This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q1b1x1_002859_TTUQ1b1x1_2792272_V09vR6vv
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 05 26.2261 2461186.7261 11.48 18:48:23.57 -04:16:42.2
28.77692 -1.27355 galactic Sct Second-epoch detections are separated by 2.6" and 5.3 pix
The object was found in VSX19" ZTF J184822.77-041656.6
Type: SR
# Max. Min./Amp. JD0 Period
14.202 r Y 0.424 r 2458292.52130 78.624062300000
The object was not found in astcheck.
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:48:23.57 -04:16:42.2: 12.38 +/- 0.03 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:48:23.57 -04:16:42.2: 12.48 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.42 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J184822.77-041656.6,2461186.7261,11.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J184822.77-041656.6 20260526.2261 11.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2261 2461186.7261 11.28 18:56:10.70 -00:15:44.4
33.23885 -1.17434 galactic Aql Second-epoch detections are separated by 2.8" and 5.2 pix
The object was found in VSX 2" V0867 Aql
Type: M
# Max. Min./Amp. JD0 Period
13.400 pg 16.200 pg 2437528.00000 195.160000000000 M7e
The object was not found in astcheck.
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:56:10.70 -00:15:44.4: 12.23 +/- 0.02 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:56:10.70 -00:15:44.4: 12.50 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.32 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0867 Aql,2461186.7261,11.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0867 Aql 20260526.2261 11.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2261 2461186.7261 11.35 18:42:33.14 -05:52:11.3
26.69687 -0.70572 galactic Sct Second-epoch detections are separated by 1.0" and 5.4 pix
The object was found in VSX 3" NSVS 13945073
Type: L:
# Max. Min./Amp. JD0 Period
11.380 R1 Y 0.100 R1
The object was not found in astcheck.
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:42:33.14 -05:52:11.3: 12.76 +/- 0.05 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:42:33.14 -05:52:11.3: 13.02 +/- 0.06 detection
Forced photometry reference-image weighted average: 12.86 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 13945073,2461186.7261,11.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 13945073 20260526.2261 11.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2261 2461186.7261 11.55 18:51:55.89 -03:53:31.5
29.52296 -1.88327 galactic Sct Second-epoch detections are separated by 1.6" and 5.5 pix
The object was found in VSX 1" GDS_J1851559-035331
Type: VAR
# Max. Min./Amp. JD0 Period
12.120 r Y 0.170 r
The object was not found in astcheck.
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:51:55.89 -03:53:31.5: 12.56 +/- 0.03 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:51:55.89 -03:53:31.5: 12.72 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.62 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GDS_J1851559-035331,2461186.7261,11.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J1851559-035331 20260526.2261 11.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2261 2461186.7261 11.20 18:38:28.86 -06:11:48.5
25.94263 0.04437 galactic Sct Second-epoch detections are separated by 2.1" and 5.8 pix
The object was found in VSX 1" NSVS 13940204
Type: LPV
# Max. Min./Amp. JD0 Period
10.930 R1 Y 0.160 R1 262.470000000000
The object was not found in astcheck.
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:38:28.86 -06:11:48.5: 12.28 +/- 0.02 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:38:28.86 -06:11:48.5: 12.64 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.38 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 13940204,2461186.7261,11.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 13940204 20260526.2261 11.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2261 2461186.7261 11.57 18:52:17.95 -04:29:22.7
29.03218 -2.23671 galactic Sct Second-epoch detections are separated by 0.8" and 5.4 pix
The object was found in VSX 1" GDS_J1852178-042921
Type: VAR
# Max. Min./Amp. JD0 Period
12.210 r Y 0.180 r
The object was not found in astcheck.
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:52:17.95 -04:29:22.7: 12.61 +/- 0.03 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:52:17.95 -04:29:22.7: 12.66 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.63 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GDS_J1852178-042921,2461186.7261,11.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J1852178-042921 20260526.2261 11.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2261 2461186.7261 11.59 18:47:34.16 -04:36:35.5
28.38824 -1.24193 galactic Sct Second-epoch detections are separated by 1.2" and 5.3 pix
The object was found in VSX 2" GDS_J1847348-043636
Type: VAR
# Max. Min./Amp. JD0 Period
12.050 r Y 0.260 r C
The object was not found in astcheck.
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:47:34.16 -04:36:35.5: 12.63 +/- 0.04 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:47:34.16 -04:36:35.5: 12.87 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.71 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GDS_J1847348-043636,2461186.7261,11.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J1847348-043636 20260526.2261 11.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2261 2461186.7261 10.97 18:42:44.42 -06:15:55.8
26.36625 -0.92815 galactic Sct Second-epoch detections are separated by 0.5" and 5.5 pix
The object was found in ASASSN-V 4" ASASSN-V J184244.22-061557.7
Type: SR
MeanMag 12.36 m Amp. 0.09 m Period 27.2801398 d
The object was not found in astcheck.
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:42:44.42 -06:15:55.8: 11.94 +/- 0.03 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:42:44.42 -06:15:55.8: 12.07 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.00 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461186.7261,10.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260526.2261 10.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2261 2461186.7261 11.47 18:42:17.40 -05:48:53.9
26.71580 -0.62262 galactic Sct Second-epoch detections are separated by 2.5" and 5.8 pix
The object was found in VSX 2" GDS_J1842172-054855
Type: VAR
# Max. Min./Amp. JD0 Period
12.560 r Y 0.310 r M5Ib
The object was not found in astcheck.
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:42:17.40 -05:48:53.9: 12.61 +/- 0.05 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:42:17.40 -05:48:53.9: 12.83 +/- 0.06 detection
Forced photometry reference-image weighted average: 12.70 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GDS_J1842172-054855,2461186.7261,11.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J1842172-054855 20260526.2261 11.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2261 2461186.7261 11.56 19:02:38.10 +01:19:22.8
35.38692 -1.88679 galactic Aql Second-epoch detections are separated by 2.6" and 5.1 pix
The object was found in VSX 1" ASAS J190238+0119.3
Type: MISC
# Max. Min./Amp. JD0 Period
8.685 Ic Y 0.592 Ic 2452737.30000 252.400000000000 M8
The object was not found in astcheck.
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 19:02:38.10 +01:19:22.8: 12.60 +/- 0.03 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 19:02:38.10 +01:19:22.8: 12.77 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.66 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J190238+0119.3,2461186.7261,11.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J190238+0119.3 20260526.2261 11.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2261 2461186.7261 11.19 18:49:44.64 -03:49:31.9
29.33372 -1.36716 galactic Aql Second-epoch detections are separated by 1.9" and 5.3 pix
The object was found in VSX 1" ASAS J184945-0349.6
Type: MISC
# Max. Min./Amp. JD0 Period
8.972 Ic Y 0.236 Ic 2452669.10000 98.800000000000
The object was not found in astcheck.
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:49:44.64 -03:49:31.9: 12.37 +/- 0.02 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:49:44.64 -03:49:31.9: 12.59 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.44 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J184945-0349.6,2461186.7261,11.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J184945-0349.6 20260526.2261 11.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2261 2461186.7261 11.04 18:42:35.13 -05:22:13.6
27.14478 -0.48475 galactic Sct Second-epoch detections are separated by 1.9" and 5.6 pix
The object was found in VSX 2" GDS_J1842351-052211
Type: VAR
# Max. Min./Amp. JD0 Period
11.620 r Y 0.090 r
The object was not found in astcheck.
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:42:35.13 -05:22:13.6: 11.91 +/- 0.02 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:42:35.13 -05:22:13.6: 12.16 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.00 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GDS_J1842351-052211,2461186.7261,11.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J1842351-052211 20260526.2261 11.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2261 2461186.7261 11.10 18:46:44.64 -04:16:41.7
28.58960 -0.90764 galactic Sct Second-epoch detections are separated by 1.3" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4258192896989325952 | 18:46:44.68 -04:16:42.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: M2 1964AbaOB..31...27A [A64] Red -04 165 J-Ks=1.585+/-0.032 (Very red! L if it's a dwarf)
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:46:44.64 -04:16:41.7: 11.91 +/- 0.02 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:46:44.64 -04:16:41.7: 12.16 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.00 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4258192896989325952,2461186.7261,11.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4258192896989325952 20260526.2261 11.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2261 2461186.7261 10.89 18:42:03.84 -05:04:57.8
27.34128 -0.23771 galactic Sct Second-epoch detections are separated by 2.4" and 5.8 pix
The object was found in VSX 1" GDS_J1842038-050457
Type: SR
# Max. Min./Amp. JD0 Period
11.760 r Y 0.280 r 2458372.91370 43.868131200000 M3
The object was not found in astcheck.
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:42:03.84 -05:04:57.8: 11.91 +/- 0.02 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:42:03.84 -05:04:57.8: 12.18 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.01 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GDS_J1842038-050457,2461186.7261,10.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J1842038-050457 20260526.2261 10.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2261 2461186.7261 11.41 18:46:27.11 -05:49:54.8
27.17336 -1.55129 galactic Sct Second-epoch detections are separated by 2.9" and 5.9 pix
The object was found in VSX 4" GDS_J1846269-054956
Type: SR
# Max. Min./Amp. JD0 Period
12.360 r Y 0.390 r 2457137.05000 31.270000000000
The object was not found in astcheck.
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:46:27.11 -05:49:54.8: 12.37 +/- 0.03 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:46:27.11 -05:49:54.8: 12.51 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.42 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GDS_J1846269-054956,2461186.7261,11.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J1846269-054956 20260526.2261 11.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2261 2461186.7261 10.76 18:44:01.87 -05:31:51.4
27.16642 -0.87812 galactic Sct Second-epoch detections are separated by 1.5" and 5.6 pix
The object was found in VSX 2" NSVS 13947066
Type: LPV:
# Max. Min./Amp. JD0 Period
10.700 R1 Y 0.240 R1 408.660000000000
The object was not found in astcheck.
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:44:01.87 -05:31:51.4: 11.88 +/- 0.02 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:44:01.87 -05:31:51.4: 12.11 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.97 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 13947066,2461186.7261,10.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 13947066 20260526.2261 10.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2261 2461186.7261 11.36 19:00:02.00 +01:41:01.9
35.41077 -1.14355 galactic Aql Second-epoch detections are separated by 1.7" and 5.7 pix
The object was found in VSX 1" ASAS J190002+0141.0
Type: MISC
# Max. Min./Amp. JD0 Period
8.824 Ic Y 0.187 Ic 2452466.20000 35.280000000000
The object was not found in astcheck.
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 19:00:02.00 +01:41:01.9: 12.31 +/- 0.02 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 19:00:02.00 +01:41:01.9: 12.39 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.35 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J190002+0141.0,2461186.7261,11.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J190002+0141.0 20260526.2261 11.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2261 2461186.7261 11.41 18:52:15.62 -04:12:09.2
29.28364 -2.09754 galactic Sct Second-epoch detections are separated by 2.2" and 5.2 pix
The object was found in VSX 5" Gaia DR3 4255247477115930368
Type: L
# Max. Min./Amp. JD0 Period
18.070 G 18.410 G
The object was not found in astcheck.
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:52:15.62 -04:12:09.2: 12.31 +/- 0.02 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:52:15.62 -04:12:09.2: 12.43 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.36 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4255247477115930368,2461186.7261,11.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4255247477115930368 20260526.2261 11.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2261 2461186.7261 11.29 19:08:04.45 +01:39:31.3
36.30834 -2.94178 galactic Aql Second-epoch detections are separated by 0.7" and 5.5 pix
The object was found in VSX 2" ASAS J190805+0139.6
Type: MISC
# Max. Min./Amp. JD0 Period
8.926 Ic Y 0.177 Ic 2452484.50000 65.060000000000 M3
The object was not found in astcheck.
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 19:08:04.45 +01:39:31.3: 12.31 +/- 0.03 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 19:08:04.45 +01:39:31.3: 12.23 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.27 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J190805+0139.6,2461186.7261,11.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J190805+0139.6 20260526.2261 11.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2261 2461186.7261 11.47 18:43:09.26 -05:45:44.5
26.86088 -0.78978 galactic Sct Second-epoch detections are separated by 0.6" and 5.5 pix
The object was found in VSX 2" GDS_J1843092-054545
Type: SR
# Max. Min./Amp. JD0 Period
14.347 g Y 0.338 g 2458314.61690 58.806533400000
The object was not found in astcheck.
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:43:09.26 -05:45:44.5: 12.79 +/- 0.06 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:43:09.26 -05:45:44.5: 13.00 +/- 0.07 detection
Forced photometry reference-image weighted average: 12.87 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GDS_J1843092-054545,2461186.7261,11.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J1843092-054545 20260526.2261 11.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2261 2461186.7261 11.74 18:54:06.84 -03:35:11.8
30.04301 -2.22917 galactic Aql Second-epoch detections are separated by 0.6" and 5.6 pix
The object was found in VSX 0" GDS_J1854068-033512
Type: VAR
# Max. Min./Amp. JD0 Period
12.510 r Y 0.270 r
The object was not found in astcheck.
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:54:06.84 -03:35:11.8: 12.81 +/- 0.04 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:54:06.84 -03:35:11.8: 13.06 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GDS_J1854068-033512,2461186.7261,11.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J1854068-033512 20260526.2261 11.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2261 2461186.7261 10.88 18:47:05.58 -03:31:45.4
29.29588 -0.64345 galactic Aql Second-epoch detections are separated by 0.4" and 5.4 pix
The object was found in VSX 0" Brh V120
Type: LPV
# Max. Min./Amp. JD0 Period
12.700 w 12.900 w M5
The object was not found in astcheck.
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:47:05.58 -03:31:45.4: 11.79 +/- 0.01 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:47:05.58 -03:31:45.4: 12.04 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.88 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Brh V120,2461186.7261,10.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Brh V120 20260526.2261 10.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2261 2461186.7261 10.72 18:41:00.87 -05:51:40.1
26.52962 -0.36167 galactic Sct Second-epoch detections are separated by 1.0" and 5.6 pix
The object was found in VSX 0" ASASSN-V J184100.87-055140.5
Type: SRS
# Max. Min./Amp. JD0 Period
12.470 V 12.570 V 2458186.09700 27.798000000000
The object was not found in astcheck.
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:41:00.87 -05:51:40.1: 11.73 +/- 0.02 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:41:00.87 -05:51:40.1: 11.90 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.80 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J184100.87-055140.5,2461186.7261,10.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J184100.87-055140.5 20260526.2261 10.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2261 2461186.7261 11.31 18:38:36.26 -06:52:40.1
25.35156 -0.29524 galactic Sct Second-epoch detections are separated by 1.2" and 5.3 pix
The object was found in VSX 1" ASASSN-V J183836.18-065240.9
Type: SRS:
# Max. Min./Amp. JD0 Period
14.890 g Y 0.260 g 2458699.22300 8.001600000000
The object was not found in astcheck.
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:38:36.26 -06:52:40.1: 12.26 +/- 0.03 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:38:36.26 -06:52:40.1: 12.45 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.33 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J183836.18-065240.9,2461186.7261,11.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J183836.18-065240.9 20260526.2261 11.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2261 2461186.7261 10.12 19:03:12.37 +02:16:05.5
36.29316 -1.58141 galactic Aql Second-epoch detections are separated by 0.6" and 5.5 pix
The object was found in VSX 1" ASAS J190312+0216.1
Type: MISC
# Max. Min./Amp. JD0 Period
7.725 Ic Y 0.289 Ic 2452604.60000 82.410000000000 M8
The object was not found in astcheck.
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 19:03:12.37 +02:16:05.5: 11.01 +/- 0.01 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 19:03:12.37 +02:16:05.5: 11.10 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.05 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J190312+0216.1,2461186.7261,10.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J190312+0216.1 20260526.2261 10.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2261 2461186.7261 11.51 18:44:02.34 -04:52:58.4
27.74387 -0.58386 galactic Sct Second-epoch detections are separated by 1.6" and 5.4 pix
The object was found in VSX 1" ASASSN-V J184402.28-045259.5
Type: L
# Max. Min./Amp. JD0 Period
13.160 V 13.290 V
The object was not found in astcheck.
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:44:02.34 -04:52:58.4: 12.47 +/- 0.04 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:44:02.34 -04:52:58.4: 12.72 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.56 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J184402.28-045259.5,2461186.7261,11.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J184402.28-045259.5 20260526.2261 11.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2261 2461186.7261 11.22 18:52:12.40 -04:23:38.1
29.10700 -2.17265 galactic Sct Second-epoch detections are separated by 2.1" and 5.6 pix
The object was found in VSX 2" GDS_J1852124-042339
Type: VAR
# Max. Min./Amp. JD0 Period
11.790 r Y 0.090 r
The object was not found in astcheck.
