This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Cam-11-Q2b1x1_233026_TTUQ2b1x1_3692653_JtedtbS7
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 09 07.1873 2461290.6873 12.13 04:18:53.58 +50:03:56.7
153.25610 -0.18054 galactic Per Second-epoch detections are separated by 0.8" and 5.1 pix
The object was found in VSX 1" ASASSN-V J041853.64+500356.6
Type: SR
# Max. Min./Amp. JD0 Period
14.670 g Y 0.310 g 2459530.86600 197.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:18:53.58 +50:03:56.7: 13.23 +/- 0.03 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:18:53.58 +50:03:56.7: 13.25 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.24 +/- 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 09 07.1873* 04 18 53.58 +50 03 56.7 12.1 U Per 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 J041853.64+500356.6,2461290.6873,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J041853.64+500356.6 20260907.1873 12.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1873 2461290.6873 12.58 04:29:24.59 +53:39:04.2
151.83836 3.49084 galactic Cam Second-epoch detections are separated by 1.0" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:29:24.59 +53:39:04.2 (user input) | T | P | (position from user input) J-Ks=1.076+/-0.032 (M)
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:29:24.59 +53:39:04.2: 13.53 +/- 0.03 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:29:24.59 +53:39:04.2: 13.52 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.52 +/- 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
target,2461290.6873,12.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1873 12.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1873 2461290.6873 12.65 04:30:39.30 +53:30:17.8
152.07200 3.52489 galactic Cam Second-epoch detections are separated by 1.6" and 4.8 pix
The object was found in VSX14" ZTF J043040.75+533012.1
Type: DSCT
# Max. Min./Amp. JD0 Period
16.810 r Y 0.063 r 2458437.84810 0.078880700000
ATTENTION: measured mag 12.65 is 4.1 mag brighter than the VSX record maximum brightness 16.75 - 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_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:30:39.30 +53:30:17.8: 13.55 +/- 0.03 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:30:39.30 +53:30:17.8: 13.55 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.55 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J043040.75+533012.1,2461290.6873,12.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J043040.75+533012.1 20260907.1873 12.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1873 2461290.6873 12.48 04:33:27.23 +53:17:58.9
152.50735 3.69032 galactic Cam Second-epoch detections are separated by 1.8" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J068.3638+53.2998 | 04:33:27.31 +53:17:59.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: K7 (LAMOST DR5) J-Ks=1.631+/-0.050 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:33:27.23 +53:17:58.9: 13.56 +/- 0.03 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:33:27.23 +53:17:58.9: 13.53 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.55 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J068.3638+53.2998,2461290.6873,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J068.3638+53.2998 20260907.1873 12.48CV 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 09 07.1873 2461290.6873 12.71 04:31:05.10 +53:04:07.7
152.43459 3.27323 galactic Cam Second-epoch detections are separated by 0.3" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:31:05.10 +53:04:07.7 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.421+/-0.032 (G)
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:31:05.10 +53:04:07.7: 13.63 +/- 0.03 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:31:05.10 +53:04:07.7: 13.66 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.64 +/- 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
target,2461290.6873,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1873 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1873 2461290.6873 12.80 04:39:29.12 +54:16:56.7
152.37453 5.00998 galactic Cam Second-epoch detections are separated by 0.5" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J069.8613+54.2790 | 04:39:29.12 +54:16:56.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.911+/-0.028 (M)
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:39:29.12 +54:16:56.7: 13.78 +/- 0.04 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:39:29.12 +54:16:56.7: 13.69 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.74 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J069.8613+54.2790,2461290.6873,12.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J069.8613+54.2790 20260907.1873 12.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1873 2461290.6873 12.90 04:43:11.56 +53:35:12.5
153.26072 4.96345 galactic Cam Second-epoch detections are separated by 1.1" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:43:11.56 +53:35:12.5 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=1.152+/-0.030 (M)
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:43:11.56 +53:35:12.5: 13.82 +/- 0.05 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:43:11.56 +53:35:12.5: 13.90 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.86 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6873,12.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1873 12.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1873 2461290.6873 12.83 04:36:24.01 +53:48:44.9
152.42343 4.35919 galactic Cam Second-epoch detections are separated by 1.0" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J069.1160+53.8146 | 04:36:24.01 +53:48:44.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=1.287+/-0.034 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:36:24.01 +53:48:44.9: 13.94 +/- 0.05 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:36:24.01 +53:48:44.9: 13.97 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.96 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J069.1160+53.8146,2461290.6873,12.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J069.1160+53.8146 20260907.1873 12.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1873 2461290.6873 12.86 04:39:20.49 +54:29:08.0
152.20780 5.12881 galactic Cam Second-epoch detections are separated by 1.1" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:39:20.49 +54:29:08.0 (user input) | T | P | (position from user input) J-Ks=1.519+/-0.028 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:39:20.49 +54:29:08.0: 13.90 +/- 0.05 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:39:20.49 +54:29:08.0: 13.87 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.88 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6873,12.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1873 12.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1873 2461290.6873 12.88 04:33:11.13 +54:16:34.9
151.76080 4.32344 galactic Cam Second-epoch detections are separated by 1.5" and 5.2 pix
The object was found in VSX 2" ZTF J043311.34+541635.1
Type: SR
# Max. Min./Amp. JD0 Period
13.040 r Y 0.388 r 2458453.41030 147.195209100000
The object was not found in astcheck.
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:33:11.13 +54:16:34.9: 13.94 +/- 0.05 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:33:11.13 +54:16:34.9: 13.87 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.90 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J043311.34+541635.1,2461290.6873,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J043311.34+541635.1 20260907.1873 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1873 2461290.6873 12.84 04:36:03.48 +54:48:22.0
151.65011 4.98827 galactic Cam Second-epoch detections are separated by 1.5" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 273996927551501312 | 04:36:03.48 +54:48:22.0 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) SpType: F5 (LAMOST DR5) J-Ks=0.529+/-0.031 (K)
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:36:03.48 +54:48:22.0: 13.90 +/- 0.04 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:36:03.48 +54:48:22.0: 13.86 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.88 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 273996927551501312,2461290.6873,12.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 273996927551501312 20260907.1873 12.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1873 2461290.6873 12.74 04:31:11.29 +53:10:36.0
152.36637 3.35828 galactic Cam Second-epoch detections are separated by 1.1" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:31:11.29 +53:10:36.0 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=1.214+/-0.028 (M)
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:31:11.29 +53:10:36.0: 13.88 +/- 0.04 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:31:11.29 +53:10:36.0: 13.84 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.86 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6873,12.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1873 12.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1873 2461290.6873 12.71 04:39:11.29 +53:33:23.8
152.89077 4.49613 galactic Cam Second-epoch detections are separated by 2.7" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:39:11.29 +53:33:23.8 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=1.165+/-0.033 (M)
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:39:11.29 +53:33:23.8: 13.85 +/- 0.05 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:39:11.29 +53:33:23.8: 13.74 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.79 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6873,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1873 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1873 2461290.6873 12.84 04:37:20.49 +54:06:13.4
152.29922 4.65696 galactic Cam Second-epoch detections are separated by 3.8" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:37:20.49 +54:06:13.4 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.947+/-0.027 (M)
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:37:20.49 +54:06:13.4: 13.82 +/- 0.04 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:37:20.49 +54:06:13.4: 13.84 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.83 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6873,12.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1873 12.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1873 2461290.6873 12.80 04:35:55.91 +53:50:20.2
152.35725 4.32570 galactic Cam Second-epoch detections are separated by 1.9" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:35:55.91 +53:50:20.2 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.769+/-0.033 (K)
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:35:55.91 +53:50:20.2: 13.78 +/- 0.04 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:35:55.91 +53:50:20.2: 13.76 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.77 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6873,12.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1873 12.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1873 2461290.6873 12.78 04:35:51.44 +53:22:45.2
152.69126 4.00870 galactic Cam Second-epoch detections are separated by 0.2" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:35:51.44 +53:22:45.2 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=1.084+/-0.035 (M)
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:35:51.44 +53:22:45.2: 13.75 +/- 0.04 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:35:51.44 +53:22:45.2: 13.84 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.79 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6873,12.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1873 12.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1873 2461290.6873 12.77 04:35:51.57 +53:29:14.9
152.61111 4.08168 galactic Cam Second-epoch detections are separated by 1.1" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:35:51.57 +53:29:14.9 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=1.253+/-0.035 (M)
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:35:51.57 +53:29:14.9: 13.71 +/- 0.04 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:35:51.57 +53:29:14.9: 13.70 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.71 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6873,12.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1873 12.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1873 2461290.6873 12.71 04:37:35.90 +53:38:10.4
152.67373 4.37304 galactic Cam Second-epoch detections are separated by 2.2" and 4.8 pix
The object was found in VSX 6" Gaia DR3 273655494832689280
Type: E
# Max. Min./Amp. JD0 Period
19.590 G 20.310 G 0.248587000000
ATTENTION: measured mag 12.71 is 6.9 mag brighter than the VSX record maximum brightness 19.59 - 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_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:37:35.90 +53:38:10.4: 13.69 +/- 0.04 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:37:35.90 +53:38:10.4: 13.64 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.67 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 273655494832689280,2461290.6873,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 273655494832689280 20260907.1873 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1873 2461290.6873 12.75 04:40:14.43 +54:03:27.5
152.61714 4.94423 galactic Cam Second-epoch detections are separated by 0.4" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J070.0600+54.0579 | 04:40:14.43 +54:03:27.5 (user input) | LPV (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.003+/-0.026 (M)
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:40:14.43 +54:03:27.5: 13.69 +/- 0.04 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:40:14.43 +54:03:27.5: 13.69 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.69 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J070.0600+54.0579,2461290.6873,12.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J070.0600+54.0579 20260907.1873 12.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1873 2461290.6873 12.63 04:31:48.95 +53:05:55.8
152.48772 3.37388 galactic Cam Second-epoch detections are separated by 2.8" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:31:48.95 +53:05:55.8 (user input) | T | P | (position from user input) SpType: K4 (LAMOST DR5) J-Ks=1.228+/-0.028 (M)
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:31:48.95 +53:05:55.8: 13.68 +/- 0.04 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:31:48.95 +53:05:55.8: 13.74 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.71 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6873,12.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1873 12.63CV 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 09 07.1873 2461290.6873 12.73 04:41:24.23 +55:49:20.6
151.39253 6.23142 galactic Cam Second-epoch detections are separated by 2.4" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J070.3507+55.8224 | 04:41:24.23 +55:49:20.6 (user input) | IRR (ATLAS) | (ATLAS) | (position from user input) SpType: M1 (LAMOST DR5) J-Ks=1.334+/-0.028 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:41:24.23 +55:49:20.6: 13.65 +/- 0.04 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:41:24.23 +55:49:20.6: 13.72 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.68 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J070.3507+55.8224,2461290.6873,12.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J070.3507+55.8224 20260907.1873 12.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1873 2461290.6873 12.56 04:30:05.72 +54:06:32.5
151.57445 3.87876 galactic Cam Second-epoch detections are separated by 1.9" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J067.5238+54.1089 | 04:30:05.72 +54:06:32.5 (user input) | MSINE (ATLAS) | (ATLAS) | (position from user input) SpType: K4 (LAMOST DR5) J-Ks=1.122+/-0.024 (M)
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:30:05.72 +54:06:32.5: 13.63 +/- 0.03 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:30:05.72 +54:06:32.5: 13.61 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.62 +/- 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 J067.5238+54.1089,2461290.6873,12.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J067.5238+54.1089 20260907.1873 12.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1873 2461290.6873 12.71 04:31:04.21 +53:44:06.1
151.94609 3.72723 galactic Cam Second-epoch detections are separated by 3.0" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J067.7678+53.7347 | 04:31:04.21 +53:44:06.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: M0 1971PROE....7...73N Edinburgh 2- 65 J-Ks=1.382+/-0.028 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:31:04.21 +53:44:06.1: 13.61 +/- 0.04 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:31:04.21 +53:44:06.1: 13.64 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.63 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J067.7678+53.7347,2461290.6873,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J067.7678+53.7347 20260907.1873 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1873 2461290.6873 12.69 04:33:52.14 +53:31:58.7
152.37738 3.89386 galactic Cam Second-epoch detections are separated by 0.1" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 273677583845860224 | 04:33:52.15 +53:31:59.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=1.799+/-0.042 (Very red!)
