This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q2b1x1_214021_TTUQ2b1x1_3174574_KviWPu4r
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
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
RR Mon,2461158.6102,10.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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
RR Mon 20260428.1102 10.42CV 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 04 28.1102 2461158.6102 12.61 06:53:17.60 -00:15:30.1
213.37337 0.29501 galactic Mon Second-epoch detections are separated by 0.5" and 5.1 pix
The object was found in VSX 2" Gaia DR3 3113280716087249280
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.660 G 13.680 G A
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:53:17.60 -00:15:30.1: 14.18 +/- 0.25 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:53:17.60 -00:15:30.1: 15.58 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.18 +/- 0.25
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 3113280716087249280,2461158.6102,12.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 3113280716087249280 20260428.1102 12.61CV 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 04 28.1102 2461158.6102 12.62 06:54:34.04 +00:38:32.7
212.71686 0.98919 galactic Mon Second-epoch detections are separated by 0.3" and 5.1 pix
The object was found in VSX 3" Gaia DR3 3113768246414193152
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.730 G 13.750 G F
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:54:34.04 +00:38:32.7: 14.81 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:54:34.04 +00:38:32.7: 13.64 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.64 +/- 0.06
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 3113768246414193152,2461158.6102,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 3113768246414193152 20260428.1102 12.62CV 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 04 28.1102 2461158.6102 12.61 07:07:02.35 -01:54:21.4
216.40970 2.59860 galactic Mon Second-epoch detections are separated by 2.7" and 4.6 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 | ATO J106.7592-01.9064 | 07:07:02.35 -01:54:21.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.279+/-0.033 (F)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:07:02.35 -01:54:21.4: 14.39 +/- 0.24 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:07:02.35 -01:54:21.4: 15.45 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.39 +/- 0.24
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
ATO J106.7592-01.9064,2461158.6102,12.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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
ATO J106.7592-01.9064 20260428.1102 12.61CV 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 04 28.1102 2461158.6102 12.51 06:59:38.67 -06:13:05.3
219.39968 -1.01505 galactic Mon Second-epoch detections are separated by 0.6" and 5.2 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 | target | 06:59:38.67 -06:13:05.3 (user input) | T | P | (position from user input) J-Ks=0.426+/-0.035 (G)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:59:38.67 -06:13:05.3: 14.65 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:59:38.67 -06:13:05.3: 15.33 +/- 99.00 upperlimit
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
target,2461158.6102,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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
target 20260428.1102 12.51CV 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 04 28.1102 2461158.6102 12.57 07:05:38.90 -00:02:17.6
214.58755 3.14390 galactic Mon Second-epoch detections are separated by 0.5" and 5.1 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 | ATO J106.4031-00.0467 | 07:05:36.76 -00:02:48.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:05:38.90 -00:02:17.6: 14.79 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:05:38.90 -00:02:17.6: 15.53 +/- 99.00 upperlimit
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
ATO J106.4031-00.0467,2461158.6102,12.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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
ATO J106.4031-00.0467 20260428.1102 12.57CV 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 04 28.1102 2461158.6102 12.54 07:02:50.58 -03:19:44.0
217.19493 1.01526 galactic Mon Second-epoch detections are separated by 4.0" and 4.5 pix
The object was found in VSX 2" Gaia DR3 3108620917091030272
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.750 G 13.790 G A
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:02:50.58 -03:19:44.0: 13.26 +/- 0.10 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:02:50.58 -03:19:44.0: 15.50 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.26 +/- 0.10
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 3108620917091030272,2461158.6102,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 3108620917091030272 20260428.1102 12.54CV 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 04 28.1102 2461158.6102 12.38 07:01:32.59 -06:05:38.0
219.50496 -0.53853 galactic Mon Second-epoch detections are separated by 1.0" and 5.2 pix
The object was found in VSX13" Gaia DR3 3052875059089742464
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.080 G 13.100 G A
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:01:32.59 -06:05:38.0: 14.72 +/- 0.34 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:01:32.59 -06:05:38.0: 15.49 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.72 +/- 0.34
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 3052875059089742464,2461158.6102,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 3052875059089742464 20260428.1102 12.38CV 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 04 28.1102 2461158.6102 12.51 06:57:30.18 -00:57:12.2
214.47198 0.91445 galactic Mon Second-epoch detections are separated by 0.7" and 5.0 pix
The object was found in VSX 3" Gaia DR3 3112232984583836928
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.550 G 13.580 G A
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:57:30.18 -00:57:12.2: 14.72 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:57:30.18 -00:57:12.2: 15.60 +/- 99.00 upperlimit
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 3112232984583836928,2461158.6102,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 3112232984583836928 20260428.1102 12.51CV 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 04 28.1102 2461158.6102 12.40 07:15:54.37 -00:50:16.3
216.47732 5.05772 galactic Mon Second-epoch detections are separated by 1.1" and 4.9 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 | ATO J108.9768-00.8393 | 07:15:54.37 -00:50:16.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:15:54.37 -00:50:16.3: 14.61 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:15:54.37 -00:50:16.3: 15.34 +/- 99.00 upperlimit
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
ATO J108.9768-00.8393,2461158.6102,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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
ATO J108.9768-00.8393 20260428.1102 12.40CV 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 04 28.1102 2461158.6102 12.47 07:08:29.29 -00:58:29.1
215.74691 3.34704 galactic Mon Second-epoch detections are separated by 0.4" and 5.1 pix
The object was found in VSX 2" Gaia DR3 3109604288498805632
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.490 G 13.520 G A
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:08:29.29 -00:58:29.1: 14.71 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:08:29.29 -00:58:29.1: 15.38 +/- 99.00 upperlimit
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 3109604288498805632,2461158.6102,12.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 3109604288498805632 20260428.1102 12.47CV 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 04 28.1102 2461158.6102 12.43 06:53:42.65 -01:01:11.3
214.09862 0.04064 galactic Mon Second-epoch detections are separated by 1.8" and 5.2 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 | ATO J103.4228-01.0262 | 06:53:42.65 -01:01:11.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.298+/-0.036 (F)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:53:42.65 -01:01:11.3: 13.63 +/- 0.11 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:53:42.65 -01:01:11.3: 14.02 +/- 0.10 detection
Forced photometry reference-image weighted average: 13.85 +/- 0.08
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
ATO J103.4228-01.0262,2461158.6102,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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
ATO J103.4228-01.0262 20260428.1102 12.43CV 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 04 28.1102 2461158.6102 12.43 06:52:19.69 -00:56:12.2
213.86707 -0.22906 galactic Mon Second-epoch detections are separated by 0.9" and 5.1 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 3112396674377838464 | 06:52:18.55 -00:56:05.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:52:19.69 -00:56:12.2: 14.88 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:52:19.69 -00:56:12.2: 15.44 +/- 99.00 upperlimit
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 3112396674377838464,2461158.6102,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 3112396674377838464 20260428.1102 12.43CV 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 04 28.1102 2461158.6102 12.46 07:17:34.01 -02:54:22.2
218.51137 4.47350 galactic Mon Second-epoch detections are separated by 1.5" and 4.8 pix
The object was found in VSX11" Gaia DR3 3060152756607968512
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.390 G 13.460 G 0.044995900000 F
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:17:34.01 -02:54:22.2: 14.45 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:17:34.01 -02:54:22.2: 15.25 +/- 99.00 upperlimit
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 3060152756607968512,2461158.6102,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 3060152756607968512 20260428.1102 12.46CV 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 04 28.1102 2461158.6102 12.40 07:09:58.06 +00:39:41.8
214.45771 4.42412 galactic Mon Second-epoch detections are separated by 2.4" and 4.8 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 | target | 07:09:58.06 +00:39:41.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:09:58.06 +00:39:41.8: 14.64 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:09:58.06 +00:39:41.8: 15.41 +/- 99.00 upperlimit
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
target,2461158.6102,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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
target 20260428.1102 12.40CV 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 04 28.1102 2461158.6102 12.19 07:12:19.90 -01:08:21.3
216.33462 4.12556 galactic Mon Second-epoch detections are separated by 4.1" and 4.6 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 3109364290029458048 | 07:12:19.71 -01:09:07.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:12:19.90 -01:08:21.3: 14.54 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:12:19.90 -01:08:21.3: 15.39 +/- 99.00 upperlimit
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 3109364290029458048,2461158.6102,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 3109364290029458048 20260428.1102 12.19CV 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 04 28.1102 2461158.6102 12.16 07:03:26.97 -05:01:13.1
218.76782 0.37482 galactic Mon Second-epoch detections are separated by 0.4" and 5.1 pix
The object was found in VSX 2" Gaia DR3 3101503056772630528
Type: VAR
# Max. Min./Amp. JD0 Period
13.310 G 13.350 G 0.024475800000 B
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:03:26.97 -05:01:13.1: 14.42 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:03:26.97 -05:01:13.1: 15.11 +/- 99.00 upperlimit
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 3101503056772630528,2461158.6102,12.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 3101503056772630528 20260428.1102 12.16CV 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 04 28.1102 2461158.6102 12.11 07:08:41.84 +01:18:41.1
213.73243 4.43790 galactic CMi Second-epoch detections are separated by 5.8" and 5.9 pix
The object was found in VSX10" Gaia DR3 3114481210983029120
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.300 G 13.330 G A
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:08:41.84 +01:18:41.1: 14.74 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:08:41.84 +01:18:41.1: 15.46 +/- 99.00 upperlimit
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 3114481210983029120,2461158.6102,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 3114481210983029120 20260428.1102 12.11CV 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 04 28.1102 2461158.6102 12.05 07:07:21.18 -03:23:33.2
217.76775 1.98636 galactic Mon Second-epoch detections are separated by 0.3" and 5.1 pix
The object was found in VSX 5" Gaia DR3 3107912900321471104
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.240 G 13.280 G F
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:07:21.18 -03:23:33.2: 14.66 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:07:21.18 -03:23:33.2: 15.37 +/- 99.00 upperlimit
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 3107912900321471104,2461158.6102,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 3107912900321471104 20260428.1102 12.05CV 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 04 28.1102 2461158.6102 12.16 07:03:14.57 +01:07:05.2
213.28226 3.13627 galactic Mon Second-epoch detections are separated by 0.9" and 5.2 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 | ATO J105.8095+01.1236 | 07:03:14.29 +01:07:25.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:03:14.57 +01:07:05.2: 14.71 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:03:14.57 +01:07:05.2: 15.52 +/- 99.00 upperlimit
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
ATO J105.8095+01.1236,2461158.6102,12.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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
ATO J105.8095+01.1236 20260428.1102 12.16CV 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 04 28.1102 2461158.6102 12.12 07:00:46.45 -03:36:06.5
217.20134 0.43133 galactic Mon Second-epoch detections are separated by 0.7" and 5.1 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 | ATO J105.1923-03.6065 | 07:00:46.45 -03:36:06.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.236+/-0.036 (F)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:00:46.45 -03:36:06.5: 14.79 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:00:46.45 -03:36:06.5: 15.47 +/- 99.00 upperlimit
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
ATO J105.1923-03.6065,2461158.6102,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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
ATO J105.1923-03.6065 20260428.1102 12.12CV 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 04 28.1102 2461158.6102 12.04 07:18:18.12 -00:24:27.2
216.36952 5.78735 galactic Mon Second-epoch detections are separated by 2.5" and 5.0 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 | ATO J109.5734-00.4114 | 07:18:18.12 -00:24:27.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: A1IV (LAMOST DR5)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:18:18.12 -00:24:27.2: 14.02 +/- 0.25 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:18:18.12 -00:24:27.2: 15.35 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.02 +/- 0.25
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
ATO J109.5734-00.4114,2461158.6102,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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
ATO J109.5734-00.4114 20260428.1102 12.04CV 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 04 28.1102 2461158.6102 12.06 07:12:26.22 +01:50:33.8
213.68493 5.51189 galactic CMi Second-epoch detections are separated by 1.3" and 4.9 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 | target | 07:12:26.22 +01:50:33.8 (user input) | T | P | (position from user input) J-Ks=0.174+/-0.031 (F)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:12:26.22 +01:50:33.8: 14.67 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:12:26.22 +01:50:33.8: 15.39 +/- 99.00 upperlimit
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
target,2461158.6102,12.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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
target 20260428.1102 12.06CV 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 04 28.1102 2461158.6102 12.11 07:06:40.09 -04:34:47.3
218.74435 1.28939 galactic Mon Second-epoch detections are separated by 2.6" and 5.4 pix
The object was found in VSX 7" Gaia DR3 3107502473248673280
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.410 G 13.430 G F
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:06:40.09 -04:34:47.3: 14.79 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:06:40.09 -04:34:47.3: 15.54 +/- 99.00 upperlimit
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 3107502473248673280,2461158.6102,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 3107502473248673280 20260428.1102 12.11CV 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 04 28.1102 2461158.6102 11.81 06:59:39.73 -00:40:08.0
214.46520 1.52454 galactic Mon Second-epoch detections are separated by 2.1" and 5.0 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 | target | 06:59:39.73 -00:40:08.0 (user input) | T | P | (position from user input) J-Ks=0.213+/-0.053 (F)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:59:39.73 -00:40:08.0: 14.79 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:59:39.73 -00:40:08.0: 15.61 +/- 99.00 upperlimit
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
target,2461158.6102,11.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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
target 20260428.1102 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 04 28.1102 2461158.6102 11.73 07:05:36.21 -00:02:35.6
214.58688 3.13164 galactic Mon Second-epoch detections are separated by 3.0" and 5.1 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 | ATO J106.4031-00.0467 | 07:05:36.76 -00:02:48.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.017+/-0.035 (A)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:05:36.21 -00:02:35.6: 14.82 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:05:36.21 -00:02:35.6: 15.53 +/- 99.00 upperlimit
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
ATO J106.4031-00.0467,2461158.6102,11.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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
ATO J106.4031-00.0467 20260428.1102 11.73CV 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 04 28.1102 2461158.6102 11.62 07:02:00.79 +01:40:10.1
212.65050 3.11380 galactic Mon Second-epoch detections are separated by 1.5" and 4.9 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 3115398203683281280 | 07:01:59.61 +01:40:25.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:02:00.79 +01:40:10.1: 14.78 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:02:00.79 +01:40:10.1: 15.38 +/- 99.00 upperlimit
