This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Ori-02-Q1b1x1_043748_TTUQ1b1x1_2949840_gjrQHCHz
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 08 22.4004 2461274.9004 11.17 06:26:21.49 +15:58:57.2
195.88954 1.84018 galactic Gem Second-epoch detections are separated by 0.8" and 8.9 pix
The object was found in VSX 1" AP Gem
Type: LB
# Max. Min./Amp. JD0 Period
14.000 pg 15.600 pg M6.5
The object was not found in astcheck.
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:26:21.49 +15:58:57.2: 12.38 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:26:21.49 +15:58:57.2: 11.98 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.11 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
AP Gem,2461274.9004,11.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
AP Gem 20260822.4004 11.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4004 2461274.9004 11.59 06:18:03.95 +13:30:16.6
197.13572 -1.09345 galactic Ori Second-epoch detections are separated by 1.4" and 8.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3332487188218524800 | 06:18:03.97 +13:30:16.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.261+/-0.034 (Very red! L if it's a dwarf)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:18:03.95 +13:30:16.6: 12.54 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:18:03.95 +13:30:16.6: 12.56 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.55 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 18 03.95 +13 30 16.6 11.6 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 3332487188218524800,2461274.9004,11.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3332487188218524800 20260822.4004 11.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4004 2461274.9004 11.85 05:58:59.97 +09:16:46.1
198.59967 -7.22078 galactic Ori Second-epoch detections are separated by 0.4" and 9.1 pix
The object was found in VSX 1" ASASSN-V J055859.94+091644.8
Type: SR
# Max. Min./Amp. JD0 Period
14.000 g Y 0.160 g 2459535.45100 41.830000000000
The object was not found in astcheck.
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 05:58:59.97 +09:16:46.1: 12.73 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 05:58:59.97 +09:16:46.1: 12.81 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.77 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 05 58 59.97 +09 16 46.1 11.8 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J055859.94+091644.8,2461274.9004,11.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J055859.94+091644.8 20260822.4004 11.85CV 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 08 22.4004 2461274.9004 11.87 06:20:10.05 +13:20:58.6
197.51391 -0.71633 galactic Ori Second-epoch detections are separated by 5.3" and 9.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J095.0478+13.3543 | 06:20:10.06 +13:20:57.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.814+/-0.026 (K)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:20:10.05 +13:20:58.6: 12.79 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:20:10.05 +13:20:58.6: 12.80 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.80 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 20 10.05 +13 20 58.6 11.9 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J095.0478+13.3543,2461274.9004,11.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J095.0478+13.3543 20260822.4004 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 08 22.4004 2461274.9004 11.91 06:21:10.22 +12:58:17.9
197.96235 -0.67909 galactic Ori Second-epoch detections are separated by 1.3" and 8.9 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 3332417571089133184 | 06:21:10.14 +12:58:17.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=1.057+/-0.031 (M)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:21:10.22 +12:58:17.9: 12.80 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:21:10.22 +12:58:17.9: 12.84 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.82 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 21 10.22 +12 58 17.9 11.9 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 3332417571089133184,2461274.9004,11.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3332417571089133184 20260822.4004 11.91CV 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 08 22.4004 2461274.9004 11.90 06:20:56.55 +15:15:27.3
195.91966 0.34860 galactic Ori Second-epoch detections are separated by 0.7" and 8.9 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 J095.2365+15.2534 | 06:20:56.55 +15:15:27.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.331+/-0.029 (G)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:20:56.55 +15:15:27.3: 12.86 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:20:56.55 +15:15:27.3: 12.85 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.85 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 20 56.55 +15 15 27.3 11.9 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J095.2365+15.2534,2461274.9004,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J095.2365+15.2534 20260822.4004 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 08 22.4004 2461274.9004 11.82 06:22:27.61 +16:05:21.6
195.35728 1.06207 galactic Ori Second-epoch detections are separated by 2.5" and 8.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3369141603055616768 | 06:22:27.52 +16:05:22.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.072+/-0.035 (M)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:22:27.61 +16:05:21.6: 12.86 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:22:27.61 +16:05:21.6: 12.84 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.85 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 22 27.61 +16 05 21.6 11.8 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 3369141603055616768,2461274.9004,11.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3369141603055616768 20260822.4004 11.82CV 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 08 22.4004 2461274.9004 11.93 06:24:56.21 +14:49:23.4
196.75572 0.99654 galactic Ori Second-epoch detections are separated by 0.7" and 9.1 pix
The object was found in VSX 1" ASASSN-V J062456.21+144922.3
Type: SR
# Max. Min./Amp. JD0 Period
14.320 g Y 0.270 g 2458822.01100 431.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:24:56.21 +14:49:23.4: 12.87 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:24:56.21 +14:49:23.4: 12.80 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.83 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 24 56.21 +14 49 23.4 11.9 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J062456.21+144922.3,2461274.9004,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J062456.21+144922.3 20260822.4004 11.93CV 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 08 22.4004 2461274.9004 11.84 06:12:25.54 +10:30:59.9
199.11065 -3.72724 galactic Ori Second-epoch detections are separated by 2.3" and 8.7 pix
The object was found in VSX 1" ASASSN-V J061225.46+103100.8
Type: L
# Max. Min./Amp. JD0 Period
13.290 V 13.880 V
The object was not found in astcheck.
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:12:25.54 +10:30:59.9: 12.89 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:12:25.54 +10:30:59.9: 12.85 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.87 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 12 25.54 +10 30 59.9 11.8 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J061225.46+103100.8,2461274.9004,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J061225.46+103100.8 20260822.4004 11.84CV 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 08 22.4004 2461274.9004 11.89 06:19:44.97 +14:56:40.9
196.05977 -0.05288 galactic Ori Second-epoch detections are separated by 1.1" and 9.1 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 3344761994292543616 | 06:19:44.92 +14:56:41.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.132+/-0.030 (M)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:19:44.97 +14:56:40.9: 12.92 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:19:44.97 +14:56:40.9: 12.89 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.91 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 19 44.97 +14 56 40.9 11.9 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 3344761994292543616,2461274.9004,11.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3344761994292543616 20260822.4004 11.89CV 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 08 22.4004 2461274.9004 11.82 06:16:58.38 +12:25:08.5
197.96573 -1.84240 galactic Ori Second-epoch detections are separated by 1.3" and 8.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3331987352805482880 | 06:16:58.41 +12:25:09.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.373+/-0.048 (Very red! L if it's a dwarf)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:16:58.38 +12:25:08.5: 12.93 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:16:58.38 +12:25:08.5: 12.94 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.93 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 16 58.38 +12 25 08.5 11.8 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 3331987352805482880,2461274.9004,11.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3331987352805482880 20260822.4004 11.82CV 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 08 22.4004 2461274.9004 12.02 06:24:38.86 +15:35:16.9
196.04673 1.29219 galactic Ori Second-epoch detections are separated by 3.3" and 9.2 pix
The object was found in VSX 2" ASASSN-V J062438.76+153517.2
Type: L
# Max. Min./Amp. JD0 Period
13.270 V 13.350 V
The object was not found in astcheck.
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:24:38.86 +15:35:16.9: 12.98 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:24:38.86 +15:35:16.9: 12.94 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.96 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 24 38.86 +15 35 16.9 12.0 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J062438.76+153517.2,2461274.9004,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J062438.76+153517.2 20260822.4004 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 08 22.4004 2461274.9004 12.08 06:15:15.56 +12:02:24.1
198.10052 -2.39085 galactic Ori Second-epoch detections are separated by 1.2" and 8.7 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 | DocumentRef: VOTx2922616 | 06:15:15.56 +12:02:24.1 (user input) | (VSX @ VizieR) | (VSX @ VizieR) | (position from user input) J-Ks=0.416+/-0.030 (G)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:15:15.56 +12:02:24.1: 13.04 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:15:15.56 +12:02:24.1: 13.05 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.05 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 15 15.56 +12 02 24.1 12.1 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DocumentRef: VOTx2922616,2461274.9004,12.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DocumentRef: VOTx2922616 20260822.4004 12.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4004 2461274.9004 12.08 06:17:36.16 +13:06:06.3
197.43718 -1.38355 galactic Ori Second-epoch detections are separated by 1.9" and 9.1 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 | 06:17:36.16 +13:06:06.3 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.806+/-0.028 (K)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:17:36.16 +13:06:06.3: 13.07 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:17:36.16 +13:06:06.3: 13.09 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 17 36.16 +13 06 06.3 12.1 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461274.9004,12.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4004 12.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4004 2461274.9004 12.17 06:21:34.28 +14:08:35.2
196.97452 -0.04184 galactic Ori Second-epoch detections are separated by 4.4" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:21:34.28 +14:08:35.2 (user input) | T | P | (position from user input) J-Ks=0.262+/-0.033 (F)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:21:34.28 +14:08:35.2: 13.19 +/- 0.03 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:21:34.28 +14:08:35.2: 13.20 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 21 34.28 +14 08 35.2 12.2 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461274.9004,12.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4004 12.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4004 2461274.9004 12.19 06:16:33.61 +12:04:50.5
198.21589 -2.09167 galactic Ori Second-epoch detections are separated by 1.4" and 8.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | DocumentRef: VOTx3304987 | 06:16:33.61 +12:04:50.5 (user input) | (GCVS) | (GCVS) | (position from user input)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:16:33.61 +12:04:50.5: 13.36 +/- 0.03 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:16:33.61 +12:04:50.5: 13.31 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.33 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 16 33.61 +12 04 50.5 12.2 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DocumentRef: VOTx3304987,2461274.9004,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DocumentRef: VOTx3304987 20260822.4004 12.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4004 2461274.9004 12.19 06:16:52.29 +12:39:03.5
197.74968 -1.75418 galactic Ori Second-epoch detections are separated by 1.5" and 9.1 pix
The object was found in VSX 1" ASASSN-V J061652.28+123902.5
Type: SR
# Max. Min./Amp. JD0 Period
13.800 V 13.890 V 2457264.00000 158.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:16:52.29 +12:39:03.5: 13.47 +/- 0.03 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:16:52.29 +12:39:03.5: 13.36 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.42 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 16 52.29 +12 39 03.5 12.2 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J061652.28+123902.5,2461274.9004,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J061652.28+123902.5 20260822.4004 12.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4004 2461274.9004 12.07 06:12:38.91 +10:38:15.1
199.03033 -3.62146 galactic Ori Second-epoch detections are separated by 1.5" and 8.8 pix
The object was found in VSX 1" ASASSN-V J061238.93+103813.8
Type: SRS
# Max. Min./Amp. JD0 Period
14.570 g Y 0.240 g 2458891.65800 26.828000000000
The object was not found in astcheck.
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:12:38.91 +10:38:15.1: 13.29 +/- 0.03 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:12:38.91 +10:38:15.1: 13.28 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 12 38.91 +10 38 15.1 12.1 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J061238.93+103813.8,2461274.9004,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J061238.93+103813.8 20260822.4004 12.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4004 2461274.9004 12.16 06:23:40.76 +15:24:49.4
196.09169 1.00448 galactic Ori Second-epoch detections are separated by 1.1" and 8.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:23:40.76 +15:24:49.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:23:40.76 +15:24:49.4: 13.24 +/- 0.03 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:23:40.76 +15:24:49.4: 13.17 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.20 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 23 40.76 +15 24 49.4 12.2 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461274.9004,12.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4004 12.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4004 2461274.9004 12.07 06:17:17.52 +12:47:01.7
197.68134 -1.60091 galactic Ori Second-epoch detections are separated by 2.4" and 8.5 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 | DocumentRef: VOTx3510432 | 06:17:17.52 +12:47:01.7 (user input) | (VSX @ VizieR) | (VSX @ VizieR) | (position from user input) J-Ks=0.380+/-0.030 (G)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:17:17.52 +12:47:01.7: 13.22 +/- 0.03 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:17:17.52 +12:47:01.7: 13.16 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 17 17.52 +12 47 01.7 12.1 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DocumentRef: VOTx3510432,2461274.9004,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DocumentRef: VOTx3510432 20260822.4004 12.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4004 2461274.9004 12.03 06:15:19.32 +11:42:51.1
198.39473 -2.53227 galactic Ori Second-epoch detections are separated by 1.5" and 9.1 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 3331831050354602112 | 06:15:19.26 +11:42:50.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K7 (LAMOST DR5) J-Ks=1.379+/-0.038 (Very red! L if it's a dwarf)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:15:19.32 +11:42:51.1: 13.24 +/- 0.03 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:15:19.32 +11:42:51.1: 13.21 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.23 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 15 19.32 +11 42 51.1 12.0 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 3331831050354602112,2461274.9004,12.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3331831050354602112 20260822.4004 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 08 22.4004 2461274.9004 12.03 06:18:54.34 +12:57:04.2
197.72012 -1.17525 galactic Ori Second-epoch detections are separated by 0.7" and 9.0 pix
The object was found in VSX19" Gaia DR3 3332405034084644352
Type: VAR
# Max. Min./Amp. JD0 Period
13.940 G 14.000 G 0.203639000000 A
The object was not found in astcheck.
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:18:54.34 +12:57:04.2: 13.18 +/- 0.03 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:18:54.34 +12:57:04.2: 13.14 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.16 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 18 54.34 +12 57 04.2 12.0 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 3332405034084644352,2461274.9004,12.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3332405034084644352 20260822.4004 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 08 22.4004 2461274.9004 12.21 06:17:56.94 +13:25:25.8
197.19342 -1.15672 galactic Ori Second-epoch detections are separated by 2.0" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:17:56.94 +13:25:25.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:17:56.94 +13:25:25.8: 13.18 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:17:56.94 +13:25:25.8: 13.14 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.16 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 17 56.94 +13 25 25.8 12.2 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461274.9004,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4004 12.21CV 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 08 22.4004 2461274.9004 12.16 06:21:05.47 +16:15:55.8
195.04725 0.85473 galactic Ori Second-epoch detections are separated by 0.5" and 8.9 pix
The object was found in VSX 1" ZTF J062105.53+161556.2
Type: SR
# Max. Min./Amp. JD0 Period
15.169 g Y 0.325 g 2458510.18960 102.569905400000 C
The object was not found in astcheck.
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:21:05.47 +16:15:55.8: 13.18 +/- 0.03 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:21:05.47 +16:15:55.8: 13.11 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 21 05.47 +16 15 55.8 12.2 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J062105.53+161556.2,2461274.9004,12.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J062105.53+161556.2 20260822.4004 12.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4004 2461274.9004 12.16 06:21:58.43 +14:41:52.6
196.53068 0.30506 galactic Ori Second-epoch detections are separated by 3.2" and 8.9 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 | DocumentRef: VOTx3571955 | 06:21:58.43 +14:41:52.6 (user input) | (GCVS) | (GCVS) | (position from user input) J-Ks=0.315+/-0.035 (F)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:21:58.43 +14:41:52.6: 13.13 +/- 0.03 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:21:58.43 +14:41:52.6: 13.15 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 21 58.43 +14 41 52.6 12.2 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DocumentRef: VOTx3571955,2461274.9004,12.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DocumentRef: VOTx3571955 20260822.4004 12.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4004 2461274.9004 12.05 06:20:17.27 +14:02:56.0
196.91105 -0.36075 galactic Ori Second-epoch detections are separated by 0.3" and 9.0 pix
The object was found in VSX 0" Gaia DR3 3344635486034978176
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.010 G 13.040 G A
The object was not found in astcheck.
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:20:17.27 +14:02:56.0: 13.12 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:20:17.27 +14:02:56.0: 13.09 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 20 17.27 +14 02 56.0 12.1 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 3344635486034978176,2461274.9004,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3344635486034978176 20260822.4004 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 08 22.4004 2461274.9004 12.05 06:22:22.80 +15:58:11.2
195.45382 0.98894 galactic Ori Second-epoch detections are separated by 2.0" and 9.3 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 | 06:22:22.80 +15:58:11.2 (user input) | T | P | (position from user input) J-Ks=0.749+/-0.035 (K)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:22:22.80 +15:58:11.2: 13.12 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:22:22.80 +15:58:11.2: 13.10 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.11 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 22 22.80 +15 58 11.2 12.1 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461274.9004,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4004 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 08 22.4004 2461274.9004 12.12 06:23:51.74 +15:29:02.6
196.05018 1.07637 galactic Ori Second-epoch detections are separated by 2.1" and 9.2 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 J095.9731+15.4896 | 06:23:51.74 +15:29:02.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.846+/-0.028 (M)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:23:51.74 +15:29:02.6: 13.13 +/- 0.04 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:23:51.74 +15:29:02.6: 13.12 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 23 51.74 +15 29 02.6 12.1 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J095.9731+15.4896,2461274.9004,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J095.9731+15.4896 20260822.4004 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4004 2461274.9004 12.05 06:26:02.18 +15:41:17.8
196.11404 1.63467 galactic Gem Second-epoch detections are separated by 1.0" and 9.0 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 J096.5089+15.6877 | 06:26:02.14 +15:41:16.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.406+/-0.034 (Very red! L if it's a dwarf)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:26:02.18 +15:41:17.8: 13.10 +/- 0.03 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:26:02.18 +15:41:17.8: 13.08 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J096.5089+15.6877,2461274.9004,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J096.5089+15.6877 20260822.4004 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 08 22.4004 2461274.9004 11.91 06:21:06.61 +12:02:31.3
198.77577 -1.12954 galactic Ori Second-epoch detections are separated by 1.3" and 9.0 pix
The object was found in VSX 3" ASASSN-V J062106.76+120232.7
Type: SR
# Max. Min./Amp. JD0 Period
14.500 g Y 0.250 g 2459110.04300 283.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:21:06.61 +12:02:31.3: 13.08 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:21:06.61 +12:02:31.3: 12.97 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.02 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 21 06.61 +12 02 31.3 11.9 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J062106.76+120232.7,2461274.9004,11.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J062106.76+120232.7 20260822.4004 11.91CV 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 08 22.4004 2461274.9004 12.10 06:15:56.08 +12:04:47.7
198.14393 -2.22662 galactic Ori Second-epoch detections are separated by 0.9" and 8.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:15:56.08 +12:04:47.7 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.772+/-0.028 (K)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:15:56.08 +12:04:47.7: 13.07 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:15:56.08 +12:04:47.7: 13.04 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.05 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 15 56.08 +12 04 47.7 12.1 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461274.9004,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4004 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 08 22.4004 2461274.9004 12.11 06:16:21.84 +12:41:45.6
197.65125 -1.84176 galactic Ori Second-epoch detections are separated by 1.1" and 9.1 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 | DocumentRef: VOTx3642102 | 06:16:21.84 +12:41:45.6 (user input) | (GCVS) | (GCVS) | (position from user input)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:16:21.84 +12:41:45.6: 13.07 +/- 0.03 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:16:21.84 +12:41:45.6: 13.17 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 16 21.84 +12 41 45.6 12.1 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DocumentRef: VOTx3642102,2461274.9004,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DocumentRef: VOTx3642102 20260822.4004 12.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4004 2461274.9004 12.02 06:18:23.21 +14:09:23.0
196.59849 -0.71617 galactic Ori Second-epoch detections are separated by 0.5" and 9.0 pix
The object was found in VSX 1" ASASSN-V J061823.15+140923.1
Type: L
# Max. Min./Amp. JD0 Period
13.180 V 13.270 V
The object was not found in astcheck.
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:18:23.21 +14:09:23.0: 13.06 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:18:23.21 +14:09:23.0: 12.96 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.00 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 18 23.21 +14 09 23.0 12.0 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J061823.15+140923.1,2461274.9004,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J061823.15+140923.1 20260822.4004 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 08 22.4004 2461274.9004 11.99 06:15:56.88 +12:26:49.5
197.82217 -2.04933 galactic Ori Second-epoch detections are separated by 0.9" and 8.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3332032776379602432 | 06:15:56.88 +12:26:49.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:15:56.88 +12:26:49.5: 13.07 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:15:56.88 +12:26:49.5: 13.08 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.07 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 15 56.88 +12 26 49.5 12.0 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 3332032776379602432,2461274.9004,11.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3332032776379602432 20260822.4004 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 08 22.4004 2461274.9004 11.97 06:24:06.45 +17:23:48.7
194.38622 2.02275 galactic Ori Second-epoch detections are separated by 4.3" and 9.4 pix
The object was found in VSX 3" ZTF J062406.62+172350.7
Type: SR
# Max. Min./Amp. JD0 Period
12.272 r Y 0.252 r 2458495.49850 135.022088900000
The object was not found in astcheck.
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:24:06.45 +17:23:48.7: 13.02 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:24:06.45 +17:23:48.7: 12.90 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.95 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 24 06.45 +17 23 48.7 12.0 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J062406.62+172350.7,2461274.9004,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J062406.62+172350.7 20260822.4004 11.97CV 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 08 22.4004 2461274.9004 12.02 06:17:33.94 +12:17:36.1
198.14507 -1.77451 galactic Ori Second-epoch detections are separated by 2.9" and 8.4 pix
The object was found in VSX 2" Gaia DR3 3331970795711661952
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.890 G 12.910 G F
The object was not found in astcheck.
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:17:33.94 +12:17:36.1: 13.05 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:17:33.94 +12:17:36.1: 13.08 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.07 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 17 33.94 +12 17 36.1 12.0 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 3331970795711661952,2461274.9004,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3331970795711661952 20260822.4004 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 08 22.4004 2461274.9004 12.06 06:21:05.48 +15:36:17.8
195.63010 0.54381 galactic Ori Second-epoch detections are separated by 0.2" and 9.0 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 J095.2763+15.6141 | 06:21:05.48 +15:36:16.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.299+/-0.040 (Very red! L if it's a dwarf)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:21:05.48 +15:36:17.8: 13.05 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:21:05.48 +15:36:17.8: 12.99 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.02 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 21 05.48 +15 36 17.8 12.1 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J095.2763+15.6141,2461274.9004,12.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J095.2763+15.6141 20260822.4004 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 08 22.4004 2461274.9004 12.06 06:19:52.72 +14:03:37.0
196.85419 -0.44286 galactic Ori Second-epoch detections are separated by 2.2" and 9.3 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 | DocumentRef: VOTx3675011 | 06:19:52.72 +14:03:37.0 (user input) | (GCVS) | (GCVS) | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.734+/-0.026 (K)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:19:52.72 +14:03:37.0: 13.05 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:19:52.72 +14:03:37.0: 13.11 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 19 52.72 +14 03 37.0 12.1 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DocumentRef: VOTx3675011,2461274.9004,12.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DocumentRef: VOTx3675011 20260822.4004 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 08 22.4004 2461274.9004 12.02 06:15:58.18 +11:56:55.9
198.26342 -2.28134 galactic Ori Second-epoch detections are separated by 1.2" and 8.9 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 3331864688540863360 | 06:15:58.20 +11:56:55.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.926+/-0.035 (M)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:15:58.18 +11:56:55.9: 13.04 +/- 0.03 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:15:58.18 +11:56:55.9: 13.03 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.03 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 15 58.18 +11 56 55.9 12.0 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 3331864688540863360,2461274.9004,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3331864688540863360 20260822.4004 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 08 22.4004 2461274.9004 12.15 06:21:36.02 +14:23:07.4
196.76403 0.07833 galactic Ori Second-epoch detections are separated by 1.7" and 8.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:21:36.02 +14:23:07.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:21:36.02 +14:23:07.4: 13.04 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:21:36.02 +14:23:07.4: 13.10 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.07 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 21 36.02 +14 23 07.4 12.2 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461274.9004,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4004 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 08 22.4004 2461274.9004 12.06 06:21:18.34 +13:50:32.3
197.20962 -0.24025 galactic Ori Second-epoch detections are separated by 1.6" and 9.2 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 | DocumentRef: VOTx3724945 | 06:21:18.32 +13:50:31.5 (Gaia DR3) | (VSX @ VizieR) | (VSX @ VizieR) | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=1.279+/-0.039 (Very red! L if it's a dwarf)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:21:18.34 +13:50:32.3: 12.99 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:21:18.34 +13:50:32.3: 12.98 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.99 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 21 18.34 +13 50 32.3 12.1 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DocumentRef: VOTx3724945,2461274.9004,12.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DocumentRef: VOTx3724945 20260822.4004 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 08 22.4004 2461274.9004 12.03 06:19:41.09 +13:22:20.0
197.43857 -0.80917 galactic Ori Second-epoch detections are separated by 0.9" and 9.1 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 3332489863978687744 | 06:19:41.05 +13:22:19.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.127+/-0.028 (M)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:19:41.09 +13:22:20.0: 13.01 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:19:41.09 +13:22:20.0: 13.00 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.00 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 19 41.09 +13 22 20.0 12.0 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 3332489863978687744,2461274.9004,12.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3332489863978687744 20260822.4004 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 08 22.4004 2461274.9004 11.95 06:13:46.83 +11:22:34.6
198.51240 -3.02516 galactic Ori Second-epoch detections are separated by 1.9" and 8.9 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 | DocumentRef: VOTx3751412 | 06:13:46.83 +11:22:34.6 (user input) | (VSX @ VizieR) | (VSX @ VizieR) | (position from user input) J-Ks=11.819+/- (unrealisitic color!)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:13:46.83 +11:22:34.6: 12.97 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:13:46.83 +11:22:34.6: 12.94 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.95 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 13 46.83 +11 22 34.6 11.9 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DocumentRef: VOTx3751412,2461274.9004,11.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DocumentRef: VOTx3751412 20260822.4004 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 08 22.4004 2461274.9004 11.92 06:21:12.39 +12:29:13.2
198.39415 -0.89940 galactic Ori Second-epoch detections are separated by 1.5" and 9.2 pix
The object was found in VSX 1" ASASSN-V J062112.31+122913.1
Type: SR
# Max. Min./Amp. JD0 Period
14.650 g Y 0.230 g 2459115.00600 33.370000000000
The object was not found in astcheck.
