPT-3G survey is expected to improve the expected constraint on the dark energy equation of state w by a factor of 1.3 to σ ( w ) = 0.19. We find the largest improvements from CMB-cluster lensing measurements to be for σ 8 , where adding CMB-cluster lensing data to the cluster number counts reduces the expected uncertainty on σ 8 by respective factors of 2.4 and 3.6 for SPT-3G and CMB-S4.

Type of Medium: Online Resource

ISSN: 0004-637X , 1538-4357

URL: Article

DOI: 10.3847/1538-4357/ac6a55

RVK:

UA 1000

Language: Unknown

Publisher: American Astronomical Society

Publication Date: 2022

detail.hit.zdb_id: 2207648-7

detail.hit.zdb_id: 1473835-1

SSG: 16,12

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Constraints on Λ CDM extensions from the SPT-3G 2018 E E and T E power spectra

Balkenhol, L. ; Dutcher, D. ; Ade, P. A. R. ; [et al.]

American Physical Society (APS) ; 2021

In: Physical Review D Vol. 104, No. 8 ( 2021-10-4)

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In: Physical Review D, American Physical Society (APS), Vol. 104, No. 8 ( 2021-10-4)

Type of Medium: Online Resource

ISSN: 2470-0010 , 2470-0029

URL: Article

DOI: 10.1103/PhysRevD.104.083509

Language: English

Publisher: American Physical Society (APS)

Publication Date: 2021

detail.hit.zdb_id: 2844732-3

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