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 3115398203683281280,2461158.6102,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 3115398203683281280 20260428.1102 11.62CV 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 04 28.1102 2461158.6102 11.78 07:08:09.49 -00:32:01.7
215.31633 3.47547 galactic Mon Second-epoch detections are separated by 1.4" and 4.8 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 3109654659875228288 | 07:08:10.43 -00:32:21.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.692+/-0.029 (K)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:08:09.49 -00:32:01.7: 14.71 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:08:09.49 -00:32:01.7: 15.50 +/- 99.00 upperlimit
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 3109654659875228288,2461158.6102,11.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 3109654659875228288 20260428.1102 11.78CV 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 04 28.1102 2461158.6102 11.39 07:04:20.91 -04:41:02.2
218.57155 0.72805 galactic Mon Second-epoch detections are separated by 0.4" and 5.0 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 3101541986356735360 | 07:04:20.78 -04:41:23.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.342+/-0.031 (G)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:04:20.91 -04:41:02.2: 14.52 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:04:20.91 -04:41:02.2: 15.21 +/- 99.00 upperlimit
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 3101541986356735360,2461158.6102,11.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 3101541986356735360 20260428.1102 11.39CV 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 04 28.1102 2461158.6102 11.30 07:11:00.60 -02:53:39.1
217.74457 3.02615 galactic Mon Second-epoch detections are separated by 0.4" and 5.0 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 | ATO J107.7472-02.9052 | 07:11:00.72 -02:54:01.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F2 1949AnHar.112....1C HD 296558 J-Ks=0.245+/-0.030 (F)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:11:00.60 -02:53:39.1: 14.58 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:11:00.60 -02:53:39.1: 15.35 +/- 99.00 upperlimit
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
ATO J107.7472-02.9052,2461158.6102,11.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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
ATO J107.7472-02.9052 20260428.1102 11.30CV 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 04 28.1102 2461158.6102 10.98 07:08:43.97 -03:56:11.5
218.40947 2.04220 galactic Mon Second-epoch detections are separated by 2.3" and 5.0 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 | ATO J107.1828-03.9366 | 07:08:44.38 -03:55:56.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.613+/-0.038 (K)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:08:43.97 -03:56:11.5: 12.67 +/- 0.05 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:08:43.97 -03:56:11.5: 15.36 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 12.67 +/- 0.05
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
ATO J107.1828-03.9366,2461158.6102,10.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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
ATO J107.1828-03.9366 20260428.1102 10.98CV 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 04 28.1102 2461158.6102 10.64 07:14:38.84 -03:56:24.7
219.09327 3.34968 galactic Mon Second-epoch detections are separated by 1.0" and 5.0 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 | ATO J108.6673-03.9395 | 07:14:38.63 -03:56:02.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: B8 1949AnHar.112....1C HD 296712 J-Ks=0.114+/-0.035 (A)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:14:38.84 -03:56:24.7: 14.44 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:14:38.84 -03:56:24.7: 15.26 +/- 99.00 upperlimit
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
ATO J108.6673-03.9395,2461158.6102,10.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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
ATO J108.6673-03.9395 20260428.1102 10.64CV 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 04 28.1102 2461158.6102 11.48 07:05:30.70 +01:36:35.8
213.10237 3.86511 galactic Mon Second-epoch detections are separated by 1.0" and 5.0 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 3114643388949636736 | 07:05:31.92 +01:36:15.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A2 1949AnHar.112....1C HD 289625 J-Ks=0.365+/-0.030 (G)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:05:30.70 +01:36:35.8: 13.97 +/- 0.18 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:05:30.70 +01:36:35.8: 15.38 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.97 +/- 0.18
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 3114643388949636736,2461158.6102,11.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 3114643388949636736 20260428.1102 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 04 28.1102 2461158.6102 11.71 07:06:24.21 +00:20:27.4
214.33599 3.48498 galactic Mon Second-epoch detections are separated by 0.7" and 5.0 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 3114263159786050944 | 07:06:23.17 +00:20:49.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A 1949AnHar.112....1C HD 293175 J-Ks=0.194+/-0.035 (F)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:06:24.21 +00:20:27.4: 14.83 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:06:24.21 +00:20:27.4: 14.02 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.02 +/- 0.09
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 3114263159786050944,2461158.6102,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 3114263159786050944 20260428.1102 11.71CV 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 04 28.1102 2461158.6102 11.78 07:12:29.97 +00:35:38.2
214.80810 4.95630 galactic Mon Second-epoch detections are separated by 1.5" and 5.2 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 | target | 07:12:29.97 +00:35:38.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:12:29.97 +00:35:38.2: 14.61 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:12:29.97 +00:35:38.2: 15.28 +/- 99.00 upperlimit
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
target,2461158.6102,11.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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
target 20260428.1102 11.78CV 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 04 28.1102 2461158.6102 11.94 07:01:38.62 -04:40:49.7
218.25969 0.13058 galactic Mon Second-epoch detections are separated by 0.9" and 4.9 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 3101715086411523584 | 07:01:37.75 -04:41:16.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 1949AnHar.112....1C HD 296156 J-Ks=0.190+/-0.034 (F)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:01:38.62 -04:40:49.7: 14.82 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:01:38.62 -04:40:49.7: 15.49 +/- 99.00 upperlimit
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 3101715086411523584,2461158.6102,11.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 3101715086411523584 20260428.1102 11.94CV 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 04 28.1102 2461158.6102 12.01 07:12:18.81 +00:29:05.7
214.88412 4.86512 galactic Mon Second-epoch detections are separated by 2.0" and 5.3 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 | ATO J108.0888+00.4781 | 07:12:18.81 +00:29:05.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.783+/-0.033 (K)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:12:18.81 +00:29:05.7: 14.64 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:12:18.81 +00:29:05.7: 15.49 +/- 99.00 upperlimit
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
ATO J108.0888+00.4781,2461158.6102,12.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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
ATO J108.0888+00.4781 20260428.1102 12.01CV 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 04 28.1102 2461158.6102 12.01 07:01:07.55 -03:14:33.5
216.92207 0.67365 galactic Mon Second-epoch detections are separated by 1.6" and 5.1 pix
The object was found in VSX 3" Gaia DR3 3108634145589904768
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.120 G 13.150 G A
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:01:07.55 -03:14:33.5: 14.76 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:01:07.55 -03:14:33.5: 15.50 +/- 99.00 upperlimit
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 3108634145589904768,2461158.6102,12.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 3108634145589904768 20260428.1102 12.01CV 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 04 28.1102 2461158.6102 12.07 07:01:22.92 -06:08:22.5
219.52726 -0.59506 galactic Mon Second-epoch detections are separated by 3.0" and 4.7 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 | target | 07:01:22.92 -06:08:22.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:01:22.92 -06:08:22.5: 14.61 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:01:22.92 -06:08:22.5: 15.38 +/- 99.00 upperlimit
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
target,2461158.6102,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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
target 20260428.1102 12.07CV 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 04 28.1102 2461158.6102 12.06 07:00:56.90 -03:16:18.9
216.92785 0.62086 galactic Mon Second-epoch detections are separated by 0.7" and 4.9 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 | target | 07:00:56.90 -03:16:18.9 (user input) | T | P | (position from user input) J-Ks=0.308+/-0.036 (F)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:00:56.90 -03:16:18.9: 14.87 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:00:56.90 -03:16:18.9: 15.48 +/- 99.00 upperlimit
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
target,2461158.6102,12.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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
target 20260428.1102 12.06CV 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 04 28.1102 2461158.6102 12.05 07:15:49.67 -00:37:03.1
216.27177 5.14145 galactic Mon Second-epoch detections are separated by 2.1" and 4.8 pix
The object was found in VSX16" Gaia DR3 3110157583366513664
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
14.020 G 14.070 G A
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:15:49.67 -00:37:03.1: 14.60 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:15:49.67 -00:37:03.1: 15.25 +/- 99.00 upperlimit
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 3110157583366513664,2461158.6102,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 3110157583366513664 20260428.1102 12.05CV 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 04 28.1102 2461158.6102 12.25 06:52:57.41 -03:04:55.9
215.84837 -1.06735 galactic Mon Second-epoch detections are separated by 1.7" and 4.6 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 | target | 06:52:57.41 -03:04:55.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:52:57.41 -03:04:55.9: 14.79 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:52:57.41 -03:04:55.9: 15.45 +/- 99.00 upperlimit
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
target,2461158.6102,12.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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
target 20260428.1102 12.25CV 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 04 28.1102 2461158.6102 12.26 07:01:46.25 +01:19:49.1
212.92525 2.90543 galactic Mon Second-epoch detections are separated by 1.9" and 5.2 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 3115367176839807872 | 07:01:47.56 +01:19:29.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:01:46.25 +01:19:49.1: 14.06 +/- 0.18 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:01:46.25 +01:19:49.1: 14.96 +/- 0.23 detection
Forced photometry reference-image weighted average: 14.40 +/- 0.14
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 3115367176839807872,2461158.6102,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 3115367176839807872 20260428.1102 12.26CV 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 04 28.1102 2461158.6102 12.32 07:17:13.16 -01:33:02.6
217.26432 5.02151 galactic Mon Second-epoch detections are separated by 1.3" and 4.9 pix
The object was found in VSX 2" Gaia DR3 3109840442983964928
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.370 G 13.390 G F
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:17:13.16 -01:33:02.6: 14.57 +/- 0.33 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:17:13.16 -01:33:02.6: 15.18 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.57 +/- 0.33
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 3109840442983964928,2461158.6102,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 3109840442983964928 20260428.1102 12.32CV 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 04 28.1102 2461158.6102 12.11 07:07:11.92 -02:58:18.0
217.37588 2.14532 galactic Mon Second-epoch detections are separated by 0.8" and 5.2 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 | ATO J106.7973-02.9618 | 07:07:11.92 -02:58:18.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:07:11.92 -02:58:18.0: 14.77 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:07:11.92 -02:58:18.0: 15.45 +/- 99.00 upperlimit
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
ATO J106.7973-02.9618,2461158.6102,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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
ATO J106.7973-02.9618 20260428.1102 12.11CV 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 04 28.1102 2461158.6102 12.19 06:39:44.39 +00:57:26.2
210.74513 -2.16533 galactic Mon Second-epoch detections are separated by 4.3" and 5.8 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 | target | 06:39:44.39 +00:57:26.2 (user input) | T | P | (position from user input) SpType: K4III 2012A&A...543A.125G CoRoT 102542687
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:39:44.39 +00:57:26.2: 14.71 +/- 0.36 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:39:44.39 +00:57:26.2: 13.01 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.03 +/- 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
target,2461158.6102,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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
target 20260428.1102 12.19CV 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 04 28.1102 2461158.6102 12.16 06:47:25.92 -01:17:25.0
213.62388 -1.47950 galactic Mon Second-epoch detections are separated by 2.0" and 4.6 pix
The object was found in VSX 1" Gaia DR3 3107094447052075136
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.200 G 13.220 G F
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:47:25.92 -01:17:25.0: 14.68 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:47:25.92 -01:17:25.0: 12.94 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.94 +/- 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
Gaia DR3 3107094447052075136,2461158.6102,12.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 3107094447052075136 20260428.1102 12.16CV 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 04 28.1102 2461158.6102 12.29 06:53:58.09 -04:52:51.4
217.56503 -1.66226 galactic Mon Second-epoch detections are separated by 1.9" and 5.3 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 | ATO J103.4899-04.8802 | 06:53:58.09 -04:52:51.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G7IIIa 2012A&A...543A.125G CoRoT 110696033
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:53:58.09 -04:52:51.4: 14.58 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:53:58.09 -04:52:51.4: 15.29 +/- 99.00 upperlimit
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
ATO J103.4899-04.8802,2461158.6102,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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
ATO J103.4899-04.8802 20260428.1102 12.29CV 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 04 28.1102 2461158.6102 12.22 06:45:04.84 -01:02:23.6
213.13298 -1.88854 galactic Mon Second-epoch detections are separated by 0.5" and 5.0 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 | ATO J101.2775-01.0440 | 06:45:04.84 -01:02:23.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G2.5IVa 2012A&A...543A.125G CoRoT 102763453 J-Ks=0.342+/-0.037 (G)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:45:04.84 -01:02:23.6: 14.16 +/- 0.21 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:45:04.84 -01:02:23.6: 13.12 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.16 +/- 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
ATO J101.2775-01.0440,2461158.6102,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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
ATO J101.2775-01.0440 20260428.1102 12.22CV 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 04 28.1102 2461158.6102 12.33 06:57:00.80 +00:17:37.4
213.30612 1.37444 galactic Mon Second-epoch detections are separated by 1.5" and 4.8 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 3113688634901420928 | 06:57:00.01 +00:18:03.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A0 1949AnHar.112....1C HD 292824
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:57:00.80 +00:17:37.4: 14.93 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:57:00.80 +00:17:37.4: 15.64 +/- 99.00 upperlimit
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 3113688634901420928,2461158.6102,12.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 3113688634901420928 20260428.1102 12.33CV 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 04 28.1102 2461158.6102 12.40 06:59:40.33 -00:39:47.7
214.46132 1.52933 galactic Mon Second-epoch detections are separated by 3.2" 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 3112640181842895232 | 06:59:40.85 -00:39:03.3 (Gaia DR3) | DSCT/GDOR (local) | (local) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:59:40.33 -00:39:47.7: 14.83 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:59:40.33 -00:39:47.7: 15.61 +/- 99.00 upperlimit
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 3112640181842895232,2461158.6102,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 3112640181842895232 20260428.1102 12.40CV 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 04 28.1102 2461158.6102 12.32 07:07:58.84 -00:56:39.7
215.66168 3.24816 galactic Mon Second-epoch detections are separated by 3.2" and 4.5 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 | target | 07:07:58.84 -00:56:39.7 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:07:58.84 -00:56:39.7: 14.71 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:07:58.84 -00:56:39.7: 14.11 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.11 +/- 0.11
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
