This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_For-01-Q2b1x1_052356_TTUQ2b1x1_2819419_mo17MjFd
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 04.4307 2461287.9307 11.10 01:55:23.08 -29:55:41.5
227.97129 -75.69087 galactic For Second-epoch detections are separated by 1.2" and 7.2 pix
The object was found in VSX 1" Gaia DR3 5020775541633735296
Type: ROT
# Max. Min./Amp. JD0 Period
12.990 G 13.040 G K
The object was not found in astcheck.
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:55:23.08 -29:55:41.5: 13.23 +/- 0.19 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:55:23.08 -29:55:41.5: 13.34 +/- 0.22 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.14
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 04.4307* 01 55 23.08 -29 55 41.5 11.1 U For 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5020775541633735296,2461287.9307,11.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5020775541633735296 20260904.4307 11.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 04.4307 2461287.9307 11.04 01:56:52.35 -30:01:18.3
228.17712 -75.35932 galactic For Second-epoch detections are separated by 1.8" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:56:52.35 -30:01:18.3 (user input) | T | P | (position from user input) J-Ks=0.450+/-0.035 (G)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:56:52.35 -30:01:18.3: 13.49 +/- 0.22 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:56:52.35 -30:01:18.3: 13.47 +/- 0.25 detection
Forced photometry reference-image weighted average: 13.48 +/- 0.17
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 04.4307* 01 56 52.35 -30 01 18.3 11.0 U For 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461287.9307,11.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260904.4307 11.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 04.4307 2461287.9307 10.99 01:56:56.54 -29:59:09.4
228.02906 -75.34888 galactic For Second-epoch detections are separated by 1.4" and 7.4 pix
The object was found in VSX 0" Gaia DR3 5020719088583618688
Type: ROT
# Max. Min./Amp. JD0 Period
13.040 G 13.080 G G
The object was not found in astcheck.
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:56:56.54 -29:59:09.4: 13.40 +/- 0.22 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:56:56.54 -29:59:09.4: 13.55 +/- 0.27 detection
Forced photometry reference-image weighted average: 13.46 +/- 0.17
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 04.4307* 01 56 56.54 -29 59 09.4 11.0 U For 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5020719088583618688,2461287.9307,10.99,0.05,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
Gaia DR3 5020719088583618688 20260904.4307 10.99CV 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 04.4307 2461287.9307 11.05 01:55:10.94 -29:49:18.5
227.56560 -75.74768 galactic For Second-epoch detections are separated by 0.9" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:55:10.94 -29:49:18.5 (user input) | T | P | (position from user input) J-Ks=0.343+/-0.035 (G)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:55:10.94 -29:49:18.5: 13.20 +/- 0.17 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:55:10.94 -29:49:18.5: 13.10 +/- 0.18 detection
Forced photometry reference-image weighted average: 13.15 +/- 0.12
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 04.4307* 01 55 10.94 -29 49 18.5 11.1 U For 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461287.9307,11.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260904.4307 11.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 04.4307 2461287.9307 11.16 01:57:45.65 -29:55:09.2
227.68366 -75.18104 galactic For Second-epoch detections are separated by 1.5" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:57:45.65 -29:55:09.2 (user input) | T | P | (position from user input) J-Ks=0.380+/-0.034 (G)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:57:45.65 -29:55:09.2: 12.91 +/- 0.13 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:57:45.65 -29:55:09.2: 13.26 +/- 0.21 detection
Forced photometry reference-image weighted average: 13.01 +/- 0.11
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 04.4307* 01 57 45.65 -29 55 09.2 11.2 U For 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461287.9307,11.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260904.4307 11.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 04.4307 2461287.9307 11.39 01:57:22.45 -30:06:36.9
228.46717 -75.24018 galactic For Second-epoch detections are separated by 0.1" and 7.3 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 | 01:57:22.45 -30:06:36.9 (user input) | T | P | (position from user input) J-Ks=0.355+/-0.033 (G)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:57:22.45 -30:06:36.9: 13.60 +/- 0.26 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:57:22.45 -30:06:36.9: 13.19 +/- 0.19 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.15
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 04.4307* 01 57 22.45 -30 06 36.9 11.4 U For 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461287.9307,11.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260904.4307 11.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 04.4307 2461287.9307 10.89 01:58:44.02 -30:13:58.2
228.78697 -74.93262 galactic For Second-epoch detections are separated by 2.7" and 6.9 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 | 01:58:44.02 -30:13:58.2 (user input) | T | P | (position from user input) J-Ks=0.309+/-0.034 (F)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:58:44.02 -30:13:58.2: 12.94 +/- 0.15 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:58:44.02 -30:13:58.2: 12.94 +/- 0.15 detection
Forced photometry reference-image weighted average: 12.94 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 04.4307* 01 58 44.02 -30 13 58.2 10.9 U For 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461287.9307,10.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260904.4307 10.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 04.4307 2461287.9307 10.19 01:48:04.39 -23:17:17.0
199.35744 -76.63590 galactic Cet Second-epoch detections are separated by 0.2" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5134476279580139392 | 01:48:04.40 -23:17:17.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.626+/-0.028 (K)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:48:04.39 -23:17:17.0: 11.32 +/- 0.03 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:48:04.39 -23:17:17.0: 11.33 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.32 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 04.4307* 01 48 04.39 -23 17 17.0 10.2 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5134476279580139392,2461287.9307,10.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5134476279580139392 20260904.4307 10.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 04.4307 2461287.9307 10.11 01:42:12.18 -29:02:01.6
225.54760 -78.64769 galactic Scl Second-epoch detections are separated by 1.3" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5023317784315939712 | 01:42:12.19 -29:02:01.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.310+/-0.036 (F)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:42:12.18 -29:02:01.6: 11.37 +/- 0.03 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:42:12.18 -29:02:01.6: 11.30 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.34 +/- 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 5023317784315939712,2461287.9307,10.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5023317784315939712 20260904.4307 10.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 04.4307 2461287.9307 10.88 01:57:13.95 -29:43:12.1
226.95702 -75.31736 galactic For Second-epoch detections are separated by 0.3" and 7.4 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 | 01:57:13.95 -29:43:12.1 (user input) | T | P | (position from user input) J-Ks=0.460+/-0.032 (G)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:57:13.95 -29:43:12.1: 12.69 +/- 0.11 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:57:13.95 -29:43:12.1: 12.83 +/- 0.13 detection
Forced photometry reference-image weighted average: 12.75 +/- 0.09
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 04.4307* 01 57 13.95 -29 43 12.1 10.9 U For 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461287.9307,10.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260904.4307 10.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 04.4307 2461287.9307 10.19 01:55:53.97 -29:48:24.1
227.42962 -75.59506 galactic For Second-epoch detections are separated by 1.4" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5020777912455700352 | 01:55:53.97 -29:48:24.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.294+/-0.030 (F)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:55:53.97 -29:48:24.1: 11.77 +/- 0.05 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:55:53.97 -29:48:24.1: 11.72 +/- 0.05 detection
Forced photometry reference-image weighted average: 11.75 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 04.4307* 01 55 53.97 -29 48 24.1 10.2 U For 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5020777912455700352,2461287.9307,10.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5020777912455700352 20260904.4307 10.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 04.4307 2461287.9307 10.57 01:39:20.71 -23:29:35.3
197.00785 -78.58530 galactic Cet Second-epoch detections are separated by 1.3" and 7.8 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 5039287297356291456 | 01:39:20.70 -23:29:35.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.342+/-0.030 (G)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:39:20.71 -23:29:35.3: 11.78 +/- 0.05 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:39:20.71 -23:29:35.3: 11.70 +/- 0.05 detection
Forced photometry reference-image weighted average: 11.74 +/- 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!
TCP 2026 09 04.4307* 01 39 20.71 -23 29 35.3 10.6 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5039287297356291456,2461287.9307,10.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5039287297356291456 20260904.4307 10.57CV 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 04.4307 2461287.9307 10.64 01:45:54.32 -28:34:58.7
222.98265 -77.88015 galactic For Second-epoch detections are separated by 0.4" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5023393444459989632 | 01:45:54.38 -28:34:58.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.290+/-0.034 (F)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:45:54.32 -28:34:58.7: 11.77 +/- 0.05 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:45:54.32 -28:34:58.7: 11.74 +/- 0.05 detection
Forced photometry reference-image weighted average: 11.76 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 04.4307* 01 45 54.32 -28 34 58.7 10.6 U For 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5023393444459989632,2461287.9307,10.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5023393444459989632 20260904.4307 10.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 04.4307 2461287.9307 10.98 01:45:06.40 -28:17:00.8
221.59196 -78.07133 galactic Scl Second-epoch detections are separated by 2.0" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5023461369366804224 | 01:45:06.39 -28:17:00.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.342+/-0.034 (G)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:45:06.40 -28:17:00.8: 12.74 +/- 0.11 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:45:06.40 -28:17:00.8: 12.62 +/- 0.11 detection
Forced photometry reference-image weighted average: 12.68 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5023461369366804224,2461287.9307,10.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5023461369366804224 20260904.4307 10.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 04.4307 2461287.9307 10.33 01:48:08.88 -23:29:31.4
200.21691 -76.68684 galactic Cet Second-epoch detections are separated by 1.4" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5134460405381031936 | 01:48:08.88 -23:29:31.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.291+/-0.029 (F)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:48:08.88 -23:29:31.4: 11.71 +/- 0.04 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:48:08.88 -23:29:31.4: 11.71 +/- 0.04 detection
Forced photometry reference-image weighted average: 11.71 +/- 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!
TCP 2026 09 04.4307* 01 48 08.88 -23 29 31.4 10.3 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5134460405381031936,2461287.9307,10.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5134460405381031936 20260904.4307 10.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 04.4307 2461287.9307 10.65 01:35:55.26 -28:22:14.2
222.69946 -80.08378 galactic Scl Second-epoch detections are separated by 1.2" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5035594656274008704 | 01:35:55.27 -28:22:14.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 1971AJ.....76..338S SB 658 J-Ks=0.170+/-0.032 (F)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:35:55.26 -28:22:14.2: 11.68 +/- 0.05 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:35:55.26 -28:22:14.2: 11.61 +/- 0.05 detection
Forced photometry reference-image weighted average: 11.64 +/- 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 5035594656274008704,2461287.9307,10.65,0.05,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 5035594656274008704 20260904.4307 10.65CV 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 04.4307 2461287.9307 10.54 01:41:51.67 -25:15:07.2
206.34305 -78.53908 galactic Scl Second-epoch detections are separated by 1.3" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5037758048480716288 | 01:41:51.64 -25:15:07.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.353+/-0.035 (G)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:41:51.67 -25:15:07.2: 11.65 +/- 0.04 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:41:51.67 -25:15:07.2: 11.49 +/- 0.04 detection
Forced photometry reference-image weighted average: 11.56 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5037758048480716288,2461287.9307,10.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5037758048480716288 20260904.4307 10.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 04.4307 2461287.9307 10.02 01:46:23.55 -28:47:54.1
223.96450 -77.75812 galactic For Second-epoch detections are separated by 0.3" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5022636396343640320 | 01:46:23.54 -28:47:54.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A5 pec 1971AJ.....76..338S SB 721 J-Ks=0.076+/-0.037 (A)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:46:23.55 -28:47:54.1: 11.63 +/- 0.04 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:46:23.55 -28:47:54.1: 11.65 +/- 0.04 detection
Forced photometry reference-image weighted average: 11.64 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 04.4307* 01 46 23.55 -28 47 54.1 10.0 U For 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5022636396343640320,2461287.9307,10.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5022636396343640320 20260904.4307 10.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 04.4307 2461287.9307 10.42 01:59:01.26 -30:06:29.7
228.28147 -74.88724 galactic For Second-epoch detections are separated by 0.3" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5020616971441236352 | 01:59:01.05 -30:06:29.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:59:01.26 -30:06:29.7: 11.61 +/- 0.04 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:59:01.26 -30:06:29.7: 11.56 +/- 0.04 detection
Forced photometry reference-image weighted average: 11.59 +/- 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 Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 04.4307* 01 59 01.26 -30 06 29.7 10.4 U For 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5020616971441236352,2461287.9307,10.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5020616971441236352 20260904.4307 10.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 04.4307 2461287.9307 10.48 01:37:11.37 -24:59:31.6
203.74586 -79.50950 galactic Scl Second-epoch detections are separated by 1.2" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5038472078204212736 | 01:37:11.33 -24:59:31.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.460+/-0.029 (G)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:37:11.37 -24:59:31.6: 11.60 +/- 0.04 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:37:11.37 -24:59:31.6: 11.56 +/- 0.04 detection
Forced photometry reference-image weighted average: 11.58 +/- 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 5038472078204212736,2461287.9307,10.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5038472078204212736 20260904.4307 10.48CV 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 04.4307 2461287.9307 11.21 01:41:23.11 -25:06:58.8
205.55638 -78.61477 galactic Scl Second-epoch detections are separated by 2.3" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5037807560863675520 | 01:41:23.03 -25:06:59.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.469+/-0.030 (K)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:41:23.11 -25:06:58.8: 12.65 +/- 0.10 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:41:23.11 -25:06:58.8: 12.51 +/- 0.09 detection
Forced photometry reference-image weighted average: 12.57 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 5037807560863675520,2461287.9307,11.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5037807560863675520 20260904.4307 11.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 04.4307 2461287.9307 9.70 01:56:24.95 -29:59:57.1
228.13878 -75.46026 galactic For Second-epoch detections are separated by 0.7" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5020725032818724480 | 01:56:24.95 -29:59:57.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.285+/-0.032 (F)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:56:24.95 -29:59:57.1: 11.57 +/- 0.04 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:56:24.95 -29:59:57.1: 11.49 +/- 0.04 detection
Forced photometry reference-image weighted average: 11.53 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 04.4307* 01 56 24.95 -29 59 57.1 9.7 U For 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5020725032818724480,2461287.9307,9.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5020725032818724480 20260904.4307 9.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 04.4307 2461287.9307 10.64 01:56:41.16 -30:06:04.1
228.50979 -75.38890 galactic For Second-epoch detections are separated by 1.5" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5020711426362331648 | 01:56:41.21 -30:06:03.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.379+/-0.037 (G)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:56:41.16 -30:06:04.1: 12.68 +/- 0.11 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:56:41.16 -30:06:04.1: 12.62 +/- 0.11 detection
Forced photometry reference-image weighted average: 12.65 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 04.4307* 01 56 41.16 -30 06 04.1 10.6 U For 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5020711426362331648,2461287.9307,10.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5020711426362331648 20260904.4307 10.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 04.4307 2461287.9307 10.93 01:43:15.22 -22:07:30.8
192.71875 -77.21525 galactic Cet Second-epoch detections are separated by 0.8" and 7.8 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 | 01:43:15.22 -22:07:30.8 (user input) | T | P | (position from user input) J-Ks=0.531+/-0.032 (K)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:43:15.22 -22:07:30.8: 12.67 +/- 0.11 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:43:15.22 -22:07:30.8: 12.83 +/- 0.13 detection
Forced photometry reference-image weighted average: 12.73 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 04.4307* 01 43 15.22 -22 07 30.8 10.9 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461287.9307,10.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260904.4307 10.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 04.4307 2461287.9307 10.43 01:35:08.93 -28:14:19.5
222.00330 -80.26311 galactic Scl Second-epoch detections are separated by 0.9" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5035609151787512832 | 01:35:08.90 -28:14:19.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.423+/-0.032 (G)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:35:08.93 -28:14:19.5: 11.51 +/- 0.04 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:35:08.93 -28:14:19.5: 11.57 +/- 0.04 detection
Forced photometry reference-image weighted average: 11.53 +/- 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 5035609151787512832,2461287.9307,10.43,0.05,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 5035609151787512832 20260904.4307 10.43CV 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 04.4307 2461287.9307 10.38 01:37:27.81 -25:16:14.0
205.31282 -79.51405 galactic Scl Second-epoch detections are separated by 1.0" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5038451393641411712 | 01:37:27.83 -25:16:13.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.809+/-0.033 (K)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:37:27.81 -25:16:14.0: 11.50 +/- 0.04 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:37:27.81 -25:16:14.0: 11.40 +/- 0.04 detection
Forced photometry reference-image weighted average: 11.45 +/- 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 5038451393641411712,2461287.9307,10.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5038451393641411712 20260904.4307 10.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 04.4307 2461287.9307 10.44 01:38:47.44 -29:20:56.4
227.71922 -79.34219 galactic Scl Second-epoch detections are separated by 0.2" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5023295209967765248 | 01:38:47.40 -29:20:56.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.316+/-0.030 (F)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:38:47.44 -29:20:56.4: 11.45 +/- 0.04 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:38:47.44 -29:20:56.4: 11.43 +/- 0.04 detection
Forced photometry reference-image weighted average: 11.44 +/- 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 5023295209967765248,2461287.9307,10.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5023295209967765248 20260904.4307 10.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 04.4307 2461287.9307 10.32 01:47:53.30 -23:58:06.9
202.12169 -76.88961 galactic For Second-epoch detections are separated by 0.8" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5038317596820414464 | 01:47:53.30 -23:58:06.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.643+/-0.030 (K)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:47:53.30 -23:58:06.9: 11.45 +/- 0.03 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:47:53.30 -23:58:06.9: 11.49 +/- 0.04 detection
Forced photometry reference-image weighted average: 11.47 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 04.4307* 01 47 53.30 -23 58 06.9 10.3 U For 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5038317596820414464,2461287.9307,10.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5038317596820414464 20260904.4307 10.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 04.4307 2461287.9307 10.43 01:46:58.21 -24:04:45.2
202.32362 -77.12228 galactic For Second-epoch detections are separated by 0.5" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5038294575795223808 | 01:46:58.20 -24:04:44.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.506+/-0.037 (K)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:46:58.21 -24:04:45.2: 11.43 +/- 0.03 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:46:58.21 -24:04:45.2: 11.45 +/- 0.04 detection
Forced photometry reference-image weighted average: 11.44 +/- 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!
TCP 2026 09 04.4307* 01 46 58.21 -24 04 45.2 10.4 U For 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5038294575795223808,2461287.9307,10.43,0.05,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 5038294575795223808 20260904.4307 10.43CV 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 04.4307 2461287.9307 11.17 01:44:29.65 -29:11:22.3
226.02537 -78.13247 galactic Scl Second-epoch detections are separated by 3.1" and 7.4 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 | 01:44:29.65 -29:11:22.3 (user input) | T | P | (position from user input) J-Ks=0.594+/-0.037 (K)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:44:29.65 -29:11:22.3: 13.34 +/- 0.20 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:44:29.65 -29:11:22.3: 13.02 +/- 0.17 detection
Forced photometry reference-image weighted average: 13.15 +/- 0.13
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461287.9307,11.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260904.4307 11.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 04.4307 2461287.9307 11.20 01:55:53.35 -29:45:23.7
227.23055 -75.60311 galactic For Second-epoch detections are separated by 2.9" and 7.4 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 | 01:55:53.35 -29:45:23.7 (user input) | T | P | (position from user input) J-Ks=0.362+/-0.032 (G)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:55:53.35 -29:45:23.7: 13.00 +/- 0.15 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:55:53.35 -29:45:23.7: 12.86 +/- 0.14 detection
Forced photometry reference-image weighted average: 12.93 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 04.4307* 01 55 53.35 -29 45 23.7 11.2 U For 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461287.9307,11.20,0.05,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 20260904.4307 11.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 04.4307 2461287.9307 10.07 01:48:32.24 -23:36:39.7
200.82885 -76.64004 galactic Cet Second-epoch detections are separated by 1.0" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5134408968852040576 | 01:48:32.27 -23:36:39.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.311+/-0.031 (F)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:48:32.24 -23:36:39.7: 11.29 +/- 0.03 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:48:32.24 -23:36:39.7: 11.24 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.26 +/- 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!
