|The bright optical afterglow of
GRB030329 was imaged March 31, 2003
23 UT through Rc filter.
Copyright: Nyrölä Observatory, 2003
OBSERVATION REPORT A. Oksanen on behalf of Nyrola observatory GRB Team reports: The bright afterglow was observed with the 0.4 SCT telescope of Nyrölä observatory using short (60/120 s) exposures and Rc-filter. Sky was almost cloudy, but time to time the afterglow was visible and measurable. Photometry (AIP4Win) from the best frames (Henden photometry file reference) follows: see photometry_20030329.txt
TITLE: GCN GRB OBSERVATION REPORT NUMBER: 2010 SUBJECT: GRB 030329: visual observations DATE: 03/03/30 00:33:03 GMT FROM: Arto Oksanen at Nyrola Obs., Finland
A. Oksanen (Nyrola Observatory), R. Henriksson and M. Tuukkanen (the Finnish Deep Sky section of Astronomical Association Ursa) report: We observed the optical afterglow of GRB030329 reported by Peterson and Price (GCN 1985) visually about 8 hours after the burst. M. Tuukkanen observed the OT In Pornainen, Finland with a 0.63 m Newton telescope for about one hour starting March 29, 2003 19:30 UT. He reported it as a faint starlike object seen easily with direct vision. He did not see any flickering or distinct color. R. Henriksson was observing in Orivesi, Finland with his 0.30 m Newton telescope using 200x magnification at 20:05 UT. He reported the object stellar and faint, visible only with averted vision. His scanned sketch with notes is available on web: http://archive.ermiksson.net/record.php?id=4112 Both observers estimated the visual magnitude as 14.3 by using the 14.2 magnitude GSC 1434:322 star North of OT as reference. This message may be cited.
TITLE: GCN GRB OBSERVATION REPORT NUMBER: 2058 SUBJECT: AAVSO V & R observations of GRB030329 DATE: 03/04/01 02:44:00 GMT FROM: AAVSO GRB Network at AAVSO
A. Price (AAVSO) reports on behalf of the AAVSO International GRB Network: The AAVSO International GRB Network has obtained B, V, R, and unfiltered photometry of the afterglow to GRB030329 from numerous sources across the globe over the past 3 days. See notes for details and access to time series data. Berto Monard, South Africa Unfiltered = 14.06 @ 2003.03.29 17:15 to Unfiltered = 15.01 @ 2003.03.29 23:37 exposures: 317X45-60s Arto Oksanen, 0.4m at Nyrola Observatory, Finland R = 14.50 @ 2003.03.29 20:22:23 to R = 14.75 @ 2003.03.29 22:28:03 exposures: 10X120s (out of 148 total) Tim Schrabback and Anja von der Linden, 1.06m at Observatory Hoher List of Bonn University, Germany R = 15.0 @ 2003.03.29 22:55 exposure: 1800s Peter Brown, 0.41m at Orson Pratt Observatory, Brigham Young University, Utah USA R = 15.2 @ 2003.03.30 02:38 to R = 16.2 @ 2003.03.30 10:41 exposures: 1X300s Dan Kaiser, 0.35m at Crescent Moon Observatory, Indiana USA V = 16.62 2003.03.31 01:32:04 to V = 16.97 2003.03.31 06:18:06 R = 16.26 2003.03.31 02:10:12 to R = 16.53 2003.03.31 06:22:37 Bill Aquino, 0.3m with Buffalo Astronomical Association in New York, USA V = 16.71 @ 2003.03.31 05:33:03 exposures: 4X180s exposure Notes: * Detailed reports (observing equipment, location, conditions, etc.) and many original FITS files available at ftp://ftp.aavso.org/grb/GRB030329 or by e-mailing email@example.com. * Brown, Kaiser, Monard, and Oksanen have time series data spanning the observations posted here. Full data has already been or will be posted soon to the URL above. * Aquino, Kaiser, and Oksanen used comparison star photometry from Henden et al. (GCN 2023). Brown used comp star A described on the finder chart by Rumyantsev et al. (GCN 2005). Schrabback et al. used comp star A described on a different finder chart by Martini et al.(GCN 2012). Monard's comp star is from USNOA2, 14.0R, 3' NNE of GRB. * The decay rate in Monard's exposure varies from 0.191 CR/h in the beginning of the run to 0.103 CR/h at the end. Kaiser's time series data is fairly constant until about 5:40 when the OT begins to fade again. The CCD used by Oksanen plus other components of the AAVSO International GRB network were funded by a generous grant from the Curry Foundation.