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:52:12.40 -04:23:38.1: 12.22 +/- 0.02 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:52:12.40 -04:23:38.1: 12.29 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.25 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GDS_J1852124-042339,2461186.7261,11.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J1852124-042339 20260526.2261 11.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2261 2461186.7261 10.73 18:46:27.77 -04:33:22.9
28.31011 -0.97213 galactic Sct Second-epoch detections are separated by 1.8" and 5.8 pix
The object was found in VSX 0" GDS_J1846277-043322
Type: VAR
# Max. Min./Amp. JD0 Period
11.620 r Y 0.280 r M5
The object was not found in astcheck.
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:46:27.77 -04:33:22.9: 11.63 +/- 0.01 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:46:27.77 -04:33:22.9: 11.84 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.71 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GDS_J1846277-043322,2461186.7261,10.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J1846277-043322 20260526.2261 10.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2261 2461186.7261 11.38 18:45:27.10 -05:19:52.6
27.50550 -1.10153 galactic Sct Second-epoch detections are separated by 1.3" and 5.4 pix
The object was found in VSX 1" ASAS J184527-0519.9
Type: MISC
# Max. Min./Amp. JD0 Period
9.110 Ic Y 0.264 Ic 2452513.80000 72.380000000000
The object was not found in astcheck.
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:45:27.10 -05:19:52.6: 12.52 +/- 0.04 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:45:27.10 -05:19:52.6: 12.82 +/- 0.06 detection
Forced photometry reference-image weighted average: 12.62 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J184527-0519.9,2461186.7261,11.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J184527-0519.9 20260526.2261 11.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2261 2461186.7261 11.53 18:52:51.63 -01:20:09.9
31.90486 -0.92565 galactic Aql Second-epoch detections are separated by 2.5" and 5.5 pix
The object was found in VSX 2" ASAS J185252-0120.2
Type: SR
# Max. Min./Amp. JD0 Period
13.100 V 13.700 V 2457218.90000 50.730000000000
The object was not found in astcheck.
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:52:51.63 -01:20:09.9: 12.50 +/- 0.04 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:52:51.63 -01:20:09.9: 12.64 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.55 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J185252-0120.2,2461186.7261,11.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J185252-0120.2 20260526.2261 11.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2261 2461186.7261 10.66 18:40:53.07 -06:20:26.4
26.08847 -0.55244 galactic Sct Second-epoch detections are separated by 0.5" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4253015258043515520 | 18:40:53.04 -06:20:27.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.587+/-0.036 (Very red! L if it's a dwarf)
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:40:53.07 -06:20:26.4: 11.57 +/- 0.01 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:40:53.07 -06:20:26.4: 11.77 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.65 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4253015258043515520,2461186.7261,10.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4253015258043515520 20260526.2261 10.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2261 2461186.7261 9.85 18:41:28.14 -06:52:36.2
25.67821 -0.92679 galactic Sct Second-epoch detections are separated by 0.7" and 5.6 pix
The object was found in VSX 1" ASAS J184128-0652.6
Type: MISC
# Max. Min./Amp. JD0 Period
11.190 V Y 0.420 V 2452472.21000 299.597443000000 S1.5*2
The object was not found in astcheck.
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:41:28.14 -06:52:36.2: 10.68 +/- 0.01 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:41:28.14 -06:52:36.2: 10.90 +/- 0.01 detection
Forced photometry reference-image weighted average: 10.76 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J184128-0652.6,2461186.7261,9.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J184128-0652.6 20260526.2261 9.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2261 2461186.7261 9.60 18:42:05.56 -05:00:50.1
27.40573 -0.21259 galactic Sct Second-epoch detections are separated by 0.6" and 5.6 pix
The object was found in VSX 1" ASAS J184205-0500.8
Type: MISC
# Max. Min./Amp. JD0 Period
12.090 V Y 0.760 V 2453170.00000 340.987915000000 M2
The object was not found in astcheck.
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:42:05.56 -05:00:50.1: 10.48 +/- 0.01 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:42:05.56 -05:00:50.1: 10.82 +/- 0.01 detection
Forced photometry reference-image weighted average: 10.59 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J184205-0500.8,2461186.7261,9.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J184205-0500.8 20260526.2261 9.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2261 2461186.7261 11.28 18:51:34.89 -03:16:31.8
30.03243 -1.52483 galactic Aql Second-epoch detections are separated by 0.5" and 5.4 pix
The object was found in VSX 1" GDS_J1851349-031632
Type: VAR
# Max. Min./Amp. JD0 Period
12.060 r Y 0.180 r
The object was not found in astcheck.
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:51:34.89 -03:16:31.8: 12.44 +/- 0.02 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:51:34.89 -03:16:31.8: 12.60 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.50 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GDS_J1851349-031632,2461186.7261,11.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J1851349-031632 20260526.2261 11.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2261 2461186.7261 11.26 18:50:05.51 -04:00:13.6
29.21451 -1.52558 galactic Sct Second-epoch detections are separated by 1.2" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4255309530840211840 | 18:50:05.50 -04:00:13.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.617+/-0.027 (Very red! L if it's a dwarf)
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:50:05.51 -04:00:13.6: 12.14 +/- 0.02 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:50:05.51 -04:00:13.6: 12.33 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.21 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4255309530840211840,2461186.7261,11.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4255309530840211840 20260526.2261 11.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2261 2461186.7261 11.81 18:52:25.84 -00:53:33.0
32.25073 -0.62782 galactic Aql Second-epoch detections are separated by 2.0" and 5.4 pix
The object was found in VSX 3" NSVS 13958087
Type: L
# Max. Min./Amp. JD0 Period
10.990 R1 Y 0.180 R1
The object was not found in astcheck.
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:52:25.84 -00:53:33.0: 12.89 +/- 0.04 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:52:25.84 -00:53:33.0: 13.09 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.97 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 13958087,2461186.7261,11.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 13958087 20260526.2261 11.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2261 2461186.7261 11.31 18:47:33.60 -05:08:13.4
27.91778 -1.48012 galactic Sct Second-epoch detections are separated by 1.1" and 5.7 pix
The object was found in ASASSN-V 3" ASASSN-V J184733.41-050814.2
Type: L
MeanMag 13.72 m Amp. 0.35 m Period d
The object was not found in astcheck.
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:47:33.60 -05:08:13.4: 12.44 +/- 0.03 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:47:33.60 -05:08:13.4: 12.81 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.55 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461186.7261,11.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260526.2261 11.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2261 2461186.7261 11.31 18:47:29.40 -05:02:36.0
27.99329 -1.42190 galactic Sct Second-epoch detections are separated by 0.9" and 5.6 pix
The object was found in VSX 0" GDS_J1847293-050236
Type: VAR
# Max. Min./Amp. JD0 Period
12.220 r Y 0.170 r M3
The object was not found in astcheck.
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:47:29.40 -05:02:36.0: 12.42 +/- 0.03 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:47:29.40 -05:02:36.0: 12.63 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.50 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GDS_J1847293-050236,2461186.7261,11.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J1847293-050236 20260526.2261 11.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2261 2461186.7261 11.79 19:00:55.16 +01:22:15.8
35.23364 -1.48343 galactic Aql Second-epoch detections are separated by 4.6" and 5.1 pix
The object was found in VSX 3" ASASSN-V J190055.09+012213.7
Type: SR
# Max. Min./Amp. JD0 Period
13.550 V 13.880 V 2458289.89260 44.474656900000
The object was not found in astcheck.
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 19:00:55.16 +01:22:15.8: 12.74 +/- 0.04 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 19:00:55.16 +01:22:15.8: 12.91 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.80 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J190055.09+012213.7,2461186.7261,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J190055.09+012213.7 20260526.2261 11.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2261 2461186.7261 10.54 18:57:56.01 -00:45:25.8
32.99841 -1.79046 galactic Aql Second-epoch detections are separated by 1.0" and 5.6 pix
The object was found in VSX 1" ASAS J185756-0045.4
Type: MISC
# Max. Min./Amp. JD0 Period
12.450 V Y 0.680 V 2452640.40000 246.478867000000 M5
The object was not found in astcheck.
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:57:56.01 -00:45:25.8: 11.44 +/- 0.01 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:57:56.01 -00:45:25.8: 11.63 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.51 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J185756-0045.4,2461186.7261,10.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J185756-0045.4 20260526.2261 10.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2261 2461186.7261 11.35 18:44:45.01 -06:21:22.3
26.51363 -1.41387 galactic Sct Second-epoch detections are separated by 1.8" and 5.7 pix
The object was found in VSX 2" GDS_J1844449-062123
Type: VAR
# Max. Min./Amp. JD0 Period
12.290 r Y 0.220 r
The object was not found in astcheck.
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:44:45.01 -06:21:22.3: 12.33 +/- 0.05 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:44:45.01 -06:21:22.3: 12.55 +/- 0.06 detection
Forced photometry reference-image weighted average: 12.42 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GDS_J1844449-062123,2461186.7261,11.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J1844449-062123 20260526.2261 11.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2261 2461186.7261 11.23 18:37:09.76 -05:39:09.4
26.27565 0.58540 galactic Sct Second-epoch detections are separated by 1.6" and 5.6 pix
The object was found in VSX 1" GDS_J1837097-053910
Type: VAR
# Max. Min./Amp. JD0 Period
12.000 r Y 0.150 r
The object was not found in astcheck.
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:37:09.76 -05:39:09.4: 12.07 +/- 0.02 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:37:09.76 -05:39:09.4: 12.34 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.16 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GDS_J1837097-053910,2461186.7261,11.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J1837097-053910 20260526.2261 11.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2261 2461186.7261 8.65 18:45:41.54 -05:35:45.6
27.29720 -1.27558 galactic Sct Second-epoch detections are separated by 0.1" and 5.5 pix
The object was found in VSX 2" V0428 Sct
Type: SR
# Max. Min./Amp. JD0 Period
10.270 V Y 0.760 V 2452293.30000 380.000000000000 : M5-M6
The object was not found in astcheck.
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:45:41.54 -05:35:45.6: 9.61 +/- 0.00 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:45:41.54 -05:35:45.6: 9.89 +/- 0.01 detection
Forced photometry reference-image weighted average: 9.71 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0428 Sct,2461186.7261,8.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0428 Sct 20260526.2261 8.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2261 2461186.7261 11.10 18:38:11.63 -05:25:33.3
26.59484 0.46151 galactic Sct Second-epoch detections are separated by 2.2" and 5.2 pix
The object was found in VSX 2" ASAS J183811-0525.6
Type: MISC
# Max. Min./Amp. JD0 Period
13.180 V Y 0.650 V 2452811.60000 292.813507000000 S
The object was not found in astcheck.
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:38:11.63 -05:25:33.3: 12.07 +/- 0.02 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:38:11.63 -05:25:33.3: 12.43 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.18 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J183811-0525.6,2461186.7261,11.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J183811-0525.6 20260526.2261 11.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2261 2461186.7261 11.76 18:54:55.93 -01:21:23.5
32.12267 -1.39585 galactic Aql Second-epoch detections are separated by 0.9" and 5.4 pix
The object was found in VSX 2" NSVS J1854558-012122
Type: SR
# Max. Min./Amp. JD0 Period
16.002 g Y 0.578 g 2458327.95310 193.942508800000
The object was not found in astcheck.
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:54:55.93 -01:21:23.5: 12.68 +/- 0.03 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:54:55.93 -01:21:23.5: 12.84 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.74 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J1854558-012122,2461186.7261,11.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J1854558-012122 20260526.2261 11.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2261 2461186.7261 11.16 18:49:11.67 -04:12:21.4
28.93252 -1.41846 galactic Sct Second-epoch detections are separated by 1.9" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 4255276987825319680 | 18:49:11.69 -04:12:21.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.478+/-0.035 (Very red! L if it's a dwarf)
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:49:11.67 -04:12:21.4: 12.05 +/- 0.02 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:49:11.67 -04:12:21.4: 12.12 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.08 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4255276987825319680,2461186.7261,11.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4255276987825319680 20260526.2261 11.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2261 2461186.7261 10.47 18:41:56.86 -05:26:26.1
27.00980 -0.37565 galactic Sct Second-epoch detections are separated by 1.1" and 5.3 pix
The object was found in VSX 1" ASAS J184157-0526.4
Type: MISC
# Max. Min./Amp. JD0 Period
12.270 V Y 0.270 V 2452387.60000 147.467773000000
The object was not found in astcheck.
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:41:56.86 -05:26:26.1: 11.38 +/- 0.02 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:41:56.86 -05:26:26.1: 11.65 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.47 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J184157-0526.4,2461186.7261,10.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J184157-0526.4 20260526.2261 10.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2261 2461186.7261 11.15 18:44:49.52 -04:33:03.7
28.12859 -0.60659 galactic Sct Second-epoch detections are separated by 1.1" and 5.5 pix
The object was found in VSX23" Gaia DR3 4258161560905533568
Type: ELL
# Max. Min./Amp. JD0 Period
16.590 G 16.660 G A
The object was not found in astcheck.
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:44:49.52 -04:33:03.7: 12.04 +/- 0.02 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:44:49.52 -04:33:03.7: 12.17 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.09 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4258161560905533568,2461186.7261,11.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4258161560905533568 20260526.2261 11.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2261 2461186.7261 11.07 18:41:04.28 -06:25:11.8
26.03923 -0.62999 galactic Sct Second-epoch detections are separated by 3.4" and 5.7 pix
The object was found in VSX23" GDS_J1841054-062458
Type: VAR
# Max. Min./Amp. JD0 Period
14.270 i Y 0.560 i
The object was not found in astcheck.
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:41:04.28 -06:25:11.8: 11.95 +/- 0.02 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:41:04.28 -06:25:11.8: 12.06 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.99 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GDS_J1841054-062458,2461186.7261,11.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J1841054-062458 20260526.2261 11.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.2261 2461186.7261 11.68 19:07:20.84 +02:02:16.6
36.56247 -2.60654 galactic Aql Second-epoch detections are separated by 2.5" and 5.8 pix
The object was found in VSX 2" NSVS 14033079
Type: L
# Max. Min./Amp. JD0 Period
11.040 R1 Y 0.140 R1 M3
The object was not found in astcheck.