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:33:52.14 +53:31:58.7: 13.58 +/- 0.03 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:33:52.14 +53:31:58.7: 13.57 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.57 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 273677583845860224,2461290.6873,12.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 273677583845860224 20260907.1873 12.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1873 2461290.6873 12.54 04:30:17.10 +53:25:29.2
152.09267 3.42985 galactic Cam Second-epoch detections are separated by 2.6" and 4.8 pix
The object was found in VSX23" ZTF J043019.60+532526.7
Type: RS
# Max. Min./Amp. JD0 Period
16.754 r Y 0.069 r 2458526.69670 2.322078400000
ATTENTION: measured mag 12.54 is 4.1 mag brighter than the VSX record maximum brightness 16.69 - 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_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:30:17.10 +53:25:29.2: 13.57 +/- 0.03 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:30:17.10 +53:25:29.2: 13.58 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.58 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J043019.60+532526.7,2461290.6873,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J043019.60+532526.7 20260907.1873 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1873 2461290.6873 12.65 04:38:52.47 +53:06:38.6
153.19392 4.16502 galactic Cam Second-epoch detections are separated by 1.2" and 5.0 pix
The object was found in VSX18" Gaia DR3 272865255208388864
Type: E
# Max. Min./Amp. JD0 Period
17.540 G 18.210 G 0.373157000000
ATTENTION: measured mag 12.65 is 4.9 mag brighter than the VSX record maximum brightness 17.54 - 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_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:38:52.47 +53:06:38.6: 13.56 +/- 0.03 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:38:52.47 +53:06:38.6: 13.54 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.55 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 272865255208388864,2461290.6873,12.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 272865255208388864 20260907.1873 12.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1873 2461290.6873 12.57 04:39:21.95 +54:31:12.7
152.18409 5.15440 galactic Cam Second-epoch detections are separated by 1.0" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:39:21.95 +54:31:12.7 (user input) | T | P | (position from user input) SpType: M0 (LAMOST DR5) J-Ks=1.389+/-9.995 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:39:21.95 +54:31:12.7: 13.53 +/- 0.04 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:39:21.95 +54:31:12.7: 13.55 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.54 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6873,12.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1873 12.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1873 2461290.6873 12.57 04:31:52.78 +53:18:46.6
152.33739 3.52692 galactic Cam Second-epoch detections are separated by 1.6" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:31:52.78 +53:18:46.6 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.889+/-0.026 (M)
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:31:52.78 +53:18:46.6: 13.54 +/- 0.03 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:31:52.78 +53:18:46.6: 13.49 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.52 +/- 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
target,2461290.6873,12.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1873 12.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1873 2461290.6873 12.48 04:33:29.21 +53:12:27.7
152.57846 3.63157 galactic Cam Second-epoch detections are separated by 0.3" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:33:29.21 +53:12:27.7 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=1.132+/-0.029 (M)
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:33:29.21 +53:12:27.7: 13.53 +/- 0.03 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:33:29.21 +53:12:27.7: 13.56 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.54 +/- 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
target,2461290.6873,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1873 12.48CV 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 09 07.1873 2461290.6873 12.55 04:38:27.56 +53:12:38.2
153.07763 4.18499 galactic Cam Second-epoch detections are separated by 0.6" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:38:27.56 +53:12:38.2 (user input) | T | P | (position from user input) J-Ks=1.305+/-0.033 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:38:27.56 +53:12:38.2: 13.53 +/- 0.03 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:38:27.56 +53:12:38.2: 13.55 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.54 +/- 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
target,2461290.6873,12.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1873 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1873 2461290.6873 12.64 04:29:00.14 +53:27:22.7
151.93821 3.31280 galactic Cam Second-epoch detections are separated by 0.6" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J067.2509+53.4563 | 04:29:00.14 +53:27:22.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: M2 1971PROE....7...73N Edinburgh 2- 58 J-Ks=1.336+/-0.030 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:29:00.14 +53:27:22.7: 13.54 +/- 0.04 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:29:00.14 +53:27:22.7: 13.69 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.60 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J067.2509+53.4563,2461290.6873,12.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J067.2509+53.4563 20260907.1873 12.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1873 2461290.6873 12.56 04:33:27.63 +53:35:49.8
152.28887 3.89272 galactic Cam Second-epoch detections are separated by 0.6" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:33:27.63 +53:35:49.8 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=1.014+/-0.033 (M)
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:33:27.63 +53:35:49.8: 13.52 +/- 0.03 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:33:27.63 +53:35:49.8: 13.47 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.50 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6873,12.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1873 12.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1873 2461290.6873 12.55 04:28:25.52 +53:34:43.6
151.79012 3.33516 galactic Cam Second-epoch detections are separated by 1.3" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:28:25.52 +53:34:43.6 (user input) | T | P | (position from user input) J-Ks=0.848+/-0.032 (M)
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:28:25.52 +53:34:43.6: 13.49 +/- 0.03 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:28:25.52 +53:34:43.6: 13.59 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.53 +/- 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
target,2461290.6873,12.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1873 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1873 2461290.6873 12.54 04:31:25.09 +53:19:47.6
152.27786 3.48811 galactic Cam Second-epoch detections are separated by 1.9" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:31:25.09 +53:19:47.6 (user input) | T | P | (position from user input) SpType: G4 (LAMOST DR5) J-Ks=0.507+/-0.030 (K)
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:31:25.09 +53:19:47.6: 13.44 +/- 0.03 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:31:25.09 +53:19:47.6: 13.44 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.44 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6873,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1873 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1873 2461290.6873 12.45 04:23:52.85 +50:07:13.6
153.78407 0.42294 galactic Per Second-epoch detections are separated by 0.3" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J065.9695+50.1199 | 04:23:52.70 +50:07:11.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: M1 1971PROE....7...73N Edinburgh 2-159 J-Ks=1.558+/-0.051 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:23:52.85 +50:07:13.6: 13.43 +/- 0.03 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:23:52.85 +50:07:13.6: 13.44 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.43 +/- 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 09 07.1873* 04 23 52.85 +50 07 13.6 12.4 U Per 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 J065.9695+50.1199,2461290.6873,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J065.9695+50.1199 20260907.1873 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1873 2461290.6873 13.20 04:34:25.64 +53:39:30.5
152.34084 4.03975 galactic Cam Second-epoch detections are separated by 2.6" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:34:25.64 +53:39:30.5 (user input) | T | P | (position from user input) SpType: K7 (LAMOST DR5) J-Ks=1.317+/-0.034 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:34:25.64 +53:39:30.5: 14.60 +/- 0.08 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:34:25.64 +53:39:30.5: 14.62 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.61 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461290.6873,13.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260907.1873 13.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1873 2461290.6873 12.43 04:38:01.59 +54:35:35.9
151.99978 5.05774 galactic Cam Second-epoch detections are separated by 1.7" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 274022864854712704 | 04:38:01.62 +54:35:36.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: M5 (LAMOST DR5) J-Ks=1.398+/-0.030 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:38:01.59 +54:35:35.9: 13.38 +/- 0.03 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:38:01.59 +54:35:35.9: 13.54 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.45 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 274022864854712704,2461290.6873,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 274022864854712704 20260907.1873 12.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1873 2461290.6873 12.47 04:28:57.53 +53:41:52.5
151.75833 3.47458 galactic Cam Second-epoch detections are separated by 1.4" and 5.1 pix
The object was found in VSX 3" ASASSN-V J042857.43+534150.1
Type: EB
# Max. Min./Amp. JD0 Period
13.200 V 13.560 V 2457690.01000 2.553100000000
The object was not found in astcheck.
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:28:57.53 +53:41:52.5: 13.37 +/- 0.03 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:28:57.53 +53:41:52.5: 13.40 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J042857.43+534150.1,2461290.6873,12.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J042857.43+534150.1 20260907.1873 12.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1873 2461290.6873 12.29 04:35:14.27 +53:39:20.0
152.42418 4.12645 galactic Cam Second-epoch detections are separated by 1.0" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 273677205887445632 | 04:35:14.35 +53:39:20.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.354+/-0.030 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:35:14.27 +53:39:20.0: 13.27 +/- 0.02 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:35:14.27 +53:39:20.0: 13.25 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.26 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 273677205887445632,2461290.6873,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 273677205887445632 20260907.1873 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1873 2461290.6873 12.35 04:38:00.69 +54:11:33.3
152.29842 4.78932 galactic Cam Second-epoch detections are separated by 2.2" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 273822685018982656 | 04:38:00.75 +54:11:34.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K7 (LAMOST DR5) J-Ks=1.283+/-0.034 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:38:00.69 +54:11:33.3: 13.27 +/- 0.03 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:38:00.69 +54:11:33.3: 13.31 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.29 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 273822685018982656,2461290.6873,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 273822685018982656 20260907.1873 12.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1873 2461290.6873 12.28 04:37:42.27 +54:07:49.4
152.31491 4.71437 galactic Cam Second-epoch detections are separated by 2.2" and 4.8 pix
The object was found in VSX 0" ASASSN-V J043742.28+540749.6
Type: SR
# Max. Min./Amp. JD0 Period
13.650 V 14.240 V 2457638.10000 205.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:37:42.27 +54:07:49.4: 13.19 +/- 0.02 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:37:42.27 +54:07:49.4: 13.22 +/- 0.03 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J043742.28+540749.6,2461290.6873,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J043742.28+540749.6 20260907.1873 12.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.1873 2461290.6873 11.95 04:24:18.19 +50:11:02.0
153.78636 0.51565 galactic Per Second-epoch detections are separated by 3.5" and 5.2 pix
The object was found in VSX 3" ASASSN-V J042418.39+501059.9
Type: SR
# Max. Min./Amp. JD0 Period
13.440 V 13.750 V 2458495.53490 83.387209200000
The object was not found in astcheck.
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:24:18.19 +50:11:02.0: 12.96 +/- 0.02 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:24:18.19 +50:11:02.0: 12.92 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.94 +/- 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 09 07.1873* 04 24 18.19 +50 11 02.0 11.9 U Per 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 J042418.39+501059.9,2461290.6873,11.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J042418.39+501059.9 20260907.1873 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 09 07.1873 2461290.6873 11.99 04:34:30.24 +53:21:28.8
152.57067 3.84522 galactic Cam Second-epoch detections are separated by 0.0" and 5.0 pix
The object was found in VSX 1" ZTF J043430.35+532128.7
Type: SR
# Max. Min./Amp. JD0 Period
14.488 g Y 0.141 g 2458474.46050 262.692274200000
The object was not found in astcheck.
