This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q2b1x1_214741_TTUQ2b1x1_167185_cObK847F
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 04 22.1091 2461152.6091 13.52 07:01:16.43 -02:28:44.5
216.25983 1.05576 galactic Mon Second-epoch detections are separated by 2.4" and 6.3 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 | target | 07:01:16.43 -02:28:44.5 (user input) | T | P | (position from user input) J-Ks=0.397+/-0.071 (G)
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:01:16.43 -02:28:44.5: 14.93 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:01:16.43 -02:28:44.5: 99.00 +/- 99.00 edge
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,2461152.6091,13.52,0.05,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 20260422.1091 13.52CV 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
Mean magnitude and position on the discovery images:
2026 04 22.1091 2461152.6091 13.33 07:06:43.76 -04:24:09.9
218.59404 1.38426 galactic Mon Second-epoch detections are separated by 5.0" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:06:43.76 -04:24:09.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:06:43.76 -04:24:09.9: 14.86 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:06:43.76 -04:24:09.9: 99.00 +/- 99.00 edge
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,2461152.6091,13.33,0.05,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
target 20260422.1091 13.33CV 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 22.1091 2461152.6091 13.23 07:06:39.40 -03:57:46.9
218.19498 1.57011 galactic Mon Second-epoch detections are separated by 7.0" and 7.1 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 | target | 07:06:39.40 -03:57:46.9 (user input) | T | P | (position from user input) J-Ks=0.533+/-0.055 (K)
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:06:39.40 -03:57:46.9: 13.81 +/- 0.15 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:06:39.40 -03:57:46.9: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 13.81 +/- 0.15
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,2461152.6091,13.23,0.05,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 20260422.1091 13.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1091 2461152.6091 13.58 06:51:11.47 -02:22:10.2
215.01290 -1.13508 galactic Mon Second-epoch detections are separated by 3.9" and 5.5 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 | ATO J102.7908-02.3649 | 06:51:10.85 -02:21:53.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:51:11.47 -02:22:10.2: 15.08 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:51:11.47 -02:22:10.2: 99.00 +/- 99.00 edge
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 J102.7908-02.3649,2461152.6091,13.58,0.05,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 J102.7908-02.3649 20260422.1091 13.58CV 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 22.1091 2461152.6091 13.21 06:50:51.74 -05:58:27.0
218.18782 -2.84773 galactic Mon Second-epoch detections are separated by 1.5" and 6.2 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 | 06:50:51.74 -05:58:27.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:50:51.74 -05:58:27.0: 13.83 +/- 0.14 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:50:51.74 -05:58:27.0: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 13.83 +/- 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
target,2461152.6091,13.21,0.05,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 20260422.1091 13.21CV 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 22.1091 2461152.6091 13.27 06:57:07.07 -00:31:51.3
214.05206 1.02155 galactic Mon Second-epoch detections are separated by 3.4" and 6.6 pix
The object was found in VSX19" Gaia DR3 3112469585742136064
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.970 G 14.000 G A
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:57:07.07 -00:31:51.3: 14.61 +/- 0.24 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:57:07.07 -00:31:51.3: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 14.61 +/- 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
Gaia DR3 3112469585742136064,2461152.6091,13.27,0.05,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 3112469585742136064 20260422.1091 13.27CV 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 22.1091 2461152.6091 13.24 06:55:04.55 -00:42:42.4
213.98013 0.48478 galactic Mon Second-epoch detections are separated by 1.9" and 6.0 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 3112484051191710208 | 06:55:05.31 -00:43:02.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:55:04.55 -00:42:42.4: 15.00 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:55:04.55 -00:42:42.4: 99.00 +/- 99.00 edge
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 3112484051191710208,2461152.6091,13.24,0.05,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 3112484051191710208 20260422.1091 13.24CV 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 22.1091 2461152.6091 13.35 06:57:04.33 -04:03:27.8
217.18497 -0.59839 galactic Mon Second-epoch detections are separated by 4.4" and 7.0 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 | Large-amplitude variable Gaia DR2 3102478461016144640 | 06:57:02.56 -04:03:20.3 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.350+/-0.039 (G)
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:57:04.33 -04:03:27.8: 14.90 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:57:04.33 -04:03:27.8: 99.00 +/- 99.00 edge
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
Large-amplitude variable Gaia DR2 3102478461016144640,2461152.6091,13.35,0.05,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
Large-amplitude variable Gaia DR2 3102478461016144640 20260422.1091 13.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1091 2461152.6091 13.24 06:58:39.27 -01:55:30.2
215.46796 0.72689 galactic Mon Second-epoch detections are separated by 1.7" and 6.3 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 J104.6668-01.9250 | 06:58:39.27 -01:55:30.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.245+/-0.045 (F)
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:58:39.27 -01:55:30.2: 15.12 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:58:39.27 -01:55:30.2: 99.00 +/- 99.00 edge
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 J104.6668-01.9250,2461152.6091,13.24,0.05,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 J104.6668-01.9250 20260422.1091 13.24CV 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 22.1091 2461152.6091 13.12 06:50:09.67 -01:21:55.2
214.00163 -0.90654 galactic Mon Second-epoch detections are separated by 4.4" and 6.2 pix
The object was found in VSX22" Gaia DR3 3106354583104874368
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
14.680 G 14.740 G F
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:50:09.67 -01:21:55.2: 14.98 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:50:09.67 -01:21:55.2: 99.00 +/- 99.00 edge
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 3106354583104874368,2461152.6091,13.12,0.05,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
Gaia DR3 3106354583104874368 20260422.1091 13.12CV 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 22.1091 2461152.6091 13.23 06:58:57.82 -01:46:10.4
215.36490 0.86663 galactic Mon Second-epoch detections are separated by 4.5" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3112034312275453824 | 06:58:58.15 -01:46:47.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G3 (LAMOST DR5)
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:58:57.82 -01:46:10.4: 15.01 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:58:57.82 -01:46:10.4: 99.00 +/- 99.00 edge
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 3112034312275453824,2461152.6091,13.23,0.05,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 3112034312275453824 20260422.1091 13.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1091 2461152.6091 13.21 06:56:27.45 -01:27:42.6
214.80516 0.44989 galactic Mon Second-epoch detections are separated by 1.1" and 6.0 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 3112107704678242432 | 06:56:25.33 -01:27:59.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:56:27.45 -01:27:42.6: 14.99 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:56:27.45 -01:27:42.6: 99.00 +/- 99.00 edge
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 3112107704678242432,2461152.6091,13.21,0.05,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 3112107704678242432 20260422.1091 13.21CV 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 22.1091 2461152.6091 13.12 06:53:22.56 -03:34:23.0
216.33308 -1.19791 galactic Mon Second-epoch detections are separated by 2.6" and 6.7 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 | ATO J103.3373-03.5634 | 06:53:23.20 -03:33:55.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: B5: 1956ApJS....2..271M LF 9 -04 82
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:53:22.56 -03:34:23.0: 14.95 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:53:22.56 -03:34:23.0: 99.00 +/- 99.00 edge
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 J103.3373-03.5634,2461152.6091,13.12,0.05,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 J103.3373-03.5634 20260422.1091 13.12CV 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 22.1091 2461152.6091 12.93 07:03:39.67 -04:38:24.6
218.45412 0.59592 galactic Mon Second-epoch detections are separated by 1.4" and 6.3 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 J105.9152-04.6412 | 07:03:37.08 -04:38:14.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A0 1949AnHar.112....1C HD 296164
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:03:39.67 -04:38:24.6: 14.71 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:03:39.67 -04:38:24.6: 99.00 +/- 99.00 edge
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 J105.9152-04.6412,2461152.6091,12.93,0.05,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 J105.9152-04.6412 20260422.1091 12.93CV 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 22.1091 2461152.6091 13.26 06:46:25.32 +00:47:27.1
211.65617 -0.75525 galactic Mon Second-epoch detections are separated by 1.0" and 6.4 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 | target | 06:46:25.32 +00:47:27.1 (user input) | T | P | (position from user input) SpType: A7III 2012A&A...541A..34S CoRoT 102814727 J-Ks=0.365+/-0.063 (G)
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:46:25.32 +00:47:27.1: 14.89 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:46:25.32 +00:47:27.1: 99.00 +/- 99.00 edge
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,2461152.6091,13.26,0.05,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
target 20260422.1091 13.26CV 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 22.1091 2461152.6091 13.05 06:57:40.53 -03:53:12.3
217.10154 -0.38646 galactic Mon Second-epoch detections are separated by 1.2" and 6.5 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 | 06:57:40.53 -03:53:12.3 (user input) | T | P | (position from user input) J-Ks=0.331+/-0.042 (G)
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:57:40.53 -03:53:12.3: 14.97 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:57:40.53 -03:53:12.3: 99.00 +/- 99.00 edge
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,2461152.6091,13.05,0.05,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
target 20260422.1091 13.05CV 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 22.1091 2461152.6091 13.16 06:43:45.59 +00:35:15.7
211.53324 -1.44012 galactic Mon Second-epoch detections are separated by 3.6" and 6.5 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 | Gaia DR3 3125582872512184960 | 06:43:43.59 +00:34:43.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:43:45.59 +00:35:15.7: 14.93 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:43:45.59 +00:35:15.7: 99.00 +/- 99.00 edge
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 3125582872512184960,2461152.6091,13.16,0.05,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 3125582872512184960 20260422.1091 13.16CV 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 22.1091 2461152.6091 13.01 07:05:19.95 -02:51:43.1
217.06454 1.78157 galactic Mon Second-epoch detections are separated by 7.8" and 7.4 pix
The object was found in VSX 3" Gaia DR3 3108002544877231872
Type: RS
# Max. Min./Amp. JD0 Period
14.060 G 14.100 G K
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:05:19.95 -02:51:43.1: 14.86 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:05:19.95 -02:51:43.1: 99.00 +/- 99.00 edge
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 3108002544877231872,2461152.6091,13.01,0.05,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 3108002544877231872 20260422.1091 13.01CV 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 22.1091 2461152.6091 12.96 07:08:17.17 -04:56:02.0
219.24426 1.48460 galactic Mon Second-epoch detections are separated by 1.7" and 6.5 pix
The object was found in VSX 2" Gaia DR3 3059427667355169920
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
14.000 G 14.030 G A
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:08:17.17 -04:56:02.0: 14.72 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:08:17.17 -04:56:02.0: 99.00 +/- 99.00 edge
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 3059427667355169920,2461152.6091,12.96,0.05,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 3059427667355169920 20260422.1091 12.96CV 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 22.1091 2461152.6091 12.99 07:03:23.86 -00:39:18.2
214.87958 2.36161 galactic Mon Second-epoch detections are separated by 8.0" and 6.3 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 J105.8508-00.6575 | 07:03:23.86 -00:39:18.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.460+/-0.037 (G)
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:03:23.86 -00:39:18.2: 14.47 +/- 0.27 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:03:23.86 -00:39:18.2: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 14.47 +/- 0.27
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 J105.8508-00.6575,2461152.6091,12.99,0.05,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 J105.8508-00.6575 20260422.1091 12.99CV 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 22.1091 2461152.6091 13.07 06:53:30.37 -03:06:08.7
215.92889 -0.95451 galactic Mon Second-epoch detections are separated by 1.5" and 6.3 pix
The object was found in VSX19" Gaia DR3 3102837412905531904
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.910 G 13.930 G A
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:53:30.37 -03:06:08.7: 14.93 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:53:30.37 -03:06:08.7: 99.00 +/- 99.00 edge
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 3102837412905531904,2461152.6091,13.07,0.05,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
Gaia DR3 3102837412905531904 20260422.1091 13.07CV 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 22.1091 2461152.6091 13.11 06:58:27.06 -03:14:41.3
216.61882 0.07886 galactic Mon Second-epoch detections are separated by 1.2" and 6.3 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 J104.6016-03.2501 | 06:58:24.40 -03:14:24.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: K0: 1956ApJS....2..271M LF 9 -04 150
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:58:27.06 -03:14:41.3: 14.97 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:58:27.06 -03:14:41.3: 99.00 +/- 99.00 edge
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 J104.6016-03.2501,2461152.6091,13.11,0.05,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 J104.6016-03.2501 20260422.1091 13.11CV 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 22.1091 2461152.6091 13.07 06:52:00.95 +01:29:15.8
211.67364 0.80687 galactic Mon Second-epoch detections are separated by 0.4" and 6.3 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 | target | 06:52:00.95 +01:29:15.8 (user input) | T | P | (position from user input) J-Ks=0.308+/-0.060 (F)
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:52:00.95 +01:29:15.8: 15.03 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:52:00.95 +01:29:15.8: 99.00 +/- 99.00 edge
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,2461152.6091,13.07,0.05,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 20260422.1091 13.07CV 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 22.1091 2461152.6091 12.90 06:53:41.51 -01:02:04.6
214.10963 0.02966 galactic Mon Second-epoch detections are separated by 2.3" and 5.9 pix
The object was found in VSX20" Gaia DR3 3112377913960540288
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.490 G 13.510 G B
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:53:41.51 -01:02:04.6: 14.33 +/- 0.22 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:53:41.51 -01:02:04.6: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 14.33 +/- 0.22
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 3112377913960540288,2461152.6091,12.90,0.05,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 3112377913960540288 20260422.1091 12.90CV 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 22.1091 2461152.6091 12.97 06:53:46.06 -00:14:32.6
213.41323 0.40783 galactic Mon Second-epoch detections are separated by 1.6" and 6.2 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 J103.4439-00.2500 | 06:53:47.12 -00:14:49.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.183+/-0.044 (F)
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:53:46.06 -00:14:32.6: 14.86 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:53:46.06 -00:14:32.6: 99.00 +/- 99.00 edge
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 J103.4439-00.2500,2461152.6091,12.97,0.05,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 J103.4439-00.2500 20260422.1091 12.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1091 2461152.6091 12.91 06:54:41.07 -02:07:02.7
215.18640 -0.24345 galactic Mon Second-epoch detections are separated by 1.4" and 6.1 pix
The object was found in VSX 2" Gaia DR3 3106052732803548160
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
14.010 G 14.040 G A
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:54:41.07 -02:07:02.7: 14.89 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:54:41.07 -02:07:02.7: 99.00 +/- 99.00 edge
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 3106052732803548160,2461152.6091,12.91,0.05,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 3106052732803548160 20260422.1091 12.91CV 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 22.1091 2461152.6091 13.06 06:58:39.32 +01:21:59.1
212.53802 2.22870 galactic Mon Second-epoch detections are separated by 1.5" and 6.2 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 J104.6569+01.3693 | 06:58:39.32 +01:21:59.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:58:39.32 +01:21:59.1: 15.03 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:58:39.32 +01:21:59.1: 99.00 +/- 99.00 edge
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 J104.6569+01.3693,2461152.6091,13.06,0.05,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
ATO J104.6569+01.3693 20260422.1091 13.06CV 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 22.1091 2461152.6091 12.97 06:53:33.71 -00:32:06.2
213.65023 0.22856 galactic Mon Second-epoch detections are separated by 4.3" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3113254808845036928 | 06:53:31.24 -00:31:46.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:53:33.71 -00:32:06.2: 14.85 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:53:33.71 -00:32:06.2: 99.00 +/- 99.00 edge
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 3113254808845036928,2461152.6091,12.97,0.05,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 3113254808845036928 20260422.1091 12.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1091 2461152.6091 12.85 07:05:03.97 -03:53:19.5
217.94687 1.25173 galactic Mon Second-epoch detections are separated by 4.2" and 5.5 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 | ATO J106.2634-03.8889 | 07:05:03.97 -03:53:19.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:05:03.97 -03:53:19.5: 13.86 +/- 0.13 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:05:03.97 -03:53:19.5: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 13.86 +/- 0.13
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 J106.2634-03.8889,2461152.6091,12.85,0.05,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 J106.2634-03.8889 20260422.1091 12.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1091 2461152.6091 12.95 07:02:01.24 -00:36:16.1
214.67719 2.07849 galactic Mon Second-epoch detections are separated by 1.1" and 6.3 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 J105.4965-00.6001 | 07:02:00.46 -00:35:58.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.302+/-0.035 (F)
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:02:01.24 -00:36:16.1: 14.93 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:02:01.24 -00:36:16.1: 99.00 +/- 99.00 edge
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 J105.4965-00.6001,2461152.6091,12.95,0.05,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 J105.4965-00.6001 20260422.1091 12.95CV 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 22.1091 2461152.6091 12.83 06:54:14.55 -01:36:53.2
214.68871 -0.11247 galactic Mon Second-epoch detections are separated by 1.2" and 6.4 pix
The object was found in VSX18" Gaia DR3 3112090082431827968
Type: RS
# Max. Min./Amp. JD0 Period
16.370 G 16.450 G G
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:54:14.55 -01:36:53.2: 14.62 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:54:14.55 -01:36:53.2: 99.00 +/- 99.00 edge
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 3112090082431827968,2461152.6091,12.83,0.05,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 3112090082431827968 20260422.1091 12.83CV 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 22.1091 2461152.6091 12.77 06:48:07.59 -00:40:39.3
213.15753 -1.04572 galactic Mon Second-epoch detections are separated by 2.5" and 6.1 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 3107197805444320128 | 06:48:06.98 -00:41:00.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.292+/-0.032 (F)
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:48:07.59 -00:40:39.3: 14.90 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:48:07.59 -00:40:39.3: 99.00 +/- 99.00 edge
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 3107197805444320128,2461152.6091,12.77,0.05,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 3107197805444320128 20260422.1091 12.77CV 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 22.1091 2461152.6091 12.70 07:03:25.13 -05:00:42.0
218.75664 0.37199 galactic Mon Second-epoch detections are separated by 2.1" and 6.1 pix
The object was found in VSX16" Gaia DR3 3101503262931006720
Type: VAR
# Max. Min./Amp. JD0 Period
15.490 G 15.550 G 0.560090000000 A
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:03:25.13 -05:00:42.0: 14.45 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:03:25.13 -05:00:42.0: 99.00 +/- 99.00 edge
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 3101503262931006720,2461152.6091,12.70,0.05,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 3101503262931006720 20260422.1091 12.70CV 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 22.1091 2461152.6091 12.73 07:07:04.81 -03:10:08.0
217.53764 2.02853 galactic Mon Second-epoch detections are separated by 2.7" and 6.5 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 | ATO J106.7707-03.1723 | 07:07:04.25 -03:10:25.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.148+/-0.048 (F)
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:07:04.81 -03:10:08.0: 14.11 +/- 0.19 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:07:04.81 -03:10:08.0: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 14.11 +/- 0.19
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 J106.7707-03.1723,2461152.6091,12.73,0.05,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 J106.7707-03.1723 20260422.1091 12.73CV 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 22.1091 2461152.6091 12.84 06:51:10.39 +01:05:57.7
211.92330 0.44237 galactic Mon Second-epoch detections are separated by 0.6" and 6.2 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 | 06:51:10.39 +01:05:57.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:51:10.39 +01:05:57.7: 15.05 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:51:10.39 +01:05:57.7: 99.00 +/- 99.00 edge
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,2461152.6091,12.84,0.05,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 20260422.1091 12.84CV 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 22.1091 2461152.6091 12.91 06:53:04.49 -05:33:23.4
218.06565 -2.16773 galactic Mon Second-epoch detections are separated by 1.1" and 6.3 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 | target | 06:53:04.49 -05:33:23.4 (user input) | T | P | (position from user input) SpType: G2IV 2012A&A...543A.125G CoRoT 110689731
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:53:04.49 -05:33:23.4: 13.82 +/- 0.14 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:53:04.49 -05:33:23.4: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 13.82 +/- 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
target,2461152.6091,12.91,0.05,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 20260422.1091 12.91CV 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 22.1091 2461152.6091 12.81 06:57:24.02 -00:50:14.8
214.35709 0.94452 galactic Mon Second-epoch detections are separated by 1.9" and 6.5 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 | ATO J104.3502-00.8380 | 06:57:24.02 -00:50:14.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.196+/-0.045 (F)
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:57:24.02 -00:50:14.8: 13.68 +/- 0.10 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:57:24.02 -00:50:14.8: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 13.68 +/- 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
ATO J104.3502-00.8380,2461152.6091,12.81,0.05,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
ATO J104.3502-00.8380 20260422.1091 12.81CV 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 22.1091 2461152.6091 12.71 06:55:03.18 -01:02:50.8
214.27624 0.32659 galactic Mon Second-epoch detections are separated by 2.4" and 6.4 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 | target | 06:55:03.18 -01:02:50.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:55:03.18 -01:02:50.8: 13.88 +/- 0.15 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:55:03.18 -01:02:50.8: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 13.88 +/- 0.15
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,2461152.6091,12.71,0.05,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
target 20260422.1091 12.71CV 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 22.1091 2461152.6091 12.64 07:04:08.47 -05:07:03.8
218.93336 0.48323 galactic Mon Second-epoch detections are separated by 1.3" and 6.1 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 J106.0325-05.1158 | 07:04:08.47 -05:07:03.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.114+/-0.045 (A)
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:04:08.47 -05:07:03.8: 14.92 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:04:08.47 -05:07:03.8: 99.00 +/- 99.00 edge
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 J106.0325-05.1158,2461152.6091,12.64,0.05,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 J106.0325-05.1158 20260422.1091 12.64CV 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 22.1091 2461152.6091 12.88 06:42:40.75 -00:18:15.0
212.20391 -2.08745 galactic Mon Second-epoch detections are separated by 3.3" and 6.4 pix
The object was found in VSX23" Gaia DR3 3119460486829616640
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
15.740 G 15.780 G
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:42:40.75 -00:18:15.0: 14.89 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:42:40.75 -00:18:15.0: 99.00 +/- 99.00 edge
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 3119460486829616640,2461152.6091,12.88,0.05,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 3119460486829616640 20260422.1091 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1091 2461152.6091 12.73 07:08:48.84 -03:43:02.7
218.22408 2.16092 galactic Mon Second-epoch detections are separated by 6.5" and 6.5 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 | ATO J107.2021-03.7245 | 07:08:48.84 -03:43:02.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:08:48.84 -03:43:02.7: 14.86 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:08:48.84 -03:43:02.7: 99.00 +/- 99.00 edge
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 J107.2021-03.7245,2461152.6091,12.73,0.05,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 J107.2021-03.7245 20260422.1091 12.73CV 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 22.1091 2461152.6091 12.56 07:09:10.38 -01:30:23.5
216.29894 3.25558 galactic Mon Second-epoch detections are separated by 2.6" and 6.7 pix
The object was found in VSX17" Gaia DR3 3109336454339492608
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
16.980 G 17.020 G
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:09:10.38 -01:30:23.5: 14.73 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:09:10.38 -01:30:23.5: 99.00 +/- 99.00 edge
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 3109336454339492608,2461152.6091,12.56,0.05,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 3109336454339492608 20260422.1091 12.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1091 2461152.6091 12.70 06:46:00.22 -00:22:10.0
212.64122 -1.37756 galactic Mon Second-epoch detections are separated by 0.3" and 6.3 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 | Gaia DR3 3107459557930729984 | 06:46:03.03 -00:22:14.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G8III 1956ApJS....2..271M LF 9 -01 40 J-Ks=0.396+/-0.037 (G)
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:46:00.22 -00:22:10.0: 14.85 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:46:00.22 -00:22:10.0: 99.00 +/- 99.00 edge
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 3107459557930729984,2461152.6091,12.70,0.05,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 3107459557930729984 20260422.1091 12.70CV 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 22.1091 2461152.6091 12.66 06:41:44.19 +00:27:30.3
211.41733 -1.94917 galactic Mon Second-epoch detections are separated by 1.7" and 6.5 pix
The object was found in VSX13" Gaia DR3 3119584113167330944
Type: E
# Max. Min./Amp. JD0 Period
17.800 G 17.990 G 1.585640000000
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:41:44.19 +00:27:30.3: 15.11 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:41:44.19 +00:27:30.3: 99.00 +/- 99.00 edge
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 3119584113167330944,2461152.6091,12.66,0.05,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 3119584113167330944 20260422.1091 12.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1091 2461152.6091 12.61 06:46:13.83 +00:50:42.9
211.58593 -0.77303 galactic Mon Second-epoch detections are separated by 0.7" and 6.4 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 | ATO J101.5447+00.8442 | 06:46:13.83 +00:50:42.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:46:13.83 +00:50:42.9: 15.01 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:46:13.83 +00:50:42.9: 99.00 +/- 99.00 edge
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 J101.5447+00.8442,2461152.6091,12.61,0.05,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 J101.5447+00.8442 20260422.1091 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 22.1091 2461152.6091 12.67 07:07:06.80 +01:39:59.8
213.23448 4.24727 galactic Mon Second-epoch detections are separated by 3.4" and 6.6 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 3114694099624336256 | 07:07:06.57 +01:40:21.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:07:06.80 +01:39:59.8: 14.90 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:07:06.80 +01:39:59.8: 99.00 +/- 99.00 edge
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 3114694099624336256,2461152.6091,12.67,0.05,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 3114694099624336256 20260422.1091 12.67CV 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 22.1091 2461152.6091 12.71 07:07:51.34 -05:46:59.8
219.94926 0.99864 galactic Mon Second-epoch detections are separated by 1.3" and 6.5 pix
The object was found in VSX 4" Gaia DR3 3053304074782543488
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
14.770 G 14.810 G A
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:07:51.34 -05:46:59.8: 14.85 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:07:51.34 -05:46:59.8: 99.00 +/- 99.00 edge
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 3053304074782543488,2461152.6091,12.71,0.05,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 3053304074782543488 20260422.1091 12.71CV 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 22.1091 2461152.6091 12.66 06:54:34.23 -01:51:46.6
214.94695 -0.15272 galactic Mon Second-epoch detections are separated by 0.8" and 6.3 pix
The object was found in VSX 1" Gaia DR3 3112065790097626240
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.720 G 13.760 G A
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:54:34.23 -01:51:46.6: 14.90 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:54:34.23 -01:51:46.6: 99.00 +/- 99.00 edge
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 3112065790097626240,2461152.6091,12.66,0.05,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 3112065790097626240 20260422.1091 12.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1091 2461152.6091 12.64 06:49:52.39 -02:39:53.8
215.12600 -1.56270 galactic Mon Second-epoch detections are separated by 2.0" and 6.4 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 3105924742777831040 | 06:49:55.26 -02:39:53.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: B9 1949AnHar.112....1C HD 295505 J-Ks=0.323+/-0.033 (G)
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:49:52.39 -02:39:53.8: 13.79 +/- 0.12 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:49:52.39 -02:39:53.8: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 13.79 +/- 0.12
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 3105924742777831040,2461152.6091,12.64,0.05,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
Gaia DR3 3105924742777831040 20260422.1091 12.64CV 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 22.1091 2461152.6091 12.51 06:51:28.75 +01:57:02.8
211.20031 0.89856 galactic Mon Second-epoch detections are separated by 2.1" and 6.1 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 J102.8710+01.9494 | 06:51:28.44 +01:56:40.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F9 (LAMOST DR5) J-Ks=0.380+/-0.065 (G)
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:51:28.75 +01:57:02.8: 15.01 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:51:28.75 +01:57:02.8: 99.00 +/- 99.00 edge
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 J102.8710+01.9494,2461152.6091,12.51,0.05,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
ATO J102.8710+01.9494 20260422.1091 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 22.1091 2461152.6091 12.62 07:09:08.39 -01:41:28.4
216.45953 3.16354 galactic Mon Second-epoch detections are separated by 2.2" and 6.1 pix
The object was found in VSX 2" Gaia DR3 3109235166132304128
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.820 G 13.850 G F
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:09:08.39 -01:41:28.4: 13.71 +/- 0.12 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:09:08.39 -01:41:28.4: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 13.71 +/- 0.12
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 3109235166132304128,2461152.6091,12.62,0.05,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 3109235166132304128 20260422.1091 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 22.1091 2461152.6091 12.56 07:08:32.25 -04:39:28.5
219.02796 1.66716 galactic Mon Second-epoch detections are separated by 1.5" and 6.5 pix
The object was found in VSX20" Gaia DR3 3059453162280747520
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
15.100 G 15.120 G A
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:08:32.25 -04:39:28.5: 14.26 +/- 0.25 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:08:32.25 -04:39:28.5: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 14.26 +/- 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 3059453162280747520,2461152.6091,12.56,0.05,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 3059453162280747520 20260422.1091 12.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1091 2461152.6091 12.61 07:03:24.00 -02:49:52.4
216.81607 1.36673 galactic Mon Second-epoch detections are separated by 2.2" and 6.6 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 J105.8499-02.8303 | 07:03:24.00 -02:49:52.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:03:24.00 -02:49:52.4: 14.92 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:03:24.00 -02:49:52.4: 99.00 +/- 99.00 edge
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 J105.8499-02.8303,2461152.6091,12.61,0.05,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 J105.8499-02.8303 20260422.1091 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 22.1091 2461152.6091 12.55 07:08:02.96 -03:23:39.4
217.84913 2.13994 galactic Mon Second-epoch detections are separated by 7.3" and 6.1 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 J107.0132-03.3948 | 07:08:02.96 -03:23:39.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:08:02.96 -03:23:39.4: 14.89 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:08:02.96 -03:23:39.4: 99.00 +/- 99.00 edge
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 J107.0132-03.3948,2461152.6091,12.55,0.05,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 J107.0132-03.3948 20260422.1091 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1091 2461152.6091 12.49 07:02:17.20 -03:49:24.9
217.57122 0.66536 galactic Mon Second-epoch detections are separated by 1.1" and 6.0 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 | 07:02:17.20 -03:49:24.9 (user input) | T | P | (position from user input) J-Ks=0.263+/-0.033 (F)
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:02:17.20 -03:49:24.9: 14.80 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:02:17.20 -03:49:24.9: 99.00 +/- 99.00 edge
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,2461152.6091,12.49,0.05,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 20260422.1091 12.49CV 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 22.1091 2461152.6091 12.51 06:35:07.33 -03:03:04.3
213.79377 -5.01905 galactic Mon Second-epoch detections are separated by 0.9" and 6.0 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 J098.7797-03.0546 | 06:35:07.33 -03:03:04.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.459+/-0.035 (G)