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 19:07:20.84 +02:02:16.6: 12.64 +/- 0.03 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 19:07:20.84 +02:02:16.6: 12.56 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.60 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 14033079,2461186.7261,11.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 14033079 20260526.2261 11.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461146.82488052 16.04.2026 07:47:39.677 /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits
First image: 2461146.82488052 16.04.2026 07:47:39.677 /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits
Last image: 2461186.72640146 26.05.2026 05:25:51.086 /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q1b1x1_002859_TTUQ1b1x1_2792272_V09vR6vv/fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117.fits
JD time system (TT/UTC/UNKNOWN): UTC
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.11
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 8955
Objects passed selection criteria: 8916
Measurements per detected object (mean, median, min, max): 2.2 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.2 2.0 2 4
Average stars detected per image: 5631.25
Average stars matched: 5379.25 (95.525 %)
Memory usage VmPeak: 115352 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun May 24 19:55:43 CDT 2026
VaST build number 1.0rc89-81-g313b1a97
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-24)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue May 26 00:38:31 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461146.82488052 16.04.2026 07:47:39.677 /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits
First image: 2461146.82488052 16.04.2026 07:47:39.677 /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits
Last image: 2461186.72640146 26.05.2026 05:25:51.086 /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q1b1x1_002859_TTUQ1b1x1_2792272_V09vR6vv/fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 101
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.83
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 17 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 96470
Objects passed selection criteria: 96220
Measurements per detected object (mean, median, min, max): 2.2 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.2 2.0 2 4
Average stars detected per image: 62374.5
Average stars matched: 58680 (94.0769 %)
Memory usage VmPeak: 1939024 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun May 24 19:55:43 CDT 2026
VaST build number 1.0rc89-81-g313b1a97
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-24)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue May 26 00:42:00 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q1b1x1_002859_TTUQ1b1x1_2792272_V09vR6vv/fd_Aql-03-Q1b1x1_2026-05-26_00-25-05_20.00sec_-0.00C_LIGHTs_0116.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q1b1x1_002859_TTUQ1b1x1_2792272_V09vR6vv/fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117.fits
SExtractor catalog cache: saved Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits.cat to cache
SExtractor catalog cache: saved Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q1b1x1_002859_TTUQ1b1x1_2792272_V09vR6vv/fd_Aql-03-Q1b1x1_2026-05-26_00-25-05_20.00sec_-0.00C_LIGHTs_0116.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q1b1x1_002859_TTUQ1b1x1_2792272_V09vR6vv/fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461186.72587461
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits exists and is non-empty
Saving wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits to local_wcs_cache/
'wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits' -> 'local_wcs_cache/wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits'
wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits exists and is non-empty
Saving wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits to local_wcs_cache/
'wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits' -> 'local_wcs_cache/wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits'
wcs_fd_Aql-03-Q1b1x1_2026-05-26_00-25-05_20.00sec_-0.00C_LIGHTs_0116.fits exists and is non-empty
Saving wcs_fd_Aql-03-Q1b1x1_2026-05-26_00-25-05_20.00sec_-0.00C_LIGHTs_0116.fits to local_wcs_cache/
'wcs_fd_Aql-03-Q1b1x1_2026-05-26_00-25-05_20.00sec_-0.00C_LIGHTs_0116.fits' -> 'local_wcs_cache/wcs_fd_Aql-03-Q1b1x1_2026-05-26_00-25-05_20.00sec_-0.00C_LIGHTs_0116.fits'
wcs_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117.fits exists and is non-empty
Saving wcs_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117.fits to local_wcs_cache/
'wcs_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117.fits' -> 'local_wcs_cache/wcs_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits (1st reference image)
verification OK: wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits
Image size: 943.0'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 18:51:21.238 -02:00:51.43 J2000 4789.000 3195.000
###################################
The image scale is 5.91"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aql-03-Q1b1x1_2026-05-26_00-25-05_20.00sec_-0.00C_LIGHTs_0116.fits (1st new image)
verification OK: wcs_fd_Aql-03-Q1b1x1_2026-05-26_00-25-05_20.00sec_-0.00C_LIGHTs_0116.fits
Image size: 942.0'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 18:51:27.348 -01:59:22.23 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 18:51:21.238 -02:00:51.43
Second-epoch image center 18:51:27.348 -01:59:22.23
Angular distance between the image centers 0.0355 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117.fits (2nd new image)
verification OK: wcs_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117.fits
Image size: 941.9'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 18:51:26.604 -01:58:51.36 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 18:51:21.238 -02:00:51.43
Second-epoch image center 18:51:26.604 -01:58:51.36
Angular distance between the image centers 0.0401 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 18:51:27.348 -01:59:22.23
Second-epoch second image center 18:51:26.604 -01:58:51.36
Angular distance between the image centers 0.00912 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits &> /tmp/tmp.tzP2ztzBmz
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits &> /tmp/tmp.3Cr5eyF93N
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q1b1x1_002859_TTUQ1b1x1_2792272_V09vR6vv/fd_Aql-03-Q1b1x1_2026-05-26_00-25-05_20.00sec_-0.00C_LIGHTs_0116.fits &> /tmp/tmp.edn58CTjTY
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q1b1x1_002859_TTUQ1b1x1_2792272_V09vR6vv/fd_Aql-03-Q1b1x1_2026-05-26_00-25-05_20.00sec_-0.00C_LIGHTs_0116.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q1b1x1_002859_TTUQ1b1x1_2792272_V09vR6vv/fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117.fits &> /tmp/tmp.PJKqTItRb3
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q1b1x1_002859_TTUQ1b1x1_2792272_V09vR6vv/fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117.fits
Calibrating the magnitude scale
Found non-empty wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits and wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits.cat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits and wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits.cat
Found non-empty wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits and wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits.cat
The reference image (wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits) and catalog (wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits.cat) found
'wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits.cat' -> 'wcsmag.cat'
Read 10727 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 274.6382 to 291.0089 deg, Dec -7.7289 to +3.7311 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 274.6382 to 291.0089 deg, Dec -7.7289 to 3.7311 deg
Loaded 10967 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 6449 out of 6736 total matches.
Matched with Tycho-2 6736 out of 10727 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.621000
a=0.000000 b=1.000000 c=22.621000
From vast_summary.log: estimated ref. image limiting mag.: -8.11
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.51
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.51
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 10727 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 274.6382 to 291.0089 deg, Dec -7.7289 to +3.7311 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 274.6382 to 291.0089 deg, Dec -7.7289 to 3.7311 deg
Loaded 10967 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 6449 out of 6736 total matches.
Matched with Tycho-2 6736 out of 10727 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits:
Forced-photometry filter: calibrated wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits -> calib.txt_param_ref_wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits (aperture=6.1)
Read 10007 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 274.9538 to 290.8167 deg, Dec -7.2966 to +3.3664 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 274.9538 to 290.8167 deg, Dec -7.2966 to 3.3664 deg
Loaded 9632 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 6263 out of 6516 total matches.
Matched with Tycho-2 6516 out of 10007 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits:
Forced-photometry filter: calibrated wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits -> calib.txt_param_ref_wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits (aperture=6.4)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.2 pix Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits
2.4 pix Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits
3.8 pix fd_Aql-03-Q1b1x1_2026-05-26_00-25-05_20.00sec_-0.00C_LIGHTs_0116.fits
3.8 pix fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117.fits
2.2 pix wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits
2.4 pix wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits
Limiting magnitude estimates:
14.5 mag. Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits
14.4 mag. Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits
11.3 mag. fd_Aql-03-Q1b1x1_2026-05-26_00-25-05_20.00sec_-0.00C_LIGHTs_0116.fits
11.3 mag. fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117.fits
All-image limiting magnitude estimate: 11.3 (SNR ) 9.4 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.tzP2ztzBmz (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-26_CI_Aql-03-Q1b1x1_002859_TTUQ1b1x1_2792272_V09vR6vv/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits' -> 'wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits
WCS_IMAGE_NAME=wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits
WCS-calibrated image found: wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits
Checking if the catalog wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits.cat corresponding to the image wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits alredy exist and is non-empty...
Catalog wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits.cat corresponding to the image wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits
WCS catalog name: wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=845, passed=10727
Got 10727 stars (including 9870 good ones) from the SExtractor catalog wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits.cat
util/solve_plate_with_UCAC5 got 10727 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 943.0'
Seting catalog search parameters based on the expected field of view 943.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013097 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010478 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.7 to 3.7)
Done reading UCAC5 zone files...
Matched 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 924 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 10553 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.7 to 3.7)
Done reading UCAC5 zone files...
Matched 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 10553 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 10553 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 943 stars left (next iteration limit 1037)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits N_match=943 sigma_overall_arcsec=0.369 sigma_q1_arcsec=0.358 sigma_q2_arcsec=0.443 sigma_q3_arcsec=0.365 sigma_q4_arcsec=0.339 n_q1=197 n_q2=242 n_q3=217 n_q4=287 worst_quadrant_to_overall_ratio=1.200
The image catalog is written to wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits -region wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.3Cr5eyF93N (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-26_CI_Aql-03-Q1b1x1_002859_TTUQ1b1x1_2792272_V09vR6vv/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits' -> 'wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits
WCS_IMAGE_NAME=wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits
WCS-calibrated image found: wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits
Checking if the catalog wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits.cat corresponding to the image wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits alredy exist and is non-empty...
Catalog wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits.cat corresponding to the image wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits
WCS catalog name: wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=756, passed=10007
Got 10007 stars (including 9239 good ones) from the SExtractor catalog wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits.cat
util/solve_plate_with_UCAC5 got 10007 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.1'
Seting catalog search parameters based on the expected field of view 938.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013029 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010423 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 937 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 9836 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 9834 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 9834 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Excluding outliers - 951 stars left (next iteration limit 1046)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits N_match=951 sigma_overall_arcsec=0.602 sigma_q1_arcsec=0.535 sigma_q2_arcsec=0.709 sigma_q3_arcsec=0.574 sigma_q4_arcsec=0.602 n_q1=197 n_q2=247 n_q3=210 n_q4=297 worst_quadrant_to_overall_ratio=1.177
The image catalog is written to wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits -region wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.edn58CTjTY (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-26_CI_Aql-03-Q1b1x1_002859_TTUQ1b1x1_2792272_V09vR6vv/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q1b1x1_002859_TTUQ1b1x1_2792272_V09vR6vv/fd_Aql-03-Q1b1x1_2026-05-26_00-25-05_20.00sec_-0.00C_LIGHTs_0116.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q1b1x1_002859_TTUQ1b1x1_2792272_V09vR6vv/fd_Aql-03-Q1b1x1_2026-05-26_00-25-05_20.00sec_-0.00C_LIGHTs_0116.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q1b1x1_002859_TTUQ1b1x1_2792272_V09vR6vv/fd_Aql-03-Q1b1x1_2026-05-26_00-25-05_20.00sec_-0.00C_LIGHTs_0116.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q1b1x1_002859_TTUQ1b1x1_2792272_V09vR6vv/fd_Aql-03-Q1b1x1_2026-05-26_00-25-05_20.00sec_-0.00C_LIGHTs_0116.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q1b1x1_002859_TTUQ1b1x1_2792272_V09vR6vv/fd_Aql-03-Q1b1x1_2026-05-26_00-25-05_20.00sec_-0.00C_LIGHTs_0116.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q1b1x1_002859_TTUQ1b1x1_2792272_V09vR6vv/fd_Aql-03-Q1b1x1_2026-05-26_00-25-05_20.00sec_-0.00C_LIGHTs_0116.fits
WCS_IMAGE_NAME=wcs_fd_Aql-03-Q1b1x1_2026-05-26_00-25-05_20.00sec_-0.00C_LIGHTs_0116.fits
WCS-calibrated image found: wcs_fd_Aql-03-Q1b1x1_2026-05-26_00-25-05_20.00sec_-0.00C_LIGHTs_0116.fits
Checking if the catalog wcs_fd_Aql-03-Q1b1x1_2026-05-26_00-25-05_20.00sec_-0.00C_LIGHTs_0116.fits.cat corresponding to the image wcs_fd_Aql-03-Q1b1x1_2026-05-26_00-25-05_20.00sec_-0.00C_LIGHTs_0116.fits alredy exist and is non-empty...
Catalog wcs_fd_Aql-03-Q1b1x1_2026-05-26_00-25-05_20.00sec_-0.00C_LIGHTs_0116.fits.cat corresponding to the image wcs_fd_Aql-03-Q1b1x1_2026-05-26_00-25-05_20.00sec_-0.00C_LIGHTs_0116.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aql-03-Q1b1x1_2026-05-26_00-25-05_20.00sec_-0.00C_LIGHTs_0116.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q1b1x1_002859_TTUQ1b1x1_2792272_V09vR6vv/fd_Aql-03-Q1b1x1_2026-05-26_00-25-05_20.00sec_-0.00C_LIGHTs_0116.fits
WCS catalog name: wcs_fd_Aql-03-Q1b1x1_2026-05-26_00-25-05_20.00sec_-0.00C_LIGHTs_0116.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=45, passed=989
Got 989 stars (including 944 good ones) from the SExtractor catalog wcs_fd_Aql-03-Q1b1x1_2026-05-26_00-25-05_20.00sec_-0.00C_LIGHTs_0116.fits.cat
util/solve_plate_with_UCAC5 got 989 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.0'
Seting catalog search parameters based on the expected field of view 942.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013083 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010467 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 412 to 470 (Dec -7.5 to 3.6)
Done reading UCAC5 zone files...
Matched 886 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 883 matched stars entering correct_measured_positions(), 842 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 883 matched stars entering correct_measured_positions(), 942 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 412 to 470 (Dec -7.5 to 3.6)
Done reading UCAC5 zone files...
Matched 887 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 884 matched stars entering correct_measured_positions(), 942 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Accuracy estimation diagnostic: 884 matched stars entering correct_measured_positions(), 942 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Excluding outliers - 884 stars left (next iteration limit 971)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Aql-03-Q1b1x1_2026-05-26_00-25-05_20.00sec_-0.00C_LIGHTs_0116.fits N_match=884 sigma_overall_arcsec=0.534 sigma_q1_arcsec=0.601 sigma_q2_arcsec=0.783 sigma_q3_arcsec=0.436 sigma_q4_arcsec=0.526 n_q1=217 n_q2=105 n_q3=251 n_q4=311 worst_quadrant_to_overall_ratio=1.467
The image catalog is written to wcs_fd_Aql-03-Q1b1x1_2026-05-26_00-25-05_20.00sec_-0.00C_LIGHTs_0116.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aql-03-Q1b1x1_2026-05-26_00-25-05_20.00sec_-0.00C_LIGHTs_0116.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q1b1x1_002859_TTUQ1b1x1_2792272_V09vR6vv/fd_Aql-03-Q1b1x1_2026-05-26_00-25-05_20.00sec_-0.00C_LIGHTs_0116.fits -region wcs_fd_Aql-03-Q1b1x1_2026-05-26_00-25-05_20.00sec_-0.00C_LIGHTs_0116.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aql-03-Q1b1x1_2026-05-26_00-25-05_20.00sec_-0.00C_LIGHTs_0116.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.PJKqTItRb3 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-26_CI_Aql-03-Q1b1x1_002859_TTUQ1b1x1_2792272_V09vR6vv/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q1b1x1_002859_TTUQ1b1x1_2792272_V09vR6vv/fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q1b1x1_002859_TTUQ1b1x1_2792272_V09vR6vv/fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q1b1x1_002859_TTUQ1b1x1_2792272_V09vR6vv/fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q1b1x1_002859_TTUQ1b1x1_2792272_V09vR6vv/fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q1b1x1_002859_TTUQ1b1x1_2792272_V09vR6vv/fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q1b1x1_002859_TTUQ1b1x1_2792272_V09vR6vv/fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117.fits
WCS_IMAGE_NAME=wcs_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117.fits
WCS-calibrated image found: wcs_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117.fits
Checking if the catalog wcs_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117.fits.cat corresponding to the image wcs_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117.fits alredy exist and is non-empty...
Catalog wcs_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117.fits.cat corresponding to the image wcs_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q1b1x1_002859_TTUQ1b1x1_2792272_V09vR6vv/fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117.fits
WCS catalog name: wcs_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=40, passed=971
Got 971 stars (including 931 good ones) from the SExtractor catalog wcs_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117.fits.cat
util/solve_plate_with_UCAC5 got 971 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010466 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 412 to 470 (Dec -7.5 to 3.6)
Done reading UCAC5 zone files...
Matched 876 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 873 matched stars entering correct_measured_positions(), 837 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 873 matched stars entering correct_measured_positions(), 927 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 412 to 470 (Dec -7.5 to 3.6)
Done reading UCAC5 zone files...