target,2461158.6102,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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
target 20260428.1102 12.32CV 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 04 28.1102 2461158.6102 12.32 07:02:02.17 +00:07:45.9
214.02550 2.41696 galactic Mon Second-epoch detections are separated by 0.8" and 5.0 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 | ATO J105.5011+00.1277 | 07:02:01.39 +00:08:10.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A2 1949AnHar.112....1C HD 293049
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:02:02.17 +00:07:45.9: 14.89 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:02:02.17 +00:07:45.9: 15.61 +/- 99.00 upperlimit
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
ATO J105.5011+00.1277,2461158.6102,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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
ATO J105.5011+00.1277 20260428.1102 12.32CV 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 04 28.1102 2461158.6102 12.30 06:49:33.29 -01:23:30.4
213.95609 -1.05348 galactic Mon Second-epoch detections are separated by 1.0" and 5.0 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 | ATO J102.3878-01.3922 | 06:49:33.29 -01:23:30.4 (user input) | IRR (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:49:33.29 -01:23:30.4: 14.08 +/- 0.18 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:49:33.29 -01:23:30.4: 13.49 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.54 +/- 0.05
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
ATO J102.3878-01.3922,2461158.6102,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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
ATO J102.3878-01.3922 20260428.1102 12.30CV 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 04 28.1102 2461158.6102 12.30 06:59:52.91 -04:47:27.8
218.15724 -0.31034 galactic Mon Second-epoch detections are separated by 1.6" and 4.8 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 3101628912187905408 | 06:59:54.00 -04:47:58.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A0 1949AnHar.112....1C HD 296012 J-Ks=0.443+/-0.035 (G)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:59:52.91 -04:47:27.8: 14.44 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:59:52.91 -04:47:27.8: 15.10 +/- 0.30 detection
Forced photometry reference-image weighted average: 15.10 +/- 0.30
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 3101628912187905408,2461158.6102,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 3101628912187905408 20260428.1102 12.30CV 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 04 28.1102 2461158.6102 12.15 07:01:01.02 -00:25:44.7
214.40642 1.93535 galactic Mon Second-epoch detections are separated by 2.3" and 5.0 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 | ATO J105.2433-00.4249 | 07:01:01.31 -00:25:23.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F0: 1956ApJS....2..271M LF 9 -01 512
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:01:01.02 -00:25:44.7: 14.30 +/- 0.21 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:01:01.02 -00:25:44.7: 15.16 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.30 +/- 0.21
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
ATO J105.2433-00.4249,2461158.6102,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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
ATO J105.2433-00.4249 20260428.1102 12.15CV 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 04 28.1102 2461158.6102 12.45 07:01:10.48 +00:00:19.9
214.03747 2.16878 galactic Mon Second-epoch detections are separated by 2.7" and 4.8 pix
The object was found in VSX 7" Gaia DR3 3112882349279538816
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.650 G 13.670 G A
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:01:10.48 +00:00:19.9: 14.81 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:01:10.48 +00:00:19.9: 15.42 +/- 99.00 upperlimit
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 3112882349279538816,2461158.6102,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 3112882349279538816 20260428.1102 12.45CV 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 04 28.1102 2461158.6102 12.52 06:45:06.21 -00:02:45.5
212.25060 -1.43032 galactic Mon Second-epoch detections are separated by 1.7" and 4.8 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 | target | 06:45:06.21 -00:02:45.5 (user input) | T | P | (position from user input) SpType: G5V 2012A&A...543A.125G CoRoT 102764446/51
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:45:06.21 -00:02:45.5: 13.67 +/- 0.18 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:45:06.21 -00:02:45.5: 13.37 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.40 +/- 0.06
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
target,2461158.6102,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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
target 20260428.1102 12.52CV 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
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
AK Mon,2461158.6102,11.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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
AK Mon 20260428.1102 11.69CV 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: 2461120.60986138 21.03.2026 02:38:02.023 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits
First image: 2461120.60986138 21.03.2026 02:38:02.023 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits
Last image: 2461158.61043603 28.04.2026 02:38:51.673 /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q2b1x1_214021_TTUQ2b1x1_3174574_KviWPu4r/fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 5
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.94
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: 11 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): 29304
Objects passed selection criteria: 29189
Measurements per detected object (mean, median, min, max): 2.9 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.9 2.0 2 4
Average stars detected per image: 21737
Average stars matched: 21299 (97.985 %)
Memory usage VmPeak: 133828 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue Apr 21 18:08:25 CDT 2026
VaST build number 1.0rc89-27-g1ba0f777
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Apr 27 21:51:02 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: 2461120.60986138 21.03.2026 02:38:02.023 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits
First image: 2461120.60986138 21.03.2026 02:38:02.023 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits
Last image: 2461158.61043603 28.04.2026 02:38:51.673 /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q2b1x1_214021_TTUQ2b1x1_3174574_KviWPu4r/fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 189
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.67
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: 104 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): 180523
Objects passed selection criteria: 180191
Measurements per detected object (mean, median, min, max): 3.0 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 3.0 2 4
Average stars detected per image: 144766
Average stars matched: 140430 (97.0048 %)
Memory usage VmPeak: 2074692 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue Apr 21 18:08:25 CDT 2026
VaST build number 1.0rc89-27-g1ba0f777
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Apr 27 21:58:48 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/TTUQ2b1x1/TTUQ2_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 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q2b1x1_214021_TTUQ2b1x1_3174574_KviWPu4r/fd_Mon-02-Q2b1x1_2026-04-27_21-38-05_20.00sec_-5.00C_LIGHT_0020.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q2b1x1_214021_TTUQ2b1x1_3174574_KviWPu4r/fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021.fits
SExtractor catalog cache: saved Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits.cat to cache
SExtractor catalog cache: saved Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.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/Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q2b1x1_214021_TTUQ2b1x1_3174574_KviWPu4r/fd_Mon-02-Q2b1x1_2026-04-27_21-38-05_20.00sec_-5.00C_LIGHT_0020.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q2b1x1_214021_TTUQ2b1x1_3174574_KviWPu4r/fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021.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: 2461158.60990186
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_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits exists and is non-empty
Saving wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits to local_wcs_cache/
'wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits' -> 'local_wcs_cache/wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits'
wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits exists and is non-empty
Saving wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits to local_wcs_cache/
'wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits' -> 'local_wcs_cache/wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits'
wcs_fd_Mon-02-Q2b1x1_2026-04-27_21-38-05_20.00sec_-5.00C_LIGHT_0020.fits exists and is non-empty
Saving wcs_fd_Mon-02-Q2b1x1_2026-04-27_21-38-05_20.00sec_-5.00C_LIGHT_0020.fits to local_wcs_cache/
'wcs_fd_Mon-02-Q2b1x1_2026-04-27_21-38-05_20.00sec_-5.00C_LIGHT_0020.fits' -> 'local_wcs_cache/wcs_fd_Mon-02-Q2b1x1_2026-04-27_21-38-05_20.00sec_-5.00C_LIGHT_0020.fits'
wcs_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021.fits exists and is non-empty
Saving wcs_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021.fits to local_wcs_cache/
'wcs_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021.fits' -> 'local_wcs_cache/wcs_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits (1st reference image)
verification OK: wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits
Image size: 921.1'x633.5' 15.4(deg)x10.6(deg) 9576x6388 pix
Image scale: 5.77"/pix along the X axis and 5.95"/pix along the Y axis
Image center: 06:51:17.088 -01:58:30.73 J2000 4789.000 3195.000
###################################
The image scale is 5.77"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.8" and 8.7"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Mon-02-Q2b1x1_2026-04-27_21-38-05_20.00sec_-5.00C_LIGHT_0020.fits (1st new image)
verification OK: wcs_fd_Mon-02-Q2b1x1_2026-04-27_21-38-05_20.00sec_-5.00C_LIGHT_0020.fits
Image size: 937.3'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 06:51:29.773 -02:01:11.22 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 06:51:17.088 -01:58:30.73
Second-epoch image center 06:51:29.773 -02:01:11.22
Angular distance between the image centers 0.0691 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021.fits (2nd new image)
verification OK: wcs_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021.fits
Image size: 937.3'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 06:51:27.803 -02:01:11.85 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 06:51:17.088 -01:58:30.73
Second-epoch image center 06:51:27.803 -02:01:11.85
Angular distance between the image centers 0.0632 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 06:51:29.773 -02:01:11.22
Second-epoch second image center 06:51:27.803 -02:01:11.85
Angular distance between the image centers 0.00821 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/Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits &> /tmp/tmp.7RUttGzFX6
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits &> /tmp/tmp.2uLFahRhxf
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q2b1x1_214021_TTUQ2b1x1_3174574_KviWPu4r/fd_Mon-02-Q2b1x1_2026-04-27_21-38-05_20.00sec_-5.00C_LIGHT_0020.fits &> /tmp/tmp.7RNa4FBWBY
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q2b1x1_214021_TTUQ2b1x1_3174574_KviWPu4r/fd_Mon-02-Q2b1x1_2026-04-27_21-38-05_20.00sec_-5.00C_LIGHT_0020.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q2b1x1_214021_TTUQ2b1x1_3174574_KviWPu4r/fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021.fits &> /tmp/tmp.SaDsSB4aU4
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q2b1x1_214021_TTUQ2b1x1_3174574_KviWPu4r/fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021.fits
Calibrating the magnitude scale
Found non-empty wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.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_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits and wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits.cat
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_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits and wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits.cat
Found non-empty wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits and wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits.cat
The reference image (wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits) and catalog (wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits.cat) found
'wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits.cat' -> 'wcsmag.cat'
Read 36541 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 94.9458 to 110.5184 deg, Dec -7.3465 to +3.3006 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 94.9458 to 110.5184 deg, Dec -7.3465 to 3.3006 deg
Loaded 23388 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): 309 out of 336 total matches.
Matched with Tycho-2 336 out of 36541 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.830495
a=0.000000 b=1.000000 c=22.830495
From vast_summary.log: estimated ref. image limiting mag.: -7.94
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.89
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.89
Magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 36541 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 94.9458 to 110.5184 deg, Dec -7.3465 to +3.3006 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 94.9458 to 110.5184 deg, Dec -7.3465 to 3.3006 deg
Loaded 23388 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): 309 out of 336 total matches.
Matched with Tycho-2 336 out of 36541 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits via Tycho-2
Forced-photometry filter: calibrated wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits -> calib.txt_param_ref_wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits (aperture=6.4)
Read 36462 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 94.9286 to 110.5255 deg, Dec -7.3103 to +3.2986 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 94.9286 to 110.5255 deg, Dec -7.3103 to 3.2986 deg
Loaded 23325 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): 2099 out of 2264 total matches.
Matched with Tycho-2 2264 out of 36462 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits via Tycho-2
Forced-photometry filter: calibrated wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits -> calib.txt_param_ref_wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits (aperture=6.3)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 3 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.4 pix Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits
2.5 pix Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits
2.6 pix fd_Mon-02-Q2b1x1_2026-04-27_21-38-05_20.00sec_-5.00C_LIGHT_0020.fits
2.6 pix fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021.fits
2.4 pix wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits
2.5 pix wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits
Limiting magnitude estimates:
14.9 mag. Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits
14.9 mag. Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits
13.9 mag. fd_Mon-02-Q2b1x1_2026-04-27_21-38-05_20.00sec_-5.00C_LIGHT_0020.fits
13.9 mag. fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021.fits
All-image limiting magnitude estimate: 13.9 (SNR ) 11.1 (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.7RUttGzFX6 (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_2026-04-27_CI_Mon-02-Q2b1x1_214021_TTUQ2b1x1_3174574_KviWPu4r/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits 566.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits' -> 'wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits
WCS_IMAGE_NAME=wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits
WCS-calibrated image found: wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits
Checking if the catalog wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits.cat corresponding to the image wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits alredy exist and is non-empty...
Catalog wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits.cat corresponding to the image wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits
WCS catalog name: wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3925, passed=36541
Got 36541 stars (including 32595 good ones) from the SExtractor catalog wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits.cat
util/solve_plate_with_UCAC5 got 36541 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 921.1'
Seting catalog search parameters based on the expected field of view 921.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012793 (46.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010234 (36.8 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 3.3)
Done reading UCAC5 zone files...
Matched 436 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 320 matched stars entering correct_measured_positions(), 244 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 319 matched stars entering correct_measured_positions(), 9295 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 9.07"
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 3.3)
Done reading UCAC5 zone files...
Matched 469 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 374 matched stars entering correct_measured_positions(), 9331 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 9.04"
Accuracy estimation diagnostic: 371 matched stars entering correct_measured_positions(), 11803 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 8.95"
Excluding outliers - 371 stars left (next iteration limit 350)
The image catalog is written to wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits -region wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.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.2uLFahRhxf (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_2026-04-27_CI_Mon-02-Q2b1x1_214021_TTUQ2b1x1_3174574_KviWPu4r/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits 566.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits' -> 'wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits
WCS_IMAGE_NAME=wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits
WCS-calibrated image found: wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits
Checking if the catalog wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits.cat corresponding to the image wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits alredy exist and is non-empty...