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:21:12.39 +12:29:13.2: 12.98 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:21:12.39 +12:29:13.2: 12.89 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.93 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 21 12.39 +12 29 13.2 11.9 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J062112.31+122913.1,2461274.9004,11.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J062112.31+122913.1 20260822.4004 11.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4004 2461274.9004 12.05 06:22:02.25 +14:28:25.0
196.73593 0.21323 galactic Ori Second-epoch detections are separated by 1.2" and 9.1 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 J095.5107+14.4753 | 06:22:02.25 +14:28:25.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.368+/-0.034 (G)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:22:02.25 +14:28:25.0: 12.97 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:22:02.25 +14:28:25.0: 12.95 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.96 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 22 02.25 +14 28 25.0 12.1 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J095.5107+14.4753,2461274.9004,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J095.5107+14.4753 20260822.4004 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 08 22.4004 2461274.9004 11.97 06:21:22.94 +15:36:43.5
195.65678 0.60899 galactic Ori Second-epoch detections are separated by 1.0" and 8.9 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 3369013514247843072 | 06:21:22.93 +15:36:42.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.825+/-0.032 (M)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:21:22.94 +15:36:43.5: 12.97 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:21:22.94 +15:36:43.5: 12.90 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.93 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 21 22.94 +15 36 43.5 12.0 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 3369013514247843072,2461274.9004,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3369013514247843072 20260822.4004 11.97CV 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 08 22.4004 2461274.9004 11.89 06:19:47.99 +13:27:05.8
197.38177 -0.74704 galactic Ori Second-epoch detections are separated by 0.4" and 8.9 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 J094.9482+13.4578 | 06:19:47.58 +13:27:28.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.897+/-0.027 (M)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:19:47.99 +13:27:05.8: 12.95 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:19:47.99 +13:27:05.8: 13.01 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.97 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 19 47.99 +13 27 05.8 11.9 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J094.9482+13.4578,2461274.9004,11.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J094.9482+13.4578 20260822.4004 11.89CV 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 08 22.4004 2461274.9004 11.83 06:14:41.90 +11:18:57.9
198.67264 -2.85596 galactic Ori Second-epoch detections are separated by 0.5" and 9.0 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 3331626270613411584 | 06:14:41.91 +11:18:56.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.941+/-0.032 (M)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:14:41.90 +11:18:57.9: 12.96 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:14:41.90 +11:18:57.9: 12.94 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.95 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 14 41.90 +11 18 57.9 11.8 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 3331626270613411584,2461274.9004,11.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3331626270613411584 20260822.4004 11.83CV 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 08 22.4004 2461274.9004 11.93 06:16:19.85 +12:10:09.7
198.11117 -2.09893 galactic Ori Second-epoch detections are separated by 1.2" and 8.7 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 | DocumentRef: VOTx3779053 | 06:16:19.85 +12:10:09.7 (user input) | (GCVS) | (GCVS) | (position from user input) SpType: A0III (LAMOST DR5)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:16:19.85 +12:10:09.7: 12.96 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:16:19.85 +12:10:09.7: 12.98 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.97 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 16 19.85 +12 10 09.7 11.9 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DocumentRef: VOTx3779053,2461274.9004,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DocumentRef: VOTx3779053 20260822.4004 11.93CV 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 08 22.4004 2461274.9004 11.96 06:22:23.94 +16:08:57.8
195.29734 1.07728 galactic Ori Second-epoch detections are separated by 2.2" and 9.3 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 | DocumentRef: VOTx3797497 | 06:22:23.94 +16:08:57.8 (user input) | (VSX @ VizieR) | (VSX @ VizieR) | (position from user input)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:22:23.94 +16:08:57.8: 12.95 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:22:23.94 +16:08:57.8: 12.92 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.93 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 22 23.94 +16 08 57.8 12.0 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DocumentRef: VOTx3797497,2461274.9004,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DocumentRef: VOTx3797497 20260822.4004 11.96CV 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 08 22.4004 2461274.9004 11.97 06:19:59.25 +13:26:56.2
197.40566 -0.70807 galactic Ori Second-epoch detections are separated by 0.5" and 9.0 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 3332492131721413504 | 06:19:58.67 +13:27:40.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G3 (LAMOST DR5)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:19:59.25 +13:26:56.2: 12.93 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:19:59.25 +13:26:56.2: 12.94 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.94 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 19 59.25 +13 26 56.2 12.0 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 3332492131721413504,2461274.9004,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3332492131721413504 20260822.4004 11.97CV 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 08 22.4004 2461274.9004 11.87 06:15:34.93 +08:57:35.2
200.85383 -3.78221 galactic Ori Second-epoch detections are separated by 1.3" and 9.0 pix
The object was found in VSX 2" ASAS J061535+0857.5
Type: MISC
# Max. Min./Amp. JD0 Period
12.930 V Y 1.120 V 2452973.80000 232.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:15:34.93 +08:57:35.2: 12.92 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:15:34.93 +08:57:35.2: 13.07 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.98 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 15 34.93 +08 57 35.2 11.9 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J061535+0857.5,2461274.9004,11.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J061535+0857.5 20260822.4004 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 08 22.4004 2461274.9004 11.96 06:19:14.18 +12:05:39.4
198.51370 -1.50894 galactic Ori Second-epoch detections are separated by 1.6" and 9.2 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 | DocumentRef: VOTx3829163 | 06:19:14.18 +12:05:39.4 (user input) | (GCVS) | (GCVS) | (position from user input) J-Ks=1.269+/-0.027 (Very red! L if it's a dwarf)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:19:14.18 +12:05:39.4: 12.92 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:19:14.18 +12:05:39.4: 12.92 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.92 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 19 14.18 +12 05 39.4 12.0 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DocumentRef: VOTx3829163,2461274.9004,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DocumentRef: VOTx3829163 20260822.4004 11.96CV 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 08 22.4004 2461274.9004 11.98 06:22:36.37 +14:50:32.6
196.47496 0.50786 galactic Ori Second-epoch detections are separated by 2.9" and 8.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | DocumentRef: VOTx3833822 | 06:22:38.56 +14:50:53.6 (Gaia DR3) | (GCVS) | (GCVS) | Gaia3var=NOT_AVAILABLE J-Ks=0.794+/-0.027 (K)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:22:36.37 +14:50:32.6: 12.92 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:22:36.37 +14:50:32.6: 12.87 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.89 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 22 36.37 +14 50 32.6 12.0 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DocumentRef: VOTx3833822,2461274.9004,11.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DocumentRef: VOTx3833822 20260822.4004 11.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4004 2461274.9004 11.96 06:23:38.45 +16:21:05.8
195.25839 1.43535 galactic Ori Second-epoch detections are separated by 5.5" and 9.4 pix
The object was found in VSX15" Gaia DR3 3369170641331692800
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
14.270 G 14.300 G A
The object was not found in astcheck.
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:23:38.45 +16:21:05.8: 12.92 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:23:38.45 +16:21:05.8: 12.92 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.92 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 23 38.45 +16 21 05.8 12.0 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 3369170641331692800,2461274.9004,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3369170641331692800 20260822.4004 11.96CV 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 08 22.4004 2461274.9004 11.91 06:18:20.23 +13:57:36.2
196.76573 -0.81973 galactic Ori Second-epoch detections are separated by 1.9" and 8.6 pix
The object was found in VSX 1" ASASSN-V J061820.20+135736.5
Type: L
# Max. Min./Amp. JD0 Period
13.060 V 13.180 V
The object was not found in astcheck.
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:18:20.23 +13:57:36.2: 12.90 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:18:20.23 +13:57:36.2: 12.87 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.88 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 18 20.23 +13 57 36.2 11.9 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J061820.20+135736.5,2461274.9004,11.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J061820.20+135736.5 20260822.4004 11.91CV 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 08 22.4004 2461274.9004 11.84 06:23:02.60 +15:01:17.7
196.36625 0.68519 galactic Ori Second-epoch detections are separated by 1.0" and 8.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J095.7600+15.0235 | 06:23:02.60 +15:01:17.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.814+/-0.026 (K)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:23:02.60 +15:01:17.7: 12.90 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:23:02.60 +15:01:17.7: 12.83 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.86 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 23 02.60 +15 01 17.7 11.8 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J095.7600+15.0235,2461274.9004,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J095.7600+15.0235 20260822.4004 11.84CV 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 08 22.4004 2461274.9004 11.67 06:24:18.82 +17:36:38.1
194.22007 2.16600 galactic Gem Second-epoch detections are separated by 3.3" and 9.2 pix
The object was found in VSX 2" ASASSN-V J062418.71+173638.1
Type: SR
# Max. Min./Amp. JD0 Period
14.140 g Y 0.430 g 2458824.67800 60.880000000000
The object was not found in astcheck.
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:24:18.82 +17:36:38.1: 12.86 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:24:18.82 +17:36:38.1: 12.68 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.76 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J062418.71+173638.1,2461274.9004,11.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J062418.71+173638.1 20260822.4004 11.67CV 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 08 22.4004 2461274.9004 11.78 06:22:51.88 +15:19:35.5
196.07668 0.79013 galactic Ori Second-epoch detections are separated by 1.4" and 8.8 pix
The object was found in VSX 0" ASASSN-V J062251.86+151935.4
Type: SR
# Max. Min./Amp. JD0 Period
13.250 V 13.430 V 2457366.00000 474.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:22:51.88 +15:19:35.5: 12.86 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:22:51.88 +15:19:35.5: 12.80 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.82 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 22 51.88 +15 19 35.5 11.8 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J062251.86+151935.4,2461274.9004,11.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J062251.86+151935.4 20260822.4004 11.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4004 2461274.9004 11.89 06:21:42.82 +14:02:36.5
197.07868 -0.05825 galactic Ori Second-epoch detections are separated by 1.0" and 8.9 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 3332646406946696576 | 06:21:42.81 +14:02:36.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.939+/-0.033 (M)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:21:42.82 +14:02:36.5: 12.86 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:21:42.82 +14:02:36.5: 12.82 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.84 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 21 42.82 +14 02 36.5 11.9 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 3332646406946696576,2461274.9004,11.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3332646406946696576 20260822.4004 11.89CV 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 08 22.4004 2461274.9004 11.92 06:21:26.68 +14:52:43.1
196.31106 0.27716 galactic Ori Second-epoch detections are separated by 0.7" and 9.0 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 3368765089040999936 | 06:21:26.67 +14:52:42.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.895+/-0.035 (M)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:21:26.68 +14:52:43.1: 12.86 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:21:26.68 +14:52:43.1: 12.83 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.84 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 21 26.68 +14 52 43.1 11.9 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 3368765089040999936,2461274.9004,11.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3368765089040999936 20260822.4004 11.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4004 2461274.9004 11.90 06:19:06.89 +13:31:29.1
197.23864 -0.85928 galactic Ori Second-epoch detections are separated by 0.7" and 9.0 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 | 06:19:06.89 +13:31:29.1 (user input) | T | P | (position from user input) J-Ks=0.350+/-0.029 (G)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:19:06.89 +13:31:29.1: 12.85 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:19:06.89 +13:31:29.1: 12.83 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.84 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 19 06.89 +13 31 29.1 11.9 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461274.9004,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4004 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 08 22.4004 2461274.9004 11.86 06:16:27.39 +12:55:00.2
197.46762 -1.71710 galactic Ori Second-epoch detections are separated by 0.9" and 8.9 pix
The object was found in VSX 1" ASASSN-V J061627.32+125459.2
Type: L
# Max. Min./Amp. JD0 Period
13.100 V 13.200 V
The object was not found in astcheck.
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:16:27.39 +12:55:00.2: 12.85 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:16:27.39 +12:55:00.2: 12.80 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.82 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 16 27.39 +12 55 00.2 11.9 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J061627.32+125459.2,2461274.9004,11.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J061627.32+125459.2 20260822.4004 11.86CV 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 08 22.4004 2461274.9004 11.86 06:17:13.93 +12:57:00.4
197.52795 -1.53489 galactic Ori Second-epoch detections are separated by 1.8" and 8.7 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 | DocumentRef: VOTx3920399 | 06:17:13.92 +12:57:00.1 (Gaia DR3) | (GCVS) | (GCVS) | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:17:13.93 +12:57:00.4: 12.84 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:17:13.93 +12:57:00.4: 12.78 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.81 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 17 13.93 +12 57 00.4 11.9 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DocumentRef: VOTx3920399,2461274.9004,11.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DocumentRef: VOTx3920399 20260822.4004 11.86CV 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 08 22.4004 2461274.9004 11.90 06:20:36.88 +14:59:16.1
196.12034 0.15170 galactic Ori Second-epoch detections are separated by 2.1" and 8.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:20:36.88 +14:59:16.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:20:36.88 +14:59:16.1: 12.83 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:20:36.88 +14:59:16.1: 12.88 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.85 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 20 36.88 +14 59 16.1 11.9 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461274.9004,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4004 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 08 22.4004 2461274.9004 11.82 06:19:39.31 +13:12:58.5
197.57267 -0.88917 galactic Ori Second-epoch detections are separated by 1.9" and 8.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 3332417300510223872 | 06:19:39.25 +13:12:57.8 (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=1.051+/-0.028 (M)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:19:39.31 +13:12:58.5: 12.82 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:19:39.31 +13:12:58.5: 12.77 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.79 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 19 39.31 +13 12 58.5 11.8 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 3332417300510223872,2461274.9004,11.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 3332417300510223872 20260822.4004 11.82CV 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 08 22.4004 2461274.9004 11.84 06:24:36.07 +15:32:08.2
196.08785 1.25780 galactic Ori Second-epoch detections are separated by 0.3" and 9.0 pix
The object was found in VSX 0" ASASSN-V J062436.04+153208.2
Type: SRS
# Max. Min./Amp. JD0 Period
14.040 g Y 0.360 g 2458906.76400 27.011000000000
The object was not found in astcheck.
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:24:36.07 +15:32:08.2: 12.81 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:24:36.07 +15:32:08.2: 12.73 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.77 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 24 36.07 +15 32 08.2 11.8 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J062436.04+153208.2,2461274.9004,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J062436.04+153208.2 20260822.4004 11.84CV 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 08 22.4004 2461274.9004 11.82 06:20:06.84 +13:21:31.0
197.49983 -0.72356 galactic Ori Second-epoch detections are separated by 0.7" and 8.9 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 3332490138856595968 | 06:20:06.82 +13:21:30.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.196+/-0.030 (M)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:20:06.84 +13:21:31.0: 12.77 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:20:06.84 +13:21:31.0: 12.77 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.77 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 20 06.84 +13 21 31.0 11.8 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 3332490138856595968,2461274.9004,11.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3332490138856595968 20260822.4004 11.82CV 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 08 22.4004 2461274.9004 11.82 06:21:02.86 +13:58:55.2
197.05690 -0.22972 galactic Ori Second-epoch detections are separated by 1.7" and 9.3 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 | DocumentRef: VOTx3958352 | 06:21:02.86 +13:58:55.2 (user input) | (GCVS) | (GCVS) | (position from user input) J-Ks=0.358+/-0.032 (G)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:21:02.86 +13:58:55.2: 12.79 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:21:02.86 +13:58:55.2: 12.74 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.76 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 21 02.86 +13 58 55.2 11.8 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DocumentRef: VOTx3958352,2461274.9004,11.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DocumentRef: VOTx3958352 20260822.4004 11.82CV 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 08 22.4004 2461274.9004 11.84 06:18:17.29 +13:14:30.7
197.39281 -1.17022 galactic Ori Second-epoch detections are separated by 0.8" and 8.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:18:17.29 +13:14:30.7 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:18:17.29 +13:14:30.7: 12.78 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:18:17.29 +13:14:30.7: 12.77 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.78 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 18 17.29 +13 14 30.7 11.8 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461274.9004,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4004 11.84CV 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 08 22.4004 2461274.9004 11.85 06:18:59.71 +11:41:49.2
198.83617 -1.74853 galactic Ori Second-epoch detections are separated by 2.0" and 9.3 pix
The object was found in VSX 0" ASASSN-V J061859.72+114148.9
Type: SR
# Max. Min./Amp. JD0 Period
13.150 V 13.370 V 2457439.87600 54.690000000000
The object was not found in astcheck.
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:18:59.71 +11:41:49.2: 12.77 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:18:59.71 +11:41:49.2: 12.87 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.82 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 18 59.71 +11 41 49.2 11.8 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J061859.72+114148.9,2461274.9004,11.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J061859.72+114148.9 20260822.4004 11.85CV 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 08 22.4004 2461274.9004 11.78 06:15:58.94 +12:04:19.7
198.15632 -2.22006 galactic Ori Second-epoch detections are separated by 0.9" and 8.9 pix
The object was found in VSX23" Gaia DR3 3331870976373688064
Type: E
# Max. Min./Amp. JD0 Period
15.490 G 16.580 G 1.248230000000 A
ATTENTION: measured mag 11.78 is 3.7 mag brighter than the VSX record maximum brightness 15.49 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:15:58.94 +12:04:19.7: 12.75 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:15:58.94 +12:04:19.7: 12.67 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.70 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 15 58.94 +12 04 19.7 11.8 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 3331870976373688064,2461274.9004,11.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3331870976373688064 20260822.4004 11.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4004 2461274.9004 11.88 06:22:01.48 +15:05:42.4
196.18587 0.50256 galactic Ori Second-epoch detections are separated by 0.7" and 9.0 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 3368775190804119808 | 06:22:01.51 +15:05:41.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.989+/-0.033 (M)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:22:01.48 +15:05:42.4: 12.75 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:22:01.48 +15:05:42.4: 12.81 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.78 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 22 01.48 +15 05 42.4 11.9 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 3368775190804119808,2461274.9004,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3368775190804119808 20260822.4004 11.88CV 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 08 22.4004 2461274.9004 11.85 06:14:14.37 +11:35:24.1
198.37784 -2.82448 galactic Ori Second-epoch detections are separated by 1.6" and 9.0 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 3331823113255035776 | 06:14:14.38 +11:35:24.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.874+/-0.032 (M)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:14:14.37 +11:35:24.1: 12.74 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:14:14.37 +11:35:24.1: 12.73 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.74 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 14 14.37 +11 35 24.1 11.8 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 3331823113255035776,2461274.9004,11.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3331823113255035776 20260822.4004 11.85CV 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 08 22.4004 2461274.9004 11.71 06:17:04.67 +13:15:59.3
197.23152 -1.41791 galactic Ori Second-epoch detections are separated by 2.2" and 9.3 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 | DocumentRef: VOTx4031981 | 06:17:04.64 +13:15:58.6 (Gaia DR3) | (VSX @ VizieR) | (VSX @ VizieR) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:17:04.67 +13:15:59.3: 12.72 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:17:04.67 +13:15:59.3: 12.71 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.71 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 17 04.67 +13 15 59.3 11.7 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DocumentRef: VOTx4031981,2461274.9004,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DocumentRef: VOTx4031981 20260822.4004 11.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4004 2461274.9004 11.77 06:16:37.12 +11:38:33.8
198.60854 -2.28680 galactic Ori Second-epoch detections are separated by 2.3" and 8.9 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 | DocumentRef: VOTx4037910 | 06:16:37.12 +11:38:33.8 (user input) | (VSX @ VizieR) | (VSX @ VizieR) | (position from user input)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:16:37.12 +11:38:33.8: 12.72 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:16:37.12 +11:38:33.8: 12.71 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.72 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 16 37.12 +11 38 33.8 11.8 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DocumentRef: VOTx4037910,2461274.9004,11.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DocumentRef: VOTx4037910 20260822.4004 11.77CV 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 08 22.4004 2461274.9004 11.82 06:22:03.80 +14:30:06.5
196.71399 0.23199 galactic Ori Second-epoch detections are separated by 1.2" and 9.1 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 | DocumentRef: VOTx4041300 | 06:22:03.80 +14:30:06.5 (user input) | (GCVS) | (GCVS) | (position from user input)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:22:03.80 +14:30:06.5: 12.69 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:22:03.80 +14:30:06.5: 12.68 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.69 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 22 03.80 +14 30 06.5 11.8 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DocumentRef: VOTx4041300,2461274.9004,11.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DocumentRef: VOTx4041300 20260822.4004 11.82CV 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 08 22.4004 2461274.9004 11.62 06:15:40.38 +12:19:06.2
197.90354 -2.16957 galactic Ori Second-epoch detections are separated by 1.6" and 8.9 pix
The object was found in VSX 1" ASASSN-V J061540.32+121906.6
Type: SR
# Max. Min./Amp. JD0 Period
14.220 g Y 0.190 g 2458812.08600 30.120000000000
The object was not found in astcheck.
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:15:40.38 +12:19:06.2: 12.69 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:15:40.38 +12:19:06.2: 12.62 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.65 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 15 40.38 +12 19 06.2 11.6 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J061540.32+121906.6,2461274.9004,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J061540.32+121906.6 20260822.4004 11.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4004 2461274.9004 11.77 06:19:37.86 +13:54:56.6
196.95325 -0.56408 galactic Ori Second-epoch detections are separated by 0.3" and 8.9 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 | DocumentRef: VOTx4049973 | 06:19:37.84 +13:54:55.5 (Gaia DR3) | (GCVS) | (GCVS) | Gaia3var=NOT_AVAILABLE J-Ks=0.936+/-0.024 (M)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:19:37.86 +13:54:56.6: 12.69 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:19:37.86 +13:54:56.6: 12.67 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.68 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 19 37.86 +13 54 56.6 11.8 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DocumentRef: VOTx4049973,2461274.9004,11.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DocumentRef: VOTx4049973 20260822.4004 11.77CV 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 08 22.4004 2461274.9004 11.70 06:17:31.32 +12:40:45.1
197.80009 -1.60110 galactic Ori Second-epoch detections are separated by 0.6" and 8.9 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 3332019719679009024 | 06:17:31.20 +12:40:45.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.183+/-0.036 (M)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:17:31.32 +12:40:45.1: 12.69 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:17:31.32 +12:40:45.1: 12.68 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.68 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 17 31.32 +12 40 45.1 11.7 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 3332019719679009024,2461274.9004,11.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3332019719679009024 20260822.4004 11.70CV 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 08 22.4004 2461274.9004 11.72 06:16:05.49 +11:27:27.2
198.71039 -2.48830 galactic Ori Second-epoch detections are separated by 0.4" and 9.0 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 | 06:16:05.49 +11:27:27.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:16:05.49 +11:27:27.2: 12.67 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:16:05.49 +11:27:27.2: 12.62 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.64 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 16 05.49 +11 27 27.2 11.7 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461274.9004,11.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4004 11.72CV 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 08 22.4004 2461274.9004 11.72 06:22:12.45 +17:01:24.1
194.50388 1.44695 galactic Ori Second-epoch detections are separated by 2.1" and 9.0 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 | DocumentRef: VOTx4083930 | 06:22:12.44 +17:01:23.5 (Gaia DR3) | (VSX @ VizieR) | (VSX @ VizieR) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:22:12.45 +17:01:24.1: 12.68 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:22:12.45 +17:01:24.1: 12.61 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.64 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 22 12.45 +17 01 24.1 11.7 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DocumentRef: VOTx4083930,2461274.9004,11.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DocumentRef: VOTx4083930 20260822.4004 11.72CV 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 08 22.4004 2461274.9004 11.48 06:20:37.32 +14:08:16.7
196.87069 -0.24729 galactic Ori Second-epoch detections are separated by 1.0" and 9.1 pix
The object was found in VSX 1" ASASSN-V J062037.26+140816.0
Type: SRS
# Max. Min./Amp. JD0 Period
12.960 V 13.060 V 2457324.94100 20.739000000000
The object was not found in astcheck.
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:20:37.32 +14:08:16.7: 12.66 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:20:37.32 +14:08:16.7: 12.58 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.61 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 20 37.32 +14 08 16.7 11.5 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J062037.26+140816.0,2461274.9004,11.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J062037.26+140816.0 20260822.4004 11.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4004 2461274.9004 11.56 06:22:11.41 +14:25:20.7
196.79849 0.22179 galactic Ori Second-epoch detections are separated by 2.8" and 8.7 pix
The object was found in VSX 2" ASASSN-V J062211.46+142522.9
Type: SR
# Max. Min./Amp. JD0 Period
13.250 V 13.610 V 2458553.51850 143.465111400000
The object was not found in astcheck.