Matched 876 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 873 matched stars entering correct_measured_positions(), 928 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Accuracy estimation diagnostic: 873 matched stars entering correct_measured_positions(), 928 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Excluding outliers - 873 stars left (next iteration limit 960)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117.fits N_match=873 sigma_overall_arcsec=0.508 sigma_q1_arcsec=0.567 sigma_q2_arcsec=0.659 sigma_q3_arcsec=0.446 sigma_q4_arcsec=0.493 n_q1=217 n_q2=109 n_q3=233 n_q4=314 worst_quadrant_to_overall_ratio=1.298
The image catalog is written to wcs_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q1b1x1_002859_TTUQ1b1x1_2792272_V09vR6vv/fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117.fits -region wcs_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits sigma_overall=0.369 worst_q_ratio=1.200
ref2=Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits sigma_overall=0.602 worst_q_ratio=1.177
new1=fd_Aql-03-Q1b1x1_2026-05-26_00-25-05_20.00sec_-0.00C_LIGHTs_0116.fits sigma_overall=0.534 worst_q_ratio=1.467
new2=fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117.fits sigma_overall=0.508 worst_q_ratio=1.298
reference average sigma_overall=0.4855 worst_q_ratio=1.1885
warn-on-ratio threshold: 2.0x reference
###################################
Distribution of catalog-matched stars across the image:
plot_astrometric_residuals_xy: wrote wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245_astrometric_residuals.png (943 matched stars from wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119_astrometric_residuals.png (951 matched stars from wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_fd_Aql-03-Q1b1x1_2026-05-26_00-25-05_20.00sec_-0.00C_LIGHTs_0116_astrometric_residuals.png (884 matched stars from wcs_fd_Aql-03-Q1b1x1_2026-05-26_00-25-05_20.00sec_-0.00C_LIGHTs_0116.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117_astrometric_residuals.png (873 matched stars from wcs_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117.fits.cat.astrometric_residuals, image 9576x6388)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Aql-03-Q1b1x1_2026-05-26_00-25-05_20.00sec_-0.00C_LIGHTs_0116.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aql-03-Q1b1x1_2026-05-26_00-25-05_20.00sec_-0.00C_LIGHTs_0116.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q1b1x1_002859_TTUQ1b1x1_2792272_V09vR6vv/wcs_fd_Aql-03-Q1b1x1_2026-05-26_00-25-05_20.00sec_-0.00C_LIGHTs_0116.fits'
Saving fully-calibrated image wcs_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q1b1x1_002859_TTUQ1b1x1_2792272_V09vR6vv/wcs_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117.fits'
Preparing the HTML report for the field Aql-03-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Aql-03-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q1b1x1_002859_TTUQ1b1x1_2792272_V09vR6vv/fd_Aql-03-Q1b1x1_2026-05-26_00-25-05_20.00sec_-0.00C_LIGHTs_0116.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q1b1x1_002859_TTUQ1b1x1_2792272_V09vR6vv/fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117.fits
SExtractor catalog cache: saved Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits.cat to cache
SExtractor catalog cache: saved Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q1b1x1_002859_TTUQ1b1x1_2792272_V09vR6vv/fd_Aql-03-Q1b1x1_2026-05-26_00-25-05_20.00sec_-0.00C_LIGHTs_0116.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q1b1x1_002859_TTUQ1b1x1_2792272_V09vR6vv/fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits
Creating symlink local_wcs_cache/wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits
Creating symlink local_wcs_cache/wcs_fd_Aql-03-Q1b1x1_2026-05-26_00-25-05_20.00sec_-0.00C_LIGHTs_0116.fits
Creating symlink local_wcs_cache/wcs_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits exists and is non-empty
wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits exists and is non-empty
wcs_fd_Aql-03-Q1b1x1_2026-05-26_00-25-05_20.00sec_-0.00C_LIGHTs_0116.fits exists and is non-empty
wcs_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits (1st reference image)
verification OK: wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits
Image size: 943.0'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 18:51:21.238 -02:00:51.43 J2000 4789.000 3195.000
###################################
The image scale is 5.91"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aql-03-Q1b1x1_2026-05-26_00-25-05_20.00sec_-0.00C_LIGHTs_0116.fits (1st new image)
verification OK: wcs_fd_Aql-03-Q1b1x1_2026-05-26_00-25-05_20.00sec_-0.00C_LIGHTs_0116.fits
Image size: 942.0'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 18:51:27.348 -01:59:22.23 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 18:51:21.238 -02:00:51.43
Second-epoch image center 18:51:27.348 -01:59:22.23
Angular distance between the image centers 0.0355 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117.fits (2nd new image)
verification OK: wcs_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117.fits
Image size: 941.9'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 18:51:26.604 -01:58:51.36 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 18:51:21.238 -02:00:51.43
Second-epoch image center 18:51:26.604 -01:58:51.36
Angular distance between the image centers 0.0401 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 18:51:27.348 -01:59:22.23
Second-epoch second image center 18:51:26.604 -01:58:51.36
Angular distance between the image centers 0.00912 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits &> /tmp/tmp.umZ9aEqYxi
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits &> /tmp/tmp.L1kmUYCVXK
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q1b1x1_002859_TTUQ1b1x1_2792272_V09vR6vv/fd_Aql-03-Q1b1x1_2026-05-26_00-25-05_20.00sec_-0.00C_LIGHTs_0116.fits &> /tmp/tmp.bWB5LQ7JKp
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q1b1x1_002859_TTUQ1b1x1_2792272_V09vR6vv/fd_Aql-03-Q1b1x1_2026-05-26_00-25-05_20.00sec_-0.00C_LIGHTs_0116.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q1b1x1_002859_TTUQ1b1x1_2792272_V09vR6vv/fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117.fits &> /tmp/tmp.Zsaoi9Sw8M
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q1b1x1_002859_TTUQ1b1x1_2792272_V09vR6vv/fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117.fits
Calibrating the magnitude scale
Found non-empty wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits and wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits.cat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits and wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits.cat
Found non-empty wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits and wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits.cat
The reference image (wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits) and catalog (wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits.cat) found
'wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits.cat' -> 'wcsmag.cat'
Read 122602 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 274.5985 to 291.0381 deg, Dec -7.7684 to +3.7641 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 274.5985 to 291.0381 deg, Dec -7.7684 to 3.7641 deg
Loaded 11083 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 6807 out of 8428 total matches.
Matched with Tycho-2 8428 out of 122602 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.428700
a=0.000000 b=1.000000 c=22.428700
From vast_summary.log: estimated ref. image limiting mag.: -7.83
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.60
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.60
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 122602 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 274.5985 to 291.0381 deg, Dec -7.7684 to +3.7641 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 274.5985 to 291.0381 deg, Dec -7.7684 to 3.7641 deg
Loaded 11083 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 6807 out of 8428 total matches.
Matched with Tycho-2 8428 out of 122602 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits:
Forced-photometry filter: calibrated wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits -> calib.txt_param_ref_wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits (aperture=4.5)
Read 111944 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 274.9350 to 290.8262 deg, Dec -7.3187 to +3.3664 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 274.9350 to 290.8262 deg, Dec -7.3187 to 3.3664 deg
Loaded 9679 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 6784 out of 8259 total matches.
Matched with Tycho-2 8259 out of 111944 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits:
Forced-photometry filter: calibrated wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits -> calib.txt_param_ref_wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits (aperture=4.5)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 98 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.1 pix Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits
2.2 pix Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits
3.2 pix fd_Aql-03-Q1b1x1_2026-05-26_00-25-05_20.00sec_-0.00C_LIGHTs_0116.fits
3.1 pix fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117.fits
2.1 pix wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits
2.2 pix wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits
Limiting magnitude estimates:
14.6 mag. Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits
14.5 mag. Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits
12.1 mag. fd_Aql-03-Q1b1x1_2026-05-26_00-25-05_20.00sec_-0.00C_LIGHTs_0116.fits
12.0 mag. fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117.fits
All-image limiting magnitude estimate: 12.0 (SNR ) 11.6 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.umZ9aEqYxi (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-26_CI_Aql-03-Q1b1x1_002859_TTUQ1b1x1_2792272_V09vR6vv/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits' -> 'wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits
WCS_IMAGE_NAME=wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits
WCS-calibrated image found: wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits
Checking if the catalog wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits.cat corresponding to the image wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits alredy exist and is non-empty...
Catalog wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits.cat corresponding to the image wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits
WCS catalog name: wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=13, blended=12771, passed=122589
Got 122589 stars (including 109591 good ones) from the SExtractor catalog wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits.cat
util/solve_plate_with_UCAC5 got 122589 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 943.0'
Seting catalog search parameters based on the expected field of view 943.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013097 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010478 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.8 to 3.8)
Done reading UCAC5 zone files...
Matched 947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 935 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 121309 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.8 to 3.8)
Done reading UCAC5 zone files...
Matched 947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 121309 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 121307 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 945 stars left (next iteration limit 1039)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits N_match=945 sigma_overall_arcsec=0.385 sigma_q1_arcsec=0.366 sigma_q2_arcsec=0.434 sigma_q3_arcsec=0.347 sigma_q4_arcsec=0.402 n_q1=204 n_q2=238 n_q3=225 n_q4=278 worst_quadrant_to_overall_ratio=1.127
The image catalog is written to wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits -region wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.L1kmUYCVXK (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-26_CI_Aql-03-Q1b1x1_002859_TTUQ1b1x1_2792272_V09vR6vv/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits' -> 'wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits
WCS_IMAGE_NAME=wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits
WCS-calibrated image found: wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits
Checking if the catalog wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits.cat corresponding to the image wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits alredy exist and is non-empty...
Catalog wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits.cat corresponding to the image wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits
WCS catalog name: wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=21, blended=11221, passed=111923
Got 111923 stars (including 100547 good ones) from the SExtractor catalog wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits.cat
util/solve_plate_with_UCAC5 got 111923 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.1'
Seting catalog search parameters based on the expected field of view 938.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013029 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010423 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 936 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 110179 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 110179 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 110179 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Excluding outliers - 951 stars left (next iteration limit 1046)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits N_match=951 sigma_overall_arcsec=0.602 sigma_q1_arcsec=0.503 sigma_q2_arcsec=0.654 sigma_q3_arcsec=0.591 sigma_q4_arcsec=0.639 n_q1=187 n_q2=262 n_q3=205 n_q4=297 worst_quadrant_to_overall_ratio=1.086
The image catalog is written to wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits -region wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.bWB5LQ7JKp (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-26_CI_Aql-03-Q1b1x1_002859_TTUQ1b1x1_2792272_V09vR6vv/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q1b1x1_002859_TTUQ1b1x1_2792272_V09vR6vv/fd_Aql-03-Q1b1x1_2026-05-26_00-25-05_20.00sec_-0.00C_LIGHTs_0116.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q1b1x1_002859_TTUQ1b1x1_2792272_V09vR6vv/fd_Aql-03-Q1b1x1_2026-05-26_00-25-05_20.00sec_-0.00C_LIGHTs_0116.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q1b1x1_002859_TTUQ1b1x1_2792272_V09vR6vv/fd_Aql-03-Q1b1x1_2026-05-26_00-25-05_20.00sec_-0.00C_LIGHTs_0116.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q1b1x1_002859_TTUQ1b1x1_2792272_V09vR6vv/fd_Aql-03-Q1b1x1_2026-05-26_00-25-05_20.00sec_-0.00C_LIGHTs_0116.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q1b1x1_002859_TTUQ1b1x1_2792272_V09vR6vv/fd_Aql-03-Q1b1x1_2026-05-26_00-25-05_20.00sec_-0.00C_LIGHTs_0116.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q1b1x1_002859_TTUQ1b1x1_2792272_V09vR6vv/fd_Aql-03-Q1b1x1_2026-05-26_00-25-05_20.00sec_-0.00C_LIGHTs_0116.fits
WCS_IMAGE_NAME=wcs_fd_Aql-03-Q1b1x1_2026-05-26_00-25-05_20.00sec_-0.00C_LIGHTs_0116.fits
WCS-calibrated image found: wcs_fd_Aql-03-Q1b1x1_2026-05-26_00-25-05_20.00sec_-0.00C_LIGHTs_0116.fits
Checking if the catalog wcs_fd_Aql-03-Q1b1x1_2026-05-26_00-25-05_20.00sec_-0.00C_LIGHTs_0116.fits.cat corresponding to the image wcs_fd_Aql-03-Q1b1x1_2026-05-26_00-25-05_20.00sec_-0.00C_LIGHTs_0116.fits alredy exist and is non-empty...
Catalog wcs_fd_Aql-03-Q1b1x1_2026-05-26_00-25-05_20.00sec_-0.00C_LIGHTs_0116.fits.cat corresponding to the image wcs_fd_Aql-03-Q1b1x1_2026-05-26_00-25-05_20.00sec_-0.00C_LIGHTs_0116.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aql-03-Q1b1x1_2026-05-26_00-25-05_20.00sec_-0.00C_LIGHTs_0116.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q1b1x1_002859_TTUQ1b1x1_2792272_V09vR6vv/fd_Aql-03-Q1b1x1_2026-05-26_00-25-05_20.00sec_-0.00C_LIGHTs_0116.fits
WCS catalog name: wcs_fd_Aql-03-Q1b1x1_2026-05-26_00-25-05_20.00sec_-0.00C_LIGHTs_0116.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=227, passed=8796
Got 8796 stars (including 8553 good ones) from the SExtractor catalog wcs_fd_Aql-03-Q1b1x1_2026-05-26_00-25-05_20.00sec_-0.00C_LIGHTs_0116.fits.cat
util/solve_plate_with_UCAC5 got 8796 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.0'
Seting catalog search parameters based on the expected field of view 942.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013083 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010467 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.6 to 3.7)
Done reading UCAC5 zone files...
Matched 933 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 931 matched stars entering correct_measured_positions(), 890 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 931 matched stars entering correct_measured_positions(), 8474 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.6 to 3.7)
Done reading UCAC5 zone files...
Matched 933 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 931 matched stars entering correct_measured_positions(), 8477 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Accuracy estimation diagnostic: 931 matched stars entering correct_measured_positions(), 8477 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 931 stars left (next iteration limit 1024)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Aql-03-Q1b1x1_2026-05-26_00-25-05_20.00sec_-0.00C_LIGHTs_0116.fits N_match=931 sigma_overall_arcsec=0.478 sigma_q1_arcsec=0.605 sigma_q2_arcsec=0.712 sigma_q3_arcsec=0.400 sigma_q4_arcsec=0.452 n_q1=232 n_q2=113 n_q3=267 n_q4=319 worst_quadrant_to_overall_ratio=1.490
The image catalog is written to wcs_fd_Aql-03-Q1b1x1_2026-05-26_00-25-05_20.00sec_-0.00C_LIGHTs_0116.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aql-03-Q1b1x1_2026-05-26_00-25-05_20.00sec_-0.00C_LIGHTs_0116.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q1b1x1_002859_TTUQ1b1x1_2792272_V09vR6vv/fd_Aql-03-Q1b1x1_2026-05-26_00-25-05_20.00sec_-0.00C_LIGHTs_0116.fits -region wcs_fd_Aql-03-Q1b1x1_2026-05-26_00-25-05_20.00sec_-0.00C_LIGHTs_0116.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aql-03-Q1b1x1_2026-05-26_00-25-05_20.00sec_-0.00C_LIGHTs_0116.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.Zsaoi9Sw8M (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-26_CI_Aql-03-Q1b1x1_002859_TTUQ1b1x1_2792272_V09vR6vv/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q1b1x1_002859_TTUQ1b1x1_2792272_V09vR6vv/fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q1b1x1_002859_TTUQ1b1x1_2792272_V09vR6vv/fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q1b1x1_002859_TTUQ1b1x1_2792272_V09vR6vv/fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q1b1x1_002859_TTUQ1b1x1_2792272_V09vR6vv/fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q1b1x1_002859_TTUQ1b1x1_2792272_V09vR6vv/fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q1b1x1_002859_TTUQ1b1x1_2792272_V09vR6vv/fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117.fits
WCS_IMAGE_NAME=wcs_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117.fits
WCS-calibrated image found: wcs_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117.fits
Checking if the catalog wcs_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117.fits.cat corresponding to the image wcs_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117.fits alredy exist and is non-empty...
Catalog wcs_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117.fits.cat corresponding to the image wcs_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q1b1x1_002859_TTUQ1b1x1_2792272_V09vR6vv/fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117.fits
WCS catalog name: wcs_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=1, blended=237, passed=8856
Got 8856 stars (including 8606 good ones) from the SExtractor catalog wcs_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117.fits.cat
util/solve_plate_with_UCAC5 got 8856 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010466 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 412 to 470 (Dec -7.6 to 3.7)
Done reading UCAC5 zone files...
Matched 930 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 895 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 8505 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 412 to 470 (Dec -7.6 to 3.7)
Done reading UCAC5 zone files...
