Optimal PID tuning based on slope variation approach for position control of radio telescope by Mohamad Zaber, Nursaida

“…Radio telescope is an astronomical instrument used to study radio astronomy activities including observing the celestial activities such as sun, galaxies, pulsars, stars, monitor the submillimeter wavelength and many more. …”
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Follow-up Survey for the Binary Black Hole Merger GW200224_222234 Using Subaru/HSC and GTC/OSIRIS by Takayuki Ohgami, Josefa Becerra González, Nozomu Tominaga, Tomoki Morokuma, Yousuke Utsumi, Yuu Niino, Masaomi Tanaka, Smaranika Banerjee, Frédérick Poidevin, Jose Antonio Acosta-Pulido, Ismael Pérez-Fournon, Teo Muñoz-Darias, Hiroshi Akitaya, Kenshi Yanagisawa, Mahito Sasada, Michitoshi Yoshida, Mirko Simunovic, Ryou Ohsawa, Ichi Tanaka, Tsuyoshi Terai, Yuhei Takagi, The J-GEM collaboration

“…We also performed GTC/OSIRIS spectroscopy of the probable host galaxies for five candidates; two are likely to be located within the 3D skymap, whereas the others are not. …”
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The Intrinsic Statistical Properties and Correlations of Short Gamma-Ray Bursts by Si-Yuan Zhu, Zhi-Ying Liu, Yong-Rui Shi, Xiao-Kang Ding, Wan-Peng Sun, Fu-Wen Zhang

“…We report for the first time that there is a tighter correlation between the isotropic energy of the prompt emission of SGRBs and the star formation rate of their host galaxies, which reads $\mathrm{sSFR}\propto {E}_{\mathrm{iso}}^{0.38\pm 0.11}$ . …”
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Volumetric Rates of Luminous Red Novae and Intermediate-luminosity Red Transients with the Zwicky Transient Facility by Viraj R. Karambelkar, Mansi M. Kasliwal, Nadejda Blagorodnova, Jesper Sollerman, Robert Aloisi, Shreya G. Anand, Igor Andreoni, Thomas G. Brink, Rachel Bruch, David Cook, Kaustav Kashyap Das, Kishalay De, Andrew Drake, Alexei V. Filippenko, Christoffer Fremling, George Helou, Anna Ho, Jacob Jencson, David Jones, Russ R. Laher, Frank J. Masci, Kishore C. Patra, Josiah Purdum, Alexander Reedy, Tawny Sit, Yashvi Sharma, Anastasios Tzanidakis, Stéfan J. van der Walt, Yuhan Yao, Chaoran Zhang

“…The CLU experiment spectroscopically classifies ZTF transients associated with nearby (<150 Mpc) galaxies, achieving 80% completeness for m _r < 20 mag. …”
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THE IDENTIFICATION OF z -DROPOUTS IN PAN-STARRS1: THREE QUASARS AT 6.5< z < 6.7 by Simcoe, Robert A., Chen, Shi-Fan S., Miller, Daniel Robert, Sullivan, Peter W.

“…Luminous distant quasars are unique probes of the high-redshift intergalactic medium (IGM) and of the growth of massive galaxies and black holes in the early universe. Absorption due to neutral hydrogen in the IGM makes quasars beyond a redshift of z ≃ 6.5 very faint in the optical z band, thus locating quasars at higher redshifts requires large surveys that are sensitive above 1 micron. …”
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Some Interacting Dark Energy Models by Martiros Khurshudyan, Asatur Zh. Khurshudyan

“…Using the differential age of old galaxies expressed in terms of <inline-formula> <math display="inline"> <semantics> <mrow> <mi>H</mi> <mo>(</mo> <mi>z</mi> <mo>)</mo> </mrow> </semantics> </math> </inline-formula> data, the peak position of baryonic acoustic oscillations (known as BAO data), the SN Ia data with strong gravitational lensing data, we obtain the best fit values of the model parameters for each case. …”
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Deep Search for Gamma-Ray Emission from the Accreting X-Ray Pulsar 1A 0535+262 by X. Hou, W. Zhang, D. F. Torres, L. Ji, J. Li

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Fitting Type Ia Supernova Data to a Cosmological Model Based on Einstein–Newcomb–De Sitter Space by Vladimir N. Yershov

“…De Sitter also found that in a space with constant positive curvature, spectral lines of remote galaxies would be red-shifted (called the de Sitter effect). …”
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Spectral analysis of X-ray binaries by Fridriksson, Joel Karl

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Quasi-simultaneous Optical Flux and Polarization Variability of the Binary Super Massive Black Hole Blazar OJ 287 from 2015 to 2023: Detection of an Anticorrelation in Flux and Pol... by Alok C. Gupta, Pankaj Kushwaha, Mauri J. Valtonen, Sergey S. Savchenko, Svetlana G. Jorstad, Ryo Imazawa, Paul J. Wiita, Minfeng Gu, Alan P. Marscher, Zhongli Zhang, Rumen Bachev, G. A. Borman, Haritma Gaur, T. S. Grishina, V. A. Hagen-Thorn, E. N. Kopatskaya, V. M. Larionov, E. G. Larionova, L. V. Larionova, D. A. Morozova, T. Nakaoka, A. Strigachev, Yulia V. Troitskaya, I. S. Troitsky, M. Uemura, A. A. Vasilyev, Z. R. Weaver, A. V. Zhovtan