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:35:07.33 -03:03:04.3: 13.93 +/- 0.15 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:35:07.33 -03:03:04.3: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 13.93 +/- 0.15
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 J098.7797-03.0546,2461152.6091,12.51,0.05,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
ATO J098.7797-03.0546 20260422.1091 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 22.1091 2461152.6091 12.59 06:59:20.97 -05:44:56.3
218.94877 -0.86597 galactic Mon Second-epoch detections are separated by 2.1" and 6.0 pix
The object was found in VSX 2" Gaia DR3 3100981956976601344
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.560 G 13.590 G B
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:59:20.97 -05:44:56.3: 14.95 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:59:20.97 -05:44:56.3: 99.00 +/- 99.00 edge
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 3100981956976601344,2461152.6091,12.59,0.05,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 3100981956976601344 20260422.1091 12.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1091 2461152.6091 12.43 06:46:12.55 +00:51:08.4
211.57719 -0.77454 galactic Mon Second-epoch detections are separated by 1.2" and 6.2 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 J101.5447+00.8442 | 06:46:12.55 +00:51:08.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: A8V 2012A&A...541A..34S CoRoT 102807727 J-Ks=0.277+/-0.033 (F)
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:46:12.55 +00:51:08.4: 15.02 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:46:12.55 +00:51:08.4: 99.00 +/- 99.00 edge
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 J101.5447+00.8442,2461152.6091,12.43,0.05,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 J101.5447+00.8442 20260422.1091 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 22.1091 2461152.6091 12.44 07:05:12.07 -06:04:40.3
219.90750 0.27703 galactic Mon Second-epoch detections are separated by 2.5" and 6.0 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 | 07:05:12.07 -06:04:40.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:05:12.07 -06:04:40.3: 14.49 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:05:12.07 -06:04:40.3: 99.00 +/- 99.00 edge
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,2461152.6091,12.44,0.05,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 20260422.1091 12.44CV 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 22.1091 2461152.6091 12.38 06:43:16.49 +00:21:47.9
211.67762 -1.65041 galactic Mon Second-epoch detections are separated by 1.6" and 6.3 pix
The object was found in VSX14" Gaia DR3 3125569957548660864
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.050 G 13.080 G F
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:43:16.49 +00:21:47.9: 15.05 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:43:16.49 +00:21:47.9: 99.00 +/- 99.00 edge
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 3125569957548660864,2461152.6091,12.38,0.05,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 3125569957548660864 20260422.1091 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 22.1091 2461152.6091 12.29 06:58:25.41 -02:40:33.6
216.10968 0.33257 galactic Mon Second-epoch detections are separated by 1.1" and 6.2 pix
The object was found in VSX 1" Gaia DR3 3108912390749031168
Type: E
# Max. Min./Amp. JD0 Period
13.320 G 13.390 G 1.907940000000 B
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:58:25.41 -02:40:33.6: 15.03 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:58:25.41 -02:40:33.6: 99.00 +/- 99.00 edge
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 3108912390749031168,2461152.6091,12.29,0.05,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
Gaia DR3 3108912390749031168 20260422.1091 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 22.1091 2461152.6091 12.29 07:03:47.18 -03:20:30.1
217.31416 1.21868 galactic Mon Second-epoch detections are separated by 0.9" and 6.2 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 J105.9536-03.3472 | 07:03:47.55 -03:20:09.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.151+/-0.037 (F)
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:03:47.18 -03:20:30.1: 14.90 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:03:47.18 -03:20:30.1: 99.00 +/- 99.00 edge
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 J105.9536-03.3472,2461152.6091,12.29,0.05,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 J105.9536-03.3472 20260422.1091 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 22.1091 2461152.6091 12.30 07:03:27.01 -05:01:13.8
218.76807 0.37488 galactic Mon Second-epoch detections are separated by 1.5" and 6.2 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_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:03:27.01 -05:01:13.8: 14.49 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:03:27.01 -05:01:13.8: 99.00 +/- 99.00 edge
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 3101503056772630528,2461152.6091,12.30,0.05,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 3101503056772630528 20260422.1091 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 22.1091 2461152.6091 12.38 07:00:51.92 +00:11:59.2
213.82919 2.18859 galactic Mon Second-epoch detections are separated by 0.5" and 6.3 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 | Gaia DR3 3112897600704147072 | 07:00:50.64 +00:11:45.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F3 (LAMOST DR5) J-Ks=0.324+/-0.036 (G)
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:00:51.92 +00:11:59.2: 15.06 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:00:51.92 +00:11:59.2: 99.00 +/- 99.00 edge
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 3112897600704147072,2461152.6091,12.38,0.05,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 3112897600704147072 20260422.1091 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 22.1091 2461152.6091 12.23 07:05:18.12 -01:23:00.0
215.74568 2.45197 galactic Mon Second-epoch detections are separated by 0.7" and 6.2 pix
The object was found in VSX19" Gaia DR3 3109471389332247552
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
14.540 G 14.570 G A
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:05:18.12 -01:23:00.0: 14.99 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:05:18.12 -01:23:00.0: 99.00 +/- 99.00 edge
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 3109471389332247552,2461152.6091,12.23,0.05,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 3109471389332247552 20260422.1091 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1091 2461152.6091 12.23 07:07:47.22 -05:40:38.7
219.84740 1.03219 galactic Mon Second-epoch detections are separated by 1.7" and 6.1 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 | target | 07:07:47.22 -05:40:38.7 (user input) | T | P | (position from user input) J-Ks=0.447+/-0.035 (G)
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:07:47.22 -05:40:38.7: 14.49 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:07:47.22 -05:40:38.7: 99.00 +/- 99.00 edge
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,2461152.6091,12.23,0.05,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 20260422.1091 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1091 2461152.6091 12.06 07:06:22.80 -01:49:60.0
216.26957 2.48546 galactic Mon Second-epoch detections are separated by 2.3" and 6.1 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 | ZTF J070621.56-015037.5 | 07:06:21.77 -01:50:14.0 (Gaia DR3) | EW (local) | 2458429.90290 (local) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:06:22.80 -01:49:60.0: 14.88 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:06:22.80 -01:49:60.0: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J070621.56-015037.5,2461152.6091,12.06,0.05,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
ZTF J070621.56-015037.5 20260422.1091 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 22.1091 2461152.6091 12.06 06:59:00.64 -01:40:01.6
215.27912 0.92386 galactic Mon Second-epoch detections are separated by 3.0" and 6.6 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 3112130214607270656 | 06:59:00.13 -01:39:46.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:59:00.64 -01:40:01.6: 14.63 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:59:00.64 -01:40:01.6: 99.00 +/- 99.00 edge
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 3112130214607270656,2461152.6091,12.06,0.05,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
Gaia DR3 3112130214607270656 20260422.1091 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 22.1091 2461152.6091 12.10 07:05:04.23 -05:27:55.4
219.34843 0.52929 galactic Mon Second-epoch detections are separated by 0.6" and 6.3 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 | Gaia DR3 3053389149496017280 | 07:05:05.64 -05:27:55.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.595+/-0.036 (K)
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:05:04.23 -05:27:55.4: 14.75 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:05:04.23 -05:27:55.4: 99.00 +/- 99.00 edge
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 3053389149496017280,2461152.6091,12.10,0.05,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 3053389149496017280 20260422.1091 12.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1091 2461152.6091 12.02 07:06:54.66 -04:13:51.4
218.46220 1.50341 galactic Mon Second-epoch detections are separated by 1.6" and 6.3 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 | Large-amplitude variable Gaia DR2 3107563977176844416 | 07:06:56.24 -04:13:48.6 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) SpType: A0 1949AnHar.112....1C HD 296299 J-Ks=0.073+/-0.041 (A)
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:06:54.66 -04:13:51.4: 14.88 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:06:54.66 -04:13:51.4: 99.00 +/- 99.00 edge
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
Large-amplitude variable Gaia DR2 3107563977176844416,2461152.6091,12.02,0.05,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
Large-amplitude variable Gaia DR2 3107563977176844416 20260422.1091 12.02CV 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 22.1091 2461152.6091 11.95 07:05:50.91 -02:05:14.1
216.43459 2.25111 galactic Mon Second-epoch detections are separated by 2.1" and 6.1 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 J106.4621-02.0972 | 07:05:50.77 -02:05:30.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.072+/-0.037 (A)
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:05:50.91 -02:05:14.1: 14.85 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:05:50.91 -02:05:14.1: 99.00 +/- 99.00 edge
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 J106.4621-02.0972,2461152.6091,11.95,0.05,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 J106.4621-02.0972 20260422.1091 11.95CV 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 22.1091 2461152.6091 12.05 06:57:16.40 -00:59:39.3
214.48214 0.84472 galactic Mon Second-epoch detections are separated by 1.3" and 6.3 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 | Gaia DR3 3112231300951646592 | 06:57:17.75 -00:59:30.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F8 1956ApJS....2..271M LF 9 -01 387
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:57:16.40 -00:59:39.3: 15.07 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:57:16.40 -00:59:39.3: 99.00 +/- 99.00 edge
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 3112231300951646592,2461152.6091,12.05,0.05,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 3112231300951646592 20260422.1091 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 22.1091 2461152.6091 12.03 07:03:38.51 -02:31:49.4
216.57619 1.55815 galactic Mon Second-epoch detections are separated by 1.1" and 6.4 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 3108824601619113600 | 07:03:37.83 -02:32:05.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: N 1989PW&SO...3...53S CGCS 1523 J-Ks=0.910+/- (M)
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:03:38.51 -02:31:49.4: 13.91 +/- 0.16 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:03:38.51 -02:31:49.4: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 13.91 +/- 0.16
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 3108824601619113600,2461152.6091,12.03,0.05,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 3108824601619113600 20260422.1091 12.03CV 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 22.1091 2461152.6091 12.10 06:44:34.00 -01:35:29.5
213.56580 -2.25421 galactic Mon Second-epoch detections are separated by 1.7" and 6.1 pix
The object was found in VSX 2" Gaia DR3 3107032775621691520
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.270 G 13.300 G A
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:44:34.00 -01:35:29.5: 13.71 +/- 0.10 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:44:34.00 -01:35:29.5: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 13.71 +/- 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 3107032775621691520,2461152.6091,12.10,0.05,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 3107032775621691520 20260422.1091 12.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1091 2461152.6091 12.03 07:01:00.94 -00:25:45.2
214.40640 1.93499 galactic Mon Second-epoch detections are separated by 0.8" and 6.2 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 J105.2433-00.4249 | 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_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:01:00.94 -00:25:45.2: 14.24 +/- 0.18 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:01:00.94 -00:25:45.2: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 14.24 +/- 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
ATO J105.2433-00.4249,2461152.6091,12.03,0.05,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 20260422.1091 12.03CV 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 22.1091 2461152.6091 11.99 06:52:10.08 +00:34:37.5
212.50153 0.42557 galactic Mon Second-epoch detections are separated by 1.3" and 6.4 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 | ATO J103.0397+00.5734 | 06:52:10.08 +00:34:37.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G9 (LAMOST DR5) J-Ks=0.180+/-0.038 (F)
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:52:10.08 +00:34:37.5: 14.79 +/- 0.30 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:52:10.08 +00:34:37.5: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 14.79 +/- 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
ATO J103.0397+00.5734,2461152.6091,11.99,0.05,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 J103.0397+00.5734 20260422.1091 11.99CV 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 22.1091 2461152.6091 11.87 07:07:48.03 +00:24:43.0
214.43245 3.82812 galactic Mon Second-epoch detections are separated by 3.5" and 6.5 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 | ATO J106.9514+00.4118 | 07:07:47.15 +00:24:53.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:07:48.03 +00:24:43.0: 15.00 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:07:48.03 +00:24:43.0: 99.00 +/- 99.00 edge
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 J106.9514+00.4118,2461152.6091,11.87,0.05,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 J106.9514+00.4118 20260422.1091 11.87CV 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 22.1091 2461152.6091 11.90 06:57:47.57 -01:31:07.0
215.00801 0.72091 galactic Mon Second-epoch detections are separated by 1.4" and 6.4 pix
The object was found in VSX 2" Gaia DR3 3112151242766551808
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.070 G 13.100 G A
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:57:47.57 -01:31:07.0: 14.95 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:57:47.57 -01:31:07.0: 99.00 +/- 99.00 edge
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 3112151242766551808,2461152.6091,11.90,0.05,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 3112151242766551808 20260422.1091 11.90CV 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 22.1091 2461152.6091 11.79 07:02:21.31 -04:03:31.7
217.78817 0.57285 galactic Mon Second-epoch detections are separated by 1.4" and 6.3 pix
The object was found in VSX 2" Gaia DR3 3101821880779349888
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.760 G 12.780 G B
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:02:21.31 -04:03:31.7: 14.95 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:02:21.31 -04:03:31.7: 99.00 +/- 99.00 edge
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 3101821880779349888,2461152.6091,11.79,0.05,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 3101821880779349888 20260422.1091 11.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1091 2461152.6091 11.68 06:54:34.42 -00:35:22.5
213.81412 0.42880 galactic Mon Second-epoch detections are separated by 0.6" and 6.3 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 J103.6522-00.6011 | 06:54:35.48 -00:35:37.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G5: 1956ApJS....2..271M LF 9 -01 297 J-Ks=0.117+/-0.033 (A)
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:54:34.42 -00:35:22.5: 14.82 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:54:34.42 -00:35:22.5: 99.00 +/- 99.00 edge
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 J103.6522-00.6011,2461152.6091,11.68,0.05,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 J103.6522-00.6011 20260422.1091 11.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1091 2461152.6091 11.63 06:40:55.24 +00:01:26.5
211.71093 -2.32892 galactic Mon Second-epoch detections are separated by 1.0" and 6.1 pix
The object was found in VSX19" GDS_J0640542+000137
Type: VAR
# Max. Min./Amp. JD0 Period
11.250 r Y 0.170 r
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:40:55.24 +00:01:26.5: 14.62 +/- 0.28 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:40:55.24 +00:01:26.5: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 14.62 +/- 0.28
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GDS_J0640542+000137,2461152.6091,11.63,0.05,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
GDS_J0640542+000137 20260422.1091 11.63CV 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 22.1091 2461152.6091 10.95 07:08:39.11 -02:25:42.0
217.05937 2.71708 galactic Mon Second-epoch detections are separated by 1.0" and 6.2 pix
The object was found in VSX17" Gaia DR3 3108418465213525888
Type: ROT
# Max. Min./Amp. JD0 Period
12.410 G 12.440 G K
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:08:39.11 -02:25:42.0: 14.70 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:08:39.11 -02:25:42.0: 99.00 +/- 99.00 edge
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 3108418465213525888,2461152.6091,10.95,0.05,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 3108418465213525888 20260422.1091 10.95CV 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 22.1091 2461152.6091 11.74 07:06:17.15 +02:00:15.3
212.83865 4.21681 galactic Mon Second-epoch detections are separated by 0.3" and 6.3 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 J106.5593+02.0025 | 07:06:15.52 +02:00:25.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A7 1949AnHar.112....1C HD 289613 J-Ks=0.212+/-0.030 (F)
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:06:17.15 +02:00:15.3: 14.81 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:06:17.15 +02:00:15.3: 99.00 +/- 99.00 edge
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 J106.5593+02.0025,2461152.6091,11.74,0.05,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 J106.5593+02.0025 20260422.1091 11.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1091 2461152.6091 11.87 06:48:50.52 -00:08:31.2
212.76237 -0.64233 galactic Mon Second-epoch detections are separated by 0.7" and 6.3 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 J102.2107-00.1428 | 06:48:50.52 -00:08:31.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:48:50.52 -00:08:31.2: 14.80 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:48:50.52 -00:08:31.2: 99.00 +/- 99.00 edge
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 J102.2107-00.1428,2461152.6091,11.87,0.05,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 J102.2107-00.1428 20260422.1091 11.87CV 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 22.1091 2461152.6091 12.15 06:51:05.09 -01:41:34.8
214.39854 -0.85043 galactic Mon Second-epoch detections are separated by 0.7" and 6.2 pix
The object was found in VSX 6" Gaia DR3 3106324999372001664
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.900 G 13.930 G B
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:51:05.09 -01:41:34.8: 14.97 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:51:05.09 -01:41:34.8: 99.00 +/- 99.00 edge
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 3106324999372001664,2461152.6091,12.15,0.05,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
Gaia DR3 3106324999372001664 20260422.1091 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 22.1091 2461152.6091 12.29 06:49:33.17 -01:23:31.3
213.95609 -1.05404 galactic Mon Second-epoch detections are separated by 1.0" and 6.4 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 | ATO J102.3878-01.3922 | 06:49:33.17 -01:23:31.3 (user input) | IRR (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.321+/-0.034 (F)
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:49:33.17 -01:23:31.3: 14.93 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:49:33.17 -01:23:31.3: 99.00 +/- 99.00 edge
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 J102.3878-01.3922,2461152.6091,12.29,0.05,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 J102.3878-01.3922 20260422.1091 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 22.1091 2461152.6091 12.45 07:02:17.59 -03:14:33.0
217.05528 0.93279 galactic Mon Second-epoch detections are separated by 2.3" and 6.5 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 | Gaia DR3 3108624627942178688 | 07:02:18.89 -03:14:57.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.630+/-0.030 (K)
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:02:17.59 -03:14:33.0: 14.90 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:02:17.59 -03:14:33.0: 99.00 +/- 99.00 edge
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 3108624627942178688,2461152.6091,12.45,0.05,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 3108624627942178688 20260422.1091 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 22.1091 2461152.6091 12.36 07:03:52.65 -06:00:24.6
219.69341 0.01722 galactic Mon Second-epoch detections are separated by 1.4" and 6.2 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 J105.9816-06.0164 | 07:03:55.68 -06:00:34.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.228+/-0.036 (F)
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:03:52.65 -06:00:24.6: 14.67 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:03:52.65 -06:00:24.6: 99.00 +/- 99.00 edge
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 J105.9816-06.0164,2461152.6091,12.36,0.05,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 J105.9816-06.0164 20260422.1091 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1091 2461152.6091 12.34 06:57:11.84 -03:58:12.7
217.12133 -0.53066 galactic Mon Second-epoch detections are separated by 1.9" and 6.5 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 | ATO J104.2896-03.9733 | 06:57:10.73 -03:58:39.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: B9 1949AnHar.112....1C HD 295858 J-Ks=0.342+/-0.033 (G)
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:57:11.84 -03:58:12.7: 14.92 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:57:11.84 -03:58:12.7: 99.00 +/- 99.00 edge
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 J104.2896-03.9733,2461152.6091,12.34,0.05,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 J104.2896-03.9733 20260422.1091 12.34CV 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 22.1091 2461152.6091 12.38 06:52:57.33 -03:04:56.9
215.84847 -1.06778 galactic Mon Second-epoch detections are separated by 1.1" and 6.3 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 | target | 06:52:57.33 -03:04:56.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:52:57.33 -03:04:56.9: 14.96 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:52:57.33 -03:04:56.9: 99.00 +/- 99.00 edge
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,2461152.6091,12.38,0.05,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
target 20260422.1091 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 22.1091 2461152.6091 12.30 06:59:52.78 -04:47:26.6
218.15670 -0.31067 galactic Mon Second-epoch detections are separated by 0.5" and 6.3 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 | 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_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:59:52.78 -04:47:26.6: 14.40 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:59:52.78 -04:47:26.6: 99.00 +/- 99.00 edge
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 3101628912187905408,2461152.6091,12.30,0.05,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 20260422.1091 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 22.1091 2461152.6091 12.37 06:58:45.60 -02:28:56.6
215.97583 0.49577 galactic Mon Second-epoch detections are separated by 1.1" and 6.0 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 3108924004342074112 | 06:58:45.38 -02:29:20.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.394+/-0.050 (G)
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:58:45.60 -02:28:56.6: 14.82 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:58:45.60 -02:28:56.6: 99.00 +/- 99.00 edge
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 3108924004342074112,2461152.6091,12.37,0.05,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 3108924004342074112 20260422.1091 12.37CV 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 22.1091 2461152.6091 12.39 07:00:01.21 -05:09:19.3
218.49701 -0.44624 galactic Mon Second-epoch detections are separated by 0.9" and 6.1 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 J105.0068-05.1648 | 07:00:02.06 -05:09:45.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.330+/-0.033 (G)
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:00:01.21 -05:09:19.3: 14.81 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:00:01.21 -05:09:19.3: 99.00 +/- 99.00 edge
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 J105.0068-05.1648,2461152.6091,12.39,0.05,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
ATO J105.0068-05.1648 20260422.1091 12.39CV 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 22.1091 2461152.6091 12.51 06:56:22.04 -00:53:11.9
214.28303 0.69230 galactic Mon Second-epoch detections are separated by 1.5" and 6.1 pix
The object was found in VSX 2" Gaia DR3 3112424230887731712
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.560 G 13.590 G B
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:56:22.04 -00:53:11.9: 14.80 +/- 0.27 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:56:22.04 -00:53:11.9: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 14.80 +/- 0.27
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 3112424230887731712,2461152.6091,12.51,0.05,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 3112424230887731712 20260422.1091 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 22.1091 2461152.6091 12.49 07:04:10.05 -05:04:53.6
218.90423 0.50565 galactic Mon Second-epoch detections are separated by 0.6" and 6.4 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 | ATO J106.0471-05.0754 | 07:04:11.96 -05:04:54.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:04:10.05 -05:04:53.6: 14.87 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:04:10.05 -05:04:53.6: 99.00 +/- 99.00 edge
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 J106.0471-05.0754,2461152.6091,12.49,0.05,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 J106.0471-05.0754 20260422.1091 12.49CV 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 22.1091 2461152.6091 12.56 06:48:48.44 +00:23:30.4
212.28335 -0.40663 galactic Mon Second-epoch detections are separated by 0.8" and 6.2 pix
The object was found in VSX 2" Gaia DR3 3113610294697190784
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.590 G 13.610 G F
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:48:48.44 +00:23:30.4: 14.97 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:48:48.44 +00:23:30.4: 99.00 +/- 99.00 edge
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 3113610294697190784,2461152.6091,12.56,0.05,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 3113610294697190784 20260422.1091 12.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1091 2461152.6091 12.80 06:44:24.88 -00:04:50.0
212.20281 -1.59935 galactic Mon Second-epoch detections are separated by 1.0" and 6.1 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 | Large-amplitude variable Gaia DR2 3119491273155424256 | 06:44:24.88 -00:04:50.0 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.240+/-0.043 (F)
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:44:24.88 -00:04:50.0: 14.90 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:44:24.88 -00:04:50.0: 99.00 +/- 99.00 edge
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
Large-amplitude variable Gaia DR2 3119491273155424256,2461152.6091,12.80,0.05,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
Large-amplitude variable Gaia DR2 3119491273155424256 20260422.1091 12.80CV 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 22.1091 2461152.6091 12.64 06:44:39.61 +00:10:06.3
212.00918 -1.43116 galactic Mon Second-epoch detections are separated by 2.2" and 6.5 pix
The object was found in VSX 7" Gaia DR3 3125504223071142784
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
14.400 G 14.420 G F
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:44:39.61 +00:10:06.3: 14.39 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:44:39.61 +00:10:06.3: 99.00 +/- 99.00 edge
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 3125504223071142784,2461152.6091,12.64,0.05,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
Gaia DR3 3125504223071142784 20260422.1091 12.64CV 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 22.1091 2461152.6091 12.57 07:08:43.09 -05:05:29.5
219.43379 1.50758 galactic Mon Second-epoch detections are separated by 0.6" and 6.2 pix
The object was found in VSX19" Gaia DR3 3053416980884797824
Type: RS
# Max. Min./Amp. JD0 Period
15.430 G 15.530 G
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:08:43.09 -05:05:29.5: 14.86 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:08:43.09 -05:05:29.5: 99.00 +/- 99.00 edge
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 3053416980884797824,2461152.6091,12.57,0.05,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
Gaia DR3 3053416980884797824 20260422.1091 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 22.1091 2461152.6091 12.54 07:07:48.91 -05:43:38.0
219.89485 1.01549 galactic Mon Second-epoch detections are separated by 1.2" and 6.5 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 | ATO J106.9437-05.7308 | 07:07:48.10 -05:43:12.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:07:48.91 -05:43:38.0: 14.65 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:07:48.91 -05:43:38.0: 99.00 +/- 99.00 edge
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 J106.9437-05.7308,2461152.6091,12.54,0.05,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
ATO J106.9437-05.7308 20260422.1091 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 22.1091 2461152.6091 12.71 07:02:14.45 -03:05:58.9
216.92231 0.98654 galactic Mon Second-epoch detections are separated by 0.6" and 6.2 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 J105.5594-03.0943 | 07:02:13.15 -03:05:39.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.228+/-0.037 (F)
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:02:14.45 -03:05:58.9: 14.96 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:02:14.45 -03:05:58.9: 99.00 +/- 99.00 edge
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 J105.5594-03.0943,2461152.6091,12.71,0.05,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
ATO J105.5594-03.0943 20260422.1091 12.71CV 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 22.1091 2461152.6091 12.69 06:58:50.14 -04:41:12.9
217.94550 -0.49459 galactic Mon Second-epoch detections are separated by 1.4" and 6.5 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 | 06:58:50.14 -04:41:12.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:58:50.14 -04:41:12.9: 14.86 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:58:50.14 -04:41:12.9: 99.00 +/- 99.00 edge
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,2461152.6091,12.69,0.05,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
target 20260422.1091 12.69CV 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
Mean magnitude and position on the discovery images:
2026 04 22.1091 2461152.6091 12.71 06:56:02.56 -03:13:02.6
216.31999 -0.44345 galactic Mon Second-epoch detections are separated by 2.0" and 6.5 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 | 06:56:02.56 -03:13:02.6 (user input) | T | P | (position from user input) J-Ks=0.190+/-0.035 (F)
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:56:02.56 -03:13:02.6: 13.59 +/- 0.11 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:56:02.56 -03:13:02.6: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 13.59 +/- 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,2461152.6091,12.71,0.05,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
target 20260422.1091 12.71CV 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 22.1091 2461152.6091 12.68 06:56:49.00 +00:46:32.6
212.85457 1.55043 galactic Mon Second-epoch detections are separated by 3.1" and 6.4 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 | ATO J104.2021+00.7657 | 06:56:49.00 +00:46:32.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:56:49.00 +00:46:32.6: 15.05 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:56:49.00 +00:46:32.6: 99.00 +/- 99.00 edge
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 J104.2021+00.7657,2461152.6091,12.68,0.05,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 J104.2021+00.7657 20260422.1091 12.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1091 2461152.6091 12.71 06:48:30.53 +00:57:43.9
211.74167 -0.21288 galactic Mon Second-epoch detections are separated by 2.2" and 6.0 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 | 06:48:30.53 +00:57:43.9 (user input) | T | P | (position from user input) J-Ks=0.268+/-0.043 (F)
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:48:30.53 +00:57:43.9: 14.86 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:48:30.53 +00:57:43.9: 99.00 +/- 99.00 edge
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,2461152.6091,12.71,0.05,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
target 20260422.1091 12.71CV 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 22.1091 2461152.6091 12.75 07:06:11.94 +00:18:33.4
214.34084 3.42504 galactic Mon Second-epoch detections are separated by 1.1" and 6.4 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 | ATO J106.5494+00.3110 | 07:06:11.94 +00:18:33.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.393+/-0.035 (G)
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:06:11.94 +00:18:33.4: 14.92 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:06:11.94 +00:18:33.4: 99.00 +/- 99.00 edge
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 J106.5494+00.3110,2461152.6091,12.75,0.05,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 J106.5494+00.3110 20260422.1091 12.75CV 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 22.1091 2461152.6091 12.76 06:57:07.69 +00:36:02.2
213.04599 1.53991 galactic Mon Second-epoch detections are separated by 2.8" and 6.2 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 3113732748502887296 | 06:57:05.66 +00:36:32.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K5 1956ApJS....2..271M LF 9 +00 356
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:57:07.69 +00:36:02.2: 14.52 +/- 0.25 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:57:07.69 +00:36:02.2: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 14.52 +/- 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 3113732748502887296,2461152.6091,12.76,0.05,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 3113732748502887296 20260422.1091 12.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1091 2461152.6091 12.77 06:59:33.41 +01:05:00.1
212.89293 2.30032 galactic Mon Second-epoch detections are separated by 0.4" and 6.2 pix
The object was found in VSX 1" Gaia DR3 3113847342532829952
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.790 G 13.820 G A
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:59:33.41 +01:05:00.1: 14.97 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:59:33.41 +01:05:00.1: 99.00 +/- 99.00 edge
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 3113847342532829952,2461152.6091,12.77,0.05,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 3113847342532829952 20260422.1091 12.77CV 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 22.1091 2461152.6091 12.72 06:57:09.41 -01:07:39.1
214.58745 0.75798 galactic Mon Second-epoch detections are separated by 3.0" and 6.2 pix
The object was found in VSX 2" Gaia DR3 3112223290836561024
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.840 G 13.870 G F
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:57:09.41 -01:07:39.1: 15.00 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:57:09.41 -01:07:39.1: 99.00 +/- 99.00 edge
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 3112223290836561024,2461152.6091,12.72,0.05,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 3112223290836561024 20260422.1091 12.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1091 2461152.6091 12.78 06:57:24.09 -02:57:03.8
216.23784 -0.02007 galactic Mon Second-epoch detections are separated by 0.5" and 6.2 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 J104.3550-02.9498 | 06:57:24.09 -02:57:03.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:57:24.09 -02:57:03.8: 15.06 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:57:24.09 -02:57:03.8: 99.00 +/- 99.00 edge
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 J104.3550-02.9498,2461152.6091,12.78,0.05,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
ATO J104.3550-02.9498 20260422.1091 12.78CV 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 22.1091 2461152.6091 12.78 07:04:16.73 -03:01:39.2
217.09118 1.47187 galactic Mon Second-epoch detections are separated by 2.7" and 5.9 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 J106.0676-03.0161 | 07:04:16.73 -03:01:39.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:04:16.73 -03:01:39.2: 14.81 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:04:16.73 -03:01:39.2: 99.00 +/- 99.00 edge
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 J106.0676-03.0161,2461152.6091,12.78,0.05,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