Matched 930 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 8506 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 8506 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 928 stars left (next iteration limit 1020)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117.fits N_match=928 sigma_overall_arcsec=0.439 sigma_q1_arcsec=0.554 sigma_q2_arcsec=0.587 sigma_q3_arcsec=0.367 sigma_q4_arcsec=0.430 n_q1=227 n_q2=123 n_q3=249 n_q4=329 worst_quadrant_to_overall_ratio=1.336
The image catalog is written to wcs_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q1b1x1_002859_TTUQ1b1x1_2792272_V09vR6vv/fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117.fits -region wcs_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Aql-03-Q1b1x1_2026-05-26_00-25-05_20.00sec_-0.00C_LIGHTs_0116.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q1b1x1_002859_TTUQ1b1x1_2792272_V09vR6vv/wcs_fd_Aql-03-Q1b1x1_2026-05-26_00-25-05_20.00sec_-0.00C_LIGHTs_0116.fits
Saving fully-calibrated image wcs_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-05-26_CI_Aql-03-Q1b1x1_002859_TTUQ1b1x1_2792272_V09vR6vv/wcs_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117.fits
Preparing the HTML report for the field Aql-03-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:43:26.32 -05:46:21.0: 11.73 +/- 0.03 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:55:41.71 +00:20:49.8: 12.72 +/- 0.04 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:48:23.57 -04:16:42.2: 12.38 +/- 0.03 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:55:41.71 +00:20:49.8: 12.97 +/- 0.05 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:43:26.32 -05:46:21.0: 11.71 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.81 +/- 0.03
Forced photometry filter KEPT candidate at 18:55:41.71 +00:20:49.8: ref_mag=12.81 +/- 0.03 new_mean_mag=11.8147 delta=0.99 (need > 0.90)
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:42:33.14 -05:52:11.3: 12.76 +/- 0.05 detection
Forced photometry reference-image weighted average: 11.72 +/- 0.02
Forced photometry filter KEPT candidate at 18:43:26.32 -05:46:21.0: ref_mag=11.72 +/- 0.02 new_mean_mag=10.6822 delta=1.04 (need > 0.90)
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:56:10.70 -00:15:44.4: 12.23 +/- 0.02 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:51:55.89 -03:53:31.5: 12.56 +/- 0.03 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:48:23.57 -04:16:42.2: 12.48 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.42 +/- 0.02
Forced photometry filter KEPT candidate at 18:48:23.57 -04:16:42.2: ref_mag=12.42 +/- 0.02 new_mean_mag=11.4696 delta=0.95 (need > 0.90)
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:38:28.86 -06:11:48.5: 12.28 +/- 0.02 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:42:33.14 -05:52:11.3: 13.02 +/- 0.06 detection
Forced photometry reference-image weighted average: 12.86 +/- 0.04
Forced photometry filter KEPT candidate at 18:42:33.14 -05:52:11.3: ref_mag=12.86 +/- 0.04 new_mean_mag=11.3086 delta=1.55 (need > 0.90)
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:56:10.70 -00:15:44.4: 12.50 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.32 +/- 0.02
Forced photometry filter KEPT candidate at 18:56:10.70 -00:15:44.4: ref_mag=12.32 +/- 0.02 new_mean_mag=11.2327 delta=1.09 (need > 0.90)
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:52:17.95 -04:29:22.7: 12.61 +/- 0.03 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:47:34.16 -04:36:35.5: 12.63 +/- 0.04 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:51:55.89 -03:53:31.5: 12.72 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.62 +/- 0.03
Forced photometry filter KEPT candidate at 18:51:55.89 -03:53:31.5: ref_mag=12.62 +/- 0.03 new_mean_mag=11.5499 delta=1.07 (need > 0.90)
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:38:28.86 -06:11:48.5: 12.64 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.38 +/- 0.02
Forced photometry filter KEPT candidate at 18:38:28.86 -06:11:48.5: ref_mag=12.38 +/- 0.02 new_mean_mag=11.1866 delta=1.19 (need > 0.90)
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:47:34.16 -04:36:35.5: 12.87 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.71 +/- 0.03
Forced photometry filter KEPT candidate at 18:47:34.16 -04:36:35.5: ref_mag=12.71 +/- 0.03 new_mean_mag=11.5709 delta=1.14 (need > 0.90)
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:52:17.95 -04:29:22.7: 12.66 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.63 +/- 0.02
Forced photometry filter KEPT candidate at 18:52:17.95 -04:29:22.7: ref_mag=12.63 +/- 0.02 new_mean_mag=11.5718 delta=1.06 (need > 0.90)
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:42:44.42 -06:15:55.8: 11.94 +/- 0.03 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:42:44.42 -06:15:55.8: 12.07 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.00 +/- 0.02
Forced photometry filter KEPT candidate at 18:42:44.42 -06:15:55.8: ref_mag=12.00 +/- 0.02 new_mean_mag=10.9669 delta=1.03 (need > 0.90)
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:42:17.40 -05:48:53.9: 12.61 +/- 0.05 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:42:17.40 -05:48:53.9: 12.83 +/- 0.06 detection
Forced photometry reference-image weighted average: 12.70 +/- 0.04
Forced photometry filter KEPT candidate at 18:42:17.40 -05:48:53.9: ref_mag=12.70 +/- 0.04 new_mean_mag=11.4692 delta=1.23 (need > 0.90)
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 19:02:38.10 +01:19:22.8: 12.60 +/- 0.03 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 19:02:38.10 +01:19:22.8: 12.77 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.66 +/- 0.02
Forced photometry filter KEPT candidate at 19:02:38.10 +01:19:22.8: ref_mag=12.66 +/- 0.02 new_mean_mag=11.5663 delta=1.10 (need > 0.90)
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:49:44.64 -03:49:31.9: 12.37 +/- 0.02 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:42:35.13 -05:22:13.6: 11.91 +/- 0.02 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:46:44.64 -04:16:41.7: 11.91 +/- 0.02 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:49:44.64 -03:49:31.9: 12.59 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.44 +/- 0.02
Forced photometry filter KEPT candidate at 18:49:44.64 -03:49:31.9: ref_mag=12.44 +/- 0.02 new_mean_mag=11.1862 delta=1.26 (need > 0.90)
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:42:35.13 -05:22:13.6: 12.16 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.00 +/- 0.01
Forced photometry filter KEPT candidate at 18:42:35.13 -05:22:13.6: ref_mag=12.00 +/- 0.01 new_mean_mag=11.0392 delta=0.96 (need > 0.90)
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:42:03.84 -05:04:57.8: 11.91 +/- 0.02 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:46:44.64 -04:16:41.7: 12.16 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.00 +/- 0.01
Forced photometry filter KEPT candidate at 18:46:44.64 -04:16:41.7: ref_mag=12.00 +/- 0.01 new_mean_mag=11.0869 delta=0.91 (need > 0.90)
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:46:27.11 -05:49:54.8: 12.37 +/- 0.03 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:42:03.84 -05:04:57.8: 12.18 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.01 +/- 0.02
Forced photometry filter KEPT candidate at 18:42:03.84 -05:04:57.8: ref_mag=12.01 +/- 0.02 new_mean_mag=10.8779 delta=1.13 (need > 0.90)
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 19:00:02.00 +01:41:01.9: 12.31 +/- 0.02 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:46:27.11 -05:49:54.8: 12.51 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.42 +/- 0.02
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:44:01.87 -05:31:51.4: 11.88 +/- 0.02 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:52:15.62 -04:12:09.2: 12.31 +/- 0.02 detection
Forced photometry filter KEPT candidate at 18:46:27.11 -05:49:54.8: ref_mag=12.42 +/- 0.02 new_mean_mag=11.3670 delta=1.06 (need > 0.90)
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 19:00:02.00 +01:41:01.9: 12.39 +/- 0.03 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:52:15.62 -04:12:09.2: 12.43 +/- 0.03 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:44:01.87 -05:31:51.4: 12.11 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.35 +/- 0.02
Forced photometry filter KEPT candidate at 19:00:02.00 +01:41:01.9: ref_mag=12.35 +/- 0.02 new_mean_mag=11.3263 delta=1.02 (need > 0.90)
Forced photometry reference-image weighted average: 11.97 +/- 0.02
Forced photometry reference-image weighted average: 12.36 +/- 0.02
Forced photometry filter KEPT candidate at 18:44:01.87 -05:31:51.4: ref_mag=11.97 +/- 0.02 new_mean_mag=10.7504 delta=1.22 (need > 0.90)
Forced photometry filter KEPT candidate at 18:52:15.62 -04:12:09.2: ref_mag=12.36 +/- 0.02 new_mean_mag=11.3876 delta=0.97 (need > 0.90)
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 19:08:04.45 +01:39:31.3: 12.31 +/- 0.03 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 19:08:04.45 +01:39:31.3: 12.23 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.27 +/- 0.02
Forced photometry filter KEPT candidate at 19:08:04.45 +01:39:31.3: ref_mag=12.27 +/- 0.02 new_mean_mag=11.2979 delta=0.97 (need > 0.90)
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:43:09.26 -05:45:44.5: 12.79 +/- 0.06 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:54:06.84 -03:35:11.8: 12.81 +/- 0.04 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:43:09.26 -05:45:44.5: 13.00 +/- 0.07 detection
Forced photometry reference-image weighted average: 12.87 +/- 0.04
Forced photometry filter KEPT candidate at 18:43:09.26 -05:45:44.5: ref_mag=12.87 +/- 0.04 new_mean_mag=11.4397 delta=1.43 (need > 0.90)
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:54:06.84 -03:35:11.8: 13.06 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.03
Forced photometry filter KEPT candidate at 18:54:06.84 -03:35:11.8: ref_mag=12.90 +/- 0.03 new_mean_mag=11.7434 delta=1.16 (need > 0.90)
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:47:05.58 -03:31:45.4: 11.79 +/- 0.01 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:41:00.87 -05:51:40.1: 11.73 +/- 0.02 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:38:36.26 -06:52:40.1: 12.26 +/- 0.03 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:47:05.58 -03:31:45.4: 12.04 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.88 +/- 0.01
Forced photometry filter KEPT candidate at 18:47:05.58 -03:31:45.4: ref_mag=11.88 +/- 0.01 new_mean_mag=10.8513 delta=1.03 (need > 0.90)
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 19:03:12.37 +02:16:05.5: 11.01 +/- 0.01 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:41:00.87 -05:51:40.1: 11.90 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.80 +/- 0.01
Forced photometry filter KEPT candidate at 18:41:00.87 -05:51:40.1: ref_mag=11.80 +/- 0.01 new_mean_mag=10.7250 delta=1.07 (need > 0.90)
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:38:36.26 -06:52:40.1: 12.45 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.33 +/- 0.02
Forced photometry filter KEPT candidate at 18:38:36.26 -06:52:40.1: ref_mag=12.33 +/- 0.02 new_mean_mag=11.3079 delta=1.02 (need > 0.90)
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:44:02.34 -04:52:58.4: 12.47 +/- 0.04 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 19:03:12.37 +02:16:05.5: 11.10 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.05 +/- 0.01
Forced photometry filter KEPT candidate at 19:03:12.37 +02:16:05.5: ref_mag=11.05 +/- 0.01 new_mean_mag=10.0908 delta=0.96 (need > 0.90)
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:52:12.40 -04:23:38.1: 12.22 +/- 0.02 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:44:02.34 -04:52:58.4: 12.72 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.56 +/- 0.03
Forced photometry filter KEPT candidate at 18:44:02.34 -04:52:58.4: ref_mag=12.56 +/- 0.03 new_mean_mag=11.4877 delta=1.08 (need > 0.90)
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:52:12.40 -04:23:38.1: 12.29 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.25 +/- 0.02
Forced photometry filter KEPT candidate at 18:52:12.40 -04:23:38.1: ref_mag=12.25 +/- 0.02 new_mean_mag=11.2327 delta=1.02 (need > 0.90)
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:46:27.77 -04:33:22.9: 11.63 +/- 0.01 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:46:27.77 -04:33:22.9: 11.84 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.71 +/- 0.01
Forced photometry filter KEPT candidate at 18:46:27.77 -04:33:22.9: ref_mag=11.71 +/- 0.01 new_mean_mag=10.7184 delta=0.99 (need > 0.90)
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 19:02:04.94 +00:57:48.9: 10.80 +/- 0.01 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 19:02:04.94 +00:57:48.9: 10.86 +/- 0.01 detection
Forced photometry reference-image weighted average: 10.83 +/- 0.00
Forced photometry filter REJECTED candidate at 19:02:04.94 +00:57:48.9: ref_mag=10.83 +/- 0.00 new_mean_mag=9.9275 delta=0.90 (need > 0.90)
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:45:27.10 -05:19:52.6: 12.52 +/- 0.04 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:52:51.63 -01:20:09.9: 12.50 +/- 0.04 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:40:53.07 -06:20:26.4: 11.57 +/- 0.01 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:45:27.10 -05:19:52.6: 12.82 +/- 0.06 detection
Forced photometry reference-image weighted average: 12.62 +/- 0.03
Forced photometry filter KEPT candidate at 18:45:27.10 -05:19:52.6: ref_mag=12.62 +/- 0.03 new_mean_mag=11.3787 delta=1.25 (need > 0.90)
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:41:28.14 -06:52:36.2: 10.68 +/- 0.01 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:52:51.63 -01:20:09.9: 12.64 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.55 +/- 0.03
Forced photometry filter KEPT candidate at 18:52:51.63 -01:20:09.9: ref_mag=12.55 +/- 0.03 new_mean_mag=11.5101 delta=1.04 (need > 0.90)
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:40:53.07 -06:20:26.4: 11.77 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.65 +/- 0.01
Forced photometry filter KEPT candidate at 18:40:53.07 -06:20:26.4: ref_mag=11.65 +/- 0.01 new_mean_mag=10.6649 delta=0.98 (need > 0.90)
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:41:28.14 -06:52:36.2: 10.90 +/- 0.01 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:42:05.56 -05:00:50.1: 10.48 +/- 0.01 detection
Forced photometry reference-image weighted average: 10.76 +/- 0.01
Forced photometry filter KEPT candidate at 18:41:28.14 -06:52:36.2: ref_mag=10.76 +/- 0.01 new_mean_mag=9.8448 delta=0.92 (need > 0.90)
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:51:34.89 -03:16:31.8: 12.44 +/- 0.02 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:50:05.51 -04:00:13.6: 12.14 +/- 0.02 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:42:05.56 -05:00:50.1: 10.82 +/- 0.01 detection
Forced photometry reference-image weighted average: 10.59 +/- 0.00
Forced photometry filter KEPT candidate at 18:42:05.56 -05:00:50.1: ref_mag=10.59 +/- 0.00 new_mean_mag=9.5826 delta=1.01 (need > 0.90)
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:51:34.89 -03:16:31.8: 12.60 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.50 +/- 0.02
Forced photometry filter KEPT candidate at 18:51:34.89 -03:16:31.8: ref_mag=12.50 +/- 0.02 new_mean_mag=11.2470 delta=1.25 (need > 0.90)
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:50:05.51 -04:00:13.6: 12.33 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.21 +/- 0.01
Forced photometry filter KEPT candidate at 18:50:05.51 -04:00:13.6: ref_mag=12.21 +/- 0.01 new_mean_mag=11.2454 delta=0.97 (need > 0.90)
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:52:25.84 -00:53:33.0: 12.89 +/- 0.04 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:47:33.60 -05:08:13.4: 12.44 +/- 0.03 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:52:25.84 -00:53:33.0: 13.09 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.97 +/- 0.03
Forced photometry filter KEPT candidate at 18:52:25.84 -00:53:33.0: ref_mag=12.97 +/- 0.03 new_mean_mag=11.8159 delta=1.15 (need > 0.90)
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:47:33.60 -05:08:13.4: 12.81 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.55 +/- 0.02
Forced photometry filter KEPT candidate at 18:47:33.60 -05:08:13.4: ref_mag=12.55 +/- 0.02 new_mean_mag=11.2940 delta=1.26 (need > 0.90)
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:47:29.40 -05:02:36.0: 12.42 +/- 0.03 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 19:00:55.16 +01:22:15.8: 12.74 +/- 0.04 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:47:29.40 -05:02:36.0: 12.63 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.50 +/- 0.02
Forced photometry filter KEPT candidate at 18:47:29.40 -05:02:36.0: ref_mag=12.50 +/- 0.02 new_mean_mag=11.2949 delta=1.21 (need > 0.90)
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 19:00:55.16 +01:22:15.8: 12.91 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.80 +/- 0.03
Forced photometry filter KEPT candidate at 19:00:55.16 +01:22:15.8: ref_mag=12.80 +/- 0.03 new_mean_mag=11.7816 delta=1.02 (need > 0.90)
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:57:56.01 -00:45:25.8: 11.44 +/- 0.01 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:57:56.01 -00:45:25.8: 11.63 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.51 +/- 0.01
Forced photometry filter KEPT candidate at 18:57:56.01 -00:45:25.8: ref_mag=11.51 +/- 0.01 new_mean_mag=10.5250 delta=0.99 (need > 0.90)
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:44:45.01 -06:21:22.3: 12.33 +/- 0.05 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:37:09.76 -05:39:09.4: 12.07 +/- 0.02 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:44:45.01 -06:21:22.3: 12.55 +/- 0.06 detection
Forced photometry reference-image weighted average: 12.42 +/- 0.04
Forced photometry filter KEPT candidate at 18:44:45.01 -06:21:22.3: ref_mag=12.42 +/- 0.04 new_mean_mag=11.3521 delta=1.06 (need > 0.90)
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:45:41.54 -05:35:45.6: 9.61 +/- 0.00 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:37:09.76 -05:39:09.4: 12.34 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.16 +/- 0.02
Forced photometry filter KEPT candidate at 18:37:09.76 -05:39:09.4: ref_mag=12.16 +/- 0.02 new_mean_mag=11.1971 delta=0.96 (need > 0.90)