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:22:11.41 +14:25:20.7: 12.62 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:22:11.41 +14:25:20.7: 12.57 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.59 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 22 11.41 +14 25 20.7 11.6 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J062211.46+142522.9,2461274.9004,11.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J062211.46+142522.9 20260822.4004 11.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4004 2461274.9004 11.59 06:17:11.53 +12:44:29.7
197.70699 -1.64236 galactic Ori Second-epoch detections are separated by 0.3" and 8.9 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 3332067892032197632 | 06:17:11.57 +12:44:29.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.898+/-0.028 (M)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:17:11.53 +12:44:29.7: 12.61 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:17:11.53 +12:44:29.7: 12.62 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.61 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 17 11.53 +12 44 29.7 11.6 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 3332067892032197632,2461274.9004,11.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3332067892032197632 20260822.4004 11.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4004 2461274.9004 11.64 06:21:11.60 +14:23:30.8
196.71191 -0.00557 galactic Ori Second-epoch detections are separated by 0.6" and 8.9 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 3344669021139509888 | 06:21:11.54 +14:23:30.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.216+/-0.047 (M)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:21:11.60 +14:23:30.8: 12.60 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:21:11.60 +14:23:30.8: 12.55 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.57 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 21 11.60 +14 23 30.8 11.6 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 3344669021139509888,2461274.9004,11.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3344669021139509888 20260822.4004 11.64CV 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 08 22.4004 2461274.9004 11.63 06:14:55.53 +11:52:39.1
198.20472 -2.53996 galactic Ori Second-epoch detections are separated by 0.7" and 9.0 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 | DocumentRef: VOTx4132423 | 06:14:55.55 +11:52:38.3 (Gaia DR3) | (VSX @ VizieR) | (VSX @ VizieR) | Gaia3var=NOT_AVAILABLE J-Ks=0.970+/-0.028 (M)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:14:55.53 +11:52:39.1: 12.59 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:14:55.53 +11:52:39.1: 12.60 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.59 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 14 55.53 +11 52 39.1 11.6 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DocumentRef: VOTx4132423,2461274.9004,11.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DocumentRef: VOTx4132423 20260822.4004 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 08 22.4004 2461274.9004 11.63 06:14:21.80 +11:39:10.0
198.33705 -2.76793 galactic Ori Second-epoch detections are separated by 1.4" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:14:21.80 +11:39:10.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:14:21.80 +11:39:10.0: 12.58 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:14:21.80 +11:39:10.0: 12.62 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.60 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 14 21.80 +11 39 10.0 11.6 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461274.9004,11.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4004 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 08 22.4004 2461274.9004 11.64 06:21:00.31 +13:51:48.9
197.15651 -0.29458 galactic Ori Second-epoch detections are separated by 2.5" and 8.6 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 3332613936993949440 | 06:21:00.34 +13:51:48.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:21:00.31 +13:51:48.9: 12.56 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:21:00.31 +13:51:48.9: 12.60 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.58 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 21 00.31 +13 51 48.9 11.6 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 3332613936993949440,2461274.9004,11.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3332613936993949440 20260822.4004 11.64CV 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 08 22.4004 2461274.9004 11.61 05:42:52.71 +16:12:45.0
190.56823 -7.15435 galactic Tau Second-epoch detections are separated by 1.3" and 8.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J085.7190+16.2120 | 05:42:52.58 +16:12:43.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.148+/-0.026 (M)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 05:42:52.71 +16:12:45.0: 12.50 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 05:42:52.71 +16:12:45.0: 12.61 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.56 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 05 42 52.71 +16 12 45.0 11.6 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J085.7190+16.2120,2461274.9004,11.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J085.7190+16.2120 20260822.4004 11.61CV 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 08 22.4004 2461274.9004 11.56 06:16:05.47 +12:14:58.6
198.01267 -2.11237 galactic Ori Second-epoch detections are separated by 1.5" and 8.7 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 J094.0228+12.2496 | 06:16:05.48 +12:14:58.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.225+/-0.030 (M)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:16:05.47 +12:14:58.6: 12.50 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:16:05.47 +12:14:58.6: 12.47 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.48 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 16 05.47 +12 14 58.6 11.6 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J094.0228+12.2496,2461274.9004,11.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J094.0228+12.2496 20260822.4004 11.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4004 2461274.9004 11.52 06:20:08.32 +14:28:04.8
196.52444 -0.19492 galactic Ori Second-epoch detections are separated by 0.9" and 9.0 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 3344684410003340288 | 06:20:08.28 +14:28:04.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.028+/-0.028 (M)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:20:08.32 +14:28:04.8: 12.48 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:20:08.32 +14:28:04.8: 12.45 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.47 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 20 08.32 +14 28 04.8 11.5 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 3344684410003340288,2461274.9004,11.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3344684410003340288 20260822.4004 11.52CV 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 08 22.4004 2461274.9004 11.48 06:20:13.32 +14:22:12.0
196.62037 -0.22336 galactic Ori Second-epoch detections are separated by 1.0" and 8.9 pix
The object was found in VSX 6" ZTF J062012.93+142209.4
Type: SR
# Max. Min./Amp. JD0 Period
14.591 g Y 0.160 g 2458236.58630 39.974796000000
The object was not found in astcheck.
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:20:13.32 +14:22:12.0: 12.46 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:20:13.32 +14:22:12.0: 12.38 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.41 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 20 13.32 +14 22 12.0 11.5 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J062012.93+142209.4,2461274.9004,11.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J062012.93+142209.4 20260822.4004 11.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4004 2461274.9004 11.48 06:14:39.77 +09:56:55.2
199.87359 -3.51330 galactic Ori Second-epoch detections are separated by 2.5" and 8.8 pix
The object was found in VSX 2" ASASSN-V J061439.80+095653.7
Type: SRS
# Max. Min./Amp. JD0 Period
12.840 V 12.930 V 2457043.86200 24.827000000000
The object was not found in astcheck.
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:14:39.77 +09:56:55.2: 12.45 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:14:39.77 +09:56:55.2: 12.54 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.49 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 14 39.77 +09 56 55.2 11.5 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J061439.80+095653.7,2461274.9004,11.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J061439.80+095653.7 20260822.4004 11.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4004 2461274.9004 11.47 06:21:57.52 +16:30:57.4
194.92403 1.15612 galactic Ori Second-epoch detections are separated by 1.1" and 9.1 pix
The object was found in VSX 1" ASASSN-V J062157.50+163057.0
Type: L
# Max. Min./Amp. JD0 Period
12.640 V 12.840 V
The object was not found in astcheck.
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:21:57.52 +16:30:57.4: 12.42 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:21:57.52 +16:30:57.4: 12.36 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.39 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 21 57.52 +16 30 57.4 11.5 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J062157.50+163057.0,2461274.9004,11.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J062157.50+163057.0 20260822.4004 11.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4004 2461274.9004 11.36 06:12:17.54 +09:21:02.5
200.12265 -4.31152 galactic Ori Second-epoch detections are separated by 1.2" and 9.1 pix
The object was found in VSX 1" ASAS J061218+0921.0
Type: MISC
# Max. Min./Amp. JD0 Period
13.000 V Y 0.610 V 2452876.10000 178.110463000000 C
The object was not found in astcheck.
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:12:17.54 +09:21:02.5: 12.37 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:12:17.54 +09:21:02.5: 12.43 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.40 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 12 17.54 +09 21 02.5 11.4 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J061218+0921.0,2461274.9004,11.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J061218+0921.0 20260822.4004 11.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4004 2461274.9004 11.27 06:14:44.26 +10:32:56.3
199.35311 -3.21207 galactic Ori Second-epoch detections are separated by 0.8" and 9.0 pix
The object was found in VSX 1" ASAS J061444+1032.9
Type: MISC
# Max. Min./Amp. JD0 Period
12.560 V Y 0.280 V 2452547.90000 70.455095000000
The object was not found in astcheck.
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:14:44.26 +10:32:56.3: 12.31 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:14:44.26 +10:32:56.3: 12.25 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.28 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 14 44.26 +10 32 56.3 11.3 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J061444+1032.9,2461274.9004,11.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J061444+1032.9 20260822.4004 11.27CV 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 08 22.4004 2461274.9004 11.38 06:28:20.97 +17:32:35.3
194.72714 2.98643 galactic Gem Second-epoch detections are separated by 0.8" and 9.0 pix
The object was found in VSX 1" ASASSN-V J062820.98+173234.8
Type: L
# Max. Min./Amp. JD0 Period
12.630 V 13.130 V
The object was not found in astcheck.
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:28:20.97 +17:32:35.3: 12.26 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:28:20.97 +17:32:35.3: 12.44 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.34 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J062820.98+173234.8,2461274.9004,11.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J062820.98+173234.8 20260822.4004 11.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4004 2461274.9004 11.22 06:13:45.34 +11:31:40.2
198.37607 -2.95830 galactic Ori Second-epoch detections are separated by 0.8" and 9.0 pix
The object was found in VSX 1" ASAS J061345+1131.7
Type: MISC
# Max. Min./Amp. JD0 Period
12.880 V Y 0.550 V 2452542.60000 70.600000000000 M6
The object was not found in astcheck.
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:13:45.34 +11:31:40.2: 12.20 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:13:45.34 +11:31:40.2: 12.30 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.24 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 13 45.34 +11 31 40.2 11.2 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J061345+1131.7,2461274.9004,11.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J061345+1131.7 20260822.4004 11.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4004 2461274.9004 11.07 06:33:59.97 +15:17:02.2
197.36017 3.14930 galactic Gem Second-epoch detections are separated by 0.4" and 9.1 pix
The object was found in VSX 1" V0381 Gem
Type: SR
# Max. Min./Amp. JD0 Period
12.300 V 13.500 V 2452891.70000 107.000000000000 M10
The object was not found in astcheck.
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:33:59.97 +15:17:02.2: 12.12 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:33:59.97 +15:17:02.2: 11.90 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.99 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0381 Gem,2461274.9004,11.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0381 Gem 20260822.4004 11.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4004 2461274.9004 11.18 06:14:55.33 +10:20:22.7
199.55920 -3.27156 galactic Ori Second-epoch detections are separated by 1.2" and 9.0 pix
The object was found in VSX 0" ASAS J061455+1020.4
Type: MISC
# Max. Min./Amp. JD0 Period
12.370 V Y 0.290 V 2452526.10000 52.840000000000
The object was not found in astcheck.
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:14:55.33 +10:20:22.7: 12.10 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:14:55.33 +10:20:22.7: 12.17 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.13 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 14 55.33 +10 20 22.7 11.2 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J061455+1020.4,2461274.9004,11.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J061455+1020.4 20260822.4004 11.18CV 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 08 22.4004 2461274.9004 11.23 06:15:54.47 +10:33:56.7
199.47499 -2.95097 galactic Ori Second-epoch detections are separated by 0.3" and 9.0 pix
The object was found in VSX 1" ASASSN-V J061554.50+103357.2
Type: SRS
# Max. Min./Amp. JD0 Period
13.310 g Y 0.200 g 2458596.47500 28.810000000000
The object was not found in astcheck.
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:15:54.47 +10:33:56.7: 12.11 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:15:54.47 +10:33:56.7: 12.16 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.13 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 15 54.47 +10 33 56.7 11.2 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J061554.50+103357.2,2461274.9004,11.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J061554.50+103357.2 20260822.4004 11.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4004 2461274.9004 10.95 06:18:14.34 +11:20:45.1
199.05827 -2.07768 galactic Ori Second-epoch detections are separated by 7.1" and 7.9 pix
The object was found in VSX 3" ASASSN-V J061814.39+112047.9
Type: SR
# Max. Min./Amp. JD0 Period
12.350 V 12.540 V 2457653.00000 547.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:18:14.34 +11:20:45.1: 12.11 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:18:14.34 +11:20:45.1: 12.08 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.09 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 18 14.34 +11 20 45.1 10.9 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J061814.39+112047.9,2461274.9004,10.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J061814.39+112047.9 20260822.4004 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 08 22.4004 2461274.9004 11.12 06:19:51.02 +13:36:19.2
197.25204 -0.66366 galactic Ori Second-epoch detections are separated by 0.6" and 9.1 pix
The object was found in VSX 1" ASAS J061951+1336.3
Type: MISC
# Max. Min./Amp. JD0 Period
12.700 V Y 0.210 V 2452623.12000 1.000000000000 M4
The object was not found in astcheck.
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:19:51.02 +13:36:19.2: 12.01 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:19:51.02 +13:36:19.2: 12.31 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.13 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 19 51.02 +13 36 19.2 11.1 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J061951+1336.3,2461274.9004,11.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J061951+1336.3 20260822.4004 11.12CV 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 08 22.4004 2461274.9004 10.80 06:18:42.63 +13:02:54.4
197.61190 -1.17115 galactic Ori Second-epoch detections are separated by 0.2" and 8.9 pix
The object was found in VSX 1" ASAS J061843+1302.9
Type: MISC
# Max. Min./Amp. JD0 Period
12.130 V Y 0.480 V 2452986.40000 173.609421000000 M5
The object was not found in astcheck.
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:18:42.63 +13:02:54.4: 11.98 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:18:42.63 +13:02:54.4: 11.77 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.85 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 18 42.63 +13 02 54.4 10.8 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J061843+1302.9,2461274.9004,10.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J061843+1302.9 20260822.4004 10.80CV 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 08 22.4004 2461274.9004 10.88 06:18:05.68 +12:22:21.5
198.13641 -1.62317 galactic Ori Second-epoch detections are separated by 1.5" and 9.0 pix
The object was found in VSX 2" ASAS J061806+1222.3
Type: MISC
# Max. Min./Amp. JD0 Period
12.160 V Y 0.560 V 2452697.00000 144.700000000000 M5
The object was not found in astcheck.
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:18:05.68 +12:22:21.5: 11.87 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:18:05.68 +12:22:21.5: 11.81 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.84 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 18 05.68 +12 22 21.5 10.9 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J061806+1222.3,2461274.9004,10.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J061806+1222.3 20260822.4004 10.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4004 2461274.9004 10.91 06:14:42.50 +11:28:07.8
198.53928 -2.78115 galactic Ori Second-epoch detections are separated by 0.5" and 9.0 pix
The object was found in VSX 0" ASASSN-V J061442.47+112807.8
Type: SR
# Max. Min./Amp. JD0 Period
13.150 g Y 0.180 g 2458484.56600 217.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:14:42.50 +11:28:07.8: 11.85 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:14:42.50 +11:28:07.8: 11.82 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.84 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 14 42.50 +11 28 07.8 10.9 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J061442.47+112807.8,2461274.9004,10.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J061442.47+112807.8 20260822.4004 10.91CV 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 08 22.4004 2461274.9004 10.54 06:12:28.76 +10:28:25.6
199.15471 -3.73608 galactic Ori Second-epoch detections are separated by 1.2" and 9.1 pix
The object was found in VSX 1" ASAS J061229+1028.4
Type: MISC
# Max. Min./Amp. JD0 Period
8.508 Ic Y 0.226 Ic 2452663.10000 93.170000000000
The object was not found in astcheck.
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:12:28.76 +10:28:25.6: 11.39 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:12:28.76 +10:28:25.6: 11.55 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.46 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 12 28.76 +10 28 25.6 10.5 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J061229+1028.4,2461274.9004,10.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J061229+1028.4 20260822.4004 10.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4004 2461274.9004 10.10 06:16:06.52 +10:56:43.1
199.16381 -2.72758 galactic Ori Second-epoch detections are separated by 0.5" and 9.0 pix
The object was found in VSX 0" ASAS J061607+1056.7
Type: MISC
# Max. Min./Amp. JD0 Period
11.400 V Y 0.560 V 2452666.00000 90.795688000000
The object was not found in astcheck.
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:16:06.52 +10:56:43.1: 11.14 +/- 0.00 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:16:06.52 +10:56:43.1: 10.95 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.03 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.4004* 06 16 06.52 +10 56 43.1 10.1 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J061607+1056.7,2461274.9004,10.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J061607+1056.7 20260822.4004 10.10CV 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
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.81662337 23.12.2025 07:35:46.259 /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
First image: 2461032.81662337 23.12.2025 07:35:46.259 /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
Last image: 2461274.90082885 22.08.2026 09:37:01.613 /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Ori-02-Q1b1x1_043748_TTUQ1b1x1_2949840_gjrQHCHz/fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137.fits
JD time system (TT/UTC/UNKNOWN): UTC
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.75
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: 5 seconds
Number of parallel threads: 3
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
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 27992
Objects passed selection criteria: 27816
Measurements per detected object (mean, median, min, max): 2.2 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.2 2.0 2 4
Average stars detected per image: 17250.5
Average stars matched: 16414.8 (95.1552 %)
Memory usage VmPeak: 253100 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Aug 20 15:05:04 CDT 2026
VaST build number 1.0rc89-192-g23359006
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-20)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Aug 22 04:40:53 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: 2461032.81662337 23.12.2025 07:35:46.259 /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
First image: 2461032.81662337 23.12.2025 07:35:46.259 /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
Last image: 2461274.90082885 22.08.2026 09:37:01.613 /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Ori-02-Q1b1x1_043748_TTUQ1b1x1_2949840_gjrQHCHz/fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 224
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.41
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: 29 seconds
Number of parallel threads: 3
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
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 202990
Objects passed selection criteria: 202352
Measurements per detected object (mean, median, min, max): 2.3 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.3 2.0 2 4
Average stars detected per image: 129264
Average stars matched: 122248 (94.5731 %)
Memory usage VmPeak: 667748 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Aug 20 15:05:04 CDT 2026
VaST build number 1.0rc89-192-g23359006
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-20)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Aug 22 04:42:09 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Ori-02-Q1b1x1_043748_TTUQ1b1x1_2949840_gjrQHCHz/fd_Ori-02-Q1b1x1_2026-08-22_04-35-52_20.00sec_0.00C_LIGHTs_0136.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Ori-02-Q1b1x1_043748_TTUQ1b1x1_2949840_gjrQHCHz/fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137.fits
SExtractor catalog cache: saved Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.cat to cache
SExtractor catalog cache: saved Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.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/Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Ori-02-Q1b1x1_043748_TTUQ1b1x1_2949840_gjrQHCHz/fd_Ori-02-Q1b1x1_2026-08-22_04-35-52_20.00sec_0.00C_LIGHTs_0136.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Ori-02-Q1b1x1_043748_TTUQ1b1x1_2949840_gjrQHCHz/fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137.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: 2461274.90002491
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits exists and is non-empty
wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits exists and is non-empty
wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-35-52_20.00sec_0.00C_LIGHTs_0136.fits exists and is non-empty
wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits (1st reference image)
verification OK: wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
Image size: 941.6'x627.1' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 06:13:27.287 +13:59:26.52 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-35-52_20.00sec_0.00C_LIGHTs_0136.fits (1st new image)
verification OK: wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-35-52_20.00sec_0.00C_LIGHTs_0136.fits
Image size: 945.0'x626.9' 15.8(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 06:13:23.730 +14:00:51.79 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 06:13:27.287 +13:59:26.52
Second-epoch image center 06:13:23.730 +14:00:51.79
Angular distance between the image centers 0.0277 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137.fits (2nd new image)
verification OK: wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137.fits
Image size: 944.8'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 06:13:21.172 +14:00:13.88 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 06:13:27.287 +13:59:26.52
Second-epoch image center 06:13:21.172 +14:00:13.88
Angular distance between the image centers 0.0280 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 06:13:23.730 +14:00:51.79
Second-epoch second image center 06:13:21.172 +14:00:13.88
Angular distance between the image centers 0.01476 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits &> /tmp/tmp.zZmgbAf0me
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits &> /tmp/tmp.MMHMMssi3K
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Ori-02-Q1b1x1_043748_TTUQ1b1x1_2949840_gjrQHCHz/fd_Ori-02-Q1b1x1_2026-08-22_04-35-52_20.00sec_0.00C_LIGHTs_0136.fits &> /tmp/tmp.bVwExKy80n
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Ori-02-Q1b1x1_043748_TTUQ1b1x1_2949840_gjrQHCHz/fd_Ori-02-Q1b1x1_2026-08-22_04-35-52_20.00sec_0.00C_LIGHTs_0136.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Ori-02-Q1b1x1_043748_TTUQ1b1x1_2949840_gjrQHCHz/fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137.fits &> /tmp/tmp.9CoxaOzZpt
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Ori-02-Q1b1x1_043748_TTUQ1b1x1_2949840_gjrQHCHz/fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137.fits
Calibrating the magnitude scale
Found non-empty wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.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_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits and wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits and wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.wcscat
Found non-empty wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits and wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.wcscat
The reference image (wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits) and catalog (wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.wcscat) found
'wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.wcscat' -> 'wcsmag.cat'
Read 31404 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 85.0776 to 101.6789 deg, Dec +8.6286 to +19.2777 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 85.0776 to 101.6789 deg, Dec 8.6286 to 19.2777 deg
Loaded 17819 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): 13015 out of 14781 total matches.
Matched with Tycho-2 14781 out of 31404 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.949600
a=0.000000 b=1.000000 c=22.949600
From vast_summary.log: estimated ref. image limiting mag.: -7.75
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.20
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.20
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 31404 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 85.0776 to 101.6789 deg, Dec +8.6286 to +19.2777 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 85.0776 to 101.6789 deg, Dec 8.6286 to 19.2777 deg
Loaded 17819 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): 13015 out of 14781 total matches.
Matched with Tycho-2 14781 out of 31404 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
Forced-photometry filter: calibrated wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits -> calib.txt_param_ref_wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits (aperture=6.1)
Read 31324 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 84.9118 to 101.4962 deg, Dec +8.4421 to +19.3403 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 84.9118 to 101.4962 deg, Dec 8.4421 to 19.3403 deg
Loaded 18085 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): 12980 out of 14663 total matches.
Matched with Tycho-2 14663 out of 31324 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
Forced-photometry filter: calibrated wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits -> calib.txt_param_ref_wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits (aperture=5.9)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.1 pix Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
2.1 pix Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
2.6 pix fd_Ori-02-Q1b1x1_2026-08-22_04-35-52_20.00sec_0.00C_LIGHTs_0136.fits
2.6 pix fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137.fits
Limiting magnitude estimates:
15.2 mag. Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
15.2 mag. Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
11.6 mag. fd_Ori-02-Q1b1x1_2026-08-22_04-35-52_20.00sec_0.00C_LIGHTs_0136.fits
11.6 mag. fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137.fits
All-image limiting magnitude estimate: 11.6 (SNR ) 9.9 (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 15.5 mag.
Waiting for UCAC5 plate solver
wait
cp: cannot create regular file 'local_wcs_cache/': Not a directory
############ /tmp/tmp.zZmgbAf0me (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-22_CI_Ori-02-Q1b1x1_043748_TTUQ1b1x1_2949840_gjrQHCHz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits' -> 'wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
WCS_IMAGE_NAME=wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
WCS-calibrated image found: wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
Checking if the catalog wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.wcscat corresponding to the image wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits alredy exist and is non-empty...
Catalog wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.wcscat corresponding to the image wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
WCS catalog name: wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3718, bad_region=0, passed=31404
Got 31404 stars (including 27641 good ones) from the SExtractor catalog wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.wcscat
util/solve_plate_with_UCAC5 got 31404 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4849 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4785 matched stars entering correct_measured_positions(), 4786 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4785 matched stars entering correct_measured_positions(), 31404 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4848 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4783 matched stars entering correct_measured_positions(), 31404 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 4783 matched stars entering correct_measured_positions(), 31404 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 4783 stars left (next iteration limit 5263)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits N_match=4783 sigma_overall_arcsec=0.380 sigma_q1_arcsec=0.478 sigma_q2_arcsec=0.377 sigma_q3_arcsec=0.342 sigma_q4_arcsec=0.323 n_q1=1170 n_q2=1223 n_q3=1237 n_q4=1153 worst_quadrant_to_overall_ratio=1.257
The image catalog is written to wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits -region wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.MMHMMssi3K (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-22_CI_Ori-02-Q1b1x1_043748_TTUQ1b1x1_2949840_gjrQHCHz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits' -> 'wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
WCS_IMAGE_NAME=wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
WCS-calibrated image found: wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
Checking if the catalog wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits.wcscat corresponding to the image wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits alredy exist and is non-empty...
Catalog wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits.wcscat corresponding to the image wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
WCS catalog name: wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3619, bad_region=0, passed=31324
Got 31324 stars (including 27657 good ones) from the SExtractor catalog wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits.wcscat
util/solve_plate_with_UCAC5 got 31324 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.4 to 19.3)
Done reading UCAC5 zone files...
Matched 4850 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4788 matched stars entering correct_measured_positions(), 4788 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4788 matched stars entering correct_measured_positions(), 31324 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.4 to 19.3)
Done reading UCAC5 zone files...
Matched 4849 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4788 matched stars entering correct_measured_positions(), 31324 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 4787 matched stars entering correct_measured_positions(), 31324 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 4787 stars left (next iteration limit 5266)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits N_match=4787 sigma_overall_arcsec=0.407 sigma_q1_arcsec=0.498 sigma_q2_arcsec=0.408 sigma_q3_arcsec=0.371 sigma_q4_arcsec=0.355 n_q1=1017 n_q2=1324 n_q3=1130 n_q4=1316 worst_quadrant_to_overall_ratio=1.226
The image catalog is written to wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits -region wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.bVwExKy80n (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_2026-08-22_CI_Ori-02-Q1b1x1_043748_TTUQ1b1x1_2949840_gjrQHCHz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Ori-02-Q1b1x1_043748_TTUQ1b1x1_2949840_gjrQHCHz/fd_Ori-02-Q1b1x1_2026-08-22_04-35-52_20.00sec_0.00C_LIGHTs_0136.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Ori-02-Q1b1x1_043748_TTUQ1b1x1_2949840_gjrQHCHz/fd_Ori-02-Q1b1x1_2026-08-22_04-35-52_20.00sec_0.00C_LIGHTs_0136.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Ori-02-Q1b1x1_043748_TTUQ1b1x1_2949840_gjrQHCHz/fd_Ori-02-Q1b1x1_2026-08-22_04-35-52_20.00sec_0.00C_LIGHTs_0136.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Ori-02-Q1b1x1_043748_TTUQ1b1x1_2949840_gjrQHCHz/fd_Ori-02-Q1b1x1_2026-08-22_04-35-52_20.00sec_0.00C_LIGHTs_0136.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Ori-02-Q1b1x1_043748_TTUQ1b1x1_2949840_gjrQHCHz/fd_Ori-02-Q1b1x1_2026-08-22_04-35-52_20.00sec_0.00C_LIGHTs_0136.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_2026-08-22_CI_Ori-02-Q1b1x1_043748_TTUQ1b1x1_2949840_gjrQHCHz/fd_Ori-02-Q1b1x1_2026-08-22_04-35-52_20.00sec_0.00C_LIGHTs_0136.fits
WCS_IMAGE_NAME=wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-35-52_20.00sec_0.00C_LIGHTs_0136.fits
WCS-calibrated image found: wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-35-52_20.00sec_0.00C_LIGHTs_0136.fits
Checking if the catalog wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-35-52_20.00sec_0.00C_LIGHTs_0136.fits.wcscat corresponding to the image wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-35-52_20.00sec_0.00C_LIGHTs_0136.fits alredy exist and is non-empty...
Catalog wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-35-52_20.00sec_0.00C_LIGHTs_0136.fits.wcscat corresponding to the image wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-35-52_20.00sec_0.00C_LIGHTs_0136.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-35-52_20.00sec_0.00C_LIGHTs_0136.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Ori-02-Q1b1x1_043748_TTUQ1b1x1_2949840_gjrQHCHz/fd_Ori-02-Q1b1x1_2026-08-22_04-35-52_20.00sec_0.00C_LIGHTs_0136.fits
WCS catalog name: wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-35-52_20.00sec_0.00C_LIGHTs_0136.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=113, bad_region=0, passed=3301
Got 3301 stars (including 3187 good ones) from the SExtractor catalog wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-35-52_20.00sec_0.00C_LIGHTs_0136.fits.wcscat
util/solve_plate_with_UCAC5 got 3301 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 945.0'
Seting catalog search parameters based on the expected field of view 945.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013125 (47.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010500 (37.8 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 491 to 549 (Dec 8.3 to 19.5)
Done reading UCAC5 zone files...
Matched 3040 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2976 matched stars entering correct_measured_positions(), 2978 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2976 matched stars entering correct_measured_positions(), 3301 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 491 to 549 (Dec 8.3 to 19.5)
Done reading UCAC5 zone files...