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:34:30.24 +53:21:28.8: 12.93 +/- 0.02 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:34:30.24 +53:21:28.8: 12.87 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.90 +/- 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
ZTF J043430.35+532128.7,2461290.6873,11.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J043430.35+532128.7 20260907.1873 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 09 07.1873 2461290.6873 13.06 04:41:46.24 +53:19:59.1
153.31389 4.63731 galactic Cam Second-epoch detections are separated by 1.8" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J070.4422+53.3329 | 04:41:46.24 +53:19:59.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: M4 (LAMOST DR5) J-Ks=1.600+/-0.030 (Very red! L if it's a dwarf)
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:41:46.24 +53:19:59.1: 14.27 +/- 0.07 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:41:46.24 +53:19:59.1: 14.31 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.29 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J070.4422+53.3329,2461290.6873,13.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J070.4422+53.3329 20260907.1873 13.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 3
Ref. image: 2461093.61077987 22.02.2026 02:39:21.381 /data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits
First image: 2461093.61077987 22.02.2026 02:39:21.381 /data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits
Last image: 2461290.68701756 07.09.2026 04:29:08.317 /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Cam-11-Q2b1x1_233026_TTUQ2b1x1_3692653_JtedtbS7/fd_Cam-11-Q2b1x1_2026-09-06_23-29-08_20.00sec_-0.00C_LIGHT_0151.fits
JD time system (TT/UTC/UNKNOWN): UTC
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.67
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 8 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): 12358
Objects passed selection criteria: 12249
Measurements per detected object (mean, median, min, max): 2.1 2.0 2 3
Measurements per selected object (mean, median, min, max): 2.1 2.0 2 3
Average stars detected per image: 9109.33
Average stars matched: 8777.67 (96.359 %)
Memory usage VmPeak: 239312 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Sep 2 15:05:04 CDT 2026
VaST build number 1.0rc89-201-ga7d4d23b
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-09-02)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Sep 6 23:58:31 CDT 2026
Host name: tau
***** IMAGE PROCESSING ERROR (less than 4 images processed) *****
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461093.61077987 22.02.2026 02:39:21.381 /data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits
First image: 2461093.61077987 22.02.2026 02:39:21.381 /data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits
Last image: 2461290.68750005 07.09.2026 04:29:50.004 /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Cam-11-Q2b1x1_233026_TTUQ2b1x1_3692653_JtedtbS7/fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 85
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.29
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: 87 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): 106505
Objects passed selection criteria: 106079
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: 63321.2
Average stars matched: 60164.8 (95.0151 %)
Memory usage VmPeak: 575072 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Sep 2 15:05:04 CDT 2026
VaST build number 1.0rc89-201-ga7d4d23b
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-09-02)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Sep 7 00:00:09 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/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Cam-11-Q2b1x1_233026_TTUQ2b1x1_3692653_JtedtbS7/fd_Cam-11-Q2b1x1_2026-09-06_23-29-08_20.00sec_-0.00C_LIGHT_0151.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Cam-11-Q2b1x1_233026_TTUQ2b1x1_3692653_JtedtbS7/fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152.fits
SExtractor catalog cache: saved Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits.cat to cache
SExtractor catalog cache: saved Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.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/Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Cam-11-Q2b1x1_233026_TTUQ2b1x1_3692653_JtedtbS7/fd_Cam-11-Q2b1x1_2026-09-06_23-29-08_20.00sec_-0.00C_LIGHT_0151.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Cam-11-Q2b1x1_233026_TTUQ2b1x1_3692653_JtedtbS7/fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152.fits
Last image: 2461290.68701756 07.09.2026 04:29:08.317 UTC
ERROR running VaST on the field Cam-11-Q2b1x1 (less than 4 images processed)
exp_start= 22.02.2026 02:39:21.381 exp= 20.000 JD= 2461093.61077987 ap= 6.0 rotation= 0.000 *detected= 13240 *matched= 13240 status=OK /data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits
exp_start= 22.02.2026 02:40:33.353 exp= 20.000 JD= 2461093.61161288 ap= 6.1 rotation= 0.010 *detected= 13210 *matched= 12356 status=OK /data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits
exp_start= 07.09.2026 04:29:08.317 exp= 20.000 JD= 2461290.68701756 ap= 6.1 rotation= -174.013 *detected= 878 *matched= 737 status=OK /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Cam-11-Q2b1x1_233026_TTUQ2b1x1_3692653_JtedtbS7/fd_Cam-11-Q2b1x1_2026-09-06_23-29-08_20.00sec_-0.00C_LIGHT_0151.fits
exp_start= 07.09.2026 04:29:50.004 exp= 20.000 JD= 2461290.68750005 ap= 6.1 rotation= -174.020 *detected= 898 *matched= 884 status=ERROR /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Cam-11-Q2b1x1_233026_TTUQ2b1x1_3692653_JtedtbS7/fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152.fits
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/Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Cam-11-Q2b1x1_233026_TTUQ2b1x1_3692653_JtedtbS7/fd_Cam-11-Q2b1x1_2026-09-06_23-29-08_20.00sec_-0.00C_LIGHT_0151.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Cam-11-Q2b1x1_233026_TTUQ2b1x1_3692653_JtedtbS7/fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152.fits
SExtractor catalog cache: saved Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits.cat to cache
SExtractor catalog cache: saved Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Cam-11-Q2b1x1_233026_TTUQ2b1x1_3692653_JtedtbS7/fd_Cam-11-Q2b1x1_2026-09-06_23-29-08_20.00sec_-0.00C_LIGHT_0151.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Cam-11-Q2b1x1_233026_TTUQ2b1x1_3692653_JtedtbS7/fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152.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: 2461290.68701756
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
'asassn_transients_list.txt' -> '../asassn_transients_list.txt'
wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits exists and is non-empty
wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits exists and is non-empty
wcs_fd_Cam-11-Q2b1x1_2026-09-06_23-29-08_20.00sec_-0.00C_LIGHT_0151.fits exists and is non-empty
wcs_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits (1st reference image)
verification OK: wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.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: 04:14:08.869 +53:59:58.47 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_Cam-11-Q2b1x1_2026-09-06_23-29-08_20.00sec_-0.00C_LIGHT_0151.fits (1st new image)
verification OK: wcs_fd_Cam-11-Q2b1x1_2026-09-06_23-29-08_20.00sec_-0.00C_LIGHT_0151.fits
Image size: 940.2'x624.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 04:14:09.633 +54:00:22.30 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 04:14:08.869 +53:59:58.47
Second-epoch image center 04:14:09.633 +54:00:22.30
Angular distance between the image centers 0.0069 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152.fits (2nd new image)
verification OK: wcs_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152.fits
Image size: 940.2'x624.5' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 04:14:11.393 +54:00:47.16 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 04:14:08.869 +53:59:58.47
Second-epoch image center 04:14:11.393 +54:00:47.16
Angular distance between the image centers 0.0149 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 04:14:09.633 +54:00:22.30
Second-epoch second image center 04:14:11.393 +54:00:47.16
Angular distance between the image centers 0.00814 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/Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits &> /tmp/tmp.x7vkDT0k2i
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits &> /tmp/tmp.vEQYJj1qL8
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Cam-11-Q2b1x1_233026_TTUQ2b1x1_3692653_JtedtbS7/fd_Cam-11-Q2b1x1_2026-09-06_23-29-08_20.00sec_-0.00C_LIGHT_0151.fits &> /tmp/tmp.hm8tm213zW
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Cam-11-Q2b1x1_233026_TTUQ2b1x1_3692653_JtedtbS7/fd_Cam-11-Q2b1x1_2026-09-06_23-29-08_20.00sec_-0.00C_LIGHT_0151.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Cam-11-Q2b1x1_233026_TTUQ2b1x1_3692653_JtedtbS7/fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152.fits &> /tmp/tmp.mi8vxm3iEV
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Cam-11-Q2b1x1_233026_TTUQ2b1x1_3692653_JtedtbS7/fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152.fits
Calibrating the magnitude scale
Found non-empty wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.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_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits and wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.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_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits and wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits.wcscat
Found non-empty wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits and wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits.wcscat
The reference image (wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits) and catalog (wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits.wcscat) found
'wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits.wcscat' -> 'wcsmag.cat'
Read 140708 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 48.9404 to 78.9609 deg, Dec +47.6949 to +59.3756 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 48.9404 to 78.9609 deg, Dec 47.6949 to 59.3756 deg
Loaded 11511 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): 5993 out of 8204 total matches.
Matched with Tycho-2 8204 out of 140708 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.786700
a=0.000000 b=1.000000 c=22.786700
From vast_summary.log: estimated ref. image limiting mag.: -7.29
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.50
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.50
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 140708 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 48.9404 to 78.9609 deg, Dec +47.6949 to +59.3756 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 48.9404 to 78.9609 deg, Dec 47.6949 to 59.3756 deg
Loaded 11511 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): 5993 out of 8204 total matches.
Matched with Tycho-2 8204 out of 140708 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits
Forced-photometry filter: calibrated wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits -> calib.txt_param_ref_wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits (aperture=4.4)
Read 140191 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 48.9776 to 78.9637 deg, Dec +47.6949 to +59.3671 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 48.9776 to 78.9637 deg, Dec 47.6949 to 59.3671 deg
Loaded 11495 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): 6007 out of 8204 total matches.
Matched with Tycho-2 8204 out of 140191 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits
Forced-photometry filter: calibrated wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits -> calib.txt_param_ref_wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits (aperture=4.4)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 74 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
1.9 pix Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits
1.9 pix Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits
2.2 pix fd_Cam-11-Q2b1x1_2026-09-06_23-29-08_20.00sec_-0.00C_LIGHT_0151.fits
2.1 pix fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152.fits
Limiting magnitude estimates:
15.5 mag. Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits
15.5 mag. Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits
13.1 mag. fd_Cam-11-Q2b1x1_2026-09-06_23-29-08_20.00sec_-0.00C_LIGHT_0151.fits
13.1 mag. fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152.fits
cp: cannot create regular file 'local_wcs_cache/': Not a directory
All-image limiting magnitude estimate: 13.1 (SNR ) 12.8 (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.x7vkDT0k2i (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-06_CI_Cam-11-Q2b1x1_233026_TTUQ2b1x1_3692653_JtedtbS7/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits' -> 'wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.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/Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits
WCS_IMAGE_NAME=wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits
WCS-calibrated image found: wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits
Checking if the catalog wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits.wcscat corresponding to the image wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits alredy exist and is non-empty...
Catalog wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits.wcscat corresponding to the image wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits
WCS catalog name: wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 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=34, blended=14794, bad_region=23405, passed=140674
Got 140674 stars (including 104482 good ones) from the SExtractor catalog wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits.wcscat
util/solve_plate_with_UCAC5 got 140674 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 688 to 748 (Dec 47.7 to 59.4)
Done reading UCAC5 zone files...
Matched 4918 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4899 matched stars entering correct_measured_positions(), 4899 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4899 matched stars entering correct_measured_positions(), 122370 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
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 688 to 748 (Dec 47.7 to 59.4)
Done reading UCAC5 zone files...
Matched 4918 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4898 matched stars entering correct_measured_positions(), 122370 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 4898 matched stars entering correct_measured_positions(), 122370 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 4898 stars left (next iteration limit 5388)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits N_match=4898 sigma_overall_arcsec=0.438 sigma_q1_arcsec=0.554 sigma_q2_arcsec=0.415 sigma_q3_arcsec=0.419 sigma_q4_arcsec=0.374 n_q1=1402 n_q2=838 n_q3=1597 n_q4=1061 worst_quadrant_to_overall_ratio=1.266
The image catalog is written to wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits -region wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.vEQYJj1qL8 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-06_CI_Cam-11-Q2b1x1_233026_TTUQ2b1x1_3692653_JtedtbS7/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits' -> 'wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.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/Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits
WCS_IMAGE_NAME=wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits
WCS-calibrated image found: wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits
Checking if the catalog wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits.wcscat corresponding to the image wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits alredy exist and is non-empty...
Catalog wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits.wcscat corresponding to the image wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits
WCS catalog name: wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 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=26, blended=14593, bad_region=23295, passed=140165
Got 140165 stars (including 104241 good ones) from the SExtractor catalog wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits.wcscat
util/solve_plate_with_UCAC5 got 140165 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (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 688 to 748 (Dec 47.7 to 59.4)
Done reading UCAC5 zone files...
