Tootfinder

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Blossom Dearie:
🎵 Tout Doucement
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https://open.spotify.com/track/5jgMJKHu3HznRuVI3zmr76

#Lämmersaison2024 #SheepOfMastodon #Sheep
Da euch der Säugeeimer wohl gut gefallen hat, hier das Sequel:

Calibration requirement for Epoch of Reionization 21-cm signal observation -- III. Bias and variance in uGMRT ELAIS-N1 field power spectrum
Saikat Gayen, Rashmi Sagar, Sarvesh Mangla, Prasun Dutta, Nirupam Roy, Arnab Chakraborty, Jais Kumar, Abhirup Datta, Samir Choudhuri
https://arxiv.org/abs/2402.18306

Calibration requirement for Epoch of Reionization 21-cm signal observation -- III. Bias and variance in uGMRT ELAIS-N1 field power spectrum
Power spectrum of \HI 21 cm radiation is one of the promising probes to study large scale structure of the universe. Presence of orders of magnitude larger foregrounds in the frequency range for such observations has been one of the major challenge. The foreground contamination also introduce residual calibration errors in the interferometric data. The latter introduce bias in the 21-cm power spectrum estimates and increase systematics. There have been several efforts to understand and improve …

LOL. Federal jurisdiction is federal. How does a lawyer actively practicing in Federal courts not understand such basics? I wonder whether a fugitive lawyer has ever been arrested this way before? https://masto.ai/@Nonilex/112119662014988464

A VLBA-uGMRT search for candidate binary black holes: Study of six X-shaped radio galaxies with double-peaked emission lines
Biny Sebastian, Anderson Caproni, Preeti Kharb, A. J. Nayana, Arshi Ali, K. Rubinur, Christopher P. O'Dea, Stefi Baum, Sumana Nandi
https://arxiv.org/abs/2402.12521

A VLBA-uGMRT search for candidate binary black holes: Study of six X-shaped radio galaxies with double-peaked emission lines
Identifying methods to discover dual AGN has proven to be challenging. Several indirect tracers have been explored in the literature, including X/S-shaped radio morphologies and double-peaked (DP) emission lines in the optical spectra. However, the detection rates of confirmed dual AGN candidates from the individual methods remain extremely small. We search for binary black holes in a sample of six sources that exhibit both X-shaped radio morphology and DP emission lines using the VLBA. Three o…

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Giulian Charles:
🎵 Buy my soul
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https://open.spotify.com/track/3uij7MRTbOBKJN5m3sadPV

Towards $21$-cm intensity mapping at $z=2.28$ with uGMRT using the tapered gridded estimator -- IV. Wideband analysis
Khandakar Md Asif ElahiIndian Institute of Technology Kharagpur, Kharagpur, India, Somnath BharadwajIndian Institute of Technology Kharagpur, Kharagpur, India, Srijita PalIndian Institute of Science, Bangalore, India, Abhik GhoshBanwarilal Bhalotia College, Asansol, India, Sk. Saiyad AliJadavpur University, Kolkata, India, Samir ChoudhuriIndian Institute of Technology M…

Towards $21$-cm intensity mapping at $z=2.28$ with uGMRT using the tapered gridded estimator -- IV. Wideband analysis
We present a Wideband Tapered Gridded Estimator (TGE), which incorporates baseline migration and variation of the primary beam pattern for neutral hydrogen (${\rm H\hspace{0.5mm}}{\scriptsize {\rm I}}$) 21-cm intensity mapping (IM) with large frequency bandwidth radio-interferometric observations. Here we have analysed $394-494 \, {\rm MHz}$ $(z = 1.9 - 2.6)$ uGMRT data to estimate the Multi-frequency Angular Power Spectrum (MAPS) $C_\ell(Δν)$ from which we have removed the foregrounds using …

Da wir so viele Milchflaschen auf einmal gar nicht halten können, haben wir jetzt Unterstützung.
#Lämmersaison2024 #SheepOfMastodon #Sheep

This https://arxiv.org/abs/2402.18306 has been replaced.
initial toot: https://mastoxiv.page/@arXiv_…

Calibration requirement for Epoch of Reionization 21-cm signal observation -- III. Bias and variance in uGMRT ELAIS-N1 field power spectrum
Power spectrum of \HI 21 cm radiation is one of the promising probes to study large scale structure of the universe. Presence of orders of magnitude larger foregrounds in the frequency range for such observations has been one of the major challenge. The foreground contamination also introduce residual calibration errors in the interferometric data. The latter introduce bias in the 21-cm power spectrum estimates and increase systematics. There have been several efforts to understand and improve …

🔊 #NowPlaying on fip
Giulian Charles:
🎵 Buy my soul
#GiulianCharles
https://open.spotify.com/track/3uij7MRTbOBKJN5m3sadPV