ATO J106.0676-03.0161 20260422.1091 12.78CV 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 22.1091 2461152.6091 12.78 06:57:12.35 -03:57:46.0
217.11570 -0.52539 galactic Mon Second-epoch detections are separated by 7.9" and 7.2 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 J104.2998-03.9607 | 06:57:12.35 -03:57:46.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:57:12.35 -03:57:46.0: 14.92 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:57:12.35 -03:57:46.0: 99.00 +/- 99.00 edge
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 J104.2998-03.9607,2461152.6091,12.78,0.05,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
ATO J104.2998-03.9607 20260422.1091 12.78CV 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 22.1091 2461152.6091 12.78 07:04:56.05 -05:21:48.3
219.24226 0.54595 galactic Mon Second-epoch detections are separated by 1.8" and 6.0 pix
The object was found in VSX 2" Gaia DR3 3053393715036723840
Type: ROT
# Max. Min./Amp. JD0 Period
13.940 G 13.960 G K
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:04:56.05 -05:21:48.3: 14.74 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:04:56.05 -05:21:48.3: 99.00 +/- 99.00 edge
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 3053393715036723840,2461152.6091,12.78,0.05,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 3053393715036723840 20260422.1091 12.78CV 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 22.1091 2461152.6091 12.74 06:58:35.36 -04:20:30.2
217.61037 -0.39152 galactic Mon Second-epoch detections are separated by 1.0" and 6.2 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 J104.6490-04.3421 | 06:58:35.36 -04:20:30.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:58:35.36 -04:20:30.2: 14.75 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:58:35.36 -04:20:30.2: 99.00 +/- 99.00 edge
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 J104.6490-04.3421,2461152.6091,12.74,0.05,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 J104.6490-04.3421 20260422.1091 12.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1091 2461152.6091 12.82 06:51:18.23 -01:23:09.2
214.15011 -0.66172 galactic Mon Second-epoch detections are separated by 1.2" and 6.2 pix
The object was found in VSX 2" Gaia DR3 3106340014576032512
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
14.050 G 14.070 G F
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:51:18.23 -01:23:09.2: 14.91 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:51:18.23 -01:23:09.2: 99.00 +/- 99.00 edge
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 3106340014576032512,2461152.6091,12.82,0.05,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 3106340014576032512 20260422.1091 12.82CV 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 22.1091 2461152.6091 12.90 06:58:22.44 -02:33:53.3
216.00511 0.37236 galactic Mon Second-epoch detections are separated by 2.4" and 6.4 pix
The object was found in VSX 3" Gaia DR3 3108917372911018368
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
14.130 G 14.170 G A
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:58:22.44 -02:33:53.3: 14.84 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:58:22.44 -02:33:53.3: 99.00 +/- 99.00 edge
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 3108917372911018368,2461152.6091,12.90,0.05,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 3108917372911018368 20260422.1091 12.90CV 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 22.1091 2461152.6091 12.86 06:46:50.64 +01:18:07.4
211.24940 -0.42814 galactic Mon Second-epoch detections are separated by 0.6" and 6.3 pix
The object was found in VSX13" MGAB-V1900
Type: YSO
# Max. Min./Amp. JD0 Period
17.600 r 18.900 r
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:46:50.64 +01:18:07.4: 15.10 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:46:50.64 +01:18:07.4: 99.00 +/- 99.00 edge
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
MGAB-V1900,2461152.6091,12.86,0.05,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
MGAB-V1900 20260422.1091 12.86CV 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 22.1091 2461152.6091 12.89 06:54:41.81 -02:41:58.2
215.70582 -0.50621 galactic Mon Second-epoch detections are separated by 2.7" and 6.6 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 3105947282767695360 | 06:54:39.76 -02:41:53.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: B5 1956ApJS....2..271M LF 9 -03 284
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:54:41.81 -02:41:58.2: 15.05 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:54:41.81 -02:41:58.2: 99.00 +/- 99.00 edge
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 3105947282767695360,2461152.6091,12.89,0.05,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 3105947282767695360 20260422.1091 12.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1091 2461152.6091 12.95 06:48:34.35 +01:51:39.4
210.94912 0.21122 galactic Mon Second-epoch detections are separated by 2.4" and 6.5 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 | ATO J102.1314+01.8533 | 06:48:32.15 +01:51:48.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A1V (LAMOST DR5)
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:48:34.35 +01:51:39.4: 15.01 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:48:34.35 +01:51:39.4: 99.00 +/- 99.00 edge
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 J102.1314+01.8533,2461152.6091,12.95,0.05,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 J102.1314+01.8533 20260422.1091 12.95CV 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 22.1091 2461152.6091 12.96 06:54:49.49 -01:15:54.9
214.44405 0.17648 galactic Mon Second-epoch detections are separated by 1.0" and 6.3 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 J103.7112-01.2754 | 06:54:49.49 -01:15:54.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.334+/-0.038 (G)
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:54:49.49 -01:15:54.9: 14.63 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:54:49.49 -01:15:54.9: 99.00 +/- 99.00 edge
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 J103.7112-01.2754,2461152.6091,12.96,0.05,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 J103.7112-01.2754 20260422.1091 12.96CV 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 22.1091 2461152.6091 12.86 06:59:43.78 +00:17:12.0
213.62222 1.97557 galactic Mon Second-epoch detections are separated by 3.8" and 6.7 pix
The object was found in VSX 3" Gaia DR3 3112948251257159808
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.860 G 13.890 G B
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:59:43.78 +00:17:12.0: 15.06 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:59:43.78 +00:17:12.0: 99.00 +/- 99.00 edge
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 3112948251257159808,2461152.6091,12.86,0.05,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 3112948251257159808 20260422.1091 12.86CV 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 22.1091 2461152.6091 12.95 07:07:56.30 -01:30:30.4
216.15903 2.98045 galactic Mon Second-epoch detections are separated by 1.0" and 6.3 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 J106.9991-01.5167 | 07:07:57.91 -01:30:39.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.600+/-0.033 (K)
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:07:56.30 -01:30:30.4: 14.89 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:07:56.30 -01:30:30.4: 99.00 +/- 99.00 edge
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 J106.9991-01.5167,2461152.6091,12.95,0.05,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 J106.9991-01.5167 20260422.1091 12.95CV 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 22.1091 2461152.6091 13.11 06:50:44.76 -00:05:16.4
212.93126 -0.19403 galactic Mon Second-epoch detections are separated by 6.9" and 6.3 pix
The object was found in VSX10" Gaia DR3 3113252403663988096
Type: RS
# Max. Min./Amp. JD0 Period
15.320 G 15.380 G K
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:50:44.76 -00:05:16.4: 14.83 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:50:44.76 -00:05:16.4: 99.00 +/- 99.00 edge
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 3113252403663988096,2461152.6091,13.11,0.05,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 3113252403663988096 20260422.1091 13.11CV 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 22.1091 2461152.6091 12.94 06:48:45.22 +01:09:18.8
211.59781 -0.07038 galactic Mon Second-epoch detections are separated by 2.1" and 6.4 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 | ATO J102.1800+01.1786 | 06:48:44.22 +01:10:02.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.235+/-0.046 (F)
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:48:45.22 +01:09:18.8: 14.80 +/- 0.36 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:48:45.22 +01:09:18.8: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 14.80 +/- 0.36
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 J102.1800+01.1786,2461152.6091,12.94,0.05,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
ATO J102.1800+01.1786 20260422.1091 12.94CV 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 22.1091 2461152.6091 12.81 06:49:56.14 -02:40:54.9
215.14823 -1.55653 galactic Mon Second-epoch detections are separated by 2.6" and 6.3 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 | Gaia DR3 3105921684761121152 | 06:49:58.35 -02:41:03.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A2 1949AnHar.112....1C HD 295506
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:49:56.14 -02:40:54.9: 14.91 +/- 0.35 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:49:56.14 -02:40:54.9: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 14.91 +/- 0.35
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 3105921684761121152,2461152.6091,12.81,0.05,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
Gaia DR3 3105921684761121152 20260422.1091 12.81CV 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 22.1091 2461152.6091 12.88 06:49:07.39 -01:40:18.4
214.15621 -1.27710 galactic Mon Second-epoch detections are separated by 1.1" and 6.3 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 | target | 06:49:07.39 -01:40:18.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:49:07.39 -01:40:18.4: 14.09 +/- 0.20 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:49:07.39 -01:40:18.4: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 14.09 +/- 0.20
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,2461152.6091,12.88,0.05,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 20260422.1091 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1091 2461152.6091 12.95 06:50:00.96 -03:51:50.3
216.21042 -2.07668 galactic Mon Second-epoch detections are separated by 2.2" and 6.5 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 | ATO J102.4997-03.8557 | 06:49:57.92 -03:51:46.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.382+/-0.034 (G)
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:50:00.96 -03:51:50.3: 14.69 +/- 0.29 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:50:00.96 -03:51:50.3: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 14.69 +/- 0.29
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 J102.4997-03.8557,2461152.6091,12.95,0.05,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 J102.4997-03.8557 20260422.1091 12.95CV 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 22.1091 2461152.6091 12.95 06:53:06.38 -01:03:37.0
214.06573 -0.11229 galactic Mon Second-epoch detections are separated by 2.8" and 6.6 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 J103.2794-01.0604 | 06:53:05.51 -01:04:12.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:53:06.38 -01:03:37.0: 14.55 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:53:06.38 -01:03:37.0: 99.00 +/- 99.00 edge
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 J103.2794-01.0604,2461152.6091,12.95,0.05,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 J103.2794-01.0604 20260422.1091 12.95CV 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 22.1091 2461152.6091 12.93 06:52:51.68 -02:22:45.6
215.21182 -0.76822 galactic Mon Second-epoch detections are separated by 2.3" and 6.6 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 J103.2108-02.3799 | 06:52:51.68 -02:22:45.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:52:51.68 -02:22:45.6: 14.99 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:52:51.68 -02:22:45.6: 99.00 +/- 99.00 edge
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 J103.2108-02.3799,2461152.6091,12.93,0.05,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 J103.2108-02.3799 20260422.1091 12.93CV 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 22.1091 2461152.6091 13.03 06:51:37.26 +01:28:59.1
211.63279 0.71693 galactic Mon Second-epoch detections are separated by 2.1" and 6.2 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 3126072571803216256 | 06:51:37.91 +01:28:26.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.379+/-0.052 (G)
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:51:37.26 +01:28:59.1: 14.98 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:51:37.26 +01:28:59.1: 99.00 +/- 99.00 edge
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 3126072571803216256,2461152.6091,13.03,0.05,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 3126072571803216256 20260422.1091 13.03CV 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 22.1091 2461152.6091 13.06 07:01:22.89 -05:01:12.6
218.53183 -0.08295 galactic Mon Second-epoch detections are separated by 0.5" and 6.1 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 3101421727271429888 | 07:01:24.11 -05:00:45.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:01:22.89 -05:01:12.6: 14.99 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:01:22.89 -05:01:12.6: 99.00 +/- 99.00 edge
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 3101421727271429888,2461152.6091,13.06,0.05,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
Gaia DR3 3101421727271429888 20260422.1091 13.06CV 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 22.1091 2461152.6091 12.94 06:59:44.33 -01:15:44.8
215.00218 1.27057 galactic Mon Second-epoch detections are separated by 1.7" and 6.2 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 J104.9279-01.2566 | 06:59:44.33 -01:15:44.8 (user input) | NSINE (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:59:44.33 -01:15:44.8: 14.96 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:59:44.33 -01:15:44.8: 99.00 +/- 99.00 edge
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 J104.9279-01.2566,2461152.6091,12.94,0.05,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
ATO J104.9279-01.2566 20260422.1091 12.94CV 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 22.1091 2461152.6091 12.95 07:05:38.49 +01:26:02.4
213.27418 3.81387 galactic Mon Second-epoch detections are separated by 2.4" and 6.1 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 | target | 07:05:38.49 +01:26:02.4 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=0.224+/-0.039 (F)
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:05:38.49 +01:26:02.4: 14.98 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:05:38.49 +01:26:02.4: 99.00 +/- 99.00 edge
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,2461152.6091,12.95,0.05,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 20260422.1091 12.95CV 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 22.1091 2461152.6091 13.02 06:53:41.40 -00:33:48.6
213.69016 0.24411 galactic Mon Second-epoch detections are separated by 0.9" and 6.1 pix
The object was found in VSX 2" Gaia DR3 3112503842401083904
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
14.010 G 14.040 G A
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:53:41.40 -00:33:48.6: 14.95 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:53:41.40 -00:33:48.6: 99.00 +/- 99.00 edge
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 3112503842401083904,2461152.6091,13.02,0.05,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 3112503842401083904 20260422.1091 13.02CV 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 22.1091 2461152.6091 13.10 06:38:52.43 +01:12:24.1
210.42411 -2.24383 galactic Mon Second-epoch detections are separated by 1.6" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.391 Ingeborg 410 -370 552 16.1 -0 0
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:38:52.43 +01:12:24.1: 14.94 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:38:52.43 +01:12:24.1: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461152.6091,13.10,0.05,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
VARIABLE_NAME 20260422.1091 13.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1091 2461152.6091 13.24 06:55:11.64 +00:56:23.6
212.52346 1.26422 galactic Mon Second-epoch detections are separated by 0.6" and 6.3 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 J103.7913+00.9506 | 06:55:10.02 +00:56:20.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.464+/-0.069 (G)
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:55:11.64 +00:56:23.6: 15.00 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:55:11.64 +00:56:23.6: 99.00 +/- 99.00 edge
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 J103.7913+00.9506,2461152.6091,13.24,0.05,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 J103.7913+00.9506 20260422.1091 13.24CV 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 22.1091 2461152.6091 13.12 07:01:34.77 -00:37:08.1
214.63966 1.97378 galactic Mon Second-epoch detections are separated by 1.3" and 6.3 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 | target | 07:01:34.77 -00:37:08.1 (user input) | T | P | (position from user input) J-Ks=0.651+/-0.037 (K)
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:01:34.77 -00:37:08.1: 14.99 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:01:34.77 -00:37:08.1: 99.00 +/- 99.00 edge
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,2461152.6091,13.12,0.05,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
target 20260422.1091 13.12CV 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 22.1091 2461152.6091 13.21 06:47:46.40 -02:22:20.5
214.62649 -1.89642 galactic Mon Second-epoch detections are separated by 0.9" and 6.2 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 | 06:47:46.40 -02:22:20.5 (user input) | T | P | (position from user input) J-Ks=0.108+/-0.044 (A)
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:47:46.40 -02:22:20.5: 15.02 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:47:46.40 -02:22:20.5: 99.00 +/- 99.00 edge
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,2461152.6091,13.21,0.05,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 20260422.1091 13.21CV 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 22.1091 2461152.6091 13.18 06:39:28.94 +00:31:16.8
211.10379 -2.42177 galactic Mon Second-epoch detections are separated by 2.1" and 6.5 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 | Gaia DR3 3119761851794078976 | 06:39:30.98 +00:31:50.9 (Gaia DR3) | ACV/roAm/ (local) | (local) | Gaia3var=VARIABLE SpType: A2 1949AnHar.112....1C HD 47611 J-Ks=0.416+/-0.168 (G)
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:39:28.94 +00:31:16.8: 14.88 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:39:28.94 +00:31:16.8: 99.00 +/- 99.00 edge
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 3119761851794078976,2461152.6091,13.18,0.05,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 3119761851794078976 20260422.1091 13.18CV 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 22.1091 2461152.6091 13.25 06:41:21.30 -00:35:23.5
212.30728 -2.51235 galactic Mon Second-epoch detections are separated by 3.5" and 6.6 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 3119355071151771648 | 06:41:20.76 -00:34:55.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K3III 2012A&A...543A.125G CoRoT 102596544 J-Ks=0.357+/-0.052 (G)
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:41:21.30 -00:35:23.5: 14.96 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:41:21.30 -00:35:23.5: 99.00 +/- 99.00 edge
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 3119355071151771648,2461152.6091,13.25,0.05,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
Gaia DR3 3119355071151771648 20260422.1091 13.25CV 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 22.1091 2461152.6091 13.21 06:51:51.87 -04:03:49.1
216.59821 -1.75700 galactic Mon Second-epoch detections are separated by 1.5" and 6.4 pix
The object was found in VSX 1" CoRoT 110672896
Type: VAR
# Max. Min./Amp. JD0 Period
13.910 r Y 0.001 r 2454786.69750 1.198219000000 F5IV
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:51:51.87 -04:03:49.1: 14.98 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:51:51.87 -04:03:49.1: 99.00 +/- 99.00 edge
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
CoRoT 110672896,2461152.6091,13.21,0.05,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
CoRoT 110672896 20260422.1091 13.21CV 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 22.1091 2461152.6091 13.23 06:59:32.96 -02:32:38.2
216.12066 0.64301 galactic Mon Second-epoch detections are separated by 4.4" and 5.5 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 | ATO J104.8947-02.5666 | 06:59:34.40 -02:33:17.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G8III 1956ApJS....2..271M LF 9 -03 459 J-Ks=0.359+/-0.038 (G)
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:59:32.96 -02:32:38.2: 14.86 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:59:32.96 -02:32:38.2: 99.00 +/- 99.00 edge
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 J104.8947-02.5666,2461152.6091,13.23,0.05,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 J104.8947-02.5666 20260422.1091 13.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1091 2461152.6091 13.32 06:54:32.31 -02:12:21.7
215.24862 -0.31633 galactic Mon Second-epoch detections are separated by 2.6" and 6.2 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 J103.6315-02.2046 | 06:54:32.31 -02:12:21.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:54:32.31 -02:12:21.7: 14.94 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:54:32.31 -02:12:21.7: 99.00 +/- 99.00 edge
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 J103.6315-02.2046,2461152.6091,13.32,0.05,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 J103.6315-02.2046 20260422.1091 13.32CV 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 22.1091 2461152.6091 13.28 06:45:00.74 +00:14:03.0
211.99083 -1.32282 galactic Mon Second-epoch detections are separated by 2.4" and 5.9 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 3125505636118883328 | 06:45:02.18 +00:13:29.5 (Gaia DR3) | DSCT/GDOR (local) | (local) | Gaia3var=NOT_AVAILABLE SpType: G8.5III 2012A&A...543A.125G CoRoT 102761279
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:45:00.74 +00:14:03.0: 14.45 +/- 0.23 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:45:00.74 +00:14:03.0: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 14.45 +/- 0.23
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 3125505636118883328,2461152.6091,13.28,0.05,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 3125505636118883328 20260422.1091 13.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1091 2461152.6091 13.37 06:55:19.67 -00:57:48.9
214.23295 0.42598 galactic Mon Second-epoch detections are separated by 3.5" and 6.1 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 3112428628934381568 | 06:55:17.90 -00:57:39.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5: 1956ApJS....2..271M LF 9 -01 325
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:55:19.67 -00:57:48.9: 14.77 +/- 0.28 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:55:19.67 -00:57:48.9: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 14.77 +/- 0.28
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 3112428628934381568,2461152.6091,13.37,0.05,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 3112428628934381568 20260422.1091 13.37CV 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 22.1091 2461152.6091 13.29 06:47:11.78 +00:21:18.4
212.13229 -0.78177 galactic Mon Second-epoch detections are separated by 2.8" and 6.2 pix
The object was found in VSX 4" Gaia DR3 3113525082544566656
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
14.310 G 14.340 G B
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:47:11.78 +00:21:18.4: 15.06 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:47:11.78 +00:21:18.4: 99.00 +/- 99.00 edge
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 3113525082544566656,2461152.6091,13.29,0.05,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
Gaia DR3 3113525082544566656 20260422.1091 13.29CV 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 22.1091 2461152.6091 13.32 06:57:11.48 -01:07:45.1
214.59287 0.76490 galactic Mon Second-epoch detections are separated by 1.9" and 6.4 pix
The object was found in VSX 3" Gaia DR3 3112223325200684160
Type: RS
# Max. Min./Amp. JD0 Period
17.280 G 17.420 G K
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:57:11.48 -01:07:45.1: 15.01 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:57:11.48 -01:07:45.1: 99.00 +/- 99.00 edge
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 3112223325200684160,2461152.6091,13.32,0.05,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 3112223325200684160 20260422.1091 13.32CV 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 22.1091 2461152.6091 13.37 06:51:56.27 -01:17:01.1
214.13135 -0.47407 galactic Mon Second-epoch detections are separated by 1.6" and 6.0 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 | 06:51:56.27 -01:17:01.1 (user input) | T | P | (position from user input) J-Ks=0.375+/-0.043 (G)
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:51:56.27 -01:17:01.1: 14.60 +/- 0.31 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:51:56.27 -01:17:01.1: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 14.60 +/- 0.31
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,2461152.6091,13.37,0.05,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 20260422.1091 13.37CV 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 22.1091 2461152.6091 13.34 06:56:49.62 -05:48:25.6
218.71412 -1.45078 galactic Mon Second-epoch detections are separated by 1.2" and 6.5 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 | Gaia DR3 3101159626880841728 | 06:56:51.32 -05:48:25.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:56:49.62 -05:48:25.6: 14.21 +/- 0.17 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:56:49.62 -05:48:25.6: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 14.21 +/- 0.17
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 3101159626880841728,2461152.6091,13.34,0.05,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 3101159626880841728 20260422.1091 13.34CV 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 22.1091 2461152.6091 13.31 06:59:38.68 -00:49:25.6
214.60105 1.44994 galactic Mon Second-epoch detections are separated by 4.2" and 5.9 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 3112250164452721664 | 06:59:37.63 -00:49:58.3 (Gaia DR3) | DSCT/GDOR (local) | (local) | Gaia3var=VARIABLE J-Ks=0.401+/-0.040 (G)
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:59:38.68 -00:49:25.6: 14.96 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:59:38.68 -00:49:25.6: 99.00 +/- 99.00 edge
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 3112250164452721664,2461152.6091,13.31,0.05,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 3112250164452721664 20260422.1091 13.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1091 2461152.6091 13.42 06:48:35.53 -03:42:40.1
215.91256 -2.32350 galactic Mon Second-epoch detections are separated by 3.5" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3105425491480566784 | 06:48:32.98 -03:42:43.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K7 1949AnHar.112....1C HD 295556
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:48:35.53 -03:42:40.1: 14.97 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:48:35.53 -03:42:40.1: 99.00 +/- 99.00 edge
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 3105425491480566784,2461152.6091,13.42,0.05,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
Gaia DR3 3105425491480566784 20260422.1091 13.42CV 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 22.1091 2461152.6091 13.39 07:05:52.55 -00:01:01.8
214.59480 3.20411 galactic Mon Second-epoch detections are separated by 2.2" and 6.1 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 3112746830169900544 | 07:05:49.84 -00:00:39.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:05:52.55 -00:01:01.8: 14.02 +/- 0.15 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:05:52.55 -00:01:01.8: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 14.02 +/- 0.15
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 3112746830169900544,2461152.6091,13.39,0.05,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 3112746830169900544 20260422.1091 13.39CV 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 22.1091 2461152.6091 13.45 07:02:48.91 -01:46:40.0
215.81218 1.71890 galactic Mon Second-epoch detections are separated by 2.9" and 6.2 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 | 07:02:48.91 -01:46:40.0 (user input) | T | P | (position from user input) J-Ks=0.239+/-0.038 (F)
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:02:48.91 -01:46:40.0: 14.62 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:02:48.91 -01:46:40.0: 99.00 +/- 99.00 edge
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,2461152.6091,13.45,0.05,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
target 20260422.1091 13.45CV 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 22.1091 2461152.6091 13.63 06:45:12.00 +00:20:57.6
211.90973 -1.22853 galactic Mon Second-epoch detections are separated by 0.8" and 6.4 pix
The object was found in VSX23" ZTF J064511.00+002040.7
Type: YSO
# Max. Min./Amp. JD0 Period
17.475 r Y 0.367 r
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:45:12.00 +00:20:57.6: 14.85 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:45:12.00 +00:20:57.6: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J064511.00+002040.7,2461152.6091,13.63,0.05,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
ZTF J064511.00+002040.7 20260422.1091 13.63CV 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 22.1091 2461152.6091 13.53 06:51:44.75 -03:39:22.9
216.22194 -1.59795 galactic Mon Second-epoch detections are separated by 0.9" and 6.1 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 J102.9282-03.6451 | 06:51:44.81 -03:38:43.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: B5 1949AnHar.112....1C HD 50136
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:51:44.75 -03:39:22.9: 14.96 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:51:44.75 -03:39:22.9: 99.00 +/- 99.00 edge
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 J102.9282-03.6451,2461152.6091,13.53,0.05,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 J102.9282-03.6451 20260422.1091 13.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1091 2461152.6091 13.59 06:58:34.68 -01:38:25.6
215.20601 0.83985 galactic Mon Second-epoch detections are separated by 2.2" and 6.1 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 J104.6381-01.6369 | 06:58:34.68 -01:38:25.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:58:34.68 -01:38:25.6: 15.01 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:58:34.68 -01:38:25.6: 99.00 +/- 99.00 edge
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 J104.6381-01.6369,2461152.6091,13.59,0.05,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 J104.6381-01.6369 20260422.1091 13.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.81363703 23.12.2025 07:31:28.239 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
First image: 2461032.81363703 23.12.2025 07:31:28.239 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Last image: 2461152.60945472 22.04.2026 02:37:26.888 /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q2b1x1_214741_TTUQ2b1x1_167185_cObK847F/fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 7
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.85
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): 29516
Objects passed selection criteria: 29374
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: 22420
Average stars matched: 20467.8 (91.2924 %)
Memory usage VmPeak: 131292 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 Tue Apr 21 23:00:01 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: 2461032.81363703 23.12.2025 07:31:28.239 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
First image: 2461032.81363703 23.12.2025 07:31:28.239 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Last image: 2461152.60945472 22.04.2026 02:37:26.888 /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q2b1x1_214741_TTUQ2b1x1_167185_cObK847F/fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 482
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.50
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: 245 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): 220425
Objects passed selection criteria: 219718
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: 174975
Average stars matched: 159377 (91.0857 %)
Memory usage VmPeak: 1970940 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 Tue Apr 21 23:07:31 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_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q2b1x1_214741_TTUQ2b1x1_167185_cObK847F/fd_Mon-02-Q2b1x1_2026-04-21_21-36-27_20.00sec_-4.90C_LIGHT_0026.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q2b1x1_214741_TTUQ2b1x1_167185_cObK847F/fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027.fits
SExtractor catalog cache: saved Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat to cache
SExtractor catalog cache: saved Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.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_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q2b1x1_214741_TTUQ2b1x1_167185_cObK847F/fd_Mon-02-Q2b1x1_2026-04-21_21-36-27_20.00sec_-4.90C_LIGHT_0026.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q2b1x1_214741_TTUQ2b1x1_167185_cObK847F/fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027.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: 2461152.60877253
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits exists and is non-empty
Saving wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits to local_wcs_cache/
'wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits' -> 'local_wcs_cache/wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits'
wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits exists and is non-empty
Saving wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits to local_wcs_cache/
'wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits' -> 'local_wcs_cache/wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits'
wcs_fd_Mon-02-Q2b1x1_2026-04-21_21-36-27_20.00sec_-4.90C_LIGHT_0026.fits exists and is non-empty
Saving wcs_fd_Mon-02-Q2b1x1_2026-04-21_21-36-27_20.00sec_-4.90C_LIGHT_0026.fits to local_wcs_cache/
'wcs_fd_Mon-02-Q2b1x1_2026-04-21_21-36-27_20.00sec_-4.90C_LIGHT_0026.fits' -> 'local_wcs_cache/wcs_fd_Mon-02-Q2b1x1_2026-04-21_21-36-27_20.00sec_-4.90C_LIGHT_0026.fits'
wcs_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027.fits exists and is non-empty
Saving wcs_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027.fits to local_wcs_cache/
'wcs_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027.fits' -> 'local_wcs_cache/wcs_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits (1st reference image)
verification OK: wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Image size: 931.8'x623.6' 15.5(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.84"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 06:51:43.082 -02:00:16.78 J2000 4789.000 3195.000
###################################
The image scale is 5.84"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.8" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Mon-02-Q2b1x1_2026-04-21_21-36-27_20.00sec_-4.90C_LIGHT_0026.fits (1st new image)
verification OK: wcs_fd_Mon-02-Q2b1x1_2026-04-21_21-36-27_20.00sec_-4.90C_LIGHT_0026.fits
Image size: 937.2'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: 06:51:36.647 -01:56:50.90 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 06:51:43.082 -02:00:16.78
Second-epoch image center 06:51:36.647 -01:56:50.90
Angular distance between the image centers 0.0632 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027.fits (2nd new image)
verification OK: wcs_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027.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: 06:51:37.110 -01:57:27.84 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 06:51:43.082 -02:00:16.78
Second-epoch image center 06:51:37.110 -01:57:27.84
Angular distance between the image centers 0.0531 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 06:51:36.647 -01:56:50.90
Second-epoch second image center 06:51:37.110 -01:57:27.84
Angular distance between the image centers 0.01044 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_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits &> /tmp/tmp.YJTEg0t94M
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits &> /tmp/tmp.2zXA5pQNOB
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q2b1x1_214741_TTUQ2b1x1_167185_cObK847F/fd_Mon-02-Q2b1x1_2026-04-21_21-36-27_20.00sec_-4.90C_LIGHT_0026.fits &> /tmp/tmp.dx2zODWTnz
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q2b1x1_214741_TTUQ2b1x1_167185_cObK847F/fd_Mon-02-Q2b1x1_2026-04-21_21-36-27_20.00sec_-4.90C_LIGHT_0026.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q2b1x1_214741_TTUQ2b1x1_167185_cObK847F/fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027.fits &> /tmp/tmp.nxPr8ZGYBS
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q2b1x1_214741_TTUQ2b1x1_167185_cObK847F/fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027.fits
Calibrating the magnitude scale
Found non-empty wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.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_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits and wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.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_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits and wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
Found non-empty wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits and wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
The reference image (wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits) and catalog (wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat) found
'wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat' -> 'wcsmag.cat'
Read 36622 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 95.0306 to 110.7538 deg, Dec -7.3378 to +3.4896 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 95.0306 to 110.7538 deg, Dec -7.3378 to 3.4896 deg
Loaded 24069 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): 377 out of 430 total matches.