Matched 4924 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4904 matched stars entering correct_measured_positions(), 4904 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4904 matched stars entering correct_measured_positions(), 121947 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
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 688 to 748 (Dec 47.7 to 59.4)
Done reading UCAC5 zone files...
Matched 4924 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4905 matched stars entering correct_measured_positions(), 121947 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 4905 matched stars entering correct_measured_positions(), 121947 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 4905 stars left (next iteration limit 5394)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits N_match=4905 sigma_overall_arcsec=0.431 sigma_q1_arcsec=0.535 sigma_q2_arcsec=0.425 sigma_q3_arcsec=0.412 sigma_q4_arcsec=0.366 n_q1=1401 n_q2=849 n_q3=1588 n_q4=1067 worst_quadrant_to_overall_ratio=1.241
The image catalog is written to wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits -region wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.hm8tm213zW (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_2026-09-06_CI_Cam-11-Q2b1x1_233026_TTUQ2b1x1_3692653_JtedtbS7/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Cam-11-Q2b1x1_233026_TTUQ2b1x1_3692653_JtedtbS7/fd_Cam-11-Q2b1x1_2026-09-06_23-29-08_20.00sec_-0.00C_LIGHT_0151.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Cam-11-Q2b1x1_233026_TTUQ2b1x1_3692653_JtedtbS7/fd_Cam-11-Q2b1x1_2026-09-06_23-29-08_20.00sec_-0.00C_LIGHT_0151.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Cam-11-Q2b1x1_233026_TTUQ2b1x1_3692653_JtedtbS7/fd_Cam-11-Q2b1x1_2026-09-06_23-29-08_20.00sec_-0.00C_LIGHT_0151.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Cam-11-Q2b1x1_233026_TTUQ2b1x1_3692653_JtedtbS7/fd_Cam-11-Q2b1x1_2026-09-06_23-29-08_20.00sec_-0.00C_LIGHT_0151.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Cam-11-Q2b1x1_233026_TTUQ2b1x1_3692653_JtedtbS7/fd_Cam-11-Q2b1x1_2026-09-06_23-29-08_20.00sec_-0.00C_LIGHT_0151.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_2026-09-06_CI_Cam-11-Q2b1x1_233026_TTUQ2b1x1_3692653_JtedtbS7/fd_Cam-11-Q2b1x1_2026-09-06_23-29-08_20.00sec_-0.00C_LIGHT_0151.fits
WCS_IMAGE_NAME=wcs_fd_Cam-11-Q2b1x1_2026-09-06_23-29-08_20.00sec_-0.00C_LIGHT_0151.fits
WCS-calibrated image found: wcs_fd_Cam-11-Q2b1x1_2026-09-06_23-29-08_20.00sec_-0.00C_LIGHT_0151.fits
Checking if the catalog wcs_fd_Cam-11-Q2b1x1_2026-09-06_23-29-08_20.00sec_-0.00C_LIGHT_0151.fits.wcscat corresponding to the image wcs_fd_Cam-11-Q2b1x1_2026-09-06_23-29-08_20.00sec_-0.00C_LIGHT_0151.fits alredy exist and is non-empty...
Catalog wcs_fd_Cam-11-Q2b1x1_2026-09-06_23-29-08_20.00sec_-0.00C_LIGHT_0151.fits.wcscat corresponding to the image wcs_fd_Cam-11-Q2b1x1_2026-09-06_23-29-08_20.00sec_-0.00C_LIGHT_0151.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cam-11-Q2b1x1_2026-09-06_23-29-08_20.00sec_-0.00C_LIGHT_0151.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Cam-11-Q2b1x1_233026_TTUQ2b1x1_3692653_JtedtbS7/fd_Cam-11-Q2b1x1_2026-09-06_23-29-08_20.00sec_-0.00C_LIGHT_0151.fits
WCS catalog name: wcs_fd_Cam-11-Q2b1x1_2026-09-06_23-29-08_20.00sec_-0.00C_LIGHT_0151.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 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=4, blended=416, bad_region=4478, passed=14731
Got 14731 stars (including 9988 good ones) from the SExtractor catalog wcs_fd_Cam-11-Q2b1x1_2026-09-06_23-29-08_20.00sec_-0.00C_LIGHT_0151.fits.wcscat
util/solve_plate_with_UCAC5 got 14731 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.2'
Seting catalog search parameters based on the expected field of view 940.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013058 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010447 (37.6 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 689 to 748 (Dec 47.9 to 59.3)
Done reading UCAC5 zone files...
Matched 4885 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4844 matched stars entering correct_measured_positions(), 4847 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4844 matched stars entering correct_measured_positions(), 11681 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 689 to 748 (Dec 47.9 to 59.3)
Done reading UCAC5 zone files...
Matched 4886 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4846 matched stars entering correct_measured_positions(), 11681 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
Accuracy estimation diagnostic: 4846 matched stars entering correct_measured_positions(), 11681 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
Excluding outliers - 4846 stars left (next iteration limit 5328)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4846 robust_rms=4.871 arcsec worst_quadrant_rms=13.297 arcsec
SIP_REFIT: SIP order 3 trial: matched=4846 robust_rms=0.803 arcsec worst_quadrant_rms=1.008 arcsec
SIP_REFIT: SIP order 5 trial: matched=4846 robust_rms=0.709 arcsec worst_quadrant_rms=0.855 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4846 robust_rms_before=1.761 arcsec robust_rms_before_corrected=0.726 arcsec robust_rms_after=0.709 arcsec worst_quadrant_rms_before=0.895 worst_quadrant_rms_after=0.855
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.895 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Cam-11-Q2b1x1_2026-09-06_23-29-08_20.00sec_-0.00C_LIGHT_0151.fits N_match=4846 sigma_overall_arcsec=0.717 sigma_q1_arcsec=0.748 sigma_q2_arcsec=0.691 sigma_q3_arcsec=0.896 sigma_q4_arcsec=0.621 n_q1=1239 n_q2=1713 n_q3=775 n_q4=1119 worst_quadrant_to_overall_ratio=1.250
The image catalog is written to wcs_fd_Cam-11-Q2b1x1_2026-09-06_23-29-08_20.00sec_-0.00C_LIGHT_0151.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cam-11-Q2b1x1_2026-09-06_23-29-08_20.00sec_-0.00C_LIGHT_0151.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Cam-11-Q2b1x1_233026_TTUQ2b1x1_3692653_JtedtbS7/fd_Cam-11-Q2b1x1_2026-09-06_23-29-08_20.00sec_-0.00C_LIGHT_0151.fits -region wcs_fd_Cam-11-Q2b1x1_2026-09-06_23-29-08_20.00sec_-0.00C_LIGHT_0151.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cam-11-Q2b1x1_2026-09-06_23-29-08_20.00sec_-0.00C_LIGHT_0151.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.mi8vxm3iEV (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_2026-09-06_CI_Cam-11-Q2b1x1_233026_TTUQ2b1x1_3692653_JtedtbS7/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Cam-11-Q2b1x1_233026_TTUQ2b1x1_3692653_JtedtbS7/fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Cam-11-Q2b1x1_233026_TTUQ2b1x1_3692653_JtedtbS7/fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Cam-11-Q2b1x1_233026_TTUQ2b1x1_3692653_JtedtbS7/fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Cam-11-Q2b1x1_233026_TTUQ2b1x1_3692653_JtedtbS7/fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Cam-11-Q2b1x1_233026_TTUQ2b1x1_3692653_JtedtbS7/fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152.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_2026-09-06_CI_Cam-11-Q2b1x1_233026_TTUQ2b1x1_3692653_JtedtbS7/fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152.fits
WCS_IMAGE_NAME=wcs_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152.fits
WCS-calibrated image found: wcs_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152.fits
Checking if the catalog wcs_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152.fits.wcscat corresponding to the image wcs_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152.fits alredy exist and is non-empty...
Catalog wcs_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152.fits.wcscat corresponding to the image wcs_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Cam-11-Q2b1x1_233026_TTUQ2b1x1_3692653_JtedtbS7/fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152.fits
WCS catalog name: wcs_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 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=2, blended=395, bad_region=4443, passed=14903
Got 14903 stars (including 10240 good ones) from the SExtractor catalog wcs_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152.fits.wcscat
util/solve_plate_with_UCAC5 got 14903 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.2'
Seting catalog search parameters based on the expected field of view 940.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013058 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010447 (37.6 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 689 to 748 (Dec 47.9 to 59.3)
Done reading UCAC5 zone files...
Matched 4883 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4838 matched stars entering correct_measured_positions(), 4839 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4838 matched stars entering correct_measured_positions(), 11894 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
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 689 to 748 (Dec 47.9 to 59.3)
Done reading UCAC5 zone files...