TCP 2026 09 04.4307* 01 48 32.24 -23 36 39.7 10.1 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5134408968852040576,2461287.9307,10.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5134408968852040576 20260904.4307 10.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 04.4307 2461287.9307 10.84 01:53:19.14 -29:45:13.3
227.49230 -76.15728 galactic For Second-epoch detections are separated by 1.0" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5023775005058544384 | 01:53:19.14 -29:45:13.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.392+/-0.032 (G)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:53:19.14 -29:45:13.3: 12.49 +/- 0.09 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:53:19.14 -29:45:13.3: 12.48 +/- 0.10 detection
Forced photometry reference-image weighted average: 12.48 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 04.4307* 01 53 19.14 -29 45 13.3 10.8 U For 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5023775005058544384,2461287.9307,10.84,0.05,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
Gaia DR3 5023775005058544384 20260904.4307 10.84CV 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 04.4307 2461287.9307 11.00 01:55:58.76 -29:40:57.2
226.92599 -75.59195 galactic For Second-epoch detections are separated by 0.8" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5020785643396830592 | 01:55:58.79 -29:40:57.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.589+/-0.032 (K)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:55:58.76 -29:40:57.2: 12.49 +/- 0.09 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:55:58.76 -29:40:57.2: 12.58 +/- 0.11 detection
Forced photometry reference-image weighted average: 12.53 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 04.4307* 01 55 58.76 -29 40 57.2 11.0 U For 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5020785643396830592,2461287.9307,11.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 5020785643396830592 20260904.4307 11.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-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 04.4307 2461287.9307 10.09 01:48:50.30 -23:35:23.6
200.83546 -76.56793 galactic Cet Second-epoch detections are separated by 0.6" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5134410343242240768 | 01:48:50.29 -23:35:24.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.423+/-0.037 (G)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:48:50.30 -23:35:23.6: 11.21 +/- 0.03 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:48:50.30 -23:35:23.6: 11.19 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.20 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 04.4307* 01 48 50.30 -23 35 23.6 10.1 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5134410343242240768,2461287.9307,10.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 5134410343242240768 20260904.4307 10.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-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 04.4307 2461287.9307 9.59 01:52:21.21 -29:48:51.7
227.85903 -76.35722 galactic For Second-epoch detections are separated by 2.3" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5023770748747222528 | 01:52:21.12 -29:48:51.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.647+/-0.033 (K)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:52:21.21 -29:48:51.7: 11.18 +/- 0.03 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:52:21.21 -29:48:51.7: 11.13 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.16 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 04.4307* 01 52 21.21 -29 48 51.7 9.6 U For 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5023770748747222528,2461287.9307,9.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5023770748747222528 20260904.4307 9.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 04.4307 2461287.9307 9.99 01:36:09.31 -28:09:26.1
221.44510 -80.04702 galactic Scl Second-epoch detections are separated by 0.4" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5035616474707869056 | 01:36:09.24 -28:09:26.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.721+/-0.056 (K)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:36:09.31 -28:09:26.1: 11.15 +/- 0.03 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:36:09.31 -28:09:26.1: 11.16 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.15 +/- 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 5035616474707869056,2461287.9307,9.99,0.05,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
Gaia DR3 5035616474707869056 20260904.4307 9.99CV 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 04.4307 2461287.9307 10.66 01:53:27.20 -29:46:49.8
227.58808 -76.12500 galactic For Second-epoch detections are separated by 1.0" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5020772346178028032 | 01:53:27.16 -29:46:49.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.353+/-0.031 (G)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:53:27.20 -29:46:49.8: 12.48 +/- 0.09 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:53:27.20 -29:46:49.8: 12.48 +/- 0.10 detection
Forced photometry reference-image weighted average: 12.48 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 04.4307* 01 53 27.20 -29 46 49.8 10.7 U For 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5020772346178028032,2461287.9307,10.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5020772346178028032 20260904.4307 10.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 04.4307 2461287.9307 10.11 01:42:04.66 -28:53:14.0
224.82137 -78.69096 galactic Scl Second-epoch detections are separated by 1.1" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5023324243946147072 | 01:42:04.59 -28:53:14.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.661+/-0.039 (K)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:42:04.66 -28:53:14.0: 11.14 +/- 0.03 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:42:04.66 -28:53:14.0: 11.14 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.14 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 5023324243946147072,2461287.9307,10.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5023324243946147072 20260904.4307 10.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 04.4307 2461287.9307 9.79 01:57:56.14 -30:05:10.3
228.31206 -75.12290 galactic For Second-epoch detections are separated by 6.0" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5020527636121896320 | 01:57:56.32 -30:05:07.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:57:56.14 -30:05:10.3: 11.15 +/- 0.03 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:57:56.14 -30:05:10.3: 11.24 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.19 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 04.4307* 01 57 56.14 -30 05 10.3 9.8 U For 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5020527636121896320,2461287.9307,9.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5020527636121896320 20260904.4307 9.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 04.4307 2461287.9307 9.97 01:43:45.94 -29:08:06.2
225.85234 -78.29683 galactic Scl Second-epoch detections are separated by 0.6" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5023348467562961408 | 01:43:45.95 -29:08:05.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.577+/-0.033 (K)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:43:45.94 -29:08:06.2: 11.12 +/- 0.03 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:43:45.94 -29:08:06.2: 11.13 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.13 +/- 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 5023348467562961408,2461287.9307,9.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5023348467562961408 20260904.4307 9.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 04.4307 2461287.9307 9.67 01:57:36.25 -29:45:18.9
227.06063 -75.23336 galactic For Second-epoch detections are separated by 0.5" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5020828146393134976 | 01:57:36.23 -29:45:19.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.231+/-0.031 (F)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:57:36.25 -29:45:18.9: 11.07 +/- 0.03 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:57:36.25 -29:45:18.9: 11.06 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.06 +/- 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 04.4307* 01 57 36.25 -29 45 18.9 9.7 U For 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5020828146393134976,2461287.9307,9.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5020828146393134976 20260904.4307 9.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 04.4307 2461287.9307 10.72 01:56:51.88 -30:10:26.3
228.77451 -75.34069 galactic For Second-epoch detections are separated by 0.7" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5020707745574637824 | 01:56:53.56 -30:10:58.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.516+/-0.033 (K)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:56:51.88 -30:10:26.3: 12.45 +/- 0.09 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:56:51.88 -30:10:26.3: 12.43 +/- 0.09 detection
Forced photometry reference-image weighted average: 12.44 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 04.4307* 01 56 51.88 -30 10 26.3 10.7 U For 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5020707745574637824,2461287.9307,10.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5020707745574637824 20260904.4307 10.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 04.4307 2461287.9307 9.87 01:38:17.29 -27:49:11.0
219.43483 -79.58937 galactic Scl Second-epoch detections are separated by 0.5" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5035733022940290304 | 01:38:17.29 -27:49:10.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.323+/-0.035 (G)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:38:17.29 -27:49:11.0: 11.06 +/- 0.03 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:38:17.29 -27:49:11.0: 11.11 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.08 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 5035733022940290304,2461287.9307,9.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5035733022940290304 20260904.4307 9.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 04.4307 2461287.9307 9.79 01:38:26.31 -27:49:09.8
219.42955 -79.55614 galactic Scl Second-epoch detections are separated by 0.7" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5035730136722606592 | 01:38:26.32 -27:49:10.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.295+/-0.031 (F)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:38:26.31 -27:49:09.8: 11.01 +/- 0.02 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:38:26.31 -27:49:09.8: 11.00 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.00 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5035730136722606592,2461287.9307,9.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5035730136722606592 20260904.4307 9.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 04.4307 2461287.9307 10.58 01:56:06.75 -29:50:42.3
227.56055 -75.54462 galactic For Second-epoch detections are separated by 0.6" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5020736504675725696 | 01:56:06.78 -29:50:42.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.318+/-0.029 (F)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:56:06.75 -29:50:42.3: 12.39 +/- 0.09 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:56:06.75 -29:50:42.3: 12.39 +/- 0.09 detection
Forced photometry reference-image weighted average: 12.39 +/- 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!
TCP 2026 09 04.4307* 01 56 06.75 -29 50 42.3 10.6 U For 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5020736504675725696,2461287.9307,10.58,0.05,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
Gaia DR3 5020736504675725696 20260904.4307 10.58CV 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 04.4307 2461287.9307 9.91 01:44:12.91 -29:10:48.0
226.01452 -78.19407 galactic Scl Second-epoch detections are separated by 0.3" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5023344997229390208 | 01:44:12.92 -29:10:47.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.289+/-0.033 (F)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:44:12.91 -29:10:48.0: 10.94 +/- 0.02 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:44:12.91 -29:10:48.0: 10.93 +/- 0.02 detection
Forced photometry reference-image weighted average: 10.94 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 5023344997229390208,2461287.9307,9.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5023344997229390208 20260904.4307 9.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 04.4307 2461287.9307 9.46 01:46:35.35 -28:41:26.7
223.44391 -77.72321 galactic For Second-epoch detections are separated by 0.1" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 5023389390010880384 | 01:46:35.25 -28:41:27.7 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:46:35.35 -28:41:26.7: 10.92 +/- 0.02 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:46:35.35 -28:41:26.7: 11.01 +/- 0.02 detection
Forced photometry reference-image weighted average: 10.96 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 04.4307* 01 46 35.35 -28 41 26.7 9.5 U For 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 5023389390010880384,2461287.9307,9.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 5023389390010880384 20260904.4307 9.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 04.4307 2461287.9307 10.68 01:48:07.78 -23:47:16.5
201.43604 -76.78329 galactic For Second-epoch detections are separated by 0.8" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5038328317058337920 | 01:48:07.75 -23:47:16.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.521+/-0.029 (K)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:48:07.78 -23:47:16.5: 12.41 +/- 0.08 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:48:07.78 -23:47:16.5: 12.23 +/- 0.07 detection
Forced photometry reference-image weighted average: 12.31 +/- 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!
TCP 2026 09 04.4307* 01 48 07.78 -23 47 16.5 10.7 U For 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5038328317058337920,2461287.9307,10.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5038328317058337920 20260904.4307 10.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 04.4307 2461287.9307 9.93 01:41:39.03 -21:56:38.8
191.22686 -77.46815 galactic Cet Second-epoch detections are separated by 1.0" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5135606955490641408 | 01:41:39.04 -21:56:38.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.419+/-0.033 (G)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:41:39.03 -21:56:38.8: 10.88 +/- 0.02 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:41:39.03 -21:56:38.8: 10.92 +/- 0.02 detection
Forced photometry reference-image weighted average: 10.90 +/- 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 04.4307* 01 41 39.03 -21 56 38.8 9.9 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5135606955490641408,2461287.9307,9.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5135606955490641408 20260904.4307 9.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 04.4307 2461287.9307 10.85 01:42:20.56 -28:51:00.4
224.60369 -78.63699 galactic Scl Second-epoch detections are separated by 1.3" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5023418149111788672 | 01:42:20.55 -28:51:01.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.671+/-0.035 (K)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:42:20.56 -28:51:00.4: 12.38 +/- 0.09 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:42:20.56 -28:51:00.4: 12.25 +/- 0.08 detection
Forced photometry reference-image weighted average: 12.31 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5023418149111788672,2461287.9307,10.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5023418149111788672 20260904.4307 10.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 04.4307 2461287.9307 10.65 01:46:01.81 -28:59:14.5
224.88758 -77.82053 galactic For Second-epoch detections are separated by 5.1" and 8.1 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 5022626878696871552 | 01:46:01.65 -28:59:12.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:46:01.81 -28:59:14.5: 12.35 +/- 0.08 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:46:01.81 -28:59:14.5: 12.37 +/- 0.09 detection
Forced photometry reference-image weighted average: 12.36 +/- 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!
TCP 2026 09 04.4307* 01 46 01.81 -28 59 14.5 10.7 U For 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5022626878696871552,2461287.9307,10.65,0.05,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 5022626878696871552 20260904.4307 10.65CV 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 04.4307 2461287.9307 9.61 01:35:51.16 -27:52:08.0
219.78870 -80.12638 galactic Scl Second-epoch detections are separated by 0.4" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5035693646680267392 | 01:35:51.15 -27:52:08.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.574+/-0.035 (K)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:35:51.16 -27:52:08.0: 10.69 +/- 0.02 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:35:51.16 -27:52:08.0: 10.72 +/- 0.02 detection
Forced photometry reference-image weighted average: 10.70 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 5035693646680267392,2461287.9307,9.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5035693646680267392 20260904.4307 9.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 04.4307 2461287.9307 9.47 01:56:53.61 -30:10:58.2
228.80577 -75.33329 galactic For Second-epoch detections are separated by 0.5" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5020707745574637824 | 01:56:53.56 -30:10:58.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.356+/-0.038 (G)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:56:53.61 -30:10:58.2: 10.68 +/- 0.02 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:56:53.61 -30:10:58.2: 10.69 +/- 0.02 detection
Forced photometry reference-image weighted average: 10.68 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 04.4307* 01 56 53.61 -30 10 58.2 9.5 U For 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5020707745574637824,2461287.9307,9.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5020707745574637824 20260904.4307 9.47CV 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 04.4307 2461287.9307 9.09 01:57:07.74 -30:04:24.0
228.35067 -75.29760 galactic For Second-epoch detections are separated by 0.3" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5020714621818001024 | 01:57:07.75 -30:04:23.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F8 1954AnCap..17.....J CD-30 678 J-Ks=0.243+/-0.033 (F)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:57:07.74 -30:04:24.0: 10.60 +/- 0.02 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:57:07.74 -30:04:24.0: 10.61 +/- 0.02 detection
Forced photometry reference-image weighted average: 10.60 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 04.4307* 01 57 07.74 -30 04 24.0 9.1 U For 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5020714621818001024,2461287.9307,9.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 5020714621818001024 20260904.4307 9.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-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 04.4307 2461287.9307 9.44 01:52:57.92 -29:50:54.8
227.92771 -76.22116 galactic For Second-epoch detections are separated by 0.3" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5023768206126235264 | 01:52:57.95 -29:50:54.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G 1954AnCap..17.....J CD-30 646 J-Ks=0.377+/-0.033 (G)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:52:57.92 -29:50:54.8: 10.57 +/- 0.02 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:52:57.92 -29:50:54.8: 10.54 +/- 0.02 detection
Forced photometry reference-image weighted average: 10.56 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 04.4307* 01 52 57.92 -29 50 54.8 9.4 U For 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5023768206126235264,2461287.9307,9.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5023768206126235264 20260904.4307 9.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 04.4307 2461287.9307 10.87 01:42:09.84 -25:21:34.3
206.94242 -78.49427 galactic Scl Second-epoch detections are separated by 0.7" and 7.5 pix
The object was found in VSX 0" Gaia DR3 5037751928151886336
Type: VAR
# Max. Min./Amp. JD0 Period
12.200 G 12.240 G 0.022745100000 G
The object was not found in astcheck.
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:42:09.84 -25:21:34.3: 12.30 +/- 0.07 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:42:09.84 -25:21:34.3: 12.32 +/- 0.08 detection
Forced photometry reference-image weighted average: 12.31 +/- 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
Gaia DR3 5037751928151886336,2461287.9307,10.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5037751928151886336 20260904.4307 10.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 04.4307 2461287.9307 11.02 01:48:06.36 -23:28:33.2
200.13694 -76.69073 galactic Cet Second-epoch detections are separated by 3.3" and 8.1 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 | 01:48:06.36 -23:28:33.2 (user input) | T | P | (position from user input) J-Ks=0.383+/-0.028 (G)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:48:06.36 -23:28:33.2: 13.07 +/- 0.14 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:48:06.36 -23:28:33.2: 13.20 +/- 0.18 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.11
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 04.4307* 01 48 06.36 -23 28 33.2 11.0 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461287.9307,11.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260904.4307 11.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 04.4307 2461287.9307 10.76 01:42:57.97 -29:23:14.3
227.20480 -78.43707 galactic Scl Second-epoch detections are separated by 3.7" and 7.9 pix
The object was found in VSX 3" Gaia DR3 5023250885905344640
Type: ROT
# Max. Min./Amp. JD0 Period
11.720 G 11.750 G 0.853940000000 K
The object was not found in astcheck.
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:42:57.97 -29:23:14.3: 12.20 +/- 0.07 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:42:57.97 -29:23:14.3: 12.07 +/- 0.07 detection
Forced photometry reference-image weighted average: 12.13 +/- 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
Gaia DR3 5023250885905344640,2461287.9307,10.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5023250885905344640 20260904.4307 10.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 04.4307 2461287.9307 10.98 01:43:16.94 -22:26:54.3
194.06204 -77.34574 galactic Cet Second-epoch detections are separated by 3.6" and 8.2 pix
The object was found in VSX 1" Gaia DR3 5135529027604044032
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.170 G 12.210 G F
The object was not found in astcheck.
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:43:16.94 -22:26:54.3: 12.25 +/- 0.07 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:43:16.94 -22:26:54.3: 12.21 +/- 0.07 detection
Forced photometry reference-image weighted average: 12.23 +/- 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!
TCP 2026 09 04.4307* 01 43 16.94 -22 26 54.3 11.0 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5135529027604044032,2461287.9307,10.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5135529027604044032 20260904.4307 10.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 04.4307 2461287.9307 8.96 01:58:12.27 -30:13:06.9
228.79211 -75.04780 galactic For Second-epoch detections are separated by 0.4" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5020521417009255424 | 01:58:12.26 -30:13:06.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F3V 1982MSS...C03....0H HD 12104 J-Ks=0.247+/-0.031 (F)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:58:12.27 -30:13:06.9: 10.23 +/- 0.01 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:58:12.27 -30:13:06.9: 10.22 +/- 0.01 detection
Forced photometry reference-image weighted average: 10.22 +/- 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 Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 04.4307* 01 58 12.27 -30 13 06.9 9.0 U For 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5020521417009255424,2461287.9307,8.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5020521417009255424 20260904.4307 8.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 04.4307 2461287.9307 9.14 01:51:06.92 -29:42:30.2
227.56060 -76.63754 galactic For Second-epoch detections are separated by 0.5" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5022287198323294848 | 01:51:06.91 -29:42:30.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G2 1954AnCap..17.....J CD-30 633 J-Ks=0.709+/-0.032 (K)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:51:06.92 -29:42:30.2: 10.15 +/- 0.01 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:51:06.92 -29:42:30.2: 10.15 +/- 0.01 detection
Forced photometry reference-image weighted average: 10.15 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 04.4307* 01 51 06.92 -29 42 30.2 9.1 U For 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5022287198323294848,2461287.9307,9.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 5022287198323294848 20260904.4307 9.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-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 04.4307 2461287.9307 10.42 01:54:40.19 -29:57:10.7
228.15336 -75.84117 galactic For Second-epoch detections are separated by 0.7" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5020755131949125632 | 01:54:40.15 -29:57:10.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.254+/-0.030 (F)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:54:40.19 -29:57:10.7: 12.18 +/- 0.07 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:54:40.19 -29:57:10.7: 12.29 +/- 0.08 detection
Forced photometry reference-image weighted average: 12.23 +/- 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!