Matched 3042 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 2978 matched stars entering correct_measured_positions(), 3301 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Accuracy estimation diagnostic: 2978 matched stars entering correct_measured_positions(), 3301 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Excluding outliers - 2978 stars left (next iteration limit 3273)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=2978 robust_rms=7.132 arcsec worst_quadrant_rms=14.734 arcsec
SIP_REFIT: SIP order 3 trial: matched=2978 robust_rms=0.617 arcsec worst_quadrant_rms=0.750 arcsec
SIP_REFIT: SIP order 5 trial: matched=2978 robust_rms=0.496 arcsec worst_quadrant_rms=0.629 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=2978 robust_rms_before=1.462 arcsec robust_rms_before_corrected=0.625 arcsec robust_rms_after=0.496 arcsec worst_quadrant_rms_before=0.750 worst_quadrant_rms_after=0.629
verification OK: wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-35-52_20.00sec_0.00C_LIGHTs_0136.fits
verification OK: wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-35-52_20.00sec_0.00C_LIGHTs_0136.fits
Image size: 945.3'x626.9' 15.8(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 06:13:23.826 +14:00:50.43 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 3301 stars ###
'wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-35-52_20.00sec_0.00C_LIGHTs_0136.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-08-22_CI_Ori-02-Q1b1x1_043748_TTUQ1b1x1_2949840_gjrQHCHz/correct_sextractor_wcs_catalog_usingxy2sky3064962.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 5, robust RMS 1.462 -> 0.496 arcsec)
WCS_QUALITY_DIAG: file=fd_Ori-02-Q1b1x1_2026-08-22_04-35-52_20.00sec_0.00C_LIGHTs_0136.fits N_match=2978 sigma_overall_arcsec=0.520 sigma_q1_arcsec=0.467 sigma_q2_arcsec=0.679 sigma_q3_arcsec=0.430 sigma_q4_arcsec=0.553 n_q1=682 n_q2=809 n_q3=629 n_q4=858 worst_quadrant_to_overall_ratio=1.304
The image catalog is written to wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-35-52_20.00sec_0.00C_LIGHTs_0136.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-35-52_20.00sec_0.00C_LIGHTs_0136.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Ori-02-Q1b1x1_043748_TTUQ1b1x1_2949840_gjrQHCHz/fd_Ori-02-Q1b1x1_2026-08-22_04-35-52_20.00sec_0.00C_LIGHTs_0136.fits -region wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-35-52_20.00sec_0.00C_LIGHTs_0136.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-35-52_20.00sec_0.00C_LIGHTs_0136.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.9CoxaOzZpt (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_2026-08-22_CI_Ori-02-Q1b1x1_043748_TTUQ1b1x1_2949840_gjrQHCHz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Ori-02-Q1b1x1_043748_TTUQ1b1x1_2949840_gjrQHCHz/fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Ori-02-Q1b1x1_043748_TTUQ1b1x1_2949840_gjrQHCHz/fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Ori-02-Q1b1x1_043748_TTUQ1b1x1_2949840_gjrQHCHz/fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Ori-02-Q1b1x1_043748_TTUQ1b1x1_2949840_gjrQHCHz/fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Ori-02-Q1b1x1_043748_TTUQ1b1x1_2949840_gjrQHCHz/fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137.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_2026-08-22_CI_Ori-02-Q1b1x1_043748_TTUQ1b1x1_2949840_gjrQHCHz/fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137.fits
WCS_IMAGE_NAME=wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137.fits
WCS-calibrated image found: wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137.fits
Checking if the catalog wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137.fits.wcscat corresponding to the image wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137.fits alredy exist and is non-empty...
Catalog wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137.fits.wcscat corresponding to the image wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Ori-02-Q1b1x1_043748_TTUQ1b1x1_2949840_gjrQHCHz/fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137.fits
WCS catalog name: wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=118, bad_region=0, passed=3433
Got 3433 stars (including 3312 good ones) from the SExtractor catalog wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137.fits.wcscat
util/solve_plate_with_UCAC5 got 3433 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 944.8'
Seting catalog search parameters based on the expected field of view 944.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013122 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010498 (37.8 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 491 to 549 (Dec 8.3 to 19.5)
Done reading UCAC5 zone files...
Matched 3163 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3099 matched stars entering correct_measured_positions(), 3101 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3099 matched stars entering correct_measured_positions(), 3433 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 491 to 549 (Dec 8.3 to 19.5)
Done reading UCAC5 zone files...
Matched 3166 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 3100 matched stars entering correct_measured_positions(), 3433 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Accuracy estimation diagnostic: 3100 matched stars entering correct_measured_positions(), 3433 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Excluding outliers - 3100 stars left (next iteration limit 3408)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=3100 robust_rms=7.455 arcsec worst_quadrant_rms=14.810 arcsec
SIP_REFIT: SIP order 3 trial: matched=3100 robust_rms=0.582 arcsec worst_quadrant_rms=0.684 arcsec
SIP_REFIT: SIP order 5 trial: matched=3100 robust_rms=0.502 arcsec worst_quadrant_rms=0.630 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=3100 robust_rms_before=1.410 arcsec robust_rms_before_corrected=0.605 arcsec robust_rms_after=0.502 arcsec worst_quadrant_rms_before=0.769 worst_quadrant_rms_after=0.630
verification OK: wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137.fits
verification OK: wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137.fits
Image size: 945.1'x626.9' 15.8(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 06:13:21.262 +14:00:12.46 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 3433 stars ###
'wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-08-22_CI_Ori-02-Q1b1x1_043748_TTUQ1b1x1_2949840_gjrQHCHz/correct_sextractor_wcs_catalog_usingxy2sky3064960.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 5, robust RMS 1.410 -> 0.502 arcsec)
WCS_QUALITY_DIAG: file=fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137.fits N_match=3100 sigma_overall_arcsec=0.522 sigma_q1_arcsec=0.464 sigma_q2_arcsec=0.664 sigma_q3_arcsec=0.413 sigma_q4_arcsec=0.545 n_q1=719 n_q2=832 n_q3=655 n_q4=894 worst_quadrant_to_overall_ratio=1.272
The image catalog is written to wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Ori-02-Q1b1x1_043748_TTUQ1b1x1_2949840_gjrQHCHz/fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137.fits -region wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Saving the final (post-refit) wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits to local_wcs_cache/
'wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits' -> 'local_wcs_cache/wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits'
Saving the final (post-refit) wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits to local_wcs_cache/
'wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits' -> 'local_wcs_cache/wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits'
Saving the final (post-refit) wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-35-52_20.00sec_0.00C_LIGHTs_0136.fits to local_wcs_cache/
'wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-35-52_20.00sec_0.00C_LIGHTs_0136.fits' -> 'local_wcs_cache/wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-35-52_20.00sec_0.00C_LIGHTs_0136.fits'
Saving the final (post-refit) wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137.fits to local_wcs_cache/
'wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137.fits' -> 'local_wcs_cache/wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits sigma_overall=0.380 worst_q_ratio=1.257
ref2=Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits sigma_overall=0.407 worst_q_ratio=1.226
new1=fd_Ori-02-Q1b1x1_2026-08-22_04-35-52_20.00sec_0.00C_LIGHTs_0136.fits sigma_overall=0.520 worst_q_ratio=1.304
new2=fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137.fits sigma_overall=0.522 worst_q_ratio=1.272
reference average sigma_overall=0.3935 worst_q_ratio=1.2415
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386_astrometric_residuals.png (4783 matched stars from wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.37 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042_astrometric_residuals.png (4787 matched stars from wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.38 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-35-52_20.00sec_0.00C_LIGHTs_0136_astrometric_residuals.png (2978 matched stars from wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-35-52_20.00sec_0.00C_LIGHTs_0136.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.41 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137_astrometric_residuals.png (3100 matched stars from wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.41 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-35-52_20.00sec_0.00C_LIGHTs_0136.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-35-52_20.00sec_0.00C_LIGHTs_0136.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Ori-02-Q1b1x1_043748_TTUQ1b1x1_2949840_gjrQHCHz/wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-35-52_20.00sec_0.00C_LIGHTs_0136.fits'
Saving fully-calibrated image wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Ori-02-Q1b1x1_043748_TTUQ1b1x1_2949840_gjrQHCHz/wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137.fits'
Preparing the HTML report for the field Ori-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Ori-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Ori-02-Q1b1x1_043748_TTUQ1b1x1_2949840_gjrQHCHz/fd_Ori-02-Q1b1x1_2026-08-22_04-35-52_20.00sec_0.00C_LIGHTs_0136.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Ori-02-Q1b1x1_043748_TTUQ1b1x1_2949840_gjrQHCHz/fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137.fits
SExtractor catalog cache: saved Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.cat to cache
SExtractor catalog cache: saved Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Ori-02-Q1b1x1_043748_TTUQ1b1x1_2949840_gjrQHCHz/fd_Ori-02-Q1b1x1_2026-08-22_04-35-52_20.00sec_0.00C_LIGHTs_0136.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Ori-02-Q1b1x1_043748_TTUQ1b1x1_2949840_gjrQHCHz/fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
Creating symlink local_wcs_cache/wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
Creating symlink local_wcs_cache/wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-35-52_20.00sec_0.00C_LIGHTs_0136.fits
Creating symlink local_wcs_cache/wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137.fits
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_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits exists and is non-empty
wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits exists and is non-empty
wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-35-52_20.00sec_0.00C_LIGHTs_0136.fits exists and is non-empty
wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits (1st reference image)
verification OK: wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
Image size: 941.6'x627.1' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 06:13:27.287 +13:59:26.52 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-35-52_20.00sec_0.00C_LIGHTs_0136.fits (1st new image)
verification OK: wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-35-52_20.00sec_0.00C_LIGHTs_0136.fits
Image size: 945.3'x626.9' 15.8(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 06:13:23.826 +14:00:50.43 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 06:13:27.287 +13:59:26.52
Second-epoch image center 06:13:23.826 +14:00:50.43
Angular distance between the image centers 0.0272 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137.fits (2nd new image)
verification OK: wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137.fits
Image size: 945.1'x626.9' 15.8(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 06:13:21.262 +14:00:12.46 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 06:13:27.287 +13:59:26.52
Second-epoch image center 06:13:21.262 +14:00:12.46
Angular distance between the image centers 0.0275 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 06:13:23.826 +14:00:50.43
Second-epoch second image center 06:13:21.262 +14:00:12.46
Angular distance between the image centers 0.01479 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits &> /tmp/tmp.Rc1B7rLJ4E
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits &> /tmp/tmp.kTY4e3Krpw
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Ori-02-Q1b1x1_043748_TTUQ1b1x1_2949840_gjrQHCHz/fd_Ori-02-Q1b1x1_2026-08-22_04-35-52_20.00sec_0.00C_LIGHTs_0136.fits &> /tmp/tmp.GuzKt0gH3Q
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Ori-02-Q1b1x1_043748_TTUQ1b1x1_2949840_gjrQHCHz/fd_Ori-02-Q1b1x1_2026-08-22_04-35-52_20.00sec_0.00C_LIGHTs_0136.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Ori-02-Q1b1x1_043748_TTUQ1b1x1_2949840_gjrQHCHz/fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137.fits &> /tmp/tmp.M70nFgFZpr
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Ori-02-Q1b1x1_043748_TTUQ1b1x1_2949840_gjrQHCHz/fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137.fits
Calibrating the magnitude scale
Found non-empty wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.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_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits and wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits and wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.wcscat
Found non-empty wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits and wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.wcscat
The reference image (wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits) and catalog (wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.wcscat) found
'wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.wcscat' -> 'wcsmag.cat'
Read 229058 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 85.0776 to 101.6828 deg, Dec +8.6174 to +19.2791 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 85.0776 to 101.6828 deg, Dec 8.6174 to 19.2791 deg
Loaded 17847 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): 9852 out of 15551 total matches.
Matched with Tycho-2 15551 out of 229058 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.805100
a=0.000000 b=1.000000 c=22.805100
From vast_summary.log: estimated ref. image limiting mag.: -7.41
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.40
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.40
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 229058 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 85.0776 to 101.6828 deg, Dec +8.6174 to +19.2791 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 85.0776 to 101.6828 deg, Dec 8.6174 to 19.2791 deg
Loaded 17847 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): 9852 out of 15551 total matches.
Matched with Tycho-2 15551 out of 229058 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
Forced-photometry filter: calibrated wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits -> calib.txt_param_ref_wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits (aperture=4.6)
Read 230307 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 84.9070 to 101.4968 deg, Dec +8.4421 to +19.3422 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 84.9070 to 101.4968 deg, Dec 8.4421 to 19.3422 deg
Loaded 18095 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): 10167 out of 15481 total matches.
Matched with Tycho-2 15481 out of 230307 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
Forced-photometry filter: calibrated wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits -> calib.txt_param_ref_wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits (aperture=4.5)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 205 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
1.9 pix Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
1.9 pix Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
2.5 pix fd_Ori-02-Q1b1x1_2026-08-22_04-35-52_20.00sec_0.00C_LIGHTs_0136.fits
2.5 pix fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137.fits
Limiting magnitude estimates:
15.4 mag. Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
15.4 mag. Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
12.4 mag. fd_Ori-02-Q1b1x1_2026-08-22_04-35-52_20.00sec_0.00C_LIGHTs_0136.fits
12.5 mag. fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137.fits
All-image limiting magnitude estimate: 12.4 (SNR ) 12.1 (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 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.Rc1B7rLJ4E (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-22_CI_Ori-02-Q1b1x1_043748_TTUQ1b1x1_2949840_gjrQHCHz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits' -> 'wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
WCS_IMAGE_NAME=wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
WCS-calibrated image found: wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
Checking if the catalog wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.wcscat corresponding to the image wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits alredy exist and is non-empty...
Catalog wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.wcscat corresponding to the image wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
WCS catalog name: wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=66, blended=37651, bad_region=12, passed=228992
Got 228992 stars (including 190970 good ones) from the SExtractor catalog wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.wcscat
util/solve_plate_with_UCAC5 got 228992 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4823 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4772 matched stars entering correct_measured_positions(), 4773 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4772 matched stars entering correct_measured_positions(), 228992 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4822 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4770 matched stars entering correct_measured_positions(), 228992 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 4770 matched stars entering correct_measured_positions(), 228992 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 4770 stars left (next iteration limit 5249)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits N_match=4770 sigma_overall_arcsec=0.379 sigma_q1_arcsec=0.454 sigma_q2_arcsec=0.379 sigma_q3_arcsec=0.340 sigma_q4_arcsec=0.325 n_q1=1096 n_q2=1242 n_q3=1241 n_q4=1191 worst_quadrant_to_overall_ratio=1.197
The image catalog is written to wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits -region wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.kTY4e3Krpw (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-22_CI_Ori-02-Q1b1x1_043748_TTUQ1b1x1_2949840_gjrQHCHz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits' -> 'wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
WCS_IMAGE_NAME=wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
WCS-calibrated image found: wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
Checking if the catalog wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits.wcscat corresponding to the image wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits alredy exist and is non-empty...
Catalog wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits.wcscat corresponding to the image wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
WCS catalog name: wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=82, blended=35229, bad_region=4, passed=230225
Got 230225 stars (including 194609 good ones) from the SExtractor catalog wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits.wcscat
util/solve_plate_with_UCAC5 got 230225 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.4 to 19.3)
Done reading UCAC5 zone files...
Matched 4832 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4781 matched stars entering correct_measured_positions(), 4781 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4781 matched stars entering correct_measured_positions(), 230225 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.4 to 19.3)
Done reading UCAC5 zone files...
Matched 4831 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4778 matched stars entering correct_measured_positions(), 230225 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 4778 matched stars entering correct_measured_positions(), 230225 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 4778 stars left (next iteration limit 5259)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits N_match=4778 sigma_overall_arcsec=0.388 sigma_q1_arcsec=0.484 sigma_q2_arcsec=0.397 sigma_q3_arcsec=0.356 sigma_q4_arcsec=0.328 n_q1=1035 n_q2=1329 n_q3=1162 n_q4=1252 worst_quadrant_to_overall_ratio=1.248
The image catalog is written to wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits -region wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.GuzKt0gH3Q (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_2026-08-22_CI_Ori-02-Q1b1x1_043748_TTUQ1b1x1_2949840_gjrQHCHz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Ori-02-Q1b1x1_043748_TTUQ1b1x1_2949840_gjrQHCHz/fd_Ori-02-Q1b1x1_2026-08-22_04-35-52_20.00sec_0.00C_LIGHTs_0136.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Ori-02-Q1b1x1_043748_TTUQ1b1x1_2949840_gjrQHCHz/fd_Ori-02-Q1b1x1_2026-08-22_04-35-52_20.00sec_0.00C_LIGHTs_0136.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Ori-02-Q1b1x1_043748_TTUQ1b1x1_2949840_gjrQHCHz/fd_Ori-02-Q1b1x1_2026-08-22_04-35-52_20.00sec_0.00C_LIGHTs_0136.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Ori-02-Q1b1x1_043748_TTUQ1b1x1_2949840_gjrQHCHz/fd_Ori-02-Q1b1x1_2026-08-22_04-35-52_20.00sec_0.00C_LIGHTs_0136.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Ori-02-Q1b1x1_043748_TTUQ1b1x1_2949840_gjrQHCHz/fd_Ori-02-Q1b1x1_2026-08-22_04-35-52_20.00sec_0.00C_LIGHTs_0136.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_2026-08-22_CI_Ori-02-Q1b1x1_043748_TTUQ1b1x1_2949840_gjrQHCHz/fd_Ori-02-Q1b1x1_2026-08-22_04-35-52_20.00sec_0.00C_LIGHTs_0136.fits
WCS_IMAGE_NAME=wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-35-52_20.00sec_0.00C_LIGHTs_0136.fits
WCS-calibrated image found: wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-35-52_20.00sec_0.00C_LIGHTs_0136.fits
Checking if the catalog wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-35-52_20.00sec_0.00C_LIGHTs_0136.fits.wcscat corresponding to the image wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-35-52_20.00sec_0.00C_LIGHTs_0136.fits alredy exist and is non-empty...
Catalog wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-35-52_20.00sec_0.00C_LIGHTs_0136.fits.wcscat corresponding to the image wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-35-52_20.00sec_0.00C_LIGHTs_0136.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-35-52_20.00sec_0.00C_LIGHTs_0136.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Ori-02-Q1b1x1_043748_TTUQ1b1x1_2949840_gjrQHCHz/fd_Ori-02-Q1b1x1_2026-08-22_04-35-52_20.00sec_0.00C_LIGHTs_0136.fits
WCS catalog name: wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-35-52_20.00sec_0.00C_LIGHTs_0136.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=747, bad_region=17, passed=29604
Got 29604 stars (including 28794 good ones) from the SExtractor catalog wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-35-52_20.00sec_0.00C_LIGHTs_0136.fits.wcscat
util/solve_plate_with_UCAC5 got 29604 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 945.3'
Seting catalog search parameters based on the expected field of view 945.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013129 (47.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010503 (37.8 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 491 to 549 (Dec 8.2 to 19.5)
Done reading UCAC5 zone files...
Matched 4820 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4728 matched stars entering correct_measured_positions(), 4728 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4728 matched stars entering correct_measured_positions(), 29604 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 491 to 549 (Dec 8.2 to 19.5)
Done reading UCAC5 zone files...
Matched 4820 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4727 matched stars entering correct_measured_positions(), 29604 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Accuracy estimation diagnostic: 4727 matched stars entering correct_measured_positions(), 29604 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Excluding outliers - 4727 stars left (next iteration limit 5200)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-35-52_20.00sec_0.00C_LIGHTs_0136.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4727 robust_rms=7.502 arcsec worst_quadrant_rms=13.845 arcsec
SIP_REFIT: SIP order 3 trial: matched=4727 robust_rms=0.624 arcsec worst_quadrant_rms=0.755 arcsec
SIP_REFIT: SIP order 5 trial: matched=4727 robust_rms=0.514 arcsec worst_quadrant_rms=0.659 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4727 robust_rms_before=0.518 arcsec robust_rms_before_corrected=0.569 arcsec robust_rms_after=0.514 arcsec worst_quadrant_rms_before=0.654 worst_quadrant_rms_after=0.659
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.654 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Ori-02-Q1b1x1_2026-08-22_04-35-52_20.00sec_0.00C_LIGHTs_0136.fits N_match=4727 sigma_overall_arcsec=0.571 sigma_q1_arcsec=0.577 sigma_q2_arcsec=0.674 sigma_q3_arcsec=0.483 sigma_q4_arcsec=0.547 n_q1=1080 n_q2=1188 n_q3=1094 n_q4=1365 worst_quadrant_to_overall_ratio=1.179
The image catalog is written to wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-35-52_20.00sec_0.00C_LIGHTs_0136.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-35-52_20.00sec_0.00C_LIGHTs_0136.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Ori-02-Q1b1x1_043748_TTUQ1b1x1_2949840_gjrQHCHz/fd_Ori-02-Q1b1x1_2026-08-22_04-35-52_20.00sec_0.00C_LIGHTs_0136.fits -region wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-35-52_20.00sec_0.00C_LIGHTs_0136.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-35-52_20.00sec_0.00C_LIGHTs_0136.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.M70nFgFZpr (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_2026-08-22_CI_Ori-02-Q1b1x1_043748_TTUQ1b1x1_2949840_gjrQHCHz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Ori-02-Q1b1x1_043748_TTUQ1b1x1_2949840_gjrQHCHz/fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Ori-02-Q1b1x1_043748_TTUQ1b1x1_2949840_gjrQHCHz/fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Ori-02-Q1b1x1_043748_TTUQ1b1x1_2949840_gjrQHCHz/fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Ori-02-Q1b1x1_043748_TTUQ1b1x1_2949840_gjrQHCHz/fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Ori-02-Q1b1x1_043748_TTUQ1b1x1_2949840_gjrQHCHz/fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137.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_2026-08-22_CI_Ori-02-Q1b1x1_043748_TTUQ1b1x1_2949840_gjrQHCHz/fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137.fits
WCS_IMAGE_NAME=wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137.fits
WCS-calibrated image found: wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137.fits
Checking if the catalog wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137.fits.wcscat corresponding to the image wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137.fits alredy exist and is non-empty...
Catalog wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137.fits.wcscat corresponding to the image wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Ori-02-Q1b1x1_043748_TTUQ1b1x1_2949840_gjrQHCHz/fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137.fits
WCS catalog name: wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=830, bad_region=19, passed=31054
Got 31054 stars (including 30166 good ones) from the SExtractor catalog wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137.fits.wcscat
util/solve_plate_with_UCAC5 got 31054 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 945.1'
Seting catalog search parameters based on the expected field of view 945.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013126 (47.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010501 (37.8 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 491 to 549 (Dec 8.2 to 19.5)
Done reading UCAC5 zone files...
Matched 4815 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4721 matched stars entering correct_measured_positions(), 4722 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4720 matched stars entering correct_measured_positions(), 31054 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 491 to 549 (Dec 8.2 to 19.5)
Done reading UCAC5 zone files...
