SLS-NETZWERKTECHNIK
SLS-Netzwerktechnik is a software company that offers networking, electrical engineering, network security, and remote maintenance.
SLS-NETZWERKTECHNIK
Social Links:
Industry:
Information Technology Network Security Software
Founded:
2004-01-01
Address:
Fรผrth, Bayern, Germany
Country:
Germany
Website Url:
http://www.slsn.de
Total Employee:
11+
Status:
Active
Contact:
49-9-11 77 77 17
Email Addresses:
[email protected]
Technology used in webpage:
Viewport Meta IPhone / Mobile Compatible Google Font API Google Analytics WordPress Google Universal Analytics Font Awesome Apache Wordpress Plugins Sitelinks Search Box
Similar Organizations
DVI Technologies
DVI Technologies offers communication, IT, networking, electrical design and energy-saving solution services to its customers.
Official Site Inspections
http://www.slsn.de
- Host name: www241.your-server.de
- IP address: 188.40.28.21
- Location: Germany
- Latitude: 51.2993
- Longitude: 9.491
- Timezone: Europe/Berlin
More informations about "SLS-Netzwerktechnik"
SLS-Netzwerktechnik
SLS-Netzwerktechnik GmbH. Melli-Beese-Straße 18 90768 Fürth Tel. 0911 - 77 77 17 Fax. 0911 - 77 35 77 eMail [email protected]. Öffnungs- und Anlieferzeiten: Montag โ Donnerstag 7:00 โ 16:00See details»
Senior-Loken syndrome - National Organization for Rare Disorders
Senior-Loken syndrome (SLSN) is a very rare autosomal recessive oculo-renal disease characterized by the association of nephronophthisis (NPHP), a chronic ... Sobre los Centros โฆSee details»
Superluminous Supernovae
In De Cia et al. 2018b we characterized the light-curve properties of the largest and homogeneous sample of SLSNe-I (H-poor), from the (i)Palomar Transient Factory. We characterized the โฆSee details»
Netzwerk-Sicherheit | SLS-Netzwerktechnik
SLS-Netzwerktechnik GmbH. Melli-Beese-Straße 18 90768 Fürth Tel. 0911 - 77 77 17 Fax. 0911 - 77 35 77 eMail [email protected]. Öffnungs- und Anlieferzeiten: Montag โ Donnerstag 7:00 โ 16:00See details»
Superluminous supernova - Wikipedia
A super-luminous supernova (SLSN, plural super luminous supernovae or SLSNe) is a type of stellar explosion with a luminosity 10 or more times higher than that of standard supernovae. Like supernovae, SLSNe seem to be produced by several mechanisms, which is readily revealed by their light-curves and spectra. There are multiple models for what conditions may produce an SโฆSee details»
A UV resonance line echo from a shell around a hydrogen-poor
Sep 10, 2018 Hydrogen-poor superluminous supernovae (SLSN-I) are a class of rare and energetic explosions that have been discovered in untargeted transient surveys in the past โฆSee details»
DES15E2mlf: a spectroscopically confirmed ... - Oxford Academic
Jun 13, 2017 SLSN searches that avoid selection based on host brightness could improve our understanding of this process in high-mass galaxies and at high redshift. 5 CONCLUSIONS. โฆSee details»
[1208.3217] Luminous Supernovae - arXiv.org
Aug 15, 2012 SLSN-R, a rare class of hydrogen-poor events, are powered by very large amounts of radioactive 56Ni and arguably result from explosions of very massive stars due to โฆSee details»
Padova-Asiago Supernova Group
A SLSN II extensively monitored extensively by PESSTO, CSS121015:004244+132827 (Benetti et al. 2014, MNRAS 441, 289; see Fig. 3), is one of the most luminous SN ever. The detection โฆSee details»
Observational properties of extreme supernovae - Nature
Aug 7, 2019 As could be expected, SLSN I Slow lightcurves have been observed up to later phases compared to SLSN I Fast 42,43,52,54,55,63 and, as displayed in Fig. 2, ... De Cia, A. โฆSee details»
Spectra of Hydrogen-poor Superluminous Supernovae from the โฆ
Feb 27, 2018 The American Astronomical Society (AAS), established in 1899 and based in Washington, DC, is the major organization of professional astronomers in North America.Its โฆSee details»
Superluminous Supernovae from the Dark Energy Survey
Dec 10, 2018 We present a sample of 21 hydrogen-free superluminous supernovae (SLSNe-I), and one hydrogen-rich SLSN (SLSN-II) detected during the five-year Dark Energy Survey โฆSee details»
Comparative Spectral Analysis of the Superluminous Supernova โฆ
We present a spectroscopic analysis of the recently discovered fast-evolving Type I superluminous supernova (SLSN-I) SN 2019neq (at redshift z = 0.1059). We compare it to the โฆSee details»
A Systematic Study of Superluminous Supernova Light-curve
Superluminous supernova (SLSN) light curves exhibit superior diversity compared to their regular-luminosity counterparts in terms of rise and decline timescales, peak luminosities, and overall โฆSee details»
Luminous Supernovae - NASA/ADS
Abstract. Supernovae, the luminous explosions of stars, have been observed since antiquity. However, various examples of superluminous supernovae (SLSNe; luminosities >7 × 10 43 โฆSee details»
A Systematic Study of Superluminous Supernova Light-curve
Mar 26, 2019 An investigation of Table 1 reveals yet another interesting property of our observed SLSN sample: five SLSN-I events SN2010md, PTF09atu, PS1-10pm, SNLS 07D2bv, and โฆSee details»
Superluminous supernovae from the Dark Energy Survey
May 21, 2019 We present a sample of 21 hydrogen-free superluminous supernovae (SLSNe-I) and one hydrogen-rich SLSN (SLSN-II) detected during the five-year Dark Energy Survey โฆSee details»
ASASSN-15lh: A highly super-luminous supernova | Science - AAAS
Jan 15, 2016 SNID , a commonly used SN classification software that has a spectral library of most types of supernovae except SLSN, failed to find a good SN match. However, we noticed โฆSee details»
Superluminous Supernovae in LSST: Rates, Detection Metrics, and โฆ
Dec 21, 2018 Given the average SLSN duration of โ100 days (Figure 5), a cadence of roughly two to four days (similar to the nominal cadence) in any filter would be sufficient to recover โฆSee details»
[2104.03365] Binary pathways to SLSNe-I: SN 2017gci - arXiv.org
Apr 7, 2021 Download PDF Abstract: Some hydrogen poor superluminous supernovae (SLSNe) exhibit bumps in the tails of their light-curves associated with hydrogen features in their late โฆSee details»