Matched with Tycho-2 430 out of 36622 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.893893
a=0.000000 b=1.000000 c=22.893893
From vast_summary.log: estimated ref. image limiting mag.: -7.85
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.04
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.04
Magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 36622 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 95.0306 to 110.7538 deg, Dec -7.3378 to +3.4896 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 95.0306 to 110.7538 deg, Dec -7.3378 to 3.4896 deg
Loaded 24069 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): 377 out of 430 total matches.
Matched with Tycho-2 430 out of 36622 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits via Tycho-2
Forced-photometry filter: calibrated wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits -> calib.txt_param_ref_wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits (aperture=5.9)
Read 36412 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 39.2377 to 51.3659 deg, Dec -2.9720 to +7.3737 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 39.2377 to 51.3659 deg, Dec -2.9720 to 7.3737 deg
Loaded 3163 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): 10 out of 10 total matches.
Matched with Tycho-2 10 out of 36412 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits via Tycho-2
Forced-photometry filter: calibrated wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits -> calib.txt_param_ref_wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits (aperture=5.9)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 5 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.1 pix Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
2.1 pix Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
2.5 pix fd_Mon-02-Q2b1x1_2026-04-21_21-36-27_20.00sec_-4.90C_LIGHT_0026.fits
2.5 pix fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027.fits
2.1 pix wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
2.1 pix wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
Limiting magnitude estimates:
15.0 mag. Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
15.0 mag. Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
14.4 mag. fd_Mon-02-Q2b1x1_2026-04-21_21-36-27_20.00sec_-4.90C_LIGHT_0026.fits
14.4 mag. fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027.fits
All-image limiting magnitude estimate: 14.4 (SNR ) 11.6 (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.YJTEg0t94M (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-21_CI_Mon-02-Q2b1x1_214741_TTUQ2b1x1_167185_cObK847F/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits 568.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.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_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits' -> 'wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WCS_IMAGE_NAME=wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WCS-calibrated image found: wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Checking if the catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat corresponding to the image wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits alredy exist and is non-empty...
Catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat corresponding to the image wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.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_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WCS catalog name: wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=4596, passed=36622
Got 36622 stars (including 31982 good ones) from the SExtractor catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
util/solve_plate_with_UCAC5 got 36622 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 931.8'
Seting catalog search parameters based on the expected field of view 931.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012942 (46.6 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010353 (37.3 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 469 (Dec -7.3 to 3.5)
Done reading UCAC5 zone files...
Matched 457 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 347 matched stars entering correct_measured_positions(), 270 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 10.06"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 338 matched stars entering correct_measured_positions(), 14588 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 16.11"
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 469 (Dec -7.3 to 3.5)
Done reading UCAC5 zone files...
Matched 489 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 392 matched stars entering correct_measured_positions(), 14615 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 16.01"
Accuracy estimation diagnostic: 390 matched stars entering correct_measured_positions(), 15067 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 12.91"
Excluding outliers - 390 stars left (next iteration limit 371)
The image catalog is written to wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits -region wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.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.2zXA5pQNOB (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-21_CI_Mon-02-Q2b1x1_214741_TTUQ2b1x1_167185_cObK847F/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits 568.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.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_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits' -> 'wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WCS_IMAGE_NAME=wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WCS-calibrated image found: wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
Checking if the catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat corresponding to the image wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits alredy exist and is non-empty...
Catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat corresponding to the image wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.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_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WCS catalog name: wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=4657, passed=36412
Got 36412 stars (including 31701 good ones) from the SExtractor catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat
util/solve_plate_with_UCAC5 got 36412 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 625.6'
Seting catalog search parameters based on the expected field of view 625.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.008689 (31.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.006951 (25.0 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 435 to 488 (Dec -3.0 to 7.4)
Done reading UCAC5 zone files...
Matched 20 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Retrying with a larger catalog search radius.
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 435 to 488 (Dec -3.0 to 7.4)
Done reading UCAC5 zone files...
Matched 73 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 51 matched stars entering correct_measured_positions(), 0 with non-zero local correction accuracy
ERROR: the estimated accuracy of the plate solution seems unrealistically small! No stars (out of 51 matched) have non-zero estimated_local_correction_accuracy.
ERROR running correct_measured_positions()
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.dx2zODWTnz (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_2026-04-21_CI_Mon-02-Q2b1x1_214741_TTUQ2b1x1_167185_cObK847F/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q2b1x1_214741_TTUQ2b1x1_167185_cObK847F/fd_Mon-02-Q2b1x1_2026-04-21_21-36-27_20.00sec_-4.90C_LIGHT_0026.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q2b1x1_214741_TTUQ2b1x1_167185_cObK847F/fd_Mon-02-Q2b1x1_2026-04-21_21-36-27_20.00sec_-4.90C_LIGHT_0026.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q2b1x1_214741_TTUQ2b1x1_167185_cObK847F/fd_Mon-02-Q2b1x1_2026-04-21_21-36-27_20.00sec_-4.90C_LIGHT_0026.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q2b1x1_214741_TTUQ2b1x1_167185_cObK847F/fd_Mon-02-Q2b1x1_2026-04-21_21-36-27_20.00sec_-4.90C_LIGHT_0026.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q2b1x1_214741_TTUQ2b1x1_167185_cObK847F/fd_Mon-02-Q2b1x1_2026-04-21_21-36-27_20.00sec_-4.90C_LIGHT_0026.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_2026-04-21_CI_Mon-02-Q2b1x1_214741_TTUQ2b1x1_167185_cObK847F/fd_Mon-02-Q2b1x1_2026-04-21_21-36-27_20.00sec_-4.90C_LIGHT_0026.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q2b1x1_2026-04-21_21-36-27_20.00sec_-4.90C_LIGHT_0026.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q2b1x1_2026-04-21_21-36-27_20.00sec_-4.90C_LIGHT_0026.fits
Checking if the catalog wcs_fd_Mon-02-Q2b1x1_2026-04-21_21-36-27_20.00sec_-4.90C_LIGHT_0026.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-21_21-36-27_20.00sec_-4.90C_LIGHT_0026.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q2b1x1_2026-04-21_21-36-27_20.00sec_-4.90C_LIGHT_0026.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-21_21-36-27_20.00sec_-4.90C_LIGHT_0026.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_2026-04-21_21-36-27_20.00sec_-4.90C_LIGHT_0026.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q2b1x1_214741_TTUQ2b1x1_167185_cObK847F/fd_Mon-02-Q2b1x1_2026-04-21_21-36-27_20.00sec_-4.90C_LIGHT_0026.fits
WCS catalog name: wcs_fd_Mon-02-Q2b1x1_2026-04-21_21-36-27_20.00sec_-4.90C_LIGHT_0026.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2057, passed=22097
Got 22097 stars (including 20028 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q2b1x1_2026-04-21_21-36-27_20.00sec_-4.90C_LIGHT_0026.fits.cat
util/solve_plate_with_UCAC5 got 22097 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (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 0.010413 (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 469 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 911 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.71"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 21702 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
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 469 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 931 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(), 21703 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 21702 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.73"
Excluding outliers - 929 stars left (next iteration limit 1021)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-02-Q2b1x1_2026-04-21_21-36-27_20.00sec_-4.90C_LIGHT_0026.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q2b1x1_2026-04-21_21-36-27_20.00sec_-4.90C_LIGHT_0026.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q2b1x1_214741_TTUQ2b1x1_167185_cObK847F/fd_Mon-02-Q2b1x1_2026-04-21_21-36-27_20.00sec_-4.90C_LIGHT_0026.fits -region wcs_fd_Mon-02-Q2b1x1_2026-04-21_21-36-27_20.00sec_-4.90C_LIGHT_0026.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q2b1x1_2026-04-21_21-36-27_20.00sec_-4.90C_LIGHT_0026.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.nxPr8ZGYBS (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_2026-04-21_CI_Mon-02-Q2b1x1_214741_TTUQ2b1x1_167185_cObK847F/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q2b1x1_214741_TTUQ2b1x1_167185_cObK847F/fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q2b1x1_214741_TTUQ2b1x1_167185_cObK847F/fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q2b1x1_214741_TTUQ2b1x1_167185_cObK847F/fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q2b1x1_214741_TTUQ2b1x1_167185_cObK847F/fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q2b1x1_214741_TTUQ2b1x1_167185_cObK847F/fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027.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_2026-04-21_CI_Mon-02-Q2b1x1_214741_TTUQ2b1x1_167185_cObK847F/fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027.fits
Checking if the catalog wcs_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027.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_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q2b1x1_214741_TTUQ2b1x1_167185_cObK847F/fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027.fits
WCS catalog name: wcs_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027.fits.cat
SExtractor catalog parsing summary: zero_flux=7, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2093, passed=22221
Got 22221 stars (including 20104 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027.fits.cat
util/solve_plate_with_UCAC5 got 22221 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 469 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 920 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 21812 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
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 469 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 934 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(), 21810 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 21810 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.76"
Excluding outliers - 929 stars left (next iteration limit 1026)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q2b1x1_214741_TTUQ2b1x1_167185_cObK847F/fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027.fits -region wcs_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027.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_2026-04-21_21-36-27_20.00sec_-4.90C_LIGHT_0026.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Mon-02-Q2b1x1_2026-04-21_21-36-27_20.00sec_-4.90C_LIGHT_0026.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q2b1x1_214741_TTUQ2b1x1_167185_cObK847F/wcs_fd_Mon-02-Q2b1x1_2026-04-21_21-36-27_20.00sec_-4.90C_LIGHT_0026.fits'
Saving fully-calibrated image wcs_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q2b1x1_214741_TTUQ2b1x1_167185_cObK847F/wcs_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027.fits'
Preparing the HTML report for the field Mon-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out51876.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 1s
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 51876_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 51876_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:52:55.98 -03:45:08.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.04, MAG_FAINT_SEARCH_LIMIT=12.02)GAIADR2_OUTPUT=# 0.789 3102730592781122176 103.23306216824 -03.75253037047 11.1851 10.8050 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.789#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51877_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 51877_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:38:08.49 -01:28:14.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54694_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 54694_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 07:09:13.63 -02:21:30.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54807_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 54807_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:42:37.29 -03:49:18.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 56490_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 56490_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:44:47.52 -05:17:45.7 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 2s
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 ####
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_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q2b1x1_214741_TTUQ2b1x1_167185_cObK847F/fd_Mon-02-Q2b1x1_2026-04-21_21-36-27_20.00sec_-4.90C_LIGHT_0026.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q2b1x1_214741_TTUQ2b1x1_167185_cObK847F/fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027.fits
SExtractor catalog cache: saved Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat to cache
SExtractor catalog cache: saved Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.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_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q2b1x1_214741_TTUQ2b1x1_167185_cObK847F/fd_Mon-02-Q2b1x1_2026-04-21_21-36-27_20.00sec_-4.90C_LIGHT_0026.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q2b1x1_214741_TTUQ2b1x1_167185_cObK847F/fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Creating symlink local_wcs_cache/wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
Creating symlink local_wcs_cache/wcs_fd_Mon-02-Q2b1x1_2026-04-21_21-36-27_20.00sec_-4.90C_LIGHT_0026.fits
Creating symlink local_wcs_cache/wcs_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027.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_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits exists and is non-empty
wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits exists and is non-empty
wcs_fd_Mon-02-Q2b1x1_2026-04-21_21-36-27_20.00sec_-4.90C_LIGHT_0026.fits exists and is non-empty
wcs_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits (1st reference image)
verification OK: wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Image size: 931.8'x623.6' 15.5(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.84"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 06:51:43.082 -02:00:16.78 J2000 4789.000 3195.000
###################################
The image scale is 5.84"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.8" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Mon-02-Q2b1x1_2026-04-21_21-36-27_20.00sec_-4.90C_LIGHT_0026.fits (1st new image)
verification OK: wcs_fd_Mon-02-Q2b1x1_2026-04-21_21-36-27_20.00sec_-4.90C_LIGHT_0026.fits
Image size: 937.2'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: 06:51:36.647 -01:56:50.90 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 06:51:43.082 -02:00:16.78
Second-epoch image center 06:51:36.647 -01:56:50.90
Angular distance between the image centers 0.0632 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027.fits (2nd new image)
verification OK: wcs_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027.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: 06:51:37.110 -01:57:27.84 J2000 4789.000 3195.000
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# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 06:51:43.082 -02:00:16.78
Second-epoch image center 06:51:37.110 -01:57:27.84
Angular distance between the image centers 0.0531 deg.
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# 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 06:51:36.647 -01:56:50.90
Second-epoch second image center 06:51:37.110 -01:57:27.84
Angular distance between the image centers 0.01044 deg.
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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_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits &> /tmp/tmp.m8zF3EsCnv
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits &> /tmp/tmp.5lrngF11Kz
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q2b1x1_214741_TTUQ2b1x1_167185_cObK847F/fd_Mon-02-Q2b1x1_2026-04-21_21-36-27_20.00sec_-4.90C_LIGHT_0026.fits &> /tmp/tmp.rks44ooWZe
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q2b1x1_214741_TTUQ2b1x1_167185_cObK847F/fd_Mon-02-Q2b1x1_2026-04-21_21-36-27_20.00sec_-4.90C_LIGHT_0026.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q2b1x1_214741_TTUQ2b1x1_167185_cObK847F/fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027.fits &> /tmp/tmp.EKUPhkvPYX
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q2b1x1_214741_TTUQ2b1x1_167185_cObK847F/fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027.fits
Calibrating the magnitude scale
Found non-empty wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.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_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits and wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.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_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits and wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
Found non-empty wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits and wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
The reference image (wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits) and catalog (wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat) found
'wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat' -> 'wcsmag.cat'
Read 254624 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 95.0305 to 110.7571 deg, Dec -7.3394 to +3.4970 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 95.0305 to 110.7571 deg, Dec -7.3394 to 3.4970 deg
Loaded 24089 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): 401 out of 624 total matches.
Matched with Tycho-2 624 out of 254624 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 21.875059
a=0.000000 b=1.000000 c=21.875059
From vast_summary.log: estimated ref. image limiting mag.: -7.50
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.38
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.38
Magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 254624 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 95.0305 to 110.7571 deg, Dec -7.3394 to +3.4970 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 95.0305 to 110.7571 deg, Dec -7.3394 to 3.4970 deg
Loaded 24089 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): 401 out of 624 total matches.
Matched with Tycho-2 624 out of 254624 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits via Tycho-2
Forced-photometry filter: calibrated wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits -> calib.txt_param_ref_wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits (aperture=4.5)
Read 257656 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 39.1911 to 51.4130 deg, Dec -2.9804 to +7.3961 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 39.1911 to 51.4130 deg, Dec -2.9804 to 7.3961 deg
Loaded 3200 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): 37 out of 44 total matches.
Matched with Tycho-2 44 out of 257656 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits via Tycho-2
Forced-photometry filter: calibrated wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits -> calib.txt_param_ref_wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits (aperture=4.5)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 407 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.0 pix Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
2.0 pix Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
2.2 pix fd_Mon-02-Q2b1x1_2026-04-21_21-36-27_20.00sec_-4.90C_LIGHT_0026.fits
2.2 pix fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027.fits
2.0 pix wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
2.0 pix wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
Limiting magnitude estimates:
14.4 mag. Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
14.4 mag. Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
13.7 mag. fd_Mon-02-Q2b1x1_2026-04-21_21-36-27_20.00sec_-4.90C_LIGHT_0026.fits
13.7 mag. fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027.fits
All-image limiting magnitude estimate: 13.7 (SNR ) 13.2 (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.m8zF3EsCnv (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-21_CI_Mon-02-Q2b1x1_214741_TTUQ2b1x1_167185_cObK847F/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits 568.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.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_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits' -> 'wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WCS_IMAGE_NAME=wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WCS-calibrated image found: wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Checking if the catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat corresponding to the image wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits alredy exist and is non-empty...
Catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat corresponding to the image wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.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_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WCS catalog name: wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=59, blended=45640, passed=254565
Got 254565 stars (including 208571 good ones) from the SExtractor catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
util/solve_plate_with_UCAC5 got 254565 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 931.8'
Seting catalog search parameters based on the expected field of view 931.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012942 (46.6 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010353 (37.3 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 469 (Dec -7.3 to 3.5)
Done reading UCAC5 zone files...
Matched 468 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 369 matched stars entering correct_measured_positions(), 265 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 6.77"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 366 matched stars entering correct_measured_positions(), 92781 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.43"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 469 (Dec -7.3 to 3.5)
Done reading UCAC5 zone files...
Matched 498 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 431 matched stars entering correct_measured_positions(), 92827 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.42"
Accuracy estimation diagnostic: 428 matched stars entering correct_measured_positions(), 121659 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 6.79"
Excluding outliers - 428 stars left (next iteration limit 402)
The image catalog is written to wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits -region wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.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.5lrngF11Kz (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-21_CI_Mon-02-Q2b1x1_214741_TTUQ2b1x1_167185_cObK847F/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits 568.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.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_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits' -> 'wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WCS_IMAGE_NAME=wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WCS-calibrated image found: wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
Checking if the catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat corresponding to the image wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits alredy exist and is non-empty...
Catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat corresponding to the image wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.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_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WCS catalog name: wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=58, blended=46013, passed=257598
Got 257598 stars (including 211206 good ones) from the SExtractor catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat
util/solve_plate_with_UCAC5 got 257598 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 625.6'
Seting catalog search parameters based on the expected field of view 625.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.008689 (31.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.006951 (25.0 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 435 to 488 (Dec -3.0 to 7.4)
Done reading UCAC5 zone files...
Matched 17 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Retrying with a larger catalog search radius.
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 435 to 488 (Dec -3.0 to 7.4)
Done reading UCAC5 zone files...
Matched 68 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 44 matched stars entering correct_measured_positions(), 0 with non-zero local correction accuracy
ERROR: the estimated accuracy of the plate solution seems unrealistically small! No stars (out of 44 matched) have non-zero estimated_local_correction_accuracy.