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:45:41.54 -05:35:45.6: 9.89 +/- 0.01 detection
Forced photometry reference-image weighted average: 9.71 +/- 0.00
Forced photometry filter KEPT candidate at 18:45:41.54 -05:35:45.6: ref_mag=9.71 +/- 0.00 new_mean_mag=8.6305 delta=1.07 (need > 0.90)
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:38:11.63 -05:25:33.3: 12.07 +/- 0.02 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:54:55.93 -01:21:23.5: 12.68 +/- 0.03 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:49:11.67 -04:12:21.4: 12.05 +/- 0.02 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:38:11.63 -05:25:33.3: 12.43 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.18 +/- 0.02
Forced photometry filter KEPT candidate at 18:38:11.63 -05:25:33.3: ref_mag=12.18 +/- 0.02 new_mean_mag=11.0834 delta=1.10 (need > 0.90)
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:54:55.93 -01:21:23.5: 12.84 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.74 +/- 0.02
Forced photometry filter KEPT candidate at 18:54:55.93 -01:21:23.5: ref_mag=12.74 +/- 0.02 new_mean_mag=11.7224 delta=1.02 (need > 0.90)
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:49:11.67 -04:12:21.4: 12.12 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.08 +/- 0.01
Forced photometry filter KEPT candidate at 18:49:11.67 -04:12:21.4: ref_mag=12.08 +/- 0.01 new_mean_mag=11.1318 delta=0.95 (need > 0.90)
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:41:56.86 -05:26:26.1: 11.38 +/- 0.02 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:44:49.52 -04:33:03.7: 12.04 +/- 0.02 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:41:56.86 -05:26:26.1: 11.65 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.47 +/- 0.01
Forced photometry filter KEPT candidate at 18:41:56.86 -05:26:26.1: ref_mag=11.47 +/- 0.01 new_mean_mag=10.4489 delta=1.02 (need > 0.90)
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 18:41:04.28 -06:25:11.8: 11.95 +/- 0.02 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:44:49.52 -04:33:03.7: 12.17 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.09 +/- 0.01
Forced photometry filter KEPT candidate at 18:44:49.52 -04:33:03.7: ref_mag=12.09 +/- 0.01 new_mean_mag=11.1507 delta=0.94 (need > 0.90)
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-16_02-47-39_20.00sec_-4.90C_LIGHTs_0245.fits at 19:07:20.84 +02:02:16.6: 12.64 +/- 0.03 detection
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 18:41:04.28 -06:25:11.8: 12.06 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.99 +/- 0.02
Forced photometry filter KEPT candidate at 18:41:04.28 -06:25:11.8: ref_mag=11.99 +/- 0.02 new_mean_mag=11.0697 delta=0.92 (need > 0.90)
Forced photometry on wcs_Aql-03-Q1b1x1_2026-04-18_03-20-48_20.00sec_-4.90C_LIGHT_0119.fits at 19:07:20.84 +02:02:16.6: 12.56 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.60 +/- 0.02
Forced photometry filter KEPT candidate at 19:07:20.84 +02:02:16.6: ref_mag=12.60 +/- 0.02 new_mean_mag=11.6736 delta=0.93 (need > 0.90)
Adding exclusion_list_gaiadr2.txt__out147330.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out147349.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out03795.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04058.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out100132.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103504.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out111091.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out111836.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115521.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115718.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12771.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14023.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15392.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15941.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out16362.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out23041.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out23623.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24425.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25278.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25354.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25686.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out27771.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29323.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29524.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out30179.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31872.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33372.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35881.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36283.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36872.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out38018.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out39417.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out43502.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out43787.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out43833.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out45844.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out47109.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out47300.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out47649.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out48547.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out49216.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out50836.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52457.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52584.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54825.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55757.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out57967.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77499.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77518.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out89353.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out91102.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out93361.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 27s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 21s
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Considering the candidate 147330_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
The candidate 147330_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
**** FOUND 18:43:26.32 -05:46:21.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.69, MAG_FAINT_SEARCH_LIMIT=11.67)GAIADR2_OUTPUT=# 0.260 4253437681048005376 280.85960499514 -05.77253796580 10.8738 9.5999 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.260#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 147334_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
The candidate 147334_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
**** FOUND 19:03:37.32 +01:48:46.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 147339_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
The candidate 147339_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
**** FOUND 18:47:01.79 -04:44:31.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 147342_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
The candidate 147342_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
**** FOUND 18:44:52.99 -06:07:38.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 147348_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
The candidate 147348_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
**** FOUND 18:42:23.81 -02:22:03.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 147349_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
The candidate 147349_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
**** FOUND 18:55:41.71 +00:20:49.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.81, MAG_FAINT_SEARCH_LIMIT=12.79)GAIADR2_OUTPUT=# 0.576 4266622440300416512 283.92372481359 +00.34702115068 10.3674 8.7930 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.576#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54816_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
The candidate 54816_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
**** FOUND 18:21:17.85 -02:54:15.7 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 39367_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
The candidate 39367_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
**** FOUND 18:47:10.62 -04:44:51.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 47649_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 47649_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
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Considering the candidate 57549_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
The candidate 57549_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
**** FOUND 18:54:28.06 -03:23:58.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 119400_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
The candidate 119400_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
**** FOUND 18:56:08.83 -00:28:32.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 115521_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 115521_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
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Considering the candidate 23623_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 23623_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
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Considering the candidate 26184_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
The candidate 26184_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
**** FOUND 18:43:01.34 -05:42:32.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52457_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 52457_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
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Considering the candidate 15941_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 15941_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
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Considering the candidate 23445_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
The candidate 23445_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
**** FOUND 18:43:16.94 -05:53:18.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 45844_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 45844_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
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Considering the candidate 43502_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 43502_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
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Considering the candidate 24394_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
The candidate 24394_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
**** FOUND 18:47:40.48 -05:56:02.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 16362_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 16362_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
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Considering the candidate 24425_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 24425_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
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Considering the candidate 40647_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
The candidate 40647_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
**** FOUND 18:43:37.67 -04:46:32.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 111091_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 111091_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
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Considering the candidate 52584_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 52584_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
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Considering the candidate 31872_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 31872_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
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Considering the candidate 47300_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 47300_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
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Considering the candidate 81725_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
The candidate 81725_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
**** FOUND 19:06:05.51 -01:12:15.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 35881_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 35881_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
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Considering the candidate 38752_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
The candidate 38752_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
**** FOUND 18:51:20.45 -05:03:32.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 29293_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
The candidate 29293_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
**** FOUND 18:45:53.32 -05:32:42.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 25354_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 25354_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
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Considering the candidate 29524_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 29524_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
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Considering the candidate 100132_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 100132_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
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Considering the candidate 49216_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 49216_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
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Considering the candidate 09735_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
The candidate 09735_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
**** FOUND 18:43:16.39 -06:36:27.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 30322_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
The candidate 30322_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
**** FOUND 18:43:32.87 -05:28:59.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 103504_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 103504_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
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Considering the candidate 99311_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
The candidate 99311_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
**** FOUND 19:06:34.44 +00:25:41.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 25686_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 25686_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
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Considering the candidate 55757_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 55757_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
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Considering the candidate 58539_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
The candidate 58539_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
**** FOUND 18:52:35.81 -03:12:17.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 37302_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
The candidate 37302_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
**** FOUND 18:50:47.01 -05:09:11.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54825_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 54825_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
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Considering the candidate 78527_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
The candidate 78527_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
**** FOUND 18:53:54.58 -01:16:02.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 23041_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 23041_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
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Considering the candidate 77029_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
The candidate 77029_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
**** FOUND 18:34:14.83 -00:58:42.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 03795_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 03795_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
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Considering the candidate 89353_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 89353_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
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Considering the candidate 95640_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
The candidate 95640_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
**** FOUND 19:02:39.60 +01:29:13.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 39417_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 39417_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
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Considering the candidate 47109_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 47109_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
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Considering the candidate 43833_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 43833_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
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Considering the candidate 91594_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
The candidate 91594_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
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Considering the candidate 51377_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
The candidate 51377_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
**** FOUND 18:44:16.34 -03:48:53.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 59853_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
The candidate 59853_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