Matched 4884 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4838 matched stars entering correct_measured_positions(), 11894 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
Accuracy estimation diagnostic: 4838 matched stars entering correct_measured_positions(), 11894 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
Excluding outliers - 4838 stars left (next iteration limit 5321)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4838 robust_rms=4.908 arcsec worst_quadrant_rms=12.890 arcsec
SIP_REFIT: SIP order 3 trial: matched=4838 robust_rms=0.785 arcsec worst_quadrant_rms=0.995 arcsec
SIP_REFIT: SIP order 5 trial: matched=4838 robust_rms=0.692 arcsec worst_quadrant_rms=0.882 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4838 robust_rms_before=1.694 arcsec robust_rms_before_corrected=0.710 arcsec robust_rms_after=0.692 arcsec worst_quadrant_rms_before=0.886 worst_quadrant_rms_after=0.882
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.886 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152.fits N_match=4838 sigma_overall_arcsec=0.704 sigma_q1_arcsec=0.705 sigma_q2_arcsec=0.700 sigma_q3_arcsec=0.878 sigma_q4_arcsec=0.648 n_q1=1268 n_q2=1699 n_q3=737 n_q4=1134 worst_quadrant_to_overall_ratio=1.247
The image catalog is written to wcs_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Cam-11-Q2b1x1_233026_TTUQ2b1x1_3692653_JtedtbS7/fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152.fits -region wcs_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
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_Cam-11-Q2b1x1_2026-09-06_23-29-08_20.00sec_-0.00C_LIGHT_0151.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cam-11-Q2b1x1_2026-09-06_23-29-08_20.00sec_-0.00C_LIGHT_0151.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Cam-11-Q2b1x1_233026_TTUQ2b1x1_3692653_JtedtbS7/wcs_fd_Cam-11-Q2b1x1_2026-09-06_23-29-08_20.00sec_-0.00C_LIGHT_0151.fits'
Saving fully-calibrated image wcs_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Cam-11-Q2b1x1_233026_TTUQ2b1x1_3692653_JtedtbS7/wcs_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152.fits'
Preparing the HTML report for the field Cam-11-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:16:35.52 +52:58:44.7: 11.63 +/- 0.01 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:43:04.49 +57:12:07.6: 12.45 +/- 0.02 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:24:10.75 +53:30:25.9: 12.49 +/- 0.02 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:19:29.69 +50:14:48.9: 12.91 +/- 0.02 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:18:53.58 +50:03:56.7: 13.23 +/- 0.03 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:30:39.30 +53:30:17.8: 13.55 +/- 0.03 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:43:04.49 +57:12:07.6: 12.43 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.44 +/- 0.01
Forced photometry filter REJECTED candidate at 04:43:04.49 +57:12:07.6: ref_mag=12.44 +/- 0.01 new_mean_mag=12.2922 delta=0.14 (need > 0.90)
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:16:35.52 +52:58:44.7: 11.61 +/- 0.01 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:18:53.58 +50:03:56.7: 13.25 +/- 0.03 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:24:10.75 +53:30:25.9: 12.47 +/- 0.02 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:19:29.69 +50:14:48.9: 12.87 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.62 +/- 0.00
Forced photometry reference-image weighted average: 12.48 +/- 0.01
Forced photometry reference-image weighted average: 13.24 +/- 0.02
Forced photometry filter REJECTED candidate at 04:24:10.75 +53:30:25.9: ref_mag=12.48 +/- 0.01 new_mean_mag=12.2286 delta=0.25 (need > 0.90)
Forced photometry filter KEPT candidate at 04:18:53.58 +50:03:56.7: ref_mag=13.24 +/- 0.02 new_mean_mag=12.1262 delta=1.11 (need > 0.90)
Forced photometry reference-image weighted average: 12.89 +/- 0.01
Forced photometry filter REJECTED candidate at 04:16:35.52 +52:58:44.7: ref_mag=11.62 +/- 0.00 new_mean_mag=11.7374 delta=-0.12 (need > 0.90)
Forced photometry filter REJECTED candidate at 04:19:29.69 +50:14:48.9: ref_mag=12.89 +/- 0.01 new_mean_mag=12.3855 delta=0.51 (need > 0.90)
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:29:24.59 +53:39:04.2: 13.53 +/- 0.03 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:30:39.30 +53:30:17.8: 13.55 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.55 +/- 0.02
Forced photometry filter KEPT candidate at 04:30:39.30 +53:30:17.8: ref_mag=13.55 +/- 0.02 new_mean_mag=12.6395 delta=0.91 (need > 0.90)
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:33:27.23 +53:17:58.9: 13.56 +/- 0.03 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:41:46.02 +54:01:00.0: 13.57 +/- 0.03 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:29:24.59 +53:39:04.2: 13.52 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.52 +/- 0.02
Forced photometry filter KEPT candidate at 04:29:24.59 +53:39:04.2: ref_mag=13.52 +/- 0.02 new_mean_mag=12.5786 delta=0.94 (need > 0.90)
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:41:46.02 +54:01:00.0: 13.65 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.61 +/- 0.03
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:33:27.23 +53:17:58.9: 13.53 +/- 0.03 detection
Forced photometry filter REJECTED candidate at 04:41:46.02 +54:01:00.0: ref_mag=13.61 +/- 0.03 new_mean_mag=12.7092 delta=0.90 (need > 0.90)
Forced photometry reference-image weighted average: 13.55 +/- 0.02
Forced photometry filter KEPT candidate at 04:33:27.23 +53:17:58.9: ref_mag=13.55 +/- 0.02 new_mean_mag=12.4781 delta=1.07 (need > 0.90)
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:38:04.81 +55:04:57.1: 13.58 +/- 0.03 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:31:05.10 +53:04:07.7: 13.63 +/- 0.03 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:38:04.81 +55:04:57.1: 13.71 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.63 +/- 0.03
Forced photometry filter REJECTED candidate at 04:38:04.81 +55:04:57.1: ref_mag=13.63 +/- 0.03 new_mean_mag=12.7550 delta=0.88 (need > 0.90)
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:39:29.12 +54:16:56.7: 13.78 +/- 0.04 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:43:11.56 +53:35:12.5: 13.82 +/- 0.05 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:31:05.10 +53:04:07.7: 13.66 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.64 +/- 0.02
Forced photometry filter KEPT candidate at 04:31:05.10 +53:04:07.7: ref_mag=13.64 +/- 0.02 new_mean_mag=12.7096 delta=0.93 (need > 0.90)
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:39:29.12 +54:16:56.7: 13.69 +/- 0.04 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:36:24.01 +53:48:44.9: 13.94 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.74 +/- 0.03
Forced photometry filter KEPT candidate at 04:39:29.12 +54:16:56.7: ref_mag=13.74 +/- 0.03 new_mean_mag=12.8038 delta=0.93 (need > 0.90)
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:43:11.56 +53:35:12.5: 13.90 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.86 +/- 0.03
Forced photometry filter KEPT candidate at 04:43:11.56 +53:35:12.5: ref_mag=13.86 +/- 0.03 new_mean_mag=12.8976 delta=0.96 (need > 0.90)
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:36:24.01 +53:48:44.9: 13.97 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.96 +/- 0.03
Forced photometry filter KEPT candidate at 04:36:24.01 +53:48:44.9: ref_mag=13.96 +/- 0.03 new_mean_mag=12.8190 delta=1.14 (need > 0.90)
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:33:11.13 +54:16:34.9: 13.94 +/- 0.05 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:39:20.49 +54:29:08.0: 13.90 +/- 0.05 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:33:11.13 +54:16:34.9: 13.87 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.90 +/- 0.03
Forced photometry filter KEPT candidate at 04:33:11.13 +54:16:34.9: ref_mag=13.90 +/- 0.03 new_mean_mag=12.8645 delta=1.04 (need > 0.90)
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:39:20.49 +54:29:08.0: 13.87 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.88 +/- 0.03
Forced photometry filter KEPT candidate at 04:39:20.49 +54:29:08.0: ref_mag=13.88 +/- 0.03 new_mean_mag=12.8570 delta=1.03 (need > 0.90)
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:36:03.48 +54:48:22.0: 13.90 +/- 0.04 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:36:03.48 +54:48:22.0: 13.86 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.88 +/- 0.03
Forced photometry filter KEPT candidate at 04:36:03.48 +54:48:22.0: ref_mag=13.88 +/- 0.03 new_mean_mag=12.8306 delta=1.05 (need > 0.90)
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:31:11.29 +53:10:36.0: 13.88 +/- 0.04 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:31:11.29 +53:10:36.0: 13.84 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.86 +/- 0.03
Forced photometry filter KEPT candidate at 04:31:11.29 +53:10:36.0: ref_mag=13.86 +/- 0.03 new_mean_mag=12.7294 delta=1.13 (need > 0.90)
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:39:11.29 +53:33:23.8: 13.85 +/- 0.05 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:39:11.29 +53:33:23.8: 13.74 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.79 +/- 0.03
Forced photometry filter KEPT candidate at 04:39:11.29 +53:33:23.8: ref_mag=13.79 +/- 0.03 new_mean_mag=12.7068 delta=1.08 (need > 0.90)
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:37:20.49 +54:06:13.4: 13.82 +/- 0.04 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:37:38.77 +53:23:11.6: 13.70 +/- 0.04 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:37:20.49 +54:06:13.4: 13.84 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.83 +/- 0.03
Forced photometry filter KEPT candidate at 04:37:20.49 +54:06:13.4: ref_mag=13.83 +/- 0.03 new_mean_mag=12.8285 delta=1.00 (need > 0.90)
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:37:38.77 +53:23:11.6: 13.73 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.71 +/- 0.03
Forced photometry filter KEPT candidate at 04:37:38.77 +53:23:11.6: ref_mag=13.71 +/- 0.03 new_mean_mag=12.7468 delta=0.97 (need > 0.90)
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:35:55.91 +53:50:20.2: 13.78 +/- 0.04 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:35:51.44 +53:22:45.2: 13.75 +/- 0.04 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:35:55.91 +53:50:20.2: 13.76 +/- 0.04 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:35:51.44 +53:22:45.2: 13.84 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.77 +/- 0.03
Forced photometry reference-image weighted average: 13.79 +/- 0.03
Forced photometry filter KEPT candidate at 04:35:55.91 +53:50:20.2: ref_mag=13.77 +/- 0.03 new_mean_mag=12.7854 delta=0.98 (need > 0.90)
Forced photometry filter KEPT candidate at 04:35:51.44 +53:22:45.2: ref_mag=13.79 +/- 0.03 new_mean_mag=12.7737 delta=1.02 (need > 0.90)
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:35:51.57 +53:29:14.9: 13.71 +/- 0.04 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:35:51.57 +53:29:14.9: 13.70 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.71 +/- 0.03
Forced photometry filter KEPT candidate at 04:35:51.57 +53:29:14.9: ref_mag=13.71 +/- 0.03 new_mean_mag=12.7362 delta=0.97 (need > 0.90)
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:37:35.90 +53:38:10.4: 13.69 +/- 0.04 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:37:35.90 +53:38:10.4: 13.64 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.67 +/- 0.03
Forced photometry filter KEPT candidate at 04:37:35.90 +53:38:10.4: ref_mag=13.67 +/- 0.03 new_mean_mag=12.6873 delta=0.98 (need > 0.90)
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:40:14.43 +54:03:27.5: 13.69 +/- 0.04 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:40:14.43 +54:03:27.5: 13.69 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.69 +/- 0.03
Forced photometry filter KEPT candidate at 04:40:14.43 +54:03:27.5: ref_mag=13.69 +/- 0.03 new_mean_mag=12.7479 delta=0.94 (need > 0.90)
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:31:48.95 +53:05:55.8: 13.68 +/- 0.04 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:38:48.75 +54:23:57.8: 13.61 +/- 0.04 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:31:48.95 +53:05:55.8: 13.74 +/- 0.04 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:38:48.75 +54:23:57.8: 13.74 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.66 +/- 0.03
Forced photometry reference-image weighted average: 13.71 +/- 0.03
Forced photometry filter KEPT candidate at 04:31:48.95 +53:05:55.8: ref_mag=13.71 +/- 0.03 new_mean_mag=12.6317 delta=1.08 (need > 0.90)
Forced photometry filter REJECTED candidate at 04:38:48.75 +54:23:57.8: ref_mag=13.66 +/- 0.03 new_mean_mag=12.7676 delta=0.90 (need > 0.90)
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:41:24.23 +55:49:20.6: 13.65 +/- 0.04 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:41:24.23 +55:49:20.6: 13.72 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.68 +/- 0.03
Forced photometry filter KEPT candidate at 04:41:24.23 +55:49:20.6: ref_mag=13.68 +/- 0.03 new_mean_mag=12.6830 delta=1.00 (need > 0.90)
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:30:05.72 +54:06:32.5: 13.63 +/- 0.03 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:31:04.21 +53:44:06.1: 13.61 +/- 0.04 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:31:04.21 +53:44:06.1: 13.64 +/- 0.04 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:30:05.72 +54:06:32.5: 13.61 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.63 +/- 0.03
Forced photometry reference-image weighted average: 13.62 +/- 0.02
Forced photometry filter KEPT candidate at 04:31:04.21 +53:44:06.1: ref_mag=13.63 +/- 0.03 new_mean_mag=12.6907 delta=0.94 (need > 0.90)
Forced photometry filter KEPT candidate at 04:30:05.72 +54:06:32.5: ref_mag=13.62 +/- 0.02 new_mean_mag=12.5606 delta=1.06 (need > 0.90)
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:33:52.14 +53:31:58.7: 13.58 +/- 0.03 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:33:52.14 +53:31:58.7: 13.57 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.57 +/- 0.02
Forced photometry filter KEPT candidate at 04:33:52.14 +53:31:58.7: ref_mag=13.57 +/- 0.02 new_mean_mag=12.6597 delta=0.91 (need > 0.90)