Matched 4817 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4724 matched stars entering correct_measured_positions(), 31054 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Accuracy estimation diagnostic: 4724 matched stars entering correct_measured_positions(), 31054 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Excluding outliers - 4724 stars left (next iteration limit 5192)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4724 robust_rms=7.740 arcsec worst_quadrant_rms=14.169 arcsec
SIP_REFIT: SIP order 3 trial: matched=4724 robust_rms=0.597 arcsec worst_quadrant_rms=0.708 arcsec
SIP_REFIT: SIP order 5 trial: matched=4724 robust_rms=0.525 arcsec worst_quadrant_rms=0.646 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4724 robust_rms_before=0.528 arcsec robust_rms_before_corrected=0.568 arcsec robust_rms_after=0.525 arcsec worst_quadrant_rms_before=0.648 worst_quadrant_rms_after=0.646
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.648 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137.fits N_match=4724 sigma_overall_arcsec=0.559 sigma_q1_arcsec=0.525 sigma_q2_arcsec=0.678 sigma_q3_arcsec=0.490 sigma_q4_arcsec=0.541 n_q1=1071 n_q2=1191 n_q3=1117 n_q4=1345 worst_quadrant_to_overall_ratio=1.211
The image catalog is written to wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Ori-02-Q1b1x1_043748_TTUQ1b1x1_2949840_gjrQHCHz/fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137.fits -region wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-35-52_20.00sec_0.00C_LIGHTs_0136.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_2026-08-22_CI_Ori-02-Q1b1x1_043748_TTUQ1b1x1_2949840_gjrQHCHz/wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-35-52_20.00sec_0.00C_LIGHTs_0136.fits
Saving fully-calibrated image wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137.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_2026-08-22_CI_Ori-02-Q1b1x1_043748_TTUQ1b1x1_2949840_gjrQHCHz/wcs_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137.fits
Preparing the HTML report for the field Ori-02-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:12:44.63 +15:29:42.9: 12.27 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:38:07.63 +08:39:31.7: 99.00 +/- 99.00 edge
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:43:14.39 +09:21:54.0: 9.77 +/- 0.00 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:41:32.87 +09:19:03.3: 9.73 +/- 0.00 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:42:15.91 +09:32:40.8: 9.30 +/- 0.00 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:43:18.84 +08:44:48.4: 9.59 +/- 0.00 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:38:07.63 +08:39:31.7: 99.00 +/- 99.00 edge
Forced photometry filter REJECTED candidate at 06:38:07.63 +08:39:31.7: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:43:18.84 +08:44:48.4: 99.00 +/- 99.00 edge
Forced photometry filter REJECTED candidate at 06:43:18.84 +08:44:48.4: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:42:30.80 +09:13:52.9: 10.28 +/- 0.00 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:43:29.76 +08:48:23.8: 9.88 +/- 0.00 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:41:22.34 +09:07:36.7: 10.12 +/- 0.00 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:42:34.66 +08:58:31.1: 10.15 +/- 0.00 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:43:29.76 +08:48:23.8: 99.00 +/- 99.00 edge
Forced photometry filter REJECTED candidate at 06:43:29.76 +08:48:23.8: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:12:44.63 +15:29:42.9: 12.32 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:41:32.87 +09:19:03.3: 9.69 +/- 0.00 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:43:14.39 +09:21:54.0: 9.71 +/- 0.00 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:42:15.91 +09:32:40.8: 9.23 +/- 0.00 detection
Forced photometry reference-image weighted average: 12.30 +/- 0.01
Forced photometry reference-image weighted average: 9.71 +/- 0.00
Forced photometry filter REJECTED candidate at 06:12:44.63 +15:29:42.9: ref_mag=12.30 +/- 0.01 new_mean_mag=12.3033 delta=-0.01 (need > 0.90)
Forced photometry reference-image weighted average: 9.74 +/- 0.00
Forced photometry reference-image weighted average: 9.26 +/- 0.00
Forced photometry filter REJECTED candidate at 06:41:32.87 +09:19:03.3: ref_mag=9.71 +/- 0.00 new_mean_mag=10.5007 delta=-0.79 (need > 0.90)
Forced photometry filter REJECTED candidate at 06:43:14.39 +09:21:54.0: ref_mag=9.74 +/- 0.00 new_mean_mag=10.2499 delta=-0.51 (need > 0.90)
Forced photometry filter REJECTED candidate at 06:42:15.91 +09:32:40.8: ref_mag=9.26 +/- 0.00 new_mean_mag=9.9980 delta=-0.74 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:42:34.66 +08:58:31.1: 10.07 +/- 0.00 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:41:22.34 +09:07:36.7: 10.07 +/- 0.00 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:42:30.80 +09:13:52.9: 10.23 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.11 +/- 0.00
Forced photometry filter REJECTED candidate at 06:42:34.66 +08:58:31.1: ref_mag=10.11 +/- 0.00 new_mean_mag=10.6834 delta=-0.57 (need > 0.90)
Forced photometry reference-image weighted average: 10.10 +/- 0.00
Forced photometry reference-image weighted average: 10.26 +/- 0.00
Forced photometry filter REJECTED candidate at 06:41:22.34 +09:07:36.7: ref_mag=10.10 +/- 0.00 new_mean_mag=10.7812 delta=-0.68 (need > 0.90)
Forced photometry filter REJECTED candidate at 06:42:30.80 +09:13:52.9: ref_mag=10.26 +/- 0.00 new_mean_mag=10.7831 delta=-0.53 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:43:21.87 +09:12:07.5: 10.58 +/- 0.00 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:43:06.61 +09:04:07.4: 10.71 +/- 0.00 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:42:44.25 +08:39:28.1: 99.00 +/- 99.00 edge
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:43:21.87 +09:12:07.5: 10.52 +/- 0.00 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:42:14.52 +08:44:27.5: 10.42 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.55 +/- 0.00
Forced photometry filter REJECTED candidate at 06:43:21.87 +09:12:07.5: ref_mag=10.55 +/- 0.00 new_mean_mag=10.7177 delta=-0.17 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:42:44.25 +08:39:28.1: 99.00 +/- 99.00 edge
Forced photometry filter REJECTED candidate at 06:42:44.25 +08:39:28.1: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:42:14.52 +08:44:27.5: 99.00 +/- 99.00 edge
Forced photometry filter REJECTED candidate at 06:42:14.52 +08:44:27.5: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:41:11.28 +09:11:14.1: 10.35 +/- 0.00 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:41:45.39 +08:41:21.9: 10.82 +/- 0.00 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:39:54.18 +08:41:14.1: 10.71 +/- 0.00 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:43:40.29 +09:14:25.9: 10.83 +/- 0.00 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:40:47.30 +08:52:01.7: 10.96 +/- 0.00 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:41:45.39 +08:41:21.9: 99.00 +/- 99.00 edge
Forced photometry filter REJECTED candidate at 06:41:45.39 +08:41:21.9: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:39:54.18 +08:41:14.1: 99.00 +/- 99.00 edge
Forced photometry filter REJECTED candidate at 06:39:54.18 +08:41:14.1: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:43:06.61 +09:04:07.4: 10.64 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.68 +/- 0.00
Forced photometry filter REJECTED candidate at 06:43:06.61 +09:04:07.4: ref_mag=10.68 +/- 0.00 new_mean_mag=10.7352 delta=-0.06 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:43:31.16 +08:49:07.1: 10.99 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:43:31.16 +08:49:07.1: 99.00 +/- 99.00 edge
Forced photometry filter REJECTED candidate at 06:43:31.16 +08:49:07.1: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:41:11.28 +09:11:14.1: 10.30 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.33 +/- 0.00
Forced photometry filter REJECTED candidate at 06:41:11.28 +09:11:14.1: ref_mag=10.33 +/- 0.00 new_mean_mag=11.1177 delta=-0.79 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:43:40.29 +09:14:25.9: 10.77 +/- 0.00 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:40:47.30 +08:52:01.7: 99.00 +/- 99.00 edge
Forced photometry filter REJECTED candidate at 06:40:47.30 +08:52:01.7: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry reference-image weighted average: 10.80 +/- 0.00
Forced photometry filter REJECTED candidate at 06:43:40.29 +09:14:25.9: ref_mag=10.80 +/- 0.00 new_mean_mag=11.3122 delta=-0.51 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:43:11.59 +09:59:52.3: 11.44 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:42:37.73 +09:00:30.0: 11.31 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:41:07.24 +09:02:51.8: 11.69 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:43:35.71 +09:54:12.0: 11.92 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:43:35.32 +09:00:57.9: 11.16 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:43:11.59 +09:59:52.3: 11.33 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.38 +/- 0.00
Forced photometry filter REJECTED candidate at 06:43:11.59 +09:59:52.3: ref_mag=11.38 +/- 0.00 new_mean_mag=11.4087 delta=-0.03 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:33:14.75 +08:40:44.9: 99.00 +/- 99.00 edge
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:33:14.75 +08:40:44.9: 99.00 +/- 99.00 edge
Forced photometry filter REJECTED candidate at 06:33:14.75 +08:40:44.9: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:42:26.12 +08:54:10.5: 11.27 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:42:37.73 +09:00:30.0: 11.26 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.29 +/- 0.00
Forced photometry filter REJECTED candidate at 06:42:37.73 +09:00:30.0: ref_mag=11.29 +/- 0.00 new_mean_mag=11.5702 delta=-0.28 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:41:07.24 +09:02:51.8: 11.65 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.67 +/- 0.01
Forced photometry filter REJECTED candidate at 06:41:07.24 +09:02:51.8: ref_mag=11.67 +/- 0.01 new_mean_mag=11.6035 delta=0.06 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:43:35.71 +09:54:12.0: 11.83 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:43:35.32 +09:00:57.9: 11.10 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.88 +/- 0.01
Forced photometry reference-image weighted average: 11.13 +/- 0.00
Forced photometry filter REJECTED candidate at 06:43:35.71 +09:54:12.0: ref_mag=11.88 +/- 0.01 new_mean_mag=11.7498 delta=0.13 (need > 0.90)
Forced photometry filter REJECTED candidate at 06:43:35.32 +09:00:57.9: ref_mag=11.13 +/- 0.00 new_mean_mag=11.5984 delta=-0.47 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:43:25.77 +09:29:56.5: 11.75 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:19:23.89 +12:58:05.1: 12.67 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:43:25.05 +08:48:41.3: 11.47 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:43:25.05 +08:48:41.3: 99.00 +/- 99.00 edge
Forced photometry filter REJECTED candidate at 06:43:25.05 +08:48:41.3: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:42:26.12 +08:54:10.5: 11.20 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.24 +/- 0.00
Forced photometry filter REJECTED candidate at 06:42:26.12 +08:54:10.5: ref_mag=11.24 +/- 0.00 new_mean_mag=11.6350 delta=-0.40 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:43:25.77 +09:29:56.5: 11.71 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:19:23.89 +12:58:05.1: 12.67 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.73 +/- 0.01
Forced photometry reference-image weighted average: 12.67 +/- 0.02
Forced photometry filter REJECTED candidate at 06:43:25.77 +09:29:56.5: ref_mag=11.73 +/- 0.01 new_mean_mag=11.8691 delta=-0.14 (need > 0.90)
Forced photometry filter REJECTED candidate at 06:19:23.89 +12:58:05.1: ref_mag=12.67 +/- 0.02 new_mean_mag=11.8186 delta=0.85 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:43:16.80 +09:10:28.3: 11.54 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:25:08.92 +18:21:40.2: 12.18 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:43:16.80 +09:10:28.3: 11.45 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.50 +/- 0.01
Forced photometry filter REJECTED candidate at 06:43:16.80 +09:10:28.3: ref_mag=11.50 +/- 0.01 new_mean_mag=11.8202 delta=-0.33 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:24:04.69 +16:19:39.7: 12.41 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:26:21.49 +15:58:57.2: 12.38 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:18:03.95 +13:30:16.6: 12.54 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 05:58:59.97 +09:16:46.1: 12.73 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:25:08.92 +18:21:40.2: 12.20 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.19 +/- 0.01
Forced photometry filter REJECTED candidate at 06:25:08.92 +18:21:40.2: ref_mag=12.19 +/- 0.01 new_mean_mag=11.7530 delta=0.44 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:20:10.05 +13:20:58.6: 12.79 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:21:10.22 +12:58:17.9: 12.80 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:24:04.69 +16:19:39.7: 12.25 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.31 +/- 0.01
Forced photometry filter REJECTED candidate at 06:24:04.69 +16:19:39.7: ref_mag=12.31 +/- 0.01 new_mean_mag=11.4350 delta=0.88 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:26:21.49 +15:58:57.2: 11.98 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.11 +/- 0.01
Forced photometry filter KEPT candidate at 06:26:21.49 +15:58:57.2: ref_mag=12.11 +/- 0.01 new_mean_mag=11.1716 delta=0.94 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:18:03.95 +13:30:16.6: 12.56 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.55 +/- 0.01
Forced photometry filter KEPT candidate at 06:18:03.95 +13:30:16.6: ref_mag=12.55 +/- 0.01 new_mean_mag=11.5870 delta=0.97 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 05:58:59.97 +09:16:46.1: 12.81 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.77 +/- 0.01
Forced photometry filter KEPT candidate at 05:58:59.97 +09:16:46.1: ref_mag=12.77 +/- 0.01 new_mean_mag=11.8421 delta=0.93 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:24:40.19 +16:44:46.2: 12.77 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:20:56.55 +15:15:27.3: 12.86 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:20:10.05 +13:20:58.6: 12.80 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.80 +/- 0.01
Forced photometry filter KEPT candidate at 06:20:10.05 +13:20:58.6: ref_mag=12.80 +/- 0.01 new_mean_mag=11.8701 delta=0.93 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:21:10.22 +12:58:17.9: 12.84 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.82 +/- 0.01
Forced photometry filter KEPT candidate at 06:21:10.22 +12:58:17.9: ref_mag=12.82 +/- 0.01 new_mean_mag=11.9096 delta=0.91 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:20:56.55 +15:15:27.3: 12.85 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:24:40.19 +16:44:46.2: 12.79 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:22:27.61 +16:05:21.6: 12.86 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.78 +/- 0.02
Forced photometry reference-image weighted average: 12.85 +/- 0.01
Forced photometry filter KEPT candidate at 06:20:56.55 +15:15:27.3: ref_mag=12.85 +/- 0.01 new_mean_mag=11.8931 delta=0.96 (need > 0.90)
Forced photometry filter REJECTED candidate at 06:24:40.19 +16:44:46.2: ref_mag=12.78 +/- 0.02 new_mean_mag=11.9115 delta=0.87 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:24:56.21 +14:49:23.4: 12.87 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:22:27.61 +16:05:21.6: 12.84 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.85 +/- 0.01
Forced photometry filter KEPT candidate at 06:22:27.61 +16:05:21.6: ref_mag=12.85 +/- 0.01 new_mean_mag=11.8180 delta=1.03 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:12:25.54 +10:30:59.9: 12.89 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:24:56.21 +14:49:23.4: 12.80 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.83 +/- 0.01
Forced photometry filter KEPT candidate at 06:24:56.21 +14:49:23.4: ref_mag=12.83 +/- 0.01 new_mean_mag=11.9272 delta=0.91 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:12:25.54 +10:30:59.9: 12.85 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.87 +/- 0.02
Forced photometry filter KEPT candidate at 06:12:25.54 +10:30:59.9: ref_mag=12.87 +/- 0.02 new_mean_mag=11.8332 delta=1.03 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:19:44.97 +14:56:40.9: 12.92 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:19:44.97 +14:56:40.9: 12.89 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.91 +/- 0.01
Forced photometry filter KEPT candidate at 06:19:44.97 +14:56:40.9: ref_mag=12.91 +/- 0.01 new_mean_mag=11.8984 delta=1.01 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:16:58.38 +12:25:08.5: 12.93 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:18:53.84 +14:04:19.0: 12.73 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:16:58.38 +12:25:08.5: 12.94 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.93 +/- 0.01
Forced photometry filter KEPT candidate at 06:16:58.38 +12:25:08.5: ref_mag=12.93 +/- 0.01 new_mean_mag=11.8172 delta=1.12 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:18:53.84 +14:04:19.0: 12.68 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.70 +/- 0.01
Forced photometry filter REJECTED candidate at 06:18:53.84 +14:04:19.0: ref_mag=12.70 +/- 0.01 new_mean_mag=11.9214 delta=0.78 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:24:38.86 +15:35:16.9: 12.98 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:15:15.56 +12:02:24.1: 13.04 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:17:36.16 +13:06:06.3: 13.07 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:24:38.86 +15:35:16.9: 12.94 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.96 +/- 0.02
Forced photometry filter KEPT candidate at 06:24:38.86 +15:35:16.9: ref_mag=12.96 +/- 0.02 new_mean_mag=11.9892 delta=0.97 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:15:15.56 +12:02:24.1: 13.05 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.05 +/- 0.01
Forced photometry filter KEPT candidate at 06:15:15.56 +12:02:24.1: ref_mag=13.05 +/- 0.01 new_mean_mag=12.0696 delta=0.98 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:17:36.16 +13:06:06.3: 13.09 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.02
Forced photometry filter KEPT candidate at 06:17:36.16 +13:06:06.3: ref_mag=13.08 +/- 0.02 new_mean_mag=12.0506 delta=1.03 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:21:34.28 +14:08:35.2: 13.19 +/- 0.03 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:21:34.28 +14:08:35.2: 13.20 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.02
Forced photometry filter KEPT candidate at 06:21:34.28 +14:08:35.2: ref_mag=13.19 +/- 0.02 new_mean_mag=12.1535 delta=1.04 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:16:33.61 +12:04:50.5: 13.36 +/- 0.03 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:16:33.61 +12:04:50.5: 13.31 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.33 +/- 0.02
Forced photometry filter KEPT candidate at 06:16:33.61 +12:04:50.5: ref_mag=13.33 +/- 0.02 new_mean_mag=12.1627 delta=1.17 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:16:52.29 +12:39:03.5: 13.47 +/- 0.03 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:16:52.29 +12:39:03.5: 13.36 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.42 +/- 0.02
Forced photometry filter KEPT candidate at 06:16:52.29 +12:39:03.5: ref_mag=13.42 +/- 0.02 new_mean_mag=12.1774 delta=1.24 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:12:38.91 +10:38:15.1: 13.29 +/- 0.03 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:12:38.91 +10:38:15.1: 13.28 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.02
Forced photometry filter KEPT candidate at 06:12:38.91 +10:38:15.1: ref_mag=13.28 +/- 0.02 new_mean_mag=12.0684 delta=1.21 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:23:40.76 +15:24:49.4: 13.24 +/- 0.03 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:23:40.76 +15:24:49.4: 13.17 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.20 +/- 0.02
Forced photometry filter KEPT candidate at 06:23:40.76 +15:24:49.4: ref_mag=13.20 +/- 0.02 new_mean_mag=12.1641 delta=1.04 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:17:17.52 +12:47:01.7: 13.22 +/- 0.03 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:17:17.52 +12:47:01.7: 13.16 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.02
Forced photometry filter KEPT candidate at 06:17:17.52 +12:47:01.7: ref_mag=13.19 +/- 0.02 new_mean_mag=12.0806 delta=1.11 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:15:19.32 +11:42:51.1: 13.24 +/- 0.03 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:15:19.32 +11:42:51.1: 13.21 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.23 +/- 0.02
Forced photometry filter KEPT candidate at 06:15:19.32 +11:42:51.1: ref_mag=13.23 +/- 0.02 new_mean_mag=11.9953 delta=1.23 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:18:54.34 +12:57:04.2: 13.18 +/- 0.03 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:18:54.34 +12:57:04.2: 13.14 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.16 +/- 0.02
Forced photometry filter KEPT candidate at 06:18:54.34 +12:57:04.2: ref_mag=13.16 +/- 0.02 new_mean_mag=12.0043 delta=1.15 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:17:56.94 +13:25:25.8: 13.18 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:17:56.94 +13:25:25.8: 13.14 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.16 +/- 0.02
Forced photometry filter KEPT candidate at 06:17:56.94 +13:25:25.8: ref_mag=13.16 +/- 0.02 new_mean_mag=12.1883 delta=0.97 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:21:05.47 +16:15:55.8: 13.18 +/- 0.03 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:21:05.47 +16:15:55.8: 13.11 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.02
Forced photometry filter KEPT candidate at 06:21:05.47 +16:15:55.8: ref_mag=13.14 +/- 0.02 new_mean_mag=12.1434 delta=1.00 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:12:23.02 +09:38:46.1: 12.89 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:12:23.02 +09:38:46.1: 12.81 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.85 +/- 0.01
Forced photometry filter REJECTED candidate at 06:12:23.02 +09:38:46.1: ref_mag=12.85 +/- 0.01 new_mean_mag=11.9979 delta=0.85 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:21:58.43 +14:41:52.6: 13.13 +/- 0.03 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:21:58.43 +14:41:52.6: 13.15 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.02
Forced photometry filter KEPT candidate at 06:21:58.43 +14:41:52.6: ref_mag=13.14 +/- 0.02 new_mean_mag=12.1638 delta=0.97 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:20:17.27 +14:02:56.0: 13.12 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:20:17.27 +14:02:56.0: 13.09 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.02
Forced photometry filter KEPT candidate at 06:20:17.27 +14:02:56.0: ref_mag=13.10 +/- 0.02 new_mean_mag=12.0606 delta=1.04 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:22:22.80 +15:58:11.2: 13.12 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:22:22.80 +15:58:11.2: 13.10 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.11 +/- 0.02
Forced photometry filter KEPT candidate at 06:22:22.80 +15:58:11.2: ref_mag=13.11 +/- 0.02 new_mean_mag=12.0580 delta=1.05 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:23:51.74 +15:29:02.6: 13.13 +/- 0.04 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:23:51.74 +15:29:02.6: 13.12 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.03
Forced photometry filter KEPT candidate at 06:23:51.74 +15:29:02.6: ref_mag=13.12 +/- 0.03 new_mean_mag=12.1146 delta=1.01 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:26:02.18 +15:41:17.8: 13.10 +/- 0.03 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:26:02.18 +15:41:17.8: 13.08 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.02
Forced photometry filter KEPT candidate at 06:26:02.18 +15:41:17.8: ref_mag=13.09 +/- 0.02 new_mean_mag=12.0148 delta=1.08 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:21:06.61 +12:02:31.3: 13.08 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:21:06.61 +12:02:31.3: 12.97 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.02 +/- 0.02
Forced photometry filter KEPT candidate at 06:21:06.61 +12:02:31.3: ref_mag=13.02 +/- 0.02 new_mean_mag=11.9097 delta=1.11 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:15:56.08 +12:04:47.7: 13.07 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:15:56.08 +12:04:47.7: 13.04 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.05 +/- 0.02
Forced photometry filter KEPT candidate at 06:15:56.08 +12:04:47.7: ref_mag=13.05 +/- 0.02 new_mean_mag=12.0963 delta=0.96 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:16:21.84 +12:41:45.6: 13.07 +/- 0.03 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:16:21.84 +12:41:45.6: 13.17 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.02
Forced photometry filter KEPT candidate at 06:16:21.84 +12:41:45.6: ref_mag=13.12 +/- 0.02 new_mean_mag=12.1071 delta=1.01 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:18:23.21 +14:09:23.0: 13.06 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:18:23.21 +14:09:23.0: 12.96 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.00 +/- 0.01
Forced photometry filter KEPT candidate at 06:18:23.21 +14:09:23.0: ref_mag=13.00 +/- 0.01 new_mean_mag=11.9814 delta=1.02 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:15:56.88 +12:26:49.5: 13.07 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:15:56.88 +12:26:49.5: 13.08 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.07 +/- 0.02
Forced photometry filter KEPT candidate at 06:15:56.88 +12:26:49.5: ref_mag=13.07 +/- 0.02 new_mean_mag=11.9837 delta=1.09 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:24:06.45 +17:23:48.7: 13.02 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:24:06.45 +17:23:48.7: 12.90 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.95 +/- 0.02
Forced photometry filter KEPT candidate at 06:24:06.45 +17:23:48.7: ref_mag=12.95 +/- 0.02 new_mean_mag=11.9694 delta=0.99 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:17:33.94 +12:17:36.1: 13.05 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:17:33.94 +12:17:36.1: 13.08 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.07 +/- 0.02
Forced photometry filter KEPT candidate at 06:17:33.94 +12:17:36.1: ref_mag=13.07 +/- 0.02 new_mean_mag=11.9931 delta=1.07 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:21:05.48 +15:36:17.8: 13.05 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:21:05.48 +15:36:17.8: 12.99 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.02 +/- 0.02
Forced photometry filter KEPT candidate at 06:21:05.48 +15:36:17.8: ref_mag=13.02 +/- 0.02 new_mean_mag=12.0596 delta=0.96 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:19:52.72 +14:03:37.0: 13.05 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:19:52.72 +14:03:37.0: 13.11 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.02
Forced photometry filter KEPT candidate at 06:19:52.72 +14:03:37.0: ref_mag=13.08 +/- 0.02 new_mean_mag=12.0535 delta=1.03 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:15:58.18 +11:56:55.9: 13.04 +/- 0.03 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:15:58.18 +11:56:55.9: 13.03 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.03 +/- 0.02
Forced photometry filter KEPT candidate at 06:15:58.18 +11:56:55.9: ref_mag=13.03 +/- 0.02 new_mean_mag=12.0128 delta=1.02 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:21:36.02 +14:23:07.4: 13.04 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:21:36.02 +14:23:07.4: 13.10 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.07 +/- 0.02
Forced photometry filter KEPT candidate at 06:21:36.02 +14:23:07.4: ref_mag=13.07 +/- 0.02 new_mean_mag=12.1444 delta=0.92 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:17:54.05 +13:09:16.2: 12.54 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:17:54.05 +13:09:16.2: 12.55 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.55 +/- 0.01
Forced photometry filter REJECTED candidate at 06:17:54.05 +13:09:16.2: ref_mag=12.55 +/- 0.01 new_mean_mag=11.6854 delta=0.86 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:21:18.34 +13:50:32.3: 12.99 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:19:41.09 +13:22:20.0: 13.01 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:21:18.34 +13:50:32.3: 12.98 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.99 +/- 0.01
Forced photometry filter KEPT candidate at 06:21:18.34 +13:50:32.3: ref_mag=12.99 +/- 0.01 new_mean_mag=12.0409 delta=0.95 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:19:41.09 +13:22:20.0: 13.00 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.00 +/- 0.02
Forced photometry filter KEPT candidate at 06:19:41.09 +13:22:20.0: ref_mag=13.00 +/- 0.02 new_mean_mag=12.0300 delta=0.97 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:13:46.83 +11:22:34.6: 12.97 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:13:46.83 +11:22:34.6: 12.94 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.95 +/- 0.02
Forced photometry filter KEPT candidate at 06:13:46.83 +11:22:34.6: ref_mag=12.95 +/- 0.02 new_mean_mag=11.9446 delta=1.01 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:21:12.39 +12:29:13.2: 12.98 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:21:12.39 +12:29:13.2: 12.89 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.93 +/- 0.01
Forced photometry filter KEPT candidate at 06:21:12.39 +12:29:13.2: ref_mag=12.93 +/- 0.01 new_mean_mag=11.9034 delta=1.03 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:22:02.25 +14:28:25.0: 12.97 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:22:02.25 +14:28:25.0: 12.95 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.96 +/- 0.02
Forced photometry filter KEPT candidate at 06:22:02.25 +14:28:25.0: ref_mag=12.96 +/- 0.02 new_mean_mag=12.0434 delta=0.92 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:21:22.94 +15:36:43.5: 12.97 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:21:22.94 +15:36:43.5: 12.90 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.93 +/- 0.01
Forced photometry filter KEPT candidate at 06:21:22.94 +15:36:43.5: ref_mag=12.93 +/- 0.01 new_mean_mag=11.9699 delta=0.96 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:19:47.99 +13:27:05.8: 12.95 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:19:47.99 +13:27:05.8: 13.01 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.97 +/- 0.01
Forced photometry filter KEPT candidate at 06:19:47.99 +13:27:05.8: ref_mag=12.97 +/- 0.01 new_mean_mag=11.8968 delta=1.07 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:14:41.90 +11:18:57.9: 12.96 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:14:41.90 +11:18:57.9: 12.94 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.95 +/- 0.02
Forced photometry filter KEPT candidate at 06:14:41.90 +11:18:57.9: ref_mag=12.95 +/- 0.02 new_mean_mag=11.8092 delta=1.14 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:16:19.85 +12:10:09.7: 12.96 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:16:19.85 +12:10:09.7: 12.98 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.97 +/- 0.02
Forced photometry filter KEPT candidate at 06:16:19.85 +12:10:09.7: ref_mag=12.97 +/- 0.02 new_mean_mag=11.9308 delta=1.04 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:22:23.94 +16:08:57.8: 12.95 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:22:23.94 +16:08:57.8: 12.92 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.93 +/- 0.02
Forced photometry filter KEPT candidate at 06:22:23.94 +16:08:57.8: ref_mag=12.93 +/- 0.02 new_mean_mag=11.9572 delta=0.98 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:19:59.25 +13:26:56.2: 12.93 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:19:59.25 +13:26:56.2: 12.94 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.94 +/- 0.01
Forced photometry filter KEPT candidate at 06:19:59.25 +13:26:56.2: ref_mag=12.94 +/- 0.01 new_mean_mag=11.9614 delta=0.97 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:15:34.93 +08:57:35.2: 12.92 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:15:34.93 +08:57:35.2: 13.07 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.98 +/- 0.02
Forced photometry filter KEPT candidate at 06:15:34.93 +08:57:35.2: ref_mag=12.98 +/- 0.02 new_mean_mag=11.8713 delta=1.11 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:19:14.18 +12:05:39.4: 12.92 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:19:14.18 +12:05:39.4: 12.92 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.92 +/- 0.02
Forced photometry filter KEPT candidate at 06:19:14.18 +12:05:39.4: ref_mag=12.92 +/- 0.02 new_mean_mag=11.9635 delta=0.96 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:22:36.37 +14:50:32.6: 12.92 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:22:36.37 +14:50:32.6: 12.87 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.89 +/- 0.01
Forced photometry filter KEPT candidate at 06:22:36.37 +14:50:32.6: ref_mag=12.89 +/- 0.01 new_mean_mag=11.9736 delta=0.92 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:23:38.45 +16:21:05.8: 12.92 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:23:38.45 +16:21:05.8: 12.92 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.92 +/- 0.02
Forced photometry filter KEPT candidate at 06:23:38.45 +16:21:05.8: ref_mag=12.92 +/- 0.02 new_mean_mag=11.9513 delta=0.97 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:18:20.23 +13:57:36.2: 12.90 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:18:20.23 +13:57:36.2: 12.87 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.88 +/- 0.01
Forced photometry filter KEPT candidate at 06:18:20.23 +13:57:36.2: ref_mag=12.88 +/- 0.01 new_mean_mag=11.8759 delta=1.01 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:23:02.60 +15:01:17.7: 12.90 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:23:02.60 +15:01:17.7: 12.83 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.86 +/- 0.01
Forced photometry filter KEPT candidate at 06:23:02.60 +15:01:17.7: ref_mag=12.86 +/- 0.01 new_mean_mag=11.8370 delta=1.02 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:24:18.82 +17:36:38.1: 12.86 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:24:18.82 +17:36:38.1: 12.68 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.76 +/- 0.01
Forced photometry filter KEPT candidate at 06:24:18.82 +17:36:38.1: ref_mag=12.76 +/- 0.01 new_mean_mag=11.6665 delta=1.09 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:22:51.88 +15:19:35.5: 12.86 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:22:51.88 +15:19:35.5: 12.80 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.82 +/- 0.01
Forced photometry filter KEPT candidate at 06:22:51.88 +15:19:35.5: ref_mag=12.82 +/- 0.01 new_mean_mag=11.7680 delta=1.06 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:21:42.82 +14:02:36.5: 12.86 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:21:26.68 +14:52:43.1: 12.86 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:21:42.82 +14:02:36.5: 12.82 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.84 +/- 0.02
Forced photometry filter KEPT candidate at 06:21:42.82 +14:02:36.5: ref_mag=12.84 +/- 0.02 new_mean_mag=11.8928 delta=0.95 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:21:26.68 +14:52:43.1: 12.83 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.84 +/- 0.01
Forced photometry filter KEPT candidate at 06:21:26.68 +14:52:43.1: ref_mag=12.84 +/- 0.01 new_mean_mag=11.9070 delta=0.94 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:19:06.89 +13:31:29.1: 12.85 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:19:06.89 +13:31:29.1: 12.83 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.84 +/- 0.01
Forced photometry filter KEPT candidate at 06:19:06.89 +13:31:29.1: ref_mag=12.84 +/- 0.01 new_mean_mag=11.9066 delta=0.93 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:16:27.39 +12:55:00.2: 12.85 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:16:27.39 +12:55:00.2: 12.80 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.82 +/- 0.01
Forced photometry filter KEPT candidate at 06:16:27.39 +12:55:00.2: ref_mag=12.82 +/- 0.01 new_mean_mag=11.8304 delta=0.99 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:17:13.93 +12:57:00.4: 12.84 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:17:13.93 +12:57:00.4: 12.78 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.81 +/- 0.01
Forced photometry filter KEPT candidate at 06:17:13.93 +12:57:00.4: ref_mag=12.81 +/- 0.01 new_mean_mag=11.8558 delta=0.95 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:20:36.88 +14:59:16.1: 12.83 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:20:36.88 +14:59:16.1: 12.88 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.85 +/- 0.01
Forced photometry filter KEPT candidate at 06:20:36.88 +14:59:16.1: ref_mag=12.85 +/- 0.01 new_mean_mag=11.9027 delta=0.95 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:19:39.31 +13:12:58.5: 12.82 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:19:39.31 +13:12:58.5: 12.77 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.79 +/- 0.01
Forced photometry filter KEPT candidate at 06:19:39.31 +13:12:58.5: ref_mag=12.79 +/- 0.01 new_mean_mag=11.8251 delta=0.97 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:24:36.07 +15:32:08.2: 12.81 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:24:36.07 +15:32:08.2: 12.73 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.77 +/- 0.01
Forced photometry filter KEPT candidate at 06:24:36.07 +15:32:08.2: ref_mag=12.77 +/- 0.01 new_mean_mag=11.8239 delta=0.94 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:20:06.84 +13:21:31.0: 12.77 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:21:02.86 +13:58:55.2: 12.79 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:20:06.84 +13:21:31.0: 12.77 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.77 +/- 0.01
Forced photometry filter KEPT candidate at 06:20:06.84 +13:21:31.0: ref_mag=12.77 +/- 0.01 new_mean_mag=11.8201 delta=0.95 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:21:02.86 +13:58:55.2: 12.74 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.76 +/- 0.01
Forced photometry filter KEPT candidate at 06:21:02.86 +13:58:55.2: ref_mag=12.76 +/- 0.01 new_mean_mag=11.8314 delta=0.93 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:18:17.29 +13:14:30.7: 12.78 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:18:17.29 +13:14:30.7: 12.77 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.78 +/- 0.01
Forced photometry filter KEPT candidate at 06:18:17.29 +13:14:30.7: ref_mag=12.78 +/- 0.01 new_mean_mag=11.8029 delta=0.97 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:18:59.71 +11:41:49.2: 12.77 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:18:59.71 +11:41:49.2: 12.87 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.82 +/- 0.01