TCP 2026 09 04.4307* 01 54 40.19 -29 57 10.7 10.4 U For 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5020755131949125632,2461287.9307,10.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5020755131949125632 20260904.4307 10.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 04.4307 2461287.9307 8.84 01:56:07.84 -29:49:25.4
227.47371 -75.54325 galactic For Second-epoch detections are separated by 0.1" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5020736543330705792 | 01:56:07.85 -29:49:25.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G3/5V 1982MSS...C03....0H HD 11877 J-Ks=0.317+/-0.041 (F)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:56:07.84 -29:49:25.4: 9.97 +/- 0.01 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:56:07.84 -29:49:25.4: 9.94 +/- 0.01 detection
Forced photometry reference-image weighted average: 9.95 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 04.4307* 01 56 07.84 -29 49 25.4 8.8 U For 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5020736543330705792,2461287.9307,8.84,0.05,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
Gaia DR3 5020736543330705792 20260904.4307 8.84CV 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 04.4307 2461287.9307 10.90 01:49:26.96 -22:38:35.0
197.27209 -76.11138 galactic Cet Second-epoch detections are separated by 1.6" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5135277441303970560 | 01:49:26.93 -22:38:34.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.586+/-0.030 (K)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:49:26.96 -22:38:35.0: 12.12 +/- 0.06 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:49:26.96 -22:38:35.0: 12.11 +/- 0.07 detection
Forced photometry reference-image weighted average: 12.12 +/- 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!
TCP 2026 09 04.4307* 01 49 26.96 -22 38 35.0 10.9 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5135277441303970560,2461287.9307,10.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5135277441303970560 20260904.4307 10.90CV 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 04.4307 2461287.9307 10.48 01:43:34.32 -29:03:46.4
225.52210 -78.34712 galactic Scl Second-epoch detections are separated by 0.3" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5023361524262974720 | 01:43:34.28 -29:03:46.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.578+/-0.035 (K)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:43:34.32 -29:03:46.4: 12.07 +/- 0.06 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:43:34.32 -29:03:46.4: 11.95 +/- 0.06 detection
Forced photometry reference-image weighted average: 12.01 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5023361524262974720,2461287.9307,10.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5023361524262974720 20260904.4307 10.48CV 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 04.4307 2461287.9307 10.54 01:58:33.80 -29:46:16.5
227.03594 -75.02468 galactic For Second-epoch detections are separated by 2.8" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5020813990180940800 | 01:58:33.70 -29:46:17.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.397+/-0.031 (G)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:58:33.80 -29:46:16.5: 12.09 +/- 0.06 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:58:33.80 -29:46:16.5: 12.11 +/- 0.07 detection
Forced photometry reference-image weighted average: 12.10 +/- 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!
TCP 2026 09 04.4307* 01 58 33.80 -29 46 16.5 10.5 U For 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5020813990180940800,2461287.9307,10.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5020813990180940800 20260904.4307 10.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 04.4307 2461287.9307 10.89 01:43:18.43 -29:20:02.8
226.89142 -78.37087 galactic Scl Second-epoch detections are separated by 0.9" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5023248549443149312 | 01:43:18.48 -29:20:02.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.353+/-0.032 (G)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:43:18.43 -29:20:02.8: 12.09 +/- 0.06 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:43:18.43 -29:20:02.8: 12.10 +/- 0.07 detection
Forced photometry reference-image weighted average: 12.09 +/- 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
Gaia DR3 5023248549443149312,2461287.9307,10.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5023248549443149312 20260904.4307 10.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 04.4307 2461287.9307 10.54 01:36:41.48 -28:10:08.3
221.47334 -79.92837 galactic Scl Second-epoch detections are separated by 1.6" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5035627023147957376 | 01:36:41.43 -28:10:08.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.451+/-0.035 (G)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:36:41.48 -28:10:08.3: 12.03 +/- 0.06 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:36:41.48 -28:10:08.3: 12.10 +/- 0.07 detection
Forced photometry reference-image weighted average: 12.06 +/- 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
Gaia DR3 5035627023147957376,2461287.9307,10.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5035627023147957376 20260904.4307 10.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 04.4307 2461287.9307 10.84 01:58:07.61 -29:46:39.8
227.10013 -75.11817 galactic For Second-epoch detections are separated by 7.2" and 6.4 pix
The object was found in VSX 4" Gaia DR3 5020816910758704896
Type: ROT
# Max. Min./Amp. JD0 Period
12.480 G 12.520 G K
The object was not found in astcheck.
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:58:07.61 -29:46:39.8: 12.87 +/- 0.13 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:58:07.61 -29:46:39.8: 12.87 +/- 0.14 detection
Forced photometry reference-image weighted average: 12.87 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 04.4307* 01 58 07.61 -29 46 39.8 10.8 U For 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5020816910758704896,2461287.9307,10.84,0.05,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
Gaia DR3 5020816910758704896 20260904.4307 10.84CV 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 04.4307 2461287.9307 10.29 01:54:06.75 -29:47:43.6
227.57538 -75.98123 galactic For Second-epoch detections are separated by 0.4" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5020769734837930112 | 01:54:06.74 -29:47:43.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.310+/-0.034 (F)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:54:06.75 -29:47:43.6: 11.98 +/- 0.06 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:54:06.75 -29:47:43.6: 12.06 +/- 0.07 detection
Forced photometry reference-image weighted average: 12.02 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 04.4307* 01 54 06.75 -29 47 43.6 10.3 U For 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5020769734837930112,2461287.9307,10.29,0.05,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 5020769734837930112 20260904.4307 10.29CV 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 04.4307 2461287.9307 10.87 01:46:52.76 -28:41:22.9
223.41813 -77.65980 galactic For Second-epoch detections are separated by 5.7" and 6.9 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 | 01:46:52.76 -28:41:22.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:46:52.76 -28:41:22.9: 12.96 +/- 0.14 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:46:52.76 -28:41:22.9: 12.89 +/- 0.13 detection
Forced photometry reference-image weighted average: 12.92 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 04.4307* 01 46 52.76 -28 41 22.9 10.9 U For 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461287.9307,10.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260904.4307 10.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 04.4307 2461287.9307 10.52 01:43:22.05 -29:01:52.6
225.39089 -78.39505 galactic Scl Second-epoch detections are separated by 0.7" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5023362516399531264 | 01:43:22.06 -29:01:52.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.468+/-0.033 (K)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:43:22.05 -29:01:52.6: 12.00 +/- 0.06 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:43:22.05 -29:01:52.6: 12.02 +/- 0.07 detection
Forced photometry reference-image weighted average: 12.01 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5023362516399531264,2461287.9307,10.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5023362516399531264 20260904.4307 10.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 04.4307 2461287.9307 10.56 01:46:05.26 -28:35:37.4
223.02147 -77.83952 galactic For Second-epoch detections are separated by 0.4" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5023394024279508224 | 01:46:05.27 -28:35:37.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.409+/-0.034 (G)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:46:05.26 -28:35:37.4: 11.95 +/- 0.06 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:46:05.26 -28:35:37.4: 12.04 +/- 0.06 detection
Forced photometry reference-image weighted average: 11.99 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 04.4307* 01 46 05.26 -28 35 37.4 10.6 U For 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5023394024279508224,2461287.9307,10.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5023394024279508224 20260904.4307 10.56CV 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 04.4307 2461287.9307 10.46 01:44:52.71 -29:15:00.1
226.26749 -78.04195 galactic Scl Second-epoch detections are separated by 1.3" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5022593927707758464 | 01:44:52.70 -29:15:00.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.278+/-0.033 (F)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:44:52.71 -29:15:00.1: 11.99 +/- 0.06 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:44:52.71 -29:15:00.1: 11.96 +/- 0.06 detection
Forced photometry reference-image weighted average: 11.97 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5022593927707758464,2461287.9307,10.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5022593927707758464 20260904.4307 10.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 04.4307 2461287.9307 10.86 01:44:59.72 -29:05:47.2
225.51722 -78.03434 galactic Scl Second-epoch detections are separated by 0.6" and 7.2 pix
The object was found in VSX 0" Gaia DR3 5022601899167058560
Type: ROT
# Max. Min./Amp. JD0 Period
12.410 G 12.450 G K
The object was not found in astcheck.
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:44:59.72 -29:05:47.2: 12.80 +/- 0.12 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:44:59.72 -29:05:47.2: 12.67 +/- 0.12 detection
Forced photometry reference-image weighted average: 12.73 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5022601899167058560,2461287.9307,10.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5022601899167058560 20260904.4307 10.86CV 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 04.4307 2461287.9307 10.39 01:47:57.96 -23:50:54.6
201.63990 -76.83721 galactic For Second-epoch detections are separated by 0.1" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5038327522488873472 | 01:47:57.93 -23:50:54.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.335+/-0.030 (G)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:47:57.96 -23:50:54.6: 11.88 +/- 0.05 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:47:57.96 -23:50:54.6: 11.88 +/- 0.05 detection
Forced photometry reference-image weighted average: 11.88 +/- 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!
TCP 2026 09 04.4307* 01 47 57.96 -23 50 54.6 10.4 U For 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5038327522488873472,2461287.9307,10.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5038327522488873472 20260904.4307 10.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461242.96007139 21.07.2026 11:02:20.168 /data_ssd/NMW-TexasTech/reference_imgs/For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits
First image: 2461242.96007139 21.07.2026 11:02:20.168 /data_ssd/NMW-TexasTech/reference_imgs/For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits
Last image: 2461287.93103405 04.09.2026 10:20:31.342 /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_For-01-Q2b1x1_052356_TTUQ2b1x1_2819419_mo17MjFd/fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707.fits
JD time system (TT/UTC/UNKNOWN): UTC
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -9.35
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: 2 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): 1022
Objects passed selection criteria: 1017
Measurements per detected object (mean, median, min, max): 2.1 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.1 2.0 2 4
Average stars detected per image: 571.25
Average stars matched: 562.25 (98.4245 %)
Memory usage VmPeak: 228220 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 Fri Sep 4 05:26:24 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461242.96007139 21.07.2026 11:02:20.168 /data_ssd/NMW-TexasTech/reference_imgs/For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits
First image: 2461242.96007139 21.07.2026 11:02:20.168 /data_ssd/NMW-TexasTech/reference_imgs/For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits
Last image: 2461287.93103405 04.09.2026 10:20:31.342 /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_For-01-Q2b1x1_052356_TTUQ2b1x1_2819419_mo17MjFd/fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 107
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -9.07
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 5 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 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): 6169
Objects passed selection criteria: 6151
Measurements per detected object (mean, median, min, max): 2.3 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.3 2.0 2 4
Average stars detected per image: 4022.75
Average stars matched: 3764.25 (93.574 %)
Memory usage VmPeak: 233160 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 Fri Sep 4 05:27:40 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/For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits /data_ssd/NMW-TexasTech/reference_imgs/For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_For-01-Q2b1x1_052356_TTUQ2b1x1_2819419_mo17MjFd/fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_For-01-Q2b1x1_052356_TTUQ2b1x1_2819419_mo17MjFd/fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707.fits
SExtractor catalog cache: saved For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits.cat to cache
SExtractor catalog cache: saved For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.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/For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits /data_ssd/NMW-TexasTech/reference_imgs/For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_For-01-Q2b1x1_052356_TTUQ2b1x1_2819419_mo17MjFd/fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_For-01-Q2b1x1_052356_TTUQ2b1x1_2819419_mo17MjFd/fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707.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: 2461287.93032927
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits exists and is non-empty
wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits exists and is non-empty
wcs_fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits exists and is non-empty
wcs_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits (1st reference image)
verification OK: wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits
Image size: 941.4'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 01:55:22.664 -26:00:04.01 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_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits (1st new image)
verification OK: wcs_fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits
Image size: 937.2'x624.5' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 01:55:13.477 -25:58:17.11 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 01:55:22.664 -26:00:04.01
Second-epoch image center 01:55:13.477 -25:58:17.11
Angular distance between the image centers 0.0454 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707.fits (2nd new image)
verification OK: wcs_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707.fits
Image size: 937.2'x624.5' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 01:55:16.474 -25:58:36.27 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 01:55:22.664 -26:00:04.01
Second-epoch image center 01:55:16.474 -25:58:36.27
Angular distance between the image centers 0.0336 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 01:55:13.477 -25:58:17.11
Second-epoch second image center 01:55:16.474 -25:58:36.27
Angular distance between the image centers 0.01242 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/For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits &> /tmp/tmp.D6yurpoKk1
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits &> /tmp/tmp.GqA0dR6QHp
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_For-01-Q2b1x1_052356_TTUQ2b1x1_2819419_mo17MjFd/fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits &> /tmp/tmp.TmwFnpW4Yq
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_For-01-Q2b1x1_052356_TTUQ2b1x1_2819419_mo17MjFd/fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_For-01-Q2b1x1_052356_TTUQ2b1x1_2819419_mo17MjFd/fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707.fits &> /tmp/tmp.UWT58rdCCt
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_For-01-Q2b1x1_052356_TTUQ2b1x1_2819419_mo17MjFd/fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707.fits
Calibrating the magnitude scale
Found non-empty wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.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_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits and wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.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_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits and wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits.wcscat
Found non-empty wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits and wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits.wcscat
The reference image (wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits) and catalog (wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits.wcscat) found
'wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits.wcscat' -> 'wcsmag.cat'
Read 1410 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 19.5210 to 37.6556 deg, Dec -31.4428 to -20.2852 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 19.5210 to 37.6556 deg, Dec -31.4428 to -20.2852 deg
Loaded 4541 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): 1056 out of 1077 total matches.
Matched with Tycho-2 1077 out of 1410 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.598350
a=0.000000 b=1.000000 c=22.598350
From vast_summary.log: estimated ref. image limiting mag.: -9.35
Updating vast_summary.log: Estimated ref. image limiting mag.: 13.25
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 13.25
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 1410 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 19.5210 to 37.6556 deg, Dec -31.4428 to -20.2852 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 19.5210 to 37.6556 deg, Dec -31.4428 to -20.2852 deg
Loaded 4541 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): 1056 out of 1077 total matches.
Matched with Tycho-2 1077 out of 1410 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits
Forced-photometry filter: calibrated wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits -> calib.txt_param_ref_wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits (aperture=6.5)
Read 1319 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 19.5208 to 37.6551 deg, Dec -31.4009 to -20.2852 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 19.5208 to 37.6551 deg, Dec -31.4009 to -20.2852 deg
Loaded 4524 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): 969 out of 996 total matches.
Matched with Tycho-2 996 out of 1319 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits
Forced-photometry filter: calibrated wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits -> calib.txt_param_ref_wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits (aperture=6.4)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.8 pix For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits
2.7 pix For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits
2.2 pix fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits
2.2 pix fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707.fits
Limiting magnitude estimates:
13.3 mag. For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits
13.2 mag. For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits
11.4 mag. fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits
11.0 mag. fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707.fits
All-image limiting magnitude estimate: 11.0 (SNR ) 8.5 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
cp: cannot create regular file 'local_wcs_cache/': Not a directory
############ /tmp/tmp.D6yurpoKk1 (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/For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.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_2026-09-04_CI_For-01-Q2b1x1_052356_TTUQ2b1x1_2819419_mo17MjFd/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits 574.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits' -> 'wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.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/For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits
WCS_IMAGE_NAME=wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits
WCS-calibrated image found: wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits
Checking if the catalog wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits.wcscat corresponding to the image wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits alredy exist and is non-empty...
Catalog wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits.wcscat corresponding to the image wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits
WCS catalog name: wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.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=0, blended=215, bad_region=306, passed=1410
Got 1410 stars (including 952 good ones) from the SExtractor catalog wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits.wcscat
util/solve_plate_with_UCAC5 got 1410 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (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 292 to 350 (Dec -31.4 to -20.3)
Done reading UCAC5 zone files...
Matched 941 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 941 matched stars entering correct_measured_positions(), 933 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 941 matched stars entering correct_measured_positions(), 1122 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
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 292 to 350 (Dec -31.4 to -20.3)
Done reading UCAC5 zone files...
Matched 940 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 940 matched stars entering correct_measured_positions(), 1121 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 940 matched stars entering correct_measured_positions(), 1121 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 940 stars left (next iteration limit 1035)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits N_match=940 sigma_overall_arcsec=0.300 sigma_q1_arcsec=0.299 sigma_q2_arcsec=0.270 sigma_q3_arcsec=0.297 sigma_q4_arcsec=0.298 n_q1=303 n_q2=192 n_q3=280 n_q4=165 worst_quadrant_to_overall_ratio=0.996
The image catalog is written to wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits -region wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.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.GqA0dR6QHp (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/For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.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_2026-09-04_CI_For-01-Q2b1x1_052356_TTUQ2b1x1_2819419_mo17MjFd/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits 574.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits' -> 'wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.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/For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits
WCS_IMAGE_NAME=wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits
WCS-calibrated image found: wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits
Checking if the catalog wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits.wcscat corresponding to the image wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits alredy exist and is non-empty...
Catalog wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits.wcscat corresponding to the image wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits
WCS catalog name: wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.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=0, blended=225, bad_region=280, passed=1319
Got 1319 stars (including 881 good ones) from the SExtractor catalog wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits.wcscat
util/solve_plate_with_UCAC5 got 1319 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (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 292 to 350 (Dec -31.4 to -20.3)
Done reading UCAC5 zone files...
Matched 870 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 870 matched stars entering correct_measured_positions(), 861 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 870 matched stars entering correct_measured_positions(), 1054 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
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 292 to 350 (Dec -31.4 to -20.3)
Done reading UCAC5 zone files...
Matched 870 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 870 matched stars entering correct_measured_positions(), 1053 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 870 matched stars entering correct_measured_positions(), 1053 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 870 stars left (next iteration limit 957)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits N_match=870 sigma_overall_arcsec=0.315 sigma_q1_arcsec=0.371 sigma_q2_arcsec=0.332 sigma_q3_arcsec=0.282 sigma_q4_arcsec=0.312 n_q1=277 n_q2=181 n_q3=262 n_q4=150 worst_quadrant_to_overall_ratio=1.178
The image catalog is written to wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits -region wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.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.TmwFnpW4Yq (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_2026-09-04_CI_For-01-Q2b1x1_052356_TTUQ2b1x1_2819419_mo17MjFd/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_For-01-Q2b1x1_052356_TTUQ2b1x1_2819419_mo17MjFd/fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_For-01-Q2b1x1_052356_TTUQ2b1x1_2819419_mo17MjFd/fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_For-01-Q2b1x1_052356_TTUQ2b1x1_2819419_mo17MjFd/fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_For-01-Q2b1x1_052356_TTUQ2b1x1_2819419_mo17MjFd/fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_For-01-Q2b1x1_052356_TTUQ2b1x1_2819419_mo17MjFd/fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.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_2026-09-04_CI_For-01-Q2b1x1_052356_TTUQ2b1x1_2819419_mo17MjFd/fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits
WCS_IMAGE_NAME=wcs_fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits
WCS-calibrated image found: wcs_fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits
Checking if the catalog wcs_fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits.wcscat corresponding to the image wcs_fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits alredy exist and is non-empty...
Catalog wcs_fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits.wcscat corresponding to the image wcs_fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_For-01-Q2b1x1_052356_TTUQ2b1x1_2819419_mo17MjFd/fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits
WCS catalog name: wcs_fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.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=0, blended=11, bad_region=38, passed=100
Got 100 stars (including 54 good ones) from the SExtractor catalog wcs_fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits.wcscat
util/solve_plate_with_UCAC5 got 100 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 294 to 348 (Dec -31.1 to -20.7)
Done reading UCAC5 zone files...
Matched 46 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Retrying with a larger catalog search radius.
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 294 to 348 (Dec -31.1 to -20.7)
Done reading UCAC5 zone files...
Matched 47 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 46 matched stars entering correct_measured_positions(), 1 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.96"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 46 matched stars entering correct_measured_positions(), 1 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
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 294 to 348 (Dec -31.1 to -20.7)
Done reading UCAC5 zone files...