**** FOUND 18:46:32.07 -02:57:22.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 33372_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 33372_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
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Considering the candidate 77499_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 77499_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
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Considering the candidate 14023_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 14023_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
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Considering the candidate 40830_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
The candidate 40830_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
**** FOUND 18:46:39.95 -04:48:37.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 04058_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 04058_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
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Considering the candidate 04923_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
The candidate 04923_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
**** FOUND 18:39:58.21 -06:49:02.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 36283_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 36283_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
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Considering the candidate 57967_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 57967_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
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Considering the candidate 105892_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
The candidate 105892_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
**** FOUND 19:03:43.27 +01:50:45.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 50836_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 50836_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
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Considering the candidate 115718_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 115718_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
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Considering the candidate 36872_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 36872_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
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Considering the candidate 38018_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 38018_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
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Considering the candidate 91102_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 91102_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
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Considering the candidate 88870_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
The candidate 88870_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
**** FOUND 19:06:13.63 +02:16:19.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 10426_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
The candidate 10426_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
**** FOUND 18:37:04.31 -06:23:26.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 93361_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 93361_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
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Considering the candidate 96297_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
The candidate 96297_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
**** FOUND 19:02:21.07 +01:30:40.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 15392_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 15392_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
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Considering the candidate 59920_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
The candidate 59920_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
**** FOUND 18:21:58.92 -02:29:38.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 25278_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 25278_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
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Considering the candidate 27771_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 27771_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
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Considering the candidate 108045_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
The candidate 108045_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
**** FOUND 19:08:36.90 -00:04:48.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 107162_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
The candidate 107162_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
**** FOUND 19:04:28.15 +00:03:07.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 29323_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 29323_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
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Considering the candidate 77518_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 77518_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
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Considering the candidate 48547_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 48547_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
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Considering the candidate 30179_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 30179_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
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Considering the candidate 43787_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 43787_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
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Considering the candidate 20068_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
The candidate 20068_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
**** FOUND 18:42:39.79 -06:03:09.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 12771_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 12771_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
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Considering the candidate 111836_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
Preparing report for the candidate 111836_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
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Considering the candidate 53617_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
The candidate 53617_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
**** FOUND 18:42:31.51 -03:35:38.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56883_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
The candidate 56883_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
**** FOUND 18:51:22.18 -03:19:05.0 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 24422_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
The candidate 24422_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
**** FOUND 18:47:28.96 -05:42:18.0 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 25753_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
The candidate 25753_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
**** FOUND 18:57:03.77 -05:50:48.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 27648_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
The candidate 27648_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
**** FOUND 19:01:40.73 -05:44:22.6 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 42697_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
The candidate 42697_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
**** FOUND 19:06:14.74 -04:53:01.1 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103502_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
The candidate 103502_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
**** FOUND 18:44:50.04 +02:03:32.3 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 91958_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
The candidate 91958_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
**** FOUND 19:18:32.51 +01:05:04.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 65516_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
The candidate 65516_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
**** FOUND 18:29:41.12 -01:59:09.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 87250_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117
The candidate 87250_fd_Aql-03-Q1b1x1_2026-05-26_00-25-51_20.00sec_-0.00C_LIGHTs_0117 did not pass the final checks
**** FOUND 19:13:42.75 +02:17:36.2 in the exclusion list exclusion_list_bsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 4s
make_report_in_HTML.sh TOTAL: 52s
Prepared the HTML report for the field Aql-03-Q1b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
18:38:36.26 -06:52:40.1
18:41:28.14 -06:52:36.2
19:00:02.00 +01:41:01.9
19:08:04.45 +01:39:31.3
19:02:38.10 +01:19:22.8
19:07:20.84 +02:02:16.6
18:56:10.70 -00:15:44.4
18:52:25.84 -00:53:33.0
18:41:04.28 -06:25:11.8
18:40:53.07 -06:20:26.4
18:44:45.01 -06:21:22.3
18:38:28.86 -06:11:48.5
18:42:44.42 -06:15:55.8
18:41:00.87 -05:51:40.1
18:42:33.14 -05:52:11.3
18:42:17.40 -05:48:53.9
18:37:09.76 -05:39:09.4
18:46:27.11 -05:49:54.8
18:43:09.26 -05:45:44.5
18:45:41.54 -05:35:45.6
18:38:11.63 -05:25:33.3
18:44:01.87 -05:31:51.4
18:41:56.86 -05:26:26.1
18:42:35.13 -05:22:13.6
18:45:27.10 -05:19:52.6
18:42:03.84 -05:04:57.8
18:42:05.56 -05:00:50.1
18:47:33.60 -05:08:13.4
18:47:29.40 -05:02:36.0
18:44:02.34 -04:52:58.4
18:47:34.16 -04:36:35.5
18:44:49.52 -04:33:03.7
18:46:27.77 -04:33:22.9
18:52:17.95 -04:29:22.7
18:52:12.40 -04:23:38.1
18:46:44.64 -04:16:41.7
18:48:23.57 -04:16:42.2
18:49:11.67 -04:12:21.4
18:52:15.62 -04:12:09.2
18:50:05.51 -04:00:13.6
18:51:55.89 -03:53:31.5
18:49:44.64 -03:49:31.9
18:47:05.58 -03:31:45.4
18:54:06.84 -03:35:11.8
18:51:34.89 -03:16:31.8
18:52:51.63 -01:20:09.9
18:54:55.93 -01:21:23.5
19:03:12.37 +02:16:05.5
19:00:55.16 +01:22:15.8
18:57:56.01 -00:45:25.8
########### Completed Aql-03-Q1b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ1.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
18:48:23.57 -04:16:42.2
18:56:10.70 -00:15:44.4
18:42:33.14 -05:52:11.3
18:51:55.89 -03:53:31.5
18:38:28.86 -06:11:48.5
18:52:17.95 -04:29:22.7
18:47:34.16 -04:36:35.5
18:42:44.42 -06:15:55.8
18:42:17.40 -05:48:53.9
19:02:38.10 +01:19:22.8
18:49:44.64 -03:49:31.9
18:42:35.13 -05:22:13.6
18:46:44.64 -04:16:41.7
18:42:03.84 -05:04:57.8
18:46:27.11 -05:49:54.8
18:44:01.87 -05:31:51.4
19:00:02.00 +01:41:01.9
18:52:15.62 -04:12:09.2
19:08:04.45 +01:39:31.3
18:43:09.26 -05:45:44.5
18:54:06.84 -03:35:11.8
18:47:05.58 -03:31:45.4
18:41:00.87 -05:51:40.1
18:38:36.26 -06:52:40.1
19:03:12.37 +02:16:05.5
18:44:02.34 -04:52:58.4
18:52:12.40 -04:23:38.1
18:46:27.77 -04:33:22.9
18:45:27.10 -05:19:52.6
18:52:51.63 -01:20:09.9
18:40:53.07 -06:20:26.4
18:41:28.14 -06:52:36.2
18:42:05.56 -05:00:50.1
18:51:34.89 -03:16:31.8
18:50:05.51 -04:00:13.6
18:52:25.84 -00:53:33.0
18:47:33.60 -05:08:13.4
18:47:29.40 -05:02:36.0
19:00:55.16 +01:22:15.8
18:57:56.01 -00:45:25.8
18:44:45.01 -06:21:22.3
18:37:09.76 -05:39:09.4
18:45:41.54 -05:35:45.6
18:38:11.63 -05:25:33.3
18:54:55.93 -01:21:23.5
18:49:11.67 -04:12:21.4
18:41:56.86 -05:26:26.1
18:44:49.52 -04:33:03.7
18:41:04.28 -06:25:11.8
19:07:20.84 +02:02:16.6
###################################################################################
18:48:23.57 -04:16:42.2 -- not an asteroid (will add it to exclusion list)
18:56:10.70 -00:15:44.4 -- not an asteroid (will add it to exclusion list)
18:42:33.14 -05:52:11.3 -- not an asteroid (will add it to exclusion list)
18:51:55.89 -03:53:31.5 -- not an asteroid (will add it to exclusion list)
18:38:28.86 -06:11:48.5 -- not an asteroid (will add it to exclusion list)
18:52:17.95 -04:29:22.7 -- not an asteroid (will add it to exclusion list)
18:47:34.16 -04:36:35.5 -- not an asteroid (will add it to exclusion list)
18:42:44.42 -06:15:55.8 -- not an asteroid (will add it to exclusion list)
18:42:17.40 -05:48:53.9 -- not an asteroid (will add it to exclusion list)
19:02:38.10 +01:19:22.8 -- not an asteroid (will add it to exclusion list)
18:49:44.64 -03:49:31.9 -- not an asteroid (will add it to exclusion list)
18:42:35.13 -05:22:13.6 -- not an asteroid (will add it to exclusion list)
18:46:44.64 -04:16:41.7 -- not an asteroid (will add it to exclusion list)
18:42:03.84 -05:04:57.8 -- not an asteroid (will add it to exclusion list)
18:46:27.11 -05:49:54.8 -- not an asteroid (will add it to exclusion list)
18:44:01.87 -05:31:51.4 -- not an asteroid (will add it to exclusion list)
19:00:02.00 +01:41:01.9 -- not an asteroid (will add it to exclusion list)
18:52:15.62 -04:12:09.2 -- not an asteroid (will add it to exclusion list)
19:08:04.45 +01:39:31.3 -- not an asteroid (will add it to exclusion list)
18:43:09.26 -05:45:44.5 -- not an asteroid (will add it to exclusion list)
18:54:06.84 -03:35:11.8 -- not an asteroid (will add it to exclusion list)
18:47:05.58 -03:31:45.4 -- not an asteroid (will add it to exclusion list)
18:41:00.87 -05:51:40.1 -- not an asteroid (will add it to exclusion list)
18:38:36.26 -06:52:40.1 -- not an asteroid (will add it to exclusion list)
19:03:12.37 +02:16:05.5 -- not an asteroid (will add it to exclusion list)
18:44:02.34 -04:52:58.4 -- not an asteroid (will add it to exclusion list)
18:52:12.40 -04:23:38.1 -- not an asteroid (will add it to exclusion list)
18:46:27.77 -04:33:22.9 -- not an asteroid (will add it to exclusion list)
18:45:27.10 -05:19:52.6 -- not an asteroid (will add it to exclusion list)
18:52:51.63 -01:20:09.9 -- not an asteroid (will add it to exclusion list)
18:40:53.07 -06:20:26.4 -- not an asteroid (will add it to exclusion list)
18:41:28.14 -06:52:36.2 -- not an asteroid (will add it to exclusion list)
18:42:05.56 -05:00:50.1 -- not an asteroid (will add it to exclusion list)
18:51:34.89 -03:16:31.8 -- not an asteroid (will add it to exclusion list)
18:50:05.51 -04:00:13.6 -- not an asteroid (will add it to exclusion list)
18:52:25.84 -00:53:33.0 -- not an asteroid (will add it to exclusion list)
18:47:33.60 -05:08:13.4 -- not an asteroid (will add it to exclusion list)
18:47:29.40 -05:02:36.0 -- not an asteroid (will add it to exclusion list)
19:00:55.16 +01:22:15.8 -- not an asteroid (will add it to exclusion list)
18:57:56.01 -00:45:25.8 -- not an asteroid (will add it to exclusion list)
18:44:45.01 -06:21:22.3 -- not an asteroid (will add it to exclusion list)
18:37:09.76 -05:39:09.4 -- not an asteroid (will add it to exclusion list)
18:45:41.54 -05:35:45.6 -- not an asteroid (will add it to exclusion list)
18:38:11.63 -05:25:33.3 -- not an asteroid (will add it to exclusion list)
18:54:55.93 -01:21:23.5 -- not an asteroid (will add it to exclusion list)
18:49:11.67 -04:12:21.4 -- not an asteroid (will add it to exclusion list)
18:41:56.86 -05:26:26.1 -- not an asteroid (will add it to exclusion list)
18:44:49.52 -04:33:03.7 -- not an asteroid (will add it to exclusion list)
18:41:04.28 -06:25:11.8 -- not an asteroid (will add it to exclusion list)
19:07:20.84 +02:02:16.6 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
18:37:09.76 -05:39:09.4 -- does not seem to be a hot pixel (will add it to exclusion list)
18:38:11.63 -05:25:33.3 -- does not seem to be a hot pixel (will add it to exclusion list)
18:38:28.86 -06:11:48.5 -- does not seem to be a hot pixel (will add it to exclusion list)
18:38:36.26 -06:52:40.1 -- does not seem to be a hot pixel (will add it to exclusion list)
18:40:53.07 -06:20:26.4 -- does not seem to be a hot pixel (will add it to exclusion list)
18:41:00.87 -05:51:40.1 -- does not seem to be a hot pixel (will add it to exclusion list)
18:41:04.28 -06:25:11.8 -- does not seem to be a hot pixel (will add it to exclusion list)
18:41:28.14 -06:52:36.2 -- does not seem to be a hot pixel (will add it to exclusion list)
18:41:56.86 -05:26:26.1 -- does not seem to be a hot pixel (will add it to exclusion list)
18:42:03.84 -05:04:57.8 -- does not seem to be a hot pixel (will add it to exclusion list)
18:42:05.56 -05:00:50.1 -- does not seem to be a hot pixel (will add it to exclusion list)
18:42:17.40 -05:48:53.9 -- does not seem to be a hot pixel (will add it to exclusion list)
18:42:33.14 -05:52:11.3 -- does not seem to be a hot pixel (will add it to exclusion list)
18:42:35.13 -05:22:13.6 -- does not seem to be a hot pixel (will add it to exclusion list)
18:42:44.42 -06:15:55.8 -- does not seem to be a hot pixel (will add it to exclusion list)
18:43:09.26 -05:45:44.5 -- does not seem to be a hot pixel (will add it to exclusion list)
18:44:01.87 -05:31:51.4 -- does not seem to be a hot pixel (will add it to exclusion list)
18:44:02.34 -04:52:58.4 -- does not seem to be a hot pixel (will add it to exclusion list)
18:44:45.01 -06:21:22.3 -- does not seem to be a hot pixel (will add it to exclusion list)
18:44:49.52 -04:33:03.7 -- does not seem to be a hot pixel (will add it to exclusion list)
18:45:27.10 -05:19:52.6 -- does not seem to be a hot pixel (will add it to exclusion list)
18:45:41.54 -05:35:45.6 -- does not seem to be a hot pixel (will add it to exclusion list)
18:46:27.11 -05:49:54.8 -- does not seem to be a hot pixel (will add it to exclusion list)
18:46:27.77 -04:33:22.9 -- does not seem to be a hot pixel (will add it to exclusion list)
18:46:44.64 -04:16:41.7 -- does not seem to be a hot pixel (will add it to exclusion list)
18:47:05.58 -03:31:45.4 -- does not seem to be a hot pixel (will add it to exclusion list)
18:47:29.40 -05:02:36.0 -- does not seem to be a hot pixel (will add it to exclusion list)
18:47:33.60 -05:08:13.4 -- does not seem to be a hot pixel (will add it to exclusion list)
18:47:34.16 -04:36:35.5 -- does not seem to be a hot pixel (will add it to exclusion list)
18:48:23.57 -04:16:42.2 -- does not seem to be a hot pixel (will add it to exclusion list)
18:49:11.67 -04:12:21.4 -- does not seem to be a hot pixel (will add it to exclusion list)
18:49:44.64 -03:49:31.9 -- does not seem to be a hot pixel (will add it to exclusion list)
18:50:05.51 -04:00:13.6 -- does not seem to be a hot pixel (will add it to exclusion list)