ERROR running correct_measured_positions()
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.rks44ooWZe (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_2026-04-21_CI_Mon-02-Q2b1x1_214741_TTUQ2b1x1_167185_cObK847F/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q2b1x1_214741_TTUQ2b1x1_167185_cObK847F/fd_Mon-02-Q2b1x1_2026-04-21_21-36-27_20.00sec_-4.90C_LIGHT_0026.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q2b1x1_214741_TTUQ2b1x1_167185_cObK847F/fd_Mon-02-Q2b1x1_2026-04-21_21-36-27_20.00sec_-4.90C_LIGHT_0026.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q2b1x1_214741_TTUQ2b1x1_167185_cObK847F/fd_Mon-02-Q2b1x1_2026-04-21_21-36-27_20.00sec_-4.90C_LIGHT_0026.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q2b1x1_214741_TTUQ2b1x1_167185_cObK847F/fd_Mon-02-Q2b1x1_2026-04-21_21-36-27_20.00sec_-4.90C_LIGHT_0026.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q2b1x1_214741_TTUQ2b1x1_167185_cObK847F/fd_Mon-02-Q2b1x1_2026-04-21_21-36-27_20.00sec_-4.90C_LIGHT_0026.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_2026-04-21_CI_Mon-02-Q2b1x1_214741_TTUQ2b1x1_167185_cObK847F/fd_Mon-02-Q2b1x1_2026-04-21_21-36-27_20.00sec_-4.90C_LIGHT_0026.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q2b1x1_2026-04-21_21-36-27_20.00sec_-4.90C_LIGHT_0026.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q2b1x1_2026-04-21_21-36-27_20.00sec_-4.90C_LIGHT_0026.fits
Checking if the catalog wcs_fd_Mon-02-Q2b1x1_2026-04-21_21-36-27_20.00sec_-4.90C_LIGHT_0026.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-21_21-36-27_20.00sec_-4.90C_LIGHT_0026.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q2b1x1_2026-04-21_21-36-27_20.00sec_-4.90C_LIGHT_0026.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-21_21-36-27_20.00sec_-4.90C_LIGHT_0026.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_2026-04-21_21-36-27_20.00sec_-4.90C_LIGHT_0026.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q2b1x1_214741_TTUQ2b1x1_167185_cObK847F/fd_Mon-02-Q2b1x1_2026-04-21_21-36-27_20.00sec_-4.90C_LIGHT_0026.fits
WCS catalog name: wcs_fd_Mon-02-Q2b1x1_2026-04-21_21-36-27_20.00sec_-4.90C_LIGHT_0026.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=58, blended=21667, passed=168628
Got 168628 stars (including 146788 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q2b1x1_2026-04-21_21-36-27_20.00sec_-4.90C_LIGHT_0026.fits.cat
util/solve_plate_with_UCAC5 got 168628 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (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 0.010413 (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 469 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 932 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(), 912 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 165511 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
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 469 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 932 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 931 matched stars entering correct_measured_positions(), 165508 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
Accuracy estimation diagnostic: 931 matched stars entering correct_measured_positions(), 165505 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
Excluding outliers - 931 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_2026-04-21_21-36-27_20.00sec_-4.90C_LIGHT_0026.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q2b1x1_2026-04-21_21-36-27_20.00sec_-4.90C_LIGHT_0026.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q2b1x1_214741_TTUQ2b1x1_167185_cObK847F/fd_Mon-02-Q2b1x1_2026-04-21_21-36-27_20.00sec_-4.90C_LIGHT_0026.fits -region wcs_fd_Mon-02-Q2b1x1_2026-04-21_21-36-27_20.00sec_-4.90C_LIGHT_0026.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q2b1x1_2026-04-21_21-36-27_20.00sec_-4.90C_LIGHT_0026.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.EKUPhkvPYX (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_2026-04-21_CI_Mon-02-Q2b1x1_214741_TTUQ2b1x1_167185_cObK847F/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q2b1x1_214741_TTUQ2b1x1_167185_cObK847F/fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q2b1x1_214741_TTUQ2b1x1_167185_cObK847F/fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q2b1x1_214741_TTUQ2b1x1_167185_cObK847F/fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q2b1x1_214741_TTUQ2b1x1_167185_cObK847F/fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q2b1x1_214741_TTUQ2b1x1_167185_cObK847F/fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027.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_2026-04-21_CI_Mon-02-Q2b1x1_214741_TTUQ2b1x1_167185_cObK847F/fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027.fits
Checking if the catalog wcs_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027.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_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q2b1x1_214741_TTUQ2b1x1_167185_cObK847F/fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027.fits
WCS catalog name: wcs_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027.fits.cat
SExtractor catalog parsing summary: zero_flux=1, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=63, blended=21319, passed=167037
Got 167037 stars (including 145564 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027.fits.cat
util/solve_plate_with_UCAC5 got 167037 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 469 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 930 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 930 matched stars entering correct_measured_positions(), 911 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 930 matched stars entering correct_measured_positions(), 164007 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
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 469 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 930 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 164003 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 164003 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
Excluding outliers - 928 stars left (next iteration limit 1023)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q2b1x1_214741_TTUQ2b1x1_167185_cObK847F/fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027.fits -region wcs_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027.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_2026-04-21_21-36-27_20.00sec_-4.90C_LIGHT_0026.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_2026-04-21_CI_Mon-02-Q2b1x1_214741_TTUQ2b1x1_167185_cObK847F/wcs_fd_Mon-02-Q2b1x1_2026-04-21_21-36-27_20.00sec_-4.90C_LIGHT_0026.fits
Saving fully-calibrated image wcs_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027.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_2026-04-21_CI_Mon-02-Q2b1x1_214741_TTUQ2b1x1_167185_cObK847F/wcs_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027.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__out283508.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283524.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283538.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283543.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283582.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283594.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283625.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283627.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283631.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283639.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283641.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283646.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283655.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283656.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283669.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283687.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283708.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283710.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283722.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283726.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283727.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283733.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283737.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283747.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283750.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283755.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283756.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283764.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283765.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283770.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283778.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283785.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283790.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283796.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283801.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283802.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283807.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283810.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283812.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283814.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283816.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283823.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283858.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283860.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283865.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283884.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283885.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283894.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283895.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283896.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283897.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283899.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283909.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283914.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283915.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283919.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283928.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283929.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283930.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283932.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283938.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283949.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283971.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283972.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283987.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283993.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283994.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294907.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out298047.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out298321.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out299828.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out300321.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out300748.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out301119.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out301345.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out302417.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out302525.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out302837.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out303024.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out303554.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out305073.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out305413.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out305643.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out306345.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out306350.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out306816.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out306861.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out307248.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out308045.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out308702.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out308806.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out308957.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out310093.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out310473.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out310495.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out310531.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out310780.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out311418.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out311513.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out311550.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out311587.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out312361.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out312567.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out312590.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out313162.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out313287.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out313387.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out313530.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out313531.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out313962.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out314022.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out314023.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out314163.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out314529.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out314575.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out314951.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out314972.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out315224.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out315472.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316093.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316128.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316312.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316377.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316422.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316631.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316667.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316825.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out317218.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out317489.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out317820.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out318552.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out318663.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out319246.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out319323.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out319971.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out320319.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out320328.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out321317.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out321707.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out322077.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out322424.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out322668.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out322763.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out322781.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out283637.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out308444.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out316018.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out322317.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out283551.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283563.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283578.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283593.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283606.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283610.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283616.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283645.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283648.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283650.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283674.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283681.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283686.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283693.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283695.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283697.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283706.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283716.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283720.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283732.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283734.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283745.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283752.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283758.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283767.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283776.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283777.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283789.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283791.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283799.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283803.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283806.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283808.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283820.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283822.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283825.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283828.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283830.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283835.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283838.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283840.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283849.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283850.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283851.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283853.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283854.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283856.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283862.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283868.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283871.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283875.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283876.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283877.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283880.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283887.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283890.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283898.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283906.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283907.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283916.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283918.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283920.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283921.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283922.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283925.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283927.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283937.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283942.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283943.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283945.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283950.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283952.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283954.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283956.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283958.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283960.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283961.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283963.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283968.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283973.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283974.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283999.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294003.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295594.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out298956.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out300407.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out301761.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out301847.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out301899.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out301958.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out302278.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out302993.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out303212.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out303942.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out303993.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out304297.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out305306.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out306249.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out306360.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out306512.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out306753.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out307464.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out307477.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out307944.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out308542.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out308559.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out308561.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out308876.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out309021.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out309060.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out309125.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out309296.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out309575.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out310021.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out310226.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out310251.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out311031.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out311266.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out311614.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out311649.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out311673.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out312513.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out312736.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out312899.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out312935.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out312949.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out313714.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out313900.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out314486.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out314631.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out314855.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out315201.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out315453.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out316481.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out316900.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out316988.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out317123.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out317630.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out318165.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out318272.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out318737.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out319472.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out319532.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out319623.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out320137.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out320172.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out320409.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out320620.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out320713.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out321172.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out321354.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out321797.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out321983.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out322461.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out322475.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out322637.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 266s
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: 112s
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Considering the candidate 283508_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 283508_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:53:18.53 -05:31:40.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 2.426 3101146918078112896 103.32743924094 -05.52855001437 14.4150 13.5183 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.426#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283524_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 283524_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:53:04.47 +00:38:06.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)GAIADR2_OUTPUT=# 3.521 3113583592879746048 103.26904664927 +00.63420082836 14.5790 14.0241 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.521#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283538_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 283538_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:56:35.29 -06:06:21.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)GAIADR2_OUTPUT=# 1.682 3100864240513080064 104.14691339354 -06.10650504466 14.1829 13.6393 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.682#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283543_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 283543_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:53:18.32 +01:05:28.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 3.342 3113991000596997504 103.32633576755 +01.09026611931 14.3224 13.7220 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.342#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283551_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 283551_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 283563_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 283563_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 283578_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 283578_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 283582_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 283582_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:46:10.34 +01:00:16.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 2.498 3125713821773344640 101.54272357930 +01.00410104796 14.2178 13.5838 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.498#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283593_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 283593_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 283594_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 283594_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:59:25.02 -01:21:42.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)GAIADR2_OUTPUT=# 2.227 3112157113982160896 104.85456231523 -01.36233944921 14.3834 14.0654 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.227#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283606_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 283606_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 283610_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 283610_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 283616_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 283616_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 283618_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 283618_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
Rejecting candidate due to large distance (8.9") between the two second-epoch detections
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Considering the candidate 283625_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 283625_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:37:55.97 +00:48:03.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.39, MAG_FAINT_SEARCH_LIMIT=14.37)GAIADR2_OUTPUT=# 1.811 3119831739505299200 099.48321128109 +00.80041368826 14.1506 13.5830 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.811#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283627_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 283627_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 07:04:53.90 -03:03:18.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 1.244 3107904516543291136 106.22492779806 -03.05516246071 13.8752 13.0586 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.244#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283631_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 283631_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:39:23.57 -00:23:28.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)GAIADR2_OUTPUT=# 2.809 3119418293069471360 099.84830254289 -00.39194123631 13.9457 13.3191 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.809#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283637_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 283637_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:55:07.81 -00:16:29.4 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)
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Considering the candidate 283639_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 283639_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:54:12.37 -02:00:06.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 1.348 3106057504510134144 103.55142824856 -02.00219018737 13.8583 12.9554 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.348#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283641_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 283641_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:47:09.26 +00:44:31.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 3.654 3125644724339983744 101.78871008674 +00.74104857530 14.2112 13.6608 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.654#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283644_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 283644_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:42:01.83 +02:11:58.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 283645_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 283645_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 283646_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 283646_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:59:25.34 -02:10:14.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.32, MAG_FAINT_SEARCH_LIMIT=14.30)
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Considering the candidate 283648_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 283648_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 283649_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 283649_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:54:05.26 -01:51:49.4: 13.89 +/- 0.15 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:54:05.26 -01:51:49.4: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 13.89 +/- 0.15
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Considering the candidate 283650_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 283650_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 283655_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 283655_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 07:00:19.54 -03:32:01.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)GAIADR2_OUTPUT=# 3.075 3102620607258624000 105.08153655364 -03.53454019159 13.9178 13.2849 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.075#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283656_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 283656_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:51:03.52 -02:47:49.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)GAIADR2_OUTPUT=# 4.760 3105904504893575808 102.76500304932 -02.79841784748 13.9888 13.4867 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.760#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283660_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 283660_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:44:16.09 -03:32:32.3: 13.87 +/- 0.14 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:44:16.09 -03:32:32.3: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 13.87 +/- 0.14
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Considering the candidate 283669_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 283669_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:56:46.10 +01:59:33.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 1.223 3114213853560360192 104.19204350808 +01.99227385474 13.6903 12.7389 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.223#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283674_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 283674_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 283681_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 283681_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 283686_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 283686_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 283687_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 283687_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:49:53.24 +01:01:22.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.17, MAG_FAINT_SEARCH_LIMIT=14.15)GAIADR2_OUTPUT=# 1.553 3113667331861561728 102.47196760975 +01.02256213902 13.9973 13.5646 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.553#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283693_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 283693_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 283695_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 283695_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 283697_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 283697_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 283701_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 283701_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
Rejecting candidate due to large distance (14.8") between the two second-epoch detections
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Considering the candidate 283706_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 283706_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 283708_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 283708_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:56:40.84 -01:01:31.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 2.896 3112413441930195328 104.17019618330 -01.02613714310 14.0287 13.4693 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.896#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283710_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 283710_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 07:02:33.51 -01:58:00.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)GAIADR2_OUTPUT=# 2.750 3109049314307207680 105.63950162813 -01.96758727063 13.9169 13.1322 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.750#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283716_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 283716_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 283720_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 283720_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 283722_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 283722_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 07:03:24.15 +01:44:13.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 0.822 3115407858769508864 105.85054732941 +01.73724252246 13.7366 12.8891 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.822#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283726_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 283726_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:43:04.62 +01:03:13.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)GAIADR2_OUTPUT=# 3.441 3125820714918979840 100.76924916467 +01.05284958449 13.7488 12.9598 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.441#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283727_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 283727_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 07:08:32.29 -04:52:12.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 3.013 3059428423269301248 107.13498037393 -04.87093591462 13.8481 13.1876 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.013#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283732_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 283732_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 283733_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 283733_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:51:47.98 -01:23:24.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)GAIADR2_OUTPUT=# 1.977 3112343726021758336 102.94940029937 -01.39027097196 13.8590 13.0180 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.977#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283734_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 283734_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 283737_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 283737_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:45:38.78 -06:15:15.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)GAIADR2_OUTPUT=# 1.751 3100286412791014400 101.41200221884 -06.25441817747 13.6538 13.1805 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.751#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283742_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 283742_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:48:44.34 -04:10:19.4: 12.30 +/- 0.03 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:48:44.34 -04:10:19.4: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 12.30 +/- 0.03
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Considering the candidate 283745_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 283745_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 283747_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 283747_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:55:36.65 -01:03:22.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.07, MAG_FAINT_SEARCH_LIMIT=14.05)GAIADR2_OUTPUT=# 2.459 3112415331715647360 103.90268016435 -01.05696012761 13.7754 12.6606 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.459#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283750_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 283750_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 07:05:27.58 -01:00:11.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)GAIADR2_OUTPUT=# 1.394 3109568623093291648 106.36453423089 -01.00305075955 13.7684 12.8340 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.394#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283752_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 283752_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 283755_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 283755_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:52:04.33 -05:53:12.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.90, MAG_FAINT_SEARCH_LIMIT=13.88)GAIADR2_OUTPUT=# 1.837 3101108259073557760 103.01829861414 -05.88727505251 13.5348 13.0509 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.837#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283756_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 283756_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:39:29.99 -00:09:22.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.94, MAG_FAINT_SEARCH_LIMIT=13.92)GAIADR2_OUTPUT=# 4.803 3119441206717309824 099.87464747814 -00.15749177367 13.7133 12.9001 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.803#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283758_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 283758_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 283764_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 283764_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 07:09:03.79 -01:19:32.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.85, MAG_FAINT_SEARCH_LIMIT=13.83)GAIADR2_OUTPUT=# 2.929 3109387482852637312 107.26623640237 -01.32634810055 13.6962 13.0876 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.929#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283765_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 283765_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 07:05:05.70 -03:34:36.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 2.943 3107823290122505600 106.27336488213 -03.57763826488 13.9752 13.7154 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.943#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283767_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 283767_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 283770_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 283770_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 07:08:52.23 -00:44:32.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.93, MAG_FAINT_SEARCH_LIMIT=13.91)GAIADR2_OUTPUT=# 2.489 3109635113484885248 107.21776257479 -00.74292765116 13.7584 13.3194 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.489#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283776_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 283776_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 283777_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 283777_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 283778_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 283778_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:46:49.00 -00:40:03.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 3.102 3107388433273217536 101.70428377390 -00.66846482585 13.8561 13.4047 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.102#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283785_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 283785_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:54:29.31 -03:35:25.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.06, MAG_FAINT_SEARCH_LIMIT=14.04)GAIADR2_OUTPUT=# 1.860 3102754163561342208 103.62189494822 -03.59079608507 13.8389 12.9507 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.860#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283789_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 283789_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 283790_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 283790_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 07:05:19.30 -01:29:13.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.85, MAG_FAINT_SEARCH_LIMIT=13.83)GAIADR2_OUTPUT=# 3.253 3109468056438096000 106.33034015352 -01.48790042039 13.5034 12.6642 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.253#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283791_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 283791_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 283796_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 283796_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:40:43.57 -01:24:09.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.84, MAG_FAINT_SEARCH_LIMIT=13.82)GAIADR2_OUTPUT=# 2.161 3107274358943072000 100.18166907339 -01.40328102820 13.7805 13.4061 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.161#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283799_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 283799_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 283801_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 283801_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:38:36.78 -02:21:03.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 1.848 3106690209028922496 099.65301746258 -02.35129119740 13.7068 13.1520 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.848#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283802_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 283802_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:47:38.26 -03:41:21.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.81, MAG_FAINT_SEARCH_LIMIT=13.79)