Catalog wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits.cat corresponding to the image wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits
WCS catalog name: wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3920, passed=36462
Got 36462 stars (including 32518 good ones) from the SExtractor catalog wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits.cat
util/solve_plate_with_UCAC5 got 36462 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 924.5'
Seting catalog search parameters based on the expected field of view 924.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012840 (46.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010272 (37.0 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 3.3)
Done reading UCAC5 zone files...
Matched 634 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 574 matched stars entering correct_measured_positions(), 509 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 3.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 574 matched stars entering correct_measured_positions(), 17673 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 4.15"
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 3.3)
Done reading UCAC5 zone files...
Matched 682 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 641 matched stars entering correct_measured_positions(), 17690 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 4.07"
Accuracy estimation diagnostic: 640 matched stars entering correct_measured_positions(), 19306 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.84"
Excluding outliers - 640 stars left (next iteration limit 631)
The image catalog is written to wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits -region wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.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.7RNa4FBWBY (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_2026-04-27_CI_Mon-02-Q2b1x1_214021_TTUQ2b1x1_3174574_KviWPu4r/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q2b1x1_214021_TTUQ2b1x1_3174574_KviWPu4r/fd_Mon-02-Q2b1x1_2026-04-27_21-38-05_20.00sec_-5.00C_LIGHT_0020.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q2b1x1_214021_TTUQ2b1x1_3174574_KviWPu4r/fd_Mon-02-Q2b1x1_2026-04-27_21-38-05_20.00sec_-5.00C_LIGHT_0020.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q2b1x1_214021_TTUQ2b1x1_3174574_KviWPu4r/fd_Mon-02-Q2b1x1_2026-04-27_21-38-05_20.00sec_-5.00C_LIGHT_0020.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q2b1x1_214021_TTUQ2b1x1_3174574_KviWPu4r/fd_Mon-02-Q2b1x1_2026-04-27_21-38-05_20.00sec_-5.00C_LIGHT_0020.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q2b1x1_214021_TTUQ2b1x1_3174574_KviWPu4r/fd_Mon-02-Q2b1x1_2026-04-27_21-38-05_20.00sec_-5.00C_LIGHT_0020.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_2026-04-27_CI_Mon-02-Q2b1x1_214021_TTUQ2b1x1_3174574_KviWPu4r/fd_Mon-02-Q2b1x1_2026-04-27_21-38-05_20.00sec_-5.00C_LIGHT_0020.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q2b1x1_2026-04-27_21-38-05_20.00sec_-5.00C_LIGHT_0020.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q2b1x1_2026-04-27_21-38-05_20.00sec_-5.00C_LIGHT_0020.fits
Checking if the catalog wcs_fd_Mon-02-Q2b1x1_2026-04-27_21-38-05_20.00sec_-5.00C_LIGHT_0020.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-27_21-38-05_20.00sec_-5.00C_LIGHT_0020.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q2b1x1_2026-04-27_21-38-05_20.00sec_-5.00C_LIGHT_0020.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-27_21-38-05_20.00sec_-5.00C_LIGHT_0020.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Mon-02-Q2b1x1_2026-04-27_21-38-05_20.00sec_-5.00C_LIGHT_0020.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q2b1x1_214021_TTUQ2b1x1_3174574_KviWPu4r/fd_Mon-02-Q2b1x1_2026-04-27_21-38-05_20.00sec_-5.00C_LIGHT_0020.fits
WCS catalog name: wcs_fd_Mon-02-Q2b1x1_2026-04-27_21-38-05_20.00sec_-5.00C_LIGHT_0020.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1035, passed=14533
Got 14533 stars (including 13481 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q2b1x1_2026-04-27_21-38-05_20.00sec_-5.00C_LIGHT_0020.fits.cat
util/solve_plate_with_UCAC5 got 14533 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (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 0.010414 (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 3.3)
Done reading UCAC5 zone files...
Matched 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 918 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 14345 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
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 3.3)
Done reading UCAC5 zone files...
Matched 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 14343 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 14343 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
Excluding outliers - 929 stars left (next iteration limit 1025)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-02-Q2b1x1_2026-04-27_21-38-05_20.00sec_-5.00C_LIGHT_0020.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q2b1x1_2026-04-27_21-38-05_20.00sec_-5.00C_LIGHT_0020.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q2b1x1_214021_TTUQ2b1x1_3174574_KviWPu4r/fd_Mon-02-Q2b1x1_2026-04-27_21-38-05_20.00sec_-5.00C_LIGHT_0020.fits -region wcs_fd_Mon-02-Q2b1x1_2026-04-27_21-38-05_20.00sec_-5.00C_LIGHT_0020.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q2b1x1_2026-04-27_21-38-05_20.00sec_-5.00C_LIGHT_0020.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.SaDsSB4aU4 (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_2026-04-27_CI_Mon-02-Q2b1x1_214021_TTUQ2b1x1_3174574_KviWPu4r/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q2b1x1_214021_TTUQ2b1x1_3174574_KviWPu4r/fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q2b1x1_214021_TTUQ2b1x1_3174574_KviWPu4r/fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q2b1x1_214021_TTUQ2b1x1_3174574_KviWPu4r/fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q2b1x1_214021_TTUQ2b1x1_3174574_KviWPu4r/fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q2b1x1_214021_TTUQ2b1x1_3174574_KviWPu4r/fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021.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_2026-04-27_CI_Mon-02-Q2b1x1_214021_TTUQ2b1x1_3174574_KviWPu4r/fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021.fits
Checking if the catalog wcs_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q2b1x1_214021_TTUQ2b1x1_3174574_KviWPu4r/fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021.fits
WCS catalog name: wcs_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1055, passed=14630
Got 14630 stars (including 13565 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021.fits.cat
util/solve_plate_with_UCAC5 got 14630 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (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 0.010414 (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 3.3)
Done reading UCAC5 zone files...
Matched 938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 919 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 14411 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 3.3)
Done reading UCAC5 zone files...
Matched 938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 14410 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 14410 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
Excluding outliers - 932 stars left (next iteration limit 1027)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q2b1x1_214021_TTUQ2b1x1_3174574_KviWPu4r/fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021.fits -region wcs_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Mon-02-Q2b1x1_2026-04-27_21-38-05_20.00sec_-5.00C_LIGHT_0020.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Mon-02-Q2b1x1_2026-04-27_21-38-05_20.00sec_-5.00C_LIGHT_0020.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q2b1x1_214021_TTUQ2b1x1_3174574_KviWPu4r/wcs_fd_Mon-02-Q2b1x1_2026-04-27_21-38-05_20.00sec_-5.00C_LIGHT_0020.fits'
Saving fully-calibrated image wcs_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q2b1x1_214021_TTUQ2b1x1_3174574_KviWPu4r/wcs_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021.fits'
Preparing the HTML report for the field Mon-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_local.txt__out06854.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 6s
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: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51585_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 51585_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:10:16.98 +01:29:54.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51586_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 51586_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:07:17.11 +01:47:30.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06854_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 06854_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 7s
Prepared the HTML report for the field Mon-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
07:17:30.81 +01:05:34.7
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 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q2b1x1_214021_TTUQ2b1x1_3174574_KviWPu4r/fd_Mon-02-Q2b1x1_2026-04-27_21-38-05_20.00sec_-5.00C_LIGHT_0020.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q2b1x1_214021_TTUQ2b1x1_3174574_KviWPu4r/fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021.fits
SExtractor catalog cache: saved Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits.cat to cache
SExtractor catalog cache: saved Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q2b1x1_214021_TTUQ2b1x1_3174574_KviWPu4r/fd_Mon-02-Q2b1x1_2026-04-27_21-38-05_20.00sec_-5.00C_LIGHT_0020.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q2b1x1_214021_TTUQ2b1x1_3174574_KviWPu4r/fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits
Creating symlink local_wcs_cache/wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits
Creating symlink local_wcs_cache/wcs_fd_Mon-02-Q2b1x1_2026-04-27_21-38-05_20.00sec_-5.00C_LIGHT_0020.fits
Creating symlink local_wcs_cache/wcs_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021.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_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits exists and is non-empty
wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits exists and is non-empty
wcs_fd_Mon-02-Q2b1x1_2026-04-27_21-38-05_20.00sec_-5.00C_LIGHT_0020.fits exists and is non-empty
wcs_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits (1st reference image)
verification OK: wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits
Image size: 921.1'x633.5' 15.4(deg)x10.6(deg) 9576x6388 pix
Image scale: 5.77"/pix along the X axis and 5.95"/pix along the Y axis
Image center: 06:51:17.088 -01:58:30.73 J2000 4789.000 3195.000
###################################
The image scale is 5.77"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.8" and 8.7"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Mon-02-Q2b1x1_2026-04-27_21-38-05_20.00sec_-5.00C_LIGHT_0020.fits (1st new image)
verification OK: wcs_fd_Mon-02-Q2b1x1_2026-04-27_21-38-05_20.00sec_-5.00C_LIGHT_0020.fits
Image size: 937.3'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 06:51:29.773 -02:01:11.22 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 06:51:17.088 -01:58:30.73
Second-epoch image center 06:51:29.773 -02:01:11.22
Angular distance between the image centers 0.0691 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021.fits (2nd new image)
verification OK: wcs_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021.fits
Image size: 937.3'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 06:51:27.803 -02:01:11.85 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 06:51:17.088 -01:58:30.73
Second-epoch image center 06:51:27.803 -02:01:11.85
Angular distance between the image centers 0.0632 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 06:51:29.773 -02:01:11.22
Second-epoch second image center 06:51:27.803 -02:01:11.85
Angular distance between the image centers 0.00821 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/Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits &> /tmp/tmp.1ZnIuurTbu
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits &> /tmp/tmp.FQLQb2Ygov
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q2b1x1_214021_TTUQ2b1x1_3174574_KviWPu4r/fd_Mon-02-Q2b1x1_2026-04-27_21-38-05_20.00sec_-5.00C_LIGHT_0020.fits &> /tmp/tmp.TIjXn78VdV
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q2b1x1_214021_TTUQ2b1x1_3174574_KviWPu4r/fd_Mon-02-Q2b1x1_2026-04-27_21-38-05_20.00sec_-5.00C_LIGHT_0020.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q2b1x1_214021_TTUQ2b1x1_3174574_KviWPu4r/fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021.fits &> /tmp/tmp.edSZ4JBuNs
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q2b1x1_214021_TTUQ2b1x1_3174574_KviWPu4r/fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021.fits
Calibrating the magnitude scale
Found non-empty wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.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_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits and wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits.cat
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_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits and wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits.cat
Found non-empty wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits and wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits.cat
The reference image (wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits) and catalog (wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits.cat) found
'wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits.cat' -> 'wcsmag.cat'
Read 220722 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 94.9439 to 110.5351 deg, Dec -7.3473 to +3.3081 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 94.9439 to 110.5351 deg, Dec -7.3473 to 3.3081 deg
Loaded 23446 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): 371 out of 484 total matches.
Matched with Tycho-2 484 out of 220722 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 21.868254
a=0.000000 b=1.000000 c=21.868254
From vast_summary.log: estimated ref. image limiting mag.: -7.67
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.20
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.20
Magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 220722 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 94.9439 to 110.5351 deg, Dec -7.3473 to +3.3081 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 94.9439 to 110.5351 deg, Dec -7.3473 to 3.3081 deg
Loaded 23446 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): 371 out of 484 total matches.
Matched with Tycho-2 484 out of 220722 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits via Tycho-2
Forced-photometry filter: calibrated wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits -> calib.txt_param_ref_wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits (aperture=5.0)
Read 220494 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 94.9245 to 110.5311 deg, Dec -7.3125 to +3.2993 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 94.9245 to 110.5311 deg, Dec -7.3125 to 3.2993 deg
Loaded 23349 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): 1804 out of 2528 total matches.
Matched with Tycho-2 2528 out of 220494 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits via Tycho-2
Forced-photometry filter: calibrated wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits -> calib.txt_param_ref_wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits (aperture=5.0)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 152 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.3 pix Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits
2.4 pix Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits
2.5 pix fd_Mon-02-Q2b1x1_2026-04-27_21-38-05_20.00sec_-5.00C_LIGHT_0020.fits
2.5 pix fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021.fits
2.3 pix wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits
2.4 pix wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits
Limiting magnitude estimates:
14.2 mag. Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits
14.2 mag. Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits
13.1 mag. fd_Mon-02-Q2b1x1_2026-04-27_21-38-05_20.00sec_-5.00C_LIGHT_0020.fits
13.1 mag. fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021.fits
All-image limiting magnitude estimate: 13.1 (SNR ) 12.5 (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.1ZnIuurTbu (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_2026-04-27_CI_Mon-02-Q2b1x1_214021_TTUQ2b1x1_3174574_KviWPu4r/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits 566.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits' -> 'wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits
WCS_IMAGE_NAME=wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits
WCS-calibrated image found: wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits
Checking if the catalog wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits.cat corresponding to the image wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits alredy exist and is non-empty...
Catalog wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits.cat corresponding to the image wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits
WCS catalog name: wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=28, blended=38776, passed=220694
Got 220694 stars (including 181701 good ones) from the SExtractor catalog wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits.cat
util/solve_plate_with_UCAC5 got 220694 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 921.1'
Seting catalog search parameters based on the expected field of view 921.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012793 (46.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010234 (36.8 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 3.3)
Done reading UCAC5 zone files...
Matched 418 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 311 matched stars entering correct_measured_positions(), 233 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.15"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 307 matched stars entering correct_measured_positions(), 49872 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 9.33"
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 3.3)
Done reading UCAC5 zone files...
