diff --git a/FGRP1_discoveries.html b/FGRP1_discoveries.html index 0e79b72a7c3d1eb5b81e02f5b81b4f96d6159e39..af9f082cb9e5055bccc8c587d8b1bb79f607d721 100644 --- a/FGRP1_discoveries.html +++ b/FGRP1_discoveries.html @@ -3,8 +3,8 @@
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+ Volunteers (Country): + UW-Madison CAE (USA) and UH RCC - Maxwell (USA) + Date: + 03 Oct 2014 + Survey: + FGRP4 + Selected pulsar parameters: + Right ascension: 12:08:13.96(6) + Declination: -62:38:02.3(4) + Spin frequency: 2.27 Hz + First frequency derivate: -1.68 x 10-11 Hz/s + Characteristic age: 2,700 yrs + Spin-down power: 1.5 x 1036 erg/s + |
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Volunteers (Country): - PeRu (Czech Republic) and Bryden Kanngiesser (Canada) + PeRu (Czech Republic) and Bryden Kanngiesser (Canada) Date: 19 Jun 2015 Survey: @@ -443,7 +487,7 @@ gamma-ray emission as a function of pulsar rotation phase and resolve the pulse |
Volunteers (Country): - Mak-ino (Japan) and Thomas M. Jackson (USA) + Mak-ino (Japan) and Thomas M. Jackson (USA) Date: 14 Dec 2011 Survey: @@ -489,7 +533,7 @@ gamma-ray emission as a function of pulsar rotation phase and resolve the pulse |
Volunteers (Country): - The NEMO computing cluster (USA) and Chen (USA) + The NEMO computing cluster (USA) and Chen (USA) Date: 30 Sep 2011 Survey: @@ -533,7 +577,7 @@ gamma-ray emission as a function of pulsar rotation phase and resolve the pulse |
Volunteers (Country): - fred c (USA) and Gabriel Vasquez + fred c (USA) and Gabriel Vasquez Date: 25 Mar 2015 Survey: @@ -577,7 +621,7 @@ gamma-ray emission as a function of pulsar rotation phase and resolve the pulse |
Volunteers (Country): - r4p and Greg Dorais (USA) + r4p and Greg Dorais (USA) Date: 04 Oct 2014 Survey: @@ -621,7 +665,7 @@ gamma-ray emission as a function of pulsar rotation phase and resolve the pulse |
Volunteers (Country): - xio.nyc (Antarctica) and Hung Tran (USA) + xio.nyc (Antarctica) and Hung Tran (USA) Date: 20 Dec 2014 Survey: @@ -665,7 +709,7 @@ gamma-ray emission as a function of pulsar rotation phase and resolve the pulse |
Volunteers (Country): - Syracuse University (USA) and Eric Schwartz (USA) + Syracuse University (USA) and Eric Schwartz (USA) Date: 17 Oct 2014 Survey: @@ -709,7 +753,7 @@ gamma-ray emission as a function of pulsar rotation phase and resolve the pulse |
Volunteers (Country): - ATLAS AEI Hannover (Germany) and LLO_LDAS (USA) + ATLAS AEI Hannover (Germany) and LLO_LDAS (USA) Date: 19 Dec 2014 Survey: @@ -753,7 +797,7 @@ gamma-ray emission as a function of pulsar rotation phase and resolve the pulse |
Volunteers (Country): - Aurelien FAUCHEUX (France) and Roger (USA) + Aurelien FAUCHEUX (France) and Roger (USA) Date: 18 Nov 2014 Survey: @@ -800,7 +844,7 @@ gamma-ray emission as a function of pulsar rotation phase and resolve the pulse |
Volunteers (Country): - Connor Barry (USA) and Richard Johnson (USA) + Connor Barry (USA) and Richard Johnson (USA) Date: 11 Sep 2014 Survey: @@ -846,7 +890,7 @@ gamma-ray emission as a function of pulsar rotation phase and resolve the pulse |
Volunteers (Country): - Doug Lean (Australia) and Hans-Peter Tobler (Germany) + Doug Lean (Australia) and Hans-Peter Tobler (Germany) Date: 19 Sep 2011 Survey: @@ -890,7 +934,7 @@ gamma-ray emission as a function of pulsar rotation phase and resolve the pulse |
Volunteers (Country): - gramoll (USA) and Rogir (Germany) + gramoll (USA) and Rogir (Germany) Date: 09 Sep 2014 Survey: @@ -919,8 +963,8 @@ gamma-ray emission as a function of pulsar rotation phase and resolve the pulse |
- Einstein@Home - Colin J. Clark (Last Update: Feb 22, 2016) + Einstein@Home + Colin J. Clark (Last Update: Nov 17, 2016) |