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Considering the candidate 283803_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 283803_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 283804_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 283804_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:54:23.47 -04:11:25.1: 10.44 +/- 0.01 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:54:23.47 -04:11:25.1: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 10.44 +/- 0.01
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Considering the candidate 283806_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 283806_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 283807_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 283807_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 07:06:06.22 -05:15:51.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)GAIADR2_OUTPUT=# 0.942 3053398632783930496 106.52589333582 -05.26456627313 13.5298 13.0497 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.942#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283808_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 283808_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 283809_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 283809_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
Rejecting candidate due to large distance (12.7") between the two second-epoch detections
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Considering the candidate 283810_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 283810_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:40:19.61 +01:45:36.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.76, MAG_FAINT_SEARCH_LIMIT=13.74)GAIADR2_OUTPUT=# 2.682 3126679394843801856 100.08151708014 +01.75936322406 12.9914 11.9342 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.682#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283812_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 283812_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 07:02:40.66 -01:25:21.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.86, MAG_FAINT_SEARCH_LIMIT=13.84)GAIADR2_OUTPUT=# 1.540 3109153630471761792 105.66971000478 -01.42295052539 13.7315 13.4886 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.540#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283814_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 283814_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 07:05:06.01 -04:00:13.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.72, MAG_FAINT_SEARCH_LIMIT=13.70)GAIADR2_OUTPUT=# 2.302 3107769203592227584 106.27515859253 -04.00446217511 13.6174 13.0843 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.302#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283816_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 283816_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 07:09:03.67 -00:36:18.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)GAIADR2_OUTPUT=# 2.005 3109644386314358144 107.26497435016 -00.60570780031 13.6141 13.0161 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.005#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283820_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 283820_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 283822_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 283822_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 283823_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 283823_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:46:17.88 +02:17:52.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.66, MAG_FAINT_SEARCH_LIMIT=13.64)GAIADR2_OUTPUT=# 1.858 3126420670311196160 101.57442198979 +02.29746190754 13.5646 12.9689 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.858#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283825_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 283825_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 283828_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 283828_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 283830_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 283830_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 283835_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 283835_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 283838_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 283838_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 283840_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 283840_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 283842_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 283842_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:47:10.56 -03:58:21.1: 12.46 +/- 0.04 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:47:10.56 -03:58:21.1: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 12.46 +/- 0.04
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Considering the candidate 283849_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 283849_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 283850_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 283850_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 283851_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 283851_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 283853_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 283853_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 283854_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 283854_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 283856_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 283856_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 283858_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 283858_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:44:22.49 -00:41:09.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.60, MAG_FAINT_SEARCH_LIMIT=13.58)GAIADR2_OUTPUT=# 2.990 3107422999169573888 101.09402970642 -00.68659923376 13.1689 12.3844 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.990#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283860_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 283860_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:53:17.30 -02:59:40.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.52, MAG_FAINT_SEARCH_LIMIT=13.50)
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Considering the candidate 283861_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 283861_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
Rejecting candidate due to large distance (21.1") between the two second-epoch detections
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Considering the candidate 283862_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 283862_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 283863_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 283863_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:48:31.46 -04:05:32.5: 11.75 +/- 0.02 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:48:31.46 -04:05:32.5: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 11.75 +/- 0.02
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Considering the candidate 283865_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 283865_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 07:08:43.59 +01:59:20.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.59, MAG_FAINT_SEARCH_LIMIT=13.57)GAIADR2_OUTPUT=# 3.035 3114730628324738432 107.18117361815 +01.98960102822 13.4946 12.6526 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.035#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283868_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 283868_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 283871_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 283871_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 283875_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 283875_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 283876_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 283876_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 283877_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 283877_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 283880_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 283880_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 283884_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 283884_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:57:23.14 -00:34:38.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.60, MAG_FAINT_SEARCH_LIMIT=13.58)GAIADR2_OUTPUT=# 2.178 3112466214186931456 104.34660264398 -00.57788112600 13.5547 13.2633 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.178#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283885_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 283885_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 07:07:25.40 +02:12:20.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.56, MAG_FAINT_SEARCH_LIMIT=13.54)GAIADR2_OUTPUT=# 1.161 3114795327712115072 106.85615195023 +02.20564379253 13.4253 12.6756 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.161#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283887_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 283887_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 283890_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 283890_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 283891_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 283891_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:54:01.76 -00:11:57.1: 12.93 +/- 0.06 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:54:01.76 -00:11:57.1: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 12.93 +/- 0.06
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Considering the candidate 283894_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 283894_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:49:46.78 -00:33:13.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.51, MAG_FAINT_SEARCH_LIMIT=13.49)GAIADR2_OUTPUT=# 2.349 3113199352226204672 102.44499550161 -00.55439773710 13.4120 12.8854 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.349#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283895_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 283895_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:57:07.19 +00:11:05.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.44, MAG_FAINT_SEARCH_LIMIT=13.42)GAIADR2_OUTPUT=# 2.762 3113685164567882624 104.27949820848 +00.18435819526 12.7771 11.5845 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.762#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283896_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 283896_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 07:01:13.02 -05:30:39.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.48, MAG_FAINT_SEARCH_LIMIT=13.46)GAIADR2_OUTPUT=# 1.401 3101370496899876736 105.30446381534 -05.51129812120 13.3660 12.6653 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.401#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283897_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 283897_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:49:08.70 +00:42:49.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.57, MAG_FAINT_SEARCH_LIMIT=13.55)GAIADR2_OUTPUT=# 3.059 3113634243433657472 102.28627901066 +00.71284521586 13.1110 12.2193 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.059#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283898_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 283898_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 283899_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 283899_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:57:53.29 -00:24:37.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 2.455 3112475323818314752 104.47188036842 -00.41113470113 13.3040 12.4449 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.455#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283902_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 283902_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:04:06.67 -06:07:38.9: 13.23 +/- 0.11 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:04:06.67 -06:07:38.9: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 13.23 +/- 0.11
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Considering the candidate 283906_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 283906_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 283907_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 283907_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 283909_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 283909_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:49:22.86 +01:06:38.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.39, MAG_FAINT_SEARCH_LIMIT=13.37)GAIADR2_OUTPUT=# 1.082 3125681313161965056 102.34535478729 +01.11030157285 13.3610 12.8932 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.082#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283914_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 283914_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 07:00:12.29 -01:48:15.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.40, MAG_FAINT_SEARCH_LIMIT=13.38)GAIADR2_OUTPUT=# 2.313 3109122839844853120 105.05125778979 -01.80505729345 13.2021 12.4583 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.313#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283915_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 283915_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:41:45.09 -01:18:55.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.30, MAG_FAINT_SEARCH_LIMIT=13.28)GAIADR2_OUTPUT=# 3.235 3107234982682679808 100.43805540528 -01.31615820583 13.1525 12.7239 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.235#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283916_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 283916_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 283918_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 283918_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 283919_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 283919_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 07:08:33.05 +00:32:12.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.39, MAG_FAINT_SEARCH_LIMIT=13.37)GAIADR2_OUTPUT=# 1.852 3114294122208651008 107.13787303785 +00.53631806316 13.1529 12.4015 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.852#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283920_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 283920_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 283921_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 283921_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 283922_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 283922_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 283925_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 283925_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 283927_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 283927_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 283928_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 283928_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 07:09:17.96 -05:28:45.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.35, MAG_FAINT_SEARCH_LIMIT=13.33)GAIADR2_OUTPUT=# 1.561 3053339293515033856 107.32508959536 -05.47973955931 13.3130 12.6436 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.561#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283929_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 283929_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:58:50.32 -01:53:14.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.24, MAG_FAINT_SEARCH_LIMIT=13.22)GAIADR2_OUTPUT=# 3.380 3109030828766502528 104.70977051143 -01.88815536144 13.1130 12.4796 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.380#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283930_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 283930_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:59:30.37 +00:22:06.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.35, MAG_FAINT_SEARCH_LIMIT=13.33)GAIADR2_OUTPUT=# 2.104 3112954092412665728 104.87635027586 +00.36800335858 13.3157 12.8274 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.104#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283932_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 283932_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:40:13.60 +01:34:05.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 1.182 3126640293461251840 100.05661954788 +01.56798053311 12.8907 11.9582 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.182#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283937_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 283937_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 283938_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 283938_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:47:48.66 -03:49:07.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.19, MAG_FAINT_SEARCH_LIMIT=13.17)
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Considering the candidate 283942_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 283942_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 283943_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 283943_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 283945_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 283945_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 283949_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 283949_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 07:06:42.39 -03:09:14.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.03, MAG_FAINT_SEARCH_LIMIT=13.01)GAIADR2_OUTPUT=# 2.769 3107979111536590592 106.67588059035 -03.15417042601 13.0043 12.3122 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.769#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283950_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 283950_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 283952_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 283952_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283954_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 283954_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 283956_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 283956_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 283957_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 283957_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:51:02.36 +01:07:16.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 283958_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 283958_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 283959_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 283959_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:54:08.13 -05:53:01.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 283960_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 283960_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 283961_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 283961_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 283963_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 283963_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 283967_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 283967_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:56:13.87 -05:00:25.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 283968_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 283968_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 283971_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 283971_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 07:08:48.37 +00:19:42.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.64, MAG_FAINT_SEARCH_LIMIT=12.62)GAIADR2_OUTPUT=# 3.309 3114274601576731904 107.20115234593 +00.32769523318 12.5229 11.7962 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.309#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283972_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 283972_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 07:09:05.06 -02:00:18.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.54, MAG_FAINT_SEARCH_LIMIT=12.52)GAIADR2_OUTPUT=# 1.518 3109208739192432768 107.27081890339 -02.00546754613 11.8572 10.7860 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.518#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283973_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 283973_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 283974_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 283974_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 283978_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 283978_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
Rejecting candidate due to large distance (10.8") between the two second-epoch detections
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Considering the candidate 283984_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 283984_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 07:08:35.58 +01:46:44.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 283986_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 283986_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:53:11.73 -01:33:36.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 283987_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 283987_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 07:07:02.74 -05:51:47.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.30, MAG_FAINT_SEARCH_LIMIT=12.28)GAIADR2_OUTPUT=# 1.245 3053304585873439104 106.76166013969 -05.86341342732 12.2758 11.5678 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.245#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283991_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 283991_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 07:08:38.01 -05:29:36.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 283993_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 283993_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 07:07:26.97 -01:50:34.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.34, MAG_FAINT_SEARCH_LIMIT=12.32)GAIADR2_OUTPUT=# 1.540 3109207296085297536 106.86238560713 -01.84331649968 12.1404 11.6766 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.540#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283994_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 283994_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 07:01:24.82 -01:42:51.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.21, MAG_FAINT_SEARCH_LIMIT=12.19)GAIADR2_OUTPUT=# 2.549 3109118373080196224 105.35380665429 -01.71484121383 12.1150 11.6916 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.549#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283996_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 283996_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:58:26.58 -00:54:51.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 283999_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 283999_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 284005_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 284005_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 07:07:49.41 -05:43:07.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 286888_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 286888_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:50:40.18 -00:32:22.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 287143_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 287143_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:45:12.35 -00:01:52.3: 10.68 +/- 0.01 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:45:12.35 -00:01:52.3: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 10.68 +/- 0.01
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Considering the candidate 288531_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 288531_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:51:37.21 +00:26:59.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 289359_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 289359_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:51:39.70 +00:25:32.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 289573_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 289573_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:48:15.53 +01:46:16.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 290288_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 290288_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:40:37.67 +00:43:02.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 290678_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 290678_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:40:30.51 -01:04:42.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291051_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 291051_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 07:04:10.67 -03:14:38.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291648_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 291648_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:50:41.54 -00:33:42.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291712_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 291712_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 07:02:11.23 -06:02:36.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 294003_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 294003_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 294797_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 294797_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:36:41.01 -05:13:21.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 294907_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 294907_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 07:00:03.13 -03:18:51.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.73, MAG_FAINT_SEARCH_LIMIT=12.71)GAIADR2_OUTPUT=# 1.979 3102674856983028992 105.01302286340 -03.31474392753 12.6850 12.0425 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.979#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294929_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 294929_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 07:03:11.90 -02:15:21.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 295269_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 295269_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:53:08.09 -04:35:53.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 295594_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 295594_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 296268_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 296268_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:51:44.47 -04:35:29.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 296468_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 296468_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 07:01:52.70 -01:19:05.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 297152_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 297152_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:45:10.82 -03:57:02.4: 12.33 +/- 0.04 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:45:10.82 -03:57:02.4: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 12.33 +/- 0.04
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Considering the candidate 297229_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 297229_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:50:44.40 -00:31:38.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 298047_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 298047_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 07:01:19.07 -03:06:45.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.08, MAG_FAINT_SEARCH_LIMIT=13.06)GAIADR2_OUTPUT=# 1.311 3108642013970584960 105.32947967388 -03.11291923132 13.0508 12.9273 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.311#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 298071_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 298071_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:53:16.50 +02:11:48.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 298321_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 298321_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 07:09:03.28 -02:29:06.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.21, MAG_FAINT_SEARCH_LIMIT=13.19)GAIADR2_OUTPUT=# 1.970 3108405756407264640 107.26382902829 -02.48563387066 13.1420 12.7775 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#
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Considering the candidate 298572_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 298572_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:54:30.07 -04:07:30.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 298609_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 298609_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:41:30.08 +00:57:45.1: 12.02 +/- 0.03 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:41:30.08 +00:57:45.1: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 12.02 +/- 0.03
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Considering the candidate 298708_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 298708_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:54:09.44 -05:52:26.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 298956_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 298956_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 299190_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 299190_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:43:35.18 -01:19:42.0: 12.16 +/- 0.03 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:43:35.18 -01:19:42.0: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 12.16 +/- 0.03
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Considering the candidate 299283_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 299283_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:45:00.17 -00:03:31.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 299511_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 299511_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 07:02:39.52 -04:37:51.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 299691_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 299691_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:37:58.49 -01:25:24.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 299828_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 299828_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:45:04.71 -01:02:23.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.28, MAG_FAINT_SEARCH_LIMIT=13.26)GAIADR2_OUTPUT=# 2.054 3107346681891637888 101.26967865935 -01.04031808691 13.2059 12.6723 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.054#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 300321_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 300321_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:35:07.07 -01:31:24.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)GAIADR2_OUTPUT=# 4.350 3118812874479474048 098.77860290306 -01.52424273167 13.1457 12.5678 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.350#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 300407_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 300407_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 300603_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 300603_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:35:16.31 -04:45:57.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 300748_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 300748_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 07:02:23.00 +00:25:55.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)GAIADR2_OUTPUT=# 2.254 3113001715010265856 105.59586879156 +00.43145813945 12.8711 12.0519 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.254#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 301119_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 301119_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:56:27.50 +00:06:17.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)GAIADR2_OUTPUT=# 2.350 3113677261828133888 104.11429280310 +00.10422085836 13.1732 12.4789 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.350#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 301345_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 301345_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:38:54.24 +00:00:12.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.28, MAG_FAINT_SEARCH_LIMIT=13.26)GAIADR2_OUTPUT=# 2.311 3119634652045900032 099.72581188348 +00.00294192467 13.1884 12.6963 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.311#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 301761_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 301761_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 301847_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 301847_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 301899_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 301899_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 301957_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 301957_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
Rejecting candidate due to large distance (19.3") between the two second-epoch detections
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Considering the candidate 301958_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 301958_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 302278_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 302278_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 302417_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 302417_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:34:14.95 -05:19:04.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.41, MAG_FAINT_SEARCH_LIMIT=13.39)GAIADR2_OUTPUT=# 1.450 3103462897582381312 098.56209663853 -05.31829740534 13.0894 12.5053 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.450#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 302525_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 302525_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 07:01:22.76 -06:08:19.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.36, MAG_FAINT_SEARCH_LIMIT=13.34)GAIADR2_OUTPUT=# 0.241 3052874406254774656 105.34484077065 -06.13892768243 13.2836 12.7701 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.241#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 302534_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 302534_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:56:45.60 +00:46:08.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 302719_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 302719_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:54:15.12 -05:59:30.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 302837_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 302837_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:40:17.47 -04:25:57.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.41, MAG_FAINT_SEARCH_LIMIT=13.39)GAIADR2_OUTPUT=# 1.581 3103981287255761536 100.07307980311 -04.43283226625 13.2340 12.7718 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.581#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 302993_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 302993_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 303024_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 303024_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 07:05:01.43 +01:48:38.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.35, MAG_FAINT_SEARCH_LIMIT=13.33)GAIADR2_OUTPUT=# 1.399 3114755436055724928 106.25598204354 +01.81022333530 13.0723 12.2193 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.399#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 303198_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 303198_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:47:03.88 -03:46:14.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 303212_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 303212_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 303288_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 303288_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:42:28.70 -06:03:11.0: 13.05 +/- 0.07 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:42:28.70 -06:03:11.0: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 13.05 +/- 0.07
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Considering the candidate 303544_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 303544_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:54:45.31 -01:43:48.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 303554_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 303554_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 07:01:50.89 -01:07:00.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.43, MAG_FAINT_SEARCH_LIMIT=13.41)GAIADR2_OUTPUT=# 1.951 3112551568078572160 105.46258255986 -01.11679803352 13.3869 13.0466 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.951#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 303563_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 303563_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:43:50.50 +01:35:52.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 303704_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 303704_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 07:06:30.36 -06:00:08.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 303942_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 303942_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 303993_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 303993_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 304278_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 304278_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:53:07.26 -01:52:42.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 304297_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 304297_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 304686_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 304686_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 07:02:47.16 -04:14:52.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 304711_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 304711_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:39:36.60 -04:34:36.3: 12.49 +/- 0.05 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:39:36.60 -04:34:36.3: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 12.49 +/- 0.05
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Considering the candidate 304747_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 304747_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 07:01:22.37 -03:06:02.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 304893_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 304893_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:42:03.28 -06:07:19.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 304894_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 304894_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:58:28.12 -05:44:54.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 305073_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 305073_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:58:39.01 -04:20:16.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 2.982 3101710349067118720 104.66302468638 -04.33867408529 13.0563 12.0264 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.982#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 305125_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 305125_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:42:33.19 -03:28:07.1: 12.99 +/- 0.06 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:42:33.19 -03:28:07.1: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 12.99 +/- 0.06
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Considering the candidate 305287_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 305287_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:50:00.06 -03:51:12.4: 12.88 +/- 0.05 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:50:00.06 -03:51:12.4: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 12.88 +/- 0.05
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Considering the candidate 305306_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 305306_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 305413_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 305413_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:46:14.71 -02:18:25.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.59, MAG_FAINT_SEARCH_LIMIT=13.57)GAIADR2_OUTPUT=# 3.580 3106174641154272896 101.56114866774 -02.30809529203 13.4455 12.5508 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.580#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 305635_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 305635_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:42:38.99 -02:16:09.5: 13.38 +/- 0.10 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:42:38.99 -02:16:09.5: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 13.38 +/- 0.10
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Considering the candidate 305643_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 305643_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:45:06.01 -00:02:45.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.59, MAG_FAINT_SEARCH_LIMIT=13.57)GAIADR2_OUTPUT=# 1.778 3107483330569016576 101.27521621046 -00.04654528542 13.5111 12.9685 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.778#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 305838_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 305838_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:44:16.66 -03:13:32.4: 12.72 +/- 0.04 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:44:16.66 -03:13:32.4: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 12.72 +/- 0.04