18:51:34.89 -03:16:31.8 -- does not seem to be a hot pixel (will add it to exclusion list)
18:51:55.89 -03:53:31.5 -- does not seem to be a hot pixel (will add it to exclusion list)
18:52:12.40 -04:23:38.1 -- does not seem to be a hot pixel (will add it to exclusion list)
18:52:15.62 -04:12:09.2 -- does not seem to be a hot pixel (will add it to exclusion list)
18:52:17.95 -04:29:22.7 -- does not seem to be a hot pixel (will add it to exclusion list)
18:52:25.84 -00:53:33.0 -- does not seem to be a hot pixel (will add it to exclusion list)
18:52:51.63 -01:20:09.9 -- does not seem to be a hot pixel (will add it to exclusion list)
18:54:06.84 -03:35:11.8 -- does not seem to be a hot pixel (will add it to exclusion list)
18:54:55.93 -01:21:23.5 -- does not seem to be a hot pixel (will add it to exclusion list)
18:56:10.70 -00:15:44.4 -- does not seem to be a hot pixel (will add it to exclusion list)
18:57:56.01 -00:45:25.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:00:02.00 +01:41:01.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:00:55.16 +01:22:15.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:02:38.10 +01:19:22.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:03:12.37 +02:16:05.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:07:20.84 +02:02:16.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:08:04.45 +01:39:31.3 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
18:37:09.76 -05:39:09.4 -- a known variable star
18:38:11.63 -05:25:33.3 -- a known variable star
18:38:28.86 -06:11:48.5 -- a known variable star
18:38:36.26 -06:52:40.1 -- a known variable star
18:40:53.07 -06:20:26.4 -- not a known variable star
18:41:00.87 -05:51:40.1 -- a known variable star
18:41:04.28 -06:25:11.8 -- a known variable star
18:41:28.14 -06:52:36.2 -- a known variable star
18:41:56.86 -05:26:26.1 -- a known variable star
18:42:03.84 -05:04:57.8 -- a known variable star
18:42:05.56 -05:00:50.1 -- a known variable star
18:42:17.40 -05:48:53.9 -- a known variable star
18:42:33.14 -05:52:11.3 -- a known variable star
18:42:35.13 -05:22:13.6 -- a known variable star
18:42:44.42 -06:15:55.8 -- a known variable star
18:43:09.26 -05:45:44.5 -- a known variable star
18:44:01.87 -05:31:51.4 -- a known variable star
18:44:02.34 -04:52:58.4 -- a known variable star
18:44:45.01 -06:21:22.3 -- a known variable star
18:44:49.52 -04:33:03.7 -- a known variable star
18:45:27.10 -05:19:52.6 -- a known variable star
18:45:41.54 -05:35:45.6 -- a known variable star
18:46:27.11 -05:49:54.8 -- a known variable star
18:46:27.77 -04:33:22.9 -- a known variable star
18:46:44.64 -04:16:41.7 -- not a known variable star
18:47:05.58 -03:31:45.4 -- a known variable star
18:47:29.40 -05:02:36.0 -- a known variable star
18:47:33.60 -05:08:13.4 -- a known variable star
18:47:34.16 -04:36:35.5 -- a known variable star
18:48:23.57 -04:16:42.2 -- a known variable star
18:49:11.67 -04:12:21.4 -- not a known variable star
18:49:44.64 -03:49:31.9 -- a known variable star
18:50:05.51 -04:00:13.6 -- not a known variable star
18:51:34.89 -03:16:31.8 -- a known variable star
18:51:55.89 -03:53:31.5 -- a known variable star
18:52:12.40 -04:23:38.1 -- a known variable star
18:52:15.62 -04:12:09.2 -- a known variable star
18:52:17.95 -04:29:22.7 -- a known variable star
18:52:25.84 -00:53:33.0 -- a known variable star
18:52:51.63 -01:20:09.9 -- a known variable star
18:54:06.84 -03:35:11.8 -- a known variable star
18:54:55.93 -01:21:23.5 -- a known variable star
18:56:10.70 -00:15:44.4 -- a known variable star
18:57:56.01 -00:45:25.8 -- a known variable star
19:00:02.00 +01:41:01.9 -- a known variable star
19:00:55.16 +01:22:15.8 -- a known variable star
19:02:38.10 +01:19:22.8 -- a known variable star
19:03:12.37 +02:16:05.5 -- a known variable star
19:07:20.84 +02:02:16.6 -- a known variable star
19:08:04.45 +01:39:31.3 -- a known variable star
Found 4 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
50 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
###################################################################################
Adding identified Gaia sources from exclusion_list_gaiadr2.txt
exclusion_list_apass.txt NOT FOUND
IS_THIS_TEST_RUN= NO ALLOW_EXCLUSION_LIST_UPDATE= YES
#### Adding the following to the exclusion list ####
18:37:09.76 -05:39:09.4
18:38:11.63 -05:25:33.3
18:38:28.86 -06:11:48.5
18:38:36.26 -06:52:40.1
18:40:53.07 -06:20:26.4
18:41:00.87 -05:51:40.1
18:41:04.28 -06:25:11.8
18:41:28.14 -06:52:36.2
18:41:56.86 -05:26:26.1
18:42:03.84 -05:04:57.8
18:42:05.56 -05:00:50.1
18:42:17.40 -05:48:53.9
18:42:33.14 -05:52:11.3
18:42:35.13 -05:22:13.6
18:42:44.42 -06:15:55.8
18:43:09.26 -05:45:44.5
18:44:01.87 -05:31:51.4
18:44:02.34 -04:52:58.4
18:44:45.01 -06:21:22.3
18:44:49.52 -04:33:03.7
18:45:27.10 -05:19:52.6
18:45:41.54 -05:35:45.6
18:46:27.11 -05:49:54.8
18:46:27.77 -04:33:22.9
18:46:44.64 -04:16:41.7
18:47:05.58 -03:31:45.4
18:47:29.40 -05:02:36.0
18:47:33.60 -05:08:13.4
18:47:34.16 -04:36:35.5
18:48:23.57 -04:16:42.2
18:49:11.67 -04:12:21.4
18:49:44.64 -03:49:31.9
18:50:05.51 -04:00:13.6
18:51:34.89 -03:16:31.8
18:51:55.89 -03:53:31.5
18:52:12.40 -04:23:38.1
18:52:15.62 -04:12:09.2
18:52:17.95 -04:29:22.7
18:52:25.84 -00:53:33.0
18:52:51.63 -01:20:09.9
18:54:06.84 -03:35:11.8
18:54:55.93 -01:21:23.5
18:56:10.70 -00:15:44.4
18:57:56.01 -00:45:25.8
19:00:02.00 +01:41:01.9
19:00:55.16 +01:22:15.8
19:02:38.10 +01:19:22.8
19:03:12.37 +02:16:05.5
19:07:20.84 +02:02:16.6
19:08:04.45 +01:39:31.3
18:43:26.32 -05:46:21.0
18:55:41.71 +00:20:49.8
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The observatory MPC code is V36
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Positions of planets computed with util/planet_finder/main.py for JD(UT)2461186.72587461 -observatory V36
05:07:34.38 +24:43:54.0 Mercury (-1.1mag)
06:36:07.60 +24:58:51.9 Venus (-3.9mag)
02:12:10.52 +12:34:31.4 Mars (1.3mag)
07:38:01.10 +21:56:21.2 Jupiter (-1.9mag)
00:45:18.91 +02:25:57.9 Saturn (0.9mag)
03:57:04.76 +20:16:20.6 Uranus (5.8mag)
00:15:13.93 +00:11:34.9 Neptune (7.8mag)
20:33:56.19 -23:00:04.6 Pluto (14.5mag)
12:20:56.36 -06:00:54.9 Moon (-11.2mag)
-rw-r--r-- 1 apache apache 363 May 26 00:38 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461186.72587461:
07:37:55.81 +21:56:34.8 Io (5.9mag)
07:38:11.29 +21:55:52.0 Europa (6.1mag)
07:37:54.51 +21:56:44.6 Ganymede (5.5mag)
07:37:39.06 +21:57:15.3 Callisto (6.7mag)
07:39:06.06 +21:32:41.6 Himalia (15.5mag)
07:38:02.72 +21:56:18.0 Thebe (16.5mag)
07:39:24.38 +21:53:55.9 Elara (17.5mag)
07:39:29.05 +22:15:05.0 Pasiphae (17.7mag)
07:45:08.13 +21:57:10.9 Carme (18.8mag)
00:45:21.22 +02:25:38.1 Titan (8.7mag)
00:45:14.90 +02:26:05.3 Rhea (10.0mag)
00:45:41.66 +02:26:05.1 Iapetus (11.4mag)
00:45:33.61 +02:26:01.0 Hyperion (14.7mag)
00:46:16.50 +02:29:44.5 Phoebe (16.7mag)
-rw-r--r-- 1 apache apache 569 May 26 00:38 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461186.72587461:
17:17:18.26 -33:21:53.8 JWST
16:08:31.34 +51:44:30.6 Chandra
08:27:51.12 -46:27:42.7 XMM-Newton
-rw-r--r-- 1 apache apache 96 May 26 00:38 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461186.72587461 -observatory V36
13:20:44.67 -27:03:21.0 14.4mag D/1884 O1 (Barnard)
06:37:26.84 +30:40:15.1 15.7mag D/1886 K1 (Brooks)
15:26:15.26 +01:21:04.2 14.6mag D/1895 Q1 (Swift)
05:28:14.90 +24:39:00.0 17.2mag D/1918 W1 (Schorr)
09:31:40.34 +14:30:26.2 17.9mag P/2009 WX51 (Catalina)
18:50:59.86 -31:39:38.5 13.7mag P/2010 H2 (Vales)
05:40:55.50 -68:15:59.3 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:44:22.26 +31:48:31.8 17.4mag C/2017 K2 (PANSTARRS)
17:19:50.68 +14:33:07.9 17.7mag C/2021 G2 (ATLAS)
23:14:32.67 +31:02:56.5 17.2mag C/2022 E2 (ATLAS)
05:18:03.79 +26:51:30.3 16.4mag C/2022 N2 (PANSTARRS)
09:20:59.42 +31:29:31.6 16.5mag C/2022 QE78 (ATLAS)
08:44:02.31 +03:13:16.1 17.6mag C/2022 R6 (PANSTARRS)
18:36:20.16 +21:12:23.3 17.7mag C/2023 A3 (Tsuchinshan-ATLAS)
15:24:25.88 -11:02:15.4 17.5mag P/2023 B1 (PANSTARRS)
22:16:12.54 +65:39:56.7 17.7mag C/2023 H5 (Lemmon)
18:17:00.32 -05:32:21.8 13.7mag C/2023 R1 (PANSTARRS)
13:39:38.78 +85:47:30.6 17.9mag C/2023 X2 (Lemmon)
06:53:29.26 +63:55:46.0 17.6mag C/2024 A1 (ATLAS)
06:26:57.48 +26:29:12.2 13.1mag C/2024 E1 (Wierzchos)
15:47:50.78 +12:12:50.8 17.3mag C/2024 G6 (ATLAS)
20:19:46.92 +27:11:15.4 14.1mag C/2024 J3 (ATLAS)
04:05:01.59 -17:11:58.2 16.1mag C/2024 T5 (ATLAS)
05:53:42.09 +36:48:25.0 17.9mag C/2025 J1 (Borisov)
11:45:38.34 +53:20:08.0 16.9mag C/2025 L1 (ATLAS)
06:25:00.57 -10:11:28.6 12.7mag C/2025 R3 (PANSTARRS)
12:40:56.75 +04:37:01.4 17.2mag C/2025 Y1 (ATLAS)
01:36:24.30 +42:23:10.1 15.7mag C/2026 B2 (Sun-Gao)
11:10:26.29 -08:58:03.5 16.3mag A/2026 E1
19:59:45.07 -08:07:26.0 9.5mag 10P/Tempel
14:18:44.20 -02:35:49.2 17.6mag 24P/Schaumasse
10:59:43.45 -00:51:55.3 15.9mag 29P/Schwassmann-Wachmann
10:51:20.90 -02:34:29.0 17.8mag 43P/Wolf-Harrington
02:51:31.76 +23:50:32.6 17.6mag 47P/Ashbrook-Jackson
08:32:20.35 +27:21:23.5 16.9mag 63P/Wild
00:14:55.71 -07:19:07.2 15.7mag 65P/Gunn
06:01:46.96 +31:41:33.0 16.5mag 76P/West-Kohoutek-Ikemura
02:38:04.18 +15:23:49.2 13.9mag 78P/Gehrels
00:51:15.47 +01:49:50.1 15.3mag 88P/Howell
04:12:54.79 +28:57:01.5 15.1mag 93P/Lovas
02:07:31.96 +25:21:41.5 17.9mag 114P/Wiseman-Skiff
06:20:05.73 +33:19:26.1 15.7mag 123P/West-Hartley
09:28:01.83 +20:14:59.8 16.4mag 124P/Mrkos
03:37:40.53 +18:17:34.4 16.4mag 128P/Shoemaker-Holt
04:07:39.61 +18:21:04.5 17.7mag 131P/Mueller
04:58:54.99 +19:38:37.4 13.0mag 141P/Machholz
05:01:33.57 +16:23:18.8 13.0mag 141P-A/Machholz
03:46:45.10 +13:43:43.1 10.6mag 141P-D/Machholz
02:48:13.85 -26:38:47.5 17.3mag 161P/Hartley-IRAS
03:00:02.24 +18:15:08.9 14.9mag 162P/SidingSpring
19:34:45.81 -01:42:03.3 17.6mag 169P/NEAT
17:02:19.22 -09:21:19.2 16.2mag 235P/LINEAR
07:05:08.04 +35:51:50.0 17.3mag 240P/NEAT
23:58:40.04 -07:45:12.5 16.7mag 260P/McNaught
03:30:06.96 +29:55:55.0 17.7mag 295P/LINEAR
22:05:41.32 -27:27:06.9 17.7mag 320P/McNaught
15:21:43.31 +08:21:36.2 17.4mag 391P/Kowalski
07:57:15.08 +21:02:15.9 17.8mag 450P/LONEOS
06:38:49.77 +42:35:03.8 17.8mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.9K May 26 00:38 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
21:27:08.58 +33:24:38.10 AT2026lli 2026-05-19.34 15.86
00:31:01.41 -13:38:51.70 AT2026nad 2026-05-19.39 15.34
15:16:06.61 -79:16:32.40 ASASSN-26dm 2026-05-19.03 14.44
11:24:25.21 -59:23:19.10 ASASSN-26dl 2026-05-18.02 13.55
13:45:51.52 -53:16:01.00 ASASSN-26dk 2026-05-18.16 12.96
02:05:49.69 -30:29:09.60 ASASSN-26dh 2026-05-18.43 15.37
17:50:22.87 -39:42:33.90 ASASSN-26dj 2026-05-17.05 15.7
01:13:11.60 -33:25:16.10 ASASSN-26dg 2026-05-13.41 16.8
16:44:31.77 -27:15:18.40 AT2026mhn 2026-05-12.33 15.8
09:46:31.08 -33:41:51.00 ASASSN-26di 2026-05-12.14 14.63
21:23:11.57 -19:09:45.00 AT2026kwu 2026-05-12.26 16.9
14:20:14.30 -30:20:51.90 AT2026ktm 2026-05-12.06 17.21
14:41:39.01 -37:13:46.40 AT2026lkm 2026-05-11.18 16.89
12:59:50.45 -10:58:38.80 SN2026kep 2026-05-9.06 17.5
13:37:29.61 -29:50:30.90 AT2026lkd 2026-05-9.09 17.23
09:46:42.01 -14:52:03.60 SN2026kmo 2026-05-8.99 17.51
15:03:05.28 +22:02:03.40 AT2026lxf 2026-05-8.07 13.88
10:23:49.41 -20:57:25.30 ASASSN-26df 2026-05-8.21 16.52
22:14:40.56 +05:04:51.60 2026lda 2026-05-7.56 16.2
21:35:33.81 -14:05:16.30 ASASSN-26de 2026-05-6.29 14.51
16:21:49.13 -61:36:14.60 ASASSN-26dd 2026-05-5.15 15.93
14:26:40.22 -24:48:37.50 AT2026lig 2026-05-4.27 14.63
13:17:51.04 +30:25:13.50 SN2026kcp 2026-05-4.46 16.43
11:27:55.57 -13:38:56.90 SN2026kza 2026-05-1.08 15.59
22:28:27.10 +30:17:54.30 SN 2026fov 2026-04-29.6 14.36
21:00:10.71 -32:17:03.90 AT2026kis 2026-04-27.36 16.15
14:32:57.37 -58:13:26.40 ASASSN-26dc 2026-04-27.27 13.42
15:32:05.35 -43:54:34.60 ASASSN-26db 2026-04-27.37 16.06
16:34:34.94 -54:34:58.20 ASASSN-26da 2026-04-25.14 15.99
10:06:55.04 -01:13:49.70 SN2026jsg 2026-04-24.99 16.28
15:15:57.17 +56:18:32.80 SN2026kid 2026-04-24.52 -3.65
07:58:28.45 +57:03:42.40 AT2026kcf 2026-04-24.2 16.89
11:38:21.80 -50:43:06.50 SN2026jkb 2026-04-24.24 15.38
10:06:11.41 -39:41:04.20 AT2026dil 2026-04-24.2 16.85
14:21:40.08 +13:13:46.30 SN2026jlm 2026-04-22.16 15.12
10:53:55.42 -16:06:08.10 ASASSN-26cz 2026-04-22.12 16.24
21:27:08.58 +33:24:38.10 2026-05-19.34 15.86
13:45:02.03 +15:17:14.50 ASASSN-26cy 2026-04-21.27 15.78
13:20:52.22 -35:57:03.60 AT2026jcm 2026-04-19.01 16.65
13:36:15.66 -36:53:48.40 SN 2026iqy 2026-04-18.92 17.31
06:34:01.33 -40:07:34.00 ASASSN-26cx 2026-04-19.07 16.16
23:33:57.97 -45:12:11.90 SN 2026idu 2026-04-19.41 15.9
12:10:50.92 +66:55:31.20 SN 2026icv 2026-04-17.14 16.03
21:36:59.06 -60:43:35.90 ASASSN-26cv 2026-04-17.35 -1.18
08:13:26.26 -27:07:30.50 ASASSN-26cw 2026-04-17.07 -1.01
14:49:14.13 -27:29:20.60 ASASSN-26cu 2026-04-16.06 14.03
17:21:59.44 -38:54:04.60 ASASSN-26ct 2026-04-14.4 15.15
15:25:54.99 +07:49:24.50 SN2026huo 2026-04-12.14 16.96
21:27:08.58 +33:24:38.10 2026-05-19.34 15.86
12:23:20.40 +04:53:39.10 AT2026ixd 2026-04-12.14 17.65
17:46:09.76 -61:19:50.40 SN2026icy 2026-04-12.2 17.03
09:25:46.42 +02:13:46.30 SN2026gud 2026-04-11.98 16.49
16:52:15.46 -60:27:45.90 ASASSN-26cs 2026-04-12.4 15.5
04:20:55.37 -51:15:31.10 ASASSN-26cr 2026-04-12.01 15.37
22:25:39.35 +36:45:06.90 AT2026ihl 2026-04-10.48 14.21
19:40:44.94 +00:41:03.80 AT2026imw 2026-04-10.32 16.06
19:52:04.70 +05:53:33.50 ASASSN-26cq 2026-04-9.31 14.98
16:08:18.39 -64:11:08.80 ASASSN-26cp 2026-04-9.14 13.64
09:22:22.90 -61:02:43.70 SN2026idh 2026-04-7.97 16.34
05:06:54.12 -19:42:26.40 AT2026imr 2026-04-8 17.49
07:14:55.34 -36:03:21.40 AT2026hei 2026-04-8.12 16.7
21:35:33.14 -19:01:34.80 AT2026ihm 2026-04-8.36 16.7
04:28:24.08 -32:25:35.30 AT2026imo 2026-04-8.02 16.81
05:10:35.79 -39:38:40.80 SN 2026hnn 2026-04-7.04 17.07
09:54:32.04 -01:17:25.80 ASASSN-26cn 2026-04-7.01 15.58
07:46:24.43 -77:29:36.30 ASASSN-26co 2026-04-7.15 15.11
05:00:45.52 -29:51:06.20 AT2026hvw 2026-04-6.03 16.51
19:49:33.10 -23:37:11.00 ASASSN-26cl 2026-04-5.29 14.98
19:32:43.55 -22:39:33.40 ASASSN-26cm 2026-04-4.3 13.88
18:08:57.38 +76:48:23.60 ASASSN-26ck 2026-04-2.37 15.38
16:16:36.10 +44:52:30.20 AT2026hyy 2026-04-2.58 13.81
21:55:23.31 -34:48:53.90 ASASSN-26cj 2026-03-30.4 -1.47
11:19:50.81 -27:51:50.40 SN2026gvk 2026-03-30 15.28
11:53:57.02 -23:09:46.20 SN2026gzx 2026-03-28.75 15.27
07:13:46.14 -33:10:15.70 ASASSN-26ci 2026-03-28.15 15.14
09:03:36.09 -67:58:13.00 SN2026hkg 2026-03-28.19 15.82
07:03:00.72 +39:14:43.00 SN2026fin 2026-03-28.27 15.82
05:35:42.79 -63:44:05.60 ASASSN-26ch 2026-03-28.12 13.14
11:23:19.04 +34:22:38.00 SN2026fwt 2026-03-27.3 16.56
19:03:49.79 +37:04:05.20 ASASSN-26ce 2026-03-26.56 16.3
20:26:56.07 -52:54:06.50 AT2026hiy 2026-03-26.35 16.95
05:25:54.76 -30:15:35.80 ASASSN-26cg 2026-03-25.07 16.88
06:57:16.49 -26:54:37.20 SN2026fzb 2026-03-25.14 15.8
14:37:38.23 -43:00:52.30 ASASSN-26cd 2026-03-24.24 12.52
17:34:53.03 +06:04:29.70 AT2026gzl 2026-03-23.27 15.82
08:30:02.60 -35:12:47.50 ASASSN-26cf 2026-03-23.2 14.82
16:54:25.33 +37:49:56.60 SN 2026evz 2026-03-21.32 17.54
17:06:19.20 -18:54:19.50 ASASSN-26bx 2026-03-21.25 16.39
19:01:16.28 -29:29:23.10 ASASSN-26bw 2026-03-21.33 15.81
08:46:05.75 +10:47:39.80 ASASSN-26ca 2026-03-21.13 14.27
12:14:58.16 +63:47:16.20 SN 2026fvx 2026-03-21.12 15.6
18:02:55.90 -75:23:02.60 ASASSN-26bz 2026-03-21.32 16.16
12:16:02.88 -53:16:33.80 ASASSN-26cc 2026-03-20.04 15.48
13:08:21.85 +29:13:44.20 SN 2026fmh 2026-03-20.16 -0.33
19:56:38.48 -34:45:21.50 ASASSN-26cb 2026-03-20.35 -3.26
14:32:41.15 -41:38:48.50 ASASSN-26by 2026-03-20.15 -1.31
13:00:42.99 +37:18:34.60 SN2026fjc 2026-03-19.5 15.97
06:02:44.21 -04:11:06.20 ASASSN-26bv 2026-03-19.19 15.67
12:20:27.96 -45:55:38.40 ASASSN-26bt 2026-03-18.8 16.32
07:49:57.30 -56:14:35.10 ASASSN-26bu 2026-03-19.19 15.74
-rw-r--r-- 1 apache apache 5.6K May 26 00:38 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
07:03:25.76 -12:41:40.1 TCP J07032576-1241401 2026-03-10.4268 15.4mag
00:42:36.82 +41:16:05.8 PNV J00423682+4116058 2026-03-12.5744 17.24Cmag
07:26:45.79 -27:45:14.1 TCP J07264579-2745141 2026-03-17.4417 14.8mag
17:57:19.56 -28:08:14.7 TCP J17571956-2808147 2026-03-19.7972 14.5mag
08:46:05.73 +10:47:39.7 TCP J08460573+1047397 2026-03-21.1936 14.5mag
09:55:38.83 +69:05:21.7 PNV J09553883+6905217 2026-04-01.893 19.4mag
19:32:43.67 -22:39:30.7 TCP J19324367-2239307 2026-04-05.4395 13.6mag
16:16:36.03 +44:52:28.9 TCP J16163603+4452289 2026-04-05.6655 14.2mag
00:43:38.36 +41:15:32.4 PNV J00433836+4115324 2026-04-08.079 17.2mag
15:41:11.68 +59:18:26.8 TCP J15411168+5918268 2026-04-12.9625 19.2mag
00:43:35.02 +41:46:28.0 PNV J00433502+4146280 2026-04-23.056 15.9mag
00:42:55.64 +41:14:12.2 PNV J00425564+4114122 2026-04-24.042 16.2mag
21:14:03.38 +56:46:44.1 TCP J21140338+5646441 2026-05-05.3534 16.7mag
15:03:05.19 +22:02:04.1 TCP J15030519+2202041 2026-05-08.3260 13.9mag
07:15:18.25 +47:53:16.7 TCP J07151825+4753167 2026-05-09.1599 14.4mag
16:00:18.44 -22:30:10.6 TCP J16001844-2230106 2026-05-09.6135 13.3mag
00:42:47.45 +41:16:58.5 PNV J00424745+4116585 2026-05-10.030 16.8mag
09:55:02.89 +69:02:13.8 PNV J09550289+6902138 2026-05-18.925 20.7mag
00:43:01.82 +41:18:16.6 PNV J00430182+4118166 2026-05-21.8651 18.83Cmag
00:42:51.20 +41:16:59.4 PNV J00425120+4116594 2022-10-26.135 19.3mag
-rw-r--r-- 1 apache apache 188K May 26 00:38 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
10:00:42.117 +02:58:53.47 AT 2026myy 2026-05-12.00 23.51
23:08:43.405 -02:58:43.07 AT 2026myx 2026-05-17.39 19.223
06:45:38.272 -34:46:50.78 AT 2026myw 2026-05-17.97 19.366
22:51:00.147 -40:59:30.34 AT 2026myv 2026-05-04.40 19.85
23:01:42.557 -37:41:28.08 AT 2026myu 2026-05-14.36 20.03
17:40:41.796 +55:46:35.59 AT 2026myt 2026-05-13.08 19.76
11:57:21.623 +08:17:50.60 AT 2026mys 2026-05-17.92 20.12
18:08:09.175 +24:46:16.68 AT 2026myr 2026-05-16.11 19.59
19:44:08.720 +05:58:44.85 AT 2026myq 2026-05-18.09 19.96
22:15:03.694 +37:18:03.97 SN 2026myp 2026-05-17.58 17.878
13:28:54.990 -05:49:13.50 AT 2026myo 2026-05-17.76 18.69
13:35:39.060 +60:25:07.59 AT 2026myn 2026-05-17.79 18.94
15:11:37.375 +27:04:22.10 AT 2026mym 2026-05-17.80 19.01
15:45:32.128 +08:10:41.12 AT 2026myl 2026-05-17.84 19.27
16:38:47.743 +40:50:56.52 AT 2026myk 2026-05-17.88 18.14
13:21:16.033 -33:01:10.62 AT 2026myj 2026-05-10.44 20.34
14:04:07.440 +19:21:36.43 AT 2026myi 2026-05-16.96 20.28
12:09:08.262 +13:15:11.92 AT 2026myh 2026-05-05.92 20.33
17:37:21.286 +36:24:32.57 AT 2026myg 2026-05-12.55 19.89
14:40:52.425 +10:22:25.10 AT 2026myf 2026-05-14.32 20.45
-rw-r--r-- 1 apache apache 30K May 26 00:38 tns_transients_list.txt