OBSERVATION REPORT A. Oksanen on behalf of Nyrola observatory GRB Team reports: Photometry run in V and Rc was performed with the 0.40 m SCT telescope under good conditions from March 31 19:00 UT to April 1, 2003 01:30 UT. The light curves are pretty flat as expected, but there is one intresting feature near noise level. The OT started to fade faster around 23 UT and then started to rise again. This 0.1 magnitude dip is visible both in Rc and V. BUT the dip seem to be 30 minutes later in R! Attendum April 4, 2003: This dip was not confirmed statistically from the data. More datailed analysis is in progress.
TITLE: GCN GRB OBSERVATION REPORT NUMBER: 2104 SUBJECT: GRB030329: More AAVSO VR obs DATE: 03/04/06 19:40:40 GMT FROM: AAVSO GRB Network at AAVSO
A. Price, B. Monard, A. Oksanen, T. DiLapo, D. West, D. Kaiser, D. Starkey, P. Nelson, P. Pääkkönen and J. Mattei (AAVSO); T. Durig, A. L. Seifert, C. B. Norton, G.F. Garland, J.K.Cole, J.B. Cherry (University of the South); A. Henden (USRA/USNO) report on behalf of the AAVSO International GRB Network: This is a 3rd set of observations of the OT found by Peterson and Price (GCN 1985) dating from March 29th to April 6th. Included in the observations is a URL where a full report (equipment, seeing, etc.) is available. Many times the original FITS image is also available. When time series data is available we only put the first and last observation. A light curve of all AAVSO data to date has been made by B. Gary and posted at http://www.aavso.org/grb/grb030329.jpg Bruce L. Gary, .25m at Arizona, USA. Rc = 15.67 +/- 0.04 @ 2003.03.30 07:08 to Rc = 16.82 +/- 0.04 @ 2003.03.30 04:26 V = 15.89 +/- 0.06 @ 2003.03.30 07:16 to V = 16.13 +/- 0.04 @ 2003.04.01 08:38 Rc = 18.07 +/- 0.05 @ 2003.04.05 03:49 Rc = 18.78 +/- 0.12 @ 2003.04.06 03:50 exposures:64X15s,70X30s(for last obs) ftp://ftp.aavso.org/grb/GRB030329/BruceL.Gary_GRB030329_2452731.81361_.txt Arto Oksanen and Petri Tikkanen, .4m at Nyrola Observatory, Finland. Rc = 16.714 merr: 0.051 @ 2003.03.31 19:09 to Rc = 16.842 merr: 0.060 @ 2003.04.01 00:59 V = 17.157 merr: 0.053 @ 2003.03.31 19:48 to V = 17.297 merr: 0.077 @ 2003.04.01 00:55 Rc = 18.59 merr: 0.04 @ 2003.04.05 21:35 exposures: 78x240s, 34x240s (last obs) ftp://ftp.aavso.org/grb/GRB030329/arto-030329-2nreport.txt http://nyrola.jklsirius.fi/grb/grb030329/ Tristan DiLapo, .31m at Orbit Jet Observatory, New York, USA. Rc = 16.32 err: 0.06 @ 2003.03.31 02:56 to Rc = 16.34 err: 0.06 @ 2003.03.31 04:02 exposures: 10X120s ftp://ftp.aavso.org/grb/GRB030329/TristanDiLapo_GRB030329_2452732.28043_.txt Doug West, .2m at West Skies Observatory, Kansas, USA. Unfiltered = 17.2 +/- 0.14 2003.04.02 02:08 7*30s exposures Unfiltered = 17.5 +/- 0.13 2003.04.04 02:09 14*35s exposures Unfiltered = 18.3 +/- 0.20 2003.04.05 02:11 19X35s exposures exposures: 7X30s ftp://ftp.aavso.org/grb/GRB030329/west-grb030329.txt Dan Kaiser, .35m at Crescent Moon Observatory, Indiana, USA. Rc = 17.44 @ 2003.04.02 02:13 exposures: 14X240s ftp://ftp.aavso.org/grb/GRB030329/kaiser-grb030329.txt D. T. Durig, A. L. Seifert, C. B. Norton, G.F. Garland, J.K.Cole, J.B. Cherry, .3m at Cordell-Lorenz Observatory, Tennessee, USA Rc = 17.96 @ 2003.04.02 02:36 Rc = 18.06 @ 2003.04.02 03:38 Rc = 18.36 +/- 0.2 @ 2003.04.03 03:45 Rc = 18.46 +/- 0.2 @ 2003.04.03 03:59 exposures: 4X600s ftp://ftp.aavso.org/grb/GRB030329/DrDouglasT.Durig_GRB030329_2452732.69648_.txt Donn Starkey, .36m at DeKalb