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Considering the candidate 306249_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 306249_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 306345_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 306345_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:40:19.71 -03:22:50.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.63, MAG_FAINT_SEARCH_LIMIT=13.61)GAIADR2_OUTPUT=# 2.087 3105616604643085952 100.08227451735 -03.38133788963 13.4827 13.0462 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.087#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 306350_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 306350_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 07:02:19.50 -03:20:39.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.66, MAG_FAINT_SEARCH_LIMIT=13.64)GAIADR2_OUTPUT=# 2.327 3108619920658643968 105.58111518078 -03.34490994692 13.4942 12.9329 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.327#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 306360_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 306360_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 306512_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 306512_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 306551_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 306551_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:44:35.92 +01:45:26.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 306753_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 306753_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 306816_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 306816_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:54:23.30 -01:37:01.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.65, MAG_FAINT_SEARCH_LIMIT=13.63)GAIADR2_OUTPUT=# 1.038 3112090426029207936 103.59710334630 -01.61731541411 13.2806 12.4210 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.038#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 306861_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 306861_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:41:18.53 -00:51:04.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 2.617 3107333114094700416 100.32703194946 -00.85181643927 13.5990 13.1234 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.617#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 307248_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 307248_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:52:54.99 -02:23:05.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.57, MAG_FAINT_SEARCH_LIMIT=13.55)GAIADR2_OUTPUT=# 2.376 3106018510504636160 103.22925868247 -02.38539636749 13.5296 12.9702 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.376#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 307340_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 307340_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:40:25.81 -03:31:15.2: 13.04 +/- 0.08 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:40:25.81 -03:31:15.2: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 13.04 +/- 0.08
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Considering the candidate 307381_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 307381_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 07:06:28.66 -05:58:00.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 307453_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 307453_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:54:25.79 -01:06:06.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 307464_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 307464_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 307477_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 307477_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 307879_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 307879_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:49:10.39 -02:16:27.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 307932_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 307932_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:08:59.10 -00:34:32.2: 13.41 +/- 0.10 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:08:59.10 -00:34:32.2: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 13.41 +/- 0.10
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Considering the candidate 307944_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 307944_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 308045_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 308045_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 07:07:12.70 -04:08:07.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.69, MAG_FAINT_SEARCH_LIMIT=13.67)GAIADR2_OUTPUT=# 2.399 3107567000838631936 106.80293572744 -04.13605509089 13.4970 13.0581 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.399#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 308444_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 308444_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:58:24.62 -03:02:35.5 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.73, MAG_FAINT_SEARCH_LIMIT=13.71)
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Considering the candidate 308542_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 308542_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 308559_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 308559_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 308561_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 308561_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 308702_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 308702_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:53:59.62 -02:44:17.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.73, MAG_FAINT_SEARCH_LIMIT=13.71)GAIADR2_OUTPUT=# 2.824 3105945972795426816 103.49787131933 -02.73864765651 13.4074 12.4613 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.824#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 308806_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 308806_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:44:26.10 -06:06:22.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.70, MAG_FAINT_SEARCH_LIMIT=13.68)GAIADR2_OUTPUT=# 4.062 3100303317781995776 101.10954090124 -06.10697565398 13.0595 11.9466 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.062#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 308876_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 308876_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 308904_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 308904_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:03:06.36 -00:13:11.3: 13.30 +/- 0.08 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:03:06.36 -00:13:11.3: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 13.30 +/- 0.08
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Considering the candidate 308905_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 308905_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 07:06:29.54 -05:59:51.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 308957_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 308957_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:39:24.94 +00:07:07.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.86, MAG_FAINT_SEARCH_LIMIT=13.84)GAIADR2_OUTPUT=# 1.307 3119729764098083584 099.85426175068 +00.11897430785 13.7172 12.9279 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.307#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 309021_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 309021_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 309060_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 309060_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 309125_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 309125_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 309296_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 309296_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 309493_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 309493_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:47:10.23 -05:37:13.3: 12.93 +/- 0.06 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:47:10.23 -05:37:13.3: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 12.93 +/- 0.06
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Considering the candidate 309575_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 309575_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 309813_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 309813_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:49:35.81 +01:59:10.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 310021_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 310021_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 310093_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 310093_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 07:01:00.38 -00:27:55.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 2.371 3112649836929196672 105.25161924724 -00.46612989853 13.7232 13.2855 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.371#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 310122_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 310122_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:56:43.09 +02:11:50.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 310226_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 310226_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 310251_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 310251_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 310473_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 310473_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:54:59.54 -01:03:05.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 2.591 3112333791758054272 103.74773607348 -01.05207476769 13.3921 12.4083 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.591#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 310495_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 310495_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:43:42.35 -04:26:31.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 1.832 3105302487915881984 100.92693219573 -04.44232787110 13.7957 13.3898 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.832#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 310531_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 310531_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 07:00:53.36 +02:12:20.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.80, MAG_FAINT_SEARCH_LIMIT=13.78)GAIADR2_OUTPUT=# 3.040 3115684141125661184 105.22312254508 +02.20541996486 13.5853 12.6957 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.040#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 310598_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 310598_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:55:24.46 -05:54:32.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 310780_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 310780_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 07:04:50.28 -01:48:51.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 2.576 3109266055536999040 106.20982338393 -01.81483283230 13.7387 13.2803 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.576#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 311031_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 311031_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 311214_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 311214_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:48:20.45 -00:31:48.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 311266_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 311266_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 311418_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 311418_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:41:46.98 -00:16:15.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.83, MAG_FAINT_SEARCH_LIMIT=13.81)GAIADR2_OUTPUT=# 2.401 3119468149051361920 100.44582555146 -00.27157940447 13.7130 13.3699 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.401#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 311513_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 311513_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:35:57.15 -02:34:26.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 1.070 3106665332578815488 098.98842000814 -02.57393459680 13.6156 12.7486 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.070#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 311550_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 311550_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:46:14.11 +00:45:29.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)GAIADR2_OUTPUT=# 2.733 3125565078465888768 101.55954576647 +00.75816110703 13.9059 12.9956 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.733#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 311587_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 311587_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:42:29.59 -04:08:22.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.81, MAG_FAINT_SEARCH_LIMIT=13.79)GAIADR2_OUTPUT=# 1.496 3105326264854304256 100.62362023901 -04.13992208149 13.6824 12.7988 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.496#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 311614_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 311614_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 311649_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 311649_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 311673_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 311673_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 312114_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 312114_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:44:48.55 +01:46:38.7: 11.21 +/- 0.02 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:44:48.55 +01:46:38.7: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 11.21 +/- 0.02
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Considering the candidate 312361_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 312361_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:52:21.06 -05:34:36.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.00, MAG_FAINT_SEARCH_LIMIT=13.98)GAIADR2_OUTPUT=# 1.776 3101891734129376896 103.08775253888 -05.57718780004 13.3163 12.2056 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.776#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 312513_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 312513_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 312567_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 312567_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 07:03:39.42 -00:16:05.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 3.495 3112714776834452352 105.91520285602 -00.26824174127 13.2419 11.2621 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.495#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 312590_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 312590_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 07:04:24.56 -04:44:38.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.94, MAG_FAINT_SEARCH_LIMIT=13.92)GAIADR2_OUTPUT=# 4.324 3101515254479426176 106.10305967209 -04.74501396050 13.8733 13.4014 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.324#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 312736_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 312736_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 312858_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 312858_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:48:33.34 +01:51:08.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 312867_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 312867_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:40:19.62 -03:15:28.6: 13.09 +/- 0.06 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:40:19.62 -03:15:28.6: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 13.09 +/- 0.06
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Considering the candidate 312899_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 312899_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 312935_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 312935_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 312949_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 312949_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 313162_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 313162_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:39:08.62 -03:48:11.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 2.131 3104098655825331328 099.78608026695 -03.80376338268 13.9078 13.3117 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.131#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 313208_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 313208_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:47:33.74 -06:11:00.9: 12.70 +/- 0.05 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:47:33.74 -06:11:00.9: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 12.70 +/- 0.05
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Considering the candidate 313287_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 313287_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:42:46.38 -02:44:16.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.87, MAG_FAINT_SEARCH_LIMIT=13.85)GAIADR2_OUTPUT=# 1.890 3106508927049985280 100.69338451398 -02.73839649824 13.7626 13.2404 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.890#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 313387_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 313387_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:48:20.95 -03:11:21.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.94, MAG_FAINT_SEARCH_LIMIT=13.92)GAIADR2_OUTPUT=# 2.419 3105495173029126528 102.08747105884 -03.18998084017 13.8439 13.1397 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.419#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 313530_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 313530_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 07:01:10.29 -01:01:15.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.87, MAG_FAINT_SEARCH_LIMIT=13.85)GAIADR2_OUTPUT=# 2.917 3112567987734134144 105.29366963077 -01.02124268361 13.7541 13.2446 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.917#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 313531_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 313531_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:48:53.08 +01:49:28.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 1.799 3126153111029053568 102.22144351024 +01.82425048629 13.8939 13.4215 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.799#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 313618_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 313618_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:46:10.32 -03:14:00.7: 13.24 +/- 0.07 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:46:10.32 -03:14:00.7: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 13.24 +/- 0.07
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Considering the candidate 313714_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 313714_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 313900_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 313900_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 313962_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 313962_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:46:12.54 -05:08:49.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 3.714 3100657291808314112 101.55197132706 -05.14813242199 13.6082 12.7719 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.714#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 314022_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 314022_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:50:01.68 +00:15:03.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.01, MAG_FAINT_SEARCH_LIMIT=13.99)GAIADR2_OUTPUT=# 3.397 3113554838079394432 102.50697226187 +00.24994566152 13.7718 12.8036 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.397#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 314023_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 314023_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:35:06.97 +00:53:04.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)GAIADR2_OUTPUT=# 1.993 3120501896137383424 098.77931044842 +00.88418266888 13.7165 13.1212 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.993#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 314163_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 314163_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:40:25.94 -01:49:07.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.00, MAG_FAINT_SEARCH_LIMIT=13.98)GAIADR2_OUTPUT=# 4.744 3106835447643595264 100.10754055648 -01.81981189803 13.5127 12.5464 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.744#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 314196_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 314196_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:37:13.50 -01:07:57.2: 12.94 +/- 0.05 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:37:13.50 -01:07:57.2: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 12.94 +/- 0.05
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Considering the candidate 314249_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 314249_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:59:49.70 -06:00:37.1: 13.04 +/- 0.08 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:59:49.70 -06:00:37.1: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 13.04 +/- 0.08
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Considering the candidate 314285_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 314285_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 07:06:54.11 +02:10:48.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 314486_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 314486_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 314529_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 314529_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 07:06:38.54 -00:36:58.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 1.797 3109678956510644992 106.66014041170 -00.61650773442 13.7470 12.8165 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.797#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 314575_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 314575_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:58:56.87 -01:06:47.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.07, MAG_FAINT_SEARCH_LIMIT=14.05)GAIADR2_OUTPUT=# 2.425 3112234943088845952 104.73669433005 -01.11373099072 13.8605 13.4601 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.425#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 314631_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 314631_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 314855_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 314855_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 314951_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 314951_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 07:08:49.30 +00:27:16.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 1.598 3114279519319862400 107.20543385668 +00.45405634620 13.8903 13.4119 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.598#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 314972_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 314972_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 07:01:26.77 -00:55:27.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 2.190 3112570461635443584 105.36207810215 -00.92448145232 13.7792 12.9935 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.190#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 315201_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 315201_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 315224_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 315224_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:41:20.86 -01:43:18.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 2.066 3106831942950099584 100.33652100745 -01.72233248144 13.6881 12.6456 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.066#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 315453_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 315453_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 315472_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 315472_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:37:33.18 +01:24:38.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 2.674 3120687370005889280 099.38804092931 +01.40995382945 13.9336 13.3825 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.674#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 316018_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 316018_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 07:07:26.73 -02:55:50.1 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.95, MAG_FAINT_SEARCH_LIMIT=13.93)
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Considering the candidate 316093_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 316093_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:37:39.73 -03:41:21.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.08, MAG_FAINT_SEARCH_LIMIT=14.06)GAIADR2_OUTPUT=# 4.343 3104851168454225536 099.41476409075 -03.69025718129 13.7704 12.8283 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.343#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 316128_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 316128_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:57:35.61 +01:13:52.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 4.110 3113913996123980800 104.39787524035 +01.23033451357 14.0646 13.7846 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.110#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 316312_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 316312_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:45:33.64 -00:26:17.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 3.897 3107451723910491520 101.39020146722 -00.43924863840 14.0394 13.6227 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.897#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 316377_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 316377_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:54:22.91 -02:46:56.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 3.497 3105945010722645376 103.59538251039 -02.78344079194 13.4180 12.3250 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.497#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 316422_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 316422_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 07:09:39.34 -01:21:49.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 3.474 3109339619737041536 107.41478777276 -01.36419332163 13.8942 13.1712 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.474#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 316481_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 316481_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 316631_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 316631_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:43:55.42 -05:04:03.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)GAIADR2_OUTPUT=# 1.273 3100716802874635136 100.98061063149 -05.06745965125 14.0739 13.7942 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.273#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 316667_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 316667_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 07:03:46.74 -01:04:51.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)GAIADR2_OUTPUT=# 1.193 3109553199868724224 105.94499944489 -01.08113492279 14.0995 13.5489 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.193#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 316825_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 316825_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:50:36.98 -01:46:53.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.17, MAG_FAINT_SEARCH_LIMIT=14.15)GAIADR2_OUTPUT=# 2.780 3106322662908980736 102.65406281871 -01.78241089868 14.1429 13.7557 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.780#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 316900_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 316900_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 316988_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 316988_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 317123_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 317123_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 317218_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 317218_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:51:48.66 -04:02:32.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.06, MAG_FAINT_SEARCH_LIMIT=14.04)GAIADR2_OUTPUT=# 2.212 3102343049290484992 102.95330842454 -04.04267620034 13.9995 13.2065 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.212#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 317453_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 317453_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:50:32.84 -01:45:42.0: 11.23 +/- 0.01 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:50:32.84 -01:45:42.0: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 11.23 +/- 0.01
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Considering the candidate 317489_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 317489_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 07:02:01.06 -00:33:55.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)GAIADR2_OUTPUT=# 1.660 3112656021682569600 105.50481814040 -00.56507854051 13.8943 13.0707 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.660#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 317494_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 317494_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:51:34.20 -01:39:24.7: 12.98 +/- 0.06 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:51:34.20 -01:39:24.7: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 12.98 +/- 0.06
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Considering the candidate 317497_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 317497_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:47:04.05 +01:58:35.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 317630_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 317630_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 317736_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 317736_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:35:10.20 -00:43:20.0: 13.56 +/- 0.11 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:35:10.20 -00:43:20.0: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 13.56 +/- 0.11
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Considering the candidate 317820_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 317820_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:49:24.53 -00:56:18.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.30, MAG_FAINT_SEARCH_LIMIT=14.28)GAIADR2_OUTPUT=# 1.719 3107130769594752128 102.35183201837 -00.93873825599 14.2056 13.6642 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.719#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 317936_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 317936_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:48:56.85 -03:30:58.4: 12.37 +/- 0.03 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:48:56.85 -03:30:58.4: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 12.37 +/- 0.03
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Considering the candidate 318012_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 318012_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:39:41.56 -01:32:16.1: 13.04 +/- 0.06 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:39:41.56 -01:32:16.1: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 13.04 +/- 0.06
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Considering the candidate 318165_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 318165_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 318272_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 318272_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 318552_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 318552_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:42:56.76 -02:49:56.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)GAIADR2_OUTPUT=# 1.384 3105756758015606784 100.73661177352 -02.83259014075 14.1330 13.5956 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.384#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 318663_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 318663_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:49:20.22 -05:56:13.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 3.985 3100367879732234240 102.33434054124 -05.93815871466 14.0187 12.9401 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.985#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 318737_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 318737_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 319246_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 319246_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:53:47.78 +00:29:50.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 0.965 3113390186212355840 103.44929652812 +00.49714290746 14.1518 13.6648 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.965#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 319323_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 319323_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:58:20.37 -00:32:39.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 2.230 3112460617850838784 104.58465531557 -00.54491251100 14.1966 13.6113 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.230#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 319472_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 319472_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 319532_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 319532_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 319623_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 319623_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 319971_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 319971_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:59:45.78 -03:24:18.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 3.240 3102672387384334464 104.94054368107 -03.40607048421 14.1574 13.6542 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.240#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 320137_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 320137_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 320172_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 320172_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 320319_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 320319_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:59:36.45 -03:22:53.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 1.417 3102673379515556224 104.90194329535 -03.38191555110 14.3076 13.6031 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.417#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 320328_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 320328_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:59:23.82 -01:22:04.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)GAIADR2_OUTPUT=# 5.464 3112157083922470272 104.84972239633 -01.36944247534 14.3800 13.4938 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.464#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 320336_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 320336_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:49:54.59 +02:12:16.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 320409_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 320409_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 320620_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 320620_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 320666_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 320666_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:50:32.98 -01:45:21.8: 10.39 +/- 0.00 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:50:32.98 -01:45:21.8: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 10.39 +/- 0.00
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Considering the candidate 320713_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 320713_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 321172_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 321172_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 321317_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 321317_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:57:52.40 -02:41:34.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)GAIADR2_OUTPUT=# 2.564 3108914417973693568 104.46791192837 -02.69335244921 14.2020 13.6689 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.564#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 321343_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 321343_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:53:47.16 -02:38:44.3: 11.08 +/- 0.01 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:53:47.16 -02:38:44.3: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 11.08 +/- 0.01
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Considering the candidate 321354_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 321354_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 321707_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 321707_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 07:08:59.98 -01:54:17.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 2.700 3109214515930298368 107.24941075468 -01.90538722625 13.9700 13.5046 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.700#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 321797_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 321797_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 321983_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 321983_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 322077_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 322077_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 07:04:35.22 -02:55:36.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)GAIADR2_OUTPUT=# 2.574 3108751518456730240 106.14659876532 -02.92747671806 14.4783 13.9795 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.574#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 322298_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 322298_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:47:04.21 +01:23:19.7: 13.77 +/- 0.12 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:47:04.21 +01:23:19.7: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 13.77 +/- 0.12
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Considering the candidate 322317_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 322317_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:56:47.27 +00:29:41.3 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.61, MAG_FAINT_SEARCH_LIMIT=14.59)
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Considering the candidate 322424_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 322424_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 07:05:22.91 -02:34:19.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.75, MAG_FAINT_SEARCH_LIMIT=14.73)GAIADR2_OUTPUT=# 2.691 3108767731951448832 106.34518519799 -02.57266825557 14.5088 14.1876 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.691#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 322461_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 322461_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 322475_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 322475_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 322637_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
Preparing report for the candidate 322637_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
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Considering the candidate 322668_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 322668_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:55:37.81 -01:51:09.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 3.027 3112067439364877824 103.90737594518 -01.85351887980 14.6026 13.8632 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.027#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 322763_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 322763_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:39:46.09 -02:14:00.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.80, MAG_FAINT_SEARCH_LIMIT=14.78)GAIADR2_OUTPUT=# 2.221 3106783152122101120 099.94209701518 -02.23397557183 14.5512 13.9164 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.221#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 322781_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 322781_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:50:50.95 +00:13:18.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.70, MAG_FAINT_SEARCH_LIMIT=14.68)GAIADR2_OUTPUT=# 1.875 3113542812171630592 102.71226484202 +00.22120217560 14.6311 13.7524 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.875#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 47889_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 47889_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:44:47.57 -05:17:44.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 121122_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 121122_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 07:09:13.61 -02:21:31.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 199360_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 199360_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 07:08:45.31 +00:41:48.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 154583_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 154583_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:41:59.23 -01:11:08.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31804_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 31804_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:37:53.15 -05:55:16.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 228912_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027
The candidate 228912_fd_Mon-02-Q2b1x1_2026-04-21_21-37-26_20.00sec_-4.90C_LIGHT_0027 did not pass the final checks
**** FOUND 06:50:00.72 +01:46:33.4 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 10s
make_report_in_HTML.sh TOTAL: 388s
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 ####
07:01:16.43 -02:28:44.5
07:06:43.76 -04:24:09.9
07:06:39.40 -03:57:46.9
06:51:11.47 -02:22:10.2
06:50:51.74 -05:58:27.0
06:57:07.07 -00:31:51.3
06:55:04.55 -00:42:42.4
06:57:04.33 -04:03:27.8
06:58:39.27 -01:55:30.2
06:50:09.67 -01:21:55.2
06:58:57.82 -01:46:10.4
06:56:27.45 -01:27:42.6
06:53:22.56 -03:34:23.0
07:03:39.67 -04:38:24.6
06:46:25.32 +00:47:27.1
06:57:40.53 -03:53:12.3
06:43:45.59 +00:35:15.7
07:05:19.95 -02:51:43.1
07:08:17.17 -04:56:02.0
07:03:23.86 -00:39:18.2
06:53:30.37 -03:06:08.7
06:58:27.06 -03:14:41.3
06:52:00.95 +01:29:15.8
06:53:41.51 -01:02:04.6
06:53:46.06 -00:14:32.6
06:54:41.07 -02:07:02.7
06:58:39.32 +01:21:59.1
06:53:33.71 -00:32:06.2
07:05:03.97 -03:53:19.5
07:02:01.24 -00:36:16.1
06:54:14.55 -01:36:53.2
06:48:07.59 -00:40:39.3
07:03:25.13 -05:00:42.0
07:07:04.81 -03:10:08.0
06:51:10.39 +01:05:57.7
06:53:04.49 -05:33:23.4
06:57:24.02 -00:50:14.8
06:55:03.18 -01:02:50.8
07:04:08.47 -05:07:03.8
06:42:40.75 -00:18:15.0
07:08:48.84 -03:43:02.7
07:09:10.38 -01:30:23.5
06:46:00.22 -00:22:10.0
06:41:44.19 +00:27:30.3
06:46:13.83 +00:50:42.9
07:07:06.80 +01:39:59.8
07:07:51.34 -05:46:59.8
06:54:34.23 -01:51:46.6
06:49:52.39 -02:39:53.8
06:51:28.75 +01:57:02.8
07:09:08.39 -01:41:28.4
07:08:32.25 -04:39:28.5
07:03:24.00 -02:49:52.4
07:08:02.96 -03:23:39.4
07:02:17.20 -03:49:24.9
06:35:07.33 -03:03:04.3
06:59:20.97 -05:44:56.3
06:46:12.55 +00:51:08.4
07:05:12.07 -06:04:40.3
06:43:16.49 +00:21:47.9
06:58:25.41 -02:40:33.6
07:03:47.18 -03:20:30.1
07:03:27.01 -05:01:13.8
07:00:51.92 +00:11:59.2
07:05:18.12 -01:23:00.0
07:07:47.22 -05:40:38.7
07:06:22.80 -01:49:60.0
06:59:00.64 -01:40:01.6
07:05:04.23 -05:27:55.4
07:06:54.66 -04:13:51.4
07:05:50.91 -02:05:14.1
06:57:16.40 -00:59:39.3
07:03:38.51 -02:31:49.4
06:44:34.00 -01:35:29.5
07:01:00.94 -00:25:45.2
06:52:10.08 +00:34:37.5
07:07:48.03 +00:24:43.0
06:57:47.57 -01:31:07.0
07:02:21.31 -04:03:31.7
06:54:34.42 -00:35:22.5
06:40:55.24 +00:01:26.5
07:08:39.11 -02:25:42.0
07:06:17.15 +02:00:15.3
06:48:50.52 -00:08:31.2
06:51:05.09 -01:41:34.8
06:49:33.17 -01:23:31.3
07:02:17.59 -03:14:33.0
07:03:52.65 -06:00:24.6
06:57:11.84 -03:58:12.7
06:52:57.33 -03:04:56.9
06:59:52.78 -04:47:26.6
06:58:45.60 -02:28:56.6
07:00:01.21 -05:09:19.3
06:56:22.04 -00:53:11.9
07:04:10.05 -05:04:53.6
06:48:48.44 +00:23:30.4
06:44:24.88 -00:04:50.0
06:44:39.61 +00:10:06.3
07:08:43.09 -05:05:29.5
07:07:48.91 -05:43:38.0
07:02:14.45 -03:05:58.9
06:58:50.14 -04:41:12.9
06:56:02.56 -03:13:02.6
06:56:49.00 +00:46:32.6
06:48:30.53 +00:57:43.9
07:06:11.94 +00:18:33.4
06:57:07.69 +00:36:02.2
06:59:33.41 +01:05:00.1
06:57:09.41 -01:07:39.1
06:57:24.09 -02:57:03.8
07:04:16.73 -03:01:39.2
06:57:12.35 -03:57:46.0
07:04:56.05 -05:21:48.3
06:58:35.36 -04:20:30.2
06:51:18.23 -01:23:09.2
06:58:22.44 -02:33:53.3
06:46:50.64 +01:18:07.4