Matched 451 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 367 matched stars entering correct_measured_positions(), 49901 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 9.32"
Accuracy estimation diagnostic: 364 matched stars entering correct_measured_positions(), 64427 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 8.21"
Excluding outliers - 364 stars left (next iteration limit 337)
The image catalog is written to wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits -region wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.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.FQLQb2Ygov (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_2026-04-27_CI_Mon-02-Q2b1x1_214021_TTUQ2b1x1_3174574_KviWPu4r/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits 566.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits' -> 'wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits
WCS_IMAGE_NAME=wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits
WCS-calibrated image found: wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits
Checking if the catalog wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits.cat corresponding to the image wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits alredy exist and is non-empty...
Catalog wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits.cat corresponding to the image wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits
WCS catalog name: wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=22, blended=38902, passed=220472
Got 220472 stars (including 181352 good ones) from the SExtractor catalog wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits.cat
util/solve_plate_with_UCAC5 got 220472 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 924.5'
Seting catalog search parameters based on the expected field of view 924.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012840 (46.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010272 (37.0 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 3.3)
Done reading UCAC5 zone files...
Matched 633 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 556 matched stars entering correct_measured_positions(), 490 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 3.15"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 554 matched stars entering correct_measured_positions(), 100492 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 3.72"
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 3.3)
Done reading UCAC5 zone files...
Matched 668 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 620 matched stars entering correct_measured_positions(), 100512 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 3.71"
Accuracy estimation diagnostic: 619 matched stars entering correct_measured_positions(), 116714 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.90"
Excluding outliers - 619 stars left (next iteration limit 609)
The image catalog is written to wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits -region wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.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.TIjXn78VdV (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_2026-04-27_CI_Mon-02-Q2b1x1_214021_TTUQ2b1x1_3174574_KviWPu4r/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q2b1x1_214021_TTUQ2b1x1_3174574_KviWPu4r/fd_Mon-02-Q2b1x1_2026-04-27_21-38-05_20.00sec_-5.00C_LIGHT_0020.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q2b1x1_214021_TTUQ2b1x1_3174574_KviWPu4r/fd_Mon-02-Q2b1x1_2026-04-27_21-38-05_20.00sec_-5.00C_LIGHT_0020.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q2b1x1_214021_TTUQ2b1x1_3174574_KviWPu4r/fd_Mon-02-Q2b1x1_2026-04-27_21-38-05_20.00sec_-5.00C_LIGHT_0020.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q2b1x1_214021_TTUQ2b1x1_3174574_KviWPu4r/fd_Mon-02-Q2b1x1_2026-04-27_21-38-05_20.00sec_-5.00C_LIGHT_0020.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q2b1x1_214021_TTUQ2b1x1_3174574_KviWPu4r/fd_Mon-02-Q2b1x1_2026-04-27_21-38-05_20.00sec_-5.00C_LIGHT_0020.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_2026-04-27_CI_Mon-02-Q2b1x1_214021_TTUQ2b1x1_3174574_KviWPu4r/fd_Mon-02-Q2b1x1_2026-04-27_21-38-05_20.00sec_-5.00C_LIGHT_0020.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q2b1x1_2026-04-27_21-38-05_20.00sec_-5.00C_LIGHT_0020.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q2b1x1_2026-04-27_21-38-05_20.00sec_-5.00C_LIGHT_0020.fits
Checking if the catalog wcs_fd_Mon-02-Q2b1x1_2026-04-27_21-38-05_20.00sec_-5.00C_LIGHT_0020.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-27_21-38-05_20.00sec_-5.00C_LIGHT_0020.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q2b1x1_2026-04-27_21-38-05_20.00sec_-5.00C_LIGHT_0020.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-27_21-38-05_20.00sec_-5.00C_LIGHT_0020.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Mon-02-Q2b1x1_2026-04-27_21-38-05_20.00sec_-5.00C_LIGHT_0020.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q2b1x1_214021_TTUQ2b1x1_3174574_KviWPu4r/fd_Mon-02-Q2b1x1_2026-04-27_21-38-05_20.00sec_-5.00C_LIGHT_0020.fits
WCS catalog name: wcs_fd_Mon-02-Q2b1x1_2026-04-27_21-38-05_20.00sec_-5.00C_LIGHT_0020.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=1, no_mag_err=0, low_SNR=7, blended=9601, passed=103580
Got 103580 stars (including 93877 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q2b1x1_2026-04-27_21-38-05_20.00sec_-5.00C_LIGHT_0020.fits.cat
util/solve_plate_with_UCAC5 got 103580 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (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 0.010414 (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 3.3)
Done reading UCAC5 zone files...
Matched 929 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 927 matched stars entering correct_measured_positions(), 905 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 927 matched stars entering correct_measured_positions(), 101925 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 3.3)
Done reading UCAC5 zone files...
Matched 929 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 927 matched stars entering correct_measured_positions(), 101925 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Accuracy estimation diagnostic: 927 matched stars entering correct_measured_positions(), 101924 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
Excluding outliers - 927 stars left (next iteration limit 1019)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-02-Q2b1x1_2026-04-27_21-38-05_20.00sec_-5.00C_LIGHT_0020.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q2b1x1_2026-04-27_21-38-05_20.00sec_-5.00C_LIGHT_0020.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q2b1x1_214021_TTUQ2b1x1_3174574_KviWPu4r/fd_Mon-02-Q2b1x1_2026-04-27_21-38-05_20.00sec_-5.00C_LIGHT_0020.fits -region wcs_fd_Mon-02-Q2b1x1_2026-04-27_21-38-05_20.00sec_-5.00C_LIGHT_0020.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q2b1x1_2026-04-27_21-38-05_20.00sec_-5.00C_LIGHT_0020.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.edSZ4JBuNs (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_2026-04-27_CI_Mon-02-Q2b1x1_214021_TTUQ2b1x1_3174574_KviWPu4r/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q2b1x1_214021_TTUQ2b1x1_3174574_KviWPu4r/fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q2b1x1_214021_TTUQ2b1x1_3174574_KviWPu4r/fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q2b1x1_214021_TTUQ2b1x1_3174574_KviWPu4r/fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q2b1x1_214021_TTUQ2b1x1_3174574_KviWPu4r/fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q2b1x1_214021_TTUQ2b1x1_3174574_KviWPu4r/fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021.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_2026-04-27_CI_Mon-02-Q2b1x1_214021_TTUQ2b1x1_3174574_KviWPu4r/fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021.fits
Checking if the catalog wcs_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q2b1x1_214021_TTUQ2b1x1_3174574_KviWPu4r/fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021.fits
WCS catalog name: wcs_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=9742, passed=105337
Got 105337 stars (including 95485 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021.fits.cat
util/solve_plate_with_UCAC5 got 105337 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (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 0.010414 (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 3.3)
Done reading UCAC5 zone files...
Matched 929 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 927 matched stars entering correct_measured_positions(), 908 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 927 matched stars entering correct_measured_positions(), 103489 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 3.3)
Done reading UCAC5 zone files...
Matched 929 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 925 matched stars entering correct_measured_positions(), 103486 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Accuracy estimation diagnostic: 925 matched stars entering correct_measured_positions(), 103486 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
Excluding outliers - 925 stars left (next iteration limit 1019)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q2b1x1_214021_TTUQ2b1x1_3174574_KviWPu4r/fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021.fits -region wcs_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Mon-02-Q2b1x1_2026-04-27_21-38-05_20.00sec_-5.00C_LIGHT_0020.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_2026-04-27_CI_Mon-02-Q2b1x1_214021_TTUQ2b1x1_3174574_KviWPu4r/wcs_fd_Mon-02-Q2b1x1_2026-04-27_21-38-05_20.00sec_-5.00C_LIGHT_0020.fits
Saving fully-calibrated image wcs_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021.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_2026-04-27_CI_Mon-02-Q2b1x1_214021_TTUQ2b1x1_3174574_KviWPu4r/wcs_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021.fits
Preparing the HTML report for the field Mon-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Adding exclusion_list_gaiadr2.txt__out246439.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out246453.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out246463.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out246469.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out246470.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out246471.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out246477.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out246485.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out246520.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out246529.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out246532.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out246549.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out246552.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out246555.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out246559.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out246565.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out246566.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out246570.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out246574.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out246579.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out246581.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out246708.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out246950.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out247068.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out247206.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out247265.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out247268.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out247283.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out247289.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out247291.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out247317.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out247325.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out247339.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out247343.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out247378.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out247386.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out247418.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out247430.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out247480.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out247484.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out247526.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out247556.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out247609.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out247648.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out246505.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out129332.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246455.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246460.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246461.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246473.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246476.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246478.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246483.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246487.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246491.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246493.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246495.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246502.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246504.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246510.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246521.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246523.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246525.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246531.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246533.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246534.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246539.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246545.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246546.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246557.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246564.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246573.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246576.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246585.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246586.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246595.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246598.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246949.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247020.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247162.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247182.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247190.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247202.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247208.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247241.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247271.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247294.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247302.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247314.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247341.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247344.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247355.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247372.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247396.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247397.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247412.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247415.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247416.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247432.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247436.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247444.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247529.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247565.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 103s
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: 41s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246439_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 246439_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:59:14.43 -03:28:48.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.70, MAG_FAINT_SEARCH_LIMIT=13.68)GAIADR2_OUTPUT=# 1.970 3102664553364102016 104.80958162134 -03.48026694023 13.6652 13.1213 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.970#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246453_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 246453_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:08:03.67 +01:51:13.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 2.293 3114721866591630848 107.01498515286 +01.85316392246 13.5199 13.3689 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.293#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246455_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246455_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246460_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246460_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246461_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246461_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246463_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 246463_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:08:39.21 -00:21:40.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.51, MAG_FAINT_SEARCH_LIMIT=13.49)GAIADR2_OUTPUT=# 1.226 3109664456700761600 107.16306297148 -00.36135835888 13.1910 12.3130 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.226#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246469_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 246469_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:08:32.68 -00:30:37.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.56, MAG_FAINT_SEARCH_LIMIT=13.54)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246470_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 246470_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:03:13.75 +00:35:38.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.53, MAG_FAINT_SEARCH_LIMIT=13.51)GAIADR2_OUTPUT=# 2.843 3113028202068372608 105.80657819021 +00.59368913725 13.4034 12.5609 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.843#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246471_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 246471_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:10:13.97 -00:48:11.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.41, MAG_FAINT_SEARCH_LIMIT=13.39)GAIADR2_OUTPUT=# 0.896 3109446993918462720 107.55796624694 -00.80316469191 13.3222 13.0864 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.896#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246473_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246473_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246476_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246476_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246477_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 246477_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:44:22.71 -00:41:11.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.52, MAG_FAINT_SEARCH_LIMIT=13.50)GAIADR2_OUTPUT=# 2.148 3107422999169573888 101.09402970642 -00.68659923376 13.1689 12.3844 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.148#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246478_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246478_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246483_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246483_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246485_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 246485_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:07:20.79 -00:46:54.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.53, MAG_FAINT_SEARCH_LIMIT=13.51)GAIADR2_OUTPUT=# 2.342 3109623190655283968 106.83616090144 -00.78220607274 13.4448 12.9601 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.342#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246486_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 246486_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:14:51.43 -01:21:00.8: 14.62 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:14:51.43 -01:21:00.8: 10.37 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.37 +/- 0.00
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246487_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246487_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246488_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 246488_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:04:00.51 -00:30:19.1: 11.67 +/- 0.02 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:04:00.51 -00:30:19.1: 15.48 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 11.67 +/- 0.02
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246491_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246491_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246493_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246493_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246495_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246495_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246502_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246502_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246504_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246504_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246505_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 246505_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:06:36.93 -01:52:56.5 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246510_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246510_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246511_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 246511_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:03:42.72 +02:18:21.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246520_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 246520_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:17:17.54 -01:16:05.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)GAIADR2_OUTPUT=# 2.265 3110060074730787840 109.32259039609 -01.26844658731 13.1751 12.5654 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.265#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246521_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246521_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246523_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246523_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246525_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246525_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246527_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 246527_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:49:16.61 +01:46:34.9: 14.86 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:49:16.61 +01:46:34.9: 12.86 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.86 +/- 0.03