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:30:17.10 +53:25:29.2: 13.57 +/- 0.03 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:30:17.10 +53:25:29.2: 13.58 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.58 +/- 0.02
Forced photometry filter KEPT candidate at 04:30:17.10 +53:25:29.2: ref_mag=13.58 +/- 0.02 new_mean_mag=12.5261 delta=1.05 (need > 0.90)
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:38:52.47 +53:06:38.6: 13.56 +/- 0.03 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:39:21.95 +54:31:12.7: 13.53 +/- 0.04 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:31:52.78 +53:18:46.6: 13.54 +/- 0.03 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:38:52.47 +53:06:38.6: 13.54 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.55 +/- 0.02
Forced photometry filter KEPT candidate at 04:38:52.47 +53:06:38.6: ref_mag=13.55 +/- 0.02 new_mean_mag=12.6250 delta=0.92 (need > 0.90)
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:39:21.95 +54:31:12.7: 13.55 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.54 +/- 0.03
Forced photometry filter KEPT candidate at 04:39:21.95 +54:31:12.7: ref_mag=13.54 +/- 0.03 new_mean_mag=12.5721 delta=0.97 (need > 0.90)
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:31:52.78 +53:18:46.6: 13.49 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.52 +/- 0.02
Forced photometry filter KEPT candidate at 04:31:52.78 +53:18:46.6: ref_mag=13.52 +/- 0.02 new_mean_mag=12.5558 delta=0.96 (need > 0.90)
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:33:29.21 +53:12:27.7: 13.53 +/- 0.03 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:33:29.21 +53:12:27.7: 13.56 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.54 +/- 0.02
Forced photometry filter KEPT candidate at 04:33:29.21 +53:12:27.7: ref_mag=13.54 +/- 0.02 new_mean_mag=12.4799 delta=1.06 (need > 0.90)
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:38:27.56 +53:12:38.2: 13.53 +/- 0.03 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:29:00.14 +53:27:22.7: 13.54 +/- 0.04 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:38:27.56 +53:12:38.2: 13.55 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.54 +/- 0.02
Forced photometry filter KEPT candidate at 04:38:27.56 +53:12:38.2: ref_mag=13.54 +/- 0.02 new_mean_mag=12.5547 delta=0.99 (need > 0.90)
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:33:27.63 +53:35:49.8: 13.52 +/- 0.03 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:29:00.14 +53:27:22.7: 13.69 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.60 +/- 0.03
Forced photometry filter KEPT candidate at 04:29:00.14 +53:27:22.7: ref_mag=13.60 +/- 0.03 new_mean_mag=12.5854 delta=1.02 (need > 0.90)
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:33:27.63 +53:35:49.8: 13.47 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.50 +/- 0.02
Forced photometry filter KEPT candidate at 04:33:27.63 +53:35:49.8: ref_mag=13.50 +/- 0.02 new_mean_mag=12.5146 delta=0.98 (need > 0.90)
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:28:25.52 +53:34:43.6: 13.49 +/- 0.03 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:31:25.09 +53:19:47.6: 13.44 +/- 0.03 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:28:25.52 +53:34:43.6: 13.59 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.53 +/- 0.02
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:23:52.85 +50:07:13.6: 13.43 +/- 0.03 detection
Forced photometry filter KEPT candidate at 04:28:25.52 +53:34:43.6: ref_mag=13.53 +/- 0.02 new_mean_mag=12.5476 delta=0.99 (need > 0.90)
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:31:25.09 +53:19:47.6: 13.44 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.44 +/- 0.02
Forced photometry filter KEPT candidate at 04:31:25.09 +53:19:47.6: ref_mag=13.44 +/- 0.02 new_mean_mag=12.5169 delta=0.92 (need > 0.90)
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:23:52.85 +50:07:13.6: 13.44 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.43 +/- 0.02
Forced photometry filter KEPT candidate at 04:23:52.85 +50:07:13.6: ref_mag=13.43 +/- 0.02 new_mean_mag=12.4289 delta=1.00 (need > 0.90)
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:34:25.64 +53:39:30.5: 14.60 +/- 0.08 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:34:25.64 +53:39:30.5: 14.62 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.61 +/- 0.06
Forced photometry filter KEPT candidate at 04:34:25.64 +53:39:30.5: ref_mag=14.61 +/- 0.06 new_mean_mag=13.1746 delta=1.43 (need > 0.90)
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:38:01.59 +54:35:35.9: 13.38 +/- 0.03 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:28:57.53 +53:41:52.5: 13.37 +/- 0.03 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:38:01.59 +54:35:35.9: 13.54 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.45 +/- 0.02
Forced photometry filter KEPT candidate at 04:38:01.59 +54:35:35.9: ref_mag=13.45 +/- 0.02 new_mean_mag=12.4291 delta=1.02 (need > 0.90)
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:35:14.27 +53:39:20.0: 13.27 +/- 0.02 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:28:57.53 +53:41:52.5: 13.40 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.02
Forced photometry filter KEPT candidate at 04:28:57.53 +53:41:52.5: ref_mag=13.39 +/- 0.02 new_mean_mag=12.4668 delta=0.92 (need > 0.90)
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:35:14.27 +53:39:20.0: 13.25 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.26 +/- 0.02
Forced photometry filter KEPT candidate at 04:35:14.27 +53:39:20.0: ref_mag=13.26 +/- 0.02 new_mean_mag=12.2945 delta=0.97 (need > 0.90)
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:38:00.69 +54:11:33.3: 13.27 +/- 0.03 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:38:00.69 +54:11:33.3: 13.31 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.29 +/- 0.02
Forced photometry filter KEPT candidate at 04:38:00.69 +54:11:33.3: ref_mag=13.29 +/- 0.02 new_mean_mag=12.3393 delta=0.95 (need > 0.90)
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:37:42.27 +54:07:49.4: 13.19 +/- 0.02 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:37:42.27 +54:07:49.4: 13.22 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.20 +/- 0.02
Forced photometry filter KEPT candidate at 04:37:42.27 +54:07:49.4: ref_mag=13.20 +/- 0.02 new_mean_mag=12.2751 delta=0.93 (need > 0.90)
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:24:18.19 +50:11:02.0: 12.96 +/- 0.02 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:34:30.24 +53:21:28.8: 12.93 +/- 0.02 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:24:18.19 +50:11:02.0: 12.92 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.94 +/- 0.02
Forced photometry filter KEPT candidate at 04:24:18.19 +50:11:02.0: ref_mag=12.94 +/- 0.02 new_mean_mag=11.9447 delta=0.99 (need > 0.90)
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:34:30.24 +53:21:28.8: 12.87 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.01
Forced photometry filter KEPT candidate at 04:34:30.24 +53:21:28.8: ref_mag=12.90 +/- 0.01 new_mean_mag=11.9859 delta=0.91 (need > 0.90)
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-39-21_20.00sec_-15.00C_LIGHT_0046.fits at 04:41:46.24 +53:19:59.1: 14.27 +/- 0.07 detection
Forced photometry on wcs_Cam-11-Q2b1x1_2026-02-21_20-40-33_20.00sec_-15.00C_LIGHT_0047.fits at 04:41:46.24 +53:19:59.1: 14.31 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.29 +/- 0.05
Forced photometry filter KEPT candidate at 04:41:46.24 +53:19:59.1: ref_mag=14.29 +/- 0.05 new_mean_mag=13.0506 delta=1.24 (need > 0.90)
Adding exclusion_list_gaiadr2.txt__out70607.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out109623.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out111417.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out112506.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out39536.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54357.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out56127.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out56622.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out57100.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out59195.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out60604.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out60946.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out61367.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out61712.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out61946.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out63667.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out65611.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out65814.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out66545.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out67599.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out67886.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out68066.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out68083.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out68126.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out68857.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out69151.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out69377.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out69828.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out69873.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out70084.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out70523.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out70911.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out71225.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out71659.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out71814.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out72050.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out72554.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out72834.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out73007.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out73138.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out73751.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out74041.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out74988.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out75917.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out76471.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 50s
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: 30s
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Considering the candidate 161680_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
The candidate 161680_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152 did not pass the final checks
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Considering the candidate 161681_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
The candidate 161681_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152 did not pass the final checks
**** FOUND 04:28:59.77 +53:48:09.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 161682_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
The candidate 161682_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152 did not pass the final checks
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Considering the candidate 161684_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
The candidate 161684_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152 did not pass the final checks
**** FOUND 04:18:05.28 +50:18:00.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 161726_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
The candidate 161726_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152 did not pass the final checks
Rejecting candidate due to large distance (29.1") between the two second-epoch detections
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Considering the candidate 162320_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
The candidate 162320_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152 did not pass the final checks
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Considering the candidate 162364_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
The candidate 162364_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152 did not pass the final checks
Rejecting candidate due to large distance (29.4") between the two second-epoch detections
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Considering the candidate 162501_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
The candidate 162501_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152 did not pass the final checks
**** FOUND 04:40:17.86 +53:28:30.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 162541_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
The candidate 162541_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152 did not pass the final checks
**** FOUND 04:40:15.66 +53:28:20.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 162577_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
The candidate 162577_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152 did not pass the final checks
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Considering the candidate 162661_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
The candidate 162661_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152 did not pass the final checks
Rejecting candidate due to large distance (30.2") between the two second-epoch detections
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Considering the candidate 162829_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
The candidate 162829_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152 did not pass the final checks
**** FOUND 04:28:33.44 +53:54:29.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 162920_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
The candidate 162920_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152 did not pass the final checks
**** FOUND 04:15:19.43 +53:43:22.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 113617_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
The candidate 113617_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152 did not pass the final checks