Forced photometry filter KEPT candidate at 06:18:59.71 +11:41:49.2: ref_mag=12.82 +/- 0.01 new_mean_mag=11.8423 delta=0.97 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:15:58.94 +12:04:19.7: 12.75 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:15:58.94 +12:04:19.7: 12.67 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.70 +/- 0.01
Forced photometry filter KEPT candidate at 06:15:58.94 +12:04:19.7: ref_mag=12.70 +/- 0.01 new_mean_mag=11.7762 delta=0.93 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:22:01.48 +15:05:42.4: 12.75 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:22:01.48 +15:05:42.4: 12.81 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.78 +/- 0.01
Forced photometry filter KEPT candidate at 06:22:01.48 +15:05:42.4: ref_mag=12.78 +/- 0.01 new_mean_mag=11.8630 delta=0.92 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:14:14.37 +11:35:24.1: 12.74 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:14:14.37 +11:35:24.1: 12.73 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.74 +/- 0.01
Forced photometry filter KEPT candidate at 06:14:14.37 +11:35:24.1: ref_mag=12.74 +/- 0.01 new_mean_mag=11.8154 delta=0.92 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:17:04.67 +13:15:59.3: 12.72 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:17:04.67 +13:15:59.3: 12.71 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.71 +/- 0.01
Forced photometry filter KEPT candidate at 06:17:04.67 +13:15:59.3: ref_mag=12.71 +/- 0.01 new_mean_mag=11.7059 delta=1.01 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:16:37.12 +11:38:33.8: 12.72 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:16:37.12 +11:38:33.8: 12.71 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.72 +/- 0.01
Forced photometry filter KEPT candidate at 06:16:37.12 +11:38:33.8: ref_mag=12.72 +/- 0.01 new_mean_mag=11.7524 delta=0.96 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:22:03.80 +14:30:06.5: 12.69 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:22:03.80 +14:30:06.5: 12.68 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.69 +/- 0.01
Forced photometry filter KEPT candidate at 06:22:03.80 +14:30:06.5: ref_mag=12.69 +/- 0.01 new_mean_mag=11.7797 delta=0.91 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:15:40.38 +12:19:06.2: 12.69 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:15:40.38 +12:19:06.2: 12.62 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.65 +/- 0.01
Forced photometry filter KEPT candidate at 06:15:40.38 +12:19:06.2: ref_mag=12.65 +/- 0.01 new_mean_mag=11.6132 delta=1.04 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:19:37.86 +13:54:56.6: 12.69 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:19:37.86 +13:54:56.6: 12.67 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.68 +/- 0.01
Forced photometry filter KEPT candidate at 06:19:37.86 +13:54:56.6: ref_mag=12.68 +/- 0.01 new_mean_mag=11.7498 delta=0.93 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:17:31.32 +12:40:45.1: 12.69 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:17:31.32 +12:40:45.1: 12.68 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.68 +/- 0.01
Forced photometry filter KEPT candidate at 06:17:31.32 +12:40:45.1: ref_mag=12.68 +/- 0.01 new_mean_mag=11.6935 delta=0.99 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:23:36.49 +15:10:36.0: 12.62 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:23:36.49 +15:10:36.0: 12.61 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.61 +/- 0.01
Forced photometry filter REJECTED candidate at 06:23:36.49 +15:10:36.0: ref_mag=12.61 +/- 0.01 new_mean_mag=11.7422 delta=0.87 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:16:05.49 +11:27:27.2: 12.67 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:16:05.49 +11:27:27.2: 12.62 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.64 +/- 0.01
Forced photometry filter KEPT candidate at 06:16:05.49 +11:27:27.2: ref_mag=12.64 +/- 0.01 new_mean_mag=11.7296 delta=0.91 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:22:12.45 +17:01:24.1: 12.68 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:22:12.45 +17:01:24.1: 12.61 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.64 +/- 0.01
Forced photometry filter KEPT candidate at 06:22:12.45 +17:01:24.1: ref_mag=12.64 +/- 0.01 new_mean_mag=11.6853 delta=0.95 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:20:37.32 +14:08:16.7: 12.66 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:20:37.32 +14:08:16.7: 12.58 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.61 +/- 0.01
Forced photometry filter KEPT candidate at 06:20:37.32 +14:08:16.7: ref_mag=12.61 +/- 0.01 new_mean_mag=11.4845 delta=1.13 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:22:11.41 +14:25:20.7: 12.62 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:22:11.41 +14:25:20.7: 12.57 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.59 +/- 0.01
Forced photometry filter KEPT candidate at 06:22:11.41 +14:25:20.7: ref_mag=12.59 +/- 0.01 new_mean_mag=11.5609 delta=1.03 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:17:11.53 +12:44:29.7: 12.61 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:17:11.53 +12:44:29.7: 12.62 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.61 +/- 0.01
Forced photometry filter KEPT candidate at 06:17:11.53 +12:44:29.7: ref_mag=12.61 +/- 0.01 new_mean_mag=11.5901 delta=1.02 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:21:11.60 +14:23:30.8: 12.60 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:21:11.60 +14:23:30.8: 12.55 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.57 +/- 0.01
Forced photometry filter KEPT candidate at 06:21:11.60 +14:23:30.8: ref_mag=12.57 +/- 0.01 new_mean_mag=11.6303 delta=0.94 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:14:55.53 +11:52:39.1: 12.59 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:14:55.53 +11:52:39.1: 12.60 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.59 +/- 0.01
Forced photometry filter KEPT candidate at 06:14:55.53 +11:52:39.1: ref_mag=12.59 +/- 0.01 new_mean_mag=11.6319 delta=0.96 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:14:21.80 +11:39:10.0: 12.58 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:14:21.80 +11:39:10.0: 12.62 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.60 +/- 0.01
Forced photometry filter KEPT candidate at 06:14:21.80 +11:39:10.0: ref_mag=12.60 +/- 0.01 new_mean_mag=11.6327 delta=0.96 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:21:00.31 +13:51:48.9: 12.56 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:21:00.31 +13:51:48.9: 12.60 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.58 +/- 0.01
Forced photometry filter KEPT candidate at 06:21:00.31 +13:51:48.9: ref_mag=12.58 +/- 0.01 new_mean_mag=11.6455 delta=0.93 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 05:42:52.71 +16:12:45.0: 12.50 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 05:42:52.71 +16:12:45.0: 12.61 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.56 +/- 0.01
Forced photometry filter KEPT candidate at 05:42:52.71 +16:12:45.0: ref_mag=12.56 +/- 0.01 new_mean_mag=11.5745 delta=0.98 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:16:05.47 +12:14:58.6: 12.50 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:16:05.47 +12:14:58.6: 12.47 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.48 +/- 0.01
Forced photometry filter KEPT candidate at 06:16:05.47 +12:14:58.6: ref_mag=12.48 +/- 0.01 new_mean_mag=11.5639 delta=0.92 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:12:31.63 +10:21:09.8: 12.12 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:12:31.63 +10:21:09.8: 12.03 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.07 +/- 0.01
Forced photometry filter REJECTED candidate at 06:12:31.63 +10:21:09.8: ref_mag=12.07 +/- 0.01 new_mean_mag=11.3444 delta=0.72 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:20:08.32 +14:28:04.8: 12.48 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:20:08.32 +14:28:04.8: 12.45 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.47 +/- 0.01
Forced photometry filter KEPT candidate at 06:20:08.32 +14:28:04.8: ref_mag=12.47 +/- 0.01 new_mean_mag=11.5212 delta=0.95 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:20:13.32 +14:22:12.0: 12.46 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:20:13.32 +14:22:12.0: 12.38 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.41 +/- 0.01
Forced photometry filter KEPT candidate at 06:20:13.32 +14:22:12.0: ref_mag=12.41 +/- 0.01 new_mean_mag=11.4812 delta=0.93 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:31:48.66 +15:28:57.9: 12.46 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:31:48.66 +15:28:57.9: 12.30 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.37 +/- 0.01
Forced photometry filter REJECTED candidate at 06:31:48.66 +15:28:57.9: ref_mag=12.37 +/- 0.01 new_mean_mag=11.4814 delta=0.89 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:14:39.77 +09:56:55.2: 12.45 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:21:57.52 +16:30:57.4: 12.42 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:14:39.77 +09:56:55.2: 12.54 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.49 +/- 0.01
Forced photometry filter KEPT candidate at 06:14:39.77 +09:56:55.2: ref_mag=12.49 +/- 0.01 new_mean_mag=11.4780 delta=1.02 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:21:57.52 +16:30:57.4: 12.36 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.39 +/- 0.01
Forced photometry filter KEPT candidate at 06:21:57.52 +16:30:57.4: ref_mag=12.39 +/- 0.01 new_mean_mag=11.4701 delta=0.92 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:12:17.54 +09:21:02.5: 12.37 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:14:44.26 +10:32:56.3: 12.31 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:28:20.97 +17:32:35.3: 12.26 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:12:17.54 +09:21:02.5: 12.43 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.40 +/- 0.01
Forced photometry filter KEPT candidate at 06:12:17.54 +09:21:02.5: ref_mag=12.40 +/- 0.01 new_mean_mag=11.3596 delta=1.04 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:14:44.26 +10:32:56.3: 12.25 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.28 +/- 0.01
Forced photometry filter KEPT candidate at 06:14:44.26 +10:32:56.3: ref_mag=12.28 +/- 0.01 new_mean_mag=11.2695 delta=1.01 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:28:20.97 +17:32:35.3: 12.44 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.34 +/- 0.01
Forced photometry filter KEPT candidate at 06:28:20.97 +17:32:35.3: ref_mag=12.34 +/- 0.01 new_mean_mag=11.3749 delta=0.96 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:13:45.34 +11:31:40.2: 12.20 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:33:59.97 +15:17:02.2: 12.12 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:14:55.33 +10:20:22.7: 12.10 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:13:45.34 +11:31:40.2: 12.30 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.24 +/- 0.01
Forced photometry filter KEPT candidate at 06:13:45.34 +11:31:40.2: ref_mag=12.24 +/- 0.01 new_mean_mag=11.2261 delta=1.02 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:33:59.97 +15:17:02.2: 11.90 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:14:55.33 +10:20:22.7: 12.17 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.99 +/- 0.01
Forced photometry filter KEPT candidate at 06:33:59.97 +15:17:02.2: ref_mag=11.99 +/- 0.01 new_mean_mag=11.0439 delta=0.95 (need > 0.90)
Forced photometry reference-image weighted average: 12.13 +/- 0.01
Forced photometry filter KEPT candidate at 06:14:55.33 +10:20:22.7: ref_mag=12.13 +/- 0.01 new_mean_mag=11.1641 delta=0.97 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:15:54.47 +10:33:56.7: 12.11 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:15:54.47 +10:33:56.7: 12.16 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.13 +/- 0.01
Forced photometry filter KEPT candidate at 06:15:54.47 +10:33:56.7: ref_mag=12.13 +/- 0.01 new_mean_mag=11.2116 delta=0.92 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:18:14.34 +11:20:45.1: 12.11 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:18:42.63 +13:02:54.4: 11.98 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:19:51.02 +13:36:19.2: 12.01 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:18:14.34 +11:20:45.1: 12.08 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.09 +/- 0.01
Forced photometry filter KEPT candidate at 06:18:14.34 +11:20:45.1: ref_mag=12.09 +/- 0.01 new_mean_mag=10.9212 delta=1.17 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:18:42.63 +13:02:54.4: 11.77 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:19:51.02 +13:36:19.2: 12.31 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.85 +/- 0.01
Forced photometry filter KEPT candidate at 06:18:42.63 +13:02:54.4: ref_mag=11.85 +/- 0.01 new_mean_mag=10.7999 delta=1.05 (need > 0.90)
Forced photometry reference-image weighted average: 12.13 +/- 0.01
Forced photometry filter KEPT candidate at 06:19:51.02 +13:36:19.2: ref_mag=12.13 +/- 0.01 new_mean_mag=11.1230 delta=1.00 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:18:05.68 +12:22:21.5: 11.87 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:18:05.68 +12:22:21.5: 11.81 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.84 +/- 0.01
Forced photometry filter KEPT candidate at 06:18:05.68 +12:22:21.5: ref_mag=11.84 +/- 0.01 new_mean_mag=10.8765 delta=0.96 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:14:42.50 +11:28:07.8: 11.85 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:14:42.50 +11:28:07.8: 11.82 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.84 +/- 0.01
Forced photometry filter KEPT candidate at 06:14:42.50 +11:28:07.8: ref_mag=11.84 +/- 0.01 new_mean_mag=10.9045 delta=0.93 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:12:28.76 +10:28:25.6: 11.39 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:16:06.52 +10:56:43.1: 11.14 +/- 0.00 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:12:28.76 +10:28:25.6: 11.55 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.46 +/- 0.00
Forced photometry filter KEPT candidate at 06:12:28.76 +10:28:25.6: ref_mag=11.46 +/- 0.00 new_mean_mag=10.5125 delta=0.95 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:16:06.52 +10:56:43.1: 10.95 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.03 +/- 0.00
Forced photometry filter KEPT candidate at 06:16:06.52 +10:56:43.1: ref_mag=11.03 +/- 0.00 new_mean_mag=10.0932 delta=0.94 (need > 0.90)
Adding exclusion_list_local.txt__out104131.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out105008.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out105187.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out106639.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out107020.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out107058.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out107667.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out112340.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out112420.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out112923.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out114418.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out114709.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out114782.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116628.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116975.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out117938.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out118967.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out119465.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out125705.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out126860.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out127682.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out128660.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out128868.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out129331.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out130499.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out130913.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131234.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133147.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133562.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134209.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136842.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138678.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out139886.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out140564.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out140599.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out141195.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out144185.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out145381.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out146370.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out146881.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out147418.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out151105.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out152036.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out152737.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out154415.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out155034.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out155266.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out156526.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out158073.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out159710.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out160049.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out160054.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out160354.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out160824.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out160911.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out162888.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out164538.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168086.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168554.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out169542.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out169769.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out170880.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out172550.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out173664.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out173803.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175335.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176575.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176588.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out183237.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out185529.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out185828.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out187101.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out187412.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out188830.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195556.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out205235.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out211426.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out213745.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out224981.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33798.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35224.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out38232.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out46467.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out57621.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out61096.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out61522.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out62801.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out65183.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out66433.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out69085.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out69409.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out75426.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77468.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77740.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out78018.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out79181.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out80343.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out82061.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out84244.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out84586.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out85986.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out89800.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out91590.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out92609.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out93692.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out95109.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out95933.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out96133.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out99313.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 781s
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: 51s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266155_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 266155_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266163_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 266163_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
**** FOUND 05:53:16.42 +18:58:32.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266191_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 266191_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
**** FOUND 06:42:43.61 +08:51:17.0 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266221_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 266221_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266227_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 266227_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
**** FOUND 06:41:49.69 +09:30:28.7 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266229_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 266229_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
**** FOUND 06:41:18.69 +09:12:47.9 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266259_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 266259_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266261_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 266261_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266271_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 266271_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266287_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 266287_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266298_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 266298_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266313_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 266313_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266315_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 266315_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266316_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 266316_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266333_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 266333_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
**** FOUND 06:29:57.33 +16:35:42.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266337_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 266337_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266340_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 266340_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
**** FOUND 05:45:20.65 +19:07:51.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266341_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 266341_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266359_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 266359_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
**** FOUND 06:25:55.94 +08:43:05.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266371_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 266371_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266381_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 266381_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266384_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 266384_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
**** FOUND 06:27:20.21 +08:42:01.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266387_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 266387_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
**** FOUND 05:59:02.31 +19:13:59.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266420_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 266420_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266428_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 266428_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266435_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 266435_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266440_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 266440_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266466_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 266466_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266518_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 266518_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266519_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 266519_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266528_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 266528_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
**** FOUND 06:42:18.87 +17:37:58.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266546_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 266546_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
**** FOUND 06:43:56.04 +13:15:35.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266551_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 266551_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266564_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 266564_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
**** FOUND 06:15:03.41 +13:50:06.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266574_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 266574_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266584_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 266584_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266596_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 266596_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266599_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 266599_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266604_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 266604_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
**** FOUND 06:31:04.46 +16:56:46.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266669_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 266669_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266670_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 266670_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
**** FOUND 06:11:27.41 +13:39:42.2 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266676_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 266676_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
**** FOUND 06:34:47.67 +16:12:06.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266718_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 266718_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266726_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 266726_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266742_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 266742_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266765_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 266765_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
**** FOUND 06:19:58.31 +14:38:22.2 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266785_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 266785_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
**** FOUND 06:12:02.84 +14:11:58.3 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 266817_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 266817_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 69409_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 69409_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 61953_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 61953_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 127682_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 127682_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 18783_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 18783_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 211426_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 211426_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131234_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 131234_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 139886_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 139886_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 85986_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 85986_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51939_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 51939_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 66433_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 66433_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 96133_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 96133_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 185828_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 185828_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 93692_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 93692_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 152737_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 152737_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 114225_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 114225_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 78018_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 78018_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160911_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 160911_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136842_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 136842_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112420_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 112420_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160049_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 160049_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 155639_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 155639_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
**** FOUND 06:24:19.38 +12:15:56.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 82516_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 82516_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
**** FOUND 06:16:43.27 +15:24:11.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 147418_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 147418_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 84514_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 84514_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
**** FOUND 06:22:34.31 +15:19:06.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 164118_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 164118_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
**** FOUND 06:16:27.88 +11:54:52.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 188830_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 188830_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 119392_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 119392_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
**** FOUND 06:20:53.32 +13:50:47.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 174803_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 174803_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
**** FOUND 06:03:20.96 +11:26:15.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 82061_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 82061_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 144185_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 144185_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 168086_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 168086_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 46076_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 46076_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
**** FOUND 06:25:14.22 +17:01:53.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 140599_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 140599_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 129331_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 129331_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62801_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 62801_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 218950_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 218950_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 99313_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 99313_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 114709_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 114709_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 69085_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 69085_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 80343_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 80343_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 137851_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 137851_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
**** FOUND 06:27:24.64 +13:02:03.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 75426_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 75426_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160824_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 160824_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160054_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 160054_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 146370_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 146370_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112340_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 112340_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 152036_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 152036_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 38232_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 38232_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 155266_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 155266_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 77740_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 77740_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 114418_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 114418_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 162888_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 162888_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 107058_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 107058_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 135616_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 135616_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 223139_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 223139_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
**** FOUND 06:11:51.42 +09:50:26.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 184758_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 184758_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
**** FOUND 06:26:52.82 +10:23:47.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 119465_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 119465_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 130499_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 130499_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 175335_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 175335_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151105_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 151105_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 105008_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 105008_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 77468_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 77468_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 128660_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 128660_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 176588_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 176588_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 158073_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 158073_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 65183_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 65183_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 128868_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 128868_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 205235_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 205235_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159710_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 159710_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 95933_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 95933_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 61096_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 61096_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116975_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 116975_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21204_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 21204_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
**** FOUND 06:19:43.66 +18:15:21.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 91590_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 91590_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 186785_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 186785_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
**** FOUND 06:18:03.70 +10:31:16.