Universe@Home: Difference between revisions

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== Project team / Sponsors ==

Copernicus Astronomical Centre of the Polish Academy of Sciences. Project server managed: Krzysztof 'krzyszp' Piszczek.

== Scientific results ==

* external links

At the moment there are six sets of data:

#'''''[https://universeathome.pl/universe/x-ray.php X-ray]'''''

#'''''[https://universeathome.pl/universe/qs.php QuarkStars]'''''

#'''''[https://universeathome.pl/universe/bhdb.php Black hole database]'''''

#'''''[https://universeathome.pl/universe/xbhms.php Dynamical formation of XRBs with black holes]'''''

#'''[https://universeathome.pl/universe/bhns.php ''BH NS formation database files'']'''

#'''''[https://universeathome.pl/universe/self_lensing.php Self-lensing binary predictions]'''''

== Scientific publications ==

~~Format example~~:

# ~~Durech~~, J., ~~B. Carry~~, M. ~~Delbo, M~~. ~~Kaasalainen and M~~. ~~Viikinkoski~~. [https://arxiv.org/abs/~~1502~~.~~04816 Asteroid Models from Multiple Data Sources~~.] ~~(2015)~~. ~~DOI~~: 10.~~48550~~/~~ARXIV~~.~~1502~~.~~04816~~.

# '''[https://arxiv.org/pdf/2302.10851.pdf ''Symmetry breaking in merging binary black holes from young massive clusters and isolated binaries'']''' Banerjee et al. 2023

# '''[https://arxiv.org/abs/1907.11431 ''Populations of stellar mass Black holes from binary systems'']''' Wiktorowicz et al. 2019

# '''[https://arxiv.org/abs/1904.01545 ''Merger of compact stars in the two-families scenario'']''' De Pietri et al. 2019

# '''[https://arxiv.org/abs/1811.08998 ''The observed vs total population of ULXs'']''' Wiktorowicz et al. 2019

# '''[https://arxiv.org/abs/1812.10065 ''Binary neutron star formation and the origin of GW170817'']''' Belczynki et al. 2018

# '''[https://arxiv.org/abs/1712.00632 The origin of the first neutron star -- neutron star merger]''' Belczynki et al. 2018

# '''[https://arxiv.org/abs/1708.07885 ''Double neutron stars: merger rates revisited'']''' Chruślińska et al. 2017

# '''[https://arxiv.org/abs/1707.01586 ''Strange quark stars in binaries: formation rates, mergers and explosive phenomena'']''' Wiktorowicz et al. 2017

# '''[https://arxiv.org/abs/1706.07053 ''The evolutionary roads leading to low effective spins, high black hole masses, and O1/O2 rates of LIGO/Virgo binary black holes'']''' Belczynski et al. 2017

# '''[https://arxiv.org/abs/1705.06155 ''The origin of the Ultraluminous X-ray Sources'']''' Wiktorowicz et al. 2017

# '''[https://arxiv.org/abs/1607.03116 ''The Effect of Pair-Instability Mass Loss on Black Hole Mergers'']''' Belczynski et al. 2016

# '''''[https://arxiv.org/abs/1605.09286 Spectroscopy of Kerr black holes with Earth- and space-based interferometers]''''' Berti et al. 2016

# '''''[https://arxiv.org/abs/1602.04531 The first gravitational-wave source from the isolated evolution of two 40-100 Msun stars]''''' Belczynski et al. 2016

# '''''[https://arxiv.org/abs/1503.08745 Nature of the Extreme Ultraluminous X-ray Sources]''''' Wiktorowicz et al. 2015

@@ Line 18: / Line 18: @@
 == Project team / Sponsors ==
+Copernicus Astronomical Centre of the Polish Academy of Sciences. Project server managed: Krzysztof 'krzyszp' Piszczek.
 == Scientific results ==
-* external links
+At the moment there are six sets of data:
+#'''''[https://universeathome.pl/universe/x-ray.php X-ray]'''''
+#'''''[https://universeathome.pl/universe/qs.php QuarkStars]'''''
+#'''''[https://universeathome.pl/universe/bhdb.php Black hole database]'''''
+#'''''[https://universeathome.pl/universe/xbhms.php Dynamical formation of XRBs with black holes]'''''
+#'''[https://universeathome.pl/universe/bhns.php ''BH NS formation database files'']'''
+#'''''[https://universeathome.pl/universe/self_lensing.php Self-lensing binary predictions]'''''
 == Scientific publications ==
-Format example:
-# Durech, J., B. Carry, M. Delbo, M. Kaasalainen and M. Viikinkoski. [https://arxiv.org/abs/1502.04816 Asteroid Models from Multiple Data Sources.] (2015). DOI: 10.48550/ARXIV.1502.04816.
+# '''[https://arxiv.org/pdf/2302.10851.pdf ''Symmetry breaking in merging binary black holes from young massive clusters and isolated binaries'']''' Banerjee et al. 2023
+# '''[https://arxiv.org/abs/1907.11431 ''Populations of stellar mass Black holes from binary systems'']''' Wiktorowicz et al. 2019
+# '''[https://arxiv.org/abs/1904.01545 ''Merger of compact stars in the two-families scenario'']''' De Pietri et al. 2019
+# '''[https://arxiv.org/abs/1811.08998 ''The observed vs total population of ULXs'']''' Wiktorowicz et al. 2019
+# '''[https://arxiv.org/abs/1812.10065 ''Binary neutron star formation and the origin of GW170817'']''' Belczynki et al. 2018
+# '''[https://arxiv.org/abs/1712.00632 The origin of the first neutron star -- neutron star merger]''' Belczynki et al. 2018
+# '''[https://arxiv.org/abs/1708.07885 ''Double neutron stars: merger rates revisited'']''' Chruślińska et al. 2017
+# '''[https://arxiv.org/abs/1707.01586 ''Strange quark stars in binaries: formation rates, mergers and explosive phenomena'']''' Wiktorowicz et al. 2017
+# '''[https://arxiv.org/abs/1706.07053 ''The evolutionary roads leading to low effective spins, high black hole masses, and O1/O2 rates of LIGO/Virgo binary black holes'']''' Belczynski et al. 2017
+# '''[https://arxiv.org/abs/1705.06155 ''The origin of the Ultraluminous X-ray Sources'']''' Wiktorowicz et al. 2017
+# '''[https://arxiv.org/abs/1607.03116 ''The Effect of Pair-Instability Mass Loss on Black Hole Mergers'']''' Belczynski et al. 2016
+# '''''[https://arxiv.org/abs/1605.09286 Spectroscopy of Kerr black holes with Earth- and space-based interferometers]''''' Berti et al. 2016
+# '''''[https://arxiv.org/abs/1602.04531 The first gravitational-wave source from the isolated evolution of two 40-100 Msun stars]''''' Belczynski et al. 2016
+# '''''[https://arxiv.org/abs/1503.08745 Nature of the Extreme Ultraluminous X-ray Sources]''''' Wiktorowicz et al. 2015