Matched 46 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 46 matched stars entering correct_measured_positions(), 1 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
Accuracy estimation diagnostic: 46 matched stars entering correct_measured_positions(), 1 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
Excluding outliers - 46 stars left (next iteration limit 50)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: only 46 catalog matches (<100) - keeping the original solution
WCS_QUALITY_DIAG: file=fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits N_match=46 sigma_overall_arcsec=0.661 sigma_q1_arcsec=0.923 sigma_q2_arcsec=0.590 sigma_q3_arcsec=0.614 sigma_q4_arcsec=0.717 n_q1=8 n_q2=12 n_q3=14 n_q4=12 worst_quadrant_to_overall_ratio=1.397
The image catalog is written to wcs_fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_For-01-Q2b1x1_052356_TTUQ2b1x1_2819419_mo17MjFd/fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits -region wcs_fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.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.UWT58rdCCt (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_2026-09-04_CI_For-01-Q2b1x1_052356_TTUQ2b1x1_2819419_mo17MjFd/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_For-01-Q2b1x1_052356_TTUQ2b1x1_2819419_mo17MjFd/fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_For-01-Q2b1x1_052356_TTUQ2b1x1_2819419_mo17MjFd/fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_For-01-Q2b1x1_052356_TTUQ2b1x1_2819419_mo17MjFd/fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_For-01-Q2b1x1_052356_TTUQ2b1x1_2819419_mo17MjFd/fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_For-01-Q2b1x1_052356_TTUQ2b1x1_2819419_mo17MjFd/fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707.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_2026-09-04_CI_For-01-Q2b1x1_052356_TTUQ2b1x1_2819419_mo17MjFd/fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707.fits
WCS_IMAGE_NAME=wcs_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707.fits
WCS-calibrated image found: wcs_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707.fits
Checking if the catalog wcs_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707.fits.wcscat corresponding to the image wcs_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707.fits alredy exist and is non-empty...
Catalog wcs_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707.fits.wcscat corresponding to the image wcs_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_For-01-Q2b1x1_052356_TTUQ2b1x1_2819419_mo17MjFd/fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707.fits
WCS catalog name: wcs_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707.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=0, blended=15, bad_region=55, passed=146
Got 146 stars (including 82 good ones) from the SExtractor catalog wcs_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707.fits.wcscat
util/solve_plate_with_UCAC5 got 146 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 294 to 348 (Dec -31.1 to -20.7)
Done reading UCAC5 zone files...
Matched 74 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 74 matched stars entering correct_measured_positions(), 6 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.77"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 74 matched stars entering correct_measured_positions(), 9 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.90"
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 294 to 348 (Dec -31.1 to -20.7)
Done reading UCAC5 zone files...
Matched 73 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 73 matched stars entering correct_measured_positions(), 9 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.97"
Accuracy estimation diagnostic: 73 matched stars entering correct_measured_positions(), 8 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.03"
Excluding outliers - 73 stars left (next iteration limit 81)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: only 73 catalog matches (<100) - keeping the original solution
WCS_QUALITY_DIAG: file=fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707.fits N_match=73 sigma_overall_arcsec=0.543 sigma_q1_arcsec=0.646 sigma_q2_arcsec=0.474 sigma_q3_arcsec=0.588 sigma_q4_arcsec=0.935 n_q1=16 n_q2=20 n_q3=27 n_q4=10 worst_quadrant_to_overall_ratio=1.722
The image catalog is written to wcs_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_For-01-Q2b1x1_052356_TTUQ2b1x1_2819419_mo17MjFd/fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707.fits -region wcs_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707.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
Saving the final (post-refit) wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits to local_wcs_cache/
'wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits' -> 'local_wcs_cache/wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits'
Saving the final (post-refit) wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits to local_wcs_cache/
'wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits' -> 'local_wcs_cache/wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits'
Saving the final (post-refit) wcs_fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits to local_wcs_cache/
'wcs_fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits' -> 'local_wcs_cache/wcs_fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits'
Saving the final (post-refit) wcs_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707.fits to local_wcs_cache/
'wcs_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707.fits' -> 'local_wcs_cache/wcs_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits sigma_overall=0.300 worst_q_ratio=0.996
ref2=For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits sigma_overall=0.315 worst_q_ratio=1.178
new1=fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits sigma_overall=0.661 worst_q_ratio=1.397
new2=fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707.fits sigma_overall=0.543 worst_q_ratio=1.722
reference average sigma_overall=0.3075 worst_q_ratio=1.087
warn-on-ratio threshold: 2.0x reference
###################################
WCS_QUALITY_RETRY: 1st new image (fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits) flagged: sigma=0.661 (ref avg 0.3075), ratio=1.397 (ref avg 1.087), threshold=2.0x. Retrying with --tweak-order 2.
Running with VAST_TWEAK_ORDER=2: util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_For-01-Q2b1x1_052356_TTUQ2b1x1_2819419_mo17MjFd/fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits
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_2026-09-04_CI_For-01-Q2b1x1_052356_TTUQ2b1x1_2819419_mo17MjFd/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_For-01-Q2b1x1_052356_TTUQ2b1x1_2819419_mo17MjFd/fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_For-01-Q2b1x1_052356_TTUQ2b1x1_2819419_mo17MjFd/fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_For-01-Q2b1x1_052356_TTUQ2b1x1_2819419_mo17MjFd/fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_For-01-Q2b1x1_052356_TTUQ2b1x1_2819419_mo17MjFd/fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_For-01-Q2b1x1_052356_TTUQ2b1x1_2819419_mo17MjFd/fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.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_2026-09-04_CI_For-01-Q2b1x1_052356_TTUQ2b1x1_2819419_mo17MjFd/fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits
WCS_IMAGE_NAME=wcs_fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits
No image with WCS calibration found for /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_For-01-Q2b1x1_052356_TTUQ2b1x1_2819419_mo17MjFd/fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits .... Determining astrometry method...
Using the local copy of Astrometry.net software...
Choosing aperture...
Using the catalog image00003.cat SExtracted earlier from the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_For-01-Q2b1x1_052356_TTUQ2b1x1_2819419_mo17MjFd/fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-04_CI_For-01-Q2b1x1_052356_TTUQ2b1x1_2819419_mo17MjFd/lib/make_outxyls_for_astrometric_calibration found 99 high-SNR stars for plate solving
This service uses tools provided by Astrometry.net.
For more information visit http://astrometry.net/
######### Trying to solve plate assuming 605' field of view #########
/data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_For-01-Q2b1x1_052356_TTUQ2b1x1_2819419_mo17MjFd/fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits
Using the local copy of Astrometry.net code
IMAGE_SIZE= --width 9576 --height 6388 SCALE_LOW=544.5 SCALE_HIGH=3025.0
Using solve-field binary
/usr/local/astrometry/bin/solve-field
Reading input file 1 of 1: "out3009218.xyls"...
Reading sort column "FLUX_APER"
Sorting sort column
mmapping input file
Copying table header.
Writing row 0
Done
Solving...
Reading file "./out3009218.axy"...
Field 1 did not solve (index index-4119.fits, field objects 1-10).
Field 1 did not solve (index index-4118.fits, field objects 1-10).
Field 1 did not solve (index index-4117.fits, field objects 1-10).
Field 1 did not solve (index index-4116.fits, field objects 1-10).
Field 1 did not solve (index index-4115.fits, field objects 1-10).
Field 1 did not solve (index index-4114.fits, field objects 1-10).
Field 1 did not solve (index index-4113.fits, field objects 1-10).
Field 1 did not solve (index index-4112.fits, field objects 1-10).
Field 1 did not solve (index index-4111.fits, field objects 1-10).
Field 1 did not solve (index index-4110.fits, field objects 1-10).
Field 1 did not solve (index index-4109.fits, field objects 1-10).
Field 1 did not solve (index index-4108.fits, field objects 1-10).
Field 1 did not solve (index index-4119.fits, field objects 11-20).
Field 1 did not solve (index index-4118.fits, field objects 11-20).
log-odds ratio 84.9902 (8.14248e+36), 10 match, 0 conflict, 62 distractors, 16 index.
RA,Dec = (28.8089,-25.9721), pixel scale 5.95144 arcsec/pix.
Hit/miss: Hit/miss: -++---++---+---------+--+----+--------+--------------------------------+(best)------------------------+++
Field 1: solved with index index-4117.fits.
Field 1 solved: writing to file ./out3009218.solved to indicate this.
Field: out3009218.xyls
Field center: (RA,Dec) = (28.803413, -25.968768) deg.
Field center: (RA H:M:S, Dec D:M:S) = (01:55:12.819, -25:58:07.563).
Field size: 15.723 x 10.5387 degrees
Field rotation angle: up is 179.897 degrees E of N
Field parity: neg
Inserting WCS header... '/data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_For-01-Q2b1x1_052356_TTUQ2b1x1_2819419_mo17MjFd/fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits' -> 'fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits'
WCS keywords and Astrometry.net provenance markers have been successfully stripped from all HDUs in the file.
-rw-r--r-- 1 apache apache 117M Sep 4 05:27 fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits
-rw-r--r-- 1 apache apache 12K Sep 4 05:27 out3009218.wcs
Inserting WCS header (1st iteration local)... Opening FITS image file fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits for reading... done!
Creating new image file (wcs_fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits)... done!
done!
All done!
done
The WCS header appears to be added with no errors in /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_For-01-Q2b1x1_052356_TTUQ2b1x1_2819419_mo17MjFd/fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits (fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits)
Keyword does not exist
Keyword has been changed to:
VAST001 = 'wcs_image_calibration.sh' / VaST script name
Keyword does not exist
Keyword has been changed to:
VAST002 = 'local ' / ASTROMETRYNET_LOCAL_OR_REMOTE
Keyword does not exist
Keyword has been changed to:
VAST003 = 'local ' / PLATE_SOLVE_SERVER
Keyword does not exist
Keyword has been changed to:
VAST004 = 'iteration01' / astrometry.net run
Reading input file 1 of 1: "out3009218.xyls"...
Reading sort column "FLUX_APER"
Sorting sort column
mmapping input file
Copying table header.
Writing row 0
Done
Solving...
Reading file "./out3009218.axy"...
Only searching for solutions within 15.6517 degrees of RA,Dec (28.8025,-25.9696)
log-odds ratio 84.8549 (7.11224e+36), 11 match, 0 conflict, 16 distractors, 28 index.
RA,Dec = (28.8095,-25.9725), pixel scale 5.95566 arcsec/pix.
Hit/miss: Hit/miss: +--+-++++----++-----++----+(best)----------------------------------------------+-+---+----------------+++
Field 1: solved with index index-4116.fits.
Field 1 solved: writing to file ./out3009218.solved to indicate this.
Field: out3009218.xyls
Field center: (RA,Dec) = (28.806621, -25.968631) deg.
Field center: (RA H:M:S, Dec D:M:S) = (01:55:13.589, -25:58:07.073).
Field size: 15.7295 x 10.5396 degrees
Field rotation angle: up is 179.909 degrees E of N
Field parity: neg
WCS keywords and Astrometry.net provenance markers have been successfully stripped from all HDUs in the file.
-rw-r--r-- 1 apache apache 117M Sep 4 05:27 fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits
-rw-r--r-- 1 apache apache 12K Sep 4 05:27 out3009218.wcs
Inserting WCS header (2nd iteration local)... Opening FITS image file fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits for reading... done!
Creating new image file (wcs_fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits)... done!
done!
All done!
The WCS header appears to be added with no errors.
Keyword does not exist
Keyword has been changed to:
VAST001 = 'wcs_image_calibration.sh' / VaST script name
Keyword does not exist
Keyword has been changed to:
VAST002 = 'local ' / ASTROMETRYNET_LOCAL_OR_REMOTE
Keyword does not exist
Keyword has been changed to:
VAST003 = 'local ' / PLATE_SOLVE_SERVER
Keyword does not exist
Keyword has been changed to:
VAST004 = 'iteration02' / astrometry.net run
Checking if the catalog wcs_fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits.wcscat corresponding to the image wcs_fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits alredy exist and is non-empty...
Catalog wcs_fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits.wcscat corresponding to the image wcs_fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits was not found.
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_For-01-Q2b1x1_052356_TTUQ2b1x1_2819419_mo17MjFd/fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits
verification OK: wcs_fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits
Generating wcs_fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits.wcscat from image00003.cat
Catalog wcs_fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits.wcscat corresponding to the image wcs_fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits created.
verification OK: wcs_fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits
verification OK: wcs_fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits
Image size: 938.9'x626.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.88"/pix along the Y axis
Image center: 01:55:13.369 -25:58:10.06 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 100 stars ###
'wcs_fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-09-04_CI_For-01-Q2b1x1_052356_TTUQ2b1x1_2819419_mo17MjFd/correct_sextractor_wcs_catalog_usingxy2sky3017255.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
The plate-solved (WCS-calibrated) image is saved to wcs_fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_For-01-Q2b1x1_052356_TTUQ2b1x1_2819419_mo17MjFd/fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits
WCS catalog name: wcs_fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.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=0, blended=11, bad_region=38, passed=100
Got 100 stars (including 54 good ones) from the SExtractor catalog wcs_fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits.wcscat
util/solve_plate_with_UCAC5 got 100 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.9'
Seting catalog search parameters based on the expected field of view 938.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013040 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010432 (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 294 to 348 (Dec -31.1 to -20.7)
Done reading UCAC5 zone files...
Matched 46 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Retrying with a larger catalog search radius.
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 294 to 348 (Dec -31.1 to -20.7)
Done reading UCAC5 zone files...
Matched 48 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 46 matched stars entering correct_measured_positions(), 2 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 3.27"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 46 matched stars entering correct_measured_positions(), 2 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.21"
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 294 to 348 (Dec -31.1 to -20.7)
Done reading UCAC5 zone files...
Matched 47 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 46 matched stars entering correct_measured_positions(), 1 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.08"
Accuracy estimation diagnostic: 46 matched stars entering correct_measured_positions(), 1 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.46"
Excluding outliers - 46 stars left (next iteration limit 50)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: only 46 catalog matches (<100) - keeping the original solution
WCS_QUALITY_DIAG: file=fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits N_match=46 sigma_overall_arcsec=7.690 sigma_q1_arcsec=4.620 sigma_q2_arcsec=6.151 sigma_q3_arcsec=6.492 sigma_q4_arcsec=5.591 n_q1=8 n_q2=12 n_q3=14 n_q4=12 worst_quadrant_to_overall_ratio=0.844
The image catalog is written to wcs_fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_For-01-Q2b1x1_052356_TTUQ2b1x1_2819419_mo17MjFd/fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits -region wcs_fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.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
WCS_QUALITY_RETRY: --tweak-order 2 did NOT improve 1st new image (fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits): sigma 0.661->7.690, ratio 1.397->0.844; reverting to order 3
WARNING: 1st new image has sigma_overall_arcsec=7.690 -- 25.01x the reference average (0.3075); plate solution may be of low accuracy
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897_astrometric_residuals.png (940 matched stars from wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.28 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898_astrometric_residuals.png (870 matched stars from wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.30 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706_astrometric_residuals.png (46 matched stars from wcs_fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.60 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707_astrometric_residuals.png (73 matched stars from wcs_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.58 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_For-01-Q2b1x1_052356_TTUQ2b1x1_2819419_mo17MjFd/wcs_fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits'
Saving fully-calibrated image wcs_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_For-01-Q2b1x1_052356_TTUQ2b1x1_2819419_mo17MjFd/wcs_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707.fits'
Preparing the HTML report for the field For-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field For-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits /data_ssd/NMW-TexasTech/reference_imgs/For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_For-01-Q2b1x1_052356_TTUQ2b1x1_2819419_mo17MjFd/fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_For-01-Q2b1x1_052356_TTUQ2b1x1_2819419_mo17MjFd/fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707.fits
SExtractor catalog cache: saved For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits.cat to cache
SExtractor catalog cache: saved For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits /data_ssd/NMW-TexasTech/reference_imgs/For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_For-01-Q2b1x1_052356_TTUQ2b1x1_2819419_mo17MjFd/fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_For-01-Q2b1x1_052356_TTUQ2b1x1_2819419_mo17MjFd/fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits
Creating symlink local_wcs_cache/wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits
Creating symlink local_wcs_cache/wcs_fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits
Creating symlink local_wcs_cache/wcs_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707.fits
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits exists and is non-empty
wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits exists and is non-empty
wcs_fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits exists and is non-empty
wcs_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits (1st reference image)
verification OK: wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits
Image size: 941.4'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 01:55:22.664 -26:00:04.01 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_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits (1st new image)
verification OK: wcs_fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits
Image size: 937.2'x624.5' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 01:55:13.477 -25:58:17.11 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 01:55:22.664 -26:00:04.01
Second-epoch image center 01:55:13.477 -25:58:17.11
Angular distance between the image centers 0.0454 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707.fits (2nd new image)
verification OK: wcs_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707.fits
Image size: 937.2'x624.5' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 01:55:16.474 -25:58:36.27 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 01:55:22.664 -26:00:04.01
Second-epoch image center 01:55:16.474 -25:58:36.27
Angular distance between the image centers 0.0336 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 01:55:13.477 -25:58:17.11
Second-epoch second image center 01:55:16.474 -25:58:36.27
Angular distance between the image centers 0.01242 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/For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits &> /tmp/tmp.I0dpxKvodK
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits &> /tmp/tmp.OooxOw7Gnu
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_For-01-Q2b1x1_052356_TTUQ2b1x1_2819419_mo17MjFd/fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits &> /tmp/tmp.zhI5l8jmns
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_For-01-Q2b1x1_052356_TTUQ2b1x1_2819419_mo17MjFd/fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_For-01-Q2b1x1_052356_TTUQ2b1x1_2819419_mo17MjFd/fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707.fits &> /tmp/tmp.qPILQ5pGuV
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_For-01-Q2b1x1_052356_TTUQ2b1x1_2819419_mo17MjFd/fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707.fits
Calibrating the magnitude scale
Found non-empty wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.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_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits and wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.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_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits and wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits.wcscat
Found non-empty wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits and wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits.wcscat
The reference image (wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits) and catalog (wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits.wcscat) found
'wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits.wcscat' -> 'wcsmag.cat'
Read 8445 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 19.4281 to 37.6591 deg, Dec -31.4428 to -20.1306 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 19.4281 to 37.6591 deg, Dec -31.4428 to -20.1306 deg
Loaded 4632 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): 3537 out of 3586 total matches.
Matched with Tycho-2 3586 out of 8445 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.468500
a=0.000000 b=1.000000 c=22.468500
From vast_summary.log: estimated ref. image limiting mag.: -9.07
Updating vast_summary.log: Estimated ref. image limiting mag.: 13.40
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 13.40
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 8445 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 19.4281 to 37.6591 deg, Dec -31.4428 to -20.1306 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 19.4281 to 37.6591 deg, Dec -31.4428 to -20.1306 deg
Loaded 4632 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): 3537 out of 3586 total matches.
Matched with Tycho-2 3586 out of 8445 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits
Forced-photometry filter: calibrated wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits -> calib.txt_param_ref_wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits (aperture=5.2)
Read 7913 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 19.4274 to 37.6551 deg, Dec -31.4418 to -20.1302 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 19.4274 to 37.6551 deg, Dec -31.4418 to -20.1302 deg
Loaded 4630 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): 3535 out of 3585 total matches.
Matched with Tycho-2 3585 out of 7913 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits
Forced-photometry filter: calibrated wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits -> calib.txt_param_ref_wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits (aperture=5.2)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 78 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.5 pix For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits
2.5 pix For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits
2.0 pix fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits
2.0 pix fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707.fits
Limiting magnitude estimates:
13.4 mag. For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits
13.3 mag. For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits
11.4 mag. fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits
11.2 mag. fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707.fits
All-image limiting magnitude estimate: 11.2 (SNR ) 11.1 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.I0dpxKvodK (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/For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.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_2026-09-04_CI_For-01-Q2b1x1_052356_TTUQ2b1x1_2819419_mo17MjFd/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits 574.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits' -> 'wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.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/For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits
WCS_IMAGE_NAME=wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits
WCS-calibrated image found: wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits
Checking if the catalog wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits.wcscat corresponding to the image wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits alredy exist and is non-empty...
