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Journal articles on the topic 'Census, 1532'

Author: Grafiati

Published: 28 July 2024

Last updated: 31 July 2025

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1

Martín Humanes, José María. "Reses, pastos y tributos en la Banda Morisca. Las cifras del padrón de las yerbas de Morón de la Frontera (1532)." Historia. Instituciones. Documentos, no. 48 (2021): 285–317. http://dx.doi.org/10.12795/hid.2021.i48.10.

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La presente contribución analiza el conjunto de datos ofrecidos por el padrón de las yerbas de Morón de la Frontera (1532), cuya edición vio la luz en esta misma revista en 2017 bajo el título “Ganadería y fiscalidad en la Banda Morisca: los primeros condes de Ureña y el padrón de las yerbas de Morón de la Frontera (1532)” (2017, n. 44). Fruto de los avances de esta investigación, este artículo estudia y edita también la conocida capitulación de la yerba, ordenanza que complementa a dicho padrón ganadero y que elaborada por los concejos de Morón de la Frontera, Arahal y la Casa de Osuna, venía

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Katz, Paul R., Jurgis Karuza, John Kolassa, and Alan Hutson. "Medical Practice with Nursing Home Residents: Results from the National Physician Professional Activities Census." Journal of the American Geriatrics Society 45, no. 8 (1997): 911–17. http://dx.doi.org/10.1111/j.1532-5415.1997.tb02958.x.

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Wilkinson, Tim J., and Richard Sainsbury. "A Census-Based Comparison of Centenarians in New Zealand with Those in the United States." Journal of the American Geriatrics Society 46, no. 4 (1998): 488–91. http://dx.doi.org/10.1111/j.1532-5415.1998.tb02472.x.

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Skovgaard-Petersen, Karen. "Censur og Manipulation – Om et forandret årstal i Robert Estiennes bibel fra 1532." Magasin fra Det Kongelige Bibliotek 16, no. 1 (2003): 43–53. http://dx.doi.org/10.7146/mag.v16i1.66506.

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Webb, C. C. "A Census of York Clergy? The Clerical Subsidy of 1523-1528." Studies in Church History. Subsidia 12 (1999): 257–93. http://dx.doi.org/10.1017/s0143045900002532.

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Thanks to the work of Claire Cross and others, the multiplicity of sources available for the study of early sixteenth-century clergy has been used to yield information about many facets of clerical lives and careers. One source, however, has hitherto been largely neglected. The clerical subsidy of 1523-8 has, despite some printed versions for some places having been available for many years, been overshadowed by the Valor ecclesiasticus. This essay will try to show, from evidence relating to York City, that the subsidy was an important precursor to the Valor, and that, combined with other sour

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6

Heleniak, Timothy. "The 2002 Census in Russia: Preliminary Results." Eurasian Geography and Economics 44, no. 6 (2003): 430–42. http://dx.doi.org/10.2747/1538-7216.44.6.430.

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7

Astorri, Paolo. "Early Modern Lutheran Theologians and the Redeemable Census." Studia Historica: Historia Moderna 44, no. 1 (2022): 53–76. http://dx.doi.org/10.14201/shhmo20224415376.

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In sixteenth-century Germany, a particular financial operation called widerkaufflicher Zins or five percent contract sparked massive legal and theological controversies. This contract produced effects like a loan and therefore countered the interest-taking prohibition. Martin Luther (1483-1546), Philipp Melanchthon (1497-1560), Johannes Brenz (1499-1570), Johannes Aepinus (1499-1553), Urbanus Rhegius (1489-1541), Martin Chemnitz (1522-1586), Aegidius Hunnius (1550-1603), and Johann Gerhard (1582-1637) addressed this issue. They ended up reformulating the prohibition on interest and mapping out

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Andrejić, Živojin. "CRKVENI ŠEMATIZAM BEOGRADSKO-SREMSKE EPARHIJE -NAHIJE BEOGRAD, ŽELEZNIK, AVALA I ZEMUN – U XVI VEKU PREMA TURSKIM KATASTARSKIM POPISIMA." Šumadijski anali 18, no. 12 (2022): 64–88. http://dx.doi.org/10.46793/sanali18.12.064a.