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246529_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 246529_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:12:10.00 +01:52:14.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)GAIADR2_OUTPUT=# 2.913 3114889335955565440 108.04095643351 +01.87027812878 13.1614 12.7350 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.913#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246531_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246531_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246532_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 246532_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:13:11.76 +01:02:12.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.22, MAG_FAINT_SEARCH_LIMIT=13.20)GAIADR2_OUTPUT=# 2.202 3111419174178442112 108.29880385177 +01.03633721655 13.1414 13.0877 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.202#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246533_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246533_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246534_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246534_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246539_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246539_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246545_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246545_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246546_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246546_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246547_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 246547_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:51:02.47 +01:07:15.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246549_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 246549_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:50:26.62 +01:01:28.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.05, MAG_FAINT_SEARCH_LIMIT=13.03)GAIADR2_OUTPUT=# 1.556 3113672412805244544 102.61053048368 +01.02430569162 12.2346 11.0584 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.556#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246551_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 246551_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:54:08.29 -05:53:02.3 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246552_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 246552_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:16:12.89 -04:06:20.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.04, MAG_FAINT_SEARCH_LIMIT=13.02)GAIADR2_OUTPUT=# 2.680 3059915193379489024 109.05299124807 -04.10595624574 12.9249 12.4416 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.680#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246554_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 246554_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:52:13.81 -00:19:18.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246555_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 246555_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:54:06.99 -01:27:59.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.89, MAG_FAINT_SEARCH_LIMIT=12.87)GAIADR2_OUTPUT=# 2.583 3112284318034616192 103.52878928410 -01.46702302221 12.8078 12.2175 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.583#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246557_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246557_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246559_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 246559_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:52:18.96 +02:12:25.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.78, MAG_FAINT_SEARCH_LIMIT=12.76)GAIADR2_OUTPUT=# 2.250 3126274778862660992 103.07844319640 +02.20677067365 12.7018 12.3479 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.250#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246560_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 246560_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:37:41.38 -06:04:36.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246564_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246564_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246565_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 246565_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:01:37.30 -04:14:40.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.82, MAG_FAINT_SEARCH_LIMIT=12.80)GAIADR2_OUTPUT=# 1.870 3101747972982311552 105.40574746029 -04.24506783820 12.7532 12.0169 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.870#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246566_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 246566_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:56:23.96 +01:22:18.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.82, MAG_FAINT_SEARCH_LIMIT=12.80)GAIADR2_OUTPUT=# 2.175 3114102218772312704 104.10002976772 +01.37115075284 12.7076 11.9544 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.175#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246570_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 246570_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:06:04.91 -02:19:39.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.75, MAG_FAINT_SEARCH_LIMIT=12.73)GAIADR2_OUTPUT=# 1.364 3108812472631846016 106.52019261220 -02.32731304734 12.7137 11.9922 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.364#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246573_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246573_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246574_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 246574_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:09:18.47 -01:42:34.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.79, MAG_FAINT_SEARCH_LIMIT=12.77)GAIADR2_OUTPUT=# 1.449 3109224617692615680 107.32664531728 -01.70983647051 12.2567 11.3087 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.449#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246576_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246576_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246579_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 246579_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:09:21.30 +02:14:09.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.56, MAG_FAINT_SEARCH_LIMIT=12.54)GAIADR2_OUTPUT=# 1.768 3115156963958576256 107.33847751877 +02.23567456553 12.4681 12.0482 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.768#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246581_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 246581_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:59:03.29 -02:17:52.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.58, MAG_FAINT_SEARCH_LIMIT=12.56)GAIADR2_OUTPUT=# 2.165 3108998320154606464 104.76311203704 -02.29796996872 12.4004 11.6148 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.165#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246585_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246585_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246586_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246586_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246588_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 246588_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:10:59.32 -03:55:09.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246591_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 246591_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:59:16.73 +02:09:16.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246592_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 246592_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:51:44.43 +00:29:59.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246595_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246595_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246598_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246598_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246602_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 246602_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:38:07.46 -01:28:05.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246603_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 246603_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:10:17.05 +01:29:54.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246604_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 246604_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:07:17.16 +01:47:30.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246708_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 246708_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:03:02.22 +01:23:57.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.31, MAG_FAINT_SEARCH_LIMIT=11.29)GAIADR2_OUTPUT=# 0.954 3114625143928364160 105.75911570779 +01.39910487476 11.2408 11.0074 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.954#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246920_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 246920_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:54:00.53 -04:24:08.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246935_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 246935_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:03:00.82 -04:14:53.0 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246949_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246949_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246950_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 246950_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:00:37.50 -01:51:44.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.45, MAG_FAINT_SEARCH_LIMIT=12.43)GAIADR2_OUTPUT=# 1.618 3109109680066395904 105.15642782143 -01.86277396635 12.3871 11.5938 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.618#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247012_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 247012_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:52:25.55 -05:17:27.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247013_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 247013_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:12:19.63 -02:33:39.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247020_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 247020_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247024_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 247024_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:53:24.20 -01:27:18.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247068_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 247068_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:18:30.82 -04:34:34.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.69, MAG_FAINT_SEARCH_LIMIT=12.67)GAIADR2_OUTPUT=# 1.440 3059640766449151488 109.62829009448 -04.57674061862 12.5879 11.8510 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.440#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247070_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 247070_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:10:20.76 -04:14:38.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247088_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 247088_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:53:08.23 -04:35:54.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247129_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 247129_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:43:32.76 -01:21:19.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247161_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 247161_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:01:13.52 +02:02:02.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247162_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 247162_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247168_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 247168_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:34:14.69 -04:53:31.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247170_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 247170_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:36:41.10 -05:13:21.3 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247182_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 247182_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247187_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 247187_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:02:39.71 -04:37:49.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247190_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 247190_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247195_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 247195_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:52:07.81 +00:28:17.7: 12.90 +/- 0.07 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:52:07.81 +00:28:17.7: 12.80 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.82 +/- 0.03
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247202_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 247202_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247206_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 247206_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:15:41.83 -03:23:27.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.04, MAG_FAINT_SEARCH_LIMIT=13.02)GAIADR2_OUTPUT=# 3.848 3060026248353746688 108.92463740659 -03.39203949534 12.8586 11.9322 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.848#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247208_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 247208_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247209_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 247209_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:50:44.54 -00:31:39.0 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247215_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 247215_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:01:52.75 -01:19:04.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247237_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 247237_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:00:06.67 -02:51:35.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247238_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 247238_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:44:33.79 -01:39:38.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247241_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 247241_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247265_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 247265_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:47:19.75 +01:31:51.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 1.487 3125766220373632256 101.83212084767 +01.53059619715 12.9717 12.4642 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.487#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247268_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 247268_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:17:39.23 -03:44:21.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.02, MAG_FAINT_SEARCH_LIMIT=13.00)GAIADR2_OUTPUT=# 2.146 3059953130831431680 109.41318559446 -03.73972481062 12.9025 12.4423 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.146#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247271_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 247271_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247275_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 247275_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:16:56.05 -05:22:51.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247278_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 247278_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:11:28.58 -00:19:01.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247283_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 247283_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:08:51.15 -01:46:32.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.17, MAG_FAINT_SEARCH_LIMIT=13.15)GAIADR2_OUTPUT=# 3.376 3109234234118285952 107.21394667394 -01.77617496224 13.0380 12.3331 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.376#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247289_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 247289_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:01:32.41 -05:17:17.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.19, MAG_FAINT_SEARCH_LIMIT=13.17)GAIADR2_OUTPUT=# 3.162 3101401244562695680 105.38457775638 -05.28896930257 12.4362 11.2755 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.162#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247291_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 247291_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:41:30.14 +00:57:44.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.19, MAG_FAINT_SEARCH_LIMIT=13.17)GAIADR2_OUTPUT=# 0.978 3125804325323474944 100.37578011780 +00.96206277387 13.1485 12.7058 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.978#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247293_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 247293_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:54:09.59 -05:52:27.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247294_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 247294_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247297_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 247297_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:54:51.39 -01:22:19.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247302_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 247302_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247310_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 247310_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:43:35.24 -01:19:41.9: 12.64 +/- 0.05 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:43:35.24 -01:19:41.9: 12.95 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.84 +/- 0.03
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247314_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 247314_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247317_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 247317_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:00:21.46 -05:50:35.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.09, MAG_FAINT_SEARCH_LIMIT=13.07)GAIADR2_OUTPUT=# 2.876 3100935640049817728 105.08895116582 -05.84376213725 12.7701 11.8846 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.876#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247320_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 247320_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:54:30.14 -04:07:30.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247325_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 247325_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:09:37.59 -01:22:34.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.20, MAG_FAINT_SEARCH_LIMIT=13.18)GAIADR2_OUTPUT=# 2.001 3109339379218885888 107.40665275024 -01.37683283674 13.0624 12.5912 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.001#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247326_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 247326_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:05:07.76 -04:50:56.2: 12.89 +/- 0.07 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:05:07.76 -04:50:56.2: 15.31 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 12.89 +/- 0.07
