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@scott@carfree.city
2026-09-05 03:41:31

This story buries the lede that the three biggest donors to the SF Democratic Party are, literally, Republican donors.
1. Neighbors for a Better San Francisco, whose top backer is William Oberndorf, a "Republican mega-donor" according to April 2024 Mission Local coverage;
2. Chris Larsen, who co-founded Ripple, which donated to Trump's White House ballroom per CNN;
3. SF Believes, funded by "MAGA WhatsApp co-founder Jan Koum"
The SF Democratic Par…

@arXiv_mathCV_bot@mastoxiv.page
2026-08-05 09:09:43

Replaced article(s) found for math.CV. arxiv.org/list/math.CV/new
[1/1]:
- On weak Wolff--Denjoy theorem for certain non-convex domains
Vikramjeet Singh Chandel, Sanjoy Chatterjee, Chandan Sur
arxiv.org/abs/2604.07215 mastoxiv.page/@arXiv_mathCV_bo
- Analytic properties of the parametric harmonic zeta function, with applications to harmonic Stiel...
Merve Kara \"Ozt\"urk, M\"um\"un Can
arxiv.org/abs/2606.27827 mastoxiv.page/@arXiv_mathCV_bo
- The convergence of power matrices
Vyacheslav M. Abramov
arxiv.org/abs/2307.13142 mastoxiv.page/@arXiv_mathCA_bo
- Three topological phases of the elliptic Ginibre ensembles with a point charge
Sung-Soo Byun, Eui Yoo
arxiv.org/abs/2502.02948 mastoxiv.page/@arXiv_mathph_bo
- A Criterion for the Algebraic Density Property of Affine $SL_2$-Manifolds
Rafael B. Andrist, Jan Draisma, Gene Freudenburg, Gaofeng Huang, Frank Kutzschebauch
arxiv.org/abs/2502.13903 mastoxiv.page/@arXiv_mathAC_bo
- Continuous first-order logic of abstract harmonic spaces
Haoming Wang
arxiv.org/abs/2604.14020 mastoxiv.page/@arXiv_mathLO_bo
toXiv_bot_toot

@BBC3MusicBot@mastodonapp.uk
2026-07-09 16:21:55

🇺🇦 #NowPlaying on BBCRadio3's #InTune
Claude Debussy, Maurice Ravel, Orchestre national de France & Jean Martinon:
🎵 Tarantelle styrienne
#ClaudeDebussy #MauriceRavel #OrchestrenationaldeFrance #JeanMartinon

@arXiv_astrophGA_bot@mastoxiv.page
2026-07-22 08:02:08

The Next Generation Virgo Cluster Survey (NGVS). II. A Catalog of Galaxies in the Virgo Cluster
Laura Ferrarese, Patrick Cote, Lauren A. MacArthur, Joel C. Roediger, John P. Blakeslee, Michele Cantiello, Jean-Charles Cuillandre, Puragra Guhathakurta, Stephen Gwyn, Max M. Kurzner, Eric W. Peng, Matthew Santos, Eleanore B. Todd, Elisa Toloba, Pierre-Alain Duc, Patrick R. Durrell, Nicholas Fantin, Yuting Feng, Ariane Lancon, Sungsoon Lim, Chengze Liu, Deborah Lokhorst, Alessia Longobardi, Simona Mei, J. Christopher Mihos, Sanjaya Paudel, Thomas H. Puzia, Anand Raichoor, Ruben Sanchez-Janssen, Kaixiang Wang, Hongxin Zhang, Alessandro Boselli, Michael L. Balogh, Samuel Boissier, Eric Emsellem, J. J. Kavelaars, Alan W. McConnachie, Cameron R. Morgan, Chelsea Spengler, James E. Taylor, Matthew A. Taylor, Toby Brown, Sebastien Fabbro, Raphael Gavazzi, Hendrik Hildebrandt, Rashi Jain, Andres Jordan, Rory Smith, Solveig Thompson, Haruka Yoshino, Wim van Driel, Ludovic van Waerbeke, Tyrone E. Woods, Jade Yeung
arxiv.org/abs/2607.18414 arxiv.org/pdf/2607.18414 arxiv.org/html/2607.18414
arXiv:2607.18414v1 Announce Type: new
Abstract: The Next Generation Virgo Cluster Survey (NGVS) is a deep, high resolution imaging campaign that used the 1 deg$^2$ MegaCam instrument on the Canada-France-Hawaii Telescope to carry out a comprehensive optical survey of the Virgo cluster, from its core to its virial radius. The NGVS covers a contiguous area of 104 deg$^2$ (8.63 Mpc$^2$ at the 16.5 Mpc distance of Virgo) in the $u^*$-,$g$-,$i$-, and $z$-band, with additional limited coverage in $r$. In this paper, we present the final catalog of Virgo galaxies across the entire NGVS area. The catalog includes 3680 galaxies considered to be $bona~fide$ members of the cluster, spanning a factor of 2.5 million in luminosity, from $g = 8.42$ mag to $g = 24.41$ mag ($M_g = -22.67$ mag to $M_g = -6.68$ mag). With 2100 previously uncataloged galaxies, the NGVS catalog augments the number of known Virgo members by a factor 2.3. The catalog is complete down to $g = 18.6$ mag ($M_g=-12.5$ mag, corresponding to a stellar mass $M_* \sim 1.6\times10^7~M_{\odot}$ for an old stellar population) and 50% complete at $g = 22.0$ mag ($M_g=-9.1$ mag, $M_* \sim 6.2\times10^5~M_{\odot}$), three magnitudes deeper than the venerable Virgo Cluster Catalog (VCC), which for over 40 years has served as the reference standard for Virgo. Photometric and structural parameters are derived for all NGVS galaxies and presented in a series of tables, alongside nuclear and morphological classification, as well as stellar masses and, when available, radial velocities.
toXiv_bot_toot