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According to the census from 1528-1530, Železnik had 625 households with about 4,500 residents. Belgrade nahia had 2413 households with about 17,000 inhabitants, 22000 in total with the city of Belgrade. Nahia Zemun, in 1546, had 343 households with about 2400 inhabitants. In the middle of the 16th century, in 246 villages and 4 towns, the Belgrade Eparchy had 34 churches, 38 priests, and 7 monasteries in four nahias. There are 4 permanent and weekly squares, and a total of 40 mezras and 49 mills. Nahia Zemun does not have them on the list. The city of Belgrade in 1536 had 79 Muslim homes, 4 m

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Yin, Jia, Zhiwei Chen, Rolf Chini, et al. "Census of Variable Stars toward Serpens Main." Astronomical Journal 162, no. 2 (2021): 52. http://dx.doi.org/10.3847/1538-3881/abfdcd.

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Pallanca, Cristina, Giacomo Beccari, Francesco R. Ferraro, Luca Pasquini, Barbara Lanzoni та Alessio Mucciarelli. "A Complete Census of HαEmitters in NGC 6397". Astrophysical Journal 845, № 1 (2017): 4. http://dx.doi.org/10.3847/1538-4357/aa7ca6.

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11

Deepak, Saloni, J. Christopher Howk, Nicolas Lehner, and Céline Péroux. "A Global Census of Metals in the Universe." Astrophysical Journal 987, no. 2 (2025): 199. https://doi.org/10.3847/1538-4357/add732.

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Abstract We present a census of the mass density of metals and their evolution with cosmic time on a global scale throughout the Universe, synthesizing robust estimates of metals in stars, hot intracluster gas, and gaseous absorbers tracing neutral gas as well as ionized gas in the circumgalactic and intergalactic media. We observe an order of magnitude increase in the stellar metal mass density from z ∼ 2.5 to 0.7, over which time stars emerge as the most important metal reservoir at low redshifts, housing ∼30% of the total expected metal density at z ∼ 0.1. Hot virialized intracluster/intrag

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Wortham, Jonathan M., Seth A. Meador, James L. Hadler, et al. "Census tract socioeconomic indicators and COVID-19-associated hospitalization rates—COVID-NET surveillance areas in 14 states, March 1–April 30, 2020." PLOS ONE 16, no. 9 (2021): e0257622. http://dx.doi.org/10.1371/journal.pone.0257622.

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Objectives Some studies suggested more COVID-19-associated hospitalizations among racial and ethnic minorities. To inform public health practice, the COVID-19-associated Hospitalization Surveillance Network (COVID-NET) quantified associations between race/ethnicity, census tract socioeconomic indicators, and COVID-19-associated hospitalization rates. Methods Using data from COVID-NET population-based surveillance reported during March 1–April 30, 2020 along with socioeconomic and denominator data from the US Census Bureau, we calculated COVID-19-associated hospitalization rates by racial/ethni

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Sonnentrucker, P., B. York, L. M. Hobbs, et al. "A Modern Census of the Broadest Diffuse Interstellar Bands." Astrophysical Journal Supplement Series 237, no. 2 (2018): 40. http://dx.doi.org/10.3847/1538-4365/aad4a5.

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Esplin, T. L., and K. L. Luhman. "A Census of Stars and Disks in Corona Australis*." Astronomical Journal 163, no. 2 (2022): 64. http://dx.doi.org/10.3847/1538-3881/ac3e64.