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Confirmation of X-ray Absorption by Warm-hot Intergalactic Medium in the Sculptor Wall by Fang, Taotao, Buote, David A., Humphrey, Philip J., Canizares, Claude R., Zappacosta, Luca, Maiolino, Roberto, Tagliferri, Gianpiero, Gastaldello, Fabio

“…In a previous paper, we reported a 3σ detection of an absorption line from the warm-hot intergalactic medium (WHIM) using the Chandra and XMM X-ray grating spectra of the blazar H2356-309, the sight line of which intercepts the Sculptor Wall, a large-scale superstructure of galaxies at z ~ 0.03. To verify our initial detection, we obtained a deep (500 ks), follow-up exposure of H2356-309 as part of the Cycle-10 Chandra Large Project Program. …”
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Intermittency Scaling for Mixing and Dissipation in Rotating Stratified Turbulence at the Edge of Instability by Annick Pouquet, Duane Rosenberg, Raffaele Marino, Pablo Mininni

“…These are reminiscent of (but not identical to) previous findings for other variables and systems such as oceanic and atmospheric flows, climate re-analysis data, fusion plasmas, the Solar Wind, or galaxies. For QG forcing, sharp scaling transitions take place once the Ozmidov length scale <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><msub><mi>ℓ</mi><mrow><mi>O</mi><mi>z</mi></mrow></msub></semantics></math></inline-formula> is resolved—<inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><msub><mi>ℓ</mi><mrow><mi>O</mi><mi>z</mi></mrow></msub></semantics></math></inline-formula> being the scale after which a turbulent Kolmogorov energy spectrum likely recovers at high <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><mrow><mi>R</mi><mi>e</mi></mrow></semantics></math></inline-formula>.…”
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Determination of the Magnetic Field Strength and Geometry in the Accretion Disks of AGNs by Optical Spectropolarimetry by Mikhail Piotrovich, Stanislava Buliga, Tinatin Natsvlishvili

“…Based on the spectropolarimetric data of 33 Seyfert type 1 galaxies observed with the BTA-6m telescope of the Special Astrophysical Observatory, we estimated the magnetic field values at the event horizon of the supermassive black hole <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><msub><mi>B</mi><mi mathvariant="normal">H</mi></msub></semantics></math></inline-formula> and the exponents of the power-law dependence <i>s</i> of the magnetic field on the radius. …”
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PHILOSOPHY OF PERCEPTION OF THE WORLD IN THE INFORMATION AGE by M. S. Kravets

“…The presence of an edge or a limit, to which the galaxies have moved apart at a present point in time, would mean the restriction of the existence of space itself. …”
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Social Interactivity in Live Video Experiences Reduces Loneliness by Benjamin T. Kaveladze, Robert R. Morris, Robert R. Morris, Rosa Victoria Dimitrova-Gammeltoft, Amit Goldenberg, James J. Gross, Judd Antin, Melissa Sandgren, Melissa C. Thomas-Hunt

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The R136 star cluster hosts several stars whose individual masses greatly exceed the accepted 150 M-circle dot stellar mass limit by Crowther, P.A., Schnurr, O., Hirschi, R., Yusof, N., Parker, R.J., Goodwin, S.P., Abu Kassim, H.

“…The potential for stars greatly exceeding 150 M-circle dot within metal-poor galaxies suggests that such pair-instability supernovae could occur within the local universe, as has been claimed for SN 2007bi.…”

The Seoul National University AGN Monitoring Project. III. Hβ Lag Measurements of 32 Luminous Active Galactic Nuclei and the High-luminosity End of the Size–Luminosity Relation by Jong-Hak Woo, Shu Wang, Suvendu Rakshit, Hojin Cho, Donghoon Son, Vardha N. Bennert, Elena Gallo, Edmund Hodges-Kluck, Tommaso Treu, Aaron J. Barth, Wanjin Cho, Adi Foord, Jaehyuk Geum, Hengxiao Guo, Yashashree Jadhav, Yiseul Jeon, Kyle M. Kabasares, Won-Suk Kang, Changseok Kim, Minjin Kim, Tae-Woo Kim, Huynh Anh N. Le, Matthew A. Malkan, Amit Kumar Mandal, Daeseong Park, Chance Spencer, Jaejin Shin, Hyun-il Sung, Vivian U, Peter R. Williams, Nick Yee

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Blanco DECam Bulge Survey (BDBS). VI. Extinction Maps Toward Southern Galactic Bulge Globular Clusters by Justin A. Kader, Catherine A. Pilachowski, Christian I. Johnson, R. Michael Rich, Michael D. Young, Iulia T. Simion, William I. Clarkson, Scott Michael, Andrea Kunder, Anna Katherina Vivas, Andreas J. Koch-Hansen, Tommaso Marchetti

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Quasar Winds Caught on Acceleration and Deceleration by Weimin Yi, P. B. Hall, Zunli Yuan, W. N. Brandt, D. P. Schneider, Zhicheng He, Jin-Ming Bai, Xue-Bing Wu

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Mapping the Galactic Metallicity Gradient with Open Clusters: The State-of-the-Art and Future Challenges by Lorenzo Spina, Laura Magrini, Katia Cunha

“…Finally, we compare the shape of the galactic radial metallicity gradient to those of other spiral galaxies.…”
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