**** FOUND 04:25:28.77 +50:14:25.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 109623_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
Preparing report for the candidate 109623_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 68775_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
The candidate 68775_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152 did not pass the final checks
**** FOUND 04:38:44.05 +53:29:46.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 109018_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
The candidate 109018_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152 did not pass the final checks
**** FOUND 04:23:26.18 +49:58:08.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 69377_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
Preparing report for the candidate 69377_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 70911_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
Preparing report for the candidate 70911_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 72834_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
Preparing report for the candidate 72834_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 61759_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
The candidate 61759_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 76132_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
The candidate 76132_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152 did not pass the final checks
**** FOUND 04:35:27.07 +52:56:39.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 76471_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
Preparing report for the candidate 76471_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 77810_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
The candidate 77810_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152 did not pass the final checks
**** FOUND 04:37:20.56 +52:48:30.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 50748_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
The candidate 50748_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 59195_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
Preparing report for the candidate 59195_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 66545_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
Preparing report for the candidate 66545_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 94722_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
The candidate 94722_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152 did not pass the final checks
**** FOUND 04:25:56.20 +49:53:27.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 65814_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
Preparing report for the candidate 65814_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 57100_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
Preparing report for the candidate 57100_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 60946_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
Preparing report for the candidate 60946_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54357_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
Preparing report for the candidate 54357_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 74988_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
Preparing report for the candidate 74988_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 68083_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
Preparing report for the candidate 68083_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 61946_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
Preparing report for the candidate 61946_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 70607_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
The candidate 70607_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152 did not pass the final checks
**** FOUND 04:37:38.77 +53:23:11.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.75, MAG_FAINT_SEARCH_LIMIT=13.73)GAIADR2_OUTPUT=# 1.108 273631855331805824 069.41205405278 +53.38651898063 12.6069 11.2792 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.108#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 65611_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
Preparing report for the candidate 65611_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 71225_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
Preparing report for the candidate 71225_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 69873_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
Preparing report for the candidate 69873_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 67599_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
Preparing report for the candidate 67599_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 61712_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
Preparing report for the candidate 61712_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 78328_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
The candidate 78328_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152 did not pass the final checks
**** FOUND 04:35:47.22 +52:49:59.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75917_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
Preparing report for the candidate 75917_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 58159_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
The candidate 58159_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 39536_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
Preparing report for the candidate 39536_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 63667_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
Preparing report for the candidate 63667_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 68066_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
Preparing report for the candidate 68066_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 128522_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
The candidate 128522_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152 did not pass the final checks
**** FOUND 04:30:28.53 +51:18:15.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 69828_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
Preparing report for the candidate 69828_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 72050_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
Preparing report for the candidate 72050_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 73751_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
Preparing report for the candidate 73751_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 56622_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
Preparing report for the candidate 56622_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 73138_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
Preparing report for the candidate 73138_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 74041_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
Preparing report for the candidate 74041_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 72554_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
Preparing report for the candidate 72554_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 71814_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
Preparing report for the candidate 71814_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 69151_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
Preparing report for the candidate 69151_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 77935_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
The candidate 77935_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152 did not pass the final checks
**** FOUND 04:34:17.07 +52:52:42.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 70523_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
Preparing report for the candidate 70523_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 73007_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
Preparing report for the candidate 73007_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 111417_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
Preparing report for the candidate 111417_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 68126_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
Preparing report for the candidate 68126_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 56127_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
Preparing report for the candidate 56127_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 68857_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
Preparing report for the candidate 68857_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 67886_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
Preparing report for the candidate 67886_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 60604_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
Preparing report for the candidate 60604_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112826_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
The candidate 112826_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152 did not pass the final checks
**** FOUND 04:22:06.77 +50:17:30.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 61367_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
Preparing report for the candidate 61367_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 56527_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
The candidate 56527_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152 did not pass the final checks
**** FOUND 04:42:49.01 +54:24:25.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112506_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
Preparing report for the candidate 112506_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 71659_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
Preparing report for the candidate 71659_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 63553_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
The candidate 63553_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152 did not pass the final checks
**** FOUND 04:37:44.42 +53:53:04.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 70084_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
Preparing report for the candidate 70084_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116019_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152
The candidate 116019_fd_Cam-11-Q2b1x1_2026-09-06_23-29-50_20.00sec_0.00C_LIGHT_0152 did not pass the final checks
**** FOUND 04:26:54.90 +50:22:18.7 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 5s
make_report_in_HTML.sh TOTAL: 85s
Prepared the HTML report for the field Cam-11-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
04:18:53.58 +50:03:56.7
04:23:52.85 +50:07:13.6
04:24:18.19 +50:11:02.0
04:41:24.23 +55:49:20.6
04:36:03.48 +54:48:22.0
04:38:01.59 +54:35:35.9
04:39:21.95 +54:31:12.7
04:39:20.49 +54:29:08.0
04:39:29.12 +54:16:56.7
04:38:00.69 +54:11:33.3
04:33:11.13 +54:16:34.9
04:37:42.27 +54:07:49.4
04:40:14.43 +54:03:27.5
04:37:20.49 +54:06:13.4
04:30:05.72 +54:06:32.5
04:35:55.91 +53:50:20.2
04:36:24.01 +53:48:44.9
04:43:11.56 +53:35:12.5
04:37:35.90 +53:38:10.4
04:35:14.27 +53:39:20.0
04:31:04.21 +53:44:06.1
04:39:11.29 +53:33:23.8
04:34:25.64 +53:39:30.5
04:28:57.53 +53:41:52.5
04:33:27.63 +53:35:49.8
04:29:24.59 +53:39:04.2
04:33:52.14 +53:31:58.7
04:35:51.57 +53:29:14.9
04:41:46.24 +53:19:59.1
04:28:25.52 +53:34:43.6
04:30:39.30 +53:30:17.8
04:35:51.44 +53:22:45.2
04:34:30.24 +53:21:28.8
04:29:00.14 +53:27:22.7
04:30:17.10 +53:25:29.2
04:38:27.56 +53:12:38.2
04:33:27.23 +53:17:58.9
04:31:25.09 +53:19:47.6
04:31:52.78 +53:18:46.6
04:38:52.47 +53:06:38.6
04:33:29.21 +53:12:27.7
04:31:11.29 +53:10:36.0
04:31:48.95 +53:05:55.8
04:31:05.10 +53:04:07.7
########### Completed Cam-11-Q2b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ2.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
04:18:53.58 +50:03:56.7
04:29:24.59 +53:39:04.2
04:30:39.30 +53:30:17.8
04:33:27.23 +53:17:58.9
04:31:05.10 +53:04:07.7
04:39:29.12 +54:16:56.7
04:43:11.56 +53:35:12.5
04:36:24.01 +53:48:44.9
04:39:20.49 +54:29:08.0
04:33:11.13 +54:16:34.9
04:36:03.48 +54:48:22.0
04:31:11.29 +53:10:36.0
04:39:11.29 +53:33:23.8
04:37:20.49 +54:06:13.4
04:35:55.91 +53:50:20.2
04:35:51.44 +53:22:45.2
04:35:51.57 +53:29:14.9
04:37:35.90 +53:38:10.4
04:40:14.43 +54:03:27.5
04:31:48.95 +53:05:55.8
04:41:24.23 +55:49:20.6
04:30:05.72 +54:06:32.5
04:31:04.21 +53:44:06.1
04:33:52.14 +53:31:58.7
04:30:17.10 +53:25:29.2
04:38:52.47 +53:06:38.6
04:39:21.95 +54:31:12.7
04:31:52.78 +53:18:46.6
04:33:29.21 +53:12:27.7
04:38:27.56 +53:12:38.2
04:29:00.14 +53:27:22.7
04:33:27.63 +53:35:49.8
04:28:25.52 +53:34:43.6
04:31:25.09 +53:19:47.6
04:23:52.85 +50:07:13.6
04:34:25.64 +53:39:30.5
04:38:01.59 +54:35:35.9
04:28:57.53 +53:41:52.5
04:35:14.27 +53:39:20.0
04:38:00.69 +54:11:33.3
04:37:42.27 +54:07:49.4
04:24:18.19 +50:11:02.0
04:34:30.24 +53:21:28.8
04:41:46.24 +53:19:59.1
###################################################################################
04:18:53.58 +50:03:56.7 -- not an asteroid (will add it to exclusion list)
04:29:24.59 +53:39:04.2 -- not an asteroid (will add it to exclusion list)
04:30:39.30 +53:30:17.8 -- not an asteroid (will add it to exclusion list)
04:33:27.23 +53:17:58.9 -- not an asteroid (will add it to exclusion list)
04:31:05.10 +53:04:07.7 -- not an asteroid (will add it to exclusion list)
04:39:29.12 +54:16:56.7 -- not an asteroid (will add it to exclusion list)
04:43:11.56 +53:35:12.5 -- not an asteroid (will add it to exclusion list)
04:36:24.01 +53:48:44.9 -- not an asteroid (will add it to exclusion list)
04:39:20.49 +54:29:08.0 -- not an asteroid (will add it to exclusion list)
04:33:11.13 +54:16:34.9 -- not an asteroid (will add it to exclusion list)
04:36:03.48 +54:48:22.0 -- not an asteroid (will add it to exclusion list)
04:31:11.29 +53:10:36.0 -- not an asteroid (will add it to exclusion list)
04:39:11.29 +53:33:23.8 -- not an asteroid (will add it to exclusion list)