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Abstract We have performed a census of the young stellar populations near the Corona Australis molecular cloud using photometric and kinematic data from several sources, particularly Gaia EDR3, and spectroscopy of hundreds of candidate members. We have compiled a catalog of 393 members of Corona Australis, (39 at >M6), 293 (36) of which are spectroscopically classified for the first time in this work. We find that Corona Australis can be described in terms of two stellar populations, a younger one (a few megayears) that is partially embedded in the cloud (the Coronet Cluster) and an older o

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Thanathibodee, Thanawuth, Nuria Calvet, Jesús Hernández, Karina Maucó, and César Briceño. "A Census of the Low Accretors. I. The Catalog." Astronomical Journal 163, no. 2 (2022): 74. http://dx.doi.org/10.3847/1538-3881/ac3ee6.

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Abstract Observations have shown that the disk frequency and the fraction of accreting pre-main-sequence stars decrease with the age of the population and that some stars appear to have disks while their accretion has stopped. Still, it is unclear how disk-bearing stars stop their accretion. To provide insight into the last stages of accretion in low-mass young stars, we conducted a survey of disk-bearing stars that are thought to be non-accretors to identify stars still accreting at very low rates. Here we present the first catalog of the survey of 170 disk-bearing non-accreting stars in Cham

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Xu, Duo, Stella S. R. Offner, Robert Gutermuth, Shuo Kong, and Hector G. Arce. "A Census of Protostellar Outflows in Nearby Molecular Clouds." Astrophysical Journal 926, no. 1 (2022): 19. http://dx.doi.org/10.3847/1538-4357/ac39a0.

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Abstract We adopt the deep learning method casi-3d (Convolutional Approach to Structure Identification-3D) to systemically identify protostellar outflows in 12CO and 13CO observations of the nearby molecular clouds, Ophiuchus, Taurus, Perseus, and Orion. The total outflow masses are 267 M ⊙, 795 M ⊙, 1305 M ⊙, and 6332 M ⊙ for Ophiuchus, Taurus, Perseus, and Orion, respectively. We show the outflow mass in each cloud is linearly proportional to the total number of young stellar objects. The estimated total 3D deprojected outflow energies are 9 × 1045 erg, 6 × 1046 erg, 1.2 × 1047 erg, and 6 ×

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Luhman, K. L. "A Census of the 32 Ori Association with Gaia*." Astronomical Journal 164, no. 4 (2022): 151. http://dx.doi.org/10.3847/1538-3881/ac85e2.

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Abstract I have used high-precision photometry and astrometry from the third data release of Gaia (DR3) to identify candidate members of the 32 Ori association. Spectral types and radial velocities have been measured for subsets of the candidates using new and archival spectra. For the candidates that have radial velocity measurements, I have used UVW velocities to further constrain their membership, arriving at a final catalog of 169 candidates. I estimate that the completeness of the survey is ∼90% for spectral types of ≲M7 (≳0.06 M ⊙). The histogram of spectral types for the 32 Ori candidat

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Luhman, K. L. "A Census of the TW Hya Association with Gaia*." Astronomical Journal 165, no. 6 (2023): 269. http://dx.doi.org/10.3847/1538-3881/accf19.

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Abstract I have used high-precision photometry and astrometry from the third data release of Gaia to perform a survey for members of the TW Hya association (TWA). I have identified candidate members that appear to share similar kinematics and ages with bona fide members compiled by Gagné et al. (2017), and I have assessed their membership using radial velocities and spectroscopic diagnostics of age from various sources. My new catalog of adopted members contains 67 Gaia sources in 55 systems. The histogram of spectral types for TWA peaks near M5 (∼0.15 M ⊙), resembling the distributions measur

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Thanathibodee, Thanawuth, Brandon Molina, Javier Serna, et al. "A Census of the Low Accretors. II. Accretion Properties." Astrophysical Journal 944, no. 1 (2023): 90. http://dx.doi.org/10.3847/1538-4357/acac84.

