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 @@ Einstein@Home Gamma-ray Pulsar Discoveries in Fermi-LAT Data - - + +

Einstein@Home Gamma-ray Pulsar Discoveries in Fermi-LAT Data

@@ -133,7 +133,7 @@ gamma-ray emission as a function of pulsar rotation phase and resolve the pulse Volunteers (Country):
- UW-Madison CAE (USA) and RUElwell (USA)

+ UW-Madison CAE (USA) and RUElwell (USA)

Date:
31 Dec 2014

Survey:
@@ -177,7 +177,7 @@ gamma-ray emission as a function of pulsar rotation phase and resolve the pulse Volunteers (Country):
- Whelton Miller (USA), ATLAS AEI Hannover (Germany) and Delty (USA)

+ Whelton Miller (USA), ATLAS AEI Hannover (Germany) and Delty (USA)

Date:
15 Dec 2014

Survey:
@@ -220,7 +220,7 @@ gamma-ray emission as a function of pulsar rotation phase and resolve the pulse Volunteers (Country):
- David Z (Canada) and Test (France)

+ David Z (Canada) and Test (France)

Date:
06 Jan 2012

Survey:
@@ -265,7 +265,7 @@ gamma-ray emission as a function of pulsar rotation phase and resolve the pulse Volunteers (Country):
- KataJun (Japan) and huwar

+ KataJun (Japan) and huwar

Date:
20 Jan 2015

Survey:
@@ -309,7 +309,7 @@ gamma-ray emission as a function of pulsar rotation phase and resolve the pulse Volunteers (Country):
- Syracuse University (USA) and LLO_LDAS (USA)

+ Syracuse University (USA) and LLO_LDAS (USA)

Date:
28 Oct 2014

Survey:
@@ -353,7 +353,7 @@ gamma-ray emission as a function of pulsar rotation phase and resolve the pulse Volunteers (Country):
- ATLAS AEI Hannover (Germany) and Syracuse University (USA)

+ ATLAS AEI Hannover (Germany) and Syracuse University (USA)

Date:
03 Oct 2014

Survey:
@@ -374,6 +374,50 @@ gamma-ray emission as a function of pulsar rotation phase and resolve the pulse + + + + + + + + + + + + +
+ + + + + + +
Pulsar J1208-6238
+
+
+ J1208 + J1208 +
+ 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
+
+

+ + + + @@ -397,7 +441,7 @@ gamma-ray emission as a function of pulsar rotation phase and resolve the pulse diff --git a/img/fhist-J1208.png b/img/fhist-J1208.png new file mode 100644 index 0000000000000000000000000000000000000000..4a5032804bc5919e9fd3ec89241c38c0b30c26cf Binary files /dev/null and b/img/fhist-J1208.png differ diff --git a/img/psrs_vs_time.png b/img/psrs_vs_time.png index d59a3e271d64431ab9ed0af8c09fa15c38115662..bb37aff68d98ee3bd74e4fcf93ae637d7f4a2e9c 100644 Binary files a/img/psrs_vs_time.png and b/img/psrs_vs_time.png differ diff --git a/img/tvsph-J1208.png b/img/tvsph-J1208.png new file mode 100644 index 0000000000000000000000000000000000000000..be9a375ae177dcebe6ee8c4148fbfcb3eb113bad Binary files /dev/null and b/img/tvsph-J1208.png differ diff --git a/psrs_by_time.py b/psrs_by_time.py index c714fbed7d9cc04190e47a0df94e95de4c7b7f39..fb057cae700e290d2c23c2a76019cedef4532b11 100644 --- a/psrs_by_time.py +++ b/psrs_by_time.py @@ -35,7 +35,8 @@ psr_timeline = np.array([[0,0], [64,4], # 4 E@H Pulsars, 2013 [84,1], # J1906 [91, 13], # Next bunch of FGRP4 pulsars without J1208 - [95, 0]] ) # Now + [100, 1], + [102,0]]) # J1208 FGRP1_idx = 8 FGRP4_idx = 9 AEI_idx = 5 @@ -61,16 +62,16 @@ ax.xaxis.set_major_formatter(xfmt) plt.xlim(months[0],months[-1]) # Survey labels -plt.text(months[FGRP1_idx] + 0.8, psrs[FGRP1_idx]/2.0,'E@H\nFGRP1',ha='center') -plt.text(months[FGRP4_idx] + 0.5, psrs[-1]/2.0,'E@H\nFGRP4',ha='center') -plt.text(months[AEI_idx] + 1.0, psrs[AEI_idx]/2.0,'ATLAS Cluster\n AEI Hannover',ha='center') +plt.text(months[FGRP1_idx] + 0.8, 33,'E@H\nFGRP1',ha='center') +plt.text(months[AEI_idx] + 1.0, 29,'ATLAS Cluster\n AEI Hannover',ha='center') +plt.text(months[FGRP4_idx] + 0.75, 35,'E@H\nFGRP4',ha='center') # Survey shading ax.fill_between([months[FGRP1_idx],months[FGRP1_idx+1]],[0,0],[psrs[FGRP1_idx],psrs[FGRP1_idx]],color='darkgrey') -ax.fill_between([months[FGRP4_idx],months[FGRP4_idx+1],months[FGRP4_idx+1],months[-1]], - [0,0,0,0], - [psrs[FGRP4_idx],psrs[FGRP4_idx],psrs[FGRP4_idx+1],psrs[-1]], +ax.fill_between([months[FGRP4_idx],months[FGRP4_idx+1],months[FGRP4_idx+1],months[-2],months[-2],months[-1]], + [0,0,0,0,0,0], + [psrs[FGRP4_idx],psrs[FGRP4_idx],psrs[FGRP4_idx+1],psrs[FGRP4_idx+1],psrs[-2],psrs[-1]], color='grey') ax.fill_between([months[AEI_idx],months[AEI_idx + 1],months[AEI_idx + 1],months[FGRP1_idx]],
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)