Catalog wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits.wcscat corresponding to the image wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits
WCS catalog name: wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.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=1, blended=258, bad_region=1593, passed=8444
Got 8444 stars (including 6669 good ones) from the SExtractor catalog wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits.wcscat
util/solve_plate_with_UCAC5 got 8444 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (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 292 to 351 (Dec -31.4 to -20.1)
Done reading UCAC5 zone files...
Matched 4819 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4814 matched stars entering correct_measured_positions(), 4814 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4814 matched stars entering correct_measured_positions(), 7196 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
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 292 to 351 (Dec -31.4 to -20.1)
Done reading UCAC5 zone files...
Matched 4820 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4813 matched stars entering correct_measured_positions(), 7196 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
Accuracy estimation diagnostic: 4813 matched stars entering correct_measured_positions(), 7196 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
Excluding outliers - 4813 stars left (next iteration limit 5295)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits N_match=4813 sigma_overall_arcsec=0.582 sigma_q1_arcsec=0.717 sigma_q2_arcsec=0.603 sigma_q3_arcsec=0.521 sigma_q4_arcsec=0.524 n_q1=1493 n_q2=882 n_q3=1519 n_q4=919 worst_quadrant_to_overall_ratio=1.231
The image catalog is written to wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits -region wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.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.OooxOw7Gnu (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/For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.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_2026-09-04_CI_For-01-Q2b1x1_052356_TTUQ2b1x1_2819419_mo17MjFd/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits 574.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits' -> 'wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.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/For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits
WCS_IMAGE_NAME=wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits
WCS-calibrated image found: wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits
Checking if the catalog wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits.wcscat corresponding to the image wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits alredy exist and is non-empty...
Catalog wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits.wcscat corresponding to the image wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits
WCS catalog name: wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.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=1, blended=250, bad_region=1511, passed=7912
Got 7912 stars (including 6224 good ones) from the SExtractor catalog wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits.wcscat
util/solve_plate_with_UCAC5 got 7912 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (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 292 to 351 (Dec -31.4 to -20.1)
Done reading UCAC5 zone files...
Matched 4880 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4874 matched stars entering correct_measured_positions(), 4876 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4874 matched stars entering correct_measured_positions(), 6722 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 292 to 351 (Dec -31.4 to -20.1)
Done reading UCAC5 zone files...
Matched 4880 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4874 matched stars entering correct_measured_positions(), 6722 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
Accuracy estimation diagnostic: 4874 matched stars entering correct_measured_positions(), 6722 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
Excluding outliers - 4874 stars left (next iteration limit 5361)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits N_match=4874 sigma_overall_arcsec=0.623 sigma_q1_arcsec=0.777 sigma_q2_arcsec=0.699 sigma_q3_arcsec=0.540 sigma_q4_arcsec=0.512 n_q1=1505 n_q2=891 n_q3=1543 n_q4=935 worst_quadrant_to_overall_ratio=1.248
The image catalog is written to wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits -region wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.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.zhI5l8jmns (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_2026-09-04_CI_For-01-Q2b1x1_052356_TTUQ2b1x1_2819419_mo17MjFd/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_For-01-Q2b1x1_052356_TTUQ2b1x1_2819419_mo17MjFd/fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_For-01-Q2b1x1_052356_TTUQ2b1x1_2819419_mo17MjFd/fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_For-01-Q2b1x1_052356_TTUQ2b1x1_2819419_mo17MjFd/fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_For-01-Q2b1x1_052356_TTUQ2b1x1_2819419_mo17MjFd/fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_For-01-Q2b1x1_052356_TTUQ2b1x1_2819419_mo17MjFd/fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.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_2026-09-04_CI_For-01-Q2b1x1_052356_TTUQ2b1x1_2819419_mo17MjFd/fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits
WCS_IMAGE_NAME=wcs_fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits
WCS-calibrated image found: wcs_fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits
Checking if the catalog wcs_fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits.wcscat corresponding to the image wcs_fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits alredy exist and is non-empty...
Catalog wcs_fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits.wcscat corresponding to the image wcs_fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_For-01-Q2b1x1_052356_TTUQ2b1x1_2819419_mo17MjFd/fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits
WCS catalog name: wcs_fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.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=1, no_mag_err=0, low_SNR=4, blended=65, bad_region=330, passed=1663
Got 1663 stars (including 1272 good ones) from the SExtractor catalog wcs_fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits.wcscat
util/solve_plate_with_UCAC5 got 1663 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 293 to 349 (Dec -31.2 to -20.6)
Done reading UCAC5 zone files...
Matched 1018 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1014 matched stars entering correct_measured_positions(), 988 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.88"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1014 matched stars entering correct_measured_positions(), 1383 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.90"
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 293 to 349 (Dec -31.2 to -20.6)
Done reading UCAC5 zone files...
Matched 1018 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 1014 matched stars entering correct_measured_positions(), 1385 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.95"
Accuracy estimation diagnostic: 1014 matched stars entering correct_measured_positions(), 1385 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.97"
Excluding outliers - 1014 stars left (next iteration limit 1115)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=1014 robust_rms=4.870 arcsec worst_quadrant_rms=8.122 arcsec
SIP_REFIT: SIP order 3 trial: matched=1014 robust_rms=0.874 arcsec worst_quadrant_rms=1.051 arcsec
SIP_REFIT: SIP order 5 trial: matched=1014 robust_rms=0.830 arcsec worst_quadrant_rms=0.878 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=1014 robust_rms_before=1.389 arcsec robust_rms_before_corrected=0.977 arcsec robust_rms_after=0.830 arcsec worst_quadrant_rms_before=1.045 worst_quadrant_rms_after=0.878
SIP_REFIT: applied the refit solution to the output catalog positions only (order 5, robust RMS 1.389 -> 0.830 arcsec); the image header was NOT rewritten as wcs_fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits is a symbolic link
WCS_QUALITY_DIAG: file=fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits N_match=1014 sigma_overall_arcsec=0.819 sigma_q1_arcsec=0.889 sigma_q2_arcsec=0.770 sigma_q3_arcsec=0.838 sigma_q4_arcsec=0.803 n_q1=171 n_q2=301 n_q3=236 n_q4=306 worst_quadrant_to_overall_ratio=1.085
The image catalog is written to wcs_fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_For-01-Q2b1x1_052356_TTUQ2b1x1_2819419_mo17MjFd/fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits -region wcs_fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.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.qPILQ5pGuV (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_2026-09-04_CI_For-01-Q2b1x1_052356_TTUQ2b1x1_2819419_mo17MjFd/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_For-01-Q2b1x1_052356_TTUQ2b1x1_2819419_mo17MjFd/fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_For-01-Q2b1x1_052356_TTUQ2b1x1_2819419_mo17MjFd/fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_For-01-Q2b1x1_052356_TTUQ2b1x1_2819419_mo17MjFd/fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_For-01-Q2b1x1_052356_TTUQ2b1x1_2819419_mo17MjFd/fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_For-01-Q2b1x1_052356_TTUQ2b1x1_2819419_mo17MjFd/fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707.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_2026-09-04_CI_For-01-Q2b1x1_052356_TTUQ2b1x1_2819419_mo17MjFd/fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707.fits
WCS_IMAGE_NAME=wcs_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707.fits
WCS-calibrated image found: wcs_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707.fits
Checking if the catalog wcs_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707.fits.wcscat corresponding to the image wcs_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707.fits alredy exist and is non-empty...
Catalog wcs_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707.fits.wcscat corresponding to the image wcs_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_For-01-Q2b1x1_052356_TTUQ2b1x1_2819419_mo17MjFd/fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707.fits
WCS catalog name: wcs_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707.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=5, blended=71, bad_region=552, passed=2169
Got 2169 stars (including 1560 good ones) from the SExtractor catalog wcs_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707.fits.wcscat
util/solve_plate_with_UCAC5 got 2169 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 293 to 349 (Dec -31.2 to -20.6)
Done reading UCAC5 zone files...
Matched 1318 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1313 matched stars entering correct_measured_positions(), 1287 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.84"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1313 matched stars entering correct_measured_positions(), 1705 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.85"
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 293 to 349 (Dec -31.2 to -20.6)
Done reading UCAC5 zone files...
Matched 1318 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 1312 matched stars entering correct_measured_positions(), 1705 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.90"
Accuracy estimation diagnostic: 1312 matched stars entering correct_measured_positions(), 1705 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.92"
Excluding outliers - 1312 stars left (next iteration limit 1444)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=1312 robust_rms=5.036 arcsec worst_quadrant_rms=7.056 arcsec
SIP_REFIT: SIP order 3 trial: matched=1312 robust_rms=0.906 arcsec worst_quadrant_rms=1.084 arcsec
SIP_REFIT: SIP order 5 trial: matched=1312 robust_rms=0.854 arcsec worst_quadrant_rms=0.945 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=1312 robust_rms_before=1.393 arcsec robust_rms_before_corrected=0.928 arcsec robust_rms_after=0.854 arcsec worst_quadrant_rms_before=1.103 worst_quadrant_rms_after=0.945
SIP_REFIT: applied the refit solution to the output catalog positions only (order 5, robust RMS 1.393 -> 0.854 arcsec); the image header was NOT rewritten as wcs_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707.fits is a symbolic link
WCS_QUALITY_DIAG: file=fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707.fits N_match=1312 sigma_overall_arcsec=0.802 sigma_q1_arcsec=0.829 sigma_q2_arcsec=0.718 sigma_q3_arcsec=0.892 sigma_q4_arcsec=0.765 n_q1=235 n_q2=481 n_q3=321 n_q4=275 worst_quadrant_to_overall_ratio=1.113
The image catalog is written to wcs_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_For-01-Q2b1x1_052356_TTUQ2b1x1_2819419_mo17MjFd/fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707.fits -region wcs_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707.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_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_For-01-Q2b1x1_052356_TTUQ2b1x1_2819419_mo17MjFd/wcs_fd_For-01-Q2b1x1_2026-09-04_05-19-30_20.00sec_-0.00C_LIGHT_0706.fits
Saving fully-calibrated image wcs_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_For-01-Q2b1x1_052356_TTUQ2b1x1_2819419_mo17MjFd/wcs_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707.fits
Preparing the HTML report for the field For-01-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:56:56.54 -29:59:09.4: 13.40 +/- 0.22 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:56:52.35 -30:01:18.3: 13.49 +/- 0.22 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:55:10.94 -29:49:18.5: 13.20 +/- 0.17 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:57:45.65 -29:55:09.2: 12.91 +/- 0.13 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:57:22.45 -30:06:36.9: 13.60 +/- 0.26 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:55:23.08 -29:55:41.5: 13.23 +/- 0.19 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:58:44.02 -30:13:58.2: 12.94 +/- 0.15 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:42:12.18 -29:02:01.6: 11.37 +/- 0.03 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:48:04.39 -23:17:17.0: 11.32 +/- 0.03 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:57:13.95 -29:43:12.1: 12.69 +/- 0.11 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:55:23.08 -29:55:41.5: 13.34 +/- 0.22 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:56:52.35 -30:01:18.3: 13.47 +/- 0.25 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:57:45.65 -29:55:09.2: 13.26 +/- 0.21 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:55:10.94 -29:49:18.5: 13.10 +/- 0.18 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:57:22.45 -30:06:36.9: 13.19 +/- 0.19 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:56:56.54 -29:59:09.4: 13.55 +/- 0.27 detection
Forced photometry reference-image weighted average: 13.48 +/- 0.17
Forced photometry reference-image weighted average: 13.01 +/- 0.11
Forced photometry reference-image weighted average: 13.28 +/- 0.14
Forced photometry reference-image weighted average: 13.15 +/- 0.12
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:58:44.02 -30:13:58.2: 12.94 +/- 0.15 detection
Forced photometry filter KEPT candidate at 01:56:52.35 -30:01:18.3: ref_mag=13.48 +/- 0.17 new_mean_mag=11.0356 delta=2.44 (need > 0.90)
Forced photometry filter KEPT candidate at 01:57:45.65 -29:55:09.2: ref_mag=13.01 +/- 0.11 new_mean_mag=11.1667 delta=1.85 (need > 0.90)
Forced photometry filter KEPT candidate at 01:55:23.08 -29:55:41.5: ref_mag=13.28 +/- 0.14 new_mean_mag=11.0994 delta=2.18 (need > 0.90)
Forced photometry filter KEPT candidate at 01:55:10.94 -29:49:18.5: ref_mag=13.15 +/- 0.12 new_mean_mag=11.0353 delta=2.12 (need > 0.90)
Forced photometry reference-image weighted average: 13.34 +/- 0.15
Forced photometry reference-image weighted average: 13.46 +/- 0.17
Forced photometry filter KEPT candidate at 01:57:22.45 -30:06:36.9: ref_mag=13.34 +/- 0.15 new_mean_mag=11.3619 delta=1.98 (need > 0.90)
Forced photometry filter KEPT candidate at 01:56:56.54 -29:59:09.4: ref_mag=13.46 +/- 0.17 new_mean_mag=10.9705 delta=2.49 (need > 0.90)
Forced photometry reference-image weighted average: 12.94 +/- 0.10
Forced photometry filter KEPT candidate at 01:58:44.02 -30:13:58.2: ref_mag=12.94 +/- 0.10 new_mean_mag=10.8865 delta=2.05 (need > 0.90)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:48:04.39 -23:17:17.0: 11.33 +/- 0.03 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:42:12.18 -29:02:01.6: 11.30 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.32 +/- 0.02
Forced photometry filter KEPT candidate at 01:48:04.39 -23:17:17.0: ref_mag=11.32 +/- 0.02 new_mean_mag=10.1727 delta=1.15 (need > 0.90)
Forced photometry reference-image weighted average: 11.34 +/- 0.02
Forced photometry filter KEPT candidate at 01:42:12.18 -29:02:01.6: ref_mag=11.34 +/- 0.02 new_mean_mag=10.0782 delta=1.26 (need > 0.90)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:57:13.95 -29:43:12.1: 12.83 +/- 0.13 detection
Forced photometry reference-image weighted average: 12.75 +/- 0.09
Forced photometry filter KEPT candidate at 01:57:13.95 -29:43:12.1: ref_mag=12.75 +/- 0.09 new_mean_mag=10.8362 delta=1.91 (need > 0.90)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:55:53.97 -29:48:24.1: 11.77 +/- 0.05 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:55:53.97 -29:48:24.1: 11.72 +/- 0.05 detection
Forced photometry reference-image weighted average: 11.75 +/- 0.03
Forced photometry filter KEPT candidate at 01:55:53.97 -29:48:24.1: ref_mag=11.75 +/- 0.03 new_mean_mag=10.1652 delta=1.58 (need > 0.90)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:39:20.71 -23:29:35.3: 11.78 +/- 0.05 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:39:20.71 -23:29:35.3: 11.70 +/- 0.05 detection
Forced photometry reference-image weighted average: 11.74 +/- 0.03
Forced photometry filter KEPT candidate at 01:39:20.71 -23:29:35.3: ref_mag=11.74 +/- 0.03 new_mean_mag=10.5364 delta=1.21 (need > 0.90)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:45:54.32 -28:34:58.7: 11.77 +/- 0.05 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:45:06.40 -28:17:00.8: 12.74 +/- 0.11 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:45:54.32 -28:34:58.7: 11.74 +/- 0.05 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:45:06.40 -28:17:00.8: 12.62 +/- 0.11 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:48:08.88 -23:29:31.4: 11.71 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.68 +/- 0.08
Forced photometry reference-image weighted average: 11.76 +/- 0.03
Forced photometry filter KEPT candidate at 01:45:06.40 -28:17:00.8: ref_mag=12.68 +/- 0.08 new_mean_mag=10.9776 delta=1.70 (need > 0.90)
Forced photometry filter KEPT candidate at 01:45:54.32 -28:34:58.7: ref_mag=11.76 +/- 0.03 new_mean_mag=10.6300 delta=1.13 (need > 0.90)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:48:08.88 -23:29:31.4: 11.71 +/- 0.04 detection
Forced photometry reference-image weighted average: 11.71 +/- 0.03
Forced photometry filter KEPT candidate at 01:48:08.88 -23:29:31.4: ref_mag=11.71 +/- 0.03 new_mean_mag=10.3077 delta=1.40 (need > 0.90)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:35:55.26 -28:22:14.2: 11.68 +/- 0.05 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:35:55.26 -28:22:14.2: 11.61 +/- 0.05 detection
Forced photometry reference-image weighted average: 11.64 +/- 0.03
Forced photometry filter KEPT candidate at 01:35:55.26 -28:22:14.2: ref_mag=11.64 +/- 0.03 new_mean_mag=10.5319 delta=1.11 (need > 0.90)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:41:51.67 -25:15:07.2: 11.65 +/- 0.04 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:46:23.55 -28:47:54.1: 11.63 +/- 0.04 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:59:01.26 -30:06:29.7: 11.61 +/- 0.04 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:41:51.67 -25:15:07.2: 11.49 +/- 0.04 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:46:23.55 -28:47:54.1: 11.65 +/- 0.04 detection
Forced photometry reference-image weighted average: 11.56 +/- 0.03
Forced photometry filter KEPT candidate at 01:41:51.67 -25:15:07.2: ref_mag=11.56 +/- 0.03 new_mean_mag=10.5466 delta=1.02 (need > 0.90)
Forced photometry reference-image weighted average: 11.64 +/- 0.03
Forced photometry filter KEPT candidate at 01:46:23.55 -28:47:54.1: ref_mag=11.64 +/- 0.03 new_mean_mag=10.0016 delta=1.64 (need > 0.90)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:59:01.26 -30:06:29.7: 11.56 +/- 0.04 detection
Forced photometry reference-image weighted average: 11.59 +/- 0.03
Forced photometry filter KEPT candidate at 01:59:01.26 -30:06:29.7: ref_mag=11.59 +/- 0.03 new_mean_mag=10.4216 delta=1.17 (need > 0.90)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:37:11.37 -24:59:31.6: 11.60 +/- 0.04 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:37:11.37 -24:59:31.6: 11.56 +/- 0.04 detection
Forced photometry reference-image weighted average: 11.58 +/- 0.03
Forced photometry filter KEPT candidate at 01:37:11.37 -24:59:31.6: ref_mag=11.58 +/- 0.03 new_mean_mag=10.4299 delta=1.15 (need > 0.90)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:41:23.11 -25:06:58.8: 12.65 +/- 0.10 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:41:23.11 -25:06:58.8: 12.51 +/- 0.09 detection
Forced photometry reference-image weighted average: 12.57 +/- 0.07
Forced photometry filter KEPT candidate at 01:41:23.11 -25:06:58.8: ref_mag=12.57 +/- 0.07 new_mean_mag=11.2082 delta=1.37 (need > 0.90)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:56:24.95 -29:59:57.1: 11.57 +/- 0.04 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:56:24.95 -29:59:57.1: 11.49 +/- 0.04 detection
Forced photometry reference-image weighted average: 11.53 +/- 0.03
Forced photometry filter KEPT candidate at 01:56:24.95 -29:59:57.1: ref_mag=11.53 +/- 0.03 new_mean_mag=9.7014 delta=1.83 (need > 0.90)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:56:41.16 -30:06:04.1: 12.68 +/- 0.11 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:43:15.22 -22:07:30.8: 12.67 +/- 0.11 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:35:08.93 -28:14:19.5: 11.51 +/- 0.04 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:56:41.16 -30:06:04.1: 12.62 +/- 0.11 detection
Forced photometry reference-image weighted average: 12.65 +/- 0.08