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Abstract Much is known about the processes driving accretion from protoplanetary disks onto low-mass pre-main-sequence stars (T Tauri stars). Nevertheless, it is unclear how accretion stops. To determine the accretion properties and their relation to stellar properties and gain insight into the last stages of accretion, we present a detailed analysis of 24 low and possible accretors, previously identified using the He i λ10830 line. We model moderate-resolution Hα profiles of these stars using magnetospheric accretion flow models that account for the chromospheric contribution at the line cent

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Xu 徐, Yu-Jing 雨婧, Han-Long 寒龙 Peng 彭, Shan-Shan 山杉 Weng 翁, Xiao 潇. Zhang 张, and Ming-Yu 明玉 Ge 葛. "A New X-Ray Census of Rotation Powered Pulsars." Astrophysical Journal 981, no. 2 (2025): 100. https://doi.org/10.3847/1538-4357/adaebc.

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Abstract To date, over 4000 pulsars have been detected. In this study, we identify 231 X-ray counterparts of Australia Telescope National Facility (ATNF) pulsars by performing a spatial cross match across the Chandra, XMM-Newton observational catalogs. This data set represents the largest sample of X-ray counterparts ever compiled, including 98 normal pulsars (NPs) and 133 millisecond pulsars (MSPs). Based on this significantly expanded sample, we re-establish the correlation between X-ray luminosity and spin-down power, given by L X ∝ E ̇ 0.85 ± 0.05 across the whole X-ray band. The strong co

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21

Mar, Krista, Yawei Song, Khaldoun Hamade, et al. "Abstract A017: Identifying priority neighborhoods for mobile cancer screening using georeferenced data." Cancer Epidemiology, Biomarkers & Prevention 32, no. 1_Supplement (2023): A017. http://dx.doi.org/10.1158/1538-7755.disp22-a017.

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Abstract Background: Mobile screening units (MSUs) are an evidence-based approach known to reduce barriers and increase access to preventive services such as cancer screening. Less is known about how to plan and prioritize where MSUs are deployed to maximize impact and reduce the burden of disease. We used a geographic-based approach to create an index to identify which census tracts were of greatest priority for cancer screening, thereby creating a priority scoring metric for deploying the MSU across our 7-county cancer center catchment area. Methods: We assessed publicly available data repor

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22

Armentrout, W. P., L. D. Anderson, Trey V. Wenger, Dana S. Balser, and T. M. Bania. "A VLA Census of the Galactic H II Region Population." Astrophysical Journal Supplement Series 253, no. 1 (2021): 23. http://dx.doi.org/10.3847/1538-4365/abd5c0.

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23

Lee, Jongsu, C. Y. Hui, J. Takata, A. K. H. Kong, P. H. T. Tam, and K. S. Cheng. "X-Ray Census of Millisecond Pulsars in the Galactic Field." Astrophysical Journal 864, no. 1 (2018): 23. http://dx.doi.org/10.3847/1538-4357/aad284.

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24

Luhman, K. L., and T. L. Esplin. "Refining the Census of the Upper Scorpius Association with Gaia." Astronomical Journal 160, no. 1 (2020): 44. http://dx.doi.org/10.3847/1538-3881/ab9599.

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Rowland, Richard H. "National and Regional Population Trends in Tajikistan: Results from the Recent Census." Eurasian Geography and Economics 46, no. 3 (2005): 202–23. http://dx.doi.org/10.2747/1538-7216.46.3.202.

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26

Kalinowski, Steven T., and Robin S. Waples. "Relationship of Effective to Census Size in Fluctuating Populations." Conservation Biology 16, no. 1 (2002): 129–36. http://dx.doi.org/10.1046/j.1523-1739.2002.00134.x.

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27

Leaver, Robin A., and Nicholas Temperley. "The Hymn Tune Index: A Census of English-Language Hymn Tunes in Printed Sources from 1535 to 1820." Notes 56, no. 2 (1999): 385. http://dx.doi.org/10.2307/900009.