Observatory, Indiana, USA. Rc = 16.06 @ 2003.04.02 04:30 Bu = 18.02 @ 2003.04.02 05:44 V = 16.85 @ 2003.04.02 04:52 ftp://ftp.aavso.org/grb/GRB030329/DonnStarkey_GRB030329_2452731.82174_.txt Peter Nelson, .32m at Ellinbank Observatory, Australia. Rc = 18.3 +/- 0.3 @ 2003.04.03 13:00 exposures: 3X300s ftp://ftp.aavso.org/grb/GRB030329/PeterNelson_GRB030329_2452734.05919_.txt Pertti Pääkkönen, .5m at Jakokoski Observatory, Finland. Rg = 18.55 +/- 0.04 @ 2003.04.05 22:12 exposures: 33X300s ftp://ftp.aavso.org/grb/PerttiPääkkönen_GRB030329_2452736.16987_.txt http://cc.joensuu.fi/seulaset/ccd/20030405/ Correction: The data below is a recalculation (based on a better comp star) of data posted earlier in GCN 2058. Berto Monard, .3m at Bronberg Observatory. South Africa Unfiltered: 13.8 @ 2003.03.29 17:15 to Unfiltered: 14.7 @ 2003.03.29 23:37 ftp://ftp.aavso.org/grb/GRB030329/monard-GRB030329mar29.txt * Durig et al., Gary, Starkey, Oksanen, West, Nelson, Pääkkönen and Kaiser used Henden et al. photometry (GCN 2023) for comparison. DiLapo used USNOA2. Monard used Tycho-2. * Pääkkönen's R filter (Rg) is a custom designed filter. Info at: http://cc.joensuu.fi/seulaset/ccd/rgbfilters.png The AAVSO International GRB network is greatful for a generous grant from the Curry Foundation and to NASA for the financial support for the High Energy Workshops for Amateur Astronomers.
The afterglow was imaged with Rc filter on April 9/10, 2003 20:37-00:12 UT (11 days after the burst!). Total of 50 240s exposures were stacked using Sigma Reject average. The afterglow magnitude was measured with MaxIm/DL to R=19.17 +/- 0.07 on the mid epoch of April 9.93 UT using all eight reference stars from the AAVSO f-scale chart based on Henden photometry file.
TITLE: GCN GRB OBSERVATION REPORT NUMBER: 2156 SUBJECT: GRB030329: 444 AAVSO Measurements DATE: 03/04/20 03:21:34 GMT FROM: AAVSO GRB Network at AAVSO
A. Price (AAVSO); B. Aquino (AWJ); E. Broens (BOS) & J. Hambsch (HJB) (VVS Werkgroep Veranderlijke Sterren); P. Brown (OPO01 - Brigham Young University); T. DiLapo (DLN); B. Dillon (DIL) & J. Dellinger, D. Beaver, P. Garossino, T. Garossino; N. Dunckel (DNI); T. Durig & A. L. Seifert, C. B. Norton, G.F. Garland, J.K. Cole, J.B. Cherry (CLW01 - University of the South); B. Gary (GBL); B. Granslo (GRL); A. Henden (USRA/USNO); D. Hohman (HDF); D. Kaiser (KDA); Z. Kereszty (KZX); P. Kilmartin & A. Gilmore (KPM - University of Canterbury) J. Liesmann (LJI); G. Lubcke (LBG); J. Mattei (AAVSO); B. Monard (MLF); P. Nelson (NLX); A. Oksanen (OAR) & P. Tikkanen (TPE); P. Pääkkönen (PPK); D. Starkey (SDB); A. von der Linden & T. Schrabback (XXX - IAEF, Bonn University); D. West (WJD) report on behalf of the AAVSO International GRB Network: The AAVSO has 444 measurements of of the GRB030329 OT found by Peterson and Price (GCN 1985) spanning 03:47 on March 31 to 03:09 on April 17, 2003. All observations have been rereduced using the final photometry from Henden et al. (GCN 2114) A light curve, all data plus a finder chart with the comparison and check stars used is available at this URL: http://www.aavso.org/grb/grb030329.shtml Full reports including equipment and site info are available at ftp://ftp.aavso.org/grb/GRB030329 Many of the FITS images are available there as well. The AAVSO International GRB network is grateful for a generous grant from the Curry Foundation and to NASA for the financial support for the High Energy Workshops for Amateur Astronomers.