Forced photometry filter KEPT candidate at 01:56:41.16 -30:06:04.1: ref_mag=12.65 +/- 0.08 new_mean_mag=10.6097 delta=2.04 (need > 0.90)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:43:15.22 -22:07:30.8: 12.83 +/- 0.13 detection
Forced photometry reference-image weighted average: 12.73 +/- 0.08
Forced photometry filter KEPT candidate at 01:43:15.22 -22:07:30.8: ref_mag=12.73 +/- 0.08 new_mean_mag=10.9213 delta=1.81 (need > 0.90)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:37:27.81 -25:16:14.0: 11.50 +/- 0.04 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:35:08.93 -28:14:19.5: 11.57 +/- 0.04 detection
Forced photometry reference-image weighted average: 11.53 +/- 0.03
Forced photometry filter KEPT candidate at 01:35:08.93 -28:14:19.5: ref_mag=11.53 +/- 0.03 new_mean_mag=10.4272 delta=1.11 (need > 0.90)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:37:27.81 -25:16:14.0: 11.40 +/- 0.04 detection
Forced photometry reference-image weighted average: 11.45 +/- 0.03
Forced photometry filter KEPT candidate at 01:37:27.81 -25:16:14.0: ref_mag=11.45 +/- 0.03 new_mean_mag=10.3847 delta=1.06 (need > 0.90)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:38:47.44 -29:20:56.4: 11.45 +/- 0.04 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:38:47.44 -29:20:56.4: 11.43 +/- 0.04 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:47:53.30 -23:58:06.9: 11.45 +/- 0.03 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:46:58.21 -24:04:45.2: 11.43 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.44 +/- 0.03
Forced photometry filter KEPT candidate at 01:38:47.44 -29:20:56.4: ref_mag=11.44 +/- 0.03 new_mean_mag=10.4338 delta=1.01 (need > 0.90)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:46:58.21 -24:04:45.2: 11.45 +/- 0.04 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:47:53.30 -23:58:06.9: 11.49 +/- 0.04 detection
Forced photometry reference-image weighted average: 11.47 +/- 0.03
Forced photometry reference-image weighted average: 11.44 +/- 0.02
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:44:29.65 -29:11:22.3: 13.34 +/- 0.20 detection
Forced photometry filter KEPT candidate at 01:47:53.30 -23:58:06.9: ref_mag=11.47 +/- 0.03 new_mean_mag=10.2649 delta=1.20 (need > 0.90)
Forced photometry filter KEPT candidate at 01:46:58.21 -24:04:45.2: ref_mag=11.44 +/- 0.02 new_mean_mag=10.3719 delta=1.07 (need > 0.90)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:44:29.65 -29:11:22.3: 13.02 +/- 0.17 detection
Forced photometry reference-image weighted average: 13.15 +/- 0.13
Forced photometry filter KEPT candidate at 01:44:29.65 -29:11:22.3: ref_mag=13.15 +/- 0.13 new_mean_mag=11.1361 delta=2.01 (need > 0.90)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:55:53.35 -29:45:23.7: 13.00 +/- 0.15 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:55:53.35 -29:45:23.7: 12.86 +/- 0.14 detection
Forced photometry reference-image weighted average: 12.93 +/- 0.10
Forced photometry filter KEPT candidate at 01:55:53.35 -29:45:23.7: ref_mag=12.93 +/- 0.10 new_mean_mag=11.1966 delta=1.73 (need > 0.90)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:48:32.24 -23:36:39.7: 11.29 +/- 0.03 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:48:32.24 -23:36:39.7: 11.24 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.26 +/- 0.02
Forced photometry filter KEPT candidate at 01:48:32.24 -23:36:39.7: ref_mag=11.26 +/- 0.02 new_mean_mag=10.0481 delta=1.22 (need > 0.90)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:53:19.14 -29:45:13.3: 12.49 +/- 0.09 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:55:58.76 -29:40:57.2: 12.49 +/- 0.09 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:53:19.14 -29:45:13.3: 12.48 +/- 0.10 detection
Forced photometry reference-image weighted average: 12.48 +/- 0.07
Forced photometry filter KEPT candidate at 01:53:19.14 -29:45:13.3: ref_mag=12.48 +/- 0.07 new_mean_mag=10.7926 delta=1.69 (need > 0.90)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:48:50.30 -23:35:23.6: 11.21 +/- 0.03 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:55:58.76 -29:40:57.2: 12.58 +/- 0.11 detection
Forced photometry reference-image weighted average: 12.53 +/- 0.07
Forced photometry filter KEPT candidate at 01:55:58.76 -29:40:57.2: ref_mag=12.53 +/- 0.07 new_mean_mag=10.9820 delta=1.55 (need > 0.90)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:52:21.21 -29:48:51.7: 11.18 +/- 0.03 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:48:50.30 -23:35:23.6: 11.19 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.20 +/- 0.02
Forced photometry filter KEPT candidate at 01:48:50.30 -23:35:23.6: ref_mag=11.20 +/- 0.02 new_mean_mag=10.0796 delta=1.12 (need > 0.90)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:52:21.21 -29:48:51.7: 11.13 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.16 +/- 0.02
Forced photometry filter KEPT candidate at 01:52:21.21 -29:48:51.7: ref_mag=11.16 +/- 0.02 new_mean_mag=9.5391 delta=1.62 (need > 0.90)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:36:09.31 -28:09:26.1: 11.15 +/- 0.03 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:36:09.31 -28:09:26.1: 11.16 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.15 +/- 0.02
Forced photometry filter KEPT candidate at 01:36:09.31 -28:09:26.1: ref_mag=11.15 +/- 0.02 new_mean_mag=9.9581 delta=1.20 (need > 0.90)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:53:27.20 -29:46:49.8: 12.48 +/- 0.09 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:42:04.66 -28:53:14.0: 11.14 +/- 0.03 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:53:27.20 -29:46:49.8: 12.48 +/- 0.10 detection
Forced photometry reference-image weighted average: 12.48 +/- 0.07
Forced photometry filter KEPT candidate at 01:53:27.20 -29:46:49.8: ref_mag=12.48 +/- 0.07 new_mean_mag=10.6492 delta=1.83 (need > 0.90)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:42:04.66 -28:53:14.0: 11.14 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.14 +/- 0.02
Forced photometry filter KEPT candidate at 01:42:04.66 -28:53:14.0: ref_mag=11.14 +/- 0.02 new_mean_mag=10.1009 delta=1.04 (need > 0.90)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:57:56.14 -30:05:10.3: 11.15 +/- 0.03 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:43:45.94 -29:08:06.2: 11.12 +/- 0.03 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:57:56.14 -30:05:10.3: 11.24 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.19 +/- 0.02
Forced photometry filter KEPT candidate at 01:57:56.14 -30:05:10.3: ref_mag=11.19 +/- 0.02 new_mean_mag=9.7367 delta=1.45 (need > 0.90)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:43:45.94 -29:08:06.2: 11.13 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.13 +/- 0.02
Forced photometry filter KEPT candidate at 01:43:45.94 -29:08:06.2: ref_mag=11.13 +/- 0.02 new_mean_mag=9.9615 delta=1.16 (need > 0.90)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:57:36.25 -29:45:18.9: 11.07 +/- 0.03 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:57:36.25 -29:45:18.9: 11.06 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.06 +/- 0.02
Forced photometry filter KEPT candidate at 01:57:36.25 -29:45:18.9: ref_mag=11.06 +/- 0.02 new_mean_mag=9.6106 delta=1.45 (need > 0.90)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:56:51.88 -30:10:26.3: 12.45 +/- 0.09 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:56:51.88 -30:10:26.3: 12.43 +/- 0.09 detection
Forced photometry reference-image weighted average: 12.44 +/- 0.07
Forced photometry filter KEPT candidate at 01:56:51.88 -30:10:26.3: ref_mag=12.44 +/- 0.07 new_mean_mag=10.7049 delta=1.73 (need > 0.90)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:38:17.29 -27:49:11.0: 11.06 +/- 0.03 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:38:26.31 -27:49:09.8: 11.01 +/- 0.02 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:56:06.75 -29:50:42.3: 12.39 +/- 0.09 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:38:17.29 -27:49:11.0: 11.11 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.08 +/- 0.02
Forced photometry filter KEPT candidate at 01:38:17.29 -27:49:11.0: ref_mag=11.08 +/- 0.02 new_mean_mag=9.8414 delta=1.24 (need > 0.90)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:38:26.31 -27:49:09.8: 11.00 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.00 +/- 0.02
Forced photometry filter KEPT candidate at 01:38:26.31 -27:49:09.8: ref_mag=11.00 +/- 0.02 new_mean_mag=9.7985 delta=1.20 (need > 0.90)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:56:06.75 -29:50:42.3: 12.39 +/- 0.09 detection
Forced photometry reference-image weighted average: 12.39 +/- 0.06
Forced photometry filter KEPT candidate at 01:56:06.75 -29:50:42.3: ref_mag=12.39 +/- 0.06 new_mean_mag=10.5218 delta=1.86 (need > 0.90)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:44:12.91 -29:10:48.0: 10.94 +/- 0.02 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:44:12.91 -29:10:48.0: 10.93 +/- 0.02 detection
Forced photometry reference-image weighted average: 10.94 +/- 0.02
Forced photometry filter KEPT candidate at 01:44:12.91 -29:10:48.0: ref_mag=10.94 +/- 0.02 new_mean_mag=9.8426 delta=1.09 (need > 0.90)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:46:35.35 -28:41:26.7: 10.92 +/- 0.02 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:46:35.35 -28:41:26.7: 11.01 +/- 0.02 detection
Forced photometry reference-image weighted average: 10.96 +/- 0.02
Forced photometry filter KEPT candidate at 01:46:35.35 -28:41:26.7: ref_mag=10.96 +/- 0.02 new_mean_mag=9.4618 delta=1.50 (need > 0.90)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:48:07.78 -23:47:16.5: 12.41 +/- 0.08 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:48:07.78 -23:47:16.5: 12.23 +/- 0.07 detection
Forced photometry reference-image weighted average: 12.31 +/- 0.05
Forced photometry filter KEPT candidate at 01:48:07.78 -23:47:16.5: ref_mag=12.31 +/- 0.05 new_mean_mag=10.6838 delta=1.63 (need > 0.90)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:41:39.03 -21:56:38.8: 10.88 +/- 0.02 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:41:39.03 -21:56:38.8: 10.92 +/- 0.02 detection
Forced photometry reference-image weighted average: 10.90 +/- 0.02
Forced photometry filter KEPT candidate at 01:41:39.03 -21:56:38.8: ref_mag=10.90 +/- 0.02 new_mean_mag=9.9297 delta=0.97 (need > 0.90)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:42:20.56 -28:51:00.4: 12.38 +/- 0.09 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:42:20.56 -28:51:00.4: 12.25 +/- 0.08 detection
Forced photometry reference-image weighted average: 12.31 +/- 0.06
Forced photometry filter KEPT candidate at 01:42:20.56 -28:51:00.4: ref_mag=12.31 +/- 0.06 new_mean_mag=10.8357 delta=1.48 (need > 0.90)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:46:01.81 -28:59:14.5: 12.35 +/- 0.08 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:46:01.81 -28:59:14.5: 12.37 +/- 0.09 detection
Forced photometry reference-image weighted average: 12.36 +/- 0.06
Forced photometry filter KEPT candidate at 01:46:01.81 -28:59:14.5: ref_mag=12.36 +/- 0.06 new_mean_mag=10.5901 delta=1.77 (need > 0.90)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:35:51.16 -27:52:08.0: 10.69 +/- 0.02 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:56:53.61 -30:10:58.2: 10.68 +/- 0.02 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:35:51.16 -27:52:08.0: 10.72 +/- 0.02 detection
Forced photometry reference-image weighted average: 10.70 +/- 0.01
Forced photometry filter KEPT candidate at 01:35:51.16 -27:52:08.0: ref_mag=10.70 +/- 0.01 new_mean_mag=9.5772 delta=1.12 (need > 0.90)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:57:07.74 -30:04:24.0: 10.60 +/- 0.02 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:56:53.61 -30:10:58.2: 10.69 +/- 0.02 detection
Forced photometry reference-image weighted average: 10.68 +/- 0.01
Forced photometry filter KEPT candidate at 01:56:53.61 -30:10:58.2: ref_mag=10.68 +/- 0.01 new_mean_mag=9.4859 delta=1.20 (need > 0.90)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:57:07.74 -30:04:24.0: 10.61 +/- 0.02 detection
Forced photometry reference-image weighted average: 10.60 +/- 0.01
Forced photometry filter KEPT candidate at 01:57:07.74 -30:04:24.0: ref_mag=10.60 +/- 0.01 new_mean_mag=9.0854 delta=1.52 (need > 0.90)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:52:57.92 -29:50:54.8: 10.57 +/- 0.02 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:42:09.84 -25:21:34.3: 12.30 +/- 0.07 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:52:57.92 -29:50:54.8: 10.54 +/- 0.02 detection
Forced photometry reference-image weighted average: 10.56 +/- 0.01
Forced photometry filter KEPT candidate at 01:52:57.92 -29:50:54.8: ref_mag=10.56 +/- 0.01 new_mean_mag=9.4390 delta=1.12 (need > 0.90)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:42:09.84 -25:21:34.3: 12.32 +/- 0.08 detection
Forced photometry reference-image weighted average: 12.31 +/- 0.05
Forced photometry filter KEPT candidate at 01:42:09.84 -25:21:34.3: ref_mag=12.31 +/- 0.05 new_mean_mag=10.8494 delta=1.46 (need > 0.90)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:42:57.97 -29:23:14.3: 12.20 +/- 0.07 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:48:06.36 -23:28:33.2: 13.07 +/- 0.14 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:48:06.36 -23:28:33.2: 13.20 +/- 0.18 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:42:57.97 -29:23:14.3: 12.07 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.11
Forced photometry filter KEPT candidate at 01:48:06.36 -23:28:33.2: ref_mag=13.12 +/- 0.11 new_mean_mag=11.0581 delta=2.06 (need > 0.90)
Forced photometry reference-image weighted average: 12.13 +/- 0.05
Forced photometry filter KEPT candidate at 01:42:57.97 -29:23:14.3: ref_mag=12.13 +/- 0.05 new_mean_mag=10.7648 delta=1.37 (need > 0.90)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:43:16.94 -22:26:54.3: 12.25 +/- 0.07 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:43:16.94 -22:26:54.3: 12.21 +/- 0.07 detection
Forced photometry reference-image weighted average: 12.23 +/- 0.05
Forced photometry filter KEPT candidate at 01:43:16.94 -22:26:54.3: ref_mag=12.23 +/- 0.05 new_mean_mag=10.9857 delta=1.24 (need > 0.90)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:58:12.27 -30:13:06.9: 10.23 +/- 0.01 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:58:12.27 -30:13:06.9: 10.22 +/- 0.01 detection
Forced photometry reference-image weighted average: 10.22 +/- 0.01
Forced photometry filter KEPT candidate at 01:58:12.27 -30:13:06.9: ref_mag=10.22 +/- 0.01 new_mean_mag=8.9700 delta=1.25 (need > 0.90)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:51:06.92 -29:42:30.2: 10.15 +/- 0.01 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:54:40.19 -29:57:10.7: 12.18 +/- 0.07 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:51:06.92 -29:42:30.2: 10.15 +/- 0.01 detection
Forced photometry reference-image weighted average: 10.15 +/- 0.01
Forced photometry filter KEPT candidate at 01:51:06.92 -29:42:30.2: ref_mag=10.15 +/- 0.01 new_mean_mag=9.0516 delta=1.10 (need > 0.90)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:54:40.19 -29:57:10.7: 12.29 +/- 0.08 detection
Forced photometry reference-image weighted average: 12.23 +/- 0.05
Forced photometry filter KEPT candidate at 01:54:40.19 -29:57:10.7: ref_mag=12.23 +/- 0.05 new_mean_mag=10.3918 delta=1.84 (need > 0.90)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:56:07.84 -29:49:25.4: 9.97 +/- 0.01 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:49:26.96 -22:38:35.0: 12.12 +/- 0.06 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:49:26.96 -22:38:35.0: 12.11 +/- 0.07 detection
Forced photometry reference-image weighted average: 12.12 +/- 0.05
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:56:07.84 -29:49:25.4: 9.94 +/- 0.01 detection
Forced photometry filter KEPT candidate at 01:49:26.96 -22:38:35.0: ref_mag=12.12 +/- 0.05 new_mean_mag=10.8996 delta=1.22 (need > 0.90)
Forced photometry reference-image weighted average: 9.95 +/- 0.01
Forced photometry filter KEPT candidate at 01:56:07.84 -29:49:25.4: ref_mag=9.95 +/- 0.01 new_mean_mag=8.8425 delta=1.11 (need > 0.90)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:43:34.32 -29:03:46.4: 12.07 +/- 0.06 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:58:33.80 -29:46:16.5: 12.09 +/- 0.06 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:43:34.32 -29:03:46.4: 11.95 +/- 0.06 detection
Forced photometry reference-image weighted average: 12.01 +/- 0.04
Forced photometry filter KEPT candidate at 01:43:34.32 -29:03:46.4: ref_mag=12.01 +/- 0.04 new_mean_mag=10.4828 delta=1.53 (need > 0.90)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:58:33.80 -29:46:16.5: 12.11 +/- 0.07 detection
Forced photometry reference-image weighted average: 12.10 +/- 0.05
Forced photometry filter KEPT candidate at 01:58:33.80 -29:46:16.5: ref_mag=12.10 +/- 0.05 new_mean_mag=10.5403 delta=1.56 (need > 0.90)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:43:18.43 -29:20:02.8: 12.09 +/- 0.06 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:36:41.48 -28:10:08.3: 12.03 +/- 0.06 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:43:18.43 -29:20:02.8: 12.10 +/- 0.07 detection
Forced photometry reference-image weighted average: 12.09 +/- 0.05
Forced photometry filter KEPT candidate at 01:43:18.43 -29:20:02.8: ref_mag=12.09 +/- 0.05 new_mean_mag=10.8665 delta=1.23 (need > 0.90)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:36:41.48 -28:10:08.3: 12.10 +/- 0.07 detection
Forced photometry reference-image weighted average: 12.06 +/- 0.05
Forced photometry filter KEPT candidate at 01:36:41.48 -28:10:08.3: ref_mag=12.06 +/- 0.05 new_mean_mag=10.4373 delta=1.63 (need > 0.90)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:58:07.61 -29:46:39.8: 12.87 +/- 0.13 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:58:07.61 -29:46:39.8: 12.87 +/- 0.14 detection
Forced photometry reference-image weighted average: 12.87 +/- 0.10
Forced photometry filter KEPT candidate at 01:58:07.61 -29:46:39.8: ref_mag=12.87 +/- 0.10 new_mean_mag=10.7937 delta=2.08 (need > 0.90)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:54:06.75 -29:47:43.6: 11.98 +/- 0.06 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:46:52.76 -28:41:22.9: 12.96 +/- 0.14 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:54:06.75 -29:47:43.6: 12.06 +/- 0.07 detection
Forced photometry reference-image weighted average: 12.02 +/- 0.04
Forced photometry filter KEPT candidate at 01:54:06.75 -29:47:43.6: ref_mag=12.02 +/- 0.04 new_mean_mag=10.2909 delta=1.72 (need > 0.90)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:43:22.05 -29:01:52.6: 12.00 +/- 0.06 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:46:52.76 -28:41:22.9: 12.89 +/- 0.13 detection
Forced photometry reference-image weighted average: 12.92 +/- 0.10
Forced photometry filter KEPT candidate at 01:46:52.76 -28:41:22.9: ref_mag=12.92 +/- 0.10 new_mean_mag=10.8835 delta=2.04 (need > 0.90)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:43:22.05 -29:01:52.6: 12.02 +/- 0.07 detection
Forced photometry reference-image weighted average: 12.01 +/- 0.04
Forced photometry filter KEPT candidate at 01:43:22.05 -29:01:52.6: ref_mag=12.01 +/- 0.04 new_mean_mag=10.5179 delta=1.49 (need > 0.90)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:46:05.26 -28:35:37.4: 11.95 +/- 0.06 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:46:05.26 -28:35:37.4: 12.04 +/- 0.06 detection
Forced photometry reference-image weighted average: 11.99 +/- 0.04
Forced photometry filter KEPT candidate at 01:46:05.26 -28:35:37.4: ref_mag=11.99 +/- 0.04 new_mean_mag=10.5566 delta=1.43 (need > 0.90)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:44:52.71 -29:15:00.1: 11.99 +/- 0.06 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:44:52.71 -29:15:00.1: 11.96 +/- 0.06 detection
Forced photometry reference-image weighted average: 11.97 +/- 0.04
Forced photometry filter KEPT candidate at 01:44:52.71 -29:15:00.1: ref_mag=11.97 +/- 0.04 new_mean_mag=10.4522 delta=1.52 (need > 0.90)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:44:59.72 -29:05:47.2: 12.80 +/- 0.12 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:44:59.72 -29:05:47.2: 12.67 +/- 0.12 detection
Forced photometry reference-image weighted average: 12.73 +/- 0.08
Forced photometry filter KEPT candidate at 01:44:59.72 -29:05:47.2: ref_mag=12.73 +/- 0.08 new_mean_mag=10.8189 delta=1.91 (need > 0.90)
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:47:57.96 -23:50:54.6: 11.88 +/- 0.05 detection
Forced photometry on wcs_For-01-Q2b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:47:57.96 -23:50:54.6: 11.88 +/- 0.05 detection
Forced photometry reference-image weighted average: 11.88 +/- 0.03
Forced photometry filter KEPT candidate at 01:47:57.96 -23:50:54.6: ref_mag=11.88 +/- 0.03 new_mean_mag=10.3586 delta=1.52 (need > 0.90)