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Fan, C. Cindy. "Population Change and Regional Development in China: Insights Based on the 2000 Census." Eurasian Geography and Economics 43, no. 6 (2002): 425–42. http://dx.doi.org/10.2747/1538-7216.43.6.425.

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Rowland, Richard H. "National and Regional Population Trends in Ukraine: Results from the Most Recent Census." Eurasian Geography and Economics 45, no. 7 (2004): 491–514. http://dx.doi.org/10.2747/1538-7216.45.7.491.

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Winston, Victor H. "Observations on the Population of Vilnius: The Grim Years and the 1942 Census." Eurasian Geography and Economics 47, no. 2 (2006): 176–203. http://dx.doi.org/10.2747/1538-7216.47.2.176.

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Sardone, Amy, D. J. Pisano, N. M. Pingel, A. Sorgho, Claude Carignan, and W. J. G. de Blok. "A Census of the Extended Neutral Hydrogen around 18 MHONGOOSE Galaxies." Astrophysical Journal 910, no. 1 (2021): 69. http://dx.doi.org/10.3847/1538-4357/abde45.

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McGuire, Brett A. "2018 Census of Interstellar, Circumstellar, Extragalactic, Protoplanetary Disk, and Exoplanetary Molecules." Astrophysical Journal Supplement Series 239, no. 2 (2018): 17. http://dx.doi.org/10.3847/1538-4365/aae5d2.

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Sohn, Jubee, Margaret J. Geller, and H. Jabran Zahid. "A Spectroscopic Census of X-Ray Systems in the COSMOS Field." Astrophysical Journal 880, no. 2 (2019): 142. http://dx.doi.org/10.3847/1538-4357/ab2b46.

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Luhman, K. L. "A Census of the Stellar Populations in the Sco-Cen Complex*." Astronomical Journal 163, no. 1 (2021): 24. http://dx.doi.org/10.3847/1538-3881/ac35e2.

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Abstract I have used high-precision photometry and astrometry from the early installment of the third data release of Gaia (EDR3) to perform a survey for members of the stellar populations within the Sco-Cen complex, which consist of Upper Sco, UCL/LCC, the V1062 Sco group, Ophiuchus, and Lupus. Among Gaia sources with σ π < 1 mas, I have identified 10,509 candidate members of those populations. I have compiled previous measurements of spectral types, Li equivalent widths, and radial velocities for the candidates, which are available for 3169, 1420, and 1740 objects, respectively. In a subs

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Garner, Ray, J. Christopher Mihos, Paul Harding, and Aaron E. Watkins. "A Deep Census of Outlying Star Formation in the M101 Group." Astrophysical Journal 915, no. 1 (2021): 57. http://dx.doi.org/10.3847/1538-4357/ac0055.

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McGuire, Brett A. "2021 Census of Interstellar, Circumstellar, Extragalactic, Protoplanetary Disk, and Exoplanetary Molecules." Astrophysical Journal Supplement Series 259, no. 2 (2022): 30. http://dx.doi.org/10.3847/1538-4365/ac2a48.

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Abstract To date, 241 individual molecular species, composed of 19 different elements, have been detected in the interstellar and circumstellar medium by astronomical observations. These molecules range in size from two atoms to 70 and have been detected across the electromagnetic spectrum from centimeter wavelengths to the ultraviolet. This census presents a summary of the first detection of each molecular species, including the observational facility, wavelength range, transitions, and enabling laboratory spectroscopic work, as well as listing tentative and disputed detections. Tables of mol

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Davis, Brian D., Howard E. Bond, Michael H. Siegel, and Robin Ciardullo. "A Census of Above-horizontal-branch Stars in Galactic Globular Clusters*." Astrophysical Journal 926, no. 1 (2022): 99. http://dx.doi.org/10.3847/1538-4357/ac4224.

