[Message Prev][Message Next][Thread Prev][Thread Next][Message Index][Thread Index]

[vsnet-grb-info 472] GRB 021004: Optical measurement at OHP



TITLE:   GCN GRB OBSERVATION REPORT
NUMBER:  1615
SUBJECT: GRB 021004: Optical measurement at OHP
DATE:    02/10/10 07:32:26 GMT
FROM:    Michel Boer at CESR-CNRS  <Michel.Boer@cesr.fr>

This is a multi-part message in MIME format.

------=_NextPart_000_0034_01C2703E.C401F0E0
Content-Type: text/plain;
	charset="us-ascii"
Content-Transfer-Encoding: 7bit

 

A. Klotz and M. Boer CESR/CNRS (Toulouse, France), and W. Thuillot
IMCCE/BDL Paris, France report the following data on GRB 021004 obtained
with the 1.20 meter telescope at the OHP/CNRS (Observatoire de Haute
Provence - France).

Images were R-cousin filtered. Each measurement image results of
co-addition of 4 frames of 40s (dark and flat corrected). Magnitudes are
computed compared to the USNO star at 00:26:58.713 +18:56:56.61 (Fox et
al. GCN 1564) assuming R=15.64.

Magnitudes of GRB021004 : (R band) 

2002 oct. 04 22:04:44.5 UT (JD=2452552.41996) : 18.29
2002 oct. 04 22:12:01.7 UT (JD=2452552.42502) : 18.37
2002 oct. 04 22:20:32.3 UT (JD=2452552.43093) : 18.40
2002 oct. 04 23:51:04.3 UT (JD=2452552.49380) : 18.67
2002 oct. 04 23:57:13.2 UT (JD=2452552.49807) : 18.65

Dates are middle of exposures. This data fill nicely a gap around T0 +
0.4 when the decay index of the light curve increases.

. 

 

 

 


------=_NextPart_000_0034_01C2703E.C401F0E0
Content-Type: text/html;
	charset="us-ascii"
Content-Transfer-Encoding: quoted-printable

<html>

<head>
<META HTTP-EQUIV=3D"Content-Type" CONTENT=3D"text/html; =
charset=3Dus-ascii">


<meta name=3DGenerator content=3D"Microsoft Word 10 (filtered)">

<style>
<!--
 /* Style Definitions */
 p.MsoNormal, li.MsoNormal, div.MsoNormal
	{margin:0cm;
	margin-bottom:.0001pt;
	font-size:12.0pt;
	font-family:"Times New Roman";}
a:link, span.MsoHyperlink
	{color:blue;
	text-decoration:underline;}
a:visited, span.MsoHyperlinkFollowed
	{color:purple;
	text-decoration:underline;}
p
	{margin-right:0cm;
	margin-left:0cm;
	font-size:12.0pt;
	font-family:"Times New Roman";}
span.StyleCourrierlectronique17
	{font-family:Arial;
	color:windowtext;}
@page Section1
	{size:595.3pt 841.9pt;
	margin:70.85pt 70.85pt 70.85pt 70.85pt;}
div.Section1
	{page:Section1;}
-->
</style>

</head>

<body lang=3DFR link=3Dblue vlink=3Dpurple>

<div class=3DSection1>

<p class=3DMsoNormal><font size=3D2 face=3DArial><span =
style=3D'font-size:10.0pt;
font-family:Arial'>&nbsp;</span></font></p>

<p><font size=3D3 face=3D"Times New Roman"><span lang=3DEN-GB =
style=3D'font-size:12.0pt'>A.
Klotz and M. Boer CESR/CNRS (</span></font><span =
lang=3DEN-GB>Toulouse</span><span
 lang=3DEN-GB>, </span><span lang=3DEN-GB>France</span><span =
lang=3DEN-GB>), and W.
Thuillot IMCCE/BDL Paris, France report the following data on GRB 021004
obtained with the 1.20 meter telescope at the OHP/CNRS (Observatoire de =
Haute
Provence - France).</span></p>

<p><font size=3D3 face=3D"Times New Roman"><span lang=3DEN-GB =
style=3D'font-size:12.0pt'>Images
were R-cousin filtered. Each measurement image results of co-addition of =
4
frames of 40s (dark and flat corrected). Magnitudes are computed =
compared to
the USNO star at 00:26:58.713 +18:56:56.61 (Fox et al. GCN 1564) =
assuming
R=3D15.64.</span></font></p>

<p><font size=3D3 face=3D"Times New Roman"><span lang=3DEN-GB =
style=3D'font-size:12.0pt'>Magnitudes
of GRB021004 : (R band) </span></font></p>

<p><font size=3D3 face=3D"Times New Roman"><span lang=3DEN-GB =
style=3D'font-size:12.0pt'>2002
oct. 04 22:04:44.5 UT (JD=3D2452552.41996) : 18.29<br>
2002 oct. 04 22:12:01.7 UT (JD=3D2452552.42502) : 18.37<br>
2002 oct. 04 22:20:32.3 UT (JD=3D2452552.43093) : 18.40<br>
2002 oct. 04 23:51:04.3 UT (JD=3D2452552.49380) : 18.67<br>
2002 oct. 04 23:57:13.2 UT (JD=3D2452552.49807) : =
18.65</span></font></p>

<p><font size=3D3 face=3D"Times New Roman"><span lang=3DEN-GB =
style=3D'font-size:12.0pt'>Dates
are middle of exposures. This data fill nicely a gap around T0 + 0.4 =
when the
decay index of the light curve increases.</span></font></p>

<p><font size=3D3 face=3D"Times New Roman"><span lang=3DEN-GB =
style=3D'font-size:12.0pt'>.
</span></font></p>

<p class=3DMsoNormal><font size=3D3 face=3D"Times New Roman"><span =
lang=3DEN-GB
style=3D'font-size:12.0pt'>&nbsp;</span></font></p>

<p class=3DMsoNormal><font size=3D3 face=3D"Times New Roman"><span =
lang=3DEN-GB
style=3D'font-size:12.0pt'>&nbsp;</span></font></p>

<p class=3DMsoNormal><font size=3D3 face=3D"Times New Roman"><span =
lang=3DEN-GB
style=3D'font-size:12.0pt'>&nbsp;</span></font></p>

</div>

</body>

</html>

------=_NextPart_000_0034_01C2703E.C401F0E0--

VSNET Home Page

Return to Daisaku Nogami


vsnet-adm@kusastro.kyoto-u.ac.jp