Adding exclusion_list_local.txt__out00631.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out00637.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out00649.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out00662.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out00706.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out00715.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out00719.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out00720.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out00767.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out00778.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out00812.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out00824.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out00844.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out00849.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out00858.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out00861.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out00864.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out00873.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out00875.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out00902.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out00904.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out00912.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out00925.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out00932.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out00961.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out00997.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out01041.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out01106.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out01146.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out01166.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out01222.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out01223.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out01224.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out01242.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out01320.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out01337.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out01376.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out01454.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out01531.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out01566.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out01609.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out01615.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out01627.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out01724.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out01817.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out01825.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out01867.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out02030.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out02079.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out02085.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04164.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04171.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04254.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04363.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04408.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05486.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06070.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06090.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06931.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07080.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07337.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07388.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07773.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07867.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07905.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07970.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out08056.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out08152.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out08193.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20083.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20099.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20488.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20505.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20507.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20532.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20576.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20681.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 83s
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: 42s
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Considering the candidate 20407_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
The candidate 20407_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707 did not pass the final checks
**** FOUND 01:56:03.45 -30:03:15.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20488_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
Preparing report for the candidate 20488_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
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Considering the candidate 20505_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
Preparing report for the candidate 20505_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
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Considering the candidate 20507_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
Preparing report for the candidate 20507_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
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Considering the candidate 20532_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
Preparing report for the candidate 20532_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
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Considering the candidate 20576_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
Preparing report for the candidate 20576_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
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Considering the candidate 20681_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
Preparing report for the candidate 20681_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
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Considering the candidate 00637_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
Preparing report for the candidate 00637_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
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Considering the candidate 07773_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
Preparing report for the candidate 07773_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
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Considering the candidate 01222_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
Preparing report for the candidate 01222_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
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Considering the candidate 00925_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
Preparing report for the candidate 00925_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
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Considering the candidate 00864_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
Preparing report for the candidate 00864_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
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Considering the candidate 06090_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
Preparing report for the candidate 06090_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
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Considering the candidate 01615_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
Preparing report for the candidate 01615_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
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Considering the candidate 01867_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
Preparing report for the candidate 01867_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
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Considering the candidate 07905_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
Preparing report for the candidate 07905_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
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Considering the candidate 01627_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
Preparing report for the candidate 01627_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
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Considering the candidate 04254_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
Preparing report for the candidate 04254_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
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Considering the candidate 01454_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
Preparing report for the candidate 01454_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
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Considering the candidate 00715_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
Preparing report for the candidate 00715_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
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Considering the candidate 04408_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
Preparing report for the candidate 04408_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
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Considering the candidate 04363_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
Preparing report for the candidate 04363_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
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Considering the candidate 00767_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
Preparing report for the candidate 00767_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
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Considering the candidate 00706_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
Preparing report for the candidate 00706_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
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Considering the candidate 07080_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
Preparing report for the candidate 07080_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
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Considering the candidate 01724_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
Preparing report for the candidate 01724_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
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Considering the candidate 04164_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
Preparing report for the candidate 04164_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
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Considering the candidate 00961_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
Preparing report for the candidate 00961_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
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Considering the candidate 08152_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
Preparing report for the candidate 08152_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
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Considering the candidate 08193_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
Preparing report for the candidate 08193_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
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Considering the candidate 20099_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
Preparing report for the candidate 20099_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
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Considering the candidate 20083_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
Preparing report for the candidate 20083_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
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Considering the candidate 07970_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
Preparing report for the candidate 07970_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
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Considering the candidate 00875_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
Preparing report for the candidate 00875_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
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Considering the candidate 00932_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
Preparing report for the candidate 00932_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06070_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
Preparing report for the candidate 06070_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
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Considering the candidate 00824_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
Preparing report for the candidate 00824_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
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Considering the candidate 01817_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
Preparing report for the candidate 01817_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
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Considering the candidate 00861_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
Preparing report for the candidate 00861_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
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Considering the candidate 01337_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
Preparing report for the candidate 01337_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
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Considering the candidate 00720_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
Preparing report for the candidate 00720_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
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Considering the candidate 01166_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
Preparing report for the candidate 01166_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 00904_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
Preparing report for the candidate 00904_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 00662_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
Preparing report for the candidate 00662_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
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Considering the candidate 02079_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
Preparing report for the candidate 02079_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02085_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
Preparing report for the candidate 02085_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 00844_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
Preparing report for the candidate 00844_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
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Considering the candidate 01146_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
Preparing report for the candidate 01146_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
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Considering the candidate 01531_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
Preparing report for the candidate 01531_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05486_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
Preparing report for the candidate 05486_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
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Considering the candidate 06931_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
Preparing report for the candidate 06931_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
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Considering the candidate 01376_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
Preparing report for the candidate 01376_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
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Considering the candidate 01320_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
Preparing report for the candidate 01320_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
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Considering the candidate 02030_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
Preparing report for the candidate 02030_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
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Considering the candidate 00649_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
Preparing report for the candidate 00649_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
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Considering the candidate 00719_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
Preparing report for the candidate 00719_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 00812_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
Preparing report for the candidate 00812_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
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Considering the candidate 04171_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
Preparing report for the candidate 04171_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
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Considering the candidate 07867_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
Preparing report for the candidate 07867_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
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Considering the candidate 00997_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
Preparing report for the candidate 00997_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
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Considering the candidate 07337_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
Preparing report for the candidate 07337_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
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Considering the candidate 00631_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
Preparing report for the candidate 00631_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
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Considering the candidate 00873_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
Preparing report for the candidate 00873_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 00778_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
Preparing report for the candidate 00778_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
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Considering the candidate 00849_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
Preparing report for the candidate 00849_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
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Considering the candidate 07388_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
Preparing report for the candidate 07388_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
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Considering the candidate 01223_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
Preparing report for the candidate 01223_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
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Considering the candidate 00912_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
Preparing report for the candidate 00912_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01041_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
Preparing report for the candidate 01041_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01825_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
Preparing report for the candidate 01825_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 00902_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
Preparing report for the candidate 00902_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 00858_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
Preparing report for the candidate 00858_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01566_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
Preparing report for the candidate 01566_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01242_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
Preparing report for the candidate 01242_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01609_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
Preparing report for the candidate 01609_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01106_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
Preparing report for the candidate 01106_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01224_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
Preparing report for the candidate 01224_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08056_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
Preparing report for the candidate 08056_fd_For-01-Q2b1x1_2026-09-04_05-20-31_20.00sec_-0.00C_LIGHT_0707
make_report_in_HTML.sh Phase 2 (HTML assembly): 6s
make_report_in_HTML.sh TOTAL: 131s
Prepared the HTML report for the field For-01-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
01:58:12.27 -30:13:06.9
01:58:44.02 -30:13:58.2
01:56:53.61 -30:10:58.2
01:56:51.88 -30:10:26.3
01:56:41.16 -30:06:04.1
01:59:01.26 -30:06:29.7
01:57:07.74 -30:04:24.0
01:57:56.14 -30:05:10.3
01:56:24.95 -29:59:57.1
01:54:40.19 -29:57:10.7
01:52:57.92 -29:50:54.8
01:52:21.21 -29:48:51.7
01:56:06.75 -29:50:42.3
01:56:07.84 -29:49:25.4
01:54:06.75 -29:47:43.6
01:53:27.20 -29:46:49.8
01:55:53.97 -29:48:24.1
01:51:06.92 -29:42:30.2
01:53:19.14 -29:45:13.3
01:58:07.61 -29:46:39.8
01:57:36.25 -29:45:18.9
01:58:33.80 -29:46:16.5
01:57:13.95 -29:43:12.1
01:55:58.76 -29:40:57.2
01:38:47.44 -29:20:56.4
01:42:57.97 -29:23:14.3
01:43:18.43 -29:20:02.8
01:44:52.71 -29:15:00.1
01:44:12.91 -29:10:48.0
01:43:45.94 -29:08:06.2
01:42:12.18 -29:02:01.6
01:43:34.32 -29:03:46.4
01:44:59.72 -29:05:47.2
01:43:22.05 -29:01:52.6
01:46:01.81 -28:59:14.5
01:42:04.66 -28:53:14.0
01:42:20.56 -28:51:00.4
01:46:23.55 -28:47:54.1
01:46:35.35 -28:41:26.7
01:46:52.76 -28:41:22.9
01:46:05.26 -28:35:37.4
01:45:54.32 -28:34:58.7
01:35:55.26 -28:22:14.2
01:35:08.93 -28:14:19.5
01:36:09.31 -28:09:26.1
01:36:41.48 -28:10:08.3
01:45:06.40 -28:17:00.8
01:35:51.16 -27:52:08.0
01:38:17.29 -27:49:11.0
01:38:26.31 -27:49:09.8
01:37:27.81 -25:16:14.0
01:42:09.84 -25:21:34.3
01:41:51.67 -25:15:07.2
01:41:23.11 -25:06:58.8
01:37:11.37 -24:59:31.6
01:48:07.78 -23:47:16.5
01:48:50.30 -23:35:23.6
01:39:20.71 -23:29:35.3
01:41:39.03 -21:56:38.8
01:43:15.22 -22:07:30.8
01:43:16.94 -22:26:54.3
01:49:26.96 -22:38:35.0
01:48:04.39 -23:17:17.0
01:48:06.36 -23:28:33.2
01:48:08.88 -23:29:31.4
01:48:32.24 -23:36:39.7
01:47:57.96 -23:50:54.6
01:47:53.30 -23:58:06.9
01:46:58.21 -24:04:45.2
01:55:53.35 -29:45:23.7
01:44:29.65 -29:11:22.3
01:55:23.08 -29:55:41.5
01:56:52.35 -30:01:18.3
01:56:56.54 -29:59:09.4
01:55:10.94 -29:49:18.5
01:57:45.65 -29:55:09.2
01:57:22.45 -30:06:36.9
########### Completed For-01-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 ####
01:55:23.08 -29:55:41.5
01:56:52.35 -30:01:18.3
01:56:56.54 -29:59:09.4
01:55:10.94 -29:49:18.5
01:57:45.65 -29:55:09.2
01:57:22.45 -30:06:36.9
01:58:44.02 -30:13:58.2
01:48:04.39 -23:17:17.0
01:42:12.18 -29:02:01.6
01:57:13.95 -29:43:12.1
01:55:53.97 -29:48:24.1
01:39:20.71 -23:29:35.3
01:45:54.32 -28:34:58.7
01:45:06.40 -28:17:00.8
01:48:08.88 -23:29:31.4
01:35:55.26 -28:22:14.2
01:41:51.67 -25:15:07.2
01:46:23.55 -28:47:54.1
01:59:01.26 -30:06:29.7
01:37:11.37 -24:59:31.6
01:41:23.11 -25:06:58.8
01:56:24.95 -29:59:57.1
01:56:41.16 -30:06:04.1
01:43:15.22 -22:07:30.8
01:35:08.93 -28:14:19.5
01:37:27.81 -25:16:14.0
01:38:47.44 -29:20:56.4
01:47:53.30 -23:58:06.9
01:46:58.21 -24:04:45.2
01:44:29.65 -29:11:22.3
01:55:53.35 -29:45:23.7
01:48:32.24 -23:36:39.7
01:53:19.14 -29:45:13.3
01:55:58.76 -29:40:57.2
01:48:50.30 -23:35:23.6
01:52:21.21 -29:48:51.7
01:36:09.31 -28:09:26.1
01:53:27.20 -29:46:49.8
01:42:04.66 -28:53:14.0
01:57:56.14 -30:05:10.3
01:43:45.94 -29:08:06.2
01:57:36.25 -29:45:18.9
01:56:51.88 -30:10:26.3
01:38:17.29 -27:49:11.0
