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Nouveau transit
12/04/2022
XO-1 b
135
O. Tercu, G. Neagu, D. Zlat, A. Lupoae, Galati Observatory, C73
RC 0.4m, f/8 + CCD SBIG STL-6303E
Observed in r. Exposed 60 seconds.
Observed in r. Exposed 60 seconds.
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Nouveau transit
19/07/2020
XO-1 b
135
D. Bertesteanu, I.C.Tudor, L. Demetz, SkyGems Observatory- Hakos, Namibia
20' AG Optical iDK, FL 3400mm, FLI Proline 16803
120 sec exposures, bin 1x1
120 sec exposures, bin 1x1
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Nouveau transit
16/07/2020
XO-1 b
135
Alfa Crucis - Colesanti C, De Carvalho Aguiar P, Kulh D, Napoleao T, Olim E, Rodrigues MA, Treü R, Orion Observatory - Mairinque, Sao Paulo, Brazil
12 inch Schmidt-Cassegrain (305mm, f/10), focal reducer f/3.3, Sensor: SBIG ST-7XME, Mount: Paramount MX
25s exposures binned 1x1. Each data point is the average of 5 images. Weighted ensemble photometry with 2 comp stars, apertures (6, 11, 17) More about Alfa Crucis: https://alfacrucis.org/
25s exposures binned 1x1. Each data point is the average of 5 images. Weighted ensemble photometry with 2 comp stars, apertures (6, 11, 17) More about Alfa Crucis: https://alfacrucis.org/
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Nouveau transit
10/07/2020
XO-1 b
135
O. Tercu, G. Neagu, D. Zlat, A. Lupoae, Galati Observatory, C73
RC 0.4m, f/8 + CCD SBIG STL-6303E
Observed in r. Exposed 60 seconds.
Observed in r. Exposed 60 seconds.
. . .
N-8" f/4.7 on EQ6; SBIG ST-8XME, Johnson-Cousins BVRcIc filters
150" exposures. Flip-pier run between t=0.52-0.54. Although bias, dark and flat-field correction have been rigorously applied, an off-set of -0.006 mag. should be applied to post flip-pier data in order to compensate the systemathic error generated.
150" exposures. Flip-pier run between t=0.52-0.54. Although bias, dark and flat-field correction have been rigorously applied, an off-set of -0.006 mag. should be applied to post flip-pier data in order to compensate the systemathic error generated.
. . .
Nouveau transit
25/02/2017
XO-1 b
135
Collège Antoine Courrière, IRIS - Observatoire de Haute Provence
50 cm - F/8 - ProLine 4240
http://iris.lam.fr/
http://iris.lam.fr/
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Nouveau transit
06/04/2016
XO-1 b
135
Alessandro Marchini, Astronomical Observatory, University of Siena
Mak-Cas 30cm f/5.6, CCD Sbig STL-6303
Data acquisition and analysis performed by some high school students involved in guidance astronomical activities: F.Benincasa (Liceo Sarrochi Siena), F.Cigalotti, M.Valenti (Liceo Galilei Siena), M.Bastiani (Liceo Bandini Siena), G.La Rosa (Liceo Volta Colle VE)
Data acquisition and analysis performed by some high school students involved in guidance astronomical activities: F.Benincasa (Liceo Sarrochi Siena), F.Cigalotti, M.Valenti (Liceo Galilei Siena), M.Bastiani (Liceo Bandini Siena), G.La Rosa (Liceo Volta Colle VE)
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Nouveau transit
07/08/2014
XO-1 b
135
Fabio Martinelli, Montecatini val di Cecina Astronomical Centre
SC 14\\\\\\\" f/6.3 CCD ST8-XME
. . .
Nouveau transit
24/05/2014
XO-1 b
135
CAAT - Centro Astronomico del Alto Turia, CAAT - Centro Astronomico del Alto Turia MPC-J57
Meade LX200 16\\\" + SBIG ST-7XME
30 seconds unfiltered
30 seconds unfiltered
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Nouveau transit
20/05/2012
XO-1 b
135
Stanislav Poddaný, Štefánik observatory, Prague, Czech Republic
Meade LX 200 40,6 cm, SBIG ST10XME
exp. 60s, no autoguide
exp. 60s, no autoguide
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Nouveau transit
07/04/2012
XO-1 b
135
Stan Shadick and Christine Shiels, University of Saskatchewan Physics Roof Observatory
Meade 12\\\" LX200; SBIG ST10XME CCD
Processed with artificial star at 6x4x10 at binning 2.
Used only reference stars C1-C6.
Pier 5.
Processed with artificial star at 6x4x10 at binning 2.
Used only reference stars C1-C6.
Pier 5.
. . .
Nouveau transit
11/03/2011
XO-1 b
135
Stan Shadick, University of Saskatchewan Physics Roof Observatory
Meade 12\\\" LX200; SBIG ST10XMECCD
cbb filter
Processed using Bruce Gary\\\'s artificial star spreadsheet technique at 7x4x10
Only used comparison stars C2, C4 and C12 in final analysis
cbb filter
Processed using Bruce Gary\\\'s artificial star spreadsheet technique at 7x4x10
Only used comparison stars C2, C4 and C12 in final analysis
. . .
Nouveau transit
30/04/2010
XO-1 b
135
Stan Shadick, University of Saskatchewan Physics Roof Observatory
Meade 12\\\" LX200; STL1301CCD
Following testing with Artificial Star technique, processed using reference stars 2, 4, 7, 10 and 13 only on attached map
Following testing with Artificial Star technique, processed using reference stars 2, 4, 7, 10 and 13 only on attached map
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