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33798_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 33798_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 84244_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 84244_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 114782_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 114782_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 95109_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 95109_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 126860_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 126860_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 141195_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 141195_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 140564_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 140564_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 92609_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 92609_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134209_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 134209_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 79181_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 79181_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 130913_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 130913_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116628_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 116628_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133562_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 133562_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 168554_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 168554_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160354_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 160354_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 89800_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 89800_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170880_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 170880_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133147_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 133147_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 185980_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 185980_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
**** FOUND 05:59:36.69 +10:28:42.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 169769_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 169769_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104131_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 104131_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 155034_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 155034_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 117938_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 117938_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 146881_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 146881_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 88165_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 88165_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173664_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 173664_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33322_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 33322_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
**** FOUND 06:25:18.05 +17:38:38.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 46467_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 46467_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112923_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 112923_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 106639_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 106639_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 178081_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 178081_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
**** FOUND 06:14:53.77 +11:15:24.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 145381_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 145381_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 107020_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 107020_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 164538_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 164538_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 169542_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 169542_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192045_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 192045_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
**** FOUND 06:16:00.14 +10:47:26.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118967_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 118967_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 61522_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 61522_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 156526_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 156526_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 183050_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 183050_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 28824_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 28824_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
**** FOUND 06:32:33.75 +17:50:09.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 105187_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 105187_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 26621_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 26621_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
**** FOUND 05:46:56.65 +17:54:30.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 107667_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 107667_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 79797_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 79797_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 224981_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 224981_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 57621_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 57621_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 147876_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 147876_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
**** FOUND 05:56:03.40 +12:39:03.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 213745_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 213745_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 187101_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 187101_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35224_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 35224_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 172550_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 172550_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 84586_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 84586_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 183237_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 183237_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 187412_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 187412_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 176575_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 176575_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125705_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 125705_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 138678_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 138678_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102507_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 102507_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
**** FOUND 06:28:57.60 +14:36:34.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154415_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 154415_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173803_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 173803_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 185529_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 185529_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104176_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 104176_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
**** FOUND 06:32:05.84 +14:31:13.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195556_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
Preparing report for the candidate 195556_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 114333_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 114333_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
**** FOUND 06:11:56.44 +14:12:27.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 122850_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 122850_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
**** FOUND 06:15:08.51 +13:51:02.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 109415_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 109415_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
**** FOUND 06:18:05.55 +14:22:56.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101327_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 101327_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
**** FOUND 06:07:34.47 +14:46:02.2 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 105047_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 105047_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
**** FOUND 06:20:04.16 +14:39:00.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 152021_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 152021_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
**** FOUND 06:15:44.91 +12:33:03.2 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 158801_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 158801_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
**** FOUND 06:16:26.68 +12:16:24.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 68622_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 68622_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
**** FOUND 06:12:03.30 +16:07:45.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 69363_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 69363_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
**** FOUND 06:15:25.11 +16:08:32.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189426_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 189426_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
**** FOUND 06:13:12.66 +10:37:29.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102755_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 102755_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
**** FOUND 06:25:28.12 +14:43:17.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 213932_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 213932_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
**** FOUND 06:17:06.61 +09:56:31.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32243_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 32243_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
**** FOUND 05:47:26.26 +17:43:44.3 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 217685_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 217685_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
**** FOUND 06:02:23.17 +09:38:50.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 135850_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 135850_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
**** FOUND 06:43:59.09 +13:13:35.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 225474_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 225474_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
**** FOUND 06:40:58.65 +09:53:43.0 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 149081_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 149081_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
**** FOUND 05:49:32.96 +12:39:03.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62388_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137
The candidate 62388_fd_Ori-02-Q1b1x1_2026-08-22_04-37-01_20.00sec_0.00C_LIGHTs_0137 did not pass the final checks
**** FOUND 06:37:42.65 +16:23:52.3 in the exclusion list exclusion_list_bbsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 8s
make_report_in_HTML.sh TOTAL: 840s
Prepared the HTML report for the field Ori-02-Q1b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
06:22:03.80 +14:30:06.5
06:22:02.25 +14:28:25.0
06:20:08.32 +14:28:04.8
06:22:11.41 +14:25:20.7
06:21:11.60 +14:23:30.8
06:21:36.02 +14:23:07.4
06:20:13.32 +14:22:12.0
06:18:23.21 +14:09:23.0
06:21:34.28 +14:08:35.2
06:20:37.32 +14:08:16.7
06:19:52.72 +14:03:37.0
06:20:17.27 +14:02:56.0
06:21:42.82 +14:02:36.5
06:21:02.86 +13:58:55.2
06:18:20.23 +13:57:36.2
06:19:37.86 +13:54:56.6
06:21:00.31 +13:51:48.9
06:21:18.34 +13:50:32.3
06:19:51.02 +13:36:19.2
06:19:06.89 +13:31:29.1
06:18:03.95 +13:30:16.6
06:19:47.99 +13:27:05.8
06:19:59.25 +13:26:56.2
06:17:56.94 +13:25:25.8
06:19:41.09 +13:22:20.0
06:20:06.84 +13:21:31.0
06:20:10.05 +13:20:58.6
06:17:04.67 +13:15:59.3
06:18:17.29 +13:14:30.7
06:19:39.31 +13:12:58.5
06:17:36.16 +13:06:06.3
06:18:42.63 +13:02:54.4
06:21:10.22 +12:58:17.9
06:17:13.93 +12:57:00.4
06:18:54.34 +12:57:04.2
06:16:27.39 +12:55:00.2
06:17:17.52 +12:47:01.7
06:17:11.53 +12:44:29.7
06:16:21.84 +12:41:45.6
06:17:31.32 +12:40:45.1
06:16:52.29 +12:39:03.5
06:21:12.39 +12:29:13.2
06:15:56.88 +12:26:49.5
06:16:58.38 +12:25:08.5
06:18:05.68 +12:22:21.5
06:15:40.38 +12:19:06.2
06:17:33.94 +12:17:36.1
06:16:05.47 +12:14:58.6
06:16:19.85 +12:10:09.7
06:19:14.18 +12:05:39.4
06:16:33.61 +12:04:50.5
06:15:56.08 +12:04:47.7
06:15:58.94 +12:04:19.7
06:21:06.61 +12:02:31.3
06:15:15.56 +12:02:24.1
06:15:58.18 +11:56:55.9
06:14:55.53 +11:52:39.1
06:15:19.32 +11:42:51.1
06:18:59.71 +11:41:49.2
06:14:21.80 +11:39:10.0
06:16:37.12 +11:38:33.8
06:14:14.37 +11:35:24.1
06:13:45.34 +11:31:40.2
06:16:05.49 +11:27:27.2
06:14:42.50 +11:28:07.8
06:13:46.83 +11:22:34.6
06:18:14.34 +11:20:45.1
06:14:41.90 +11:18:57.9
06:14:55.33 +10:20:22.7
06:12:28.76 +10:28:25.6
06:12:25.54 +10:30:59.9
06:14:44.26 +10:32:56.3
06:15:54.47 +10:33:56.7
06:12:38.91 +10:38:15.1
06:16:06.52 +10:56:43.1
06:15:34.93 +08:57:35.2
05:58:59.97 +09:16:46.1
06:12:17.54 +09:21:02.5
06:14:39.77 +09:56:55.2
06:24:18.82 +17:36:38.1
06:28:20.97 +17:32:35.3
06:24:06.45 +17:23:48.7
06:22:12.45 +17:01:24.1
06:21:57.52 +16:30:57.4
06:23:38.45 +16:21:05.8
05:42:52.71 +16:12:45.0
06:21:05.47 +16:15:55.8
06:22:23.94 +16:08:57.8
06:22:27.61 +16:05:21.6
06:22:22.80 +15:58:11.2
06:26:21.49 +15:58:57.2
06:26:02.18 +15:41:17.8
06:21:22.94 +15:36:43.5
06:21:05.48 +15:36:17.8
06:24:38.86 +15:35:16.9
06:24:36.07 +15:32:08.2
06:23:51.74 +15:29:02.6
06:23:40.76 +15:24:49.4
06:22:51.88 +15:19:35.5
06:33:59.97 +15:17:02.2
06:20:56.55 +15:15:27.3
06:22:01.48 +15:05:42.4
06:23:02.60 +15:01:17.7
06:20:36.88 +14:59:16.1
06:19:44.97 +14:56:40.9
06:21:26.68 +14:52:43.1
06:22:36.37 +14:50:32.6
06:24:56.21 +14:49:23.4
06:21:58.43 +14:41:52.6
########### Completed Ori-02-Q1b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ1.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
06:26:21.49 +15:58:57.2
06:18:03.95 +13:30:16.6
05:58:59.97 +09:16:46.1
06:20:10.05 +13:20:58.6
06:21:10.22 +12:58:17.9
06:20:56.55 +15:15:27.3
06:22:27.61 +16:05:21.6
06:24:56.21 +14:49:23.4
06:12:25.54 +10:30:59.9
06:19:44.97 +14:56:40.9
06:16:58.38 +12:25:08.5
06:24:38.86 +15:35:16.9
06:15:15.56 +12:02:24.1
06:17:36.16 +13:06:06.3
06:21:34.28 +14:08:35.2
06:16:33.61 +12:04:50.5
06:16:52.29 +12:39:03.5
06:12:38.91 +10:38:15.1
06:23:40.76 +15:24:49.4
06:17:17.52 +12:47:01.7
06:15:19.32 +11:42:51.1
06:18:54.34 +12:57:04.2
06:17:56.94 +13:25:25.8
06:21:05.47 +16:15:55.8
06:21:58.43 +14:41:52.6
06:20:17.27 +14:02:56.0
06:22:22.80 +15:58:11.2
06:23:51.74 +15:29:02.6
06:26:02.18 +15:41:17.8
06:21:06.61 +12:02:31.3
06:15:56.08 +12:04:47.7
06:16:21.84 +12:41:45.6
06:18:23.21 +14:09:23.0
06:15:56.88 +12:26:49.5
06:24:06.45 +17:23:48.7
06:17:33.94 +12:17:36.1
06:21:05.48 +15:36:17.8
06:19:52.72 +14:03:37.0
06:15:58.18 +11:56:55.9
06:21:36.02 +14:23:07.4
06:21:18.34 +13:50:32.3
06:19:41.09 +13:22:20.0
06:13:46.83 +11:22:34.6
06:21:12.39 +12:29:13.2
06:22:02.25 +14:28:25.0
06:21:22.94 +15:36:43.5
06:19:47.99 +13:27:05.8
06:14:41.90 +11:18:57.9
06:16:19.85 +12:10:09.7
06:22:23.94 +16:08:57.8
06:19:59.25 +13:26:56.2
06:15:34.93 +08:57:35.2
06:19:14.18 +12:05:39.4
06:22:36.37 +14:50:32.6
06:23:38.45 +16:21:05.8
06:18:20.23 +13:57:36.2
06:23:02.60 +15:01:17.7
06:24:18.82 +17:36:38.1
06:22:51.88 +15:19:35.5
06:21:42.82 +14:02:36.5
06:21:26.68 +14:52:43.1
06:19:06.89 +13:31:29.1
06:16:27.39 +12:55:00.2
06:17:13.93 +12:57:00.4
06:20:36.88 +14:59:16.1
06:19:39.31 +13:12:58.5
06:24:36.07 +15:32:08.2
06:20:06.84 +13:21:31.0
06:21:02.86 +13:58:55.2
06:18:17.29 +13:14:30.7
06:18:59.71 +11:41:49.2
06:15:58.94 +12:04:19.7
06:22:01.48 +15:05:42.4
06:14:14.37 +11:35:24.1
06:17:04.67 +13:15:59.3
06:16:37.12 +11:38:33.8
06:22:03.80 +14:30:06.5
06:15:40.38 +12:19:06.2
06:19:37.86 +13:54:56.6
06:17:31.32 +12:40:45.1
06:16:05.49 +11:27:27.2
06:22:12.45 +17:01:24.1
06:20:37.32 +14:08:16.7
06:22:11.41 +14:25:20.7
06:17:11.53 +12:44:29.7
06:21:11.60 +14:23:30.8
06:14:55.53 +11:52:39.1
06:14:21.80 +11:39:10.0
06:21:00.31 +13:51:48.9
05:42:52.71 +16:12:45.0
06:16:05.47 +12:14:58.6
06:20:08.32 +14:28:04.8
06:20:13.32 +14:22:12.0
06:14:39.77 +09:56:55.2
06:21:57.52 +16:30:57.4
06:12:17.54 +09:21:02.5
06:14:44.26 +10:32:56.3
06:28:20.97 +17:32:35.3
06:13:45.34 +11:31:40.2
06:33:59.97 +15:17:02.2
06:14:55.33 +10:20:22.7
06:15:54.47 +10:33:56.7
06:18:14.34 +11:20:45.1
06:19:51.02 +13:36:19.2
06:18:42.63 +13:02:54.4
06:18:05.68 +12:22:21.5
06:14:42.50 +11:28:07.8
06:12:28.76 +10:28:25.6
06:16:06.52 +10:56:43.1
###################################################################################
06:26:21.49 +15:58:57.2 -- not an asteroid (will add it to exclusion list)
06:18:03.95 +13:30:16.6 -- not an asteroid (will add it to exclusion list)
05:58:59.97 +09:16:46.1 -- not an asteroid (will add it to exclusion list)
06:20:10.05 +13:20:58.6 -- not an asteroid (will add it to exclusion list)
06:21:10.22 +12:58:17.9 -- not an asteroid (will add it to exclusion list)
06:20:56.55 +15:15:27.3 -- not an asteroid (will add it to exclusion list)
06:22:27.61 +16:05:21.6 -- not an asteroid (will add it to exclusion list)
06:24:56.21 +14:49:23.4 -- not an asteroid (will add it to exclusion list)
06:12:25.54 +10:30:59.9 -- not an asteroid (will add it to exclusion list)
06:19:44.97 +14:56:40.9 -- not an asteroid (will add it to exclusion list)
06:16:58.38 +12:25:08.5 -- not an asteroid (will add it to exclusion list)
06:24:38.86 +15:35:16.9 -- not an asteroid (will add it to exclusion list)
06:15:15.56 +12:02:24.1 -- not an asteroid (will add it to exclusion list)
06:17:36.16 +13:06:06.3 -- not an asteroid (will add it to exclusion list)
06:21:34.28 +14:08:35.2 -- not an asteroid (will add it to exclusion list)
06:16:33.61 +12:04:50.5 -- not an asteroid (will add it to exclusion list)
06:16:52.29 +12:39:03.5 -- not an asteroid (will add it to exclusion list)
06:12:38.91 +10:38:15.1 -- not an asteroid (will add it to exclusion list)
06:23:40.76 +15:24:49.4 -- not an asteroid (will add it to exclusion list)
06:17:17.52 +12:47:01.7 -- not an asteroid (will add it to exclusion list)
06:15:19.32 +11:42:51.1 -- not an asteroid (will add it to exclusion list)
06:18:54.34 +12:57:04.2 -- not an asteroid (will add it to exclusion list)
06:17:56.94 +13:25:25.8 -- not an asteroid (will add it to exclusion list)
06:21:05.47 +16:15:55.8 -- not an asteroid (will add it to exclusion list)
06:21:58.43 +14:41:52.6 -- not an asteroid (will add it to exclusion list)
06:20:17.27 +14:02:56.0 -- not an asteroid (will add it to exclusion list)
06:22:22.80 +15:58:11.2 -- not an asteroid (will add it to exclusion list)
06:23:51.74 +15:29:02.6 -- not an asteroid (will add it to exclusion list)
06:26:02.18 +15:41:17.8 -- not an asteroid (will add it to exclusion list)
06:21:06.61 +12:02:31.3 -- not an asteroid (will add it to exclusion list)
06:15:56.08 +12:04:47.7 -- not an asteroid (will add it to exclusion list)
06:16:21.84 +12:41:45.6 -- not an asteroid (will add it to exclusion list)
06:18:23.21 +14:09:23.0 -- not an asteroid (will add it to exclusion list)
06:15:56.88 +12:26:49.5 -- not an asteroid (will add it to exclusion list)
06:24:06.45 +17:23:48.7 -- not an asteroid (will add it to exclusion list)
06:17:33.94 +12:17:36.1 -- not an asteroid (will add it to exclusion list)
06:21:05.48 +15:36:17.8 -- not an asteroid (will add it to exclusion list)
06:19:52.72 +14:03:37.0 -- not an asteroid (will add it to exclusion list)
06:15:58.18 +11:56:55.9 -- not an asteroid (will add it to exclusion list)
06:21:36.02 +14:23:07.4 -- not an asteroid (will add it to exclusion list)
06:21:18.34 +13:50:32.3 -- not an asteroid (will add it to exclusion list)
06:19:41.09 +13:22:20.0 -- not an asteroid (will add it to exclusion list)
06:13:46.83 +11:22:34.6 -- not an asteroid (will add it to exclusion list)
06:21:12.39 +12:29:13.2 -- not an asteroid (will add it to exclusion list)
06:22:02.25 +14:28:25.0 -- not an asteroid (will add it to exclusion list)
06:21:22.94 +15:36:43.5 -- not an asteroid (will add it to exclusion list)
06:19:47.99 +13:27:05.8 -- not an asteroid (will add it to exclusion list)
06:14:41.90 +11:18:57.9 -- not an asteroid (will add it to exclusion list)
06:16:19.85 +12:10:09.7 -- not an asteroid (will add it to exclusion list)
06:22:23.94 +16:08:57.8 -- not an asteroid (will add it to exclusion list)
06:19:59.25 +13:26:56.2 -- not an asteroid (will add it to exclusion list)
06:15:34.93 +08:57:35.2 -- not an asteroid (will add it to exclusion list)
06:19:14.18 +12:05:39.4 -- not an asteroid (will add it to exclusion list)
06:22:36.37 +14:50:32.6 -- not an asteroid (will add it to exclusion list)
06:23:38.45 +16:21:05.8 -- not an asteroid (will add it to exclusion list)
06:18:20.23 +13:57:36.2 -- not an asteroid (will add it to exclusion list)
06:23:02.60 +15:01:17.7 -- not an asteroid (will add it to exclusion list)
06:24:18.82 +17:36:38.1 -- not an asteroid (will add it to exclusion list)
06:22:51.88 +15:19:35.5 -- not an asteroid (will add it to exclusion list)
06:21:42.82 +14:02:36.5 -- not an asteroid (will add it to exclusion list)
06:21:26.68 +14:52:43.1 -- not an asteroid (will add it to exclusion list)
06:19:06.89 +13:31:29.1 -- not an asteroid (will add it to exclusion list)
06:16:27.39 +12:55:00.2 -- not an asteroid (will add it to exclusion list)
06:17:13.93 +12:57:00.4 -- not an asteroid (will add it to exclusion list)
06:20:36.88 +14:59:16.1 -- not an asteroid (will add it to exclusion list)
06:19:39.31 +13:12:58.5 -- not an asteroid (will add it to exclusion list)
06:24:36.07 +15:32:08.2 -- not an asteroid (will add it to exclusion list)
06:20:06.84 +13:21:31.0 -- not an asteroid (will add it to exclusion list)
06:21:02.86 +13:58:55.2 -- not an asteroid (will add it to exclusion list)
06:18:17.29 +13:14:30.7 -- not an asteroid (will add it to exclusion list)
06:18:59.71 +11:41:49.2 -- not an asteroid (will add it to exclusion list)
06:15:58.94 +12:04:19.7 -- not an asteroid (will add it to exclusion list)
06:22:01.48 +15:05:42.4 -- not an asteroid (will add it to exclusion list)
06:14:14.37 +11:35:24.1 -- not an asteroid (will add it to exclusion list)
06:17:04.67 +13:15:59.3 -- not an asteroid (will add it to exclusion list)
06:16:37.12 +11:38:33.8 -- not an asteroid (will add it to exclusion list)
06:22:03.80 +14:30:06.5 -- not an asteroid (will add it to exclusion list)
06:15:40.38 +12:19:06.2 -- not an asteroid (will add it to exclusion list)
06:19:37.86 +13:54:56.6 -- not an asteroid (will add it to exclusion list)
06:17:31.32 +12:40:45.1 -- not an asteroid (will add it to exclusion list)
06:16:05.49 +11:27:27.2 -- not an asteroid (will add it to exclusion list)
06:22:12.45 +17:01:24.1 -- not an asteroid (will add it to exclusion list)
06:20:37.32 +14:08:16.7 -- not an asteroid (will add it to exclusion list)
06:22:11.41 +14:25:20.7 -- not an asteroid (will add it to exclusion list)
06:17:11.53 +12:44:29.7 -- not an asteroid (will add it to exclusion list)
06:21:11.60 +14:23:30.8 -- not an asteroid (will add it to exclusion list)
06:14:55.53 +11:52:39.1 -- not an asteroid (will add it to exclusion list)
06:14:21.80 +11:39:10.0 -- not an asteroid (will add it to exclusion list)
06:21:00.31 +13:51:48.9 -- not an asteroid (will add it to exclusion list)
05:42:52.71 +16:12:45.0 -- not an asteroid (will add it to exclusion list)
06:16:05.47 +12:14:58.6 -- not an asteroid (will add it to exclusion list)
06:20:08.32 +14:28:04.8 -- not an asteroid (will add it to exclusion list)
06:20:13.32 +14:22:12.0 -- not an asteroid (will add it to exclusion list)
06:14:39.77 +09:56:55.2 -- not an asteroid (will add it to exclusion list)
06:21:57.52 +16:30:57.4 -- not an asteroid (will add it to exclusion list)
06:12:17.54 +09:21:02.5 -- not an asteroid (will add it to exclusion list)
06:14:44.26 +10:32:56.3 -- not an asteroid (will add it to exclusion list)
06:28:20.97 +17:32:35.3 -- not an asteroid (will add it to exclusion list)
06:13:45.34 +11:31:40.2 -- not an asteroid (will add it to exclusion list)
06:33:59.97 +15:17:02.2 -- not an asteroid (will add it to exclusion list)
06:14:55.33 +10:20:22.7 -- not an asteroid (will add it to exclusion list)
06:15:54.47 +10:33:56.7 -- not an asteroid (will add it to exclusion list)
06:18:14.34 +11:20:45.1 -- not an asteroid (will add it to exclusion list)
06:19:51.02 +13:36:19.2 -- not an asteroid (will add it to exclusion list)
06:18:42.63 +13:02:54.4 -- not an asteroid (will add it to exclusion list)
06:18:05.68 +12:22:21.5 -- not an asteroid (will add it to exclusion list)
06:14:42.50 +11:28:07.8 -- not an asteroid (will add it to exclusion list)
06:12:28.76 +10:28:25.6 -- not an asteroid (will add it to exclusion list)
06:16:06.52 +10:56:43.1 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
05:42:52.71 +16:12:45.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:58:59.97 +09:16:46.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:12:17.54 +09:21:02.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:12:25.54 +10:30:59.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:12:28.76 +10:28:25.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:12:38.91 +10:38:15.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:13:45.34 +11:31:40.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:13:46.83 +11:22:34.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:14:14.37 +11:35:24.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:14:21.80 +11:39:10.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:14:39.77 +09:56:55.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:14:41.90 +11:18:57.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:14:42.50 +11:28:07.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:14:44.26 +10:32:56.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:14:55.33 +10:20:22.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:14:55.53 +11:52:39.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:15:15.56 +12:02:24.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:15:19.32 +11:42:51.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:15:34.93 +08:57:35.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:15:40.38 +12:19:06.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:15:54.47 +10:33:56.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:15:56.08 +12:04:47.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:15:56.88 +12:26:49.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:15:58.18 +11:56:55.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:15:58.94 +12:04:19.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:16:05.47 +12:14:58.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:16:05.49 +11:27:27.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:16:06.52 +10:56:43.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:16:19.85 +12:10:09.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:16:21.84 +12:41:45.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:16:27.39 +12:55:00.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:16:33.61 +12:04:50.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:16:37.12 +11:38:33.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:16:52.29 +12:39:03.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:16:58.38 +12:25:08.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:17:04.67 +13:15:59.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:17:11.53 +12:44:29.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:17:13.93 +12:57:00.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:17:17.52 +12:47:01.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:17:31.32 +12:40:45.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:17:33.94 +12:17:36.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:17:36.16 +13:06:06.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:17:56.94 +13:25:25.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:18:03.95 +13:30:16.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:18:05.68 +12:22:21.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:18:14.34 +11:20:45.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:18:17.29 +13:14:30.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:18:20.23 +13:57:36.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:18:23.21 +14:09:23.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:18:42.63 +13:02:54.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:18:54.34 +12:57:04.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:18:59.71 +11:41:49.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:19:06.89 +13:31:29.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:19:14.18 +12:05:39.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:19:37.86 +13:54:56.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:19:39.31 +13:12:58.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:19:41.09 +13:22:20.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:19:44.97 +14:56:40.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:19:47.99 +13:27:05.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:19:51.02 +13:36:19.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:19:52.72 +14:03:37.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:19:59.25 +13:26:56.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:20:06.84 +13:21:31.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:20:08.32 +14:28:04.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:20:10.05 +13:20:58.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:20:13.32 +14:22:12.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:20:17.27 +14:02:56.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:20:36.88 +14:59:16.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:20:37.32 +14:08:16.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:20:56.55 +15:15:27.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:21:00.31 +13:51:48.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:21:02.86 +13:58:55.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:21:05.47 +16:15:55.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:21:05.48 +15:36:17.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:21:06.61 +12:02:31.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:21:10.22 +12:58:17.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:21:11.60 +14:23:30.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:21:12.39 +12:29:13.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:21:18.34 +13:50:32.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:21:22.94 +15:36:43.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:21:26.68 +14:52:43.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:21:34.28 +14:08:35.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:21:36.02 +14:23:07.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:21:42.82 +14:02:36.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:21:57.52 +16:30:57.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:21:58.43 +14:41:52.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:22:01.48 +15:05:42.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:22:02.25 +14:28:25.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:22:03.80 +14:30:06.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:22:11.41 +14:25:20.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:22:12.45 +17:01:24.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:22:22.80 +15:58:11.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:22:23.94 +16:08:57.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:22:27.61 +16:05:21.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:22:36.37 +14:50:32.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:22:51.88 +15:19:35.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:23:02.60 +15:01:17.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:23:38.45 +16:21:05.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:23:40.76 +15:24:49.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:23:51.74 +15:29:02.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:24:06.45 +17:23:48.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:24:18.82 +17:36:38.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:24:36.07 +15:32:08.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:24:38.86 +15:35:16.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:24:56.21 +14:49:23.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:26:02.18 +15:41:17.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:26:21.49 +15:58:57.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:28:20.97 +17:32:35.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:33:59.97 +15:17:02.2 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
05:42:52.71 +16:12:45.0 -- not a known variable star
05:58:59.97 +09:16:46.1 -- a known variable star
06:12:17.54 +09:21:02.5 -- a known variable star
06:12:25.54 +10:30:59.9 -- a known variable star
06:12:28.76 +10:28:25.6 -- a known variable star
06:12:38.91 +10:38:15.1 -- a known variable star
06:13:45.34 +11:31:40.2 -- a known variable star
06:13:46.83 +11:22:34.6 -- not a known variable star
06:14:14.37 +11:35:24.1 -- not a known variable star
06:14:21.80 +11:39:10.0 -- not a known variable star
06:14:39.77 +09:56:55.2 -- a known variable star
06:14:41.90 +11:18:57.9 -- not a known variable star
06:14:42.50 +11:28:07.8 -- a known variable star
06:14:44.26 +10:32:56.3 -- a known variable star
06:14:55.33 +10:20:22.7 -- a known variable star
06:14:55.53 +11:52:39.1 -- not a known variable star
06:15:15.56 +12:02:24.1 -- not a known variable star
06:15:19.32 +11:42:51.1 -- not a known variable star
06:15:34.93 +08:57:35.2 -- a known variable star
06:15:40.38 +12:19:06.2 -- a known variable star
06:15:54.47 +10:33:56.7 -- a known variable star
06:15:56.08 +12:04:47.7 -- not a known variable star
06:15:56.88 +12:26:49.5 -- not a known variable star
06:15:58.18 +11:56:55.9 -- not a known variable star
06:15:58.94 +12:04:19.7 -- a known variable star
06:16:05.47 +12:14:58.6 -- not a known variable star
06:16:05.49 +11:27:27.2 -- not a known variable star
06:16:06.52 +10:56:43.1 -- a known variable star
06:16:19.85 +12:10:09.7 -- not a known variable star
06:16:21.84 +12:41:45.6 -- not a known variable star
06:16:27.39 +12:55:00.2 -- a known variable star
06:16:33.61 +12:04:50.5 -- not a known variable star
06:16:37.12 +11:38:33.8 -- not a known variable star
06:16:52.29 +12:39:03.5 -- a known variable star
06:16:58.38 +12:25:08.5 -- not a known variable star
06:17:04.67 +13:15:59.3 -- not a known variable star
06:17:11.53 +12:44:29.7 -- not a known variable star
06:17:13.93 +12:57:00.4 -- not a known variable star
06:17:17.52 +12:47:01.7 -- not a known variable star
06:17:31.32 +12:40:45.1 -- not a known variable star
06:17:33.94 +12:17:36.1 -- a known variable star
06:17:36.16 +13:06:06.3 -- not a known variable star
06:17:56.94 +13:25:25.8 -- not a known variable star
06:18:03.95 +13:30:16.6 -- not a known variable star
06:18:05.68 +12:22:21.5 -- a known variable star
06:18:14.34 +11:20:45.1 -- a known variable star
06:18:17.29 +13:14:30.7 -- not a known variable star
06:18:20.23 +13:57:36.2 -- a known variable star
06:18:23.21 +14:09:23.0 -- a known variable star
06:18:42.63 +13:02:54.4 -- a known variable star
06:18:54.34 +12:57:04.2 -- a known variable star
06:18:59.71 +11:41:49.2 -- a known variable star
06:19:06.89 +13:31:29.1 -- not a known variable star
06:19:14.18 +12:05:39.4 -- not a known variable star
06:19:37.86 +13:54:56.6 -- not a known variable star
06:19:39.31 +13:12:58.5 -- not a known variable star
06:19:41.09 +13:22:20.0 -- not a known variable star
06:19:44.97 +14:56:40.9 -- not a known variable star
06:19:47.99 +13:27:05.8 -- not a known variable star
06:19:51.02 +13:36:19.2 -- a known variable star
06:19:52.72 +14:03:37.0 -- not a known variable star
06:19:59.25 +13:26:56.2 -- not a known variable star
06:20:06.84 +13:21:31.0 -- not a known variable star
06:20:08.32 +14:28:04.8 -- not a known variable star
06:20:10.05 +13:20:58.6 -- not a known variable star
06:20:13.32 +14:22:12.0 -- a known variable star
06:20:17.27 +14:02:56.0 -- a known variable star
06:20:36.88 +14:59:16.1 -- not a known variable star
06:20:37.32 +14:08:16.7 -- a known variable star
06:20:56.55 +15:15:27.3 -- not a known variable star
06:21:00.31 +13:51:48.9 -- not a known variable star
06:21:02.86 +13:58:55.2 -- not a known variable star
06:21:05.47 +16:15:55.8 -- a known variable star
06:21:05.48 +15:36:17.8 -- not a known variable star
06:21:06.61 +12:02:31.3 -- a known variable star
06:21:10.22 +12:58:17.9 -- not a known variable star
06:21:11.60 +14:23:30.8 -- not a known variable star
06:21:12.39 +12:29:13.2 -- a known variable star
06:21:18.34 +13:50:32.3 -- not a known variable star
06:21:22.94 +15:36:43.5 -- not a known variable star
06:21:26.68 +14:52:43.1 -- not a known variable star
06:21:34.28 +14:08:35.2 -- not a known variable star
06:21:36.02 +14:23:07.4 -- not a known variable star
06:21:42.82 +14:02:36.5 -- not a known variable star
06:21:57.52 +16:30:57.4 -- a known variable star
06:21:58.43 +14:41:52.6 -- not a known variable star
06:22:01.48 +15:05:42.4 -- not a known variable star
06:22:02.25 +14:28:25.0 -- not a known variable star
06:22:03.80 +14:30:06.5 -- not a known variable star
06:22:11.41 +14:25:20.7 -- a known variable star
06:22:12.45 +17:01:24.1 -- not a known variable star
06:22:22.80 +15:58:11.2 -- not a known variable star
06:22:23.94 +16:08:57.8 -- not a known variable star
06:22:27.61 +16:05:21.6 -- not a known variable star
06:22:36.37 +14:50:32.6 -- not a known variable star
06:22:51.88 +15:19:35.5 -- a known variable star
06:23:02.60 +15:01:17.7 -- not a known variable star
06:23:38.45 +16:21:05.8 -- a known variable star
06:23:40.76 +15:24:49.4 -- not a known variable star
06:23:51.74 +15:29:02.6 -- not a known variable star
06:24:06.45 +17:23:48.7 -- a known variable star
06:24:18.82 +17:36:38.1 -- a known variable star
06:24:36.07 +15:32:08.2 -- a known variable star
06:24:38.86 +15:35:16.9 -- a known variable star
06:24:56.21 +14:49:23.4 -- a known variable star
06:26:02.18 +15:41:17.8 -- not a known variable star
06:26:21.49 +15:58:57.2 -- a known variable star
06:28:20.97 +17:32:35.3 -- a known variable star
06:33:59.97 +15:17:02.2 -- a known variable star
Found 65 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
109 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 109 (excluding asteroids and hot pixels, 65 new), not updating the exclusion list!