01:38:26.31 -27:49:09.8
01:56:06.75 -29:50:42.3
01:44:12.91 -29:10:48.0
01:46:35.35 -28:41:26.7
01:48:07.78 -23:47:16.5
01:41:39.03 -21:56:38.8
01:42:20.56 -28:51:00.4
01:46:01.81 -28:59:14.5
01:35:51.16 -27:52:08.0
01:56:53.61 -30:10:58.2
01:57:07.74 -30:04:24.0
01:52:57.92 -29:50:54.8
01:42:09.84 -25:21:34.3
01:48:06.36 -23:28:33.2
01:42:57.97 -29:23:14.3
01:43:16.94 -22:26:54.3
01:58:12.27 -30:13:06.9
01:51:06.92 -29:42:30.2
01:54:40.19 -29:57:10.7
01:56:07.84 -29:49:25.4
01:49:26.96 -22:38:35.0
01:43:34.32 -29:03:46.4
01:58:33.80 -29:46:16.5
01:43:18.43 -29:20:02.8
01:36:41.48 -28:10:08.3
01:58:07.61 -29:46:39.8
01:54:06.75 -29:47:43.6
01:46:52.76 -28:41:22.9
01:43:22.05 -29:01:52.6
01:46:05.26 -28:35:37.4
01:44:52.71 -29:15:00.1
01:44:59.72 -29:05:47.2
01:47:57.96 -23:50:54.6
###################################################################################
01:55:23.08 -29:55:41.5 -- not an asteroid (will add it to exclusion list)
01:56:52.35 -30:01:18.3 -- not an asteroid (will add it to exclusion list)
01:56:56.54 -29:59:09.4 -- not an asteroid (will add it to exclusion list)
01:55:10.94 -29:49:18.5 -- not an asteroid (will add it to exclusion list)
01:57:45.65 -29:55:09.2 -- not an asteroid (will add it to exclusion list)
01:57:22.45 -30:06:36.9 -- not an asteroid (will add it to exclusion list)
01:58:44.02 -30:13:58.2 -- not an asteroid (will add it to exclusion list)
01:48:04.39 -23:17:17.0 -- not an asteroid (will add it to exclusion list)
01:42:12.18 -29:02:01.6 -- not an asteroid (will add it to exclusion list)
01:57:13.95 -29:43:12.1 -- not an asteroid (will add it to exclusion list)
01:55:53.97 -29:48:24.1 -- not an asteroid (will add it to exclusion list)
01:39:20.71 -23:29:35.3 -- not an asteroid (will add it to exclusion list)
01:45:54.32 -28:34:58.7 -- not an asteroid (will add it to exclusion list)
01:45:06.40 -28:17:00.8 -- not an asteroid (will add it to exclusion list)
01:48:08.88 -23:29:31.4 -- not an asteroid (will add it to exclusion list)
01:35:55.26 -28:22:14.2 -- not an asteroid (will add it to exclusion list)
01:41:51.67 -25:15:07.2 -- not an asteroid (will add it to exclusion list)
01:46:23.55 -28:47:54.1 -- not an asteroid (will add it to exclusion list)
01:59:01.26 -30:06:29.7 -- not an asteroid (will add it to exclusion list)
01:37:11.37 -24:59:31.6 -- not an asteroid (will add it to exclusion list)
01:41:23.11 -25:06:58.8 -- not an asteroid (will add it to exclusion list)
01:56:24.95 -29:59:57.1 -- not an asteroid (will add it to exclusion list)
01:56:41.16 -30:06:04.1 -- not an asteroid (will add it to exclusion list)
01:43:15.22 -22:07:30.8 -- not an asteroid (will add it to exclusion list)
01:35:08.93 -28:14:19.5 -- not an asteroid (will add it to exclusion list)
01:37:27.81 -25:16:14.0 -- not an asteroid (will add it to exclusion list)
01:38:47.44 -29:20:56.4 -- not an asteroid (will add it to exclusion list)
01:47:53.30 -23:58:06.9 -- not an asteroid (will add it to exclusion list)
01:46:58.21 -24:04:45.2 -- not an asteroid (will add it to exclusion list)
01:44:29.65 -29:11:22.3 -- not an asteroid (will add it to exclusion list)
01:55:53.35 -29:45:23.7 -- not an asteroid (will add it to exclusion list)
01:48:32.24 -23:36:39.7 -- not an asteroid (will add it to exclusion list)
01:53:19.14 -29:45:13.3 -- not an asteroid (will add it to exclusion list)
01:55:58.76 -29:40:57.2 -- not an asteroid (will add it to exclusion list)
01:48:50.30 -23:35:23.6 -- not an asteroid (will add it to exclusion list)
01:52:21.21 -29:48:51.7 -- not an asteroid (will add it to exclusion list)
01:36:09.31 -28:09:26.1 -- not an asteroid (will add it to exclusion list)
01:53:27.20 -29:46:49.8 -- not an asteroid (will add it to exclusion list)
01:42:04.66 -28:53:14.0 -- not an asteroid (will add it to exclusion list)
01:57:56.14 -30:05:10.3 -- not an asteroid (will add it to exclusion list)
01:43:45.94 -29:08:06.2 -- not an asteroid (will add it to exclusion list)
01:57:36.25 -29:45:18.9 -- not an asteroid (will add it to exclusion list)
01:56:51.88 -30:10:26.3 -- not an asteroid (will add it to exclusion list)
01:38:17.29 -27:49:11.0 -- not an asteroid (will add it to exclusion list)
01:38:26.31 -27:49:09.8 -- not an asteroid (will add it to exclusion list)
01:56:06.75 -29:50:42.3 -- not an asteroid (will add it to exclusion list)
01:44:12.91 -29:10:48.0 -- not an asteroid (will add it to exclusion list)
01:46:35.35 -28:41:26.7 -- not an asteroid (will add it to exclusion list)
01:48:07.78 -23:47:16.5 -- not an asteroid (will add it to exclusion list)
01:41:39.03 -21:56:38.8 -- not an asteroid (will add it to exclusion list)
01:42:20.56 -28:51:00.4 -- not an asteroid (will add it to exclusion list)
01:46:01.81 -28:59:14.5 -- not an asteroid (will add it to exclusion list)
01:35:51.16 -27:52:08.0 -- not an asteroid (will add it to exclusion list)
01:56:53.61 -30:10:58.2 -- not an asteroid (will add it to exclusion list)
01:57:07.74 -30:04:24.0 -- not an asteroid (will add it to exclusion list)
01:52:57.92 -29:50:54.8 -- not an asteroid (will add it to exclusion list)
01:42:09.84 -25:21:34.3 -- not an asteroid (will add it to exclusion list)
01:48:06.36 -23:28:33.2 -- not an asteroid (will add it to exclusion list)
01:42:57.97 -29:23:14.3 -- not an asteroid (will add it to exclusion list)
01:43:16.94 -22:26:54.3 -- not an asteroid (will add it to exclusion list)
01:58:12.27 -30:13:06.9 -- not an asteroid (will add it to exclusion list)
01:51:06.92 -29:42:30.2 -- not an asteroid (will add it to exclusion list)
01:54:40.19 -29:57:10.7 -- not an asteroid (will add it to exclusion list)
01:56:07.84 -29:49:25.4 -- not an asteroid (will add it to exclusion list)
01:49:26.96 -22:38:35.0 -- not an asteroid (will add it to exclusion list)
01:43:34.32 -29:03:46.4 -- not an asteroid (will add it to exclusion list)
01:58:33.80 -29:46:16.5 -- not an asteroid (will add it to exclusion list)
01:43:18.43 -29:20:02.8 -- not an asteroid (will add it to exclusion list)
01:36:41.48 -28:10:08.3 -- not an asteroid (will add it to exclusion list)
01:58:07.61 -29:46:39.8 -- not an asteroid (will add it to exclusion list)
01:54:06.75 -29:47:43.6 -- not an asteroid (will add it to exclusion list)
01:46:52.76 -28:41:22.9 -- not an asteroid (will add it to exclusion list)
01:43:22.05 -29:01:52.6 -- not an asteroid (will add it to exclusion list)
01:46:05.26 -28:35:37.4 -- not an asteroid (will add it to exclusion list)
01:44:52.71 -29:15:00.1 -- not an asteroid (will add it to exclusion list)
01:44:59.72 -29:05:47.2 -- not an asteroid (will add it to exclusion list)
01:47:57.96 -23:50:54.6 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
01:35:08.93 -28:14:19.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:35:51.16 -27:52:08.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:35:55.26 -28:22:14.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:36:09.31 -28:09:26.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:36:41.48 -28:10:08.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:37:11.37 -24:59:31.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:37:27.81 -25:16:14.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:38:17.29 -27:49:11.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:38:26.31 -27:49:09.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:38:47.44 -29:20:56.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:39:20.71 -23:29:35.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:41:23.11 -25:06:58.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:41:39.03 -21:56:38.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:41:51.67 -25:15:07.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:42:04.66 -28:53:14.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:42:09.84 -25:21:34.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:42:12.18 -29:02:01.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:42:20.56 -28:51:00.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:42:57.97 -29:23:14.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:43:15.22 -22:07:30.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:43:16.94 -22:26:54.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:43:18.43 -29:20:02.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:43:22.05 -29:01:52.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:43:34.32 -29:03:46.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:43:45.94 -29:08:06.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:12.91 -29:10:48.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:29.65 -29:11:22.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:52.71 -29:15:00.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:59.72 -29:05:47.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:45:06.40 -28:17:00.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:45:54.32 -28:34:58.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:46:01.81 -28:59:14.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:46:05.26 -28:35:37.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:46:23.55 -28:47:54.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:46:35.35 -28:41:26.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:46:52.76 -28:41:22.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:46:58.21 -24:04:45.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:47:53.30 -23:58:06.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:47:57.96 -23:50:54.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:48:04.39 -23:17:17.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:48:06.36 -23:28:33.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:48:07.78 -23:47:16.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:48:08.88 -23:29:31.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:48:32.24 -23:36:39.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:48:50.30 -23:35:23.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:49:26.96 -22:38:35.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:51:06.92 -29:42:30.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:52:21.21 -29:48:51.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:52:57.92 -29:50:54.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:53:19.14 -29:45:13.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:53:27.20 -29:46:49.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:54:06.75 -29:47:43.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:54:40.19 -29:57:10.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:55:10.94 -29:49:18.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:55:23.08 -29:55:41.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:55:53.35 -29:45:23.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:55:53.97 -29:48:24.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:55:58.76 -29:40:57.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:56:06.75 -29:50:42.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:56:07.84 -29:49:25.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:56:24.95 -29:59:57.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:56:41.16 -30:06:04.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:56:51.88 -30:10:26.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:56:52.35 -30:01:18.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:56:53.61 -30:10:58.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:56:56.54 -29:59:09.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:57:07.74 -30:04:24.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:57:13.95 -29:43:12.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:57:22.45 -30:06:36.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:57:36.25 -29:45:18.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:57:45.65 -29:55:09.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:57:56.14 -30:05:10.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:58:07.61 -29:46:39.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:58:12.27 -30:13:06.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:58:33.80 -29:46:16.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:58:44.02 -30:13:58.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:59:01.26 -30:06:29.7 -- 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)
01:35:08.93 -28:14:19.5 -- not a known variable star
01:35:51.16 -27:52:08.0 -- not a known variable star
01:35:55.26 -28:22:14.2 -- not a known variable star
01:36:09.31 -28:09:26.1 -- not a known variable star
01:36:41.48 -28:10:08.3 -- not a known variable star
01:37:11.37 -24:59:31.6 -- not a known variable star
01:37:27.81 -25:16:14.0 -- not a known variable star
01:38:17.29 -27:49:11.0 -- not a known variable star
01:38:26.31 -27:49:09.8 -- not a known variable star
01:38:47.44 -29:20:56.4 -- not a known variable star
01:39:20.71 -23:29:35.3 -- not a known variable star
01:41:23.11 -25:06:58.8 -- not a known variable star
01:41:39.03 -21:56:38.8 -- not a known variable star
01:41:51.67 -25:15:07.2 -- not a known variable star
01:42:04.66 -28:53:14.0 -- not a known variable star
01:42:09.84 -25:21:34.3 -- a known variable star
01:42:12.18 -29:02:01.6 -- not a known variable star
01:42:20.56 -28:51:00.4 -- not a known variable star
01:42:57.97 -29:23:14.3 -- a known variable star
01:43:15.22 -22:07:30.8 -- not a known variable star
01:43:16.94 -22:26:54.3 -- a known variable star
01:43:18.43 -29:20:02.8 -- not a known variable star
01:43:22.05 -29:01:52.6 -- not a known variable star
01:43:34.32 -29:03:46.4 -- not a known variable star
01:43:45.94 -29:08:06.2 -- not a known variable star
01:44:12.91 -29:10:48.0 -- not a known variable star
01:44:29.65 -29:11:22.3 -- not a known variable star
01:44:52.71 -29:15:00.1 -- not a known variable star
01:44:59.72 -29:05:47.2 -- a known variable star
01:45:06.40 -28:17:00.8 -- not a known variable star
01:45:54.32 -28:34:58.7 -- not a known variable star
01:46:01.81 -28:59:14.5 -- not a known variable star
01:46:05.26 -28:35:37.4 -- not a known variable star
01:46:23.55 -28:47:54.1 -- not a known variable star
01:46:35.35 -28:41:26.7 -- not a known variable star
01:46:52.76 -28:41:22.9 -- not a known variable star
01:46:58.21 -24:04:45.2 -- not a known variable star
01:47:53.30 -23:58:06.9 -- not a known variable star
01:47:57.96 -23:50:54.6 -- not a known variable star
01:48:04.39 -23:17:17.0 -- not a known variable star
01:48:06.36 -23:28:33.2 -- not a known variable star
01:48:07.78 -23:47:16.5 -- not a known variable star
01:48:08.88 -23:29:31.4 -- not a known variable star
01:48:32.24 -23:36:39.7 -- not a known variable star
01:48:50.30 -23:35:23.6 -- not a known variable star
01:49:26.96 -22:38:35.0 -- not a known variable star
01:51:06.92 -29:42:30.2 -- not a known variable star
01:52:21.21 -29:48:51.7 -- not a known variable star
01:52:57.92 -29:50:54.8 -- not a known variable star
01:53:19.14 -29:45:13.3 -- not a known variable star
01:53:27.20 -29:46:49.8 -- not a known variable star
01:54:06.75 -29:47:43.6 -- not a known variable star
01:54:40.19 -29:57:10.7 -- not a known variable star
01:55:10.94 -29:49:18.5 -- not a known variable star
01:55:23.08 -29:55:41.5 -- a known variable star
01:55:53.35 -29:45:23.7 -- not a known variable star
01:55:53.97 -29:48:24.1 -- not a known variable star
01:55:58.76 -29:40:57.2 -- not a known variable star
01:56:06.75 -29:50:42.3 -- not a known variable star
01:56:07.84 -29:49:25.4 -- not a known variable star
01:56:24.95 -29:59:57.1 -- not a known variable star
01:56:41.16 -30:06:04.1 -- not a known variable star
01:56:51.88 -30:10:26.3 -- not a known variable star
01:56:52.35 -30:01:18.3 -- not a known variable star
01:56:53.61 -30:10:58.2 -- not a known variable star
01:56:56.54 -29:59:09.4 -- a known variable star
01:57:07.74 -30:04:24.0 -- not a known variable star
01:57:13.95 -29:43:12.1 -- not a known variable star
01:57:22.45 -30:06:36.9 -- not a known variable star
01:57:36.25 -29:45:18.9 -- not a known variable star
01:57:45.65 -29:55:09.2 -- not a known variable star
01:57:56.14 -30:05:10.3 -- not a known variable star
01:58:07.61 -29:46:39.8 -- a known variable star
01:58:12.27 -30:13:06.9 -- not a known variable star
01:58:33.80 -29:46:16.5 -- not a known variable star
01:58:44.02 -30:13:58.2 -- not a known variable star
01:59:01.26 -30:06:29.7 -- not a known variable star
Found 70 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
77 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 77 (excluding asteroids and hot pixels, 70 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)2461287.93032927 -observatory V36
11:20:26.24 +05:42:34.0 Mercury (-1.1mag)
13:28:38.65 -13:24:22.7 Venus (-4.7mag)
07:06:12.73 +23:09:12.5 Mars (1.2mag)
09:06:40.52 +17:07:32.2 Jupiter (-1.8mag)
00:52:22.49 +02:43:13.4 Saturn (0.5mag)
04:13:38.26 +21:01:51.7 Uranus (5.7mag)
00:14:00.84 -00:01:25.0 Neptune (7.7mag)
20:25:47.76 -23:38:56.0 Pluto (14.5mag)
04:45:14.12 +27:15:34.3 Moon (-10.3mag)
-rw-r--r-- 1 apache apache 363 Sep 4 05:26 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461287.93032927:
09:06:36.16 +17:07:54.7 Io (6.2mag)
09:06:31.94 +17:08:15.0 Europa (6.3mag)
09:06:43.22 +17:07:21.8 Ganymede (5.7mag)
09:06:20.60 +17:09:08.0 Callisto (6.9mag)
09:04:21.50 +17:22:44.2 Himalia (15.7mag)
09:06:41.57 +17:07:27.6 Thebe (16.6mag)
09:04:00.18 +17:16:53.9 Elara (17.7mag)
09:10:37.87 +16:36:00.4 Pasiphae (17.9mag)
09:07:57.97 +17:24:32.1 Carme (19.0mag)
00:52:31.55 +02:43:19.0 Titan (8.3mag)
00:52:26.32 +02:42:55.9 Rhea (9.6mag)
00:52:44.76 +02:45:54.1 Iapetus (11.0mag)
00:52:27.59 +02:42:28.8 Hyperion (14.3mag)
00:51:12.30 +02:33:14.1 Phoebe (16.4mag)
-rw-r--r-- 1 apache apache 568 Sep 4 05:26 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461287.93032927:
21:41:25.66 -01:56:46.0 JWST
17:20:41.13 +37:42:19.4 Chandra
06:50:25.29 +04:49:47.4 XMM-Newton
-rw-r--r-- 1 apache apache 96 Sep 4 05:26 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461287.93032927 -observatory V36
03:38:37.16 +19:12:07.7 17.4mag P/1996 R2 (Lagerkvist)
18:01:59.38 -34:15:47.1 14.3mag P/2010 H2 (Vales)
07:17:16.08 -70:08:43.8 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
06:15:20.33 +33:37:36.5 17.7mag C/2017 K2 (PANSTARRS)
04:47:00.92 +45:02:12.3 15.7mag P/2021 N1 (ZTF)
04:47:00.95 +45:02:12.2 15.7mag P/2021 N1 (ZTF)
22:15:47.72 +29:00:42.3 17.4mag C/2022 E2 (ATLAS)
07:07:57.94 +26:01:59.5 16.9mag C/2022 N2 (PANSTARRS)
10:46:51.09 +27:19:52.8 17.1mag C/2022 QE78 (ATLAS)
09:46:50.39 +05:14:53.5 18.0mag C/2022 R6 (PANSTARRS)
15:30:23.95 -15:23:49.3 14.8mag C/2023 R1 (PANSTARRS)
08:35:50.30 +32:43:12.4 15.8mag C/2024 E1 (Wierzchos)
15:06:16.29 +15:21:23.4 17.9mag C/2024 G6 (ATLAS)
18:35:31.83 +43:16:29.0 13.7mag C/2024 J3 (ATLAS)
20:30:09.29 +49:26:18.1 17.4mag C/2024 R4 (PANSTARRS)
05:34:01.76 -12:59:26.5 15.1mag C/2024 T5 (ATLAS)
07:10:35.12 +19:06:43.6 17.8mag C/2025 J1 (Borisov)
11:13:24.16 +18:59:27.2 16.9mag C/2025 V2 (Rankin)
13:17:17.90 +00:20:45.3 16.8mag C/2025 Y1 (ATLAS)
16:34:15.91 +74:29:21.9 16.2mag C/2026 A2 (Bok)
03:07:04.27 +46:12:49.3 17.4mag C/2026 B2 (Sun-Gao)
12:10:37.79 +11:02:50.2 17.5mag A/2026 E1
22:23:36.60 -34:47:22.9 13.3mag 10P/Tempel
11:46:15.63 -05:15:16.9 16.3mag 29P/Schwassmann-Wachmann
12:02:47.91 -04:11:04.8 17.6mag 63P/Wild
00:46:11.45 -06:53:11.2 15.4mag 65P/Gunn
06:33:43.15 +19:27:47.7 17.1mag 78P/Gehrels
03:16:57.19 +14:57:12.3 16.7mag 88P/Howell
05:28:46.69 +27:31:47.2 17.5mag 112P/Urata-Niijima
07:23:13.11 +25:31:46.0 17.9mag 114P/Wiseman-Skiff
10:21:28.21 +21:28:13.9 14.8mag 123P/West-Hartley
12:40:19.89 -20:19:58.0 17.4mag 124P/Mrkos
06:13:53.51 +20:43:28.2 15.9mag 128P/Shoemaker-Holt
23:53:47.90 +02:31:17.7 17.3mag 139P/Vaisala-Oterma
02:42:10.75 -17:54:00.8 15.4mag 161P/Hartley-IRAS
09:44:08.47 +15:44:03.6 12.0mag 169P/NEAT
03:21:50.68 +08:41:50.2 14.4mag 220P/McNaught
04:40:15.04 +35:24:20.7 15.2mag 260P/McNaught
08:24:07.06 +35:59:42.8 17.3mag 295P/LINEAR
15:23:25.34 +00:04:25.5 17.9mag 391P/Kowalski
09:25:17.91 +16:59:50.4 17.9mag 450P/LONEOS
-rw-r--r-- 1 apache apache 2.0K Sep 4 05:26 comets.txt
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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
-rw-r--r-- 1 apache apache 5.7K Sep 4 05:26 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
02:19:17.36 +28:57:15.8 TCP J02191736+2857158 2026-07-12.3549 12.5mag
00:44:56.43 +41:57:41.6 PNV J00445643+4157416 2026-07-13.8026 17.98Cmag
00:42:55.36 +41:17:27.0 PNV J00425536+4117270 2026-07-20.1813 17.7mag
20:35:43.64 +61:31:32.9 TCP J20354364+6131329 2026-07-20.5443 14.4mag
21:17:31.48 +22:25:51.0 TCP J21173148+2225510 2026-07-23.5577 14.8mag
00:41:24.04 +40:49:02.8 PNV J00412404+4049028 2026-07-25.0157 18.7mag
00:43:04.26 +41:02:28.6 PNV J00430426+4102286 2026-07-26.1512 20mag
14:51:51.40 +66:13:24.0 TCP J14515140+6613240 2026-07-29.2561 13.5mag
00:43:06.15 +41:22:08.2 PNV J00430615+4122082 2026-07-30.0085 19.4mag
00:41:33.23 +41:10:12.2 PNV J00413323+4110122 2026-08-02.8913 17.1mag
05:21:07.63 +23:38:19.4 TCP J05210763+2338194 2026-08-06.4109 11.2mag
22:57:17.96 +47:07:41.8 TCP J22571796+4707418 2026-08-09.3289 14.3mag
09:13:38.17 +76:28:18.1 PSN J09133817+7628181 2026-08-09.8037 15.4mag
00:43:17.29 +41:26:48.6 PNV J00431729+4126486 2026-08-14.0920 16.8mag
00:42:52.82 +41:10:58.6 PNV J00425282+4110586 2026-08-17.7723 19.9mag
00:42:52.83 +41:10:59.6 PNV J00425283+4110596 2026-08-18.6119 19.3mag
18:25:12.76 -22:25:29.3 TCP J18251276-2225293 2026-08-19.1062 9.4mag
18:03:09.04 +12:18:14.0 TCP J18030904+1218140 2026-08-19.5199 14.9mag
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
-rw-r--r-- 1 apache apache 190K Sep 4 05:26 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
21:12:40.320 +04:03:41.65 AT 2026yfu 2026-08-06.43 21.27
17:57:17.885 +25:16:17.44 AT 2026yft 2026-08-06.41 20.23
15:51:50.093 +15:05:39.28 AT 2026yfs 2026-08-07.27 20.99
00:57:22.776 -24:27:56.06 AT 2026yfr 2026-06-23.81 20.08
00:30:20.591 -54:41:49.80 AT 2026yfq 2026-07-20.77 19.38
02:32:12.791 -22:10:48.74 AT 2026yfp 2026-07-20.79 19.5
01:41:52.083 -42:11:48.39 AT 2026yfo 2026-07-20.75 20.09
23:56:49.152 -38:37:39.87 AT 2026yfn 2026-07-27.78 19.61
23:42:35.374 -40:35:39.21 AT 2026yfm 2026-08-06.67 20.01
00:59:35.904 -40:19:34.17 AT 2026yfl 2026-08-06.70 20.35
00:09:47.092 -52:13:41.85 AT 2026yfk 2026-08-06.71 19.78
01:29:51.734 -23:34:18.41 AT 2026yfj 2026-08-06.73 19.55
02:10:09.536 -24:08:21.00 AT 2026yfi 2026-07-20.77 20.04
03:25:21.580 -50:44:20.31 AT 2026yfh 2026-08-06.77 20.01
04:26:28.926 -21:02:33.55 AT 2026yfg 2026-08-06.78 19.34
02:45:19.042 -55:38:20.40 AT 2026yff 2026-08-06.78 19.68
03:57:14.486 -09:10:35.02 AT 2026yfe 2026-08-06.79 19.58
04:48:25.059 -18:04:11.02 AT 2026yfd 2026-08-06.79 19.24
03:12:28.807 -53:09:31.17 AT 2026yfc 2026-08-06.80 20.22
03:12:34.990 -53:15:23.14 AT 2026yfb 2026-08-06.80 19.82
-rw-r--r-- 1 apache apache 88K Sep 4 05:26 tns_transients_list.txt
