Tootfinder

Opt-in global Mastodon full text search. Join the index!

No exact results. Similar results found.
@jamesthebard@social.linux.pizza
2024-05-06 16:54:12

Okay, this should be good enough to get things done. The file format supports monochrome and 8-bit RGB data along with static and animated images and should be fairly easy to read off of an SDcard connencted to the Arduino. Pretty happy with the result, but now I need to figure out how to properly document all of this... #programming

A screenshot of ImHex showing two files: a monochrome graphics file and an RGB graphics file.  The right-pane shows the pattern editor code for each field, and the pattern data shows the resulting data.
@arXiv_csCL_bot@mastoxiv.page
2024-05-06 08:26:28

This arxiv.org/abs/2310.06555 has been replaced.
link: scholar.google.com/scholar?q=a

@arXiv_csPL_bot@mastoxiv.page
2024-05-07 08:47:27

This arxiv.org/abs/2403.08056 has been replaced.
initial toot: mastoxiv.page/@arXiv_csPL_…

@arXiv_astrophGA_bot@mastoxiv.page
2024-03-06 07:15:57

Chemical abundances and deviations from the solar S/O ratio in the gas-phase ISM of galaxies based on infrared emission lines
Borja P\'erez-D\'iaz, Enrique P\'erez-Montero, Juan A. Fern\'andez-Ontiveros, Jos\'e M. V\'ilchez, Antonio Hern\'an-Caballero, Ricardo Amor\'in
arxiv.org/abs/2403.02903 arxiv.org/pdf/2403.02903
arXiv:2403.02903v1 Announce Type: new
Abstract: The infrared (IR) range is extremely useful in the context of chemical abundance studies of the gas-phase interstellar medium (ISM) due to the large variety of ionic species traced in this regime, the negligible effects from dust attenuation or temperature stratification, and the amount of data that has been and will be released in the coming years. Taking advantage of available IR emission lines, we analysed the chemical content of the gas-phase ISM in a sample of 131 Star-Forming Galaxies (SFGs) and 73 Active Galactic Nuclei (AGNs). Particularly, we derived the chemical content via their total oxygen abundance in combination with nitrogen and sulfur abundances, and with the ionisation parameter. We used a new version of the code HII-CHI-Mistry-IR v3.1 which allows us to estimate log(N/O), 12 log(O/H), log(U), and, for the first time, 12 log(S/H) from IR emission lines, which can be applied to both SFGs and AGNs. We tested that the estimations from this new version, that only considers sulfur lines for the derivation of sulfur abundances, are compatible with previous studies. While most of the SFGs and AGNs show solar log(N/O) abundances, we found a large spread in the log(S/O) relative abundances. Specifically, we found extremely low log(S/O) values (1/10th solar) in some SFGs and AGNs with solar-like oxygen abundances. This result warns against the use of optical and IR sulfur emission lines to estimate oxygen abundances when no prior estimation of log(S/O) is provided.

@usul@piaille.fr
2024-04-07 03:49:54

Burundi: des centaines de «concubines» chassées de leurs ménages par les autorités au nom de l'ordre moral
rfi.fr/fr/afrique/20240405-bur

@arXiv_eessSP_bot@mastoxiv.page
2024-05-07 08:50:15

This arxiv.org/abs/2308.11647 has been replaced.
initial toot: mastoxiv.page/@arXiv_ees…

@arXiv_csIT_bot@mastoxiv.page
2024-05-07 08:49:10

This arxiv.org/abs/2404.13624 has been replaced.
initial toot: mastoxiv.page/@arXiv_csIT_…

@arXiv_astrophCO_bot@mastoxiv.page
2024-05-06 07:24:23

A Parameter-Masked Mock Data Challenge for Beyond-Two-Point Galaxy Clustering Statistics
2pt Collaboration, Elisabeth Krause, Yosuke Kobayashi, Andr\'es N. Salcedo, Mikhail M. Ivanov, Tom Abel, Kazuyuki Akitsu, Raul E. Angulo, Giovanni Cabass, Sofia Contarini, Carolina Cuesta-Lazaro, ChangHoon Hahn, Nico Hamaus, Donghui Jeong, Chirag Modi, Nhat-Minh Nguyen, Takahiro Nishimichi, Enrique Paillas, Marcos Pellejero Iba\~nez, Oliver H. E. Philcox, Alice Pisani, Fabian Schmidt, Satoshi T…

@arXiv_csIT_bot@mastoxiv.page
2024-03-08 06:50:15

Bi-Static Sensing in OFDM Wireless Systems for Indoor Scenarios
Vijaya Yajnanarayana, Philipp Geuer
arxiv.org/abs/2403.04201