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247339_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 247339_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:17:25.96 +01:37:35.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)GAIADR2_OUTPUT=# 3.779 3111920547185261696 109.35876621578 +01.62744516688 13.1980 12.9185 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.779#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247341_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 247341_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247343_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 247343_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:56:27.62 +00:06:16.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.26, MAG_FAINT_SEARCH_LIMIT=13.24)GAIADR2_OUTPUT=# 3.219 3113677261828133888 104.11429280310 +00.10422085836 13.1732 12.4789 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.219#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247344_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 247344_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247355_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 247355_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247358_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 247358_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:43:00.75 -02:52:20.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247372_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 247372_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247378_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 247378_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:50:05.71 +00:15:20.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)GAIADR2_OUTPUT=# 1.974 3113554112226157568 102.52351755616 +00.25513630730 13.0221 12.1110 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.974#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247386_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 247386_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:43:00.79 +00:23:39.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.28, MAG_FAINT_SEARCH_LIMIT=13.26)GAIADR2_OUTPUT=# 2.325 3119568410766803968 100.75309723994 +00.39363410704 13.2345 12.5585 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.325#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247396_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 247396_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247397_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 247397_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247412_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 247412_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247415_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 247415_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247416_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 247416_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247418_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 247418_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:47:23.10 -01:59:42.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.34, MAG_FAINT_SEARCH_LIMIT=13.32)GAIADR2_OUTPUT=# 0.592 3106212776163414144 101.84609672672 -01.99519846415 13.3080 12.7592 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.592#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247430_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 247430_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:08:23.08 -05:23:40.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.23, MAG_FAINT_SEARCH_LIMIT=13.21)GAIADR2_OUTPUT=# 1.519 3053355992347959808 107.09595799605 -05.39489496071 13.0832 12.5766 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.519#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247432_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 247432_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247435_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 247435_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:54:15.96 -00:38:31.5: 11.06 +/- 0.01 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:54:15.96 -00:38:31.5: 15.53 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 11.06 +/- 0.01
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247436_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 247436_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247444_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 247444_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247470_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 247470_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:37:58.57 -01:25:25.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247474_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 247474_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:53:07.60 -01:52:43.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247480_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 247480_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:11:26.67 -01:03:06.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.39, MAG_FAINT_SEARCH_LIMIT=13.37)GAIADR2_OUTPUT=# 4.124 3109380129868098176 107.86006082161 -01.05220251966 13.3067 12.8199 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.124#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247484_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 247484_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:58:39.13 -04:20:17.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.39, MAG_FAINT_SEARCH_LIMIT=13.37)GAIADR2_OUTPUT=# 1.428 3101710349067118720 104.66302468638 -04.33867408529 13.0563 12.0264 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.428#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247512_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 247512_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:44:31.62 +00:07:34.1: 14.70 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:44:31.62 +00:07:34.1: 13.14 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.05
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247526_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 247526_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:47:18.09 +01:32:00.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.48, MAG_FAINT_SEARCH_LIMIT=13.46)GAIADR2_OUTPUT=# 1.443 3125769175311132288 101.82503425206 +01.53365566575 13.0807 12.1097 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.443#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247529_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 247529_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247549_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 247549_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:48:16.77 -01:48:40.8: 11.23 +/- 0.02 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:48:16.77 -01:48:40.8: 13.24 +/- 0.05 detection
Forced photometry reference-image weighted average: 11.40 +/- 0.01
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247553_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 247553_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:52:44.23 -02:03:21.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247556_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 247556_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:40:17.61 -04:25:56.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 1.674 3103981287255761536 100.07307980311 -04.43283226625 13.2340 12.7718 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.674#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247557_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 247557_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:54:15.29 -05:59:32.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247565_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 247565_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247568_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 247568_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:54:45.42 -01:43:47.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247609_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 247609_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:53:59.79 -02:44:16.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 5.433 3105945972795426816 103.49787131933 -02.73864765651 13.4074 12.4613 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.433#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247648_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 247648_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:02:19.61 -03:20:39.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.57, MAG_FAINT_SEARCH_LIMIT=13.55)GAIADR2_OUTPUT=# 3.118 3108619920658643968 105.58111518078 -03.34490994692 13.4942 12.9329 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.118#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247706_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 247706_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:55:35.60 -01:32:36.6: 12.78 +/- 0.07 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:55:35.60 -01:32:36.6: 15.47 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 12.78 +/- 0.07
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 37203_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
The candidate 37203_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:17:30.81 +01:05:34.6 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 129332_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 129332_fd_Mon-02-Q2b1x1_2026-04-27_21-38-51_20.00sec_-5.00C_LIGHT_0021
make_report_in_HTML.sh Phase 2 (HTML assembly): 4s
make_report_in_HTML.sh TOTAL: 148s
Prepared the HTML report for the field Mon-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
07:17:30.81 +01:05:34.7
07:12:49.78 -03:03:25.1
06:53:17.60 -00:15:30.1
06:54:34.04 +00:38:32.7
07:07:02.35 -01:54:21.4
06:59:38.67 -06:13:05.3
07:05:38.90 -00:02:17.6
07:02:50.58 -03:19:44.0
07:01:32.59 -06:05:38.0
06:57:30.18 -00:57:12.2
07:15:54.37 -00:50:16.3
07:08:29.29 -00:58:29.1
06:53:42.65 -01:01:11.3
06:52:19.69 -00:56:12.2
07:17:34.01 -02:54:22.2
07:09:58.06 +00:39:41.8
07:12:19.90 -01:08:21.3
07:03:26.97 -05:01:13.1
07:08:41.84 +01:18:41.1
07:07:21.18 -03:23:33.2
07:03:14.57 +01:07:05.2
07:00:46.45 -03:36:06.5
07:18:18.12 -00:24:27.2
07:12:26.22 +01:50:33.8
07:06:40.09 -04:34:47.3
06:59:39.73 -00:40:08.0
07:05:36.21 -00:02:35.6
07:02:00.79 +01:40:10.1
07:08:09.49 -00:32:01.7
07:04:20.91 -04:41:02.2
07:11:00.60 -02:53:39.1
07:08:43.97 -03:56:11.5
07:14:38.84 -03:56:24.7
07:05:30.70 +01:36:35.8
07:06:24.21 +00:20:27.4
07:12:29.97 +00:35:38.2
07:01:38.62 -04:40:49.7
07:12:18.81 +00:29:05.7
07:01:07.55 -03:14:33.5
07:01:22.92 -06:08:22.5
07:00:56.90 -03:16:18.9
07:15:49.67 -00:37:03.1
06:52:57.41 -03:04:55.9
07:01:46.25 +01:19:49.1
07:17:13.16 -01:33:02.6
07:07:11.92 -02:58:18.0
06:39:44.39 +00:57:26.2
06:47:25.92 -01:17:25.0
06:53:58.09 -04:52:51.4
06:45:04.84 -01:02:23.6
06:57:00.80 +00:17:37.4
06:59:40.33 -00:39:47.7
07:07:58.84 -00:56:39.7
07:02:02.17 +00:07:45.9
06:49:33.29 -01:23:30.4
06:59:52.91 -04:47:27.8
07:01:01.02 -00:25:44.7
07:01:10.48 +00:00:19.9
06:45:06.21 -00:02:45.5
########### Completed Mon-02-Q2b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ2.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
07:17:30.81 +01:05:34.7
06:53:17.60 -00:15:30.1
06:54:34.04 +00:38:32.7
07:07:02.35 -01:54:21.4
06:59:38.67 -06:13:05.3
07:05:38.90 -00:02:17.6
07:02:50.58 -03:19:44.0
07:01:32.59 -06:05:38.0
06:57:30.18 -00:57:12.2
07:15:54.37 -00:50:16.3
07:08:29.29 -00:58:29.1
06:53:42.65 -01:01:11.3
06:52:19.69 -00:56:12.2
07:17:34.01 -02:54:22.2
07:09:58.06 +00:39:41.8
07:12:19.90 -01:08:21.3
07:03:26.97 -05:01:13.1
07:08:41.84 +01:18:41.1
07:07:21.18 -03:23:33.2
07:03:14.57 +01:07:05.2
07:00:46.45 -03:36:06.5
07:18:18.12 -00:24:27.2
07:12:26.22 +01:50:33.8
07:06:40.09 -04:34:47.3
06:59:39.73 -00:40:08.0
07:05:36.21 -00:02:35.6
07:02:00.79 +01:40:10.1
07:08:09.49 -00:32:01.7
07:04:20.91 -04:41:02.2
07:11:00.60 -02:53:39.1
07:08:43.97 -03:56:11.5
07:14:38.84 -03:56:24.7
07:05:30.70 +01:36:35.8
07:06:24.21 +00:20:27.4
07:12:29.97 +00:35:38.2
07:01:38.62 -04:40:49.7
07:12:18.81 +00:29:05.7
07:01:07.55 -03:14:33.5
07:01:22.92 -06:08:22.5
07:00:56.90 -03:16:18.9
07:15:49.67 -00:37:03.1
06:52:57.41 -03:04:55.9
07:01:46.25 +01:19:49.1
07:17:13.16 -01:33:02.6
07:07:11.92 -02:58:18.0
06:39:44.39 +00:57:26.2
06:47:25.92 -01:17:25.0
06:53:58.09 -04:52:51.4
06:45:04.84 -01:02:23.6
06:57:00.80 +00:17:37.4
06:59:40.33 -00:39:47.7
07:07:58.84 -00:56:39.7
07:02:02.17 +00:07:45.9
06:49:33.29 -01:23:30.4
06:59:52.91 -04:47:27.8
07:01:01.02 -00:25:44.7
07:01:10.48 +00:00:19.9
06:45:06.21 -00:02:45.5
07:12:49.78 -03:03:25.1
###################################################################################
07:17:30.81 +01:05:34.7 -- not an asteroid (will add it to exclusion list)
06:53:17.60 -00:15:30.1 -- not an asteroid (will add it to exclusion list)
06:54:34.04 +00:38:32.7 -- not an asteroid (will add it to exclusion list)
07:07:02.35 -01:54:21.4 -- not an asteroid (will add it to exclusion list)
06:59:38.67 -06:13:05.3 -- not an asteroid (will add it to exclusion list)
07:05:38.90 -00:02:17.6 -- not an asteroid (will add it to exclusion list)
07:02:50.58 -03:19:44.0 -- not an asteroid (will add it to exclusion list)
07:01:32.59 -06:05:38.0 -- not an asteroid (will add it to exclusion list)
06:57:30.18 -00:57:12.2 -- not an asteroid (will add it to exclusion list)
07:15:54.37 -00:50:16.3 -- not an asteroid (will add it to exclusion list)
07:08:29.29 -00:58:29.1 -- not an asteroid (will add it to exclusion list)
06:53:42.65 -01:01:11.3 -- not an asteroid (will add it to exclusion list)
06:52:19.69 -00:56:12.2 -- not an asteroid (will add it to exclusion list)
07:17:34.01 -02:54:22.2 -- not an asteroid (will add it to exclusion list)
07:09:58.06 +00:39:41.8 -- not an asteroid (will add it to exclusion list)
07:12:19.90 -01:08:21.3 -- not an asteroid (will add it to exclusion list)
07:03:26.97 -05:01:13.1 -- not an asteroid (will add it to exclusion list)
07:08:41.84 +01:18:41.1 -- not an asteroid (will add it to exclusion list)
07:07:21.18 -03:23:33.2 -- not an asteroid (will add it to exclusion list)
07:03:14.57 +01:07:05.2 -- not an asteroid (will add it to exclusion list)
07:00:46.45 -03:36:06.5 -- not an asteroid (will add it to exclusion list)
07:18:18.12 -00:24:27.2 -- not an asteroid (will add it to exclusion list)
07:12:26.22 +01:50:33.8 -- not an asteroid (will add it to exclusion list)
07:06:40.09 -04:34:47.3 -- not an asteroid (will add it to exclusion list)
06:59:39.73 -00:40:08.0 -- not an asteroid (will add it to exclusion list)
07:05:36.21 -00:02:35.6 -- not an asteroid (will add it to exclusion list)
07:02:00.79 +01:40:10.1 -- not an asteroid (will add it to exclusion list)
07:08:09.49 -00:32:01.7 -- not an asteroid (will add it to exclusion list)
07:04:20.91 -04:41:02.2 -- not an asteroid (will add it to exclusion list)
07:11:00.60 -02:53:39.1 -- not an asteroid (will add it to exclusion list)
07:08:43.97 -03:56:11.5 -- not an asteroid (will add it to exclusion list)
07:14:38.84 -03:56:24.7 -- not an asteroid (will add it to exclusion list)
07:05:30.70 +01:36:35.8 -- not an asteroid (will add it to exclusion list)
07:06:24.21 +00:20:27.4 -- not an asteroid (will add it to exclusion list)
07:12:29.97 +00:35:38.2 -- not an asteroid (will add it to exclusion list)
07:01:38.62 -04:40:49.7 -- not an asteroid (will add it to exclusion list)
07:12:18.81 +00:29:05.7 -- not an asteroid (will add it to exclusion list)
07:01:07.55 -03:14:33.5 -- not an asteroid (will add it to exclusion list)
07:01:22.92 -06:08:22.5 -- not an asteroid (will add it to exclusion list)
07:00:56.90 -03:16:18.9 -- not an asteroid (will add it to exclusion list)
07:15:49.67 -00:37:03.1 -- not an asteroid (will add it to exclusion list)
06:52:57.41 -03:04:55.9 -- not an asteroid (will add it to exclusion list)
07:01:46.25 +01:19:49.1 -- not an asteroid (will add it to exclusion list)
07:17:13.16 -01:33:02.6 -- not an asteroid (will add it to exclusion list)
07:07:11.92 -02:58:18.0 -- not an asteroid (will add it to exclusion list)
06:39:44.39 +00:57:26.2 -- not an asteroid (will add it to exclusion list)
06:47:25.92 -01:17:25.0 -- not an asteroid (will add it to exclusion list)
06:53:58.09 -04:52:51.4 -- not an asteroid (will add it to exclusion list)
06:45:04.84 -01:02:23.6 -- not an asteroid (will add it to exclusion list)
06:57:00.80 +00:17:37.4 -- not an asteroid (will add it to exclusion list)
06:59:40.33 -00:39:47.7 -- not an asteroid (will add it to exclusion list)
07:07:58.84 -00:56:39.7 -- not an asteroid (will add it to exclusion list)
07:02:02.17 +00:07:45.9 -- not an asteroid (will add it to exclusion list)
06:49:33.29 -01:23:30.4 -- not an asteroid (will add it to exclusion list)
06:59:52.91 -04:47:27.8 -- not an asteroid (will add it to exclusion list)
07:01:01.02 -00:25:44.7 -- not an asteroid (will add it to exclusion list)
07:01:10.48 +00:00:19.9 -- not an asteroid (will add it to exclusion list)
06:45:06.21 -00:02:45.5 -- not an asteroid (will add it to exclusion list)
07:12:49.78 -03:03:25.1 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
06:39:44.39 +00:57:26.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:04.84 -01:02:23.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:06.21 -00:02:45.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:47:25.92 -01:17:25.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:49:33.29 -01:23:30.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:19.69 -00:56:12.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:57.41 -03:04:55.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:17.60 -00:15:30.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:42.65 -01:01:11.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:58.09 -04:52:51.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:34.04 +00:38:32.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:00.80 +00:17:37.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:30.18 -00:57:12.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:38.67 -06:13:05.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:39.73 -00:40:08.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:40.33 -00:39:47.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:52.91 -04:47:27.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:00:46.45 -03:36:06.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:00:56.90 -03:16:18.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:01.02 -00:25:44.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:07.55 -03:14:33.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:10.48 +00:00:19.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:22.92 -06:08:22.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:32.59 -06:05:38.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:38.62 -04:40:49.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:46.25 +01:19:49.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:00.79 +01:40:10.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:02.17 +00:07:45.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:50.58 -03:19:44.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:14.57 +01:07:05.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:26.97 -05:01:13.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:20.91 -04:41:02.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:30.70 +01:36:35.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:36.21 -00:02:35.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:38.90 -00:02:17.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:24.21 +00:20:27.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:40.09 -04:34:47.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:02.35 -01:54:21.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:11.92 -02:58:18.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:21.18 -03:23:33.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:58.84 -00:56:39.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:09.49 -00:32:01.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:29.29 -00:58:29.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:41.84 +01:18:41.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:43.97 -03:56:11.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:58.06 +00:39:41.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:11:00.60 -02:53:39.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:12:18.81 +00:29:05.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:12:19.90 -01:08:21.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:12:26.22 +01:50:33.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:12:29.97 +00:35:38.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:12:49.78 -03:03:25.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:14:38.84 -03:56:24.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:15:49.67 -00:37:03.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:15:54.37 -00:50:16.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:17:13.16 -01:33:02.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:17:30.81 +01:05:34.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:17:34.01 -02:54:22.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:18:18.12 -00:24:27.2 -- 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)
06:39:44.39 +00:57:26.2 -- not a known variable star
06:45:04.84 -01:02:23.6 -- not a known variable star
06:45:06.21 -00:02:45.5 -- not a known variable star
06:47:25.92 -01:17:25.0 -- a known variable star
06:49:33.29 -01:23:30.4 -- not a known variable star
06:52:19.69 -00:56:12.2 -- not a known variable star
06:52:57.41 -03:04:55.9 -- not a known variable star
06:53:17.60 -00:15:30.1 -- a known variable star
06:53:42.65 -01:01:11.3 -- not a known variable star
06:53:58.09 -04:52:51.4 -- not a known variable star
06:54:34.04 +00:38:32.7 -- a known variable star
06:57:00.80 +00:17:37.4 -- not a known variable star
06:57:30.18 -00:57:12.2 -- a known variable star
06:59:38.67 -06:13:05.3 -- not a known variable star
06:59:39.73 -00:40:08.0 -- not a known variable star
06:59:40.33 -00:39:47.7 -- not a known variable star
06:59:52.91 -04:47:27.8 -- not a known variable star
07:00:46.45 -03:36:06.5 -- not a known variable star
07:00:56.90 -03:16:18.9 -- not a known variable star
07:01:01.02 -00:25:44.7 -- not a known variable star
07:01:07.55 -03:14:33.5 -- a known variable star
07:01:10.48 +00:00:19.9 -- a known variable star
07:01:22.92 -06:08:22.5 -- not a known variable star
07:01:32.59 -06:05:38.0 -- a known variable star
07:01:38.62 -04:40:49.7 -- not a known variable star
07:01:46.25 +01:19:49.1 -- not a known variable star
07:02:00.79 +01:40:10.1 -- not a known variable star
07:02:02.17 +00:07:45.9 -- not a known variable star
07:02:50.58 -03:19:44.0 -- a known variable star
07:03:14.57 +01:07:05.2 -- not a known variable star
07:03:26.97 -05:01:13.1 -- a known variable star
07:04:20.91 -04:41:02.2 -- not a known variable star
07:05:30.70 +01:36:35.8 -- not a known variable star
07:05:36.21 -00:02:35.6 -- not a known variable star
07:05:38.90 -00:02:17.6 -- not a known variable star
07:06:24.21 +00:20:27.4 -- not a known variable star
07:06:40.09 -04:34:47.3 -- a known variable star
07:07:02.35 -01:54:21.4 -- not a known variable star
07:07:11.92 -02:58:18.0 -- not a known variable star
07:07:21.18 -03:23:33.2 -- a known variable star
07:07:58.84 -00:56:39.7 -- not a known variable star
07:08:09.49 -00:32:01.7 -- not a known variable star
07:08:29.29 -00:58:29.1 -- a known variable star
07:08:41.84 +01:18:41.1 -- a known variable star
07:08:43.97 -03:56:11.5 -- not a known variable star
07:09:58.06 +00:39:41.8 -- not a known variable star
07:11:00.60 -02:53:39.1 -- not a known variable star
07:12:18.81 +00:29:05.7 -- not a known variable star
07:12:19.90 -01:08:21.3 -- not a known variable star
07:12:26.22 +01:50:33.8 -- not a known variable star
07:12:29.97 +00:35:38.2 -- not a known variable star
07:12:49.78 -03:03:25.1 -- a known variable star
07:14:38.84 -03:56:24.7 -- not a known variable star
07:15:49.67 -00:37:03.1 -- a known variable star
07:15:54.37 -00:50:16.3 -- not a known variable star
07:17:13.16 -01:33:02.6 -- a known variable star
07:17:30.81 +01:05:34.7 -- a known variable star
07:17:34.01 -02:54:22.2 -- a known variable star
07:18:18.12 -00:24:27.2 -- not a known variable star
Found 41 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
59 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 59 (excluding asteroids and hot pixels, 41 new), not updating the exclusion list!