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Abstract We have carried out a search for above-horizontal-branch (AHB) stars—objects lying above the horizontal branch (HB) and blueward of the asymptotic giant branch (AGB) in the color–magnitude diagram—in 97 Galactic and seven Magellanic Cloud globular clusters (GCs). We selected AHB candidates based on photometry in the uBVI system, which is optimized for detection of low-surface-gravity stars with large Balmer jumps, in the color range −0.05 ≤ (B − V)0 ≤1.0. We then used Gaia astrometry and Gaussian-mixture modeling to confirm cluster membership and remove field interlopers. Our final ca

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Sohn, Jubee, Margaret J. Geller, H. Jabran Zahid, and Daniel G. Fabricant. "A Complete Spectroscopic Census of A2029: A Tale of Three Histories." Astrophysical Journal 872, no. 2 (2019): 192. http://dx.doi.org/10.3847/1538-4357/ab0213.

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Pucha, Ragadeepika, S. Juneau, Arjun Dey, et al. "Tripling the Census of Dwarf AGN Candidates Using DESI Early Data." Astrophysical Journal 982, no. 1 (2025): 10. https://doi.org/10.3847/1538-4357/adb1dd.

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Abstract Using early data from the Dark Energy Spectroscopic Instrument (DESI) survey, we search for active galactic nuclei (AGN) signatures in 410,757 line-emitting galaxies. By employing the BPT emission-line ratio diagnostic diagram, we identify AGNs in 75,928/296,261 (≈25.6%) high-mass ( log ( M ⋆ / M ⊙ ) > 9.5) and 2444/114,496 (≈2.1%) dwarf ( log ( M ⋆ / M ⊙ ) ≤ 9.5) galaxies. Of these AGN candidates, 4181 sources exhibit a broad Hα component, allowing us to estimate their BH masses via virial techniques. This study more than triples the census of dwarf AGNs and doubles the number of

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Xuan, Zherui, and Jennifer Cullen. "Abstract B092: Area-level socioeconomic influences on rates of cervical and colon cancer screenings." Cancer Epidemiology, Biomarkers & Prevention 32, no. 12_Supplement (2023): B092. http://dx.doi.org/10.1158/1538-7755.disp23-b092.

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Abstract Introduction and Study Purpose: Cancer screening is one of the most important preventive modifiers of cancer outcome. The general correlation between negative socioeconomic influences (SEIs) and poorer cancer screening rates is known. However, variations on SEI correlation with cancer screening need to be confirmed at a smaller local level since there could be significant local variations. CDC PLACES is a high resolution dataset that provides data on cancer screening rates at a census tract level with coverage across the US. It is made up of small area estimates constructed with demog

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Rowland, Richard H. "National and Regional Population Trends in Georgia, 1989-2002: Results from the 2002 Census." Eurasian Geography and Economics 47, no. 2 (2006): 221–42. http://dx.doi.org/10.2747/1538-7216.47.2.221.

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Rowland, Richard H. "Recent Demographic Trends in Armenia: Results of the 2001 Census and Update to 2006." Eurasian Geography and Economics 48, no. 1 (2007): 73–94. http://dx.doi.org/10.2747/1538-7216.48.1.73.

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Rowland, Richard H. "Population Trends in Europe's Poorest Country: Results of the Most Recent Census of Moldova." Eurasian Geography and Economics 50, no. 4 (2009): 480–95. http://dx.doi.org/10.2747/1539-7216.50.3.480.

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Akras, Stavros, Lizette Guzman-Ramirez, Marcelo L. Leal-Ferreira, and Gerardo Ramos-Larios. "A Census of Symbiotic Stars in the 2MASS, WISE , and Gaia Surveys." Astrophysical Journal Supplement Series 240, no. 2 (2019): 21. http://dx.doi.org/10.3847/1538-4365/aaf88c.

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Winston, Elaine, Joseph Hora, Robert Gutermuth, and Volker Tolls. "A Census of Star Formation in the Outer Galaxy: The SMOG Field." Astrophysical Journal 880, no. 1 (2019): 9. http://dx.doi.org/10.3847/1538-4357/ab27c8.