04:37:20.49 +54:06:13.4 -- not an asteroid (will add it to exclusion list)
04:35:55.91 +53:50:20.2 -- not an asteroid (will add it to exclusion list)
04:35:51.44 +53:22:45.2 -- not an asteroid (will add it to exclusion list)
04:35:51.57 +53:29:14.9 -- not an asteroid (will add it to exclusion list)
04:37:35.90 +53:38:10.4 -- not an asteroid (will add it to exclusion list)
04:40:14.43 +54:03:27.5 -- not an asteroid (will add it to exclusion list)
04:31:48.95 +53:05:55.8 -- not an asteroid (will add it to exclusion list)
04:41:24.23 +55:49:20.6 -- not an asteroid (will add it to exclusion list)
04:30:05.72 +54:06:32.5 -- not an asteroid (will add it to exclusion list)
04:31:04.21 +53:44:06.1 -- not an asteroid (will add it to exclusion list)
04:33:52.14 +53:31:58.7 -- not an asteroid (will add it to exclusion list)
04:30:17.10 +53:25:29.2 -- not an asteroid (will add it to exclusion list)
04:38:52.47 +53:06:38.6 -- not an asteroid (will add it to exclusion list)
04:39:21.95 +54:31:12.7 -- not an asteroid (will add it to exclusion list)
04:31:52.78 +53:18:46.6 -- not an asteroid (will add it to exclusion list)
04:33:29.21 +53:12:27.7 -- not an asteroid (will add it to exclusion list)
04:38:27.56 +53:12:38.2 -- not an asteroid (will add it to exclusion list)
04:29:00.14 +53:27:22.7 -- not an asteroid (will add it to exclusion list)
04:33:27.63 +53:35:49.8 -- not an asteroid (will add it to exclusion list)
04:28:25.52 +53:34:43.6 -- not an asteroid (will add it to exclusion list)
04:31:25.09 +53:19:47.6 -- not an asteroid (will add it to exclusion list)
04:23:52.85 +50:07:13.6 -- not an asteroid (will add it to exclusion list)
04:34:25.64 +53:39:30.5 -- not an asteroid (will add it to exclusion list)
04:38:01.59 +54:35:35.9 -- not an asteroid (will add it to exclusion list)
04:28:57.53 +53:41:52.5 -- not an asteroid (will add it to exclusion list)
04:35:14.27 +53:39:20.0 -- not an asteroid (will add it to exclusion list)
04:38:00.69 +54:11:33.3 -- not an asteroid (will add it to exclusion list)
04:37:42.27 +54:07:49.4 -- not an asteroid (will add it to exclusion list)
04:24:18.19 +50:11:02.0 -- not an asteroid (will add it to exclusion list)
04:34:30.24 +53:21:28.8 -- not an asteroid (will add it to exclusion list)
04:41:46.24 +53:19:59.1 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
04:18:53.58 +50:03:56.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:23:52.85 +50:07:13.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:24:18.19 +50:11:02.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:28:25.52 +53:34:43.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:28:57.53 +53:41:52.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:29:00.14 +53:27:22.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:29:24.59 +53:39:04.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:30:05.72 +54:06:32.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:30:17.10 +53:25:29.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:30:39.30 +53:30:17.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:31:04.21 +53:44:06.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:31:05.10 +53:04:07.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:31:11.29 +53:10:36.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:31:25.09 +53:19:47.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:31:48.95 +53:05:55.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:31:52.78 +53:18:46.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:33:11.13 +54:16:34.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:33:27.23 +53:17:58.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:33:27.63 +53:35:49.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:33:29.21 +53:12:27.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:33:52.14 +53:31:58.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:34:25.64 +53:39:30.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:34:30.24 +53:21:28.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:35:14.27 +53:39:20.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:35:51.44 +53:22:45.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:35:51.57 +53:29:14.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:35:55.91 +53:50:20.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:36:03.48 +54:48:22.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:36:24.01 +53:48:44.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:37:20.49 +54:06:13.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:37:35.90 +53:38:10.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:37:42.27 +54:07:49.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:38:00.69 +54:11:33.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:38:01.59 +54:35:35.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:38:27.56 +53:12:38.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:38:52.47 +53:06:38.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:39:11.29 +53:33:23.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:39:20.49 +54:29:08.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:39:21.95 +54:31:12.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:39:29.12 +54:16:56.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:40:14.43 +54:03:27.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:41:24.23 +55:49:20.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:41:46.24 +53:19:59.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:43:11.56 +53:35:12.5 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
04:18:53.58 +50:03:56.7 -- a known variable star
04:23:52.85 +50:07:13.6 -- not a known variable star
04:24:18.19 +50:11:02.0 -- a known variable star
04:28:25.52 +53:34:43.6 -- not a known variable star
04:28:57.53 +53:41:52.5 -- a known variable star
04:29:00.14 +53:27:22.7 -- not a known variable star
04:29:24.59 +53:39:04.2 -- not a known variable star
04:30:05.72 +54:06:32.5 -- not a known variable star
04:30:17.10 +53:25:29.2 -- a known variable star
04:30:39.30 +53:30:17.8 -- a known variable star
04:31:04.21 +53:44:06.1 -- not a known variable star
04:31:05.10 +53:04:07.7 -- not a known variable star
04:31:11.29 +53:10:36.0 -- not a known variable star
04:31:25.09 +53:19:47.6 -- not a known variable star
04:31:48.95 +53:05:55.8 -- not a known variable star
04:31:52.78 +53:18:46.6 -- not a known variable star
04:33:11.13 +54:16:34.9 -- a known variable star
04:33:27.23 +53:17:58.9 -- not a known variable star
04:33:27.63 +53:35:49.8 -- not a known variable star
04:33:29.21 +53:12:27.7 -- not a known variable star
04:33:52.14 +53:31:58.7 -- not a known variable star
04:34:25.64 +53:39:30.5 -- not a known variable star
04:34:30.24 +53:21:28.8 -- a known variable star
04:35:14.27 +53:39:20.0 -- not a known variable star
04:35:51.44 +53:22:45.2 -- not a known variable star
04:35:51.57 +53:29:14.9 -- not a known variable star
04:35:55.91 +53:50:20.2 -- not a known variable star
04:36:03.48 +54:48:22.0 -- not a known variable star
04:36:24.01 +53:48:44.9 -- not a known variable star
04:37:20.49 +54:06:13.4 -- not a known variable star
04:37:35.90 +53:38:10.4 -- a known variable star
04:37:42.27 +54:07:49.4 -- a known variable star
04:38:00.69 +54:11:33.3 -- not a known variable star
04:38:01.59 +54:35:35.9 -- not a known variable star
04:38:27.56 +53:12:38.2 -- not a known variable star
04:38:52.47 +53:06:38.6 -- a known variable star
04:39:11.29 +53:33:23.8 -- not a known variable star
04:39:20.49 +54:29:08.0 -- not a known variable star
04:39:21.95 +54:31:12.7 -- not a known variable star
04:39:29.12 +54:16:56.7 -- not a known variable star
04:40:14.43 +54:03:27.5 -- not a known variable star
04:41:24.23 +55:49:20.6 -- not a known variable star
04:41:46.24 +53:19:59.1 -- not a known variable star
04:43:11.56 +53:35:12.5 -- not a known variable star
Found 34 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
44 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 44 (excluding asteroids and hot pixels, 34 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)2461290.68701756 -observatory V36
11:38:12.65 +03:32:41.9 Mercury (-0.9mag)
13:35:47.37 -14:28:41.2 Venus (-4.7mag)
07:13:41.59 +22:59:17.7 Mars (1.2mag)
09:08:57.58 +16:57:55.6 Jupiter (-1.8mag)
00:51:45.53 +02:38:48.5 Saturn (0.4mag)
04:13:41.21 +21:01:59.2 Uranus (5.7mag)
00:13:45.43 -00:03:09.4 Neptune (7.7mag)
20:25:36.06 -23:39:35.5 Pluto (14.5mag)
07:39:23.61 +23:55:29.3 Moon (-9.4mag)
-rw-r--r-- 1 apache apache 362 Sep 7 00:00 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461290.68701756:
09:09:03.12 +16:57:28.7 Io (6.2mag)
09:08:55.08 +16:58:09.2 Europa (6.3mag)
09:09:08.23 +16:57:02.0 Ganymede (5.7mag)
09:08:32.65 +16:59:58.5 Callisto (6.9mag)
09:06:43.61 +17:14:24.9 Himalia (15.7mag)
09:09:00.34 +16:57:43.0 Thebe (16.6mag)
09:06:20.92 +17:08:24.0 Elara (17.7mag)
09:12:51.38 +16:25:32.1 Pasiphae (17.9mag)
09:10:03.11 +17:15:40.5 Carme (19.0mag)
00:51:42.04 +02:39:11.9 Titan (8.3mag)
00:51:38.85 +02:38:43.8 Rhea (9.6mag)
00:52:01.03 +02:41:20.0 Iapetus (11.0mag)
00:51:59.49 +02:38:14.7 Hyperion (14.3mag)
00:50:32.41 +02:28:33.4 Phoebe (16.4mag)
-rw-r--r-- 1 apache apache 568 Sep 7 00:00 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461290.68701756:
22:04:08.20 +00:53:28.3 JWST
17:31:49.34 +37:16:33.4 Chandra
09:47:34.80 -54:50:39.7 XMM-Newton
-rw-r--r-- 1 apache apache 96 Sep 7 00:00 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461290.68701756 -observatory V36
03:40:21.58 +19:20:06.4 17.4mag P/1996 R2 (Lagerkvist)
18:02:52.30 -34:12:48.7 14.3mag P/2010 H2 (Vales)
07:19:23.25 -70:17:43.5 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
06:15:40.82 +33:41:50.8 17.7mag C/2017 K2 (PANSTARRS)
04:51:15.88 +45:27:39.2 15.8mag P/2021 N1 (ZTF)
04:51:15.88 +45:27:39.2 15.8mag P/2021 N1 (ZTF)
04:51:15.88 +45:27:39.2 15.8mag P/2021 N1 (ZTF)
04:51:15.88 +45:27:39.2 15.8mag P/2021 N1 (ZTF)
04:51:15.88 +45:27:39.2 15.8mag P/2021 N1 (ZTF)
22:13:34.42 +28:41:01.8 17.4mag C/2022 E2 (ATLAS)
07:10:06.54 +25:58:51.0 16.9mag C/2022 N2 (PANSTARRS)
10:49:23.74 +27:13:48.0 17.1mag C/2022 QE78 (ATLAS)
09:48:36.00 +05:14:01.2 18.0mag C/2022 R6 (PANSTARRS)
15:29:33.79 -15:38:22.8 14.8mag C/2023 R1 (PANSTARRS)
08:38:17.75 +32:53:07.6 15.8mag C/2024 E1 (Wierzchos)
15:06:34.79 +15:19:27.6 17.9mag C/2024 G6 (ATLAS)
18:33:40.68 +43:10:45.6 13.7mag C/2024 J3 (ATLAS)
20:26:19.24 +49:18:27.5 17.4mag C/2024 R4 (PANSTARRS)
05:35:32.97 -13:01:29.9 15.1mag C/2024 T5 (ATLAS)
07:11:35.56 +18:33:55.3 17.8mag C/2025 J1 (Borisov)
11:17:48.19 +18:46:39.7 16.8mag C/2025 V2 (Rankin)
13:19:32.01 +00:07:30.6 16.8mag C/2025 Y1 (ATLAS)
16:41:05.70 +74:03:10.8 16.1mag C/2026 A2 (Bok)
03:05:51.05 +46:08:18.1 17.4mag C/2026 B2 (Sun-Gao)
12:13:10.14 +11:16:26.4 17.5mag A/2026 E1
22:25:55.47 -35:02:01.4 13.4mag 10P/Tempel
01:19:19.31 +37:00:32.6 17.9mag 11P/Tempel-Swift-LINEAR
11:48:05.83 -05:27:35.8 16.3mag 29P/Schwassmann-Wachmann
12:08:20.85 -05:03:36.1 17.6mag 63P/Wild
00:44:43.82 -07:03:45.1 15.4mag 65P/Gunn
06:39:07.14 +19:15:37.4 17.1mag 78P/Gehrels
03:17:16.56 +14:59:48.8 16.7mag 88P/Howell
05:37:51.39 +28:35:19.4 17.5mag 112P/Urata-Niijima
07:31:28.48 +24:50:40.0 17.9mag 114P/Wiseman-Skiff
10:27:38.80 +20:53:27.8 14.8mag 123P/West-Hartley
12:46:21.35 -21:18:01.6 17.4mag 124P/Mrkos
06:17:17.03 +20:38:33.0 15.9mag 128P/Shoemaker-Holt
02:32:38.73 -17:37:29.2 15.2mag 161P/Hartley-IRAS
09:37:47.42 +13:48:36.5 12.1mag 169P/NEAT
03:24:21.07 +08:29:02.3 14.5mag 220P/McNaught
04:47:46.60 +36:17:09.3 15.2mag 260P/McNaught
08:31:34.91 +35:42:45.7 17.3mag 295P/LINEAR
15:25:09.76 -00:14:12.3 17.9mag 391P/Kowalski
09:27:41.42 +16:51:21.4 17.9mag 450P/LONEOS
-rw-r--r-- 1 apache apache 2.2K Sep 7 00:00 comets.txt
############################################################
List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
19:45:06.20 +18:22:48.80 V488 2026-08-30.13 9.37
18:25:12.74 -22:25:28.60 V8055 2026-08-30.22 10.89
17:17:45.96 +64:31:40.10 ASASSN-26ez 2026-08-25.13 10.87
19:02:47.09 +58:08:21.00 AT2026zwo 2026-08-24.16 15.78
04:20:07.58 -42:26:59.90 AT2026zjy 2026-08-23.03 15.91
03:08:18.02 +11:54:46.50 SN2026ymb 2026-08-23.4 16.44
20:22:32.48 -50:45:14.30 SN2026yid 2026-08-22.82 15.13
04:24:28.39 -56:20:21.60 ASASSN-26ey 2026-08-20.02 15.55
16:46:37.81 -63:14:59.80 ASASSN-26ex 2026-08-18.78 3.63
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
23:47:50.89 +49:28:51.30 SN2026wjs 2026-08-9.24 17.09
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
02:02:26.78 +32:04:21.30 AT2026ovz 2026-06-14.59 15.39
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
14:23:56.59 -58:37:47.40 ASASSN-26dn 2026-05-20.01 14.59
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
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
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
19:45:06.48 +18:22:42.2 PNV J19450648+1822422 2026-08-25.1278 9.0mag
00:42:54.65 +41:22:59.3 PNV J00425465+4122593 2026-08-25.4712 18.9mag
00:42:50.38 +41:18:58.76 PNV J00425038+4118587 2026-09-04.1512 18.2mag
-rw-r--r-- 1 apache apache 190K Sep 7 00:00 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
00:34:06.502 +12:42:13.91 AT 2026ypz 2026-08-08.10 20
21:30:05.008 +02:38:33.95 AT 2026ypy 2026-08-06.53 20.21
21:00:04.179 -04:29:11.16 AT 2026ypx 2026-08-10.99 20.06
02:37:12.256 +15:20:39.63 AT 2026ypw 2026-08-12.19 20.13
20:30:21.422 +77:41:45.40 AT 2026ypv 2026-08-02.23 20.4969
13:32:08.201 +00:21:43.54 AT 2026ypu 2026-08-05.16 19.6868
14:07:14.862 +00:31:05.95 AT 2026ypt 2026-08-08.16 20.0684
17:39:38.555 +44:15:43.22 AT 2026yps 2026-07-22.33 20.9161
23:51:42.078 +03:04:27.33 AT 2026ypr 2026-08-12.07 20.05
02:34:15.880 +40:31:56.36 AT 2026ypq 2026-08-11.58 18.82
15:38:07.902 +06:01:37.84 AT 2026ypp 2026-08-11.26 20.34
15:24:17.953 +11:26:31.29 AT 2026ypo 2026-08-11.26 20.8
14:21:16.003 +25:15:33.98 AT 2026ypn 2026-08-11.26 18.72
16:23:56.085 +09:36:23.21 AT 2026ypm 2026-08-11.28 20.97
20:54:11.595 +10:54:51.15 SN 2026ypl 2026-08-09.34 20.4
00:40:25.122 +24:26:45.82 AT 2026ypk 2026-08-07.45 20.4501
17:05:06.872 +77:16:36.60 AT 2026ypj 2026-08-11.31 18.807
20:49:46.878 -06:36:38.40 AT 2026ypi 2026-08-09.29 20.4359
00:12:21.150 -17:28:55.44 AT 2026yph 2026-08-08.42 20.4034
00:48:58.972 +17:28:17.78 AT 2026ypg 2026-08-05.48 20.2336
-rw-r--r-- 1 apache apache 88K Sep 7 00:00 tns_transients_list.txt