###################################################################################
Not allowed to update the exclusion list IS_THIS_TEST_RUN=NO ALLOW_EXCLUSION_LIST_UPDATE= NO
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461158.60990186 -observatory V36
01:18:26.41 +05:53:50.1 Mercury (-0.6mag)
04:09:09.67 +21:46:43.0 Venus (-3.9mag)
00:52:09.62 +04:36:09.9 Mars (1.2mag)
07:18:52.47 +22:35:26.7 Jupiter (-2.0mag)
00:34:27.34 +01:21:31.8 Saturn (0.9mag)
03:50:21.71 +19:55:54.8 Uranus (5.8mag)
00:12:21.67 -00:05:51.3 Neptune (7.8mag)
20:34:08.40 -22:53:41.5 Pluto (14.5mag)
11:44:55.77 -00:33:54.3 Moon (-11.6mag)
-rw-r--r-- 1 apache apache 363 Apr 27 21:51 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461158.60990186:
07:18:45.70 +22:35:42.4 Io (5.8mag)
07:18:57.43 +22:35:12.8 Europa (6.0mag)
07:18:54.42 +22:35:29.1 Ganymede (5.4mag)
07:18:45.48 +22:35:50.7 Callisto (6.7mag)
07:21:36.90 +22:18:03.0 Himalia (15.4mag)
07:18:56.06 +22:35:16.8 Thebe (16.3mag)
07:22:00.81 +22:47:53.4 Elara (17.4mag)
07:18:34.38 +23:09:06.6 Pasiphae (17.5mag)
07:26:54.32 +22:34:29.7 Carme (18.6mag)
00:34:39.36 +01:21:32.5 Titan (8.8mag)
00:34:27.00 +01:21:47.8 Rhea (10.1mag)
00:33:57.61 +01:19:56.1 Iapetus (11.5mag)
00:34:30.68 +01:21:13.6 Hyperion (14.8mag)
00:35:53.90 +01:28:57.2 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Apr 27 21:51 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461158.60990186:
16:23:25.98 -23:30:45.2 JWST
18:13:19.48 +31:13:51.0 Chandra
07:54:05.08 -35:47:38.1 XMM-Newton
-rw-r--r-- 1 apache apache 96 Apr 27 21:51 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461158.60990186 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
06:07:56.16 +30:22:19.3 17.9mag P/2009 WX51 (Catalina)
18:55:23.36 -29:32:43.2 13.8mag P/2010 H2 (Vales)
05:16:00.83 -69:07:53.9 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:35:25.55 +31:31:45.0 17.3mag C/2017 K2 (PANSTARRS)
17:28:31.76 +11:55:59.8 17.7mag C/2021 G2 (ATLAS)
23:12:55.18 +29:44:41.2 17.1mag C/2022 E2 (ATLAS)
04:43:36.21 +26:20:49.0 16.1mag C/2022 N2 (PANSTARRS)
09:06:55.78 +32:00:26.1 16.3mag C/2022 QE78 (ATLAS)
08:33:37.54 +01:02:56.9 17.4mag C/2022 R6 (PANSTARRS)
18:50:03.91 +19:30:15.0 17.6mag C/2023 A3 (Tsuchinshan-ATLAS)
15:36:16.89 -11:20:38.4 17.5mag P/2023 B1 (PANSTARRS)
09:03:07.43 -10:02:59.0 17.8mag C/2023 F3 (ATLAS)
22:04:45.46 +63:40:17.5 17.6mag C/2023 H5 (Lemmon)
19:06:19.37 -04:01:04.0 14.0mag C/2023 R1 (PANSTARRS)
20:30:29.90 +87:34:56.5 17.8mag C/2023 X2 (Lemmon)
06:25:21.39 +63:30:49.2 17.3mag C/2024 A1 (ATLAS)
05:37:44.93 +21:42:16.3 11.8mag C/2024 E1 (Wierzchos)
16:10:46.34 +08:20:11.4 17.3mag C/2024 G6 (ATLAS)
20:23:11.74 +18:40:45.5 14.5mag C/2024 J3 (ATLAS)
03:37:32.69 -20:37:35.4 16.3mag C/2024 T5 (ATLAS)
05:27:23.31 +42:27:10.9 17.8mag C/2025 J1 (Borisov)
12:51:27.42 +50:57:30.2 15.7mag C/2025 L1 (ATLAS)
03:45:28.37 -28:14:37.6 17.9mag C/2025 Q3 (ATLAS)
03:01:27.89 +04:58:18.1 8.0mag C/2025 R3 (PANSTARRS)
12:49:05.75 +03:41:08.1 17.3mag C/2025 Y1 (ATLAS)
04:40:00.08 +01:50:10.2 16.0mag C/2026 A1 (MAPS)
00:32:15.69 +39:11:43.3 15.0mag C/2026 B2 (Sun-Gao)
19:06:23.12 -09:03:34.8 11.1mag 10P/Tempel
14:44:01.26 +01:44:46.3 15.1mag 24P/Schaumasse
11:00:15.08 -01:11:11.9 15.8mag 29P/Schwassmann-Wachmann
10:38:39.21 -03:17:10.3 17.2mag 43P/Wolf-Harrington
02:07:30.41 +19:30:32.8 17.3mag 47P/Ashbrook-Jackson
07:34:03.90 +34:19:35.0 17.0mag 63P/Wild
23:44:02.04 -10:03:09.4 15.7mag 65P/Gunn
04:36:43.83 +25:07:41.5 16.0mag 76P/West-Kohoutek-Ikemura
01:32:41.71 +10:33:37.1 14.2mag 78P/Gehrels
23:38:20.91 -05:49:27.6 14.8mag 88P/Howell
02:45:35.74 +23:41:13.0 15.0mag 93P/Lovas
05:18:38.59 +32:50:58.1 16.1mag 123P/West-Hartley
08:44:09.84 +32:48:18.1 16.3mag 124P/Mrkos
02:52:11.48 +15:40:35.4 16.4mag 128P/Shoemaker-Holt
03:11:27.40 +15:52:52.3 17.6mag 131P/Mueller
02:31:14.82 +16:48:55.3 10.6mag 141P/Machholz
02:38:03.21 +09:15:43.7 10.6mag 141P-A/Machholz
01:18:59.86 +04:59:47.4 11.5mag 141P-D/Machholz
01:36:30.18 +04:35:38.9 14.9mag 162P/SidingSpring
22:11:16.38 -08:36:09.0 17.9mag 218P/LINEAR
17:17:00.03 -12:26:42.7 16.1mag 235P/LINEAR
06:01:09.85 +35:26:13.5 16.9mag 240P/NEAT
07:45:18.16 -03:58:07.4 17.8mag 242P/Spahr
22:47:15.27 -17:31:20.3 17.5mag 260P/McNaught
02:23:44.70 +23:27:57.0 17.9mag 295P/LINEAR
15:37:10.01 +07:41:46.7 17.4mag 391P/Kowalski
07:39:39.30 +21:21:36.9 17.7mag 450P/LONEOS
05:54:04.29 +44:19:28.2 17.6mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.8K Apr 27 21:51 comets.txt
############################################################
List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
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
10:53:55.47 -16:06:07.00 ASASSN-26cz 2026-04-22.24 16.32
16:34:34.94 -54:34:58.20 2026-04-25.14 15.99
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
16:34:34.94 -54:34:58.20 2026-04-25.14 15.99
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 -77:29:35.90 ASASSN-26co 2026-04-7.15 14.93
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
05:35:42.80 -63:44:05.50 ASASSN-26ch 2026-03-27.86 13.02
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
12:16:02.87 -53:16:33.70 ASASSN-26cc 2026-03-20.08 3.93
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
06:04:29.75 +53:23:34.00 SN 2026eza 2026-03-18.2 17.48
11:54:57.87 +69:19:28.90 AT2026fsf 2026-03-18.14 16.95
10:44:46.95 +58:27:29.30 SN 2026enn 2026-03-18.13 17.53
20:45:54.04 -73:26:43.00 AT 2026ezy 2026-03-18.13 16.83
06:53:18.10 -59:10:49.30 ASASSN-26bs 2026-03-18.02 16.93
07:45:09.29 -62:14:36.20 ASASSN-26br 2026-03-16.16 16.78
19:24:27.93 -52:04:36.40 AT 2023uk 2026-03-16.35 14.2
04:52:54.50 -15:20:57.10 AT2026fhw 2026-03-14.06 SDSS
11:10:34.24 +02:58:48.10 SN2026drr 2026-03-14.08 0.2
07:26:45.73 -27:45:13.90 ASASSN-26bo 2026-03-14.17 13.8
16:35:46.94 +58:12:28.40 SN2026ebt 2026-03-12.41 17.12
13:01:19.45 +15:42:15.00 SN2026ehe 2026-03-12.11 -0.29
09:15:55.41 +10:08:09.70 SN2026efq 2026-03-12.16 0.06
03:31:20.92 -35:29:29.00 SN2026evh 2026-03-12.05 17.29
06:26:19.15 -85:18:28.10 AT2026ffp 2026-03-12.16 0.37
14:16:42.30 -41:18:36.50 AT2026fij 2026-03-12.05 15.97
10:45:04.71 +00:06:13.10 SN 2026exe 2026-03-11.78 16.48
18:07:45.58 +69:43:01.00 SN2026ess 2026-03-12.37 17.37
13:11:03.58 +49:06:31.80 AT2026ewa 2026-03-12.42 16.77
15:03:25.23 -63:11:22.20 ASASSN-26bp 2026-03-11.92 13.33
13:09:37.25 -35:50:25.20 AT2024cmo 2026-03-11.12 16.29
13:06:01.97 -15:50:14.40 AT2026fdy 2026-03-10.33 16.68
11:30:09.70 -47:26:45.00 ASASSN-26bn 2026-03-10.3 15.14
05:03:25.25 -24:16:50.40 (= Gaia 2026-03-9.09 14.32
03:42:32.53 -04:17:53.70 ASASSN-26bm 2026-03-8.04 15.22
04:31:00.53 -68:29:50.20 ASASSN-26bl 2026-03-7.9 10.26
16:18:17.61 +41:25:11.40 SN 2026dkf 2026-03-6.31 16.7
13:45:00.35 +61:16:50.90 SN 2026ejl 2026-03-6.41 -0.66
-rw-r--r-- 1 apache apache 5.8K Apr 27 21:51 asassn_transients_list.txt
############################################################
Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
08:01:11.02 -03:43:14.1 TCP J08011102-0343141 2026-02-08.8090 15.10Cmag
05:19:15.40 -02:04:51.5 TCP J05191540-0204515 2026-02-13.4306 14.5mag
10:52:41.26 +36:40:08.9 TCP J10524126+3640089 2026-02-17.6065 17.4mag
05:50:50.81 +36:22:45.1 TCP J05505081+3622451 2026-02-17.5511 15.7mag
00:42:51.33 +41:13:49.1 PNV J00425133+4113491 2026-02-20.738 18.3mag
00:43:04.88 +41:29:41.4 PNV J00430488+4129414 2026-02-20.5923 18.84Cmag
17:43:29.74 +11:24:00.3 TCP J17432974+1124003 2026-02-22.3773 13.6mag
09:55:01.59 +69:08:42.7 PNV J09550159+6908427 2026-02-20.893 19.0mag
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
-rw-r--r-- 1 apache apache 188K Apr 27 21:51 tocp_transients_list.txt
############################################################
Truncated list of recent TNS transients from https://www.wis-tns.org/ :
19:23:59.111 -12:30:36.58 AT 2026kgc 2026-04-15.48 18.635
18:39:37.719 +06:55:20.96 AT 2026kgb 2026-04-17.43 16.308
15:06:42.954 -01:17:07.82 AT 2026kga 2026-04-20.40 19.507
17:53:09.200 +11:02:30.70 AT 2026kfz 2026-04-16.84 18.68
16:03:08.437 +31:48:52.12 AT 2026kfy 2026-04-15.37 20.9066
12:40:00.450 -17:44:25.00 AT 2026kfx 2026-04-21.19 17.9
09:56:52.772 +01:49:59.18 AT 2026kfw 2026-04-21.04 22.5328
09:59:02.400 +01:44:31.96 AT 2026kfv 2026-04-16.08 23.04
13:20:14.744 +79:52:47.47 AT 2026kfu 2026-04-20.39 20.1588
15:56:36.952 +46:26:50.20 AT 2026kft 2026-04-15.37 20.5825
14:36:13.311 -40:29:09.08 AT 2026kfs 2026-04-17.20 19.109
17:55:24.804 -72:52:42.49 AT 2026kfr 2026-04-19.04 19.559
14:53:17.557 +07:16:56.07 AT 2026kfq 2026-04-20.44 20.1681
14:23:33.083 +17:33:13.27 AT 2026kfp 2026-04-15.41 20.3946
11:23:12.007 -46:35:10.13 AT 2026kfo 2026-04-18.14 19.338
09:22:59.874 +10:47:32.59 AT 2026kfn 2026-04-15.92 20.064
08:41:46.826 -08:01:26.25 AT 2026kfm 2026-04-20.87 19.199
08:23:28.067 -08:48:36.88 AT 2026kfl 2026-04-19.02 18.681
14:03:29.355 +22:20:30.16 AT 2026kfk 2026-04-15.41 20.4393
16:25:23.534 -76:28:24.80 AT 2026kfj 2026-04-19.01 19.458
-rw-r--r-- 1 apache apache 29K Apr 27 21:51 tns_transients_list.txt