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Luhman, K. L. "A Census of the Circumstellar Disk Populations in the Sco-Cen Complex*." Astronomical Journal 163, no. 1 (2021): 25. http://dx.doi.org/10.3847/1538-3881/ac35e3.

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Abstract I have used mid-infrared (IR) photometry from the Wide-field Infrared Survey Explorer (WISE) to perform a census of circumstellar disks among ∼10,000 candidate members of the Sco-Cen complex that were recently identified with data from the Gaia mission. IR excesses are detected for more than 1200 of the WISE counterparts that are within the commonly adopted boundary for Sco-Cen, ∼400 of which are newly reported in this work. The richest population in Sco-Cen, UCL/LCC, contains the largest available sample of disks (>500) for any population near its age (∼20 Myr). UCL/LCC also provi

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Conroy, Charlie, Jay Strader, Pieter van Dokkum, et al. "A Complete Census of Luminous Stellar Variability on Day to Decade Timescales." Astrophysical Journal 864, no. 2 (2018): 111. http://dx.doi.org/10.3847/1538-4357/aad460.

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Carlin, Jeffrey L., David J. Sand, Burçin Mutlu-Pakdil, et al. "A Census of Dwarf Galaxy Satellites around LMC-mass Galaxy NGC 2403*." Astrophysical Journal 977, no. 1 (2024): 112. https://doi.org/10.3847/1538-4357/ad8dcd.

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Abstract We present the first comprehensive census of the satellite population around a Large Magellanic Cloud stellar-mass galaxy, as part of the Magellanic Analog Dwarf Companions and Stellar Halos (MADCASH) survey. We have surveyed NGC 2403 (D = 3.0 Mpc) with the Subaru/Hyper Suprime-Cam imager out to a projected radius of 90 kpc (with partial coverage extending out to ∼110 kpc, or ∼80% of the virial radius of NGC 2403), resolving stars in the uppermost ∼2.5 mag of its red giant branch. By looking for stellar overdensities in the red giant branch spatial density map, we identify 149 satelli

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Xu, Duo, Stella S. R. Offner, Robert Gutermuth, and Jonathan C. Tan. "A Census of Outflow to Magnetic Field Orientations in Nearby Molecular Clouds." Astrophysical Journal 941, no. 1 (2022): 81. http://dx.doi.org/10.3847/1538-4357/aca153.

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Abstract We define a sample of 200 protostellar outflows showing blue- and redshifted CO emission in the nearby molecular clouds Ophiuchus, Taurus, Perseus, and Orion, to investigate the correlation between outflow orientations and local, but relatively large-scale, magnetic field directions traced by Planck 353 GHz dust polarization. At high significance (p ∼ 10−4), we exclude a random distribution of relative orientations and find that there is a preference for alignment of projected plane of sky outflow axes with magnetic field directions. The distribution of relative position angles peaks

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Goldtooth, Aaron, Ann I. Zabludoff, Sixiang Wen, Peter G. Jonker, Nicholas C. Stone, and Zheng Cao. "A Census of Archival X-Ray Spectra for Modeling Tidal Disruption Events." Publications of the Astronomical Society of the Pacific 135, no. 1045 (2023): 034101. http://dx.doi.org/10.1088/1538-3873/acb9bc.

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Abstract Tidal disruption events (TDEs) are highly energetic phenomena that occur when a star is tidally disrupted by the central massive black hole in a galaxy. Fitting the observed X-ray spectra of TDEs with a first-principles, general-relativistic slim-disk model for the emission from the inner accretion disk can constrain the black hole mass M • and dimensionless spin a •. Multiepoch spectra can break degeneracies in parameter estimation, particularly when they include a period of super-Eddington mass accretion. Even one observed super-Eddington epoch can be useful. Constraints on {M •, a

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