06:54:41.81 -02:41:58.2
06:48:34.35 +01:51:39.4
06:54:49.49 -01:15:54.9
06:59:43.78 +00:17:12.0
07:07:56.30 -01:30:30.4
06:50:44.76 -00:05:16.4
06:48:45.22 +01:09:18.8
06:49:56.14 -02:40:54.9
06:49:07.39 -01:40:18.4
06:50:00.96 -03:51:50.3
06:53:06.38 -01:03:37.0
06:52:51.68 -02:22:45.6
06:51:37.26 +01:28:59.1
07:01:22.89 -05:01:12.6
06:59:44.33 -01:15:44.8
07:05:38.49 +01:26:02.4
06:53:41.40 -00:33:48.6
06:38:52.43 +01:12:24.1
06:55:11.64 +00:56:23.6
07:01:34.77 -00:37:08.1
06:47:46.40 -02:22:20.5
06:39:28.94 +00:31:16.8
06:41:21.30 -00:35:23.5
06:51:51.87 -04:03:49.1
06:59:32.96 -02:32:38.2
06:54:32.31 -02:12:21.7
06:45:00.74 +00:14:03.0
06:55:19.67 -00:57:48.9
06:47:11.78 +00:21:18.4
06:57:11.48 -01:07:45.1
06:51:56.27 -01:17:01.1
06:56:49.62 -05:48:25.6
06:59:38.68 -00:49:25.6
06:48:35.53 -03:42:40.1
07:05:52.55 -00:01:01.8
07:02:48.91 -01:46:40.0
06:45:12.00 +00:20:57.6
06:51:44.75 -03:39:22.9
06:58:34.68 -01:38:25.6
########### 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 ####
07:01:16.43 -02:28:44.5
07:06:43.76 -04:24:09.9
07:06:39.40 -03:57:46.9
06:51:11.47 -02:22:10.2
06:50:51.74 -05:58:27.0
06:57:07.07 -00:31:51.3
06:55:04.55 -00:42:42.4
06:57:04.33 -04:03:27.8
06:58:39.27 -01:55:30.2
06:50:09.67 -01:21:55.2
06:58:57.82 -01:46:10.4
06:56:27.45 -01:27:42.6
06:53:22.56 -03:34:23.0
07:03:39.67 -04:38:24.6
06:46:25.32 +00:47:27.1
06:57:40.53 -03:53:12.3
06:43:45.59 +00:35:15.7
07:05:19.95 -02:51:43.1
07:08:17.17 -04:56:02.0
07:03:23.86 -00:39:18.2
06:53:30.37 -03:06:08.7
06:58:27.06 -03:14:41.3
06:52:00.95 +01:29:15.8
06:53:41.51 -01:02:04.6
06:53:46.06 -00:14:32.6
06:54:41.07 -02:07:02.7
06:58:39.32 +01:21:59.1
06:53:33.71 -00:32:06.2
07:05:03.97 -03:53:19.5
07:02:01.24 -00:36:16.1
06:54:14.55 -01:36:53.2
06:48:07.59 -00:40:39.3
07:03:25.13 -05:00:42.0
07:07:04.81 -03:10:08.0
06:51:10.39 +01:05:57.7
06:53:04.49 -05:33:23.4
06:57:24.02 -00:50:14.8
06:55:03.18 -01:02:50.8
07:04:08.47 -05:07:03.8
06:42:40.75 -00:18:15.0
07:08:48.84 -03:43:02.7
07:09:10.38 -01:30:23.5
06:46:00.22 -00:22:10.0
06:41:44.19 +00:27:30.3
06:46:13.83 +00:50:42.9
07:07:06.80 +01:39:59.8
07:07:51.34 -05:46:59.8
06:54:34.23 -01:51:46.6
06:49:52.39 -02:39:53.8
06:51:28.75 +01:57:02.8
07:09:08.39 -01:41:28.4
07:08:32.25 -04:39:28.5
07:03:24.00 -02:49:52.4
07:08:02.96 -03:23:39.4
07:02:17.20 -03:49:24.9
06:35:07.33 -03:03:04.3
06:59:20.97 -05:44:56.3
06:46:12.55 +00:51:08.4
07:05:12.07 -06:04:40.3
06:43:16.49 +00:21:47.9
06:58:25.41 -02:40:33.6
07:03:47.18 -03:20:30.1
07:03:27.01 -05:01:13.8
07:00:51.92 +00:11:59.2
07:05:18.12 -01:23:00.0
07:07:47.22 -05:40:38.7
07:06:22.80 -01:49:60.0
06:59:00.64 -01:40:01.6
07:05:04.23 -05:27:55.4
07:06:54.66 -04:13:51.4
07:05:50.91 -02:05:14.1
06:57:16.40 -00:59:39.3
07:03:38.51 -02:31:49.4
06:44:34.00 -01:35:29.5
07:01:00.94 -00:25:45.2
06:52:10.08 +00:34:37.5
07:07:48.03 +00:24:43.0
06:57:47.57 -01:31:07.0
07:02:21.31 -04:03:31.7
06:54:34.42 -00:35:22.5
06:40:55.24 +00:01:26.5
07:08:39.11 -02:25:42.0
07:06:17.15 +02:00:15.3
06:48:50.52 -00:08:31.2
06:51:05.09 -01:41:34.8
06:49:33.17 -01:23:31.3
07:02:17.59 -03:14:33.0
07:03:52.65 -06:00:24.6
06:57:11.84 -03:58:12.7
06:52:57.33 -03:04:56.9
06:59:52.78 -04:47:26.6
06:58:45.60 -02:28:56.6
07:00:01.21 -05:09:19.3
06:56:22.04 -00:53:11.9
07:04:10.05 -05:04:53.6
06:48:48.44 +00:23:30.4
06:44:24.88 -00:04:50.0
06:44:39.61 +00:10:06.3
07:08:43.09 -05:05:29.5
07:07:48.91 -05:43:38.0
07:02:14.45 -03:05:58.9
06:58:50.14 -04:41:12.9
06:56:02.56 -03:13:02.6
06:56:49.00 +00:46:32.6
06:48:30.53 +00:57:43.9
07:06:11.94 +00:18:33.4
06:57:07.69 +00:36:02.2
06:59:33.41 +01:05:00.1
06:57:09.41 -01:07:39.1
06:57:24.09 -02:57:03.8
07:04:16.73 -03:01:39.2
06:57:12.35 -03:57:46.0
07:04:56.05 -05:21:48.3
06:58:35.36 -04:20:30.2
06:51:18.23 -01:23:09.2
06:58:22.44 -02:33:53.3
06:46:50.64 +01:18:07.4
06:54:41.81 -02:41:58.2
06:48:34.35 +01:51:39.4
06:54:49.49 -01:15:54.9
06:59:43.78 +00:17:12.0
07:07:56.30 -01:30:30.4
06:50:44.76 -00:05:16.4
06:48:45.22 +01:09:18.8
06:49:56.14 -02:40:54.9
06:49:07.39 -01:40:18.4
06:50:00.96 -03:51:50.3
06:53:06.38 -01:03:37.0
06:52:51.68 -02:22:45.6
06:51:37.26 +01:28:59.1
07:01:22.89 -05:01:12.6
06:59:44.33 -01:15:44.8
07:05:38.49 +01:26:02.4
06:53:41.40 -00:33:48.6
06:38:52.43 +01:12:24.1
06:55:11.64 +00:56:23.6
07:01:34.77 -00:37:08.1
06:47:46.40 -02:22:20.5
06:39:28.94 +00:31:16.8
06:41:21.30 -00:35:23.5
06:51:51.87 -04:03:49.1
06:59:32.96 -02:32:38.2
06:54:32.31 -02:12:21.7
06:45:00.74 +00:14:03.0
06:55:19.67 -00:57:48.9
06:47:11.78 +00:21:18.4
06:57:11.48 -01:07:45.1
06:51:56.27 -01:17:01.1
06:56:49.62 -05:48:25.6
06:59:38.68 -00:49:25.6
06:48:35.53 -03:42:40.1
07:05:52.55 -00:01:01.8
07:02:48.91 -01:46:40.0
06:45:12.00 +00:20:57.6
06:51:44.75 -03:39:22.9
06:58:34.68 -01:38:25.6
###################################################################################
07:01:16.43 -02:28:44.5 -- not an asteroid (will add it to exclusion list)
07:06:43.76 -04:24:09.9 -- not an asteroid (will add it to exclusion list)
07:06:39.40 -03:57:46.9 -- not an asteroid (will add it to exclusion list)
06:51:11.47 -02:22:10.2 -- not an asteroid (will add it to exclusion list)
06:50:51.74 -05:58:27.0 -- not an asteroid (will add it to exclusion list)
06:57:07.07 -00:31:51.3 -- not an asteroid (will add it to exclusion list)
06:55:04.55 -00:42:42.4 -- not an asteroid (will add it to exclusion list)
06:57:04.33 -04:03:27.8 -- not an asteroid (will add it to exclusion list)
06:58:39.27 -01:55:30.2 -- not an asteroid (will add it to exclusion list)
06:50:09.67 -01:21:55.2 -- not an asteroid (will add it to exclusion list)
06:58:57.82 -01:46:10.4 -- not an asteroid (will add it to exclusion list)
06:56:27.45 -01:27:42.6 -- not an asteroid (will add it to exclusion list)
06:53:22.56 -03:34:23.0 -- not an asteroid (will add it to exclusion list)
07:03:39.67 -04:38:24.6 -- not an asteroid (will add it to exclusion list)
06:46:25.32 +00:47:27.1 -- not an asteroid (will add it to exclusion list)
06:57:40.53 -03:53:12.3 -- not an asteroid (will add it to exclusion list)
06:43:45.59 +00:35:15.7 -- not an asteroid (will add it to exclusion list)
07:05:19.95 -02:51:43.1 -- not an asteroid (will add it to exclusion list)
07:08:17.17 -04:56:02.0 -- not an asteroid (will add it to exclusion list)
07:03:23.86 -00:39:18.2 -- not an asteroid (will add it to exclusion list)
06:53:30.37 -03:06:08.7 -- not an asteroid (will add it to exclusion list)
06:58:27.06 -03:14:41.3 -- not an asteroid (will add it to exclusion list)
06:52:00.95 +01:29:15.8 -- not an asteroid (will add it to exclusion list)
06:53:41.51 -01:02:04.6 -- not an asteroid (will add it to exclusion list)
06:53:46.06 -00:14:32.6 -- not an asteroid (will add it to exclusion list)
06:54:41.07 -02:07:02.7 -- not an asteroid (will add it to exclusion list)
06:58:39.32 +01:21:59.1 -- not an asteroid (will add it to exclusion list)
06:53:33.71 -00:32:06.2 -- not an asteroid (will add it to exclusion list)
07:05:03.97 -03:53:19.5 -- not an asteroid (will add it to exclusion list)
07:02:01.24 -00:36:16.1 -- not an asteroid (will add it to exclusion list)
06:54:14.55 -01:36:53.2 -- not an asteroid (will add it to exclusion list)
06:48:07.59 -00:40:39.3 -- not an asteroid (will add it to exclusion list)
07:03:25.13 -05:00:42.0 -- not an asteroid (will add it to exclusion list)
07:07:04.81 -03:10:08.0 -- not an asteroid (will add it to exclusion list)
06:51:10.39 +01:05:57.7 -- not an asteroid (will add it to exclusion list)
06:53:04.49 -05:33:23.4 -- not an asteroid (will add it to exclusion list)
06:57:24.02 -00:50:14.8 -- not an asteroid (will add it to exclusion list)
06:55:03.18 -01:02:50.8 -- not an asteroid (will add it to exclusion list)
07:04:08.47 -05:07:03.8 -- not an asteroid (will add it to exclusion list)
06:42:40.75 -00:18:15.0 -- not an asteroid (will add it to exclusion list)
07:08:48.84 -03:43:02.7 -- not an asteroid (will add it to exclusion list)
07:09:10.38 -01:30:23.5 -- not an asteroid (will add it to exclusion list)
06:46:00.22 -00:22:10.0 -- not an asteroid (will add it to exclusion list)
06:41:44.19 +00:27:30.3 -- not an asteroid (will add it to exclusion list)
06:46:13.83 +00:50:42.9 -- not an asteroid (will add it to exclusion list)
07:07:06.80 +01:39:59.8 -- not an asteroid (will add it to exclusion list)
07:07:51.34 -05:46:59.8 -- not an asteroid (will add it to exclusion list)
06:54:34.23 -01:51:46.6 -- not an asteroid (will add it to exclusion list)
06:49:52.39 -02:39:53.8 -- not an asteroid (will add it to exclusion list)
06:51:28.75 +01:57:02.8 -- not an asteroid (will add it to exclusion list)
07:09:08.39 -01:41:28.4 -- not an asteroid (will add it to exclusion list)
07:08:32.25 -04:39:28.5 -- not an asteroid (will add it to exclusion list)
07:03:24.00 -02:49:52.4 -- not an asteroid (will add it to exclusion list)
07:08:02.96 -03:23:39.4 -- not an asteroid (will add it to exclusion list)
07:02:17.20 -03:49:24.9 -- not an asteroid (will add it to exclusion list)
06:35:07.33 -03:03:04.3 -- not an asteroid (will add it to exclusion list)
06:59:20.97 -05:44:56.3 -- not an asteroid (will add it to exclusion list)
06:46:12.55 +00:51:08.4 -- not an asteroid (will add it to exclusion list)
07:05:12.07 -06:04:40.3 -- not an asteroid (will add it to exclusion list)
06:43:16.49 +00:21:47.9 -- not an asteroid (will add it to exclusion list)
06:58:25.41 -02:40:33.6 -- not an asteroid (will add it to exclusion list)
07:03:47.18 -03:20:30.1 -- not an asteroid (will add it to exclusion list)
07:03:27.01 -05:01:13.8 -- not an asteroid (will add it to exclusion list)
07:00:51.92 +00:11:59.2 -- not an asteroid (will add it to exclusion list)
07:05:18.12 -01:23:00.0 -- not an asteroid (will add it to exclusion list)
07:07:47.22 -05:40:38.7 -- not an asteroid (will add it to exclusion list)
07:06:22.80 -01:49:60.0 -- not an asteroid (will add it to exclusion list)
06:59:00.64 -01:40:01.6 -- not an asteroid (will add it to exclusion list)
07:05:04.23 -05:27:55.4 -- not an asteroid (will add it to exclusion list)
07:06:54.66 -04:13:51.4 -- not an asteroid (will add it to exclusion list)
07:05:50.91 -02:05:14.1 -- not an asteroid (will add it to exclusion list)
06:57:16.40 -00:59:39.3 -- not an asteroid (will add it to exclusion list)
07:03:38.51 -02:31:49.4 -- not an asteroid (will add it to exclusion list)
06:44:34.00 -01:35:29.5 -- not an asteroid (will add it to exclusion list)
07:01:00.94 -00:25:45.2 -- not an asteroid (will add it to exclusion list)
06:52:10.08 +00:34:37.5 -- not an asteroid (will add it to exclusion list)
07:07:48.03 +00:24:43.0 -- not an asteroid (will add it to exclusion list)
06:57:47.57 -01:31:07.0 -- not an asteroid (will add it to exclusion list)
07:02:21.31 -04:03:31.7 -- not an asteroid (will add it to exclusion list)
06:54:34.42 -00:35:22.5 -- not an asteroid (will add it to exclusion list)
06:40:55.24 +00:01:26.5 -- not an asteroid (will add it to exclusion list)
07:08:39.11 -02:25:42.0 -- not an asteroid (will add it to exclusion list)
07:06:17.15 +02:00:15.3 -- not an asteroid (will add it to exclusion list)
06:48:50.52 -00:08:31.2 -- not an asteroid (will add it to exclusion list)
06:51:05.09 -01:41:34.8 -- not an asteroid (will add it to exclusion list)
06:49:33.17 -01:23:31.3 -- not an asteroid (will add it to exclusion list)
07:02:17.59 -03:14:33.0 -- not an asteroid (will add it to exclusion list)
07:03:52.65 -06:00:24.6 -- not an asteroid (will add it to exclusion list)
06:57:11.84 -03:58:12.7 -- not an asteroid (will add it to exclusion list)
06:52:57.33 -03:04:56.9 -- not an asteroid (will add it to exclusion list)
06:59:52.78 -04:47:26.6 -- not an asteroid (will add it to exclusion list)
06:58:45.60 -02:28:56.6 -- not an asteroid (will add it to exclusion list)
07:00:01.21 -05:09:19.3 -- not an asteroid (will add it to exclusion list)
06:56:22.04 -00:53:11.9 -- not an asteroid (will add it to exclusion list)
07:04:10.05 -05:04:53.6 -- not an asteroid (will add it to exclusion list)
06:48:48.44 +00:23:30.4 -- not an asteroid (will add it to exclusion list)
06:44:24.88 -00:04:50.0 -- not an asteroid (will add it to exclusion list)
06:44:39.61 +00:10:06.3 -- not an asteroid (will add it to exclusion list)
07:08:43.09 -05:05:29.5 -- not an asteroid (will add it to exclusion list)
07:07:48.91 -05:43:38.0 -- not an asteroid (will add it to exclusion list)
07:02:14.45 -03:05:58.9 -- not an asteroid (will add it to exclusion list)
06:58:50.14 -04:41:12.9 -- not an asteroid (will add it to exclusion list)
06:56:02.56 -03:13:02.6 -- not an asteroid (will add it to exclusion list)
06:56:49.00 +00:46:32.6 -- not an asteroid (will add it to exclusion list)
06:48:30.53 +00:57:43.9 -- not an asteroid (will add it to exclusion list)
07:06:11.94 +00:18:33.4 -- not an asteroid (will add it to exclusion list)
06:57:07.69 +00:36:02.2 -- not an asteroid (will add it to exclusion list)
06:59:33.41 +01:05:00.1 -- not an asteroid (will add it to exclusion list)
06:57:09.41 -01:07:39.1 -- not an asteroid (will add it to exclusion list)
06:57:24.09 -02:57:03.8 -- not an asteroid (will add it to exclusion list)
07:04:16.73 -03:01:39.2 -- not an asteroid (will add it to exclusion list)
06:57:12.35 -03:57:46.0 -- not an asteroid (will add it to exclusion list)
07:04:56.05 -05:21:48.3 -- not an asteroid (will add it to exclusion list)
06:58:35.36 -04:20:30.2 -- not an asteroid (will add it to exclusion list)
06:51:18.23 -01:23:09.2 -- not an asteroid (will add it to exclusion list)
06:58:22.44 -02:33:53.3 -- not an asteroid (will add it to exclusion list)
06:46:50.64 +01:18:07.4 -- not an asteroid (will add it to exclusion list)
06:54:41.81 -02:41:58.2 -- not an asteroid (will add it to exclusion list)
06:48:34.35 +01:51:39.4 -- not an asteroid (will add it to exclusion list)
06:54:49.49 -01:15:54.9 -- not an asteroid (will add it to exclusion list)
06:59:43.78 +00:17:12.0 -- not an asteroid (will add it to exclusion list)
07:07:56.30 -01:30:30.4 -- not an asteroid (will add it to exclusion list)
06:50:44.76 -00:05:16.4 -- not an asteroid (will add it to exclusion list)
06:48:45.22 +01:09:18.8 -- not an asteroid (will add it to exclusion list)
06:49:56.14 -02:40:54.9 -- not an asteroid (will add it to exclusion list)
06:49:07.39 -01:40:18.4 -- not an asteroid (will add it to exclusion list)
06:50:00.96 -03:51:50.3 -- not an asteroid (will add it to exclusion list)
06:53:06.38 -01:03:37.0 -- not an asteroid (will add it to exclusion list)
06:52:51.68 -02:22:45.6 -- not an asteroid (will add it to exclusion list)
06:51:37.26 +01:28:59.1 -- not an asteroid (will add it to exclusion list)
07:01:22.89 -05:01:12.6 -- not an asteroid (will add it to exclusion list)
06:59:44.33 -01:15:44.8 -- not an asteroid (will add it to exclusion list)
07:05:38.49 +01:26:02.4 -- not an asteroid (will add it to exclusion list)
06:53:41.40 -00:33:48.6 -- not an asteroid (will add it to exclusion list)
06:38:52.43 +01:12:24.1 -- asteroid (will NOT add it to exclusion list)
06:55:11.64 +00:56:23.6 -- not an asteroid (will add it to exclusion list)
07:01:34.77 -00:37:08.1 -- not an asteroid (will add it to exclusion list)
06:47:46.40 -02:22:20.5 -- not an asteroid (will add it to exclusion list)
06:39:28.94 +00:31:16.8 -- not an asteroid (will add it to exclusion list)
06:41:21.30 -00:35:23.5 -- not an asteroid (will add it to exclusion list)
06:51:51.87 -04:03:49.1 -- not an asteroid (will add it to exclusion list)
06:59:32.96 -02:32:38.2 -- not an asteroid (will add it to exclusion list)
06:54:32.31 -02:12:21.7 -- not an asteroid (will add it to exclusion list)
06:45:00.74 +00:14:03.0 -- not an asteroid (will add it to exclusion list)
06:55:19.67 -00:57:48.9 -- not an asteroid (will add it to exclusion list)
06:47:11.78 +00:21:18.4 -- not an asteroid (will add it to exclusion list)
06:57:11.48 -01:07:45.1 -- not an asteroid (will add it to exclusion list)
06:51:56.27 -01:17:01.1 -- not an asteroid (will add it to exclusion list)
06:56:49.62 -05:48:25.6 -- not an asteroid (will add it to exclusion list)
06:59:38.68 -00:49:25.6 -- not an asteroid (will add it to exclusion list)
06:48:35.53 -03:42:40.1 -- not an asteroid (will add it to exclusion list)
07:05:52.55 -00:01:01.8 -- not an asteroid (will add it to exclusion list)
07:02:48.91 -01:46:40.0 -- not an asteroid (will add it to exclusion list)
06:45:12.00 +00:20:57.6 -- not an asteroid (will add it to exclusion list)
06:51:44.75 -03:39:22.9 -- not an asteroid (will add it to exclusion list)
06:58:34.68 -01:38:25.6 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
06:35:07.33 -03:03:04.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:39:28.94 +00:31:16.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:40:55.24 +00:01:26.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:41:21.30 -00:35:23.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:41:44.19 +00:27:30.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:42:40.75 -00:18:15.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:16.49 +00:21:47.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:45.59 +00:35:15.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:24.88 -00:04:50.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:34.00 -01:35:29.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:39.61 +00:10:06.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:00.74 +00:14:03.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:12.00 +00:20:57.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:00.22 -00:22:10.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:12.55 +00:51:08.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:13.83 +00:50:42.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:25.32 +00:47:27.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:50.64 +01:18:07.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:47:11.78 +00:21:18.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:47:46.40 -02:22:20.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:07.59 -00:40:39.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:30.53 +00:57:43.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:34.35 +01:51:39.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:35.53 -03:42:40.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:45.22 +01:09:18.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:48.44 +00:23:30.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:50.52 -00:08:31.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:49:07.39 -01:40:18.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:49:33.17 -01:23:31.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:49:52.39 -02:39:53.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:49:56.14 -02:40:54.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:00.96 -03:51:50.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:09.67 -01:21:55.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:44.76 -00:05:16.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:51.74 -05:58:27.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:05.09 -01:41:34.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:10.39 +01:05:57.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:11.47 -02:22:10.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:18.23 -01:23:09.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:28.75 +01:57:02.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:37.26 +01:28:59.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:44.75 -03:39:22.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:51.87 -04:03:49.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:56.27 -01:17:01.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:00.95 +01:29:15.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:10.08 +00:34:37.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:51.68 -02:22:45.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:57.33 -03:04:56.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:04.49 -05:33:23.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:06.38 -01:03:37.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:22.56 -03:34:23.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:30.37 -03:06:08.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:33.71 -00:32:06.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:41.40 -00:33:48.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:41.51 -01:02:04.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:46.06 -00:14:32.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:14.55 -01:36:53.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:32.31 -02:12:21.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:34.23 -01:51:46.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:34.42 -00:35:22.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:41.07 -02:07:02.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:41.81 -02:41:58.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:49.49 -01:15:54.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:03.18 -01:02:50.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:04.55 -00:42:42.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:11.64 +00:56:23.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:19.67 -00:57:48.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:02.56 -03:13:02.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:22.04 -00:53:11.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:27.45 -01:27:42.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:49.00 +00:46:32.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:49.62 -05:48:25.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:04.33 -04:03:27.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:07.07 -00:31:51.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:07.69 +00:36:02.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:09.41 -01:07:39.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:11.48 -01:07:45.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:11.84 -03:58:12.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:12.35 -03:57:46.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:16.40 -00:59:39.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:24.02 -00:50:14.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:24.09 -02:57:03.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:40.53 -03:53:12.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:47.57 -01:31:07.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:22.44 -02:33:53.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:25.41 -02:40:33.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:27.06 -03:14:41.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:34.68 -01:38:25.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:35.36 -04:20:30.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:39.27 -01:55:30.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:39.32 +01:21:59.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:45.60 -02:28:56.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:50.14 -04:41:12.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:57.82 -01:46:10.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:00.64 -01:40:01.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:20.97 -05:44:56.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:32.96 -02:32:38.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:33.41 +01:05:00.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:38.68 -00:49:25.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:43.78 +00:17:12.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:44.33 -01:15:44.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:52.78 -04:47:26.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:00:01.21 -05:09:19.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:00:51.92 +00:11:59.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:00.94 -00:25:45.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:16.43 -02:28:44.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:22.89 -05:01:12.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:34.77 -00:37:08.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:01.24 -00:36:16.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:14.45 -03:05:58.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:17.20 -03:49:24.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:17.59 -03:14:33.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:21.31 -04:03:31.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:48.91 -01:46:40.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:23.86 -00:39:18.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:24.00 -02:49:52.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:25.13 -05:00:42.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:27.01 -05:01:13.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:38.51 -02:31:49.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:39.67 -04:38:24.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:47.18 -03:20:30.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:52.65 -06:00:24.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:08.47 -05:07:03.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:10.05 -05:04:53.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:16.73 -03:01:39.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:56.05 -05:21:48.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:03.97 -03:53:19.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:04.23 -05:27:55.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:12.07 -06:04:40.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:18.12 -01:23:00.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:19.95 -02:51:43.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:38.49 +01:26:02.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:50.91 -02:05:14.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:52.55 -00:01:01.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:11.94 +00:18:33.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:17.15 +02:00:15.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:22.80 -01:49:60.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:39.40 -03:57:46.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:43.76 -04:24:09.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:54.66 -04:13:51.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:04.81 -03:10:08.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:06.80 +01:39:59.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:47.22 -05:40:38.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:48.03 +00:24:43.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:48.91 -05:43:38.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:51.34 -05:46:59.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:56.30 -01:30:30.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:02.96 -03:23:39.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:17.17 -04:56:02.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:32.25 -04:39:28.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:39.11 -02:25:42.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:43.09 -05:05:29.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:48.84 -03:43:02.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:08.39 -01:41:28.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:10.38 -01:30:23.5 -- 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)
06:35:07.33 -03:03:04.3 -- not a known variable star
06:39:28.94 +00:31:16.8 -- not a known variable star
06:40:55.24 +00:01:26.5 -- a known variable star
06:41:21.30 -00:35:23.5 -- not a known variable star
06:41:44.19 +00:27:30.3 -- a known variable star
06:42:40.75 -00:18:15.0 -- a known variable star
06:43:16.49 +00:21:47.9 -- a known variable star
06:43:45.59 +00:35:15.7 -- not a known variable star
06:44:24.88 -00:04:50.0 -- not a known variable star
06:44:34.00 -01:35:29.5 -- a known variable star
06:44:39.61 +00:10:06.3 -- a known variable star
06:45:00.74 +00:14:03.0 -- not a known variable star
06:45:12.00 +00:20:57.6 -- a known variable star
06:46:00.22 -00:22:10.0 -- not a known variable star
06:46:12.55 +00:51:08.4 -- not a known variable star
06:46:13.83 +00:50:42.9 -- not a known variable star
06:46:25.32 +00:47:27.1 -- not a known variable star
06:46:50.64 +01:18:07.4 -- a known variable star
06:47:11.78 +00:21:18.4 -- a known variable star
06:47:46.40 -02:22:20.5 -- not a known variable star
06:48:07.59 -00:40:39.3 -- not a known variable star
06:48:30.53 +00:57:43.9 -- not a known variable star
06:48:34.35 +01:51:39.4 -- not a known variable star
06:48:35.53 -03:42:40.1 -- not a known variable star
06:48:45.22 +01:09:18.8 -- not a known variable star
06:48:48.44 +00:23:30.4 -- a known variable star
06:48:50.52 -00:08:31.2 -- not a known variable star
06:49:07.39 -01:40:18.4 -- not a known variable star
06:49:33.17 -01:23:31.3 -- not a known variable star
06:49:52.39 -02:39:53.8 -- not a known variable star
06:49:56.14 -02:40:54.9 -- not a known variable star
06:50:00.96 -03:51:50.3 -- not a known variable star
06:50:09.67 -01:21:55.2 -- a known variable star
06:50:44.76 -00:05:16.4 -- a known variable star
06:50:51.74 -05:58:27.0 -- not a known variable star
06:51:05.09 -01:41:34.8 -- a known variable star
06:51:10.39 +01:05:57.7 -- not a known variable star
06:51:11.47 -02:22:10.2 -- not a known variable star
06:51:18.23 -01:23:09.2 -- a known variable star
06:51:28.75 +01:57:02.8 -- not a known variable star
06:51:37.26 +01:28:59.1 -- not a known variable star
06:51:44.75 -03:39:22.9 -- not a known variable star
06:51:51.87 -04:03:49.1 -- a known variable star
06:51:56.27 -01:17:01.1 -- not a known variable star
06:52:00.95 +01:29:15.8 -- not a known variable star
06:52:10.08 +00:34:37.5 -- not a known variable star
06:52:51.68 -02:22:45.6 -- not a known variable star
06:52:57.33 -03:04:56.9 -- not a known variable star
06:53:04.49 -05:33:23.4 -- not a known variable star
06:53:06.38 -01:03:37.0 -- not a known variable star
06:53:22.56 -03:34:23.0 -- not a known variable star
06:53:30.37 -03:06:08.7 -- a known variable star
06:53:33.71 -00:32:06.2 -- not a known variable star
06:53:41.40 -00:33:48.6 -- a known variable star
06:53:41.51 -01:02:04.6 -- a known variable star
06:53:46.06 -00:14:32.6 -- not a known variable star
06:54:14.55 -01:36:53.2 -- a known variable star
06:54:32.31 -02:12:21.7 -- not a known variable star
06:54:34.23 -01:51:46.6 -- a known variable star
06:54:34.42 -00:35:22.5 -- not a known variable star
06:54:41.07 -02:07:02.7 -- a known variable star
06:54:41.81 -02:41:58.2 -- not a known variable star
06:54:49.49 -01:15:54.9 -- not a known variable star
06:55:03.18 -01:02:50.8 -- not a known variable star
06:55:04.55 -00:42:42.4 -- not a known variable star
06:55:11.64 +00:56:23.6 -- not a known variable star
06:55:19.67 -00:57:48.9 -- not a known variable star
06:56:02.56 -03:13:02.6 -- not a known variable star
06:56:22.04 -00:53:11.9 -- a known variable star
06:56:27.45 -01:27:42.6 -- not a known variable star
06:56:49.00 +00:46:32.6 -- not a known variable star
06:56:49.62 -05:48:25.6 -- not a known variable star
06:57:04.33 -04:03:27.8 -- not a known variable star
06:57:07.07 -00:31:51.3 -- a known variable star
06:57:07.69 +00:36:02.2 -- not a known variable star
06:57:09.41 -01:07:39.1 -- a known variable star
06:57:11.48 -01:07:45.1 -- a known variable star
06:57:11.84 -03:58:12.7 -- not a known variable star
06:57:12.35 -03:57:46.0 -- not a known variable star
06:57:16.40 -00:59:39.3 -- not a known variable star
06:57:24.02 -00:50:14.8 -- not a known variable star
06:57:24.09 -02:57:03.8 -- not a known variable star
06:57:40.53 -03:53:12.3 -- not a known variable star
06:57:47.57 -01:31:07.0 -- a known variable star
06:58:22.44 -02:33:53.3 -- a known variable star
06:58:25.41 -02:40:33.6 -- a known variable star
06:58:27.06 -03:14:41.3 -- not a known variable star
06:58:34.68 -01:38:25.6 -- not a known variable star
06:58:35.36 -04:20:30.2 -- not a known variable star
06:58:39.27 -01:55:30.2 -- not a known variable star
06:58:39.32 +01:21:59.1 -- not a known variable star
06:58:45.60 -02:28:56.6 -- not a known variable star
06:58:50.14 -04:41:12.9 -- not a known variable star
06:58:57.82 -01:46:10.4 -- not a known variable star
06:59:00.64 -01:40:01.6 -- not a known variable star
06:59:20.97 -05:44:56.3 -- a known variable star
06:59:32.96 -02:32:38.2 -- not a known variable star
06:59:33.41 +01:05:00.1 -- a known variable star
06:59:38.68 -00:49:25.6 -- not a known variable star
06:59:43.78 +00:17:12.0 -- a known variable star
06:59:44.33 -01:15:44.8 -- not a known variable star
06:59:52.78 -04:47:26.6 -- not a known variable star
07:00:01.21 -05:09:19.3 -- not a known variable star
07:00:51.92 +00:11:59.2 -- not a known variable star
07:01:00.94 -00:25:45.2 -- not a known variable star
07:01:16.43 -02:28:44.5 -- not a known variable star
07:01:22.89 -05:01:12.6 -- not a known variable star
07:01:34.77 -00:37:08.1 -- not a known variable star
07:02:01.24 -00:36:16.1 -- not a known variable star
07:02:14.45 -03:05:58.9 -- not a known variable star
07:02:17.20 -03:49:24.9 -- not a known variable star
07:02:17.59 -03:14:33.0 -- not a known variable star
07:02:21.31 -04:03:31.7 -- a known variable star
07:02:48.91 -01:46:40.0 -- not a known variable star
07:03:23.86 -00:39:18.2 -- not a known variable star
07:03:24.00 -02:49:52.4 -- not a known variable star
07:03:25.13 -05:00:42.0 -- a known variable star
07:03:27.01 -05:01:13.8 -- a known variable star
07:03:38.51 -02:31:49.4 -- not a known variable star
07:03:39.67 -04:38:24.6 -- not a known variable star
07:03:47.18 -03:20:30.1 -- not a known variable star
07:03:52.65 -06:00:24.6 -- not a known variable star
07:04:08.47 -05:07:03.8 -- not a known variable star
07:04:10.05 -05:04:53.6 -- not a known variable star
07:04:16.73 -03:01:39.2 -- not a known variable star
07:04:56.05 -05:21:48.3 -- a known variable star
07:05:03.97 -03:53:19.5 -- not a known variable star
07:05:04.23 -05:27:55.4 -- not a known variable star
07:05:12.07 -06:04:40.3 -- not a known variable star
07:05:18.12 -01:23:00.0 -- a known variable star
07:05:19.95 -02:51:43.1 -- a known variable star
07:05:38.49 +01:26:02.4 -- not a known variable star
07:05:50.91 -02:05:14.1 -- not a known variable star
07:05:52.55 -00:01:01.8 -- not a known variable star
07:06:11.94 +00:18:33.4 -- not a known variable star
07:06:17.15 +02:00:15.3 -- not a known variable star
07:06:22.80 -01:49:60.0 -- not a known variable star
07:06:39.40 -03:57:46.9 -- not a known variable star
07:06:43.76 -04:24:09.9 -- not a known variable star
07:06:54.66 -04:13:51.4 -- not a known variable star
07:07:04.81 -03:10:08.0 -- not a known variable star
07:07:06.80 +01:39:59.8 -- not a known variable star
07:07:47.22 -05:40:38.7 -- not a known variable star
07:07:48.03 +00:24:43.0 -- not a known variable star
07:07:48.91 -05:43:38.0 -- not a known variable star
07:07:51.34 -05:46:59.8 -- a known variable star
07:07:56.30 -01:30:30.4 -- not a known variable star
07:08:02.96 -03:23:39.4 -- not a known variable star
07:08:17.17 -04:56:02.0 -- a known variable star
07:08:32.25 -04:39:28.5 -- a known variable star
07:08:39.11 -02:25:42.0 -- a known variable star
07:08:43.09 -05:05:29.5 -- a known variable star
07:08:48.84 -03:43:02.7 -- not a known variable star
07:09:08.39 -01:41:28.4 -- a known variable star
07:09:10.38 -01:30:23.5 -- a known variable star
Found 111 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
155 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 155 (excluding asteroids and hot pixels, 111 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
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Positions of planets computed with util/planet_finder/main.py for JD(UT)2461152.60877253 -observatory V36
00:41:20.88 +01:39:24.5 Mercury (-0.2mag)
03:38:51.39 +19:59:48.8 Venus (-3.9mag)
00:35:10.01 +02:45:49.5 Mars (1.2mag)
07:15:36.07 +22:41:13.9 Jupiter (-2.1mag)
00:31:52.44 +01:05:41.0 Saturn (0.9mag)
03:49:00.87 +19:51:40.4 Uranus (5.8mag)
00:11:37.43 -00:10:27.1 Neptune (7.8mag)
20:33:59.09 -22:53:01.0 Pluto (14.5mag)
06:21:37.61 +27:35:35.9 Moon (-9.7mag)
-rw-r--r-- 1 apache apache 362 Apr 21 23:00 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461152.60877253:
07:15:40.53 +22:41:02.1 Io (5.8mag)
07:15:24.26 +22:41:39.9 Europa (5.9mag)
07:15:53.80 +22:40:38.7 Ganymede (5.4mag)
07:15:15.77 +22:41:49.2 Callisto (6.6mag)
07:18:39.12 +22:26:10.3 Himalia (15.4mag)
07:15:37.41 +22:41:08.6 Thebe (16.3mag)
07:18:57.65 +22:56:28.7 Elara (17.3mag)
07:14:53.82 +23:18:02.5 Pasiphae (17.4mag)
07:23:47.18 +22:39:48.4 Carme (18.6mag)
00:31:46.62 +01:05:40.2 Titan (8.8mag)
00:31:58.21 +01:05:42.4 Rhea (10.1mag)
00:31:24.56 +01:04:52.5 Iapetus (11.5mag)
00:31:41.67 +01:05:57.7 Hyperion (14.8mag)
00:33:24.30 +01:13:48.4 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Apr 21 23:00 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461152.60877253:
16:02:55.45 -20:11:07.0 JWST
17:03:19.41 +44:02:14.0 Chandra
07:52:06.74 -34:35:25.5 XMM-Newton
-rw-r--r-- 1 apache apache 96 Apr 21 23:00 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461152.60877253 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
05:29:52.78 +30:49:48.2 18.0mag P/2009 WX51 (Catalina)
18:54:05.55 -29:09:07.1 13.8mag P/2010 H2 (Vales)
05:11:16.84 -69:23:01.7 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:33:51.96 +31:28:53.4 17.3mag C/2017 K2 (PANSTARRS)
17:29:38.52 +11:15:33.9 17.6mag C/2021 G2 (ATLAS)
23:11:42.76 +29:28:52.9 17.1mag C/2022 E2 (ATLAS)
04:36:25.67 +26:11:57.1 16.1mag C/2022 N2 (PANSTARRS)
09:04:58.61 +32:01:52.8 16.3mag C/2022 QE78 (ATLAS)
08:32:11.92 +00:28:21.5 17.4mag C/2022 R6 (PANSTARRS)
18:52:04.15 +19:02:03.7 17.6mag C/2023 A3 (Tsuchinshan-ATLAS)
15:38:33.74 -11:25:53.2 17.5mag P/2023 B1 (PANSTARRS)
09:05:06.23 -10:55:55.8 17.7mag C/2023 F3 (ATLAS)
21:59:55.33 +63:16:48.0 17.6mag C/2023 H5 (Lemmon)
19:13:17.68 -03:51:15.9 14.1mag C/2023 R1 (PANSTARRS)
21:12:56.15 +86:46:10.6 17.8mag C/2023 X2 (Lemmon)
06:21:14.60 +63:30:00.3 17.2mag C/2024 A1 (ATLAS)
05:25:57.42 +20:09:45.0 11.4mag C/2024 E1 (Wierzchos)
16:15:08.90 +07:22:59.9 17.3mag C/2024 G6 (ATLAS)
20:22:15.68 +16:57:55.3 14.5mag C/2024 J3 (ATLAS)
03:31:56.33 -21:28:41.0 16.3mag C/2024 T5 (ATLAS)
05:22:00.75 +43:49:16.5 17.7mag C/2025 J1 (Borisov)
13:14:00.14 +48:47:34.2 15.5mag C/2025 L1 (ATLAS)
03:35:12.68 -27:12:06.7 17.9mag C/2025 Q3 (ATLAS)
01:03:32.33 +14:18:57.3 7.8mag C/2025 R3 (PANSTARRS)
12:51:31.26 +03:22:05.7 17.4mag C/2025 Y1 (ATLAS)
04:09:48.96 +02:07:54.0 14.8mag C/2026 A1 (MAPS)
00:16:27.55 +38:16:25.7 14.8mag C/2026 B2 (Sun-Gao)
18:54:47.54 -09:23:09.4 11.5mag 10P/Tempel
14:51:58.45 +02:31:03.9 14.5mag 24P/Schaumasse
11:01:20.97 -01:20:31.8 15.7mag 29P/Schwassmann-Wachmann
10:37:44.60 -03:39:08.8 17.0mag 43P/Wolf-Harrington
01:58:09.33 +18:31:03.6 17.3mag 47P/Ashbrook-Jackson
07:22:18.78 +35:40:42.3 17.0mag 63P/Wild
23:36:43.45 -10:43:54.2 15.7mag 65P/Gunn
04:19:52.65 +23:16:44.1 15.9mag 76P/West-Kohoutek-Ikemura
01:19:10.52 +09:25:02.8 14.3mag 78P/Gehrels
23:21:08.60 -07:35:05.2 14.7mag 88P/Howell
02:27:56.51 +22:13:27.1 15.1mag 93P/Lovas
05:06:35.97 +32:35:32.1 16.1mag 123P/West-Hartley
08:35:59.94 +35:32:59.7 16.2mag 124P/Mrkos
02:42:43.81 +15:02:24.1 16.4mag 128P/Shoemaker-Holt
02:59:34.16 +15:12:54.0 17.5mag 131P/Mueller
01:58:43.36 +15:11:52.4 10.5mag 141P/Machholz
02:06:39.81 +07:08:11.3 10.5mag 141P-A/Machholz
00:49:23.22 +02:53:28.3 12.1mag 141P-D/Machholz
02:37:17.30 +08:52:24.7 17.9mag 141P-I/Machholz
01:19:30.17 +01:33:32.6 15.0mag 162P/SidingSpring
14:40:42.42 +00:29:38.2 17.8mag 210P/Christensen
21:55:48.49 -09:59:32.3 17.8mag 218P/LINEAR
17:17:23.68 -13:11:13.5 16.1mag 235P/LINEAR
05:47:49.80 +35:06:48.9 16.8mag 240P/NEAT
07:41:44.06 -04:32:08.6 17.8mag 242P/Spahr
22:32:11.82 -19:17:31.0 17.7mag 260P/McNaught
02:10:52.00 +21:59:08.9 17.9mag 295P/LINEAR
15:40:02.92 +07:22:13.1 17.5mag 391P/Kowalski
07:36:45.89 +21:22:23.8 17.7mag 450P/LONEOS
05:44:56.15 +44:40:33.8 17.5mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.9K Apr 21 23:00 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
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
14:49:14.13 -27:29:20.60 2026-04-16.06 14.03
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 2026-04-9.29 13.32
09:22:22.90 -61:02:43.70 SN2026idh 2026-04-7.97 16.34
05:06:54.12 -19:42:26.40 AT2026imr 2026-04-8 17.49
07:14:55.34 -36:03:21.40 AT2026hei 2026-04-8.12 16.7
21:35:33.14 -19:01:34.80 AT2026ihm 2026-04-8.36 16.7
04:28:24.08 -32:25:35.30 AT2026imo 2026-04-8.02 16.81
05:10:35.79 -39:38:40.80 SN 2026hnn 2026-04-7.04 17.07
09:54:32.04 -01:17:25.80 ASASSN-26cn 2026-04-7.01 15.58
07:46:24.43 -77:29:36.30 ASASSN-26co 2026-04-7.15 15.11
05:00:45.52 -29:51:06.20 AT2026hvw 2026-04-6.03 16.51
19:49:33.10 -23:37:11.00 ASASSN-26cl 2026-04-5.29 14.98
19:32:43.55 -22:39:33.40 ASASSN-26cm 2026-04-4.3 13.88
18:08:57.38 +76:48:23.60 ASASSN-26ck 2026-04-2.37 15.38
16:16:36.10 +44:52:30.20 AT2026hyy 2026-04-2.58 13.81
21:55:23.31 -34:48:53.90 ASASSN-26cj 2026-03-30.4 -1.47
11:19:50.81 -27:51:50.40 SN2026gvk 2026-03-30 15.28
11:53:57.02 -23:09:46.20 SN2026gzx 2026-03-28.75 15.27
07:13:46.14 -33:10:15.70 ASASSN-26ci 2026-03-28.15 15.14
09:03:36.09 -67:58:13.00 SN2026hkg 2026-03-28.19 15.82
07:03:00.72 +39:14:43.00 SN2026fin 2026-03-28.27 15.82
05:35:42.79 -63:44:05.60 ASASSN-26ch 2026-03-28.12 13.14
11:23:19.04 +34:22:38.00 SN2026fwt 2026-03-27.3 16.56
19:03:49.79 +37:04:05.20 ASASSN-26ce 2026-03-26.56 16.3
20:26:56.07 -52:54:06.50 AT2026hiy 2026-03-26.35 16.95
05:25:54.76 -30:15:35.80 ASASSN-26cg 2026-03-25.07 16.88
06:57:16.49 -26:54:37.20 SN2026fzb 2026-03-25.14 15.8
14:37:38.23 -43:00:52.30 ASASSN-26cd 2026-03-24.24 12.52
17:34:53.03 +06:04:29.70 AT2026gzl 2026-03-23.27 15.82
08:30:02.60 -35:12:47.50 ASASSN-26cf 2026-03-23.2 14.82
16:54:25.33 +37:49:56.60 SN 2026evz 2026-03-21.32 17.54
17:06:19.20 -18:54:19.50 ASASSN-26bx 2026-03-21.25 16.39
19:01:16.28 -29:29:23.10 ASASSN-26bw 2026-03-21.33 15.81
08:46:05.75 +10:47:39.80 ASASSN-26ca 2026-03-21.13 14.27
12:14:58.16 +63:47:16.20 SN 2026fvx 2026-03-21.12 15.6
18:02:55.90 -75:23:02.60 ASASSN-26bz 2026-03-21.32 16.16
12:16:02.87 -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
12:20:27.90 -45:55:38.40 ASASSN-26bt 2026-03-19.05 16.24
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
11:30:09.67 -47:26:43.70 ASASSN-26bn 2026-03-10.12 15.2
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
09:27:45.48 -37:49:32.80 ASASSN-26bk 2026-03-2.3 13.11
20:22:01.20 +23:47:47.30 ASASSN-26bi 2026-02-28.51 15.86
11:16:22.10 +29:26:22.80 AT2026enm 2026-02-28.39 16.88
08:05:59.83 -48:39:35.60 ASASSN-26bh 2026-02-26.05 14.64
13:24:27.02 -45:57:01.40 ASASSN-26bg 2026-02-26.35 15.28
17:27:50.95 -68:28:46.40 ASASSN-26bf 2026-02-26.3 16.28
18:03:39.37 +19:58:46.70 ASASSN-26be 2026-02-25.58 14.8
17:40:18.19 +07:20:59.60 SN 2026crm 2026-02-24.34 16.9
18:38:36.11 -79:28:58.40 ASASSN-26bb 2026-02-24.36 16.11
17:43:29.75 +11:24:00.60 ASASSN-26bc 2026-02-23.37 -3.37
16:59:41.08 -80:01:51.20 ASASSN-26bd 2026-02-23.3 14.38
11:23:31.77 -08:39:15.40 SN2026cff 2026-02-23.15 -1.08
14:55:17.39 -05:56:05.30 SN2026dmk 2026-02-23.22 -0.76
12:28:15.19 +44:27:20.80 SN2026cjz 2026-02-23.47 15.62
12:12:29.55 -02:40:43.30 AT2026dsk 2026-02-23.4 17.21
09:21:05.29 +06:11:42.80 SN2026chr 2026-02-23.1 17.39
16:05:38.61 +18:06:07.40 SN 2026dsy 2026-02-23.36 17.15
-rw-r--r-- 1 apache apache 5.8K Apr 21 23:00 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
09:54:46.47 +69:06:31.7 PNV J09544647+6906317 2026-01-26.8081 19.3mag
18:08:51.99 -26:16:21.9 TCP J18085199-2616219 2026-01-31.8519 12.2mag
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
-rw-r--r-- 1 apache apache 188K Apr 21 23:00 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
12:06:16.602 -06:52:59.29 AT 2026jpa 2026-04-13.89 19.276
06:42:32.732 -34:30:04.15 AT 2026joz 2026-04-14.77 18.707
13:06:33.339 -08:24:24.46 AT 2026joy 2026-04-14.02 19.307
21:07:11.613 -12:36:56.09 AT 2026jox 2026-04-14.14 18.849
05:34:42.408 -28:21:31.62 AT 2026jow 2026-04-14.74 18.902
12:30:54.108 -14:11:53.07 AT 2026jov 2026-04-14.03 19.309
05:52:53.155 -34:43:22.49 AT 2026jou 2026-04-14.75 19.398
05:40:18.921 -24:52:33.50 AT 2026jot 2026-04-14.77 18.65
15:53:02.304 +04:30:53.21 AT 2026jos 2026-04-14.09 19.566
11:19:37.053 +36:36:59.54 AT 2026jor 2026-04-11.94 20.14
08:17:15.784 +16:04:01.41 AT 2026joq 2026-04-11.86 19.95
15:52:58.319 -17:01:02.93 AT 2026jop 2026-04-09.53 19.69
09:28:29.338 +17:46:10.46 AT 2026joo 2026-04-11.90 19.1
14:08:31.151 +20:01:29.32 AT 2026jon 2026-04-08.02 19.9
08:15:22.510 -21:29:08.39 AT 2026jom 2026-04-12.37 19.76
12:13:11.990 +05:30:27.70 AT 2026jol 2026-04-08.25 16.6
09:57:55.902 +03:33:01.27 AT 2026jok 2026-03-06.10 21.72
15:47:58.800 -16:07:43.45 AT 2026joj 2026-04-10.44 20.1583
09:57:44.859 +01:08:42.73 AT 2026joi 2026-04-06.02 22.85
14:40:55.647 +05:24:36.73 SN 2026joh 2026-04-14.03 17.708
-rw-r--r-- 1 apache apache 30K Apr 21 23:00 tns_transients_list.txt