###################################################################################
Not allowed to update the exclusion list IS_THIS_TEST_RUN=NO ALLOW_EXCLUSION_LIST_UPDATE= NO
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461274.90002491 -observatory V36
09:45:33.98 +15:17:16.6 Mercury (-1.7mag)
12:50:21.06 -07:47:49.3 Venus (-4.5mag)
06:29:59.62 +23:38:56.7 Mars (1.3mag)
08:55:32.31 +17:52:54.9 Jupiter (-1.8mag)
00:54:48.82 +03:01:29.2 Saturn (0.5mag)
04:13:02.44 +21:00:19.7 Uranus (5.7mag)
00:15:07.80 +00:06:15.1 Neptune (7.7mag)
20:26:50.39 -23:35:12.9 Pluto (14.5mag)
17:29:33.02 -28:25:08.8 Moon (-11.0mag)
-rw-r--r-- 1 apache apache 363 Aug 22 04:40 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461274.90002491:
08:55:35.06 +17:52:42.3 Io (6.1mag)
08:55:40.29 +17:52:18.8 Europa (6.3mag)
08:55:48.63 +17:51:40.6 Ganymede (5.6mag)
08:55:13.23 +17:54:24.7 Callisto (6.9mag)
08:53:00.55 +18:00:56.9 Himalia (15.7mag)
08:55:30.57 +17:53:03.6 Thebe (16.6mag)
08:52:39.80 +17:56:48.7 Elara (17.7mag)
08:59:39.89 +17:26:09.2 Pasiphae (17.9mag)
08:57:45.25 +18:06:30.7 Carme (19.0mag)
00:54:44.99 +03:01:54.6 Titan (8.4mag)
00:54:53.39 +03:01:20.9 Rhea (9.7mag)
00:55:24.28 +03:03:10.5 Iapetus (11.1mag)
00:54:56.49 +03:01:46.2 Hyperion (14.4mag)
00:53:53.54 +02:52:54.2 Phoebe (16.4mag)
-rw-r--r-- 1 apache apache 568 Aug 22 04:41 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461274.90002491:
20:12:01.92 -14:00:58.7 JWST
17:38:37.51 +34:04:13.0 Chandra
11:35:47.72 -60:51:32.7 XMM-Newton
-rw-r--r-- 1 apache apache 96 Aug 22 04:40 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461274.90002491 -observatory V36
03:28:17.66 +18:26:39.1 17.5mag P/1996 R2 (Lagerkvist)
17:59:54.67 -34:28:32.5 14.2mag P/2010 H2 (Vales)
07:06:32.58 -69:29:32.4 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
06:13:09.14 +33:18:30.8 17.7mag C/2017 K2 (PANSTARRS)
04:21:12.77 +42:25:10.7 17.5mag P/2021 N1 (ZTF)
22:26:41.64 +30:22:25.8 17.4mag C/2022 E2 (ATLAS)
06:56:57.05 +26:16:57.7 16.8mag C/2022 N2 (PANSTARRS)
10:34:44.90 +27:51:00.8 17.0mag C/2022 QE78 (ATLAS)
09:38:19.93 +05:17:59.1 18.0mag C/2022 R6 (PANSTARRS)
15:15:40.66 -12:52:48.6 18.0mag P/2023 B1 (PANSTARRS)
20:53:23.12 +64:03:50.0 18.0mag C/2023 H5 (Lemmon)
15:36:27.33 -14:14:13.0 14.6mag C/2023 R1 (PANSTARRS)
08:23:18.24 +32:00:53.3 15.5mag C/2024 E1 (Wierzchos)
15:05:42.19 +15:30:14.6 17.8mag C/2024 G6 (ATLAS)
18:46:48.75 +43:29:22.8 13.7mag C/2024 J3 (ATLAS)
20:49:20.65 +49:41:19.5 17.5mag C/2024 R4 (PANSTARRS)
05:25:47.51 -12:53:57.9 15.3mag C/2024 T5 (ATLAS)
07:04:38.04 +21:35:58.1 17.9mag C/2025 J1 (Borisov)
10:53:20.00 +19:57:17.5 17.1mag C/2025 V2 (Rankin)
13:07:25.57 +01:21:03.9 16.9mag C/2025 Y1 (ATLAS)
16:10:32.89 +76:17:03.5 16.5mag C/2026 A2 (Bok)
03:09:55.46 +46:20:59.7 17.3mag C/2026 B2 (Sun-Gao)
11:58:53.52 +09:55:54.5 17.4mag A/2026 E1
22:12:26.37 -32:18:50.4 7.1mag 10P/Tempel
11:37:44.94 -04:19:24.7 16.3mag 29P/Schwassmann-Wachmann
11:36:29.91 +00:00:36.8 17.4mag 63P/Wild
00:51:36.70 -06:06:18.0 15.4mag 65P/Gunn
06:06:52.35 +20:14:27.8 13.7mag 78P/Gehrels
20:25:47.87 -25:00:11.7 17.5mag 84P/Giclas
03:12:01.21 +14:32:21.0 16.9mag 88P/Howell
08:30:36.28 +25:34:47.3 16.4mag 93P/Lovas
04:47:41.81 +22:25:47.2 17.2mag 112P/Urata-Niijima
06:42:41.94 +28:17:25.3 16.1mag 114P/Wiseman-Skiff
09:51:44.93 +24:05:10.1 14.9mag 123P/West-Hartley
12:12:36.48 -15:37:15.1 17.3mag 124P/Mrkos
05:56:48.60 +21:01:43.0 16.0mag 128P/Shoemaker-Holt
06:52:01.07 +18:05:53.6 17.9mag 131P/Mueller
23:59:36.56 +03:05:56.7 17.4mag 139P/Vaisala-Oterma
03:09:34.18 -18:37:29.7 12.8mag 161P/Hartley-IRAS
08:03:45.05 +38:07:18.0 16.1mag 162P/Siding Spring
11:03:44.89 +29:52:25.5 12.2mag 169P/NEAT
03:06:14.29 +09:23:35.4 17.6mag 220P/McNaught
20:16:20.15 -51:48:15.5 18.0mag 259P/Garradd
04:03:23.38 +30:50:42.4 15.3mag 260P/McNaught
07:47:25.56 +37:05:08.0 17.3mag 295P/LINEAR
15:16:12.46 +01:33:00.2 17.8mag 391P/Kowalski
09:13:45.19 +17:39:56.6 17.9mag 450P/LONEOS
-rw-r--r-- 1 apache apache 2.3K Aug 22 04:40 comets.txt
############################################################
List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
21:28:47.85 +20:31:03.60 SN 2026sfn 2026-08-16.3 17.09
23:01:28.67 -61:00:39.00 SN 2026yib 2026-08-14.85 17.36
00:22:23.20 -32:16:02.70 SN 2026whu 2026-08-14.96 16.5
19:56:21.71 -37:24:19.90 ASASSN-26ew 2026-08-13.82 14.73
13:53:14.21 +00:26:52.00 SN 2026wkv 2026-08-10.12 15.83
05:21:07.61 +23:38:20.10 TCP J05210763+2338194 2026-08-10.59 9.34
01:28:20.49 +40:13:27.10 SN2026wpd 2026-08-9.34 16.37
23:47:50.87 +49:28:49.80 SN2026wjs 2026-08-9.35 17.12
16:03:20.92 +17:43:23.70 AT2026xau 2026-08-9.3 17.71
01:10:22.05 -09:34:08.50 SN2026weo 2026-08-7.46 15.76
00:56:54.35 -35:55:29.40 AT2026wdy 2026-08-5.05 16.08
22:08:07.63 -53:03:58.90 AT2026wek 2026-08-3.82 17.17
14:51:51.34 +66:13:24.60 ASASSN-26ev 2026-08-2.15 14.02
12:06:50.79 -36:16:06.20 SN2026wgm 2026-08-1.73 15.61
16:56:36.90 -59:29:26.00 ASASSN-26er 2026-07-25.82 15.09
01:21:27.83 -10:37:05.00 SN2026vbh 2026-07-25.61 15.97
21:17:31.59 +22:25:50.90 ASASSN-26eq 2026-07-24.37 15.13
18:53:36.89 +16:56:43.60 ASASSN-26ep 2026-07-23.47 -4.06
12:18:47.98 -30:48:47.50 ASASSN-26et 2026-07-22.76 13.98
13:00:47.82 +15:42:17.60 SN2026uwk 2026-07-21.75 16.38
18:52:31.11 -32:28:00.90 ASASSN-26en 2026-07-21.77 14.63
14:42:58.01 -62:32:59.10 ASASSN-26es 2026-07-20.79 15.36
20:12:45.57 -32:53:13.00 ASASSN-26em 2026-07-20.94 16.83
18:54:24.33 -46:11:51.70 ASASSN-26eu 2026-07-20.93 14.86
03:18:56.99 -80:55:10.40 AT2026ugi 2026-07-20.03 17.12
18:43:58.40 +24:22:41.80 ASASSN-26eo 2026-07-19.36 16.16
04:50:01.03 -02:22:33.80 ASASSN-26ej 2026-07-16.17 17.02
18:34:55.28 -31:41:00.90 ASASSN-26ek 2026-07-16.24 15.73
17:07:43.61 -44:21:53.50 ASASSN-26el 2026-07-15.86 16.01
14:45:08.35 +24:13:12.30 ASASSN-26ei 2026-07-16.17 16.46
10:00:46.44 -32:36:31.10 AT 2023mhb 2026-07-14.73 16.67
14:39:37.45 -11:22:36.20 AT 2026unl 2026-07-15.27 17.11
10:49:42.57 -11:25:55.80 ASASSN-26eh 2026-07-14.72 16.58
19:33:53.06 -07:15:00.80 ASASSN-22le 2026-07-14.15 15.5
02:45:40.52 -27:55:30.30 ASASSN-26ef 2026-07-12.35 15.86
23:26:43.80 +04:42:39.70 SN 2026qtn 2026-07-12.22 16.47
02:19:17.26 +28:57:15.40 ASASSN-26ec 2026-07-11.53 2.78
18:31:15.56 -05:34:31.50 AT2026stb 2026-07-11.28 -1.29
13:36:08.24 +23:29:05.00 AT2026pjf 2026-07-10.18 -0.72
17:33:39.82 +04:22:36.70 SN2026pir 2026-07-9.86 -0.66
11:21:41.26 -50:33:36.30 ASASSN-26ed 2026-07-8.8 -1.3
23:41:42.11 +26:29:49.10 AT2026qil 2026-07-9.3 16.15
20:21:30.50 -32:03:40.10 ASASSN-26ee 2026-07-7.22 15.53
19:37:44.09 -05:35:42.80 AT2026ryu 2026-07-7.17 14.88
11:06:55.46 -04:07:04.50 AT2026qqg 2026-07-5.01 16.82
19:07:23.69 -74:13:37.30 AT2026qly 2026-07-5.02 17.31
17:57:43.80 +27:18:40.10 ASASSN-26ea 2026-07-5.07 16.67
19:59:01.43 -32:07:34.30 ASASSN-26eb 2026-07-4.97 15.52
18:46:50.35 -57:44:13.20 SN 2026qqp 2026-07-5.03 -0.92
19:17:31.69 -39:55:29.90 ASASSN-26dz 2026-07-5.14 15.91
19:14:31.37 +12:03:52.90 AT 2026rdg 2026-07-3.43 11.81
04:05:50.09 -70:24:34.40 AT 2026qpr 2026-06-30.4 15.96
13:45:37.49 -05:59:35.80 SN 2026pub 2026-06-30.09 16.01
16:41:15.63 +39:17:14.70 SN 2026pel 2026-06-26.38 16.07
10:14:40.19 -35:38:21.30 ASASSN-26dy 2026-06-25.99 15.63
14:47:21.56 -40:15:51.30 ASASSN-26dv 2026-06-23.03 14.62
13:38:49.79 -77:21:06.70 ASASSN-26dw 2026-06-23.04 16.09
00:59:27.90 +33:08:13.20 SN 2026mke 2026-06-22.39 17.13
11:10:44.73 -30:20:45.50 SN 2026nmv 2026-06-22.06 16.56
21:36:15.68 -21:19:12.50 AT2026oxh 2026-06-22.15 17.14
17:31:38.38 -56:05:51.90 ASASSN-26dx 2026-06-22.02 14.72
14:10:13.44 -38:46:46.10 AT2026pvk 2026-06-22.06 16.53
20:56:47.23 -18:31:05.20 AT2026plb 2026-06-21.31 16.4
15:44:29.68 +21:00:59.30 SN2026ore 2026-06-21.29 17.57
23:50:05.98 -14:01:41.30 AT2026oxl 2026-06-21.52 17.64
17:36:54.73 -18:10:04.20 AT2026ouj 2026-06-20.92 15.15
00:34:04.08 -30:22:09.20 AT2026ntk 2026-06-18.09 17.34
20:49:13.39 +25:17:59.20 ASASSN-26du 2026-06-15.39 15.93
23:09:30.84 +32:40:42.00 SN2026oxc 2026-06-14.35 16.83
02:02:26.67 +32:04:22.70 AT2026ovz 2026-06-14.6 15.52
21:26:28.11 -72:31:19.50 AT2026nwc 2026-06-11 17.05
17:54:57.33 +26:32:34.20 SN 2026odc 2026-06-11.23 17.62
13:55:59.94 +17:30:37.20 SN 2026nyq 2026-06-11.1 16.24
00:50:45.14 -71:38:36.90 ASASSN-26dt 2026-06-11.13 10.22
14:42:19.73 +19:11:35.60 SN2026nyp 2026-06-10.3 16.32
12:23:23.92 +12:56:43.50 SN2026mta 2026-06-8.29 16.69
12:30:18.51 +47:12:33.20 SN2026oao 2026-06-9.32 17.02
10:51:05.21 -42:28:56.60 AT2026nvf 2026-06-8.12 16.75
13:50:22.48 -07:35:00.00 SN2026npn 2026-06-8.02 17.58
00:56:07.17 +43:01:43.20 ASASSN-26dq 2026-06-7.43 13.58
01:07:49.46 +41:59:43.70 SN 2026obc 2026-06-7.43 15.15
21:11:25.22 +14:14:31.90 ASASSN-26dr 2026-06-7.24 16.24
06:21:27.06 -65:16:42.00 ASASSN-26ds 2026-06-2.97 15.02
20:07:38.15 -21:07:05.40 SN2026mho 2026-05-25.18 -1.12
11:29:42.55 +79:01:03.10 AT2026min 2026-05-24.21 16.63
11:44:33.11 -68:48:32.90 ASASSN-26no 2026-05-24.03 8.35
19:00:42.82 -48:31:01.60 ASASSN-26dp 2026-05-22.31 -3.28
14:23:56.72 -58:37:47.60 ASASSN-26dn 2026-05-20.01 14.64
11:24:54.06 +47:57:01.60 AT2026nma 2026-05-20.29 15.46
21:27:08.58 +33:24:38.10 AT2026lli 2026-05-19.34 15.86
00:31:01.41 -13:38:51.70 AT2026nad 2026-05-19.39 15.34
15:16:06.61 -79:16:32.40 ASASSN-26dm 2026-05-19.03 14.44
11:24:25.21 -59:23:19.10 ASASSN-26dl 2026-05-18.02 13.55
13:45:51.52 -53:16:01.00 ASASSN-26dk 2026-05-18.16 12.96
02:05:49.69 -30:29:09.60 ASASSN-26dh 2026-05-18.43 15.37
17:50:22.87 -39:42:33.90 ASASSN-26dj 2026-05-17.05 15.7
01:13:11.60 -33:25:16.10 ASASSN-26dg 2026-05-13.41 16.8
16:44:31.77 -27:15:18.40 AT2026mhn 2026-05-12.33 15.8
09:46:31.08 -33:41:51.00 ASASSN-26di 2026-05-12.14 14.63
21:23:11.57 -19:09:45.00 AT2026kwu 2026-05-12.26 16.9
-rw-r--r-- 1 apache apache 5.7K Aug 22 04:40 asassn_transients_list.txt
############################################################
Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
19:57:03.87 +37:41:46.4 TCP J19570387+3741464 2026-06-18.2638 17.5mag
00:42:32.04 +41:10:28.3 PNV J00423204+4110283 2026-06-26.059 16.6mag
02:19:17.36 +28:57:15.8 TCP J02191736+2857158 2026-07-12.3549 12.5mag
00:44:56.43 +41:57:41.6 PNV J00445643+4157416 2026-07-13.8026 17.98Cmag
00:42:55.36 +41:17:27.0 PNV J00425536+4117270 2026-07-20.1813 17.7mag
20:35:43.64 +61:31:32.9 TCP J20354364+6131329 2026-07-20.5443 14.4mag
21:17:31.48 +22:25:51.0 TCP J21173148+2225510 2026-07-23.5577 14.8mag
00:41:24.04 +40:49:02.8 PNV J00412404+4049028 2026-07-25.0157 18.7mag
00:43:04.26 +41:02:28.6 PNV J00430426+4102286 2026-07-26.1512 20mag
14:51:51.40 +66:13:24.0 TCP J14515140+6613240 2026-07-29.2561 13.5mag
00:43:06.15 +41:22:08.2 PNV J00430615+4122082 2026-07-30.0085 19.4mag
00:41:33.23 +41:10:12.2 PNV J00413323+4110122 2026-08-02.8913 17.1mag
05:21:07.63 +23:38:19.4 TCP J05210763+2338194 2026-08-06.4109 11.2mag
22:57:17.96 +47:07:41.8 TCP J22571796+4707418 2026-08-09.3289 14.3mag
09:13:38.17 +76:28:18.1 PSN J09133817+7628181 2026-08-09.8037 15.4mag
00:43:17.29 +41:26:48.6 PNV J00431729+4126486 2026-08-14.0920 16.8mag
00:42:52.82 +41:10:58.6 PNV J00425282+4110586 2026-08-17.7723 19.9mag
00:42:52.83 +41:10:59.6 PNV J00425283+4110596 2026-08-18.6119 19.3mag
18:25:12.76 -22:25:29.3 TCP J18251276-2225293 2026-08-19.1062 9.4mag
18:03:09.04 +12:18:14.0 TCP J18030904+1218140 2026-08-19.5199 14.9mag
-rw-r--r-- 1 apache apache 190K Aug 22 04:40 tocp_transients_list.txt
############################################################
Truncated list of recent TNS transients from https://www.wis-tns.org/ :
11:27:30.457 +02:47:32.36 AT 2026xfu 2026-01-14.53 21.69
17:59:19.284 +29:24:54.02 AT 2026xft 2026-07-18.43 20.84
19:54:12.936 -24:01:35.76 AT 2026xfs 2026-05-17.56 19.77
08:44:08.771 +29:07:45.05 AT 2026xfr 2026-01-14.38 20.4
23:28:59.311 -21:41:17.71 AT 2026xfq 2026-07-19.57 21.15
20:34:55.430 -31:12:10.98 AT 2026xfp 2026-07-14.44 20
13:01:30.092 +38:12:35.50 AT 2026xfo 2026-06-23.28 20.85
23:22:05.758 +18:57:29.94 AT 2026xfn 2026-07-25.52 21.28
10:13:35.246 -20:37:42.73 AT 2026xfm 2026-01-27.58 21
21:57:25.287 +03:48:20.98 AT 2026xfl 2026-07-16.55 21.68
14:26:07.382 +33:39:52.18 AT 2026xfk 2026-06-13.34 20.9
02:09:31.559 -03:10:04.80 AT 2026xfj 2026-01-17.24 21.98
20:17:01.562 -20:06:27.94 AT 2026xfi 2026-05-20.56 20.93
21:08:09.912 -21:12:24.85 AT 2026xfh 2026-06-19.58 20.9
20:08:20.135 -25:53:36.34 AT 2026xfg 2026-07-19.45 20.74
14:51:25.078 +41:07:07.07 AT 2026xff 2026-06-13.34 21.62
22:33:15.210 +12:04:33.49 AT 2026xfe 2026-06-21.53 20.23
13:52:05.795 +29:21:47.19 AT 2026xfd 2026-04-24.32 20.92
13:30:27.613 +10:38:39.93 AT 2026xfc 2026-04-20.32 21.07
13:40:18.442 +39:30:10.71 AT 2026xfb 2026-05-24.29 20.6
-rw-r--r-- 1 apache apache 87K Aug 22 04:40 tns_transients_list.txt
